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On the Tesseral-Harmonics Resonance Problem in Artificial-Satellite Theory, Part 2.

Author
Romanowicz, B. A.
Published
Mar 10, 1976.
Physical Description
1 electronic document
Online Version

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Summary
Equations were derived for the perturbations on an artificial satellite when the motion of the satellite is commensurable with that of the earth. This was done by first selecting the tesseral harmonics that contribute the most to the perturbations and then by applying Hori's method by use of Lie series. Here, are introduced some modifications to the perturbations, which now result in better agreement with numerical integration.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 19760014149.
Accession ID: 76N21237.
NASA-CR-146854.
SAO-SPECIAL-REPT-373-PT-2.
Terms of Use and Reproduction
No Copyright.
View MARC record | catkey: 15736405