IGS Analysis Center Workshop - IGS - NASA

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IGS Agency Acronyms:Network Station Implementation and Operation‘.. -. .-. . . . . . ------- .IESAS Academia Sinica, Institute of Earth Sciences, TaiwanAUSLIG Australian Survey and Land Information GroupBfL ‘ Bundesamt fur Landeslopographie (Federal Topography), SwitzerlandCGS Canadian Geodetic Survey, EMR, CanadaCNES Centre National de Etudes, Toulouse, FranceCEE Centro de Estudios Espaciales, ChileCDDIS Crustal Dynamics Data Information System, USADMA Defense Mapping Agency, USAOUT Delft University of Technology, NetherlandsDOSLI Department of Survey and Land Information, Wellington, New ZealandERI Earthquake Research Institute, University of TokyoEMR Energy Mines and Resources, CanadaESA European Space AgencyESOC European Space Operations CenterFGI Finnish Geodetic Institute, FinlandGFZ GeoforschungsZentrum Institute, Potsdam, GermanyGSI Geographical Suwey Institute, Tsukuba, JapanGSC Geological Survey of Canada, EMR, CanadaGSFC Goddard Space Flight Center, USAlfAG Insti-tut fur Angewandte Geodasie, Frankfurl, GermanyIGN Institut Geographique National, Paris, FranceISAS Institute for Space and Astronautic Science, Sagamihara, JapanISRO Institute for Space Research Observatory, Graz, AustriaMA Institute of Applied Astronomy, St. Petersburg , RussiaIBGE Instituto Brasileiro de Geografia de Estatistica, BrazilfNPE Instituto National de Pesquisas Espaciais, BrazilISA Italian Space Agency, Matera, ItalyJPL Jet Propulsion Laboratory, USANASA National Aeronautics and Space Administration, USANBSM National Bureau of Surveying And Mapping, ChinaNGS National Geodetic Survey, USANOAA National Oceanic and Atmospheric Administration, USAROB Observatoire Royal de Belgium, Brussels, Belgium0s0 Onsala Space Observatory, SwedenRGO Royal Greenwich Observatory, UKSlo . Scripps Institution of Oceanography, San Diego, CA, USA ‘SAOSDCSKUFPRWUTWruShanghai Astronomical Obsewatory, ChinaSpace Device Corporation, RussiaStatens Kartverk, Norwegian Mapping Authority, NorwayUniversity Federal de Parana, BrazilWarsaw University of Technology, PolandWuhan Technical University, China109Status: Octobar 8, 1993
. Ruth Neilan16S Central BureauJet Propulsion LaboratoryM/S 238-5404800 Oak Grove DrivePasadena, CA 91109 USAPhone (818) 354-8330FAX (818) 393-6686Internet: ren@logos.jpl .noso.govIGS ~usERYxE● Lees MervartAstronc+nical Institut-University of BernUniversity of BernSidlerstrasse 5CH - 3012 BernSwitzerlandPhone 41 31 65 8591FAX41 31 653869Internet: mervart@aiub.unibe. ch● The IGS Mail Service Center will be relocated to the Central Bureau byJanuary 1994. More details will be available in Decenber, 1993.● Carey NellCrustal Dynamics Data Information SystemNASA/Goddard Space Flight CenterCode 902.2Greenbelt, MD 20771-0001 USAPhone (301) 286-9283FAX (301) 286-4943Internet: noll@cddis.gsfc .nasa.gov. Loic DanielIGN - Institut Geographique National2, avenue PasteurF - 94160 Saint-MandeFrancePhone 33 1 4398 8338FAX 33 1 4398 8488Internet: igsadn@ign.fr● Yehuda BockUniversity of California - San DiegoScripps Institution of OceanographyInstitute for Geophysics and Planetary PhysicsIGPP 0225La Jolla, CA 92093 USAPhone (619) 534-5292FAX (619) 534-5332Internet: bockt?bul l.ucsd.edu.16S COMACTL15T OCTOBER 1993110
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●INTERNATIONAL ASSOCIATION OF GEO
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TABLE OF CONTENTS.FINAL AGENDA . .
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13:30 NGS14:00 S1014:30 EMR15:00 CO
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LIST OF PARTICIPANTS:Prof. Gerhard
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Table 1. Current IGS Analysis Cente
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The first field identifies the reco
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Summary InformationThe third produc
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From Figure 1 we find that there ar
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to define a reference clock in thei
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SESSION 2(IGS orbit products)
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1. introductionThe main objectives
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ecause of the above averaging. This
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RMS per center (m)o 0 0 0 0 0 oA0Iv
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Scale (ppb)I I I I I 11+-b~ul0Amo&I
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and NGS. Note that the day to day v
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Rotation around X-axis (mas)1&0 0o
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discussed in Section 3 are here see
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-----------------------------------
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Residuals in Meters1 1 1 1 1 1 1=%m
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Residuals inMeters11111cnficJJw-o A
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I I I—Residuals in Meters..—.
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1111ResidualsMeters,—{44
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Residuals in MetersI I I II I I IIc
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Rms in MetersI 1 ! I 1 10 n0 a0n.ff
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IGS- and the COM-sets, but that the
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Table 4.1 N.A. Baseline Repeatabili
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..Figure 5.1:Clock solutions for FA
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specifically the preanalysis can be
Page 61 and 62: discussion, a question as to whethe
Page 63 and 64: SUMMARY OF SESSION 3This Session be
Page 65 and 66: IGS POSITION PAPER, IGS ANALYSIS CE
Page 67 and 68: and Earth orientation parameters (E
Page 69 and 70: LbPIERS and IGSCentral Bureausand D
Page 71 and 72: @ IGS will develop instructions, an
Page 73: 2.2 Analysis Center System DesignFi
Page 76 and 77: applied to the solution in order to
Page 78 and 79: ..standard deviations. This is conv
Page 80 and 81: known, the two solutions will be ad
Page 82 and 83: errors, and can therefore be used a
Page 84 and 85: International Terrestrial Reference
Page 86 and 87: Thus, there is the potential of fee
Page 88 and 89: 90” 100” 110” 120” 130” 1
Page 91 and 92: adiation parameters for each satell
Page 93 and 94: Bock, Y., R.I. Abbot, C.C. Counselm
Page 95 and 96: SUMMARY OF SESSION 4This session st
Page 97 and 98: INTERNATIONAL EARTH ROTATION SERVIC
Page 99 and 100: x- differences with IERS0.001”I I
Page 101 and 102: SUMMARY OF SESSION 5In the last ses
Page 103 and 104: 1) I(X3 PROCESSING/REPORTS/FORMATSS
Page 105 and 106: IGS should foster and encourage reg
Page 107 and 108: ..INTERNATIONAL GPS SERVICE FORGEOD
Page 109 and 110: ortL.s.4
Page 111: 1234567a91011121314IsIt17ItIs2C2122
Page 115 and 116: ON1T.>● Jim ZumbergeJet Propulsio
Page 117: PROPOSED ORGANIZATION OF THE INTERN
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IGS Analysis Center Workshop - IGS - NASA

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