Areas of equatorial motion in the Magnetic-Binary problem

Details Areas of equatorial motion in the Magnetic-Binary problem Areas of equatorial motion in the Magnetic-Binary problem

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cemec..37..161k&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 37, Oct. 1985, p. 161-170.

Physics

18

Earth-Moon System, Magnetic Dipoles, Particle Motion, Two Body Problem, Charged Particles, Equations Of Motion, Magnetic Moments, Steepest Descent Method, Sun

Scientific paper

In the process of modelling the magnetic-binary systems, the authors deal with the permissible areas of motion in the equatorial planes of the representative model. The zero velocity curves, derived by the well known steepest descent method, provide the means for determining these areas. Further these curves reveal all the equilibrium points located on the above planes.

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