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Daily Iowan (Iowa City, Iowa), 1953-10-22
The Weather Serving the State Partb c10., aDd eeoIH ·versity of Iowa toda,. CleariDc ....... Art slderlbb eooIer FrWar. Campus and JII,h ~aJ. T.; 1_. 52; Hla'h WednH41a7. II; low. he SUI art i.:wa City 67. attend the 1868 - A,P Leased Wile, Wirephot.o - Five Cent. Iowa City, Iowa, Thursday, Oct. 22, 1953 - Vol. 97, No. 276 the found- , Eat. College Art • ~---------------------------------------------- Department orlSin. Mln ./ '0 the rti.t trom .ohio the conter- ~ shown by ueen ·Will· Open Homecoming ence df 1he AcsthetJcs ege in. No- • Homecoming Mums Aqui Show To Feature Five Iowa sportscasters and Qne ------------ Varied Acts sports writer will judge the utes past any given point In the beauty, or~inallty and humor ot parade route. The 40 tloats wiU Three days ot 1953 Homecom , ' the I10nt entries In the fifth an- then move to the area just east In, frolic will let the ful\-steam- nual SUI Homecoming parade Frl- of Iowa stadium to remain throu,ll abead si,nal tonight when one ot day night at 7. Saturday's game as a post-parade Taking time out from their re- dISplay parade chairman Loren five campus lovelies is named porting responsibilities to score Hlcker ~on lays. Dolphin Queen for SUY'! 31st an- each of 40 floats ror beaut), will . nUIII poolsld~ sholl'. be Gene Claussen, KXIC Iowa Musical marching grou~s In the City and Gene Shumate KSO De parade will total 13, With nine Pre!\Cntatlon of the qucen-ror- Moines. • high school bands, Shriner bands a-weekend will come at 8 p.m. -
Association of Unit Owners Contact List
Association of Unit Owners Contact List Project Name/Number AOUO Designated Officer for Direct Contact/Mailing Address Management Company/Telephone Number `AKOKO AT HO`OPILI Reg.# 8073 1001 QUEEN Reg.# 7675 1001 WILDER EMILY PRESIDENT 1001 WILDER #305 HAWAIIAN PROPERTIES, LTD. Reg.# 5 WATERS HONOLULU HI 96822 8085399777 1010 WILDER RICHARD TREASURER 1010 WILDER AVE, OFFICE SELF MANAGED Reg.# 377 KENNEDY HONOLULU HI 96822 8085241961 1011 PROSPECT RICHARD PRESIDENT 1188 BISHOP ST STE 2503 CERTIFIED MANAGEMENT INC dba ASSOCI Reg.# 1130 CONRADT HONOLULU HI 96813 8088360911 1015 WILDER KEVIN PRESIDENT 1015 WILDER AVE #201 HAWAIIANA MGMT CO LTD Reg.# 1960 LIMA HONOLULU HI 96822 8085939100 1037 KAHUAMOKU VITA PRESIDENT 94-1037 KAHUAMOKU ST 3 CEN PAC PROPERTIES INC Reg.# 1551 VILI WAIPAHU HI 96797 8085932902 1040 KINAU PAUL PRESIDENT 1040 KINAU ST., #1206 HAWAIIAN PROPERTIES, LTD. Reg.# 527 FOX HONOLULU HI 96814 8085399777 1041 KAHUAMOKU ALAN PRESIDENT 94-1041 KAHUAMOKU ST 404 CEN PAC PROPERTIES INC Reg.# 1623 IGE WAIPAHU HI 96797 8085932902 1054 KALO PLACE JUANA PRESIDENT 1415 S KING ST 504 HAWAIIANA MGMT CO LTD Reg.# 5450 DAHL HONOLULU HI 96814 8085939100 1073 KINAU ANSON PRESIDENT 1073 KINAU ST 1003 HAWAIIANA MGMT CO LTD Reg.# 616 QUACH HONOLULU HI 96814 8085939100 1108 AUAHI TODD PRESIDENT 1240 ALA MOANA BLVD STE. 200 HAWAIIANA MGMT CO LTD Reg.# 7429 APO HONOLULU HI 96814 8085939100 1111 WILDER BRENDAN PRESIDENT 1111 WILDER AVE 7A HAWAIIAN PROPERTIES, LTD. Reg.# 228 BURNS HONOLULU HI 96822 8085399777 1112 KINAU LINDA Y SOLE OWNER 1112 KINAU ST PH SELF MANAGED Reg.# 1295 NAKAGAWA HONOLULU HI 96814 1118 ALA MOANA NICHOLAS PRESIDENT 1118 ALA MOANA BLVD., SUITE 200 HAWAIIANA MGMT CO LTD Reg.# 7431 VANDERBOOM HONOLULU HI 96814 8085939100 1133 WAIMANU ANNA PRESIDENT 1133 WAIMANU STREET, STE. -
Cumulated Bibliography of Biographies of Ocean Scientists Deborah Day, Scripps Institution of Oceanography Archives Revised December 3, 2001
Cumulated Bibliography of Biographies of Ocean Scientists Deborah Day, Scripps Institution of Oceanography Archives Revised December 3, 2001. Preface This bibliography attempts to list all substantial autobiographies, biographies, festschrifts and obituaries of prominent oceanographers, marine biologists, fisheries scientists, and other scientists who worked in the marine environment published in journals and books after 1922, the publication date of Herdman’s Founders of Oceanography. The bibliography does not include newspaper obituaries, government documents, or citations to brief entries in general biographical sources. Items are listed alphabetically by author, and then chronologically by date of publication under a legend that includes the full name of the individual, his/her