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The Tracking Calorimeter and Muon Detectors of the H

Exp eriment at HERA

H Collab oration

Abstract

Technical asp ects of the three ma jor comp onents of the H detector at the

storage ring HERA are describ ed This pap er covers the detector

status up to the end of when a ma jor upgrading of some of its elements was

undertaken A description of the other elements of the detector and some p erfor

mance gures from luminosity runs at HERA during and are given in a pap er previously published in this journal

H Collab oration

     

I Abt TAhmed SAid V Andreev B Andrieu RD Appuhn C Arnault

     

M Arpagaus A Babaev HBarwol JBan EBanas P Baranov

      

E Barrelet W Bartel MBarth UBassler FBasti DE Baynham JM Baze

     

GA Beck HPBeck DBederede HJ Behrend C Beigb eder A Belousov

     

Ch Berger H Bergstein R Bernard G Bernardi RBernet R Bernier

    

U Berthon G BertrandCoremans M Besancon RBeyer JC Biasci

      

P Biddulph V Bidoli E Binder PBinko JC Bizot VBlobel F Blouzon

     

H Blume K Borras VBoudry C Bourdarios F Brasse W Braunschweig

     

D Breton H Brettel VBrisson D Bruncko CBrune U Buchner

     

L Bungener JBurger FW Busser A Buniatian S Burke P Burmeister

     

A Busata G Buschhorn AJ Campb ell TCarli FCharles MCharlet

     

R Chase DClarke AB Clegg M Colombo V Commichau JF Connolly

     

U Cornett JA Coughlan ACourau MC Cousinou Ch Coutures ACoville

     

G Cozzika DA Cragg L Criegee HI Cronstrom NH Cunlie JCvach

     

A Cyz S Dagoret JBDainton MDanilov AWE Dann D Darvill

      

WD Dau JDavid MDavid RJDay EDeur B Delcourt L Del Buono

     

MDevel JP Dewulf ADeRoeck P Dingus K Djidi F Descamps

      

C Dollfus JDDowell HBDreis A Drescher U Dretzler J Duboc A Ducorps

     

D Dullmann ODunger H Duhm B Duln y F Dup ont R Ebbinghaus

     

M Eb erle JEbert TR Eb ert GEckerlin BWH Edwards V Efremenko

     

S Egli S Eichenb erger REichler F Eisele E Eisenhandler NN Ellis

     

RJ Ellison E Elsen A Epifantsev M Erdmann WErdmann G Ernst

      

E Evrard GFalley LFavart AFedotov DFeeken RFelst JFeltesse

      

ZY Feng IFFensome JFent JFerencei FFerrarotto K Finke KFlamm

y     

W Flauger M Fleischer M Flieser PS Flower GFlugge AFomenko

    

B Fominykh MForbush JFormanek JMFoster GFranke EFretwurst

    

W Frochtenicht PFuhrmann EGabathuler K Gabathuler K Gadow

     

K Gamerdinger J Garvey JGayler EGazo A Gellrich M Gennis

      

U Gensch H Genzel RGerhards KGeske I Giesgen D Gillespie W Glasgo w

    

L Go dfrey JGodlewski U Go erlach LGoerlich N Gogitidze M Goldb erg

     

AM Go o dall IGorelov P Goritchev LGosset C Grab HGrassler

     

R Grassler T Greenshaw C Gregory H Greif M Grewe G Grindhammer

     

A Grub er C Grub er SGunther JHaack M Haguenauer D Haidt

     

L Ha jduk D Hammer OHamon MHampel D Handschuh K Hangarter

      

EM Hanlon M Hapke U Harder J Harjes P Hartz PE Hatton RHaydar

    

WJ Haynes J Heatherington VHedberg CR Hedgeco ck G Heinzelmann

     

RCW Henderson HHenschel RHerma IHerynek W Hildesheim P Hill

     

DL Hill CD Hilton J Hladk y KC Ho eger RBHopes R Horisb erger

     

A Hrisoho J Hub er Ph Huet H Hufnagel N Huot JF Hupp ert

     

M Ibb otson DImbault H Itterb eck MA Jabiol AJacholkowska C Jacobsson

      

M Jare J Janoth T Jansen PJean J Jeanjean LJonsson K Johannsen

     

Jovanovic H Jung PIPKalmus DKant DP Johnson L Johnson P

     

G Kantel S Karstensen S Kasarian RKaschowitz P Kasselmann U Kathage

     

HH Kaufmann G Kemmerling IR Kenyon SKermiche CKeuker C Kiesling

     

M Klein CKleinwort GKnies WKo TKobler JKoch TKohler

     

J Kohne M Kolander H Kolanoski FKole J Koll SD Kolya B Koppitz

     

V Korb el M Korn P Kostka SK Kotelnikov MW Krasn y H Krehbiel

    

F Krivan DKrucker UKruger UKrunerMarquis MKubantsev

     

JP Kub enka TKulp er HJ Kusel HKuster M Kuhlen T Kurca

    

B Kuznik B Laforge F Lamarche R Lander MPJ Landon J Kurzhofer

      

W Lange WLange R Langkau PLanius JF Lap orte L Laptin H Laskus

     

A Leb edev M Lemler ULenhardt ALeuschner CLeverenz SLevonian

      

D Lewin Ch Ley A Lindner G Lindstrom F Linsel J Lipinski B Liss

     

PLoch AB Lo dge H Lohmander GC Lop ez JP Lottin V Lubimov

 y   

K Ludwig DLuers N Lugetski B Lundb erg K Maeshima N Magnussen

     

E Malinovski S Mani P Marage JMarks R Marshall J Martens F Martin

     

G Martin R Martin HU Martyn JMartyniak V Masb ender SMasson

     

A Mavroidis SJ Maxeld SJ McMahon AMehta KMeier J Meissner

      

D Mercer T Merz CA Meyer HMeyer JMeyer S Mikocki JL Mills

y      

V Milone JMock E Monnier BMontes FMoreau J Moreels B Morgan

     

JV Morris JM Morton KMuller PMurn SA Murray VNagovizin

    

B Naroska Th Naumann PNayman A Nep eipivo P Newman

    

D NewmanCoburn D Newton D Neyret HK Nguyen F Nieb ergall

      

C Niebuhr R Nisius TNovak HNovakova GNowak GWNoyes M Nyb erg

     

H Ob erlack U Obro ck JE Olsson JOlszowska S Orenstein F OuldSaada

     

PPailler SPalanque EPanaro APanitch JY Parey CPascaud

      

EPepp el EPerez PPerro do GD Patel APatoux CPaulot UPein

     

A Perus SPeters JP Pharab o d HT Phillips JP Phillips Ch Pichler

      

A Pieuchot W Pimpl D Pitzl APorrovecchio S Prell R Prosi H Quehl

     

G Radel F Raupach K Rauschnab el AReboux P Reimer G Reinmuth

      

S Reinshagen P Ribarics VRiech J Riedlb erger H Riege SRiess MRietz

     

SM Rob ertson P Robmann PRopnack R Ro osen K Rosenbauer A Rostovtsev

     

C Royon ARudge KRuter M Rudowicz MRuer SRusakov VRusinov

     

K Rybicki J Sacton N Sahlmann ESanchez DPC Sankey MSavitski

     

PSchacht SSchiek NSchirm SSchleif PSchlep er Wvon Schlipp e

     

C Schmidt DSchmidt GSchmidt WSchmitz HSchmuc ker VSchroder

     

ulz ASchwind WScobel U Seehausen J Schutt ESchuhmann MSch

     

F Sefkow R Sell M Seman ASemenov P Shatalov V Shekelyan

     

I Sheviakov H Sho oshtari LN Shtarkov G Siegmon USiewert Y Sirois

     

A Sirous IO Skillicorn P Skvaril P Smirnov JR Smith LSmolik D Sole

      

Y Soloviev JSpalek H Spitzer Rvon Staa J Staeck P Staroba JStastn y

     

M Steen bock P Stefan P Steen RSteinberg H Steiner BStella

     

K Stephens J Stier JStiewe U Stosslein J Strachota U Straumann

     

A Strowbridge W Struczinski JP Sutton Z Szkutnik GTapp ern STapprogge

    

RE Taylor VTchernyshov VTchudakov C Thiebaux KThiele

     

G Thompson RJ Thompson ITichomirov CTrenkel WTribanek KTroger

      

PTruol MTuriot JTurnau JTutas LUrban M Urban A Usik

     

S Valkar AValkarova CVallee GVan Beek MVanderkelen LVan Lancker

     

PVan Mechelen AVartap etian YVazdik MVecko PVerrecchia RVick

      

G Villet EVogel KWacker MWagener IW Walker AWalther GWeb er

     

Weissbach HPWellisch LWest DWhite S Willard D Wegener AWegner P

     

M Winde GG Winter Th Wol LAWomersley AE Wright EWunsch

      

N Wul BE Wyb orn TPYiou JZacek DZarbock PZavada C Zeitnitz

     

Z Zhang H Ziaeep our M Zimmer W Zimmermann F Zomer and K Zub er

 a

I Physikalisches Institut der RWTH Aachen Germany

 a

III Physikalisches Institut der RWTH Aachen Germany

 a

Institut fur Physik HumboldtUniversitat Berlin Germany

 b

School of Physics and SpaceResearch University of Birmingham Birmingham UK



InterUniversity Institute for High Energies ULBVUB Brussels Universitaire Instel ling

c

Antwerpen Wilrijk Belgium

 b

Rutherford Appleton Laboratory Chilton Didcot UK

 d

Institute for Nuclear Physics Cracow Poland

e

Physics Department and IIRPA University of California Davis California USA

 a

Institut fur Physik Universitat Dortmund Dortmund Germany



CEA DSMDAPNIA CESaclay GifsurYvette France

 b

Department of Physics and Astronomy University of Glasgow Glasgow UK

 a

DESY Hamburg Germany

 a

I Institut fur Experimentalphysik Universitat Hamburg Hamburg Germany

 a

II Institut fur Experimentalphysik Universitat Hamburg Hamburg Germany

 a

Physikalisches Institut Universitat Heidelberg Heidelberg Germany

 a

Institut fur Hochenergiephysik Universitat Heidelberg Heidelberg Germany

 a

Institut fur Reine und Angewandte Kernphysik Universitat Kiel Kiel Germany

 f

Institute of Experimental Physics Slovak Academy of Sciences Kosice Slovak Republic

 b

School of Physics and Chemistry University of Lancaster Lancaster UK

 b

Department of Physics University of Liverpool Liverpool UK

b 

Queen Mary and Westeld Col lege London UK

 g

Physics Department University of Lund Lund Sweden

 b

Physics Department University of Manchester Manchester UK



CPPM UniversitedAixMarseil le II INPCNRS Marseil le France



Institute for Theoretical and Experimental Physics Moscow Russia

 f

Lebedev Physical Institute Moscow Russia

 a

MaxPlanckInstitut fur Physik Munchen Germany



LAL Universite de ParisSud INPCNRS Orsay France



LPNHE Ecole Polytechnique INPCNRS Palaiseau France



LPNHE Universites Paris VI and VII INPCNRS Paris France

 fh

Institute of Physics Czech Academy of Sciences Praha Czech Republic

 fh

Nuclear Center Charles University Praha Czech Republic



INFN Roma and Dipartimento di Fisica Universita La Sapienza Roma Italy



Paul Scherrer Institut Vil ligen Switzerland



ertal Wuppertal Fachbereich Physik Bergische Universitat Gesamthochschule Wupp

a

Germany

 a

DESY Institut fur Hochenergiephysik Zeuthen Germany

 i

Institut fur Teilchenphysik ETH Zurich Switzerland

 i

PhysikInstitut der Universitat Zurich Zurich Switzerland



Stanford Linear Accelerator Center Stanford California USA



Visitor from Yerevan PhysInst Armenia

y

Deceased

a

Supported by the Bundesministerium fur Bildung Wissenschaft Forschung und Technologie

FRG under contract numbers ACP ACP DOI HHP HHI HDI

HDI KIP MPI and WTP

b

Supported by the UK and Astronomy Research Council and formerly by the

UK Science and Engineering Research Council

c

Supported by FNRSNFWO IISNIIKW

d

Supported by the Polish State Committee for Scientic Research grant Nos

SPUBP and POB and Stiftung fuer DeutschPolnische Zusammenarbeit

project no

e

Supportedinpart by USDOE grant DE F ER

f

Supporte d by the Deutsche Forschungsgemeinschaft

g

Supported by the Swedish Natural ScienceResearch Council

h

SupportedbyGACR grant no GA AV CR grant no and GA UK

grant no

i

Supported by the Swiss National ScienceFoundation

Contents

Intro duction

Tracking

Central chamb ers CJC and CJC

Design criteria

Mechanics

Calibration and p erformance

Track reconstruction

Track parametrization

Track nding

Vertex determination

Central z chamb ers

CIZ

COZ

Forward tracking detector

Planar drift chambers

Radial chamb ers

Transition radiators

Drift chamb er electronics readout and fron t end data pro cessing

Intro duction

Op eration of the readout

Amplier and FADC

The scanner and the front end pro cessor

Determination of charge and time Q t

Implementation

Prop ortional chambers

Forward prop ortional chamb ers FWPC

Central prop ortional chambers

CIP

COP

Backward prop ortional chamb er BWPC

Prop ortional chamb er electronics and readout

Gas systems

Gas circuits

Purication and analysis

Electronic control and safety

Scintillators

Timeofight counters

The veto wall

Calorimetry

The liquid argon LAr calorimeter

Cryostat and cryogenic system

Liquid argon purity

Stack design and construction

Electronic system

Electronic calibration system

Calorimeter data acquisition

Reconstruction techniques

Clustering

Further noise suppression

Correction for energy loss in dead material

The hadronic energy scale

Calibration and p erformance

Overview of the test runs at CERN

Test b eam results

Performance at HERA

The backward electromagnetic calorimeter BEMC

Mechanical layout

Readout electronics and trigger

Calibration

Performance

The plug calorimeter

The tail catcher TC

Electronics

Energy calibration

Performance

Muon system

Iron instrumentation

The limited streamer tub es

Gas system

High voltage system

Readout system

Track reconstruction

Performance

Forward muon sp ectrometer

General description

Chamb er design

The chamber gas and high voltage system

The chargetime analysis

Track reconstruction

Drift velo cityandt determination

Chamb er alignment

Acknowledgement

List of Figures

Schematic layout of the H detector showing the H reference frame

The H tracking system r z view

Central tracking system

Simulation of a NC event and of a CJC cell

Dep endence of the CJC z resolution on the amount of ionization

Sp ecic ionization versus particle momentum measured in the CJC in HERA runs

Longitudinal and transverse crosssection through a cell of the CIZ

Schematic view of the COZ

Forward tracker overview

Forward tracker constructional details

FADC readout system for drift chambers

Longitudinal crosssection and details of the COP

Cross section through the BWPC

MWPC front end electronics and readout system

Layout of the closed circuit gas system for the planar drift chambers

Scintillator walls

Time distribution of hits in a ToF counter

a Longitudinal view of calorimeters b Radial view of a LAr calorimeter wheel

Readout cell structure

Relative stability of the electronic chain over one month

Noise contribution summed over all channels of the LAr calorimeter

Energy lost in front of the LAr calorimeter

mass sp ectrum

Performance of the dead material correction for simulated pions at GeV

Resp onse across the CBCB z crack in a pion test b eam of GeV at CERN

Reconstructed energy for electron energies of and GeV

Energy resolution as function of electron energy for wheels BBE CB FB and IF

Energy reconstruction for pions at GeV

Energy reconstruction for pions at GeV for wheel IF

Energy resolution as function of pion energy for wheel IF

Energymomentum match of generated by cosmic muons

Transverse momentum balance p p

th te

Transverse and longitudinal views of BEMC stacks



Energy sp ectrum of lowQ DIS electrons observed in the BEMC

Cross sectional view of the PLUG calorimeter

Typical IV and CV characteristics of the PLUG Sidetectors

PLUG resp onse to ep events compared to a MC simulation solid line pro duced

using the Colour Dip ole Mo del

Muon sp ectra summed over a complete mo dule

Ratio of the total transverse hadronic energy including the corrected TC energy

and the transverse electron energy versus the energy fraction in the TC for NC

events

Structure of LST chambers

Iron instrumentation

The lo cal data acquisition system

Eciency of chamb er planes

Wire and strip multiplicity p er event

Muon reconstruction eciency

Schematic view of the forward muon sp ectrometer

List of Tables

Summary of H detector parameters

Central drift chamb er parameters

Forward tracker drift chamb er parameters

Summary of drift chamb er readout data

Prop ortional chamb er parameters

MWPC electronics

Gas circuits

Approximate energies and minimum ionizing particle equivalents

Global parameters of the PLUG calorimeter

Layout of the pad readout of the iron instrumentation

Basic prop erties of Luranyl

The LST detector

Intro duction

This pap er describ es the three ma jor detector comp onents of the H exp eriment

the central and forward tracking systems

the liquid argon and warm calorimeters

the muon detector consisting of the iron instrumentation and forward muon chamb ers

A complete overview of the detector as well as descriptions of the magnets luminosity system

trigger slowcontrol data acquisition oline data handling and simulation can b e found in a

pap er recently published in this journal see or in where b oth pap ers are combined A

survey of the detector parameters is given in Table and for the sakeofconvenience the main

elements of the detector are shown again in Figure This gure also shows the reference frame

adopted in this exp eriment

In the pap ers quoted ab ove some p erformance results obtained during the rst years of

HERA op erations can b e found and the upgrade programme undertaken during the

shutdown is outlined

Calorimetry

Main calorimeter liquid Argon LAr Electromagnetic part Hadronic part

 

Granularity to cm to cm

Depth number of channels to X to

abs

p p

Resolution E E E E

eh eh e h

Stability of electronic calibration over one month

LAr purity decrease of signal over one year

Noise p er channel to MeV

Angular coverage dead channels

Backward calorimeter Pbscintillator



Angular coverage granularity cm

p

Depth resolution E E X E

e e e

abs

Tail catcher ironstreamer tub es

Angular coverage

p

Depth resolution E E E

h h h

abs

PLUG calorimeter CuSi



Angular coverage granularity cm

p

Depth resolution E E X E

h h h

Electron tagger TlClBr



Angular coverage granularity cm

p

Depth resolution E E X E

e e e

Tracking

Coil radius eld m B TBB

Central tracking

Angular radial coverage r mm

Jet chamb er spatial resolution m mm

r z

z chamb ers spatial resolution and mm m

r z

 

Momentum dE dx resolution p GeV dE dE

p

Forwardbackward tracking

Angular radial coverage f r mm

Spatial resolution f m mm m

r r xy

Angular coverage resolution b mm

xy

Trigger prop ortional chambers

Angular coverage channels

Muon detection

Instrumented iron



Angular coverage total area m

Number of channels wires strips pads

Spatial resolution mm mm

wire str ip

Angular momentum resolution barrel mrad p

p

Forward muon toroid

Angular coverage resolution p

p



Overall size x y z weight m t

Table Summary of H detector parameters

Alternatively design and test b eam gures are given in brackets Energies are given in GeV

Tracking

The tracking system of H provides simultaneous track triggering reconstruction and particle

identication for the event top ology particular to HERA electron proton collisions It has b een

designed to reconstruct jets with high particle densities and to measure the momentum and

