Tesseral resonance on Imp 4 orbit
作者： Barbara E. Lowrey
关键词: Orbital elements 、 Orbital period 、 Gravitational field 、 Commensurability (astronomy) 、 Ground track 、 Earth's rotation 、 Rotation period 、 Physics 、 Geodesy 、 Geopotential 、 Earth-Surface Processes 、 Ecology (disciplines) 、 Earth and Planetary Sciences (miscellaneous) 、 Space and Planetary Science 、 Palaeontology 、 Forestry 、 Aquatic science 、 Atmospheric Science 、 Soil science 、 Geochemistry and Petrology 、 Geophysics 、 Oceanography 、 Water Science and Technology
摘要: The supersynchronous resonance occurred because the orbital period of 4 1/3 days was nearly commensurate with earth's rotational period. satellite launched on May 24, 1967. perturbation due to commensurability is discussed, giving attention ground track longitude at perigee passage and effect tesseral harmonic time passage. measurement Imp accurate enough provide a stringent test third-degree terms in model gravitational field.
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jaxa.jp参考文章(3)
Carl A. Wagner, Bruce C. Douglas, Perturbations of existing resonant satellites Planetary and Space Science. ,vol. 17, pp. 1505- 1517 ,(1969) , 10.1016/0032-0633(69)90171-8
Barbara E. Lowrey, Ephemeris of a Highly Eccentric Orbit - Explorer 28 Celestial Mechanics and Dynamical Astronomy. ,vol. 5, pp. 107- 125 ,(1972) , 10.1007/BF01229516
G. S. Gedeon, Tesseral resonance effects on satellite orbits Celestial Mechanics and Dynamical Astronomy. ,vol. 1, pp. 167- 189 ,(1969) , 10.1007/BF01228837