date of birth in European style(day, month in roman numeral, year), followed by his/her place of birth, then his date of death and place of death. Entries are in author-editor style following the Chicago Manual of Style (Chicago and London: University of Chicago Press, 14th ed., 1993). Citations are annotated to list the language if it is not obvious from the text. Annotations will also indicate if the citation includes a list of the scientist’s papers, if there is a relationship between the author of the citation and the scientist, or if the citation is written for a particular audience. This bibliography of biographies of scientists of the sea is based on Jacqueline Carpine-Lancre’s bibliography of biographies first published annually beginning with issue 4 of the History of Oceanography Newsletter (September 1992). It was supplemented by a bibliography maintained by Eric L. Mills and citations in the biographical files of the Archives of the Scripps Institution of Oceanography, UCSD. -
Martian Crater Morphology
ANALYSIS OF THE DEPTH-DIAMETER RELATIONSHIP OF MARTIAN CRATERS A Capstone Experience Thesis Presented by Jared Howenstine Completion Date: May 2006 Approved By: Professor M. Darby Dyar, Astronomy Professor Christopher Condit, Geology Professor Judith Young, Astronomy Abstract Title: Analysis of the Depth-Diameter Relationship of Martian Craters Author: Jared Howenstine, Astronomy Approved By: Judith Young, Astronomy Approved By: M. Darby Dyar, Astronomy Approved By: Christopher Condit, Geology CE Type: Departmental Honors Project Using a gridded version of maritan topography with the computer program Gridview, this project studied the depth-diameter relationship of martian impact craters. The work encompasses 361 profiles of impacts with diameters larger than 15 kilometers and is a continuation of work that was started at the Lunar and Planetary Institute in Houston, Texas under the guidance of Dr. Walter S. Keifer. Using the most ‘pristine,’ or deepest craters in the data a depth-diameter relationship was determined: d = 0.610D 0.327 , where d is the depth of the crater and D is the diameter of the crater, both in kilometers. This relationship can then be used to estimate the theoretical depth of any impact radius, and therefore can be used to estimate the pristine shape of the crater. With a depth-diameter ratio for a particular crater, the measured depth can then be compared to this theoretical value and an estimate of the amount of material within the crater, or fill, can then be calculated. The data includes 140 named impact craters, 3 basins, and 218 other impacts. The named data encompasses all named impact structures of greater than 100 kilometers in diameter. -
Planetary Constants and Models
JPL D-12947 PF-IOO-PMC-01 Mars Pathfinder ProJect PLANETARY CONSTANTS AND MODELS Mars at Launch Earth at La_ Dec 2, 1996 SunI, Earth at Mars at Aniva July 4, 1997 December 1995 JilL Jet Propulsion Laboratory California Institute of Technology Pasadena, California JPL D-I2947 PF-IOO-PMC-OI Mars Pathfinder Project PLANETARY CONSTANTS AND MODELS Prepared by: ' Robin Vaughan December 1995 JPL Jet Propulsion Laboratory California Institute of Technology Pasadena, California JPL D-12947 PFolOO-PMCoO1 Revision History Date Changes Status 10/95 Issued preliminary version for review by project person-el Draft 12/95 First official release; incorporated comments from prelimi- Final nary review. JPL D- !294 7 PFo 100-PMCo 01 Contents List of Figures V 4 List of Tables vii List of Acronyms and Abbreviations ix INTRODUCTION 1 1.1 Purpose ............ .......................... 1 1.2 Scope .................... ................... 1 2 COORDINATE SYSTEMS 3 2.1 Definitions 2.1.1 Frame • " • • • ° * ° • " ° • * • ° ° " ° ° * ° • • • ° " " " ' • • • • • • 3 2.1.2 Center • " " • ° " " " ' ° ° ° • * " • • " • " • • " • " " " ° • ° • • • . • 6 2.1.3 Type .................................... 7 2.2 Celestial Systems . ; ............................. 7 2.2.1 The Inertial Reference Frames ..................... 8 2.2.2 Sun-Centered Systems .......................... 9 2.2.3 Earth-Centered Systems ......................... 9 2.2.4 Mars-Centered Systems ......................... 11 2.2.5 Spacecraft-CenteredSystems ...................... 16 2.2.6 MiscellaneousSystems -
Local Lunar Gravity Field Analysis Over the South Poleaitken Basin from SELENE Farside Tracking Data
