Dynamic regimes of prominence evolution

Details Dynamic regimes of prominence evolution Dynamic regimes of prominence evolution

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..139..299b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 139, no. 2, June 1992, p. 299-314.

Physics

8

Plasma Dynamics, Solar Magnetic Field, Solar Prominences, Cold Plasmas, Dynamic Models, Maxwell Equation

Scientific paper

The dynamical model of a solar prominence taking into account plasma motion in the form of a cumulative flux was developed. Of great importance is the fact that the prominence plasma is partially ionized. Ion-neutral collisions in nonsteady flux conditions radically change the energetics and dynamics of the prominence model. In this case the equilibrum state described by the Kippenhahn-Schlueter solutions becomes unstable, and various dynamic regimes of plasma compression, as well as monotonic or quasi-periodic expansion of the plasma can exist in the prominence.

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