Quantum How Measurement Is Driving Innovation in the Emerging Quantum Industry
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Cleo/Qels 2006
CLEO/QELS 2006 Technical Conference: May 21-26, 2006 Exposition: May 23-25, 2006 Long Beach Convention Center, Long Beach, CA, USA CLEO/QELS & PhAST 2006 once again reiterated their roles as the leading events for the fields of lasers, electro-optics and photonics. With more than 1,500 talks on the latest breakthroughs in research and applications, these conferences are the source of the most timely and innovative new developments for the industry. Consistent with previous year's shows, attendance reached 5,200. Technical attendance was strong at more than 2,500 and exhibit walk-in traffic remained steady with 2005. The CLEO exhibition showcased 358 participating companies this year, with almost a 100 percent increase in corporate sponsor participation. The show really is an international must- attend event, with approximately 25% of companies coming from outside the United States. There also were exciting new programs and topics introduced at the 2006 event. The PhAST conference established the PhAST/Laser Focus World Innovation Award which recognizes a company who has developed one of the most promising new products in the field. This year, Daylight Solutions won for its submission, "Commercializing the Mid-IR" and four honorable mentions were given to Thorlabs, Sacher Lasertechnik, Fianium and PolarOnyx. CLEO also launched the Terahertz Technologies and Applications subcommittee, a new topic area developed due to a consistent increase in papers in this area over the last few meetings. CLEO/QELS and PhAST had a great year in 2006. We're looking forward to seeing you in Baltimore , May 6-11, 2007. Conference Program Postdeadline Papers CPDA-CLEO Postdeadline Session I CPDA1 St. -
RZR-P RZQ-P Service Manual
SiUS281117 Service Manual RZR-P, RZQ-P(9) Series Cooling Only / Heat Pump R-410A 60Hz SiUS281117 RZR-P, RZQ-P(9) Series Cooling Only / Heat Pump R-410A 60Hz ED Reference For items below, please refer to Engineering Data. For except FTQ No. Item ED No. Page Remarks 1 Specification - Cooling Only EDUS281120 p. 7-13 2 Specification - Heat Pump EDUS281120 p. 14-20 3 Option List EDUS281120 p. 100-102 For FTQ No. Item ED No. Page Remarks 1 Specification - Heat Pump EDUS281008 p. 4 2 Option List EDUS281008 p. 60 1. Safety Considerations.............................................................................v 1.1 Safety Considerations for Repair ............................................................. v 1.2 Safety Considerations for Users ..............................................................vi Part 1 General Information........................................................... 1 1. Model Names and Power Supply............................................................2 1.1 Cooling Only ............................................................................................2 1.2 Heat Pump ...............................................................................................2 2. External Appearance ..............................................................................3 2.1 Indoor Units..............................................................................................3 2.2 Remote Controller....................................................................................4 2.3 Outdoor Units...........................................................................................4 -
Astrodynamical Space Test of Relativity Using Optical Devices I (ASTROD I) - a Class-M Fundamental Physics Mission Proposal for Cosmic Vision 2015-2025