  

angles of charged particles to a precision of p GeV and mrad

p

Because of the asymmetry b etween the electron and proton b eam energies manycharged

particles are pro duced at small angles to the incident proton forward direction To maintain

go o d eciency for triggering and reconstruction over the whole solid angle we divide the tracking

system b etween the central and forward regions see Figure Twomechanically distinct

tracking detectors have b een constructed the central CTD and forward FTD tracking devices

resp ectivelyEach is optimised for tracking and triggering in its angular region

Track reconstruction in the central region see Figure is based on two large concentric

drift chamb ers CJC and CJC The chamb ers have wires strung parallel to the b eam axes

z direction with the drift cells inclined with resp ect to the radial direction Wehave measured

a space p oint resolution of m in the drift co ordinate r plane and can by comparing

e a resolution of one p ercent of the wire length in z signals read out at b oth wire ends achiev

From the signals recorded in these chamb ers the transverse track momentum is determined and

in addition the sp ecic energy loss dE dx is used to improve particle identication

Two thin drift chamb ers the central inner CIZ and central outer COZ z chambers mea

sure the z co ordinates with b etter accuracy than charge division and complement the measure

mentofcharged track momenta in the central chamb ers The CIZ chamb er ts inside CJC and

the COZ chamb er ts in b etween CJC and CJC These twochamb ers deliver track elements

with typically m resolution in z andtoof in This requires a drift direction

parallel to and sense wires p erp endicular to the b eam axis

Triggering over the full solid angle is based on multiwire prop ortional chamb ers with pad

readout in the central and forward region and wire readout in the backward direction They

provide a fast rst level L trigger decision which can b e used to distinguish b etween successive

b eam crossings Furthermore in the central and forward region combinations of pads hit in the

central inner prop ortional chamb er CIP the central outer prop ortional chamb er COP and

the forward prop ortional chamb ers FWPC are used to trigger on tracks coming from a nominal

interaction v ertex First level track triggers are also derived from the central drift chambers

Each of the central chamb ers has an indep endentgasvolume and separate electrostatic

shielding They were built and tested separately and then assembled and lo cked to one me

chanical unit The detector walls are thin to reduce photon conversion and in particular its

eect on identication of primary electrons Neighb ouring volumes share a thin mm cylin

der of carb on b er reinforced ep oxy with a m aluminium coating on each side The complete

system of central tracking detectors is housed in a single aluminium cylinder of mm wall thick

ness The assembly also provides a precise alignment of the chamb ers relative to the outside

supp ort

Charged tracks pro duced at p olar angles close to the b eam axis forward backward

no longer traverse the full b ending r plane radius of the solenoid magnetic eld

Consequently in the CTD b oth track pattern recognition and accuracy of track reconstruction

deteriorate as the measured track length and the numb er of precision space p oints decrease A

way of rectifying this loss is to comp ensate for the reductions in track length and the number

of p oints in the central region by means of a higher radial density of accurate space p oints

obtained using wires strung in the b ending plane closely spaced in z This is provided by

the forward tracking detector which consists of an integrated assembly of three nearly identical

sup ermo dules Each sup ermo dule includes in increasing z three dierent orientations of planar

wire drift chamb ers designed to provide accurate measurements a multiwire prop ortional

chamb er FWPC for fast triggering a passive transition radiator and a radial wire drift chamber

which provides accurate r drift co ordinate information mo derate radius measurementby

charge division and limited particle identication by measuring the transition radiation pro duced

immediately upstream

The FTD and CTD are linked together aligned and surveyed prior to installation into the

calorimeter cryostat

The description of the individual comp onents of the tracking detector b elow is followed by

sections which describ e the features common to all drift chamb ers namely the readout and pulse

shap e analysis and the gas systems used for all chambers

Central jet chamb ers CJC and CJC

Design criteria

The design of CJC and CJC follows that of the jet chamb er used in the JADE exp eriment

at PETRA The wire pattern characteristic for a jet chamb er is a plane of ano de sense wires

parallel to the b eam line with two adjacent catho de planes shaping the drift eld In the CJCs

the latter planes are also made of wires

A jet chamb er cell extends azimuthally from the sense wire plane to b oth adjacent catho de

wire planes and radially over the full radial span of CJC or CJC each with no further sub di

vision as shown in Fig This minimises the disturbing inuence of eld shaping wires at the

inner and outer radii

The jet cells are tilted by ab out such that in the presence of the magnetic eld the

ionization electrons drift approximately p erp endicular to sti high momentum tracks originating

from the center This not only giv es optimum track resolution but also leads to additional

advantages The usual drift chamber ambiguity is easily resolved by connecting track segments

of dierent cells The wrong mirror track segments do not match as demonstrated in Figure

They also do not p oint to the eventvertex and therefore obstruct only small parts of a real track

in the opp osite half cell Each sti track crosses the sense wire plane at least once in CJC and

in CJC From the ne match at the crossing the passing time of a particle can b e determined

to an accuracy of ns This allows an easy separation of tracks coming from a dierent

bunch crossing The drifting electrons from sti tracks arriveatneighb ouring sense wires with

a time shift of ab out ns and therefore pro duce only negligible disturbance by crosstalk

Every track traverses several regions of uniform drifteld inside the cells Systematic errors of

drift time measurement which are known to arise in the nonuniform elds near the catho de and

sense wire planes reverse sign at the crossing and therefore cancel in go o d approximation

Adjacent sense wires are separated bytwo p otential wires see Figures and This

reduces b oth the surface eld and the crosstalk by nearly a factor of two as compared to a

single p otential wire Most imp ortant it allows to adjust drift eld and gas amplication nearly

indep endently The actual p ositions of the sense wires are staggered o the nominal sense wire

plane by m such that adjacent wires are pulled by the electric eld to denite p ositions

on opp osite sides of the plane

A cell is azimuthally limited bytwo catho de wire planes and at the inner and outer radius

by the eld wires The catho de wires are set to a voltage prop ortional to the distance from

the sense wire plane in order to create an uniform drift eld and hence a constantdriftv elo city

over almost all the cell The voltages for the catho de wires are supplied by a resistor network

catho de chain on the adapter cards connected to the catho de wires The eld wires shap e the

eld at the inner and outer end of the cell such that the deviations from a uniform drift eld

are minimal The sense wires are connected to a p ositivevoltage and are AC coupled to the

ampliers The p otential wires are set to ground Toprevent ageing of the chamb ers due to

high electric surface elds the diameters of the p otential catho de and eld wires were chosen

conservatively large and m This limits the surface eld to KVmm The

ano des are m m at the cell ends gold plated tungsten wires with rhenium having

a resistivity of m

The electrostatics of the cells have b een studied in detail by computer simulations Figure

shows drift lines and iso chrones in CJC for a Lorentz angle of In most of the drift region

the electric eld is constant to b etter than At the rst and the last sense wires the

wire geometry pro duces lo cal distortions of the eld which however do not exceed This

intro duces only negligible variations of the drift velo city in particular around the maximum of

the drift velo city

The parameters of the jet chamb er are listed in Table All sense wires are read out at b oth

ends and yield via charge division a z measurement

Mechanics

The volume of each jet chamb er is dened bytwoendwalls p erp endicul ar to the b eam line and

an inner and outer cylinder concentric to the b eamline The volume has to b e gas tight and to

supp ort small overpressure with resp ect to the atmosphere

The bulk material of the endwalls was chosen to b e mm glass b er reinforced ep oxy

combining excellent insulation with go o d mechanical prop erties The fact that there are two jet

chamb ers allowed relatively thin endwalls b ecause the supp ort lengths b etween inner and outer

cylinders are small and thus the b ending under the summed wire tension could b e kept b elow

mm

To facilitate installation insulation and HV testing of all connections the signal and HV

leads are integrated into the endwall structure by means of multilayer printed circuit PC

b oards One b oard mm thick covers one drift cell Of its four layers one provides a nearly

complete electric shield of the chamb er while the others make the contacts b etween the wire

feedthroughs and the signal and HV connector so ckets A second PC b oard inside the chamb er

mm thick carries strips for shaping the end elds

Optimum precision of the wire p ositions is achieved by rst gluing mm thick massive brass

pins into preb ored holes in the endwalls and then drilling precision holes into the brass The

precision of the sense wire p ositions m within one cell is determined by small excentric

holes in the brass Details of the wire supp orts can b e found in ref

The endwalls are kept apart by four cylinders For the inner and the outer cylinder of

CJC and the inner cylinder of CJC carb on b er reinforced ep oxy mm thick has b een



chosen b ecause of its excellentmechanical stabilityYoungs mo dulus kNmm and

very long radiation length X mm The chamber volume forms a Faraday cage in order

to b e screened against external electromagnetic noise Since the conductivity of the carb on

b ers is not sucient in all directions an aluminium coating of the inner and outer surface

was mandatory The thickness of m of the Al surface liner was a compromise b etween

electromagnetic screening down to low frequencies skin depth at MHz in Al is m

and minimum material The outer cylinder of CJC is made of aluminium mm thick and is

the main supp ort vessel for all tracking detectors It has feet which slide on rails p ositioned on

the inner warm wall of the liquid argon cryostat and which are the mechanical link to the rest

of the H detector At b oth ends the Al cylinder has thicker anges r mm whichare

machined to mm tolerances in order to house the endwalls preciselyAt nal assembly the

stability and shap e of the Al cylinder is guaranteed by the insertion of the endwalls

unit CJC CJC CIZ COZ

active length z mm

active zone starts at z mm



total length z mm

mechanical length z mm

inner radius R mm

i

outer radius R mm

o

active radial length mm

numb er of cells rings

numb er of sense wires p er cell ring

numb er of p otential wires p er cell ring

numb er of eld wires p er cell

numb er of catho de wires p er cell

sense wire distance mm

maximum drift distance at R mm

i

maximum drift distance at R mm

o

sense wire tension N

mean wire length mm



drift velo city mms

mm

r

mm

z

double hit resolution mm

Table Central jet and z chamb er parameters

 

Incl preampliers for the gas mixtures given in Table

Calibration and p erformance

The accurate measurement of the track parameters is limited by the intrinsic resolutions namely

m for drift time measurements with a gas mixture of ArCO CH

r  

of the wirelength for the charge division measurements limited by pulseheight and

z

noise and With this gas the drift velo city at nominal HV is mms

dE dx

A large variety of constants is involved to determine the co ordinates of a hit from the timing

t and pulseintegral Q of a drift chamb er signal see Section for Q t analysis We

distinguish overall and wire dep endent constants

The overall constants event timing average drift velo city and average Lorentz angle are

sucient to determine the track parameters with mo derate accuracy eg m They

r

are determined and continuously monitored by tting them as additional parameters to long

ks see Section The use of an average eective wire length and gain high momentum trac

gives resolutions of cm and

z

dE dx

The wire dep endent constants timing signal propagation absolute gain relative gain and

p osition of b oth wire ends have b een determined in two steps The rst step consists of the

evaluation of data where the o ddeven wires of an channel amplier card on b oth chamber

ends are pulsed separately and simultaneously This gives the relative timing of the wire

groups the timing dierence and the relative gain at the two wire ends The start values for

the eective wire length are determined apart from an overall factor In the second step the

residuals of hits for reconstructed and tted tracks are evaluated to obtain the absolute values

of the individual wire constants This improves the resolution to m

r z

cm for pions and see Figures and and Table

dE dx

The resolution achieved in the z co ordinate dep ends on the dep osited ionization Figure

Data from ep collisions were analysed The dep endence of the sp ecic ionization on the

particle momentumisshow in Figure There are clearly visible bands for pions proton and

deuterons where the latter two particle sp ecies are mainly pro duced by protons colliding with

the residual gas in the b eam pip e

Track reconstruction

Track parametrization Tracks of charged particles are characterized by the ve



helix parameters the signed curvature r p ositive if the direction coincides with a

counterclo ckwise propagation along the circle the signed closest distance from the z axis in

the x y plane d p ositive if the vector to the p oint of closest approach and the tra jectory

ca

direction form a righthanded system azimuth and p olar angle and and the z p osition

z at the p oint of closest approach The rst three parameters are determined by a circle t

to the data in the xy pro jection using the noniterative algorithm of Karimaki The circle

equation is expressed in p olar co ordinates ras

 

r d d r sin d

ca ca

ca

For a track traversing b oth rings of the CJC a single parametrization for b oth rings is usually

suciently accurate Due to multiple scattering in the material b etween the two rings X

for some tracks two separate sets of parameters are determined which are constrained to join

in a p ointbetween the two rings under an angle compatible with the mean multiple scattering

angle

xy

The other two parameters are determined by a linear leastsquares t of z z S dz dS

i

i

xy

xy

where S is the track length for the p oint z in the xy pro jection with S atd The slop e

i ca

i

parameter dz dS determined by the t is converted to the angle by arctandz dS

The track nding is followed by further mo dules to determine the xy vertex for a given run

and to p erform track ts to the primary and secondary vertices The track parameters in this

stage are and together with the xy z co ordinates of the vertex and the error matrix

Track nding Twoversions are used for the track nding and tting A fast version

ecient for tracks originating from the primary vertex with a momentum MeVc is used

on the fourth trigger level lter farm see Section of reference for background rejection

and fast classication of events It is roughly a factor ten faster than the standard version which

is ecient for all kinds of tracks and is used within the normal reconstruction

The rst phase of track nding the search for short track elements curvature negligible

is done indep endently in the angular cells with CJC and CJC radial wires Within

angular sectors trackelement nding do es not dep end on parameters like the Lorentz angle or

the drift velo cityHowever accurate values of these parameters are necessary when hits from

more than one angular cell are combined Track nding is based almost exclusively on drift time

data in the xy plane and includes removal of outliers whichwould distort the circle t Only in

a later stage the measured z values are used here it is again necessary to remove outliers b efore

the data are tted

For the fast track nding it is sucient to determine the bunch crossing time t for an ev ent

from the threshold in the drift time histogram The rst step involves the search for track

elements dened by three hits within angular cells found on three wires with a wire distance of

two The algorithm starts by trying all pairs of hits at wires n n wire index Possible

n n  n  n

n

values of drift distances d at the wire n are calculated byd d d andor jd j

i i

k k

i k hit indices and stored in a list if the direction of the pair do es not deviate to o much

from the radial direction Very dense regions with many hits are not analysed This list is then

n n n

compared with the measured values d and for small dierences jd d j the indices of the hits

j j

at the three wires are stored as a p ossible track element From these hit triplets the curvature

and the angle can already b e determined with sucient accuracy assuming d The

m ca

parameter is the track angle at the mean radius r of the CJC and the CJC resp ectively

m m

No attempt is made at this stage to resolve the drift sign ambiguity triplets with a large value of

jj are rejected otherwise b oth solutions are kept A z value and a value for dE dx are assigned

to the triplets from the median of the three singlehit values and later used to determine the

z slop e and intercept z and the mean dE dx value of the track

Tracks from the origin cluster in the plane of the two parameters and of the triplets

m

with a width of typically only one degree for These clusters are suciently separated that

m

after nding them a rst track denition is achieved The co ordinates of triplets within the

z t Track candidates with clusters are then used in a circle t nowallowing d and bya

ca

large jd j and jj values are rejected

ca

The track candidates are then checked in the order of decreasing numb er of triplets decreas

ing signicance rejecting tracks with several triplets already used b efore for an accepted track

Drift sign ambiguities are normally resolved at this stage since most tracks traverse several cells

and the correct solution has a much larger numb er of triplets than the wrong one The fast track

nding is in general ecient enough to allow sensitive recognition of background or classication

of physics events

The standard track nding starts from the results of the fast track nding and rst improves

the time reference value t for an eventby ts to the drift length values of long tracks For a

given track the values of the circle parameters are used to calculate the exp ected drift length for

all p ossible wires The dierence b etween the measured and the exp ected drift length is then

calculated for all hits taking into account the sign of the drift length To these dierences an

expression is tted which in addition to a parab olic dep endence on the track length to allow

for a small inaccuracy in the track parameters parametrizes the eect of a t dierence which

dep ends on the sign of the drift length and of a small dierence of the drift velo city This t

yields an accurate value for t and allows in addition to detect changes of the drift velo cityAt

the same time the metho d impro ves the denition of tracks since often the range of the hits

found is extended Another circle t is p erformed to all long tracks traversing more than one cell



drift sign ambiguity resolved If the value of the track t after removing single bad hits

eventually is acceptable the complete set of track parameters is stored already at this stage

the hits assigned to the track are agged and not used in the following steps

The rst phase of standard track nding again searches for track elements dened by three

hits but now on adjacent wires All p ossible wires are considered except for very dense regions

Triples with common hits are connected bypointers and when all hits of an angular cell are

analysed chains of hits are extracted These chains of hits are then checked by a t to the drift

times for eects like kinks eventually long chains of hits are split into two shorter chains For

long chains the staggering of wires sometimes allows already to resolve the drift sign ambiguity

otherwise b oth solutions are kept Chains accepted at this stage are stored as track elements

with parameters from the t

Short track elements are merged to larger ones rst within the same or neighb ouring angular

cells then within one ring and lastly from b oth CJC and CJC The merging algorithm starts

with a comparison of pairs of track elements with similar helix parameters If the distance



between them is not so large that they could b elong to the same track a t in the xy plane

is p erformed The list of all acceptable pairs is sorted in the order of an increasing distance



assigned to each pair The distance is constructed from the value and other parameters eg

the length of the track element The list of pairs is then checked sequentially starting with

the close pairs Two elements from a pair are combined to a new longer track element if

acceptable If in this sequence one element of a pair has already b een used in the construction

of a new element the t to the mo died elements is rep eated and rejected eventually By this

pro cess longer and more accurate track elements are formed starting with the simple and clear

cases thus avoiding with high probability a wrong combination of short track elements

For the nal improvement of the track nding eciency and precision the exp ected drift

length is calculated for all p ossible wires and for all track elements ordered by their length Hits

at the exp ected wires which are not already used by another track are collected The dierences

between measured and exp ected drift length are analysed to reject incompatible hits Tracks

found are allowed to contain rather large gaps of several wires since parts of tracks maybe

invisible esp ecially within jets due to the limited double track resolution The ts for the track

parameters are rep eated using all acceptable hits

Very short track candidates are rejected unless they start with the rst few wires of a

ring The energy loss dE dx for a given track is determined from the mean of singlehit values

p

p

k dE dx excluding hits which are close to another track An analysis based on a

i i

likeliho o d metho d has improved the dE dX to b elow see

Vertex determination The e pinteraction vertex region in the xy plane extends

over a few hundred m with a rather stable mean p osition for a sequence of runs The mean

vertex co ordinates x y are determined using long high momentum tracks with a small value

v v

of d from a few hundred events and minimizing the sum of squares of the distance of the tracks

ca

to the vertex

The known x y p osition of the run vertex can b e used as a constraint to improvethe

v v

parameters of tracks originating from this vertex if the eect of multiple scattering in the b eam

pip e and the CJC wall for lowmomentum tracks is taken into account Since the standard

deviation of the curvature value is roughly inversely prop ortional to the track length squared

the track precision is signicantly improved by this vertex t in the xy plane A z value of the

primary interaction vertexinanevent is determined from all tracks tting to the xy vertex

The p olar angle for these tracks is changed accordingly

Within the standard reconstruction program a search is made for neutral particles decaying

into a pair of opp ositely charged particles with tracks in the CJC in addition to K and

S

particles also e e pairs from conversion are found by this mo dule Candidate pairs are

determined using simple geometrical cuts For each candidate pair a t is p erformed applying

geometrical common secondary vertex of the charged particles and kinematic constraints Use

is made of the known p osition of the primary vertex Momentum balance p erp endicular to the

direction of the neutral particle is used as kinematic constraint but no masses are assumed

