A perturbation solution of the main problem in artificial satellite theory
Approved for public release, distribution unlimited === The main problem of artificial satellite theory is a restricted two body problem in which the Legendre Polynomial representation of the cylindrically symmetric potential contains only the first two terms. A generalized asymptotic expansion is u...
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Monterey, California. Naval Postgraduate School
2013
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ndltd-nps.edu-oai-calhoun.nps.edu-10945-306622015-01-26T15:55:35Z A perturbation solution of the main problem in artificial satellite theory Sagovac, Christopher Patrick. Danielson, Donald A. Frensen, Christopher L. Naval Postgraduate School (U.S.) Applied Mathematics Approved for public release, distribution unlimited The main problem of artificial satellite theory is a restricted two body problem in which the Legendre Polynomial representation of the cylindrically symmetric potential contains only the first two terms. A generalized asymptotic expansion is used to obtain a first order approximation. The solution at the critical inclination is seen to be of a different type than at other inclinations. The solution is finite for all eccentricities and inclinations when suitably restricted in time. 2013-04-11T22:14:54Z 2013-04-11T22:14:54Z 1990-06 Thesis http://hdl.handle.net/10945/30662 en_US This publication is a work of the U.S. Government as defined in Title 17, United States Code, Section 101. As such, it is in the public domain, and under the provisions of Title 17, United States Code, Section 105, it may not be copyrighted. Monterey, California. Naval Postgraduate School |
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description |
Approved for public release, distribution unlimited === The main problem of artificial satellite theory is a restricted two body problem in which the Legendre Polynomial representation of the cylindrically symmetric potential contains only the first two terms. A generalized asymptotic expansion is used to obtain a first order approximation. The solution at the critical inclination is seen to be of a different type than at other inclinations. The solution is finite for all eccentricities and inclinations when suitably restricted in time. |
author2 |
Danielson, Donald A. |
author_facet |
Danielson, Donald A. Sagovac, Christopher Patrick. |
author |
Sagovac, Christopher Patrick. |
spellingShingle |
Sagovac, Christopher Patrick. A perturbation solution of the main problem in artificial satellite theory |
author_sort |
Sagovac, Christopher Patrick. |
title |
A perturbation solution of the main problem in artificial satellite theory |
title_short |
A perturbation solution of the main problem in artificial satellite theory |
title_full |
A perturbation solution of the main problem in artificial satellite theory |
title_fullStr |
A perturbation solution of the main problem in artificial satellite theory |
title_full_unstemmed |
A perturbation solution of the main problem in artificial satellite theory |
title_sort |
perturbation solution of the main problem in artificial satellite theory |
publisher |
Monterey, California. Naval Postgraduate School |
publishDate |
2013 |
url |
http://hdl.handle.net/10945/30662 |
work_keys_str_mv |
AT sagovacchristopherpatrick aperturbationsolutionofthemainprobleminartificialsatellitetheory AT sagovacchristopherpatrick perturbationsolutionofthemainprobleminartificialsatellitetheory |
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1716728502935355392 |