Mathematics
Scientific paper
Jul 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983cemec..30..219m&link_type=abstract
Celestial Mechanics (ISSN 0008-8714), vol. 30, July 1983, p. 219-224.
Mathematics
4
Celestial Mechanics, Circular Orbits, Magnetic Dipoles, Two Body Problem, Astronomical Models, Charged Particles, Equations Of Motion, Particle Motion, Singularity (Mathematics), Space-Time Functions
Scientific paper
The separate regularization of the singularities in a magnetic-binary system is presently achieved by changing both coordinates and time. The basis of the model employed is a pair of primary magnetic spherical bodies revolving in circular orbits around their center of mass, under mutual Newtonian attraction. Attention is given to the reason why relating the geometric transformation to the rescaling of time is the most efficient approach in the solving of this problem.
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