For a very small op ening angle of the pair the transverse momenta in the xy plane are b oth

constrained to zero to improve the stability of the t for e e pairs Pairs with an acceptable



probability are stored

At later stages of the analysis alternative metho ds for reconstructing secondary vertices are

also employed see references and Figure of reference Kalman ltering techniques

have also b een shown to b e useful

Central z chambers

The central inner and outer z chamb ers CIZ COZ surround the inner half of the jet chamber

k momenta in the latter chamb er These two and complement the measurementofcharged trac

chamb ers deliver track elements with typically m resolution in z which can b e linked to

those obtained from the jet chamb er for the nal accuracy on b oth the longitudinal as well

as the transverse momentum comp onents The p olar angles covered by CIZ and COZ are

and resp ectively Since the CIZ uses the inner carb on b er

wall of the CJC for closing its gas volume and the COZ uses the outer carb on b er cylinder

for its basic structural element the thickness of b oth chamb ers could b e kept small namely

X for CIZ and X for COZ in the active zones and and resp ectively

averaging over the cell wall material Furthermore the total amount of dead zones in azimuth

imp osed by readout channels and wire supp orts is only and of resp ectivelyThe

basic parameters of b oth chamb ers are given in Table and the gas mixtures used are given in

Table A rst level background rejecting trigger combines CIZ and COZ hits to trigger

on straight tracks p ointing to the interaction region see Section of reference

CIZ

For CIZ a laminar construction technique similar to that describ ed b elowforCIPwas used

starting from a steel mandril with an inner diameter of mm Successivelayers include m

Kapton with a m Al coating for electrical shielding a mm thick Rohacell cylinder with

its outer surface machined and p olished to pro duce at surfaces forming a regular p olygon

in crosssection see Figure and a m Kapton foil with m Cu eld forming strips on

b oth sides The indep endent cells are separated byprinted circuit b oards mm thick with

mCuoneach side serving as catho de planes The cells are closed electrically with another

Kapton foil identical to that on the b ottom of the cell here backed by mm Rohacell The end

anges of the CIZ are sealed against the CJC end plates with Orings Further constructional

details eg on the sp ecially designed wire feedthroughs can b e found in references

Figure shows the geometry of the drift cell The sense wire planes are tilted by with

resp ect to the normal to the chamb er axis with the rst nine cells in the backward direction tilted

backward and the last six in the forward direction tilted forward ie following the direction of

the tracks crossing the resp ective cells As explained in ref this tilt pro duces a distortion

of the equip otential lines resulting in a nonuniform distribution of the charge collected on the

four wires and an equivalent tilt of the iso chrones This unusual wire arrangementsolves the

leftrightambiguity automatically without a need for wire staggering and furthermore eliminates

the dep endence of the resolution on the crossing angle The wires are soldered to b oth side walls

of a mm wide cable channel at Here the signal wires are connected to line drivers

and the p otential wires to HV cables The line drivers provide the imp edance matching to the

preampliers mounted on the end plate A high resistivity alloy Elgiloy km was

selected as sense wire material m to improve the measurementofthe co ordinate

along the wire bycharge division The p otential wires are made from Au m Tosave

space the HV cables to the electro des and catho des are buried in the Rohacell chamber body

and the miniaturized M resistors mm mm mm which supply the eld

forming strips are emb edded in the printed circuit b oard chamb er partitions The structure of

the eld shaping electro des is indicated in Figure For the gas mixture listed in Table the

chamb er is op erated with a catho de voltage of V a p otential wire voltage of V and

a eld gradientofVmm

Since the CIZ is the drift chamb er closest to the interaction p oint a dedicated current

monitoring system see ref for details was included into each p otential wire supply line

It allows to measure the currents in the nA range These wires control the gas amplication in

the chamb er In this way the activityintro duced byinteraction pro ducts or stray b eam can b e

 

monitored Typically we found nA current increase p er ring for a luminosityofmb s

This corresp onds to an accumulated charge of Cbm p er wire for an integrated luminosityof



pb

Apart from a narrow strip near the cell walls the chamb er eciency was measured to

in test b eams at PSI From test b eam data the resolution was found to b e m

z

indep endent of the drift distance and the crossing angle in the range These

results could b e conrmed with cosmics ray data where central jet chamber tracks were extrap

olated into the zchamb ers and then linked to the corresp onding track elements The average

deviation from a straight line t in the r z plane is m for CIZ internal track

z

elements and m for linked tracks For the pro jection a resolution of of the wire

length was measured Double pulses can b e resolved if their separation exceeds ns which

converts into mm spatial separation in z

COZ

This chamber was also built on a Rohacell b o dy with the crosssection of a regular edge

p olygon Figure but resting on a cylinder of carb on b er reinforced plastics The Kapton

foils with eld shaping copp er strips were glued to the Rohacell surfaces Guided byamechanical

p ositioning device the wire supp orting ro ds G with Cu strips double sided were placed and

soldered to the Kapton foil Between these ro ds planar catho des were intro duced made of

GCu with holes to enable the gas ow through the chamb er The top cover of the drift cell

structure consists of a KaptonRohacell sandwich which is xed at the catho des The cham ber

has a cylindrical shap e due to its GCu gas cover held by the endanges Further details can

b e found in references Figure shows a schematic view of the COZ The dead zones

for the wire readout are distributed in azimuth which allows a corresp onding distribution of the

preampliers at the end anges and minimises the dead area of the chamb er The ano de signals

are transmitted bytwin readout lines signalground signal length to cm from the wire

ends to the preampliers on b oth chamb er ends

Each drift cell is mm high the maximum drift length is mm which limits the drift

time to ab out s Each cell has four sense wires Stablohm m km in

the symmetry plane of the cell and three pairs of p otential wires CuBe m The wire

feedthroughs in the supp orting ro ds are kept in their nominal p osition to ab out m No

wire stagger is implemented Mirror tracks can b e removed in the analysis since they do not

p ointtothevertex

The COZ is typically op erated with a catho de voltage of V a p otential wire voltage

of V and eld gradient of Vmm For the gas mixture listed in Table this gives a

drift velo cityofmmsec as determined from tracks crossing the sense wire plane and the

catho de plane resp ectively

Ineciencies along the cell walls and other p erformance parameters were studied in test

b eams GeV electrons at DESY and low energy pions and electrons at PSI see references

Apart from a small region near the sense wire feedthroughs the eciency was determined

to b e over the full drift cell For a crossing angle the resolution measured at HERA

is ab out m deteriorating to mforlow crossing angles The azimuthal angle is

of the wire length determined bycharge division to an averaged accuracy of ie

Double pulses can b e resolved if their separation is larger than ns which corresp onds to

mm distance For a discussion of the optimum metho d to resolve double tracks and a comparison

of dierent algorithms for Q t analysis we refer to

Forward tracking detector

The forward tracking system is designed to provide an accurate measurementofcharged par

 

GeV and track angular ticles in the forward direction momentum resolution p

p

resolution mrad track information on individual particles within jets electron identi

cation by means of transition radiation detection and a fast forward ray track trigger Details

ab out track nding and tting can b e found in

The layout of the FTD is illustrated in Figures and Key parameters are listed in

Table The drift chambers have dierent wire geometries the planar ones contain parallel

wires whereas the radial ones have wires radiating outwards from the b eam pip e all wires b eing

strung p erp endicul ar to the b eam direction The planar mo dule consists of three drift chamb ers

each four wires deep in z and rotated at to each other in azimuth It is lo cated closest to the

central tracker in each sup ermo dule since its homogeneous spatial precision in x and y is most

suitable for linking to tracks in the center For practical reasons the FWPC Section is

mounted directly b ehind the planar drift chamb ers in order to share the same gas mixture and

maximise the geometrical trigger eciency of the FTD After the FWPC the particles traverse

a transition radiator consisting of p olypropylene foils contained in its own gas volume The

transition radiation photons pass through a thin mylar window and are detected in the radial

chamber which pro duces up to accurate space p oints from ionization drift timing and charge

division To improve double track resolution the second and third radial mo dules are rotated

by and and of a wedge relative to the rst The interleaving of planar and

radial chamb ers provides the optimum lev er arm for momentum measurement

The individual chambers were assembled and tested separately The comp onents for a single

sup ermo dule were installed into a three section tank consisting of aluminium outer cylinders

mm and glass free carb on b er inner cylinders mm mm thick

max min

lined with Al foil each tank section forming an indep endent gas volume and electrically isolated

environment Eachchamb er is b olted to the rigid central Ushap ed outer cylinder using a set

of precision dowels for alignment Assembly was carried out on high quality surface tables with

dimensional tolerances kept to m throughout the build sequence After commissioning

each sup ermo dule on a cosmic ray test facility the three sup ermo dules were then b olted together

separated by thin gas tight Kapton windows and the end faces closed with sti plates made

from a sandwich of mm thick Al alloy and mm thick Nomex honeycomb The

nal alignment ofthewholeFTDwas measured using cosmic rays after installation into the

H exp eriment Water at constant temp erature C is circulated around each tank section

through copp er pip es in order to maintain dimensional stability and provide co oling for the

preampliers As well as maintaining the relative alignment of the tracker elements and supp ort

for the various services water gas cables preampliers p osition monitors etc the tank

provides an electromagnetically sealed environment and serves as the common ground for the

chamb ers The HV and signal cables access the tracker volume via the outer cylinder using

hermetically sealed feedthroughs where they are grounded The HV cables are also ltered

b efore entering the tank

Three dierent gas mixtures are used twoworking gases for the chamb ers and one purge

gas for the transition radiation TR volumes Gas is fed into each sup ermo dule volume via

the Ushap ed channels in the outer cylinder two feed pip es and one pip e for lo cal pressure

sensing a total of nine pip es p er sup ermo dule Gas tightness is maintained by rubb er Oring

seals at the outer and inner anges The gas is supplied at atmospheric pressure from three

computer controlled closed lo op gas circuits see Section whichmaintain gas purity and

provide the accurate pressure control bar required in order to prevent damage to the

fragile TR windows During HERA op eration the oxygen level in all volumes has b een kept to

ppm

The whole tracker is mounted on four insulated feet and rests on the cryostat rails in stress

free condition It is electrically isolated from the central tracker and the cryostat

Parameter unit Radials Planars

numb er of cells p er sup ermo dule

inner outer active radius mm

total numb er of sense wires p er cell

sense wire diameter resistance m



sense wire material Stablohm W Au plated

sense wire spacing z stagger mm

 

sense wire tension N

total numb er of grid wires p er cell

grid wire CuBe diameter m

 

grid wire tension surface eld NkVcm

sense voltage V

bulk grid eld gradient kVcm

maximum drift distance B T mm

p

drift velo cityB T mms

Lorentz angle B T



z planar x mo dule mm



z planar u mo dule mm



z planar v mo dule mm



z radial mo dule mm

from tracksegments mcm

r r xy

double track resolution mm

Table Forward tracker drift chamb er parameters and p ositions

  

alloy from ref of the limit of prop ortionality p osition of rst wire in plane

Planar drift chamb ers

Eachchamb er is constructed as a selfsupp orting mo dule containing drift cells of identical

rectangular crosssection with wire lengths b etween mm and mm as shown in Figure

The chamber walls are formed from two circular discs with an outer diameter of m and

acentral ap erture of mm diameter They are comp osed of a low mass comp osite of Fibredux

skinned Nomex honeycomb mm thick manufactured to b e parallel and at to within

m A mm thick double sided printed circuit b oard carrying the drift eld forming strips

and voltage bus on opp osite faces is b onded onto one side of the honeycomb laminate the drift

cells are dened by parallel sets of copp er clad PCBs mm thickby mm high mounted

p erp endicul arly and b onded at mm intervals into precisely machined slots in the honeycomb

panels resulting in a multiple b ox section structure of high mechanical strength and rigidity

The vertical PCBs constitute the catho de planes and dene the maximum drift distance as

mm for B Each cell contains four sense wires uniformly spaced in z and staggered

alternately meach side of the median plane of the cell Each sense wire is surrounded by

four grid wires CuBe arranged on a mm square matrix Signicant b enets arise from the

double grid design includin g reduced cross talk lower wire tensions improved cell iso chronicity

and reduced grid wire surface elds All wires are crimp ed under tension in pins which are held

in p osition by means of high precision extruded Noryl templates at each end of the cell The

m arises from the inherent inaccuracies in principal source of error in the wire p osition

the crimping technique The cell ends are closed by PCBs containing electro des which cleanly

terminate the electrostatic eld of the cell Aluminium foils covering the outer surfaces and

connected to the tank provide electromagnetic isolation b etween the individual planes A set of

precision dowels x the relativeorientation of each plane to mrad the orientation of the

planar sup ermo dule with resp ect to the FWPC and the planar chamb erFWPC combination

with resp ect to the tank

The cell electric eld distribution is controlled byseven dierentvoltages the sense voltage

denes the gas amplication the central strip voltage aects the sense eld homogeneity four

drift strips and the catho de voltages determine the eld gradient The grid wires are grounded

All voltages are supplied directly from the HV supplies after suitable fan out without the use

of resistor chains at the chamb er Field optimization and chamb er op eration are considerably

aided by the fact that the double grid geometry pro duces a strong decoupling b etween the sense

eld gas amplication and the drift eld The op erating conditions of the chambers for the

gas mixture given in Table are listed in Table

The outer end of each sense wire is AC coupled into a current sensitive preamplier two

drift cells p er preamplier and the signals transmitted via m of coaxial cable to the

FADCs Pulse prole Q t analysis in the front end data acquisition system yields one drift time

co ordinate measurement p erp endicul ar to the sense wire and one pulse integral measurement

Resolutions achieved on e p data are typically m for the single p oint spatial resolution

and mm for the double track resolution

Radial chamb ers

The radial wire drift chambers cover in with separate sectors of width Each

sector is a drift cell having sense wires staggered alternately meach side of a plane

which bisects the sector The sense wires which are all parallel within one of these cells are

separated by mm Between adjacent sense wires and p ositioned on the plane which bisects

the sector are eld wires parallel to the sense wires and half w aybetween them All these

wires are supp orted by crimp pins At the small radius end r mm the crimp pins

are mounted in a cylindrical Noryl hub and at the large radius end r mm in Noryl

templates precision b onded into the cylindrical wall of the comp osite structure which contains

the whole cells of the radial chamb er as one rigid unit The structure of these radial drift

chamb ers has b een describ ed in references

The wedgeshap ed drift cells are separated from each other by catho de planes which consist

of voltage graded copp er strips on each side of thin pap erep oxy material PCB technology

The electrostatic eld cage for each drift cell is completed byvoltage graded shap ed conducting

strips b onded onto the plane inner surface of the comp osite structure for the high z end of the

wedge and onto a complex window assembly describ ed b elow which is axed as a lid to the

comp osite structure for the low z end of the wedge

Detailed design of this window forming the plane surface of the radial chamber towards low

z was determined by the requirement to detect the transition radiation TR entering the radial

drift chamb er The Xray comp onent of TR pro duced by an ultra relativistic charged particle

contributes to an enhanced track ionization hence to enhanced charge collected on one or more

of the sense wires provided that all ionization dep osited anywhere in the cell is collected onto

the sense wires and not onto eld wires The window of the radial chamber is thus designed

to b e as Xray transparent as p ossible and to ensure maximum Xray detection eciency as

close as p ossible to it inside the drift cell Because of the imp erfect nature of the eld grading

close to the V shap ed strips ionization dep osited within ab out mm of the window cannot b e

collected onto the rst sense wire Such a loss of Xray sensitivity is signicant at the TR entry

low z side of the radial chamb er where most of the Xray photons photoionize the chamber

gas For this reason the V shap ed strips to create the drift eld are of aluminium on mylar

and are supp orted on Rohacell spacers which p osition them mm from the thin mylar

windowwhich isolates the chamb er gas volume The eect of this windowassembly on the

electrostatics is to move the drift eld inhomogeneities out of the sensitive gas volume Then

at the mylar wall closing the gas volume the drift eld is uniform and parallel to the surface

except directly opp osite the sense wire Charging eects on the mylar window are then minimal

and the ionization collection eciency on the rst sense wire is optimal right to the edge of the

gas volume

Because all the sense wires are in the radial direction a coarse determination of the radial

p osition of a trackmay b e made from charge division if a wire is read out at b oth ends However

it is not physically p ossible to have preamplier cards at the small radius end For this reason

the sense wires of one sector drift cell are connected at the inner hub to the sense wires

of another sector drift cell actually away in azimuth so that when sense wires are

read out at the outer radius charge division is p ossible along this double length of radial wire

Current sensitive preampliers are at each end of these sense wire pairs eachchannel of which

drives approximately m of cable to the FADC system Pulse prole Q t analysis gives the

drift co ordinate p erp endicul ar to the sense wire plane and two pulse integral measurements Q

L

and Q from the two ends give the radial p osition bycharge division

R

The spacing in the z direction b etween the sense wires of the radial chamb ers b etween the

three mo dules and the sets of planar drift chamb ers and the radial drift chambers maybeseen

from Table Concerning the azimuthal p osition of the radial chamb ers the plane which bisects

a sector cell and ab out which the sense wires are staggered is at in the rst

mo dule at in the second mo dule and at in the third mo dule The resolution

achieved with the argon ethane gas mixture used so far is m The gas

mixture whichisintended to use for optimal detection of transition radiation is given in the

following section

Transition radiators

A passivearray of p olypropylene layers provides a sucientnumb er of dielectric interfaces for

useful transition radiation TR Xray emission The dielectric constant the layer thickness and

the mark to space ratio of the p olypropylene sheets determine the Xray yield and the energy

sp ectrum For the values chosen the sp ectrum p eaks around keV for GeV electrons The

interface b etween the TR and the radial wire drift chamb ers has b een optimised for transmission

of these Xrays As describ ed in the previous section the radial wire drift chamb ers are designed

and op erated b oth for optimal trackpoint measurement and ecientXray detection The

combination of TR and radial wire drift chamb er is designed for electronpion discrimination at

the level of electron acceptance with less than pion contamination up to GeV for

tracks passing through all three mo dules of the FTD Toachieve this it is planned to op erate

the radial wire chamb ers with a gas containing xenon which has a high photoionization cross

section at keV A xenon helium ethane mixture satises the requirements

of TR detection with acceptable charged track dE dx ionization density and also suitable drift

velo city for the requirements of the drift cham b er Data taken with a radial drift chamber in a

test b eam at CERN haveshown that the design discrimination b etween electrons and pions can

be achieved with this gas

The assembly of p olypropylene sheets is self supp orting but is enclosed in its own gas envelop e

in order to isolate it from the gases used in the rest of the FTD The heliumethane mixture

surrounding the p olypropylene sheets is chosen to give the same partial pressure of helium as in

the radial drift chamb er This is imp ortant b ecause the interface is the thin mylar TR window

of the radial drift chamb er section which could b e damaged by pressure dierences in excess of

ab out bar

Drift chamb er electronics readout and front end data pro cessing

Intro duction

All drift chamb ers in H are connected to one of the three indep endent branches of the central

data acquisition system CDAQ The analog signals are digitized and pro cessed in a number of

Chamber Branch of of Rawdata Q tdata

crates channels Kbyte Kbyte

Radial

Planar

CJC and CJC

COZ

CIZ

Forward muons

Table Summary of drift chamb er readout data

front end crates the trigger connection is based on the H standard subsystem trigger controller

crate and interface cards and lo cal logic pro duces and distributes control signals to the frontend

crates A master crate collects the complete data from the branch and sends it to the CDAQ

Crates for lo cal data monitoring can b e added Figure shows the general layout of each drift

chamb er branch

The drift chamb ers are distributed b etween the branches according to p osition in the detec

tor The inner and outer jet chamb ers and the inner and outer z chamb ers form branch CTD

The forward radial and planar chamb ers form branch FTD The and chamb ers of

the forward muon sp ectrometer form branch FMu Table shows the sizes of the various

comp onents and the typical size of the zero suppressed digitizations raw data and pro cessed

summary data Q t data

Op eration of the readout

The analog signals from the preampliers mounted on the detector are received byMHz