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, E02005, doi:10.1029/2011JE003831, 2012 Local lunar gravity field analysis over the South Pole-Aitken basin from SELENE farside tracking data Sander Goossens,1,2,3 Yoshiaki Ishihara,1 Koji Matsumoto,1 and Sho Sasaki1 Received 16 March 2011; revised 22 November 2011; accepted 13 December 2011; published 14 February 2012. [1] We present a method with which we determined the local lunar gravity field model over the South Pole-Aitken (SPA) basin on the farside of the Moon by estimating adjustments to a global lunar gravity field model using SELENE tracking data. Our adjustments are expressed in localized functions concentrated over the SPA region in a spherical cap with a radius of 45° centered at (191.1°E, 53.2°S), and the resolution is equivalent to a 150th degree and order spherical harmonics expansion. The new solution over SPA was used in several applications of geophysical analysis. It shows an increased correlation with high-resolution lunar topography in the frequency band l =40–70, and admittance values are slightly different and more leveled when compared to other, global gravity field models using the same data. The adjustments expressed in free-air anomalies and differences in Bouguer anomalies between the local solution and the a priori global solution correlate with topographic surface features. The Moho structure beneath the SPA basin is slightly modified in our solution, most notably at the southern rim of the Apollo basin and around the Zeeman crater. Citation: Goossens, S., Y. Ishihara, K. Matsumoto, and S. Sasaki (2012), Local lunar gravity field analysis over the South Pole-Aitken basin from SELENE farside tracking data, J. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
The Very Forward CASTOR Calorimeter of the CMS Experiment
EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH (CERN) CERN-EP-2020-180 2021/02/11 CMS-PRF-18-002 The very forward CASTOR calorimeter of the CMS experiment The CMS Collaboration* Abstract The physics motivation, detector design, triggers, calibration, alignment, simulation, and overall performance of the very forward CASTOR calorimeter of the CMS exper- iment are reviewed. The CASTOR Cherenkov sampling calorimeter is located very close to the LHC beam line, at a radial distance of about 1 cm from the beam pipe, and at 14.4 m from the CMS interaction point, covering the pseudorapidity range of −6.6 < h < −5.2. It was designed to withstand high ambient radiation and strong magnetic fields. The performance of the detector in measurements of forward energy density, jets, and processes characterized by rapidity gaps, is reviewed using data collected in proton and nuclear collisions at the LHC. ”Published in the Journal of Instrumentation as doi:10.1088/1748-0221/16/02/P02010.” arXiv:2011.01185v2 [physics.ins-det] 10 Feb 2021 © 2021 CERN for the benefit of the CMS Collaboration. CC-BY-4.0 license *See Appendix A for the list of collaboration members Contents 1 Contents 1 Introduction . .1 2 Physics motivation . .3 2.1 Forward physics in proton-proton collisions . .3 2.2 Ultrahigh-energy cosmic ray air showers . .5 2.3 Proton-nucleus and nucleus-nucleus collisions . .5 3 Detector design . .6 4 Triggers and operation . .9 5 Event reconstruction and calibration . 12 5.1 Noise and baseline . 13 5.2 Gain correction factors . 15 5.3 Channel-by-channel intercalibration . -
In Pdf Format
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Special Supplement to the Bulletin of the American Meteorological Society Vol
J. Blunden, D. S. Arndt, and M. O. Baringer, Eds. Associate Eds. H. J. Diamond, A. J. Dolman, R. L. Fogt, B. D. Hall, M. Jeffries, J. M. Levy, J. M. Renwick, J. Richter-Menge, P. W. Thorne, L. A. Vincent, and K. M. Willett Special Supplement to the Bulletin of the American Meteorological Society Vol. 92, No. 6, June 2011 STATE OF THE CLIMATE IN 2010 STATE OF THE CLIMATE IN 2010 JUNE 2011 | S1 HOW TO CITE THIS DOCUMENT __________________________________________________________________________________________ Citing the complete report: Blunden, J., D. S. Arndt, and M. O. Baringer, Eds., 2011: State of the Climate in 2010. Bull. Amer. Meteor. Soc., 92 (6), S1 –S266. Citing a chapter (example): Fogt, R. L., Ed., 2011: Antarctica [in “State of the Climate in 