Astrodynamical Space Test of Relativity using Optical Devices I (ASTROD I) - A class-M fundamental physics mission proposal for Cosmic Vision 2015-2025 Thierry Appourchaux Institut d’Astrophysique Spatiale, Centre Universitaire d’Orsay, 91405 Orsay Cedex, France Raymond Burston Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany Yanbei Chen Department of Physics, California Institute of Technology, Pasadena, California 91125, USA Michael Cruise School of Physics and Astronomy, Birmingham University, Edgbaston, Birmingham, B15 2TT, UK Hansjörg Dittus Centre of Applied Space Technology and Microgravity (ZARM), University of Bremen, Am Fallturm, 28359 Bremen, Germany e-mail: [email protected] Bernard Foulon Office National D’Édudes et de Recherches Aerospatiales, BP 72 F-92322 Chatillon Cedex, France Patrick Gill National Physical Laboratory, Teddington TW11 0LW, United Kingdom Laurent Gizon Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany Hugh Klein National Physical Laboratory, Teddington TW11 0LW, United Kingdom Sergei Klioner Lohrmann-Observatorium, Institut für Planetare Geodäsie, Technische Universität Dresden, 01062 Dresden, Germany Sergei Kopeikin Department of Physics and Astronomy, University of Missouri, Columbia, Missouri 65221, USA Hans Krüger, Claus Lämmerzahl Centre of Applied Space Technology and Microgravity (ZARM), University of Bremen, Am Fallturm, 28359 Bremen, Germany Alberto Lobo Institut d´Estudis Espacials de Catalunya (IEEC), Gran Capità 2-4, 08034 -
A Physicist's Guide to Managing Career Breaks and Achieving
Equilibrium A Physicist’s Guide to Managing Career Breaks and Achieving Career Balance Few would argue that a high level of commitment is required to be successful as a physicist, but there is a difference between being committed to your career and devoting every waking minute to it. Sadly, this difference is not always accepted and many excellent, highly qualified physicists are lost to science, technology and engineering because they aren’t aware of options that will allow them to balance their professional lives with other demands, or aren’t supported to do so. This guide has been written to demonstrate how career breaks can be managed effectively and how a better balance between work and life can be achieved. Written by Dr Sara Shinton www.shintonconsulting.com Equilibrium: A Physicist’s Guide to Managing Career Breaks and Achieving Career Balance 3 Foreword At some point in our lives, most of us working in physics will find issues of work-life balance come to the fore. Maybe we find ourselves facing the challenge of caring responsibilities, which can extend far beyond simply becoming a new parent. Or perhaps we just want time to explore other options for months or years, or rebalance our working life by reducing the hours worked to allow time for other activities. This guide provides invaluable information on resources that the Institute of Physics (IOP) itself Taking control many aspects of how to approach such matters, provides for before, and during, any career break. designed to ensure that an individual has all the by being well facts at their fingertips and also understands how This guide can thus be seen as an excellent guide informed can best to approach their bosses or line managers to to have to hand as thoughts of stepping back from ensure that any achieve a “win-win” situation. -
Year in Review
Year in review For the year ended 31 March 2017 Trustees2 Executive Director YEAR IN REVIEW The Trustees of the Society are the members Dr Julie Maxton of its Council, who are elected by and from Registered address the Fellowship. Council is chaired by the 6 – 9 Carlton House Terrace President of the Society. During 2016/17, London SW1Y 5AG the members of Council were as follows: royalsociety.org President Sir Venki Ramakrishnan Registered Charity Number 207043 Treasurer Professor Anthony Cheetham The Royal Society’s Trustees’ report and Physical Secretary financial statements for the year ended Professor Alexander Halliday 31 March 2017 can be found at: Foreign Secretary royalsociety.org/about-us/funding- Professor Richard Catlow** finances/financial-statements Sir Martyn Poliakoff* Biological Secretary Sir John Skehel Members of Council Professor Gillian Bates** Professor Jean Beggs** Professor Andrea Brand* Sir Keith Burnett Professor Eleanor Campbell** Professor Michael Cates* Professor George Efstathiou Professor Brian Foster Professor Russell Foster** Professor Uta Frith Professor Joanna Haigh Dame Wendy Hall* Dr Hermann Hauser Professor Angela McLean* Dame Georgina Mace* Dame Bridget Ogilvie** Dame Carol Robinson** Dame Nancy Rothwell* Professor Stephen Sparks Professor Ian Stewart Dame Janet Thornton Professor Cheryll Tickle Sir Richard Treisman Professor Simon White * Retired 30 November 2016 ** Appointed 30 November 2016 Cover image Dancing with stars by Imre Potyó, Hungary, capturing the courtship dance of the Danube mayfly (Ephoron virgo). YEAR IN REVIEW 3 Contents President’s foreword .................................. 4 Executive Director’s report .............................. 5 Year in review ...................................... 6 Promoting science and its benefits ...................... 7 Recognising excellence in science ......................21 Supporting outstanding science ..................... -