FADC cards whichcontinually digitize and store the data at this p ointwe are recording data

at a rate of over Gbytes over all drift chamb ers On receipt of a rst level trigger L

signal the digitization is stopp ed so that the data recorded in the FADC card memory includes

for each detector all digitizations whichcouldhave o ccured b etween the time of the event and

the maximum p ossible drift time for that cham b er

At a second level trigger L signal the full Mbytes of raw data for an event is copied by

the scanner controller cards into the second level buer at a sp eed of Gbytes At a third

level trigger L signal the pro cessor card in the FADC crate reads the data from the scanner

and writes an oline format data bank into an intermediate buer whichcontains blo cks of

signicant zero suppressed data with an event size of approximately Kbyte The output is

written into a triple p orted buer memory on the intercrate connection VIC When a

complete eventisavailable from all front end crates the master pro cessor collects the data from

this buer memory and writes the complete event to the multievent buer of the optical b er

VMEtaxi link see Section of reference

Amplier and FADC

The sense wires of the tracking drift chamb ers are connected to ampliers either at one or at

b oth wire ends The eightchannel amplier cards are mounted directly on the chamber vessel

The sense wire and the grounded p otential wires serve as dierential input The sense wire is at

p ositive HV and therefore it is coupled to the amplier via a capacitor nF The sense wires

in some chamb ers and amplier are protected by a spark gap and a pair of crossed dio des to

ground Each amplier channel consists of two stages of video ampliers The amplication is

large enough so that no further amplication is needed on the readout card This gives optimum

noise rejection and minimises the inuence of pickup on the cable to the readout card The

amplier card has two test inputs which allow the application of test pulse signals to the inputs

of o dd or even amplier channels

The signals from the drift chamb er are digitized byFFADCs The sampling

frequency is MHz generated by an oscillator phase lo cked to the bunch crossing clo ckof

the HERA storage ring of MHz The dierential outputs of the ampliers are connected

to the FADC cards with multicoaxial cable of ab out m length This cable also carries the

power and test lines to the preampliers The FADCchips used have a resolution of eight bits

The combined signal is fed to the FADC chip through a transformer eliminating DC osets

and via a resistor network that includes feedback of the input signal to the voltage reference

providing a non linear resp onse with bit accuracy for small signal amplitudes and a bit

dynamic range EachFADCchip is connected to one byte deep memory which serves as

circular buer During the active sampling phase of the FADC system signals are continuously

digitized and stored in the memories This recording pro cess is stopp ed by a trigger signal

that freezes the history over s in the memory Sixteen FADCchannels are housed on one

Fcard and up to F cards are housed in a F crate It has a VME backplane

used for fast bit wide readout of the digitized signals from the FADCmemories The signal

risetime at the sense wire is a few ns It is delib erately degraded by the amplier band width

cables and coupling transformer to ns to of pulse amplitude at the input of the

digitizing FADC This is the optimum for a time measurement with a FADC sampling at

MHz

The scanner and the front end pro cessor

In each F front end crate there is an M scanner card that acts as a sample controller

for the FADCs and provides fast readout and zero suppression of the F ADC data The scanner

supplies the MHz clo ck to the FADC cards and at a L trigger gates this clo ck such that

the circular buers of the F cards contain the required time segment At a L trigger signal

it copies the data from the FADCs into a lo cal buer in a series of synchronous bursts over

the VME bus in this way a transfer sp eed of Mbytes is achieved and the data for a full

crate can b e copied within the s requirement of H During the copy the data is compared

with programmable thresholds and any signicant transition presently two subsequent time

bins ab oveorbelow threshold is recorded in the hit table

At a L trigger signal the scanner interrupts the front end pro cessor MHz FIC

presentineach F crate The interrupt handler reads the hit table from the scanner

calculates the required blo cks of raw data and copies these blo cks into a multieventrawdata

buer in an oline format data bank Each blo ck includes four presamples b efore the hit starts

to allow dynamic calculation of the p edestal and blo cks are merged in cases where a blo ckwould

inuence a subsequentblock on the same wire An output bank is written into a multievent

output buer in the memory of the VIC interconnect card using the VSB bus connecting

the pro cessor and the interconnect since the VME bus may b e o ccupied by the scanner reading

a subsequentevent The input raw buer and output buer b oth typically hold events

and this allows derandomization over manyevents of the large range in pro cessing times caused

by lo calised high track density

Determination of charge and time Q t

The relevant parameters of a signal pulse from a drift chamb er wire are signal timing t and

the pulse integral Q These signal parameters are determined by a program which runs on the

L farm see Section of reference In this way the amountofraw data is reduced bya

factor of ab out ve The zero suppressed data provided by the scanner are treated in several

steps For the CJC CIZ COZ and the radial chamb ers the rst three steps consider the data

of b oth wire ends separately while the further steps use the combined information

In the Q talgorithm the FADC data are rst linearised The leading edge of a new pulse

is found by a search for a maximum in the dierence of successive samples ab ove the threshold

The average of the six digitizations b efore the pulse start is used to evaluate the p edestal to b e

subtracted from the pulse Hits from the two ends of a wire are combined if the leading edges

dier by less than or equal to twoclock bins

The essential information for the drift time determination comes from those electrons which

arrive rst at the sense wire and which are pro duced along the track in the region tangential

to the iso chrones These electrons contribute to the sharp rise of the pulse which is however

smeared out by diusion chamber capacity and amplifying electronics The remaining o

tangential electrons arrive at later times and uctuations of their ionization density inuence

only the trailing edge of the pulse otherwise determined by the dierentiating electronics

The drift time is determined bychamb er sp ecic algorithms For the CJC eg the time at

half the full amplitude is determined by linear interp olation averaged over b oth wire ends and

used with the average risetime to extrap olate to the arrival time of the rst electrons taken at

of the pulse amplitude The average pulse consists of ab out digitizations while

MHz noise pulses extend typically over bins and can therefore partly b e rejected at the scanner

level The pulse integral is determined b y summing some fraction of these digitizations Most

imp ortant for the CJC and radial drift chamb ers is the relative error of the integral for the

z r determination It is minimised bycho osing a rather short integration interval of eight time

bins The timings of the pulses from the two wire ends dier b ecause of dierent cable length

and signal propagation along the wire Therefore the phase of the integration interval has to b e

prop erly adjusted in order to guarantee the integration over the same part of the pulse on b oth

wire ends

If a pulse is recognized on the tail of a previous one it is analysed after eects from the

previous pulse have b een subtracted on the two wire ends indep endentlyFor this subtraction

a standard pulse shap e is determined byaveraging a large numb er of pulses and then matched

in phase and normalised in height to the preceding pulse

Implementation

The subsystem trigger controller crate STC provides a standard interface to the central

trigger electronics see also section of reference The STC in the DC readout is

supplemented by a MHz phase lo cked lo op PLL card providing an accurate ns clo ck

and a logic card acting as sequence controller Although resp onses from the scanner could by

simple combination b e used directly to resp ond to the central trigger inclusion of the logic card

in the path allows b etter overall p erformance byoverlapping some stages of pro cessing with rell

and other delays of subsequentevents This places much of the resp onse time of the DC systems

in second or even third order dead time and allows the DC systems to b e run at almost full

throughput with little or no actual dead time

The master crate contains interfaces to the CDAQ VMEtaxi link and to other crates in that

branch VIC consisten t with the common H architecture see Section of reference

On startup the master pro cessor loads all other pro cessors with co de and data stored in

non volatile ram Once the other pro cessors are running all communication is made through

the buer memory of the VIC b oards connected to each of the remote pro cessors During a

run the master pro cessor op erates asynchronouslywaiting for an event to b e signalled bythe

trigger pro cessor and then p olling the front end pro cessors until the complete event is ready to

b e built The events are not buered or pro cessed by the master pro cessor

A monitoring crate provides access to the readout branch for chamber specic control and

monitoring systems A small fraction of the event data can b e passed to the monitoring crate

for lo cal monitoring esp ecially that which requires raw data that mightbeunavailable in the

CDAQ monitoring systems Data is collected from a dedicated memory in the master crate using

a dierential VSB extension the VIC connection is not used for technical reasons

Data may also b e fed back from the monitoring system into the data stream to allow imp ortant

slow control information eg HV currents to b e recorded together with the event

The drift chamb er readout uses pro cessors of the Motorola family throughout These

CISC pro cessors are relatively easily programmed at the native instruction level and all the

readout co de was written in assembler By splitting the workload b etween many pro cessors

each fullling a sp ecic task it has b een p ossible to avoid the use of an op erating system on any

of the readout pro cessors This has minimised resp onse times and maximised p erformance

Prop ortional chambers

Between and the solid angle seen from the interaction region is completely covered

bymultiwire prop ortional chamb ers Six indep endent planes in the forward direction four in

the central and also in the backward direction serve three dierent functions to deliver a fast

timing signal with a time resolution b etter than the separation of tw o succeeding HERA bunch

crossings to provide mo derately accurate space p oints for charged particle track reconstruction

at the rst level trigger and lastly to add an accurate track element in the backward direction

where the drift chamb ers fail to provide enough space p oints

The planar forward chamb ers FWPC are interspaced b etween the driftchamb ers of the

FTD describ ed ab ove and are exp osed to high particle rates increasing towards the b eam pip e

Hence minimum overall thickness and minimal amount of material traversed sucient ageing

prosp ects and catho de pad size adapted to increasing rates near the b eam pip e b ecame the

primary design criteria These p oints do also apply for the two cylindrical chamb ers in the

central region The inner one CIP is closest to the interaction region and covers the largest

solid angle In order not to degrade the track reconstruction of the surrounding drift chamb ers

the CIP and its outer partner COP were fabricated with low mass materials and a narrow

active gap Since the main purp ose of the FWPC COP and CIP is to provide space p oints

for the rst level trigger a pad segmented catho de readout was chosen with graphited surfaces

as in other chamb ers built for high rates From the reconstructed tracks the event

vertex can b e deduced and other detector data such as calorimeter and muon information can

be validated Since the trigger logic requests three space p oints p er track spurious background

hits from uncorrelated noise and synchrotron radiation are removed

In the backward direction the reconstruction of the scattered electron in low momentum

transfer even ts calls for an accurate track segment This is given by the signals from the four

dierently oriented ano de wire planes of the backward chamb er BWPC Several wires can b e

combined for triggering purp oses Standard planar chamb er construction techniques suced

here since more than one radiation length of electronics and cables from the central tracker

separate the BWPC from the interaction region The BWPC covers the front surface of the

backward electromagnetic calorimeter BEMC and hence also serves to discriminate electrons

and photons

The prop erties of all four chamber typ es are summarized in Table The front end electronics

and readout system is identical for all chambers

unit CIP COP FWPC BWPC

innerouter innerouter



active length zr mm



active zone starts at zr mm



mechanical length zr mm



total length zr mm



thickness rz mm



chamb er starts at zr mm



p osition of rst ano de rz mm



numb er of ano de planes

number of wires

wire separation mm

gap width mm

numb er of catho de pads

catho de resistivity k

 

length of pad zr mm to



width of pad

ano de wire tension N

plateau length V

plateau starts at V

Table Prop ortional chamb er parameters The separate columns for CIP and COP refer to

the two planes for the FWPC to the whole mo dule containing two planes

 

Inclusive preampliers only for the four outermost of the radial pads

 

rst co ordinate for CIP and COP second for FWPC and BWPC width increases with



radius r r wherer is the inner radius of the pad the ano de wire of each

i i i



successive plane are rotated by in active zone and at end anges

Forward prop ortional chamb ers FWPC

Each of the three chamb ers in the forward tracker volume consists of two wire planes interleaved

with three catho de planes The gap b etween the two adjacent catho de planes is mm wide as

indicated in Figure All chamb er frames are made of glass b er ep oxyTo reduce the mass in

the active area a laminated structure consisting of the following layers is used m graphited

mylar foil serving as catho de plane m printed circuit b oard carrying m Cu readout

pads mm Nomex mesh another mprinted circuit b oard covered with mCu

for the strips leading from each pad to the preampliers on the chamb er ends a further

m of graphited mylar foil in the central plane or aluminized mylar foil on the external planes

for electromagnetic shielding The graphite layers are pro duced by spraying a mixture of DAG

DAG at bars giving an initial surface resistivityofM whichwas reduced

to k by p olishing Eachchamb er is strengthened by a backplane mm thick with

twolayers of m glass b er ep oxy sandwiching mm Nomex The overall thickness is

of a radiation length The mechanical tensions of the wires and the foils are supp orted by

and axial ro ds on the external and internal frames resp ectively The ano de planes contain

gold plated tungsten wires m spaced by mm They are crimp ed on pins xed on

the frames Each wire is connected to the following one through M resistors and to ground

through nF capacitors Groups of wires are connected to separate HV lines which allows

degrading of malfunctioning sectors if necessary The catho de pads are ring shap ed and cover

an azimuthal angle of each except for the four outermost of the rings where they cover

The radial pad width increases with radius in geometrical progression from to mm

Two consecutive catho de planes are oset by one half of a ring such that the eective p olar

angle resolution is halved r r with r mm The Pluto gas

mini  mini

mixture see Table was chosen b ecause the FWPC share their gas volume with the forward

drift chamb ers and transition radiation detectors

A track crossing all three or at least two mo dules of the FWPC has to fall into the p olar angle

range or resp ectivelyFor such tracks an eective timing

resolution of ns FWHM and ns base width at of the maximum was measured

using H data well b elow the required resolution to separate two bunches

Central prop ortional chambers

CIP The laminar structure of the CIP called for sp ecial construction techniques

which are describ ed in detail in reference

The double layer of chamb ers consists of three concentric cylinders During construction each

chamb er cylinder was formed on a steel mandril milled to a precision of mover the full length

The innermost layer of the rst cylinder a m thick Alfoil provides the electromagnetic



shielding The next layermmthick Rohacell foam glued onto the Alfoil with gm

ep oxyglue gives the chamb ers the necessary rigidity The Rohacell surface w as p olished

and a second m Alfoil glued to it served as the inner catho de After cutting the cylinder to

the right length the Alfoils were connected to Cufoils at the ends and the glass b er ep oxy

end anges were added These carry the printed circuit b oards for the ano de wires whichare

supp orted further by glass b er ep oxy rings at and of the chamb er length The active

gap is mm wide The ano de wires gold plated tungsten m were transfered to the

axially prestressed cylinder from planar frames

The middle cylinder forms the outer catho de of the inner chamb er and the inner catho de of

the outer chamb er Here the innermost layeram Kapton foil is coated with high resistive

graphite k on one side and m Al on the other side The Al layer is segmented

into pads on which the induced charge on the catho de is collected The graphite layer in front

guarantees a fast disapp earance of the accumulated ion charge This has the advantage that

the readout wires of the pads can b e mounted outside the gas volume After several tests on

prototyp es the graphite layer in the nal chamber was pro duced by spraying a mixture of

DAG DAG and isobutylmethylketon IBMK in a ratio of onto the Kapton

foil with bar The catho de foils are again backed by mm Rohacell The readout wires

m Al are emb edded into m deep gro oves in the Rohacell running along the z axis from

the chamb er end z side to a hole centered over the pads The wires were contacted onto

the pads with silver paint and soldered at the ange end Another m thick Kapton foil

with Alcoating is glued onto the Rohacell which forms together with the wires a wave guide

of imp edance The Kapton foil again backed by mm Rohacell with a p olished surface

is covered by another m Al foil serving as the catho de for the outer chamb er End anges

and connections are similar to those of the rst cylinder and the sequence of layers for the third

cylinder is identical to that of the second

Gas sealing is provided bytwo Orings at the end anges mm The overpressure in the

chamb ers has to b e kept small and needs to b e monitored carefully in order not to distort the

gap The twochamb ers have indep endent gas distributions and are rotated by in with

resp ect to each other thus halving the eightfold segmentation of eachchamb er at the trigger

level by requiring coincidence of two planes In z there are pads of mm width in each

sector

With the gas mixture given in Table the single pad eciency measured in a test b eam was

while at HERA was measured with extrap olated jet chamber tracks From the

measured pulse height distributions the gap variations for this lightchamber were deduced to b e

less than mm The measured test b eam time resolution FWHM ns compares well with

the results at HERA This result converts into a probability to register a given pad with

the wrong neighb ouring bunch crossing The probability for crosstalk ie the probability

to register signals also in neighb ouring pads in z and and the ineciencies across the pad

b oundaries are discussed in detail in reference The average numb er of active pads for

crossing angles larger than in a test b eam compares well with what is observed at

HERA

COP The construction of the COP follows closely that of CIP in those asp ects

concerning the sandwich structure see Figure Steel mandrils machined to a precision of

m and appropriate to the larger chamb er radii were used To improve the stabilityofthe

sandwich structure the thickness of the core material Rohacell was increased to mm The



graphite catho des m area p er chamb er are pro duced with a screenprinting technique using

a resistor ink solution rather than spraying The ink has a resistivityofK for a

mlayer and was diluted with a solvent monobutylic ether of ethylene glycol in a ratio of

A surface resistivityofK was obtained after p olymerization at C during hour

The catho de pad structure is provided by gluing patches of m Kapton coated with m

and fold Cu to the back side of the graphite catho des giving an fold segmentation in z

segmentation in The catho de layer is backed by mm Rohacell in whichm diameter

Cu wires are emb edded A m Kapton foil coated with m Cu put on top of the previous

layer constitutes with the copp er wires the transmission line that carries the chamb er signals

to the z end of the chamb er This layer is then backed by mm Rohacell The Vetronite

G end anges of the chamb er supp ort the printed circuit b oards to which the ano de wires

p er chamb er are soldered and assure the mm chamb er gap size They form the

only rigid structure to which the gas distribution and preampliers are connected The three

cylinder sandwiches are assembled in vertical p osition Pulse height measurements showed that

the gapsize variation is of the order of mm

Despite its three times larger radius the COP is only mo derately thicker than CIP

radiation length instead of The eciency plateau is reached at V ab ove the CIP

plateau with the same gas mixture a consequence of the larger gap While in test b eams CIP

and COP b ehaved similarly at HERA the noise level in COP is slightly higher due to more

dicult grounding This requires a higher threshold setting and leads to a typical eciency of

The timing resolution is similar to that of the other chambers

Backward prop ortional chamb er BWPC

The BWPC is equipp ed with ve graphited catho de planes m Mylar foil and four ano de

wire planes It is the only chamberinHinwhich the catho des are not segmented and the

ano des are read out The graphite coating was fabricated with the same tec hnique as describ ed

for CIP The wires and the foils are stretched b etween a mm wide inner and a mm wide

outer ring of glass b er ep oxy G These rings are mm thick and sustain the active gap of

mm p er chamb er as indicated in Figure The wires are strung every mm but signals from

two neighb ouring wires are fed to one preamplier The wire orientations are vertical horizontal

and for the four layers Gas sealing and structural supp ort for the assembly is provided

by G front and back planes of mm thickness milled down to mm in the active zone

The latter starts at an inner radius of mm and ends at mm while the whole chamber

o ccupies the region b etweenn r mm and r mm The BWPC therefore covers p olar

angles of The space p oints given by the BWPC contribute mrad to

the angular resolution of the same order as the multiple scattering in the material in frontof

it For high energy electrons an eciency of p er plane was measured from extrap olated

CJC chamber tracks When requiring three out of four planes to b e hit in coincidence with the