2010”]. Bull. Amer. Meteor. Soc., 92 (6), S161 –S171. Citing a section (example): Wovrosh, A. J., S. Barreira, and R. L. Fogt, 2011: [Antarctica] Circulation [in “State of the Climate in 2010”]. Bull. Amer. Meteor. Soc., 92 (6), S161 –S163. S2 | JUNE 2011 Editor & Author Affiliations (ALPHABETICAL BY NAME ) Achberger, Christine, Earth Sciences Centre, University of Belward, Alan S., Global Environment Monitoring Unit, IES, EC Gothenburg, Gothenburg, Sweden Joint Research Centre, Ispra, Italy Ackerman, Steven A., CIMSS University of Wisconsin - Madi- Benedetti, Angela, European Centre for Medium-Range son, Madison, Wisconsin Weather Forecasts, Reading, United Kingdom Ahlstrøm, A., Geological Survey of Denmark and Greenland Berrisford, Paul, NCAS-Climate, European Centre for Medi- (GEUS), -
A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars
minerals Review A Review of Sample Analysis at Mars-Evolved Gas Analysis Laboratory Analog Work Supporting the Presence of Perchlorates and Chlorates in Gale Crater, Mars Joanna Clark 1,* , Brad Sutter 2, P. Douglas Archer Jr. 2, Douglas Ming 3, Elizabeth Rampe 3, Amy McAdam 4, Rafael Navarro-González 5,† , Jennifer Eigenbrode 4 , Daniel Glavin 4 , Maria-Paz Zorzano 6,7 , Javier Martin-Torres 7,8, Richard Morris 3, Valerie Tu 2, S. J. Ralston 2 and Paul Mahaffy 4 1 GeoControls Systems Inc—Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA 2 Jacobs JETS Contract at NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (B.S.); [email protected] (P.D.A.J.); [email protected] (V.T.); [email protected] (S.J.R.) 3 NASA Johnson Space Center, Houston, TX 77058, USA; [email protected] (D.M.); [email protected] (E.R.); [email protected] (R.M.) 4 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA; [email protected] (A.M.); [email protected] (J.E.); [email protected] (D.G.); [email protected] (P.M.) 5 Institito de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico City 04510, Mexico; [email protected] 6 Centro de Astrobiología (INTA-CSIC), Torrejon de Ardoz, 28850 Madrid, Spain; [email protected] 7 Department of Planetary Sciences, School of Geosciences, University of Aberdeen, Aberdeen AB24 3FX, UK; [email protected] 8 Instituto Andaluz de Ciencias de la Tierra (CSIC-UGR), Armilla, 18100 Granada, Spain Citation: Clark, J.; Sutter, B.; Archer, * Correspondence: [email protected] P.D., Jr.; Ming, D.; Rampe, E.; † Deceased 28 January 2021. -
Nomenclature for Lunar Features at the Chang'e-3 Landing Site
Acta Geochim (2017) 36(2):213–223 DOI 10.1007/s11631-017-0159-1 ORIGINAL ARTICLE Nomenclature for lunar features at the Chang’e-3 landing site Zhoubin Zhang1,2 · Chunlai Li1,2,3 · Wei Zuo1,2,3 · Xingguo Zeng1,2 Received: 22 December 2016 / Revised: 15 February 2017 / Accepted: 9 April 2017 / Published online: 27 April 2017 © Science Press, Institute of Geochemistry, CAS and Springer-Verlag Berlin Heidelberg 2017 Abstract Nomenclatures for lunar features always published after some necessary approval procedures by the accompany the progresses of human lunar exploration, International Astronomical Union. which has an important dual meaning in culture and sci- ence. The naming of lunar features not only can Keywords Moon · Chang’e-3 · Landing site · Lunar commemorate the outstanding contributions of academics, feature nomenclature masters in various fields, and popularize the traditional cultures of ethnic groups all over the world, but also have a critical function of providing accurate indicative informa- 1 Introduction tion on features with special morphology, origin, nature and scientific value. However, nomenclature for features at Planetary nomenclature, like terrestrial nomenclature, is the Chang’e-3 landing site, which has a more arbitrary used to uniquely identify a feature on the surface of a form without many constrains posed by a uniformed sys- planet or satellite so that the feature can be easily located, tem, is unlike the features for other morphological units. described, and discussed. Nomenclature for lunar features This paper originated from the actual needs for the originated in the seventeenth century, as early scientists in description of scientific exploration activities, interpreta- that era used telescopes to observe the lunar surface, named tion of scientific research and dissemination of scientific the remarkable features on the lunar surface according to results.