Analysis Activities' Published in the IGS Annual Report 2003/2004 (Gendt, 2005)
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Study of Existing Geodetic Datum of Nepal and Reviewing the Test Results of Seven Parameter Transformation
Study of Existing Geodetic Datum of Nepal and Reviewing the Test Results of Seven Parameter Transformation Niraj Manandhar (Geodesist) Chief Survey Officer Survey Department, Geodetic Survey Branch Abstract: In Nepal there exist different coordinate systems based on different geodetic datum. The existence of these datum and coordinate systems are poorly known. In this literature the geodetic datum that is in eXJistence in one way or other are illustrated and discussed. The next common problem encountered by users is the availability of authentic precise transformation parameter between National geodetic datum and World Geodetic Datum 1984 (WGS84) ; global datum used by global positioning system (GPS). There can exist a considerable difference in the position between local and the global system and the difference could be ofseveral hundred meters. Based on the availability of data three sets of transformation parameters has been determined. The tests have been carried out to evaluate the accuracy of the transformation parameter in this region. The final or third set of transformation parameter is recommended to transform the topographical data base of scale 1: 50, 000 and 1: 25. 000 of the whole country into WGS84 and vise versa and the parameter has been adopted by NGIJP of Survey Department of Nepal. The same set of transformation parameter can be used to transform the co-ordinates between Nepal datum a,:zd WGS84 in 87, 84 and 81 central meridian region, The final (third) set of transformation parameter is recommended in transforming the coordinates of whole country. The accuracy of the transformation parameters are specified and can be used accordingly. -
Very Long Baseline Interferometry
VERY LONG BASELINE INTERFEROMETRY R-l EARTH ORIENTATION PARAMETERS FROM IRIS-S VLBI MEASUREMENTS GIUB 93 R Ol GIUB 93 R 02 A. Nothnagel, R. Haas, J. Campbell, Geodetic Institute of the University of Bonn, Federal Republic of Germany G.D. Nicolson, Hartebeesthoek Radio Astronomy Observatory, South Africa Since 1990 the VLBI group at the Geodetic Institute of the University of Bonn (GIUB) regularly correlates and analyses VLBI experiments which are observed once per month under the acronym IRIS-S (International Radio Interferometric Surveying - South). The configuration of the IRIS-S network has undergone various changes in the recent past. Operations of the IRIS-S network started with five stations, i.e. Westford Observatory (Massachusetts, USA), Richmond Observatory (Florida, USA), Mojave Base Station (California, USA), Wettzell Geodetic Fundamental Station (Bavaria, Federal Republic of Germany) and Hartebeesthoek Radio Astronomy Observatory (South Africa). To date the IRIS-S network consists of Westford, Wettzell, Hartebeesthoek and a 12 m telescope near Santiago, Chile. The IRIS-S network configuration bears the invaluable advantage that it Covers both the northern and the southern hemisphere within the individual experiments. The data analysed consists of 34 sessions in quasi-monthly intervals from January 1990 to December 1992 (One Session had to be canceled and one is still being analysed for unresolved phase instabilities). Two different terrestrial and celestial reference frames are used in two separate analyses. In the first analysis the IERS Celestial Reference Frame 1991 (ICRF) and the IERS Terrestrial Reference Frame 1991 (ITRF) (IERS, 1992) together with the NNR-NUVEL1 Continental drift model (Argus and Gordon, 1991) are kept fixed. -
GEODETIC POSITIONING Study Guide