BEMC an eciency of is obtained

Prop ortional chamb er electronics and readout

Preamplier AmplierShap er

Dierential gain nVe Max dierential gain

Rise time ns Rise time ns

Fall time ns Pulse width FWHM ns

Input imp edance Max output voltage V

Output load Overload recovery



Dynamic range mV e V V ns

in insat

Power supply V mW V V ns

in insat



Size mm Power supply V mW



Size mm

Table Characteristics of the MWPC preamplier and ampliershap er

Aschematic picture of the frontend electronics is shown in Figure The catho de pad signals

CIP COP FWPC and ano de wires BWPC resp ectively are preamplied directly on the

chamb ers A dierential signal is then transmitted through a m long cable to the electronic

trailer Each cable contains signal pairs and is connected to a receiver card containing shaping

ampliers followed by discriminators with computer controllable thresholds The characteristics

of the preampliershap er chain are listed in Table The overall gain can b e adjusted to

chamb er pulse heightbetween Ve and Ve by means of a resistor on the receiver card

Atypical equivalent noise charge is ab out e for a chamb er capacityofpF

The digitized signals are synchronized with the HERA clo ck and stored in a pip eline con

structed from the same gate arrays as used in the muon system see Section Up on a rst

level trigger decision LKeep the pip eline clo ck is stopp ed A second level trigger decision

LKeep then initiates the data readout The synchronized pad signals are furthermore made

directly accessible to the z vertex and forward ray trigger see Section of reference

Test registers allow controlling the readout and trigger chains

The MWPC readout system an indep endentbranch of the H data acquisition system

see Figure of reference is resp onsible for reading channels originating from

receiver cards in crates and some decision data from the two rst level triggers In addition

to the frontend crates the system consists of two standard VMEbus crates and one STC crate

in a conguration common to all H subsystems see Section of reference

The frontend crates are equipp ed with a customised EasyBUS which is essentially a sim

plied bit wide VME bus with a kWord address space lacking an yinterrupt capabilities

but with added analog and ECL signal lines The latter are used to distribute the clo ck and

LKeep signals The analog lines allow measuring the digitization thresholds loaded to the

discriminators through an ADC lo cated on a crate controller CC card The primary task of

the CCs is however to connect the crate to a branchdriver card BDC residing in the master

VME crate The BDCCC combination maps the EasyBUS address space into the VME frame

Each BDC is directly connected to the STC and contains a DMA direct memory access

controller and a Kbyte deep FIFO rst in rst out buer An LKeep signal can thus initiate

a frontend data transfer to the master crate without pro cessor intervention The maximum

transfer sp eed is Mbytes Each of the six BDCs installed in the MWPC area can control

eight frontend crates The latter are group ed into pairs to make use of the bit wide data

path of the VME bus To optimise readout sp eed b etween two and six crates are connected to

one BDC

The rst order dead time is determined by the frontend transfer to the BDC as long as the

BDC FIFO are not saturated The saturation rate is given by the average time sp entbythe

data acquisition pro cessor p er event Details of the data acquisition program are available in

references An average time of ms p er event is needed This corresp onds to an average

of hits in bunch crossings

Gas systems

To op erate the nine dierenttracking detectors nine separate gas circuits are necessary with

dierent gas mixtures ows and demands on purity and overpressure control For the forward

chamb ers and CJC closed circuits are used while CIZ COZ CIP COP and BWPC are ushed

with premixed gases in op en circuits The main parameters of the gas systems are given in

Table

Detector Gas Gas mixture Pressure relative Flow rate System

volume additives to atmosphere

volume ratio typ max typ max circuit

l hPa lmin typ e

Planars ArC H C H OH I

  

FWPC closed

Radials Phase I ArC H

 

Phase I I XeC H He

 

C H OH

 

Radiators HeC H op en

 

CJC Phase I ArCO CH II

 

closed

CJC Phase I I ArC H H O

  

CIZ ArC H H O III

  

op en

COZ ArC H C H OH

   

CIP ArC H FreonH O

  

COP ArC H Freon

 

BWPC ArC H Freon

 

Table The dierent circuits of the gas systems

Gas circuits

The simplied diagram of the gas circuit of the planar chamb ers shown in Figure illustrates

the typical features of the gas systems The system is distributed over three levels the supply

outside the H hall the control ro om on the rst underground o or and nally the distribution

rack on top of the electronics trailer near the detector At the latter p oint the gas inlet owfor

each detector is adjusted bymechanical ow meters and for some chamb ers split into several

streams for further distribution as shown in Figure The static pressure of chamb ers relative

to atmosphere is measured with sensors in the bar range In order to avoid to o large hydrostatic

pressure dierences b etween chamb ers and sensors the latter are also lo cated at this p oint

From the inlet manifold either pure or premixed gases can b e fed into the circuit Flushing

is done by gently lling helium or argon via the twoow meters FL and FL into the

chamb ers while the chamb er gas at the same time is sucked out by the membrane pump CP

To hold the chamb er pressure during the whole op eration within adjustable tolerances of ab out

bar the solenoid valves SV and SV will b e either op ened or closed dep ending on

the actual pressure inside the detector As seen from Figure the ingoing and outgoing ows

of the chamb er gas are split into two paths one of them containing instruments for continuous

gas analysis like infrared meters a hygrometer and a gas chromatograph in combination with

an oxygen trace analyzer The lling of the chamb ers pro ceeds in a similar way as the purging

either with premixed gas or byintro ducing approximately the right prop ortions of rst the

nonammable and later the ammable gases Then inlet and ventvalve are closed and the

circuit is switched from the op en to the closed mo de The gas circulates through the barrel

the purication units if needed through an alcohol or water bath and through the chamb ers

Since the purication units absorb part of the gas comp onents particularly hydro carb ons a

readjustment of the mixture is necessary after typically one day of circulation To maintain

the correct mixture gas can b e added to the barrel manually Rep eated circulation for several

days esp ecially when additives likewater or alcohol are used leads then to a homogeneous gas

mixture constant in time

So far three typ es of additives are used Some mixtures contain Freon as one of the

comp onents of the premixed gas To other delivered mixtures alcohol typically or water

typically ppm is added by passing the gas over a bath of the co oled or frozen liquid stored

in a refrigerator in temp erature controlled reservoirs The admixture is adjusted byvarying the

bath temp erature

Purication and analysis

The closed lo op circuits are supplied with purication units for removing oxygen water and low

concentrations of higher organic comp ounds For oxygen removal kg BTScatalyst R

in the reduced state is used as an absorption agent and oxygen levels as low astoppm

have b een reached over long time p erio ds Optimal oxygen removal is obtained with catalyst

temp eratures of C to C However in the case of ethanol admixture as is foreseen

for the planar chamb ers the alcohol will b e cracked Working at temp eratures b elow

C circumvents this problem at the cost of a lower oxygen capacity for the purier of only

ab out to l O kg catalyst A similar problem arises when isopropanol is added to the



chamb er gas which is recommended for Stablohm wires and the radial chamb ers Since

the isopropanol molecule is more fragile than the ethanol molecule it is cracked even at ro om

temp erature into hydrogen and acetone by the catalyst Use of other O puriers working



at lo w temp erature like Oxisorb and palladiumcatalyst give similar problems with

alcoholadditives esp ecially with isopropanol so that up to now isopropanol could not b e used

in the closed circuit of the radial chambers

At ro om temp erature water and higher organic comp ounds are removed by a mixture of

kg A and kg A molecular sieves In case of water or ethanol additives the molecular

sieveeventually saturates but it is still capable of removing other impurities Both molecular

sieve and BTScatalyst are regenerated twice p er year or whenever necessary

Continuous control of gas comp osition is necessary for constant op eration Infrared meters

dedicated to a certain gas typ e but with some sensitivity left for the gas additives give p ermanent

information on changes Hygrometers in the ppmrange and an O trace analyser allow an early



detection of leaks Complete analysis of the gas comp osition is p erformed by an automatic gas

chromatograph station routinely switched into the dierent circuits Indep endently of the use

of calibrated gases this instrumentgives the dierent gas p ortions to an accuracy of of

the measured value with an overall sensitivity of ab out ppm

Electronic control and safety

The concept of the H gas system control follows the solution chosen for L time expansion

chamb er TEC A Motorola CPU serves as a crate master integrated into a

VMEsystem with the necessary resources for monitoring logging and control equipment The

instantaneous values of all analog outputs of the measuring devices esp ecially those for pressure

and temp erature but also those for supply voltages are controlled within preset limits Warnings

or alarms are generated if one of the relevant parameter values is exceeded In case of an alarm

the gas circulation is stopp ed and the HV supplies of the detectors concerned are switched

o A computer indep endent hard wired logic with a more generous alarm setting protects the

chamb ers against destruction in case of program failures or other accidents In this case also an

alarm is generated and the p owerless op en solenoid valves in the distribution rack on top of the

electronic trailer connect the chamb ers with an argon ushed reservoir at atmospheric pressure

as indicated in Figure A set of four indep endent serial links p er gas system monitors all

gas parameters and distributes this information to the slowcontrol system see Section of

reference

Gas sensors are distributed in the H detector region on the electronic trailer with the

distribution rack and in the volume o ccupied bythetrackers as well as in the ro oms where

ammable gases are handled



The tracker volume is ushed with m of nitrogen gas p er hour to preventaccumulation

of ammable gases in case of a leak Since the op erational pressure of most chamb ers is as low

as hPa relative to atmosphere and only hPa in case of CJC the amountofgaswhic h

may escap e through a sudden leak in the chamb er region is at most only a few liters Small

continuous leaks are b est controlled in the closed lo op circuits by measuring the pressure drop

in the barrel over several days The maximum working pressure in these circuits is limited to

bar absolute A typical leakage of ab out lday corresp onds to a pressure drop of hPaday

In the op en circuits additional electronic owcontrols in series with FL and FL restrict

the input ow In case of a ma jor leak the op erational chamb er pressure cannot b e reached with

the low ux adjusted by these controls

Scintillators

Both scintillator arrays discussed in this section are lo cated in the backward region see Figure

of reference and have b een installed to reject proton b eam asso ciated background at the

rst trigger level The present life time of the stored proton b eam in HERA during collisions



varies b etween and h The stored proton current design value is mA with

circulating protons in total These protons are lost by b eam gas and b eam wall interactions

pro ducing background showers of energetic p enetrating and halo muons With a b eam

life time of h the H sensitive detector volume is hit by this background with a frequency of

MHz

Timeofightcounters

The time of ight ho doscop e ToF consists of two planes of cm thick NEA scintillator

mounted p erp endicul ar to the b eam pip e upstream of the interaction region Particles from

proton induced background and from e p collisions are separated in time at this p ointby

ns The electron bunches have negligible size whereas the proton bunches are spread over to

ns FWHM The plane nearest to the interaction p ointToF lies at z m and has



butted counters measuring mm thus matching the size of four BEMC stacks The



outer plane at z m consists of eight larger counters mm

In order to op erate inside the T eld ToF utilises Hamamatsu R high eld

photomultiplier tub es PM It is necessary to mount them p erp endicul ar to the planes of ToF

requiring a light collection countersink to b e machined into one of the large faces A corresp ond

ing p ersp ex truncated cone is glued to the other side to match the PM sensitive area The PMs

themselves are housed in nonmagnetic holders and held in contact with the small light guide

by springs

Eachwall of ToF is made up of a sandwichofscintillator and lead Figure mounted on

a backing plate of nonmagnetic steel to minimise stresses from the large magnetic eld The

lead is mm thick to absorb synchrotron radiation Steel is used rather than aluminium to

minimise eddy currents pro duced during a magnet quench

The six inner coun ters four on ToF twoonToF can b e moved horizontally up to cm

from the b eam pip e using computer controlled pneumatic rams This removes them from the

high radiation uxes around the b eam pip e during injection With the counters in the op en

p osition ToF can b e split in half ab out the horizontal axis allowing removal without breaking

the vacuum in the b eam pip e

Signals pro duced by the PMs are amplied up to V b efore travelling down m

of cable to a NIM logic lo cated in the electronics trailer Here the signals are discriminated and

strob ed in three time windows background interaction and global which are used in the rst

level trigger decision see Section of reference available after ns The device as a

whole has a resolution of ns while individual counters have a resolution of the order of ns

The timing information of all counters is available in the event readout chain

The setting and width of the time windows greatly aects the p erformance of ToF and

they are continually up dated as oine analysis pro ceeds The background window currently

starts ns b efore the centre of the background distribution and is ns long The interaction

window starts ns after the background window ends and is ns long Figure A constant

background of cosmic ray hits is present ab out entries p er bin Triggers in the interaction

window are in fact much dominated by synchrotron radiation

The veto wall

In addition to the ToF device two double scintillator veto walls are installed at a distance of

and m resp ectively upstream from the interaction p oint see Figure of reference



The smaller inner veto wall covers the near b eam area cm down to a radius

of cm Figure The four scintillator pairs NE thickness mm are read via two

photomultipliers AVPVALVO each The pairs are shielded against electromagnetic showers

by lead walls of cm thickness Penetrating particles are then identied by coincidences b etween

two scintillators with a time resolution of ns The large outer veto wall with an area of



ca m overlaps the inner veto wall and nearly all of the liquid argon calorimeter The



area each Figure is group ed around the last arrayofcounter pairs of up to m



upstream HERA quadrup ole with a m sized hole The scintillators NE cm

thick are coupled to inch phototub es of typ e VALVO XP These tub es are shielded

with thick iron tub es and metal cylinders against the magnetic fringe eld mT

An iron wall of cm thickness separates the scintillator pairs of the outer wall The coin

cidence resolution of suchpairsis ns It is dominated by the light path dierences over

the large area The lightattenuation length is measured to b e larger than m and leads to



ineciencie s for the detection of minimum ionizing particles of see also references

The time resolution achieved allows a clear time separation b etween the back

ground of the passing proton b eam and event correlated hits during ebunch passing A m

concrete wall separates the outer veto wall from the main detector and protects it against low

energy showers from upstream

Amplitudes signal arrival times rates and eciencies of all counters are monitored online

and this information is used to study the background condition after each lling and during

runs The time of ight information allows to measure the z p osition of the e p interaction

p oint online with a precision of ca cm It is used in the rst level trigger see Section

of reference and is sent to the central data acquisition system for oline analysis

Calorimetry

The H detector was designed to provide clear identication and precise measurement of elec

trons muons and p enetrating neutral particles together with go o d p erformance in the measure

ment of jets with high particle densities These requirements were b est met by a calorimeter

inside a large coil to minimise b oth the amount of dead material in front of the electromagnetic

calorimeter and the overall size and weight of the calorimeter

The main reasons for cho osing the liquid argon technique were go o d stability and ease of

calibration ne granularityfore separation and energy ow measurements as well as homo

geneity of resp onse

Figure a shows the longitudinal view of the calorimeters along the b eam axis and Fig

ure b shows a transverse view of the LAr calorimeter with the wheel structure that is describ ed

b elow The LAr calorimeter covers the p olar angular range b etween and The

calorimetric coverage is completed with a small calorimeter in the proton direction PLUG

with copp er absorb er and silicon pad readout covering the region b etween the b eampip e and

the liquid argon cryostat and a lead scintillator backward electromagnetic calorimeter

BEMC lo cated in the electron direction after the tracker and covering angles

The tailcatcher system TC is used to provide a rough calorimetric measurement of hadronic

particles leaking out of the LAr calorimeter and is based on the analog readout of the pads of

the limited streamer tub es that instrument the iron yoke

In the next section the LAr calorimeter is describ ed descriptions of the BEMC the PLUG

and the TC can b e found in sections and resp ectively Further details on the

instrumentation of the iron yoke are given in the section on the muon detector see Section

For a more detailed description of the LAr calorimeter system we refer to

The liquid argon LAr calorimeter

Cryostat and cryogenic system

All walls are made of stainless steel except for the inner ones of the warm and cold vessels

around the b eam pip e and the tracker which are made of aluminium alloy to minimise the dead

material in front of the electromagnetic calorimeter EMC The cold vessel is able to withstand

a maximum pressure of bars and to supp ort the weight of the calorimeter mo dules t and



of the liquid argon load m Co oling down to LAr temp erature is achieved by circulation of

helium gas co oled through an external heat exchanger whichisremoved when no longer needed



The LAr load is transferred from a m storage tank lo cated at ground level ab out m ab ove

the detector into the cryostat through the b ottom of the cold vessel A regulated ow of liquid

N through heat exchangers lo cated within the cold and expansion vessels ensures temp erature



and pressure regulation bar Control of all pro cesses including co oldownwarmup and

llingemptying is done by a system controlled by VME pro cessors Since op erations started in

early the calorimeter has remained at liquid argon temp erature and most of the time full

of liquid argon except for the few days needed to move the detector in or out of the b eam For

more details to this system we refer to

Liquid argon purity

A liquid argon purity monitoring system has b een integrated into the LAr cryostat to checkthe

stability of the ratio of energy loss to collected charge to the level of The basic sensor is a

liquid argon ionization chamb er to which an electric eld of Vmm is applied corresp onding

 

to the nominal eld applied to the calorimeter stacks Its catho de is coated with a Bi source



of Bq activity The energy sp ectrum of the radioactivedecays is continuously monitored

The data from such prob es distributed around the cryostat show that the signal attenuation

due to p ollution from the stacks is less than p er year

Stack design and construction

The segmentation along the b eam axis is done in eight self supp orting wheels as shown in

Figure each of them segmented in into eight identical stacks or o ctants The twoforward

wheels are somewhat similar in the principle but mechanically assembled as two half rings An

eort was made to minimise dead regions due to cracks

Common features for all active cells are pad readout on the ground side and a high resistive

coated high voltage plane except for the CBH stacks with integrated decoupling capacitance

as describ ed b elow

The hadronic stacks are made of stainless steel absorb er plates with indep endent readout

cells inserted b etween the plates They dene the rigid structure on to which the corresp onding

electromagnetic stacks are mounted The orientation of the absorb er plates is such that par

ticles are incident on the calorimeter with angles not smaller than The structure of each

electromagnetic stack consists in a pile of Gep oxyglass b erPbG sandwiches separated

by spacers dening the LAr gaps The basic sampling cell is shown in Figure a It consists

of mm Pb absorb er and mm liquid argon as active material with p er gap one readout

plane with pads and one high voltage plane coated with high resistivepaint HRC The latter

is a mixture of carb on and glue with a surface resistance of M sieveprinted on a

Kapton foil The high resistivity coating pro vides the HV protection and serves as a distributed

decoupling capacitytokeep negative crosstalk small The hadronic sampling cells as shown

in Figure b consist of a total of mm stainless steel mm absorb er from the welded

structure and twice mm from the plates of the indep endent readout cells dening the active

liquid argon gap and of a double gap of mm liquid argon They have in the middle of the

active gap a G b oard with pads on b oth sides to collect the charges dep osited in the gaps A

