Abstract

Satellite formation flight missions have long durations, so long-term perturbation effects (such as the J 2 effect) must be countered to maintain the formation. One possible approach to this problem is to affix a small reflective surface (called a "solar wing") to the satellite solar radiation pressure can then be harnessed to maintain formation flight. In this paper a lull dynamic model for the long-term relative motion of formation flight is formulated, and an optimal solar wing steering law is devised for the formation-keeping problem. A numerical example is given to illustrate the approach.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.