| タイトル | Simulation and analysis of a geopotential research mission |
| 本文（外部サイト） | http://hdl.handle.net/2060/19880004727 |
| 著者（英） | White, Lisa K. |
| 著者所属（英） | Texas Univ. |
| 発行日 | 1987-12-01 |
| 言語 | eng |
| 内容記述 | Methods for the determination of the initial conditions for the two satellites that will satisfy Geopotential Research Mission (GRM) requirements are investigated. For certain gravitational recovery techniques, the satellites must remain close to a specified separation distance and their groundtracks must repeat after a specified interval of time. Since the objective of the GRM mission is to improve the gravity model, any pre-mission orbit predicted using existing gravity models will be in error. A technique has been developed to eliminate the drift between the two satellites caused by gravitational modeling errors and return them to repeating groundtracks. The concept of frozen orbits, which minimize altitude variations over given latitudes, was investigated. Finally, the effects of temporal perturbations on the relative range-rate signal were studied. At the proposed altitude of 160 km, the range-rate signal produced by perturbations other than the static geopotential field are dominated by the luni-solar effect. This study demonstrates that the combined effects of all the temporal perturbations does not prevent the orbit from being frozen or the satellites from obtaining a repeating groundtrack to within a specified closure distance. |
| NASA分類 | ASTRODYNAMICS |
| レポートNO | 88N14109
CSR-87-2
NASA-CR-182354
NAS 1.26:182354 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/147928 |
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