Conversion of spherical harmonics (Kaula, 3.3)I2.2a We want to express the terms in the expansion in Kepler variables:. C.C.Tscherning, 2005-11-03.

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Presentation transcript:

Conversion of spherical harmonics (Kaula, 3.3)I2.2a We want to express the terms in the expansion in Kepler variables:. C.C.Tscherning,

Kaula (3.48, 49) C.C.Tscherning,

Kaula (3.51) C.C.Tscherning,

Kaula (3.53, 54) C.C.Tscherning,

Kaula (3.55,56), fig. 4. C.C.Tscherning,

Kaula (3.57). C.C.Tscherning,

Development of P nm C.C.Tscherning,

Kaula (3.58,59). C.C.Tscherning,

Kaula (3.60,). C.C.Tscherning,

Kaula (3.61, 62). C.C.Tscherning,

Kaula Table 1. C.C.Tscherning,

Kaula C.C.Tscherning,

Kaula 3.72, C.C.Tscherning,

Kaula C.C.Tscherning,

Kaula With C 20 = , e=0.001, a=1.2a e C.C.Tscherning,

Kaula C.C.Tscherning,

Resonance, Kaula 3.6 Terms become zero, or ”infinite” by division with zero. C.C.Tscherning,

Orbit with repeating ground track Orbit which gives resonance with specific term(s) Orbit which is sun-syncroneous Orbit which enables close ”encounter” with an object, such as the poles. Applications C.C.Tscherning,