Chaotic Attitude Tumbling of Satellite in Magnetic Field
Abstract
In this study, the half width of the chaotic separatrix has been estimated by chrikov's criterion. Through surface of section method, it has been observed that the magnetic torque parameter, the eccentricity of the orbit and the mass distribution parameter play an important in changing the regular motion into chaotic one.
DOI: https://doi.org/10.3844/ajassp.2006.2037.2041
Copyright: © 2006 Rashmi Bhardwaj and Parsan Kaur. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
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Keywords
- Chaos
- celestial mechanics
- solar system
- periodic orbits
- poincare section