Basics of Rotating Magnetospheres: Equilibrium and Stability

Details Basics of Rotating Magnetospheres: Equilibrium and Stability Basics of Rotating Magnetospheres: Equilibrium and Stability

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.277..247f&link_type=abstract

Astrophysics and Space Science, v. 277, Issue 1/2, p. 247-257 (2001).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the basic characteristics of a rotating magnetosphere. More specifically, we describe its overall equilibrium state, explain the ‘subcorotation’ phenomenon resulting from plasma production or from outward transport, discuss the conditions under which a magnetospheric system is driven unstable, and comment on the nature of the unstable motions, with emphasis on the interchange motions believed to be responsible for the outward plasma transport.

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