Kapton foil coated byalayer of HRCIFHFBHOFstacks or with copp er CBH is glued

to the inner side of the stainless steel plates with the same functions as for the electromagnetic

mo dules The HV is applied to the HRC or copp er for CBH in which case neon spark gaps

mounted close to the gaps act as active protection For more details we refer to

The basic calorimetric material constants are given in Table of reference The granu

larity of the readout cells stems from the requirements of a go o d separation of electromagnetic

and of hadronic showers Longitudinal segmentation is and fold for the EMC over to

radiation lengths X and to fold for the hadronic calorimeter HAC overtointerac

tion lengths Furthermore the tower sizes are such that the channel capacities are kept b elow

nF so that the electronic noise is at a reasonable level with the additional constraint from

the calorimeter trigger that channels b elonging to the same trigger tower should have similar

capacities within for go o d timing adjustment

The high voltage distribution is done by indep endent lines Each line feeds a group of

non consecutive planes in a stack interleaved with planes linked to another HV line to reduce

the probability that a complete tower segmentbedeadincaseofahighvoltage problem in one

line The present op erating voltage of the calorimeter is kV which corresp onds to an electric

eld of Vmm The very go o d purity observed allows high charge collection eciency ab out

at this low eld value thus minimizing HV problems After years of op eration

less than of the high voltage lines do not reach the full voltage

Electronic system

A ma jor constraint in the design of the system is that large energies may b e dep osited at short

time intervals ns at HERA into detectors with large capacities and long collection times

and the information has to b e stored until the arrival of the trigger signal s The basic

layout of the electronic chain is describ ed in more detail elsewhere The preampliers

each with two shap ers a slow one and a fast one are lo cated just outside of the cryostat and

feed on one hand the analog readout system where the signals of the slow shap ers are read

out via twomultiplexers giving an overall multiplexing factor of and on the other hand

the trigger read out system where the outputs of the fast shap ers are pro cessed see Section

of reference To extend the dynamic range to bits while using a bit ADC a

double transmission system with two dierent gains for ab out of the channels is used thus

increasing the number of channels to b e readout to ab out electronic channels The

signals are senttwice via m twisted pair lines to dierential line receivers lo cated in the

analog receiving unit ANRU which p erforms analog baseline subtraction Each ANRU

serves calorimeter channels and is connected to an ADC b oard serving electronic

channels that is controlled and read out by a digital signal pro cessor DSP mo dule p erforming

data correction This readout system is describ ed b elow section The total amountof

channels where no signal reaches the preamplier b ecause of bad contacts within the cryostat is

and has remained stable for ab out three years after closing the cryostat

Electronic calibration system



To ensure that the calibration of the electronic chain is known and stable to within a few

calibration capacitors of pF selected to b e within are used They are charged with



voltage pulses of precisely known amplitude

Two systems have b een built into the calorimeter the rst one cold calibration with

the calibration capacitors in the liquid argon as close as p ossible m to the gaps pulses

individual channels one out of allowing detailed cross talk studies The second system with

calibration capacitors at the preamplier level warm calibration is used mainly as a backup

for calibrating channels with a problem in the calibration line within the cryostat In this case

an extrap olation technique develop ed during the runs in test b eams at CERN is used and a

precision of the order of in the determination of the calibration constants is achieved This

metho d is presently applied to less thanofthecalorimeter channels

A third order t to the calibration data is p erformed for eachchannel from whichthe

constants to b e downloaded into the DSPs are determined At H such op erations are done once

every few weeks Figure shows the stability of the calibration constants over one month

The calibration constants need no correction for diagonal crosstalk as they are determined

by pulsing the cells individuall y using the high granularity cold calibration system Non diagonal

crosstalk has b een determined from the test b eam data and was found to b e small

mainly aecting the CBH mo dules

Calorimeter data acquisition

The calorimeter data acquisition system reads out data from the LAr calorimeter the BEMC

the PLUG calorimeter and the analog part of the instrumented iron TC These detectors have

the same readout electronics starting from the ANRU The LAr calorimeter yields most of the

data and its readout is describ ed here At the preamplier level the data are split into two paths

as mentioned in section In the analog data path the rst level trigger decision samples

the slow shap er pulse at its maximum At the level trigger L s after the collision the

analog to digital conversion of the electronic channels is started total enco ding time is

ms The ADC counts of all electronic channels are then converted into calibrated charges

by DSPs working in parallel The DSP b oards used here are based on the Motorola

DSP and p erform for each cell a noise suppression done in parallel to the enco ding and

an order three p olynomial correction These DSPs provide calibrated charges formatted with

the oine numb ering of the calorimeter cells Onb oard memories are downloaded with the

current set of calibration constants for eachchannel four parameters and the noise value are

needed The co de contains less than instructions It is written in assembler language and

was optimised to t into timing sp ecications and the available program memory space in the

DSP chip

In the trigger data path the pip elined trigger chain pro duces digital sums for eachofthe

bunch crossings following the collision A rst level trigger decision L based on total and

transversal energies is derived within s Ten dedicated DSPs read the data of the fast

shap ers see Section of reference They verify the timing and the shap e integrity

of the trigger tower signals calculate pileup estimators based on charge and time analysis and

rep ort any malfunctionings They store the signal history of a total of trigger towers

over bunch crossings around the trigger time t From these data every second sample in

the interval ranging from to bunch crossings is read out for pileup studies The DSP

b oards used in this path are based on the same DSP chip as for the analog data read out but

are of a dierent design with a sp ecial interface to the trigger data

The formatted data for b oth paths within indep endent VME branches are collected bytwo

event builders based on the RISC pro cessor AM running the real time kernel VRTX The

AM event builders one for the analog data and the other for the trigger data run on top

of the real time kernel VRTX with minimal system overhead The data are passed to the event

logging task through a circular buer The event is then formatted and sent to the central data

acquisition through an optical b er link see Section of reference

Presently with an event size for the calorimeter branch of ab out Kbyte and a rst order

dead time of ms the maximum data taking rate has b een measured to b e Hz dead

time At a rate of Hz the deadtime is

A pro cessor based on the Motorola chip and op erating under an OS system is used

for run control and as a stand alone facility

Reconstruction techniques

Input to LAr calorimeter reconstruction are calibrated charges for each calorimeter cell as

provided by the DSPs The calorimeter reconstruction program converts charges to energies in

the calorimeter cells for b oth hadronic and electromagnetic showers corrected for the eects of

dead material eliminates electronic noise and forms clusters from groups of cells

The scaling from charge to energy electromagnetic scale see Section involves a charge

to energy calibration factor determined for each stack geometry in calibration runs at CERN

see Section a correction for the charge collection eciency for op erating at V derived

from HV curves obtained with cosmic muons and correction factors for lo cal variations of

gap and absorb er thicknesses measured during stack construction

The noise is measured for eachchannel during electronic calibration It varies b etween and

MeV equivalent energy dep ending on the calorimeter region see Table In events recorded

with a random trigger cells out of a total of cells pass a noise threshold on

CB IF

EMC MeV mips MeV mips

HAC MeV mips MeV mips

Table Approximate energies and minimum ionizing particle equivalents mips corresp onding

to noise in the electromagnetic and hadronic sections of the central barrel and inner forward

mo dules resp ectively

average Adding up this energy for the full calorimeter yields an average value of GeV with

a standard deviation of GeV Figure a To suppress the noise further we use the negative

noise present in the gaussian distributed noise signals after p edestal subtraction to comp ensate

the p ositive noise contribution to the measured signal Wekeep cells ab ove signal seed

and all neighb ours in a cub e around a seed cell also to keep small signals

at the fringe of showers In order to comp ensate for noise picked up in the previous step also

cells b elow around a signal seed are kept Cells b elow are kept in order to comp ensate

for noise contribution to seed cells No neighb ours are collected around these cells

which are purely noise After this pro cedure the residual noise contribution is GeV with a

GeV Figure b

The signal loss intro duced by the ab ove noise suppression pro cedure has b een studied with



simulated low Q DIS events In these events the hadronic energies are low with average

dep osited energies in the barrel region of the calorimeter of ab out GeV MeV for hadrons

and MeV for photons In this most dicult case of the energy is lost due to this

  

noise suppression For high Q events Q GeV the loss is smaller These

losses are corrected for in the reconstruction of hadronic energy see Section

For simulations noise is included for eachcellby using events recorded with random triggers

in sp ecial runs with no online noise suppression

Clustering All cells passing the cell level reconstruction are sub ject to clustering

The algorithms used are tuned so that the cells containing energy dep ositions from an electro

magnetic shower initiated by a photon or electron are most probably merged into one cluster

Hadronic showers on the other hand with their large spatial uctuations are in general split

into several clusters

Further noise suppression Clustering allows further reduction of the noise in the

hadronic part of the calorimeter A p enetrating deeply inside the calorimeter usually

dep osits enough energy to form at least one cluster with a signal well ab ove the noise level

Other small isolated energy dep ositions which are not distinguishable from noise are correlated

in space with this prominent cluster

Small signals are suppressed if they are in the last layer of EMC or in HAC and far away

cm from the direction given by the centre of gravityofany prominent cluster signicance

p

P



E ab ove and the nominal interaction p oint

i noise

This suppression do es not increase the signal loss mentioned in Section The energy

distribution of noise remaining in emptyevents after the suppression p eaks at zero with a sigma

of GeV as can b e seen in Figure b

Correction for energy loss in dead material The energy losses in dead material

in front of the calorimeter the b eam pip e the central tracker and the inner cryostat wall and in



cracks b etween the calorimeter stacks are quite substantial In low Q DIS events they amount

to of the energy dep osited in the calorimeter dead materials in front of the calorimeter

accounting for ab out of these

Corrections for the energy loss were derived using Monte Carlo simulations The eventby

event corrections are based on the measured calorimetric energies To reduce the inuence of

noise on the correction only cells with energy ab ove for cells in prominent clusters see

noise

Section and ab ove otherwise are considered

noise

Energy losses in front of the LAr calorimeter are corrected by using the rst inner layer of

cells in the LAr calorimeter For each cell in the rst layer with a signal ab ove the threshold

mentioned ab ove an energy is added according to

i i

E f

fr

loss dead

i

Here f is the energy loss of a minimum ionizing particle in the material in front of cell i

dead

in pro jective geometry with resp ect to the nominal interaction p oint A global factor was

fr

determined for each half wheel along the b eam direction bysimulation For the ab ov e energy

estimate we use only the fact of the presence of an energetic cell but not its energy This

approach allows a common correction pro cedure for losses caused by electrons and hadrons

The correlation b etween the estimate of the energy losses in the reconstruction and the true



energy lost in front of the calorimeter for simulated low Q DIS events is given in Figure An

example of the eect of the dead material correction for exp erimental data is shown in Figure

where the p eak in the eective mass of two photons em clusters is moved by the correction

into the region of the mass

The correction pro cedure for energy losses in a crack uses cells in the layers nearest to the

crack and on either side of it Cells on one side of a crack are coupled with cells on the other

side and for eachsuch pair an energy loss b etween them is estimated by

j j j j

j j

E f E E E E

r r

loss dead l l

j

j

distributed b etween the two cells of a pair in prop ortion to the cell energyHereE and E

r

l

j

are energies in a pair j dep osited at left and right sides of the crack The function f takes

dead

into accoun t lo cal inhomogeneities of dead materials A global factor was determined for each

typ e of a crack These factors dier considerably for pions and electrons For the moment

only corrections of hadronic typ e are used in the reconstruction b ecause of diculties in the

separation of hadronic and electromagnetic comp onents in and z crack regions

Figure shows the p erformance of the dead material correction as function of and for

simulated pions of GeV The crack structure which is clearly seen b efore the correction nearly

vanishes after the correction The CBCB z crack almost p ointing to the interaction p oint

was scanned by a pion test b eam of GeV at CERN Results are given in Figure The

resp onse across the crackiswell describ ed in simulation

The hadronic energy scale The LAr calorimeter is non comp ensating The charge

output for hadrons is ab out smaller than for electrons Therefore an additional correction

has to b e applied to the signal obtained on the electromagnetic scale

The ne segmentation of the LAr calorimeter allows to distinguish the primary electromag

netic comp onent of a jet which is already on the correct electromagnetic energy scale It also

allows a high level of comp ensation within hadronic showerstobereached byweighting signals

from individual calorimeter cells see b elow

The primary electromagnetic clusters are ltered using suchcharacteristics as the fraction of

cluster energy dep osited in EMC containment in EMC in the rst layer of EMC early shower

development and in the four most energetic cells of a cluster compactness see reference

The ltering is done for clusters with an energy ab ove GeV

The hadronic ob jects in the reconstruction are formed by cells which are not included in

an electromagnetic cluster and are lo cated within a radius r around the direction given bythe

nominal interaction p oint and the centre of gravity of the hadronic cluster r cm in EMC

and r cm in HAC Here a cluster is called hadronic if it is prominent see Section

and if it is not recognized in the ltering as an electromagnetic one or at lower energies if it is

developing deeply inside the calorimeter

To get the prop er hadronic scale for hadrons a software weighting technique is applied

whichwas initially prop osed by the CCFR Collab oration and used in the CDHS exp eriment

This metho d was further develop ed by H on the basis of CERN test runs

The aim is to equalize the resp onse to the electromagnetic and hadronic comp onents

of a hadronic shower and therefore to suppress the inuence of the large uctuations in the

hadronic shower comp osition on the reconstructed energy The technique exploits the fact that

lo cal energy dep osits of high density are mainly of electromagnetic origin while the hadronic

comp onentismuch more spread out Thus in a well segmented calorimeter the amount of energy

dep osited in the cells can b e used for statistical separation of electromagnetic and hadronic

energy dep ositions

i

In the reconstruction the weighted energy in a cell i E is calculated from the cell energy

rec

i

on the electromagnetic energy scale E by

i i i i

V gE fa a expE E



rec

where a a and are the parameters of the weighting function dierent for EMC and for



i

HAC and V is the volume of the cell These parameters were determined as function of the

reconstructed jet energy calculated inside cones of using a Monte Carlo simulation of jets

For hadrons with energy b elow GeV this ansatz is replaced by simple multiplicative

factors corresp onding to eective e ratios in EMC and HAC In the region to GeV

b oth metho ds contribute to the correction in order to get a smo oth transition from the simple

correction factors to the weighting

The remaining cells not included into electromagnetic clusters or hadronic ob jects are due to

low energy particles dep ositing energy in the rst two three in the forward region inner layers

of the calorimeter These leftovers are aected by noise and the energy correction to b e applied

dep ends on particle comp osition and energy sp ectra The corresp onding correction factors were



dened using simulated low Q DIS events

Calibration and p erformance

The most imp ortant task in understanding the calorimeter mo dules is the energy calibration

This was done by putting full scale calorimeter mo dules in a test b eam at CERN Checks of the

calibration qualitywere done once the H detector was fully op erational by using various tech

niques as describ ed b elow such as determining the resp onse of the electromagnetic calorimeter

to electrons generated by cosmic muons crossing the detector or verifying the P balance b etween

t

the electromagnetic and the hadronic energy in deep inelastic events at HERA

Overview of the test runs at CERN An extensive calibration program with

e and b eams was p erformed in the H test b eam at the CERN SPS with prototyp es

and with mo dules installed later in the H cryostat at HERA These b eam

tests supplied the basic calibration constants of the calorimeter

Only one of eachtyp e of the calorimeter stacks was tested as the very strict mechanical

constraints see references needed to reach a homogeneityatthelevel were achieved

during the construction phase allowing to transfer calibration constants from one mo dule to

another

Eightcharacteristic stack congurations were tested separately using the same b eam setup

calorimeter readout and calibration electronics These congurations include a full coverage

of and all imp ortantcrack congurations Sp ecial mo dules consisting of half stacks

assembled to repro duce a CBCB crack see reference and an FBFB cracksee

references were built and put into the test b eam in

The purity of the liquid argon was constantly monitored by prob es identical to those used

in the detector describ ed in section The decrease of the signal with time was much faster

than in the H detector b ecause of p olluting agents broughtby the stacks It was not p ossible

to use the same ushing and co oldown pro cedures for the test setup as in the nal detector

Big variations in the p ollution rate from one conguration to the next were attributed to the

dierent cleaning agents used during the construction of the stacks whichwere built at v arious

institutes

The same front end electronics scheme and calibration system as at HERA was used as much

as p ossible Data were taken with b eam energies in the range to GeV for electrons and

to GeV for pions

In some of the data taking p erio ds a tail catcher mo dule was added b ehind the hadronic

calorimeter allowing combined analyses The tail catcher mo dules were also calibrated

in standalone tests

Test b eam results For the electromagnetic energy scale two calibration constants

exp exp

c c were determined for each wheel which transform the measured electric charge

EM C HAC

MC MC

Q p er cell into energy dep osited by electron showers Corresp onding constants c c

i

EM C HAC

transforming visible energy into dep osited energy are obtained in Monte Carlo simulations MC

for electrons of GeV These constants are dened to b e indep endent of eects of dead

materials in front of the calorimeter anyleakage and analysis cuts

exp

is obtained by a comparison see Figure The corresp onding exp erimental constant c

EM C

of exp erimental data with detailed simulation of the test setup and requiring the reconstructed

energies to agree

EM C EM C

X X

exp

MC exp vis MC

Q E E E c c

i

rec rec j EM C

EM C

i j

exp

For the calibration constanta value of c GeVpC is obtained on average For the

EM C

exp

GeVpC was obtained by scaling hadronic stacks no electron data were available and c

HAC

the value of the EMC by MC

p

The resolutions E obtained for various stacks are in the range to E with con

stant terms b elow Figure shows the results for four dierentstacks and the parametriza

tion for FB according

q

   

E B E C E A

p

with A E B MeV and C The measured resolutions dier at low energies

due to dierent handling and inuence of electronic noise for the various stacks The observed

non linearities are b elow after corrections for eects of dead material and noise by Monte

Carlo

The calibration constants of the various stacks were found to vary by ab out This is

larger than exp ected from the known mechanical dierences of dierent wheels The main error

source were impurities in the liquid argon during the CERN test The variation is consistent

with the systematic error of the extrap olations of the high voltage plateau curves by which

the charge collection eciency was determined Further tests of the energy scale are p ossible at

HERA see b elow For further results on the calibration by test b eam electrons and simulations

we refer to and for more details to

The resp onse to pions has b een extensively studied for the dierent calorimeter wheels and

compared to detailed simulations compare references An application

of the standard H reconstruction co de section is shown in Figure where data and

GHEISHA simulation for pions at GeV are compared in dierent wheels on the

electromagnetic scale and after reconstruction of hadronic energies No attempt is made here to

correct for leakage The eect of the inclusion of the streamer tub e tail catcher see Section

and reference which adds at the test b eam another interaction lengths to the of

abs

the IF wheel can b e seen in Figure It shows the reconstruction at a pion energy of GeV

for all events and for those fully contained in liquid argon The obtained resolutions are ab out

p

E E with an energy indep endent termofasshown in Figure

Performance at HERA Data taken at HERA since April with cosmic

muons and since June with b eams allowed for checks of b oth the overall electromag

netic and hadronic energy scales

The orientation of the three CB wheels is esp ecially favourable for the study of the signals

from cosmic muons and allowed to check the charge collection the overall calibration and the

time stability The charge collection eciency at the op erating voltage of kV was determined

by high voltage plateau curves to b e The electromagnetic energy scale as determined

at the CERN b eam tests see ab ove could b e veried to More precise tests are

p ossible with electrons see b elow

The overall resp onse to muons of the individual electromagnetic and hadronic sections of the

three CB wheels varied from Octob er to November by less than

A fraction of the cosmic muons traversing the detector generates electrons Their momentum

p can b e measured in the central tracker CJC and can b e compared with the energy E measured

mainly in the CB wheels A typical eventisshown in Figure together with the measured Ep

distribution for selected electrons with p GeVc and incident angles b elow with resp ect

to the normal of the calorimeter plates The mean and width agree with

p

the simulation within errors The width corresp onds to a resolution of E E but

this value is still inuenced at these energies pGeVcby noise and dead material

corrections section of ab out

With these techniques the forward wheels cannot b e reached but the p erformance of IF and

