Magneto-Fluid Coupling - Eruptive Events in the Solar Corona

Details Magneto-Fluid Coupling - Eruptive Events in the Solar Corona Magneto-Fluid Coupling - Eruptive Events in the Solar Corona

2001-04-09

arxiv.org/abs/astro-ph/0104138v1

Astronomy and Astrophysics

Astrophysics

4 pages of two-column text (Latex) plus 3 pages of figures, submitted to The Astrophysical Journal Letters

Scientific paper

10.1086/323651

By modelling the coronal structures by "slowly" evolving Double-Beltrami
two-fluid equilibria (created by the interaction of the magnetic and velocity
fields), the conditions for catastrophic transformations of the original state
are derived. It is shown that, at the transition, much of the magnetic energy
of the original state is converted to the the flow kinetic energy.

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