Examensarbete
EXAMENSARBETE Tidsättning och övervakning Robin Dorand Lars Karlsson Högskoleexamen Datornätverk Luleå tekniska universitet Institutionen för System- och Rymdteknik Robin Dorand & Lars Karlsson 9 juni 2012 Datornätverk LTU Skellefteå Institutionen för System- och Rymdteknik Sammanfattning Detta examensarbete pågick under fem veckor på SSAB i Luleå och behandlar två uppgifter. Den första uppgiften gick ut på att forska om tid för att på bästa sätt kunna tidsätta nätverksutrustning samt övervakningsplattformar på SSAB. Den andra uppgiften gick ut på att undersöka krav samt upplägg för övervakningsplattformen SCOM. För att kunna synkronisera tid används i huvudsak tre protokoll: NTP, SNTP samt PTP. De vanligaste teknikerna för att synkronisera tid är via internet, GPS, radiokommunikation samt manuell tidsättning. Genom att samla in data jämfördes olika scenarion och utrustning konfigurerades. Utifrån undersökningar framkom det att den lämpligaste lösningen var att via NTP protokollet synkronisera utrustningen mot en lokal server. Servern är i sin tur kopplad mot en GPS mottagare. För framtida implementeringar föreslogs ny kraftigare hårdvara med stöd för redundans. SCOM är en modulbaserad övervakning och hanterings- plattform som utvecklats av Microsoft. Med hjälp av SNMP protokollet tillhandahålls hjälpmedel för att kommunicera mellan SCOM och olika nätverksutrustningar. Undersökningen kring övervakningsplattformen SCOM bestod av samtal med personal på SSAB angående önskemål samt synpunkter på utformning. Utifrån informationen togs ett upplägg fram som bestod av diagram för nätverksutrustning samt kartbilder för anläggningens områden. Överblicksbilder samt diagram sammanställdes i SCOM för att skapa ett lättnavigerat och pedagogiskt system för övervakning. Abstract This thesis project lasted during five weeks at SSAB in Luleå and dealt with two tasks. The first task was to research the best possible way to synchronize network equipment and monitoring platforms at SSAB. -
Optical Frequency Measurement and Ground State Cooling of Single Trapped Yb+ Ions
Optical frequency measurement and ground state cooling of single trapped Yb+ ions Peter Blythe March 2004 with updates and corrections August 2005 Submitted in partial ful¯lment of the requirements for the degree of Doctor of Philosophy of the University of London Abstract The thesis describes experiments on single laser-cooled ions of Yb+ in a radiofrequency ion trap. 2 2 The ion is laser-cooled on the 369 nm S1=2! P1=2 electric dipole tran- 2 2 sition, and high resolution spectroscopy of the 467 nm S1=2! F7=2 electric octupole `clock' transition has been performed. The 467 nm transition can be used as an optical frequency standard. To this end, several absolute optical frequency measurements of the F = 171 + 0; mF = 0 ! F = 3; mF = 0 component in Yb have been made with a femtosecond laser frequency comb generator. The comb was referenced to a hydrogen maser which forms part of the clock ensemble used to generate the UTC(NPL) timescale. During the work described in this thesis, the linewidth of the 467 nm probe laser has been narrowed from 4 kHz to 200 Hz, increasing the measurement resolution. The frequency measurements have been supported by a full investigation of the systematic frequency shifts of the octupole transition, including the AC Stark, second-order Zeeman, quadrupole, DC Stark, second-order Doppler and blackbody shifts. Cooling an ion of 172Yb+ to the ground motional state of the ion trap by `EIT cooling' on the 369 nm transition has been investigated, both by numerical simulation and experiment. A new technique for measuring the temperature of a trapped ion without the use of a narrow transition has been developed. -