Canadian Board of Examiners for Professional Surveyors Core Syllabus Item C 6: GEODETIC POSITIONING Study Guide: The material is organized in sections that reflect the recommended progression of study. Often questions are followed by some additional explanations which are by no means exhaustive and do not replace the study of the references. They are meant to help linking different pieces of information from different textbooks in order to get a better insight. It is recommended to first answer the questions before reading the explanations. The topics covered are: 1. Coordinate systems (revision) 2. The Earth’s gravity field 3. Geodetic reference systems 4. Time scales and astronomy 5. Geopotential numbers and orthometric heights 6. Gravity measurement 7. Calculation of coordinates from terrestrial measurement 8. Space Reference systems used worldwide and in Canada. 9. The Global Positioning System and other Global Navigation Satellite Systems 1. Coordinate systems (revision) Review the details of the following coordinate types and their related transformations: 3D Cartesian geocentric coordinates (xyz) Ellipsoidal coordinates ( h) Planar coordinates related to a conformal projection (xp yp) Transformation between 3D-Cartesian and ellipsoidal coordinates Transformation between ellipsoidal and map projection coordinates References: [Torge (2001): chapter-4.1: The Rotational Ellipsoid] [Hofmann-Wellenhof et al. (2005): chapter-5.6.1: Coordinate transformation: Ellipsoidal and rectangular coordinates] [Hofmann-Wellenhof et al. (2007): chapter-8.2.3: Ellipsoidal coordinates and plane coordinates] Additional explanations: 3D Cartesian coordinates xyz are mathematically the most simple type of coordinates. Modern space techniques, like GPS for example, allow direct determination of this type of coordinates. However, they are not very appropriate for most surveying applications. -
23Rd European VLBI Group for Geodesy and Astrometry Working Meeting 14-19 May 2017 G¨Oteborg, Sweden Information
23rd European VLBI Group for Geodesy and Astrometry Working Meeting 14-19 May 2017 G¨oteborg, Sweden Information May 11, 2017 This page is intentionally left blank. II EVGA2017 information Scientific Organising Committee (SOC) Sabine Bachmann, Bundesamt f¨urKartographie und Geod¨asie,Germany • Alessandra Bertarini, Reichert GmbH / Bundesamt f¨urKartographie und Geod¨asie, • c/o Max Planck Institute for Radio Astronomy, Germany Johannes B¨ohm,Technische Universit¨atWien, Austria • R¨udigerHaas (Chair), Chalmers Tekniska H¨ogskola, Sweden • Evgeny Nosov, Institute of Applied Astronomy of the Russian Academy of Sci- • ences, Russia Nataliya Zubko, Finnish Geospatial Research Institute, Finland • Local Organising Committee (LOC) R¨udigerHaas (Chair) • Thomas Hobiger • Niko Kareinen • Grzegorz K lopotek • Camilla Andersson (administrative services) • Series of events during the EVGA2017 Date Time Event Location 14 May 18:00-20:00 Icebreaker and registration foyer Palmstedssalen 15 May 08:45-17:45 Oral presentations Palmstedssalen 17:45-20:45 Poster session foyer Palmstedssalen 16 May 09:00-17:45 Oral presentations day-2 Palmstedssalen 19:00-23:00 Conference dinner Wijkanders Restaurang 17 May 08:45-17:00 Various splinter meetings HA4, EDIT 3364, EL42 18 May 10:45-15:45 Onsala Twin Telescopes inauguration Onsala 19 May 09:00-18:00 IVS Directing Board Meeting #37 EDIT 3364 III Polstjärneg. Lindholmspiren Student Hotel City housing centre Bus City 19 Karlavagnsg. centre LANDALA Kapell- Läraregatan Kiosk TORG platsen Buses Buses 19,55 Lindholmsallén -
T . T L ^ IERS TECHNICAL NOTE 14 Earth Orientatiun Refcrence Frames
t .t l ^ IERS TECHNICAL NOTE 14 Earth orientatiun refcrence frames and atmosphcric excitation functions submitted for the 1992 IERS Annual Report VLBI, LLR, GPS, SLR and AAM IERS Analysis Centres P. Charlot (ed.) September 1993 Central Bureau of IERS - Observatoire de Paris 61, avenue de l'Observatoire F-75014 PARIS - France ERRATUM IERS Technical Note No 13 - IERS Standards (1992) P-9 GPS Block II dz m 0.9519 m vice 1.0229 m p. 18 Table 3.1, firstline, last value should be -0.0070 vice 0.0070. p. 83 Hobart Ql EW tangential phase should be 160.4 vice -160.4. p. 89 Malibu M2 EW tangential phase should be -142.4 vice 142.4. p.98 Pearblossom M2 radial phase should be -24.14 vice 24.1. p. 137 Paragraph 3, read ...of the International Astronomical Union, p. 137 the formula reads ds2 = -c2dr2 - - (1 - ^) (dx0)2 + (i + 2U) [(dx1)2 + (dx2)2 + (dx3)2], c2 c2 (the "minus" sign was omitted in the second line) p. 140, note 2: the formulas giving TCB-TCG, read Z e KB -KG - c' C f <v */2 • ü , (xj)dt • VÄ.