Self-Shadowing of a Spacecraft in the Computation of Surface Forces. An Example in Planetary Geodesy

Author:

Balmino G.1,Marty J.C.1

Affiliation:

1. Centre National d'Etudes Spatiales, Groupe de Recherches de Geodesie Spatiale , 18, Avenue Edouard Belin, 31401 Toulouse Cedex 9, France

Abstract

Abstract We describe in details the algorithms used in modelling the self-shadowing between spacecraft components, which appears when computing the surface forces as precisely as possible and especially when moving parts are involved. This becomes necessary in planetary geodesy inverse problems using more and more precise orbital information to derive fundamental parameters of geophysical interest. Examples are given with two Mars orbiters, which show significant improvement on drag and solar radiation pressure model multiplying factors, a prerequisite for improving in turn the determination of other global models.

Publisher

Walter de Gruyter GmbH

Reference21 articles.

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3. Clavier, C. (1991), Modelisation des forces de surface sur un satellite artificiel, Technical report, C.N.E.S.

4. Folkner, W.M., R.D. Kahn, R.A. Preston, C.F. Yoder, E.M. Standish, J.G. Williams, C.D. Edwards, R.W. Hellings, T.M. Eubanks, and B.G. Bills (1997), Mars Dynamics from Earth-based trackingof the Mars Pathfinder lander, J. Geophys. Res. 102, 4057-4064.10.1029/96JE02125

5. Folkner W.M., Williams J.G., Boggs D.H., Park R.S., and Kuchynka P. (2014),The Planetary and Lunar Ephemerides DE430 and DE431, IPN Progress Report 42-196.

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