Khz Time(UTC) Days ITU Station Lng Target Remarks 16.4 0000-2400
kHz Time(UTC) Days ITU Station Lng Target Remarks 16.4 0000-2400 NOR JXN Marine Norway NEu no 18.2 0000-2400 IND VTX Indian Navy SAs v 18.3 0000-2400 F HWU French Navy WEu wu 19.6 0000-2400 G GQD Anthorn WEu an 19.8 0000-2400 AUS NWC US/Australian Navy Oc ex 20.5 0741-0747 BLR RJH69 Molodechno #NOME? EEu mo 20.5 0441-0447 KGZ RJH66 Bishkek #NOME? CAs bk 20.5 1041-1047 KGZ RJH66 Bishkek #NOME? CAs bk 20.5 1131-1141 RUS RJH63 Krasnodar #NOME? EEu kd 20.5 0941-0947 RUS RJH77 Arkhangelsk #NOME? EEu ak 20.5 0541-0547 RUS RJH99 Nizhni Novgorod #NOME? EEu nn 20.9 0000-2400 F HWU French Navy WEu wu 21.4 0000-2400 HWA NPM US Navy Oc L 21.7 0000-2400 F HWU French Navy WEu wu 23 0735-0741 BLR RJH69 Molodechno #NOME? EEu mo 23 0435-0441 KGZ RJH66 Bishkek #NOME? CAs bk 23 1035-1041 KGZ RJH66 Bishkek #NOME? CAs bk 23 1126-1131 RUS RJH63 Krasnodar #NOME? EEu kd 23 0935-0941 RUS RJH77 Arkhangelsk #NOME? EEu ak 23 0535-0541 RUS RJH99 Nizhni Novgorod #NOME? EEu nn 23.4 0000-2400 D DHO38 German Navy Eu rf 23.4 0000-2400 HWA NPM US Navy Oc L 24 0000-2400 USA NAA US Navy Cutler NAO cu 24.8 0000-2400 USA NLK US Navy Jim Creek NAO jc 25 0700-0725 BLR RJH69 Molodechno #NOME? EEu mo 25 0400-0425 KGZ RJH66 Bishkek #NOME? CAs bk 25 1000-1025 KGZ RJH66 Bishkek #NOME? CAs bk 25 1100-1120 RUS RJH63 Krasnodar #NOME? EEu kd 25 0900-0925 RUS RJH77 Arkhangelsk #NOME? EEu ak 25 0500-0525 RUS RJH99 Nizhni Novgorod #NOME? EEu nn 25.1 0725-0730 BLR RJH69 Molodechno #NOME? EEu mo 25.1 0425-0430 KGZ RJH66 Bishkek #NOME? CAs bk 25.1 1025-1030 KGZ RJH66 Bishkek #NOME? CAs bk 25.1 -
Table of Contents
Table of Contents Undergraduate Courses in Physics ................................................. 1 1.1 INTRODUCTION ................................................................................................................................. 1 1.2 PHYSICS COURSES IN THE ACADEMIC YEAR 2013-14 .................................................................. 1 1.2.1 The First Year (Part IA) .......................................................................................................... 1 1.2.2 The Second Year (Part IB) ..................................................................................................... 2 1.2.3 The Third Year (Part II) - Physics ....................................................................................... 2 1.2.4 The Fourth Year (Part III) - Physics .................................................................................... 3 1.2.5 Master of Advanced Studies (MASt) in Physics .................................................................... 3 1.3 MATHEMATICS AND THE PHYSICS COURSES .............................................................................. 3 Aims and Objectives of the Physics Teaching ................................ 4 Programme ................................................................................... 4 2.1 THE UNIVERSITY’S AIMS AND OBJECTIVES ................................................................................ 4 2.2 COURSE AIMS ................................................................................................................................... -
Transitions in the Bottomonium System
Annual Reviews www.annualreviews.org/aronline Annu. Rev. Nucl. Part. Sci. 1993.43:333-78 Copyright© 1993 by AnnualReviews lnc. All rights reserved UPSILON SPECTROSCOPY: Transitions in the Bottomonium System D. Besson Departmen~t of Physics, University of Kansas, Lawrence, Kansas 66045 T. Skwarnicki Departmentt of Physics, Southern Methodist University, Dallas, Texas 75275 KEY WORDS: potential models,radiative transitions, hadronic transitions, multiple models CONTENTS 1. INTRODUCTION................................................... 334 1.1 Bound States and Fundamental Forces in Nature ................... 334 1.2 Discovery of the Y System ........................................ 335 1.3 The Quarkonium Model .......................................... 335 1.4 Scope of This Article ............................................. 