FB wheels can b e checked bytwo photon mass sp ectra as demonstrated in Figure which

shows a clear mass p eak

Deep inelastic scattering events where the scattered electron and the hadronic jet are de

tected b oth in the LAr calorimeter can b e used for a direct comparison of the hadronic and

electromagnetic energy measurement exploiting p balance The transverse comp onents p and

t te

p are calculated by summing vectorially the calorimeter cell energies Figure shows that

th

the measured energy balance is compatible with simulation

The backward electromagnetic calorimeter BEMC

The backward z region of the H detector is instrumented with a conventional electromag

netic leadscintill ator sandwich calorimeter

The primary task of this backward electromagnetic calorimeter is to measure energies and

directions of electrons scattered under small angles from DIS pro cesses In addition the BEMC

contributes to the measurement of hadrons emerging from photopro duction and medium to

lowx highy hadronic nal states from DIS

The kinematics of DIS accessible with this calorimeter is characterised by mo derate four

  

momentum transfers GeV Q GeV Such pro cesses dominate by far the DIS cross

sectionobserved in the H detector and provide the only access to the lowx part of the proton



structure x At the same time the calorimeter has to op erate in a very high rate

environment caused by the illumination of the rear side with secondary hadrons originating

from b eamgas and b eamwall interactions of the GeV proton b eam Due to its lo cation

within the large solenoid the BEMC is exp osed to the full magnetic eld of T

A full description of the BEMC and its asso ciated trigger the backward single electron

trigger BSET can b e found in

Mechanical layout

The calorimeter elements stacks of the BEMC are mounted in an aluminium barrel with a

diameter of cm The front face is lo cated at a distance of cm from the nominal interaction

p oint Scattering angles from to are covered with full azimuthal acceptance This

corresp onds to units of pseudorapidity ranging from to

Granularity of the calorimeter is provided by segmentation into calorimeter stacks aligned

parallel to the b eam line The transverse structure can b e seen in Figure a stacks have

a square crosssection The remaining ones are of trap ezoidal and triangular shap es in order to

provide an approximation to the circular shap e of the supp ort barrel

The stacks are multilayer leadscintillator sandwich structures with active sampling layers

made of SCSN plastic scintillator of mm thickness The entire structure gures bc

corresp onds to a total of radiation lengths or The Moliere radius is cm The

scintillation light is coupled via a mm air gap to Y wavelength shifter bars Two

pairs of cm wide bars cover two opp osite sides of a square stack extending over the full active

length The remaining two sides are covered with cm wide bars extending only over the last

sampling layers in the stack thus providing a twofold segmentation in depth

The light emitted in the wavelength shifter bars is detected by PIN photo dio des S

Each long bar is equipp ed with one dio de The short bars are connected to a pair of dio des

due to their double width Sp ecial arrangements of wavelength shifters have b een made for the

nonsquare stacksSomeofthemhave a reduced numb er of readout channels In total there are

readout channels in the BEMC

Readout electronics and trigger

The electronics asso ciated with the BEMC must fulll tw o main functions It pro cesses the

analog signals from the PIN photo dio des and converts them into digital form with the required

sp eed precision and stability It further provides trigger signals

The signals from the PIN photo dio des are fed into charge sensitive preampliers mounted

directly on the backofeach calorimeter stack The preampliers pro duce fast signals of ns

rise time and a fall time of s A dierential pulse is sent from a line driver through m

twisted pair cables to a receiver lo cated in an electronics hut Here the signals are split to

provide input for the calorimetric triggers and for the readout

Two trigger signals are pro duced Firstly the analog signals of the four long wavelength

shifter bars within one stack are summed in order to provide input for the high granularity

backward single electron trigger BSET see Section in reference A second set of

stack sums is b eing formed to feed the overall calorimeter trigger sums with lowgranularity

The timing and the gain of the BSET stack sums are individuall y adjusted in order to assign

events uniquely to one bunch crossing and to comp ensate for stacktostackvariations in energy

calibration already on the rst trigger level

The readout of BEMC energies pro ceeds through a chain of shap ers sampleandhold circuits

and multiplexing similar to the one of the LAr calorimeter describ ed previously Duetothe

large crosssection of calorimeter stacks and the high proton b eam related background rates the

concept of slow shaping to match the trigger level L decision after bunch crossings cannot

b e applied for the BEMC The probability for a distortion of the energy measurement through

pileup would exceed for a background rate of kHz Toovercome this problem an

analog electronics chain consisting of a fast unip olar shap er and a subsequent analog delay line

is used The shap er has a time constant of ns FWHM in order to reduce the pileup

window to ab out ve bunch crossings To match the trigger decision time the shap ed signal is

delayed by an analog delay line with a length of s The fast shaping requires a precise

relative adjustmen t of all delay lines in order to avoid channeltochannel gain variations

of the signal Equalization of the delay lines to ns is required to keep the gain variations

within The equalization achieved is b etter than ns so that there is no contribution to

the energy scale uncertainty from this source

Calibration

The calibration of the BEMC is based on twocontributions Electronics gain and light collection

in the stacks are factorised and monitored indep endently

The gain of the electronics chain is determined with a pulser system identical to the one used

for the LAr calorimeter The pulser system measures the resp onse of the entire electronics chain

including all cables It has also b een used to transfer the initial absolute calibration from test

b eams to the nal exp eriment During data taking p erio ds the entire electronics is calibrated

once p er week The stabilityachieved is b etter than This is far b elow other sources of

calibration uncertainties

The second contribution to BEMC calibration is light collection and detection in the calorime

ter stacks Here the concept is to obtain the initial absolute energy scale from testb eam mea

surements and to conrm and improve the scale in situ using electrons scattered under small

angles from mediumhigh x partons ie in the kinematic p eak

Bj

The initial absolute calibration of individual square stacks has b een obtained from measure

ments with a GeV electron b eam at the DESY synchrotron The individual calibration con

stants of channels in quadratic stacks dier only slightly with a spread of This demonstrates

the stable and well repro ducible construction pro cedure for the optical part of the calorimeter

In the environmentofHERA e p collisions the BEMC is exp osed to a crosssection of nb

from DIS Deep inelastic scattering at small angles from mediumhigh x partons gives rise to

Bj

a p eak in the distribution of scattered electron energies at the value of the electron b eam energy

A metho d has b een devised to use this p eak for a precise determination of the calorimeter energy

scale for electrons The metho d has b een successfully applied to the high statistics data sample

collected in the and running p erio ds The calibrated energy distribution observed

in the BEMC is shown in Figure The data p oints are compared to a simulation program

taking into account energy losses in dead material as well as spatial inhomogeneities and all

known contributions to the energy resolution

Performance

The overall electromagnetic energy scale of the BEMC has b een determined using the data taken

in the run p erio d In gure a comparison of the measured energy distribution of the

leading cluster with a simulated one shaded area using the GRV structure function is shown

after adjustment of the calibration for each individual stack using the kinematic p eak metho d

Go o d matching of the data and the simulation proves the quality of the BEMC calibration

and of the understanding of the detector resp onse In the luminosity p erio d the global

energy scale for electrons in DIS was adjusted using the kinematic p eak metho d with a precision

corresp onding todominated by systematical errors

The energy resolution of the BEMC has initially b een determined in test b eam studies

p

carried out with electron b eams ranging from GeV to GeV A sampling term of E

has b een found in agreement with exp ectations from the mechanical design The average noise

p er calorimeter stackwas measured to b e MeV in the real H environment Energy clustering

is carried out over stack nonets giving rise to a contribution of MeV from noise for each

cluster The constant term in energy resolution for a single stackwas found to b e Using

the observed shap e of the kinematic p eak the residual stacktostack calibration uncertainty has

b een determined to b e for electrons dep ositing more than of their energy in a single

stack

The inherentmechanical nonuniformities in the stack construction due to the wavelength

shifters cause an impact p oint dep endent resp onse to electromagnetic showers Extensive studies

carried out with test b eam data and shower simulations exhibit a regular pattern of inhomo

geneities with losses up to close to the wavelength shifters A lo okup table has b een created

to correct this impact p oint dep endence Electrons sharing their energy among manystacks re

ceive an additional contribution of to their eective resolution caused by imp erfections in

the correction pro cedure

The matching of electron tracks measured in the tracking detectors to the cluster p osition

reconstructed in the BEMC has b een determined from DIS events with the electron scattered

into the BEMC Based on the known attenuation prop erties of light in the scintillator plates a

p osition resolution of mm transverse to the b eam has b een achieved

Interacting hadrons dep osit typically of their energy in the BEMC A satisfactory

p

hadronic resolution of E has b een estimated in detector simulations bycombining

the measurements in the BEMC and in the instrumented iron structure b ehind it with prop er

weighting

The plug calorimeter

The plug calorimeter PLUG has b een designed to close the gap of acceptance for the energy ow

measurements b etween the b eam pip e and the forward part of the LAr calorimeter

Its main task is to minimise the missing part of the total transverse momentum due

to hadrons emitted close to the b eam pip e In addition the energy emitted into a narrowcone

Position z cm

Overall radius r cm

Radius of detector planes r cm

Polar angular range mrad

Numb er of detectors

Numb er of electronic channels

Total length cm X

abs

Weight t

Table Global parameters of the PLUG calorimeter

around the b eam pip e can b e used to separate the proton jet as well as to veto b eam gas and

b eam wall background

Owing to the geometrical constraints the available space inside the return yoke of the H

magnet was restricted to a cylindrical hole of m length and a diameter of m around

the b eam axis only a most compact calorimeter could t Facing the physical requirements

of go o d angular resolution nearly full containment and linearity the solution was a sampling

calorimeter consisting of nine copp er absorb er plates interleaved with eight sensitivelayers of

large area silicon detectors The most imp ortant construction parameters are given in Table

Figure showsaschematic view of one of the two halfcylindrical parts of the PLUG

calorimeter eachmounted in one half of the return yoke The detector mo dules are placed within

mm wide slots b etween the absorb er plates These are sealed and easy to replace entities

which contain one half of a detector plane each Between two mm copp er plates a G readout

b oard equipp ed with silicon detectors of m thickness is placed Figure left part

A detailed description of the detector technology can b e found in Typical characteristics of

single silicon detectors as measured in the lab oratory are given in Figure Due to a sp ecial



edgeprotection pro cedure quadratic cm six triangular and four rectangular detectors

cover one half of the detector plane in a mosaic structure nearly completelyleaving only of

the total area inactive A total of detectors have b een installed

The readout electronics of the PLUG are included in the analog chain of the H calorimeters

and use the same comp onents see Section The detectors are read out in pairs

of c hannels Trigger towers are built by merging the signals from subsequentchannels in the

z direction

The calibration of the ADC output in units of visible energy rests on an absolute energy

measurement using particles Its conversion into total absorb ed energy is based on detailed

MCsimulation studies of electromagnetic and hadronic shower developments in silicon instru

mented calorimeters in comparison with test measurements

Since March the PLUG was op erated with instrumented detector planes During

luminosity op eration sharp increases of detector dark currents up to were observed which

could b e correlated with failures of HERA machine comp onents and consequential increase in

protonrelated backgrounds see references

The energy resolution of the PLUG calorimeter suers from b oth the amountofdeadma

p

terial in front of the device and the energy leakage Nevertheless its value of ab out E

evaluated from exp eriment supp orted MCcalculations turns out to b e sucientforthe

tasks within the H exp eriment As an illustration of the PLUGcalorimeter resp onse to selected



lowQ events the distribution of the total energy is shown in Figure It compares remark

ably well with MCsimulations pro duced using the Colour Dip ole Mo del LEPTO MEAR

see reference

The tail catcher TC

In order to measure the hadronic energy leaking out of the LAr calorimeter and BEMC eleven

of the sixteen limited streamer tub e LST layers of the instrumented iron are equipp ed with

readout electro des pads see also Section Here we describ e the features of the LST tail

catcher TC relevant for the energy measurement which is based on the analog readout of the

pad signals For more details see reference

 

The pad sizes vary from cm in the endcaps up to ab out cm in the barrel

region The pad signals from the ve inner six outer layers are summed up bytower builders

TB to form the front back tower signals The dierential analog signals from the TBs are

then relayed in groups of to the cable stations CS which reorganise the signals from the

towers into groups of From there the signals are sent to the analog sup erb oards SB whose

function is to amplifyintegrate and store the analog signals in groups of channels each The

geometry of the tower structure is briey describ ed in Table

Region range Segmentation ofchannels

Forward end cap x and y

Central barrel and z

Backward end cap x and y

Table Layout of the pad readout of the iron instrumentation

Electronics

The amplier used on the TBb oards allows for the measurement of single muons as well as

hadronic showers without saturation The signals have a dynamic range of mV to V

Each sup erb oard accepts the input of channels which are individuall y pro cessed by a line

receiver shap er and sample hold The line receiver and shap er are mo died versions of the

LAr calorimeter system cards while the sample hold cards are identical to those used in the

LAr readout system The signals are multiplexed and held in the output buer to b e read by

the analog receiving unit ANRU The data are then zero suppressed and corrected in the DSP

and read out see Section

The calibration of the sup erb oards is done by sending calibration pulses through the analog

readout chain b eginning at the tower builder b oard The calibration constants are downloaded

into the DSPs to correct for the channel to channel variations and nonlinearities Channel to

channel variations are less than for channels

During data taking and calibration acquisition is controlled by the LAr calorimeter OS

system Normal data and calibration results can also b e collected in standalone mo de in which

case the lo cal TC test station is used

Energy calibration

The conversion of the signal charge Q as measured in a tower i to hadronic energy E is

i hadi

given by

Q

hadi

E c c

hadi  i

c



The general hadronic energy calibration constant c has b een determined in test measurements



at CERN using pion and muon b eams The parameter c gives the tower charge of an



with resp ect to average minimum ionizing particle ie a muon at an angle of incidence of

the normal of the LST chamb ers The intercalibration factor for eachtower c describ es the

i

tower to tower variations of the measured charge

The constant c is derived from the linear relationship b etween the incident pion energy



and the ratio Q Q of the measured charge for pions and muons Dened in this way c



is essentially determined by the sampling fraction of the calorimeter and the gas used in the

chamb ers It do es not dep end on the angle of incidence of the hadrons and is also insensitive

in wide limits to the op erating conditions The parameter c and the charge Q on

 hadi

the other hand varywithhighvoltage pressure gas comp osition and temp erature Since the

atmospheric pressure is the only one of these op erating parameters whichcanchange rather

quicklywe comp ensate for this eect by regulating the high voltage see section of the

muon system

The transformation of ADC counts into charge is done online during the readout pro cess

according to

Q p AD C p

i i i i

The p edestals p are obtained from random triggers and the gains p are given by the slop e of

i i

the test pulser resp onse curv es of the electronic calibration Both varied by over the whole

data taking p erio d Zero suppression allows to read out only pads ab ove a certain threshold

The parameters c and c are determined from cosmic muons triggered by opp osite

 i

pairs of barrel or endcap mo dules in sp ecial cosmic runs The data have to b e corrected for

nonnormal incidence with resp ect to the chamb er plane In order to keep the corrections small

only tracks with tan are considered in the calibration pro cedure The intercalibration

constants c vary by within one mo dule There are larger mo dule to mo dule variations

i

dep ending on the mo dule lo cation in the iron yoke mainly due to dierent gas temp eratures

and pad sizes

Performance

The p erformance of the tail catcher has b een studied in test measurements at CERN with

and b eams of to GeV The energy resp onse for single pions is linear up to at least

p

E GeV and the energy resolution is E

The calibration of the tail catcher at HERA is done by cosmic muons as describ ed ab ove

and taking the energy scale from the CERN test results as c GeV Figure



shows representativemuon sp ectra of a complete mo dule for the inner and outer towers Clean

muon signals can b e seen with mean values far b eyond the p edestals The widths relativeto

the most probable values are The ratio of the mean values of inner and outer towers

corresp onds to the exp ected value of We do not observeany eect of the magnetic eld in

the iron yoke on the muon signal The intercalibration constants vary among the detector by

mostly due to a vertical temp erature gradient within H with a long term stabilityof

They are regularly measured with cosmic muons

Imp ortant for energy measurements with the H detector is the combination of the tail

catcher with the LAr calorimeter The energy resp onse can b e symmetrized and the energy

resolution can b e improved by including the information of the tail catcher Correc

tions for energy losses in dead materials have to b e done for eachevent Inside the tail catcher

dead material app ears as cracks b etween towers in particular in the transition region b etween

the end cap and barrel yoke Corrections b etween adjacenttowers are calculated using the ratio

of the tower areas with and without the crack as correction factor More involv ed corrections

are necessary for the material b etween the calorimeters eg the cryostat wall and coil b etween

the LAr calorimeter and the TC For this purp ose a hadronic ob ject in the LAr calorimeter is

geometrically linked with a TC cluster into a generalized cluster The energy losses are esti

mated by a linear interp olation of the energy dep osit in the last layer of the LAr calorimeter

E and the rst layer of the tail catcher E

LAr last T Cf ir st

E E E

loss LArlast T Cf ir st

The calculated energy loss is distributed among the cells in prop ortion to their energy contents

The function dep ends on the p olar angle of the shower or more precisely on the thickness

t of the material b etween the two calorimeters and are almost indep endent of the energy

dead

over a large range It has b een determined as a function of t from dedicated test measure

dead

ments at CERN AtHt varies from uptointeraction lengths dep ending on

dead

the p olar angle The corresp onding values for range from upto The uncertaintyof

the energy correction was estimated to Figure shows the eect of the combined LAr

and TC measurements with energy loss corrections from test b eam results

Calibration and correction pro cedures have b een successfully transferred from the test b eam

measurements to the H detector at HERA where the balance of the transv erse hadronic energy

p and the transverse electron energy p in neutral currentevents can b e used to check the over

th te

all hadronic calibration Figure shows the ratio p p of p as measured with the hadronic

th te th

section of the LAr calorimeter and the TC including the ab ove mentioned corrections and p

te

as measured with the electromagnetic section of the LAr or BEMC versus the energy fraction

dep osited in the TC The distribution is at demonstrating that calibration and corrections

have b een treated prop erly

Muon system

Iron instrumentation

The limited streamer tub es

The iron yoke of the main solenoid magnet surrounds all ma jor detector comp onents of H It

is interleaved with slits which are equipp ed with limited streamer tub es LST They serveas

hadronic tail catcher and for the measurement of p enetrating tracks Luranyl was used

to build the chamb ers since PVC tub es were excluded for safety reasons Luranyl is

a halogen free plastic material which can b e extruded with sucient precision It can also b e

coated with the graphite paint needed to obtain the required surface resistivity Some features

are listed in Table



Density g cm



Thermal expansion C



Surface resistivity

Softening p oint C

Table Basic prop erties of Luranyl

The basic chamb er elements are extruded eightfold proles with a cell surface size of



mm The mechanical precision achieved is mm the straightness of the proles is b etter

than mm p er m The proles are coated with graphite paint to yield a low surface resistivity

of k The HV is applied to this surface A silver coated CuBe wire of m

diameter is at ground p otential The wire is kept in place by spacers every cm The proles

are closed with a Luranyl cover with high resistivityof M The proles are group ed

by pairs in a gas tightbox of Luranyl All connections to the chamb er are provided on one

end of the b ox Several b oxes are put together to form a complete streamer tub e layer On the

high resistivity side planes of either strips or pads are glued onto the b oxes containing active

elements The layers are put onto an aluminium plate and wrapp ed into a non conducting foil

to guarantee electrical insulation

Aschematic view of the basic structure is given in Figure while Figure displays the

conguration of the planes within the iron together with an indication where strips and pads

are lo cated As an example the instrumentation of a barrel o ctantisshown Starting from the

interaction p oint there is rst a socalled muonb ox installed in front of the iron containing three

layers twolayers with strips p erp endicul ar to the wire direction and a third layer with pads

Pad layers are also installed in the rst three iron slits The fourth slit is twice as wide as the

others and houses a strip and a pad layer Pad layers are inserted in the remaining ve slits

