On the station keeping of a solar sail in the elliptic Sun-Earth system

被引：8

作者：

Farres, Ariadna ^{[1
]}

Jorba, Angel ^{[1
]}

机构：

[1] Univ Barcelona, E-08007 Barcelona, Spain

来源：

ADVANCES IN SPACE RESEARCH | 2011年 / 48卷 / 11期

关键词：

Solar sail; Periodic orbits; Station keeping; Dynamical systems;

D O I：

10.1016/j.asr.2011.02.004

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

In this work we focus on the dynamics of a solar sail in the Sun-Earth Elliptic Restricted Three-Body Problem with solar radiation pressure. The considered situation is the motion of a sail close to the L-1 point, but displacing the equilibrium point with the sail so that it is possible to have continuous communication with the Earth. In previous works we derived a station keeping strategy for this situation but using the Circular RTBP as a model. In this paper we discuss the effect of the eccentricity in the region close to the sail-displaced L-1 point of the Circular RTBP. Then we show how to use the information on this dynamics to design a station keeping strategy. Finally, we apply these results to the GeoStorm mission, including errors in the sail orientation and on the estimation of the position of the sail in the simulations. (C) 2011 COSPAR. Published by Elsevier Ltd. All rights reserved.

引用

页码：1785 / 1796

页数：12

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