(X - x)]. -2.. KB -KG - Lc X (JD -2443144.5) x 86400 + C*Se.(X • x^) * P (the "." in the vector product Ve. (x-xe) was omitted) 1992 IERS ANNVAL REPORT p. II-14, line 1 (title) p. 11-79, 80, 84, 86, Note 1 read ...SSC(IERS) 93 C 03 p. V-7, last table, lines 1, 3,5 Hl IERS Technical Notes This series of publications gives technical information related to the IERS activities, e.g. -
Very Long Baseline Interferometry
VERY LONG BASELINE INTERFEROMETRY EARTH ORIENTATION PARAMETERS FROM IRIS-S VLBI MEASUREMENTS GIUB92R01 GIUB 92 R 02 A. Nothnagel, J. Campbell, Geodetic Institute of the University of Bonn, Fed. Rep. of Germany G.D. Nicolson, Hartebeesthoek Radio Astronomy Observatory, South Africa In 1991 the VLBI group at the Geodetic Institute of the University of Bonn (GIUB) regularly correlated and analysed VLBI experiments which are observed once per month under the acronym IRIS-S (International Radio Interferometric Surveying - South). The Standard configuration of the IRIS-S network consists of five stations, i.e. Westford Observatory (Massachusetts, USA), Richmond Observatory (Florida, USA), Mojave Base Station (California, USA), Wettzeil Geodetic Fundamental Station (Bavaria, Federal Republic of Germany) and Hartebeesthoek Radio Astronomy Observatory (South Africa). The data analysed consists of 12 sessions in monthly intervals. Two different terrestrial and celestial reference frames were used in two separate analyses. The first set of reference frames was taken from the results of the global VLBI Solution GLB722 (= GSFC 91 R 04) of the VLBI group at the NASA Goddard Space Flight Center which contains all Mark III S/X experiments from 1979 to Decembcr 1990. The list of Station positions of GLB722 included continental drift parameters dx/dt, dy/dt, dz/dt for each Station which permitted the computation of Station coordinates refered to selected epochs. For the second set of computations the celestial reference frame RSC(IERS) 91 C 01 and the IERS Terrestrial Reference Frame 1990 (ITRF 90) for epoch 1988.0 together with the AM0-2 continental drift model (Minster and Jordan, 1978) were used. -
IERS TECHNICAL NOTE 11 Earth Orientation Reference Frames And
IERS TECHNICAL NOTE 11 Earth orientation reference frames and atmospheric excitation functions submitted for the 1991 IERS Annual Report VLBI, LLR, GPS, SLR and AAM IERS Analysis Centres P. Charlot (ed.) JUNE 1992 Central Bureau of EERS - Observatoire de Paris 61, avenue de l'Observatoire F-75014 PARIS - France IERS Technical Notes This series of publications gives technical Information about the IERS activities, e.g. reference frames, excitation of the Earth rotation, computational or analysis aspects, modeis, etc. It also contains descriptions and results of the analyses carried out by the IERS Analysis Centres and submitted for the EERS Annual Report global analyses. Back issues No 1 : C. Boucher and Z. Altamimi. The initial EERS Terrestrial Reference Frame. No 2 : Earth orientation and reference frame determinations, atmospheric excitation functions, up to 1988 (Annex to the IERS Annual Report for 1988). [No longer available, superseded by TNl. No 5]. No 3 : D.D. McCarthy (ed.). IERS Standards (1989) No 4 : C. Boucher and Z. Altamimi. Evaluation of the realizations of the Terrestrial Reference System done by the BIH and EERS (1984-1988). No 5: Earth orientation and reference frame determinations, atmospheric excitation functions, up to 1989 (Annex to the IERS Annual Report for 1989). [Superseded by T.N. No 8]. No 6 : C. Boucher and Z. Altamimi. ITRF89 and other realizations of the IERS Terrestrial Reference System for 1989. No 7 : E.F. Arias, M. Feissel and J.-F. Lestrade. The IERS extragalactic Celestial Reference Frame and its de with HIPPARCOS. No 8: Earth orientation and reference frame determinations, atmospheric excitation functions, up to 1990 (Annex to the EERS Annual Report for 1990). -