Behind the iron is a second muonb ox with three planes

The signals of consecutive pads are added inner outer layers providing twofold

energy sampling in depth All wire and stripsignals are read out digitally Three dimensional

spacep oints from tracks can b e obtained in the three chamb ers equipp ed with strips Table

lists some parameters of the LST detector

Gas system

Due to safety requirements the chamb ers are op erated with a noninammable three comp onent

gas mixture of CO argon and isobutane with relativevolume fractions of and





Total size m

Nr of proles

Nr of wires

Nr of strips

Nr of analog channels

Angular coverage

Table The LST detector



The total gas volume amounts to m Dierent parallel circuits supply the detector

with gas The owineachbranch can b e adjusted with needle valves and is measured with

computer readable ow meters branches are used includin g some spare and test branches

The numberofchamb ers connected serially was chosen such that the total gas volume p er branch

do es not exceed l The gas comp osition in particular the isobutane content is controlled

bytwo monitors The gas ow is stopp ed and the HV is switched o if the fraction of isobutane

is outside the range to



The gas quality is also monitored bytwo LST chamb ers equipp ed with a Sr source one

in the incoming and one in the outgoing gas ow The pulse height sp ectra of these chamb ers

allow the monitoring of the gas comp osition and the HV regulation

High voltage system

Five high voltage crates with a total of indep endentHVchannels are used Each

channel supplies b etween and proles Chamb ers within one gas circuit are connected to

the same HV channel A passive distribution system allows to disconnect each single prole from

HV in case of problems All switches are computer readable such that the HV conguration of

each single fold prole can b e stored in a database

Two dierent reference voltages can b e applied to the detector One is selected to b e well

b elowworking conditions at V V This setting is activated during unstable b eam and



injection conditions The normal op erating voltage is set to V V at normal pressure

Since the charge gain of streamer chamb ers dep ends on the pressure we adjust the high voltage

accordingly The gain variation amounts to dQQ dP hPa The high voltage V is

automatically adjusted by VhPa In Hamburg one observes pressure changes of up to

hPah and total variations of hPa are p ossible

Other relevant parameters such as temp erature are monitored They remain constantover

long p erio ds The currents of all HV channels are constantly monitored If a channel draws

more than A the corresp onding voltage is automatically reduced until this current is b elow

A Channels are switched o if this limit is exceeded for more than one minute

Readout system

The readout of the analog information is incorp orated as part of the LAr calorimeter and is

discussed in Section A digital readout system was develop ed for the wire and stripreadout

Each wire strip is connected to a comparator a synchronization circuit and a digital pip eline

The wire signal is digitized according to a computer adjustable threshold synchronized with the

HERA bunch crossing frequency and fed into a digital pip eline which has a depth of steps

corresp onding to a total storage time of sec

The frontend logic for eight data channels has b een integrated in a gate array The

leading edge of the input signal clo cks the rst ipop of a dead timefree synchronization

circuit The synchronized data patterns are buered in a pip eline register As so on as a trigger

is accepted the lling of pip elines is stopp ed By means of a remotely controlled signal it can

b e decided whether the data pattern of one time slice or the logical OR of twoadjacent time

slices is read out This is necessary since the signal propagation within the chamb ers can exceed

ns the time b etween two bunch crossings In addition the eightfold OR of the stored data

pattern is clo cked into a separate ipop of the readout chain providing a signal for trigger

purp oses

The electronics for channels is housed on a readout card which is directly mounted onto

the streamer chamber layers This allows for early digitization and thus provides high noise

resistance and a signicant reduction in the numb er of cables needed Multiple readout cards

can b e daisy chained A layer of chamb ers is read out serially The readout chains of a maximum

of layers are connected to sp ecial VMEbased readout controllers ROC which provide zero

suppression data enco ding and submit all relevant steering signals to the readout cards

Up on arrival of the rst level trigger L the ROCs start to collect the data from the

electronics The absolute p osition of the data corresp onding to the triggered event within the

frontend pip elines dep ends on the decision time of the trigger and the distance b etween the

central trigger logic and the resp ectivechamb ers Due to the physical dimensions of the detector

the delay is dierent for dierent areas

One ROC serves up to digital channels corresp onding to chamb er planes with

channels eac h Since we op erate of these ROCs simultaneously less than s are needed

to collect all data

The architecture of the lo cal DAQenvironmentisgiven in Figure The VME crates are

distributed in ve clusters around the detector The readout of these units starts after a second

level trigger L VME pro cessors collect the data which are then stored lo cally The data

of up to events can b e stored b efore they are delivered to the central H data acquisition

system

Track reconstruction

The track reconstruction uses wire strip and pad layers the latter b eing combined into

towers The wires measure up to p oints in the socalled wire plane and the strips up to

p oints in the p erp endicular strip plane The resolution for wire and strip hits is mm and

mm resp ectively The pads dene coarse areas in space with a precision of ab out cm

The pattern recognition starts with the wire layers Track segments are parametrized by

straight lines To get curved track candidates several segments are connected Then the pattern

recognition selects track segments in the strips whichhave a matching wire track candidate

These matching wires and strips are then combined to a three dimensional track In case of

ambiguities the pad information is used to resolve them The combination which ts b est to the

pads in space and amplitude analog pad charge divided bynumberofwireshitischosen The

towers are then assigned to their matching wire and strip combination

Due to crosstalk along the wires usually more than one pad gets a signal With the centre of

gravityofthepadcharge the co ordinate along the wires can b e measured for b oth towers with

an accuracy b etter than of the pad size With these two additional p oints a direction in

en for very short tracks the strip plane can b e determined ev

The magnetic eld B rvaries strongly inside the iron plates and in the gaps The energy

loss in one plate is on average MeV for muons at p erp endicular incidence The track t uses

an average magnetic eld for each plate and gap and p erforms a least square t simultaneously

to wire strip and tower readings The eect of the energy loss is accounted for by an iteration

pro cedure

Performance

During op eration typically of the digital channels wires strips are noisy and are

dead

Calibration data were taken during cosmic runs One result is the eciency of the chamb ers

whichisshown in Figure It agrees well with the exp ected values Figure shows the number

of wires and strips p er eventforevents triggered by the muon system The wire data showa

signal starting at a multiplicity of which is roughly the mean numb er of wires exp ected for

single p enetrating muons with a plane eciency of

With cosmic muons the chamb ers of all mo dules have b een aligned to each other with

an accuracy of a few mm In the barrel region cosmic muons can b e used to determine the

reconstruction eciency by extrap olating jet chamber tracks Geometrical acceptance limits

this eciency to in the plateau region ab ove the threshold of GeV as shown in Figure

Forward muon sp ectrometer

General description

The purp ose of the forward muon sp ectrometer is to measure high energy muons in the range

of p olar angles The detector consists of drift chamb er planes mounted on either

side of a toroidal magnet The design aim was to measure the momenta of muons in the range

between GeVc and GeVc the lower limit b eing given by the amount of material the

muons have to p enetrate and the inuence on the momentum resolution of the multiple Coulom b

scattering in the magnet iron The upp er limit is set by the magnetic eld strength of the toroid

together with the spatial resolution of the drift chamb ers The exp ected momentum resolution

at GeVc is and deteriorates slowly to at GeVc Muon momenta b elow GeVc

are measured in the forward tracker

Figure a shows schematically the detector arrangement and the toroid magnet The latter

is describ ed in Section of reference The drift chamb er planes which increase in size from

ab out m diameter for the rst detector plane to m diameter for the last are all divided

into o ctants of individual drift cells mounted on Alframes The orientation of the drift cells

is such that four of the planes essentially measure the p olar angle and thereby provide the

momentum of the traversing muon while the remaining two measure the azimuthal angle

Each plane consists of a double layer of drift cells staggered by half a cell width Figure b

This arrangement enables the resolution of leftrightambiguities and also the determination of

t as will b e explained b elow The total numb er of drift cells is

Chamb er design

All drift cells have a rectangular crosssection with a depth of cm a width of cm and lengths

between cm and cm With a central sense wire the maximum drift distance is cm The

cells havem thickNichrome wires except for the inner short cells where the diameter is

m For cells longer than m there is a wire supp ort in the middle More details can b e

found in reference

The chamb er signals are amplied digitized and read out using the same comp onents as all

other drift chamb ers within the H detector see Section

The chamb er gas and high voltage system

The choice of gas for the drift chamb ers was determined byseveral requirements One is the

desire to work in a drift voltage range where the drift velo city is constant Further the gas has

to b e fast enough for the pulse to arrive in time for the trigger and nally it should b e non

ammable for safety reasons Currently a mixture of argon CO and methane



FMS gas has b een chosen for the chamb ers The gas is mixed and puried in a recirculator



The chamb ers have a total gas volume of m and with a small overpressure of ab out hPa

measured at the output the return gas owistypically of the input and the oxygen content

is of order ppm More details can b e found in

A channel high voltage system supplies distribution b oxes on the detector with

high voltage via m long coaxial cables Two dierent mo dules are used one kV mA

supplies the drift voltage and the other kV A supplies the sense voltage One drift

channel supplies voltage to an entire o ctant feeding individual resistor chains One sense

channel supplies voltage to all but the innermost cells of a o ctant and the central section

of the o ctants These cells have another sense channel whichcanbesettoalower voltage in

case of bad b eam conditions Additionally for the o ctants the central section which is close

to the b eam tub e can b e moved outwards mechanically if necessary

There is a continuous monitoring of the gas comp osition and ow rates as well as of the high

voltage and the toroid magnet communicated via an Apple Macintosh I I ci in the control ro om

From this work station it is also p ossible to control the high voltage of the detector

The chargetime analysis

Only the rising edge and p eak region of a pulse are used to get the time and charge information

A pulse is said to start when there are two successively rising digitizings ab ove threshold see

also Section

The end of a pulse is taken as the second successive digitizing after the p eak which is b elow

threshold or eight ns time bins from the start of the pulse whichever o ccurs rst The

arrival time of the pulse is obtained by extrap olating a line tted to the steep est part of the

leading edge back to the intercept with the background level With a test set up lo oking at

cosmic muons this metho d gave a resolution of m This result was obtained with a gas

mixture of argon and propane providing a drift velo city of cms However to

satisfy the gas requirements sp ecied in Section wehavechosen the FMSgas with a drift

velo cityof cms resulting in an exp ected resolution of m Pairs of pulses which

originate from the same hit are asso ciated by requiring the dierence of their arrival times to

b e less than the full propagation time through the two sense wires and the linking resistor

The collected charge is found byintegrating the digitizings of the pulses from the two wire

ends over interv als of the same length with subtraction of a constantbackground A correction

for fractional time bins was found to b e imp ortant since the start times for the two pulses

are sub ject to variable propagation delays With cosmic muons in the test set up we found a

chargedivision versus distance characteristic linear to ab out whichiswell matched to the

resolution

Track reconstruction

The space p oints obtained from the chargetime analysis of the chamb er hits are used in a three

step pro cedure for track reconstruction which starts with the pairing of hits in each double

layer followed by asso ciation of pairs into straight track segments and nally the linking of track

segments through the toroid to form full tracks and thus provide a momentum measurement

Pair nding in the double layers is decisive due to the displacements of cells which results in

the sum of drift times b eing a constant compare Figure b A vertex p ointing requirement

is applied as selection criteria but also unpaired hits are kept to b e considered in the track

segment nding where we demand out of hits in the layers The measuring errors of the

space p oints for a pair dene a cone which is extrap olated to the other layer on the same side

of the toroid In the area dened by the cone hits are tried for segment ts and are selected by



a cut

For the linking pro cedure each pretoroid segment is tracked through the magnetic eld

of the toroid taking into account energy loss and multiple Coulomb scattering in the magnet

iron By doing this for a minimal reconstructible momentum of GeVc in the sp ectrometer

and for either of the twomuon charges p ossible regions in the layers after the toroid are

dened inside which segment candidates for linking are considered From the crossing angle

of two linked segments an estimate of the momentum is made Starting from the pretoroid

segment and the estimated momentum the tracking is rep eated as the momentum is changed in

small steps around the estimated value Each p osttoroid segment obtained from the tracking is

 

compared to the actual segment found and a is calculated The minimum of the variation

with momentum denes the momentum corresp onding to the b est t

Drift velo city and t determination

Beam halo muons are used to determine the drift velo cityFrom the uniform p opulation of the

total number of tracks N over the full drift distance y recorded in a run a rectangular

distribution is exp ected if the drift velo city is constant However due to eld variations close to

the sense wire dep endence on the angle of the track the p ossibility of tracks traversing only the

corner of a cell etc the drift velo city will b e altered and cause a smearing of the distribution

t is determined from the sp ecic geometry of the detector making true sp ecic check sums

for each track as detailed in reference The widths of the check sum distributions can b e

used to nd the spatial resolution of the chambers

Chamb er alignment

The drift chamb ers must b e aligned with resp ect to each other and to the rest of the detector

The cells of a layer are p ositioned on its supp orting Alframe to a precision of malong

the drift direction and to mm in the two other directions This is b etter than the achievable

resolution and therefore we only have to consider the alignment of the full o ctants

Simulation studies and analysis of a small sample of real data hav e shown that b eam halo

tracks are suitable for providing the two translational and one rotational quantities whichare

needed to sp ecify the p osition of the o ctant in the plane transverse to the b eam direction

Further studies with angle tracks together with the survey will determine the relative p ositions

of the o ctants along the direction of the b eam

Acknowledgement

We appreciate the immense eort of the engineers and technicians of the participating lab o

ratories who designed constructed and maintain the detector We are grateful to the HERA

machine group whose outstanding eorts contribute to making this exp eriment p ossible We

thank the funding agencies for nancial supp ort The nonDESY memb ers of the collab oration

also express their thanks the DESY directorate for the hospitality extended to them Weac

knowledge the help of DESY and CERN in providing test b eam time for the many calibration

runs The help of the computing centres at DESY and at CERN in the test and running phases

is highly appreciated

Figure Schematic layout of the H detector

Figure The H tracking system r z view

Figure Central tracking system section p erp endicular to the b eam trac Sim iue et lcrnpoo cteigev scattering Electronproton Left Figure lto faCCcl niaigteditrgoso h esswrs rf ie n s c iso and lines drift wires senses the of regions drift the indicating cell CJC a of ulation sfo h a axis eam b the from ks en sse nteCCsho CJC the in seen as t igtrac wing sfudb found ks h atr eonto rga n irrtrac mirror and program recognition pattern the y rns h straigh The hrones ie represen lines t nnt momen innite t s Righ ks tum

t

Figure Dep endence of the CJC z resolution on the amount of ionization A minimum ionizing

particle dep osits typically counts

Figure Sp ecic ionization versus particle momentum measured in the CJC in HERA runs

Figure Longitudinal and transverse crosssection through a cell of the CIZ S signal wires

P p otential wires the z co ordinates are given relative to the center of the cell mm

Figure Schematic view of the COZ

Figure Forward tracker overview Top crosssection in the rzplane showing the three

sup ermo dules Bottom crosssection in the rplane showing the basic cell structure of each

sup ermo dule comp onent in one quadrant A planar chamb er B FWPC C TR D radial

chamb er elwrsadpd o eac for pads and forw wires the cells of Details Figure u rodl oponen comp dule ermo sup h r trac ard k rcntutoT construction er Btodtiso elconstruction cell of details Bottom t p rseto nthe in crosssection op r z ln n nthe in and plane r ln sho plane igteo the wing v rl orien erall

ainof tation iueF Figure D edu ytmfrditc drift for system readout ADC ham

ers b

Figure Longitudinal crosssection and details of the COP

Figure Cross section through the backward prop ortional chamber

Figure MWPC front end electronics and readout system

Figure Layout of the closed circuit gas system for the planar drift chamb ers CP circuit

membrane pump FL mechanical ow meter FM electronic ow meter GC gas chromato

graph HM hygrometer IM infrared meter MV mechanical safetyvalve O Ometer PG

 

mechanical pressure gauge PT electronic pressure transducer SV solenoid valve V mechanical

two or threewayvalve

Figure Schematic crosssection of the inner and outer veto wall left and the ToF counters

Figure Time distribution of hits in a ToF counter

Figure a Longitudinal view of calorimeters b Radial view of a LAr calorimeter wheel

Figure Schematic structure of the readout cell a em cell b hadronic cell All dimensions

given in m

Figure Relative stability of the electronic chain over one month

Figure Noise contribution summed over all channels of the LAr calorimeter a after applying

a noise threshold b after noise suppression

tr ue

Figure Correlation b etween the true energy lost in front of the calorimeter E and its

lost

 rec

for simulated low Q DIS estimation in the reconstruction E

lost

Figure The eectivemassoftwo photons b efore dashed histogram and after hatched one

the dead material correction

Figure Performance of the dead material correction for simulated pions at GeV Ratios

tr ue tr ue rec tr ue tr ue

E E circles and E E E crosses are shown as function of and

tot tot

lost lost lost

b oth given in degrees Before the correction a crack structure is clearly seen Solid lines

corresp ond to deviations from the true energy

Figure Resp onse across the CBCB z crack in a pion test b eam of GeV at CERN

Figure Reconstructed energy for data histogram and MC p oints for electron energies of

and GeV BBE Wheel

Figure Energy resolution as function of electron energy for wheels BBE CB FB and IF

Solid line parametrization for FB

Figure Energy reconstruction for pions at GeV for wheels CB FB and IF on the elec

tromagnetic op en and hadronic energy scale closed shadowed for data histogram and MC

p oints

Figure Energy reconstruction for pions at GeV for wheel IF with tail catcher op en

histogram only IF circles and for events fully contained in IF Solid lines tted Gaussian

distributions

Figure Energy resolution as function of pion energy for wheel IF Circles IF only triangles

IF iron tail catcher Parametrization according to equation with

p

A GeV B GeV and C

Figure Energymomentum match of electrons generated by cosmic muons measured in the

CJC and LAr CB wheels

Figure Transverse momentum balance p p for b oth scattered electron and hadronic

th te

shower detected in the LAr calorimeter for data op en symb ols and Monte Carlo histogram

Figure Transverse view of the BEMC barrel and longitudinal crosssections of BEMC stacks

The p ositions of all long WLS in the BEMC are marked in a The scintillating light is read

out transversely via long WLS covering the full length of the BEMC stacks b In square and

trap ezoid stacks the last sampling layers are read out via short WLS c



Figure Energy sp ectrum of lowQ DIS electrons scattered in the region of square BEMC

stacks For simulation shaded area the structure function GRVisused

Figure Cross sectional view of the PLUG calorimeter

Figure Typical IV and CV characteristics of the PLUG Sidetectors

Figure PLUG resp onse to ep events compared to a MC simulation solid line pro duced

using the Colour Dip ole Mo del

Figure Muon sp ectra summed over a complete mo dule for a inner towers normalized to

planes and b outer towers normalized to planes The curves are ts to a Landau distribution

Figure Ratio of the total transverse hadronic energy including the corrected TC energy

and the transverse electron energy versus the energy fraction in the TC for NC events The

line is a t to the data

Figure Structure of LST chamb ers

Figure Iron instrumentation showing the p ointing pad structure of the barrel region The

crossed elements represent dummy mo dules which ll the space not o ccupied by the chamb ers in

away to ensure that the dead areas are not aligned for tracks from the vertex region Ppads

Sstrips

Figure The lo cal data acquisition system

Figure Eciency of chamb er planes The following numb ering scheme is used

backward endcap from b ottom to top backward barrel forward barrel

forward endcap from b ottom to top

Figure Wire and strip multiplicity p er event

Figure Muon reconstruction eciency in the barrel region as function of the muon energy

GeV determined from cosmic muons The average eciency in the plateau region is and

is determined by geometrical acceptance

Figure a A schematic view of the forward muon sp ectrometer and b the cell structure of

a double layer

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