Improving magnetosphere in situ observations using solar sails |
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Authors: | Khashayar Parsay Hanspeter Schaub Conrad Schiff Trevor Williams |
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Affiliation: | 1. Aerospace Engineering Sciences Department, University of Colorado, Boulder, CO 80309-0431, USA;2. NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USA |
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Abstract: | Past and current magnetosphere missions employ conventional spacecraft formations for in situ observations of the geomagnetic tail. Conventional spacecraft flying in inertially fixed Keplerian orbits are only aligned with the geomagnetic tail once per year, since the geomagnetic tail is always aligned with the Earth-Sun line, and therefore, rotates annually. Solar sails are able to artificially create sun-synchronous orbits such that the orbit apse line remains aligned with the geomagnetic tail line throughout the entire year. This continuous presence in the geomagnetic tail can significantly increase the science phase for magnetosphere missions. In this paper, the problem of solar sail formation design is explored using nonlinear programming to design optimal two-craft, triangle, and tetrahedron solar sail formations, in terms of formation quality and formation stability. The designed formations are directly compared to the formations used in NASA’s Magnetospheric Multi-Scale mission. |
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Keywords: | Solar sail Formation flying Magnetosphere mission Heliophysics |
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