338 2. STORAGE RINGS AND DETECTORS............................... 338 3. COUPLINGTO LEPTONPAIRS ..................................... 339 3.1 Measurement of Y Masses and Their Leptonic Widths ............... 339 3.2 Measurement of Leptonic Branching Ratios ........................ 341 3.3 Derivation of the Total Widths of the Y Resonances ................. 342 3.4 Comparison with Theoretical Predictions ........................... 342 4. MEASUREMENTSOF RADIATIVE TRANSITIONS .................. 343 4.1 Radiative Transitions from the Y(2S) .............................. 344 4.2 Radiative Transitions from the Y(3S) .............................. 346 5. COMPARISON WITH POTENTIAL MODELS ........................ 348 5.1 Excitation -
Moving On: the Physics Phd Student’S Guide to Boosting Employability
Moving on: The Physics PhD Student’s Guide to Boosting Employability Careers IOP Careers www.iop.org/careers 3 Contents What value can research experience add to your career? 5 Independence 5 1 Critical Thinking 6 Finding your own funding 7 Problem solving 7 Contributing to society 8 Contributing to a professional field 8 Professional working relationships 9 Confidence, initiative and drive 9 Conclusion 10 Taking control of your career 12 Making more of conferences 13 2 Gaining awards and sponsorship 14 Public engagement 16 Additional projects and industrial experience 17 Using social media 18 Taking control of your own development 19 The benefits of chartered status 22 Where do you start? 23 10 key messages and suggestions 23 3 Boosting your academic career chances 24 Useful resources to move your career forward 26 Advice on CV writing and interviews 26 4 4 IOP Careers www.iop.org/careers Moving on: The Physics PhD Student’s Guide to Boosting Employability The number of people entering the labour market with a degree has grown dramatically in the last generation. Many degrees now include industrial training and focus on developing specific skills, so you might expect employers to have their pick of great candidates. The truth, though, is that every time a group of employers is surveyed, they identify skills shortages and a need for high- calibre candidates with particular technical or personal expertise. A PhD gives you the chance to develop technical knowledge and skills to a very high level, but the nature of research is such that you will also have the opportunity to develop a broader set of valuable professional skills. -
Annual Review
ANNUAL REVIEW 2020 ANNUAL REVIEW CEO’S INTRODUCTION financial trading; and provision courses available free of charge, of environmental monitoring, allowing industry and academia to declared as critical by the freely invest in their workforce Environment Agency. whilst they were ‘working from home’ - nearly 10,000 new We were also able to rapidly learners registered for e-learning transfer resources to support the and there was a 99% satisfaction UK’s COVID-19 response, rate in the training experience. We including the government’s UK also assisted home-schooling by Ventilator Challenge which making our Virtual Physics encouraged manufacturers to re- Laboratory (VPLab) educational purpose their assembly lines and software available for secondary support new designs to meet school pupils and teachers; over anticipated demand. NPL 19,500 simulation downloads were answered the challenge by made by students to use at home. designing the PocketVent, a unique, fan-based ventilator, Foresighting - During 2020 NPL The National Physical smaller than a laptop, costing less published the results of its Laboratory’s (NPL) number one than £1,000. extensive Technology and priority during 2020 was to Measurement Foresighting ensure that all our people NPL used its wealth of experience programme, which identified major remained safe and secure and scientific capabilities to help trends in technology and during the COVID-19 pandemic. increase the availability of measurement that would impact Our focus was on prioritising Personal Protective Equipment industry and our society, as well as our people and supporting them (PPE), by signposting new how we live over the next 15 to navigate their working lives in manufacturers of PPE and medical years.