Establishment of Gps Reference Network in Ghana
DISSERTATION ESTABLISHMENT OF GPS REFERENCE NETWORK IN GHANA eingereicht von Yaw Poku-Gyamfi, M.Phil. Vollständiger Abdruck der an der Fakultät für Luft- und Raumfahrtechnik der Universität der Bundeswehr, München zur Erlangung des akademischen Grades eines Doktors der Ingenierwissenschaften (Dr.-Ing.) eingereichten Dissertation. Vorsitzender: Prof. Dr.-Ing. Bernhard Katzy (Chairman) 1. Berichterstatter: Prof. Dr.-Ing. Guenter Hein (1st Reviewer) 2. Berichterstatter: Prof. Dr.-Ing. Guenter Seeber (2nd Reviewer) 3. Berichterstatter: PD Dr.-Ing. Torben Schueler (3rd Reviewer) Der Dissertation wurde am 11.05.2009 bei der Universität der Bundeswehr München, Werner Heisenberg-Weg 39, 85577, Neubiberg eingereicht und durch die Fakultät für Luft- und Raumfahrttechnik am 16.11.2009 angenommen. Tag der mündlich Prüfung: 16.11.2009 Table of Contents Abstract The quest for the use of GNSS in developing countries is on the rise following the realization of its numerous advantages over the conventional methods of positioning, navigation and timing. Africa’s attempt to harness this technology has made it imperative to investigate the regional problems associated with its implementation by its member states, which constitute the AFREF. This study goes beyond the establishment of a GNSS reference network in Ghana by investigating and finding solutions to some of the regional problems associated with its implementation. The problem of turbulent atmospheric conditions which includes the severe ionospheric fluctuations and the erratic tropospheric conditions coupled with the sparsely populated base stations has led to the development of a new concept of correction, the Corridor Correction, which is able to correct the atmospheric effect comparable with the established concepts like the Virtual Reference Station, VRS, Flaechen-Korrektur-Parameter, FKP and Master Auxiliary Concept, MAC. -
Satellite Laser Ranging Measurements in South Africa Page 1 of 9
Review Article Satellite laser ranging measurements in South Africa Page 1 of 9 Satellite laser ranging measurements in South AUTHORS: Africa: Contributions to earth system sciences Christina M. Botai1 Ludwig Combrinck2,3 Joel O. Botai3 This contribution reassesses progress in the development of satellite laser ranging (SLR) technology and its scientific and societal applications in South Africa. We first highlight the current global SLR tracking stations AFFILIATIONS: within the framework of the International Laser Ranging Service (ILRS) and the artificial satellites currently 1South African Weather Service, being tracked by these stations. In particular, the present work focuses on analysing SLR measurements Pretoria, South Africa at Hartebeesthoek Radio Astronomy Observatory (HartRAO), South Africa, based on the MOBLAS-6 SLR 2Space Geodesy, Hartebeesthoek configuration. Generally, there is a weak geometry of ILRS stations in the southern hemisphere and the Radio Astronomy Observatory, SLR tracking station at HartRAO is the only active ILRS station operating on the African continent. The Krugersdorp, South Africa SLR-derived products – such as station positions and velocities, satellite orbits, components of earth’s 3 Department of Geography, gravity field and their temporal variations, earth orientation parameters – are collected, merged, achieved Geoinformatics and Meteorology, University of Pretoria, Pretoria, and distributed by the ILRS under the Crustal Dynamic Data Information System. These products are used in South Africa various research fields such as detection and monitoring of tectonic plate motion, crustal deformation, earth rotation, polar motion, and the establishment and monitoring of International Terrestrial Reference Frames, CORRESPONDENCE TO: as well as modelling of the spatio-temporal variations of the earth’s gravity field.