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학술연구/단체지원/교육 등 연구자 활동을 지속하도록 DBpia가 지원하고 있어요.
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논문 기본 정보
- 자료유형
- 학술저널
- 저자정보
- 저널정보
- 한국우주과학회 Journal of Astronomy and Space Sciences Journal of Astronomy and Space Sciences 제38권 제2호
- 발행연도
- 2021.1
- 수록면
- 93 - 103 (11page)
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초록· 키워드
오류제보하기
In this work, the problem of resonance caused by some gravitational potentials due to Mercury and a third body, namely the Sun, together with some non-gravitational perturbations, specifically coronal mass ejections and solar wind in addition to radiation pressure, are investigated. Some simplifying assumptions without loss of accuracy are employed. The considered force model is constructed. Then the Delaunay canonical set is introduced. The Hamiltonian of the problem is obtained then it is expressed in terms of the Deluanay canonical set. The Hamiltonian is re-ordered to adopt it to the perturbation technique used to solve the problem. The Lie transform method is surveyed. The Hamiltonian is doubly averaged. The resonance capture is investigated. Finally, some numerical simulations are illustrated and are analyzed. Many resonant inclinations are revealed.
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참고문헌 (51)
참고문헌 신청
F.A. Abd El-Salam / 2006 / Invariant relative orbits for satellite constellations: A second order theory / Applied Mathematics and Computation 181(1):6~20
F.A. Abd El-Salam / 2007 / Perturbative effects on a Mercurian orbiter due to the solar radiation pressure, solar wind and the coronal mass ejections / New Astronomy 12(6):490~496
L. Anselmo / 1983 / Orbital perturbations due to radiation pressure for a spacecraft of complex shape / Celestial Mechanics 29(1):27~43
Arfken GB / 2012 / Mathematical Methods for Physicists: A Comprehensive Guide / Academic Press
A. R. Breen / 2002 / The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations / Annales Geophysicae 20(9):1291~1309
F.A. Abd El-Salam / 2007 / Perturbative effects on a Mercurian orbiter due to the solar radiation pressure, solar wind and the coronal mass ejections / New Astronomy 12(6):490~496
L. Anselmo / 1983 / Orbital perturbations due to radiation pressure for a spacecraft of complex shape / Celestial Mechanics 29(1):27~43
Arfken GB / 2012 / Mathematical Methods for Physicists: A Comprehensive Guide / Academic Press
A. R. Breen / 2002 / The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations / Annales Geophysicae 20(9):1291~1309
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