Motions in the field of two rotating magnetic dipoles. II - Stability of the equilibrium points

Details Motions in the field of two rotating magnetic dipoles. II - Stability of the equilibrium points Motions in the field of two rotating magnetic dipoles. II - Stability of the equilibrium points

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986cemec..39...57g&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 39, May 1986, p. 57-65.

Mathematics

4

Gyromagnetism, Lagrangian Equilibrium Points, Magnetic Dipoles, Stellar Magnetic Fields, Equations Of Motion, Matrices (Mathematics), Roots Of Equations

Scientific paper

The stability of the equilibrium points found to exist (cf. Goudas et al., 1985) in the problem of two parallel, or antiparallel, magnetic dipoles that rotate about the centre of mass of their carrier stars, is studied by computing the characteristic roots of their variational equations. The characteristic equation, a biquadratic, solved for many combinations of μ and λ showed that all equilibrium points of this problem are unstable.

Affiliated with

Also associated with

No associations

Rating

Motions in the field of two rotating magnetic dipoles. II - Stability of the equilibrium points does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Motions in the field of two rotating magnetic dipoles. II - Stability of the equilibrium points, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Motions in the field of two rotating magnetic dipoles. II - Stability of the equilibrium points will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1773478