VLBI satellite tracking for the realization of frame ties /
详细信息    VLBI satellite tracking for the realization of frame ties /
  • 出版日期:2014.
  • 语种:eng
  • 出版者:The Dept. of Geodesy and Geoinformation of the Vienna University of Technology,
  • 出版地:Vienna, Austria :
  • 第一责任说明:Lucia Plank.
  • 尺寸:30 cm.
  • 分类号:a814
  • ISBN:(pbk.) :
MARC全文
02h0065681 20141224165716.0 141204s2014 au a frb |000|||eng | (pbk.) : CNY419.00 NGL NGL NGL eng eng ; ger a814 Plank, Lucia. VLBI satellite tracking for the realization of frame ties / Lucia Plank. Vienna, Austria : The Dept. of Geodesy and Geoinformation of the Vienna University of Technology, 2014. ix, 143 p. : ill. ; 30 cm. Geowissenschaftliche Mitteilungen, 1811-8380 ; Heft Nr. 95 Includes bibliographic reference. Very Long Baseline Interferometry (VLBI) is a well-probed space geodetic technique used to determine the Celestial Reference Frame (CRF), the Terrestrial Reference Frame (TRF) and the Earth Orientation Parameters (EOP) in between. Alternatively, VLBI is generally used in spacecraft tracking. Today’s most precise and reliable realizations of the TRF rely on the measurements of several space geodetic techniques and the corresponding inter-technique ties. For future improvement, alternative methods for connecting the various space geodetic techniques, establishing precise frame ties, are urgently needed. A promising solution is the use of VLBI satellite observations, either in combination with a so-called space tie realized by a dedicated satellite or by directly observing satellites of the Global Navigation Satellite Systems (GNSS) with VLBI. This thesis contains a detailed simulation study of VLBI observations to satellites, identifying adequate observing strategies for the precise determination of antenna positions on Earth in the satellite’s system. For satellites at heights between 1000 and 20000 km, adequate observation strategies are found that allow the determination of the station coordinates at the level of a few millimeters. Hereby, the approach of weekly solutions in chosen, meaning that one satellite is observed by either a regional or a global antenna network during seven consecutive days. In the case of VLBI observations to a satellite of the GNSS, alternative observing strategies are needed. In this thesis the combination with a classical VLBI session observing extragalactic radio sources or the observation of a satellite constellation are also introduced. Abstract in English and German. Very long baseline interferometry. ; Satellite navigation. Geowissenschaftliche Mitteilungen ; Helf Nr. 95. aCN b010001 010001 P 206.6 G29w v95 ; h1 ; rCNY419.00 gljx1405

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