Magnetic Reconnection Model for X-Ray Flare Loop Interaction

Details Magnetic Reconnection Model for X-Ray Flare Loop Interaction Magnetic Reconnection Model for X-Ray Flare Loop Interaction

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.226...31z&link_type=abstract

Astrophysics and Space Science, Volume 226, Issue 1, pp.31-46

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The subtle interactions between the magnetohydrodynamics (MHD) and transverse plasmons are investigated. It is shown that there is a resistive instability by the plasmon's soliton in a current sheet, which eventually turns into an eruptive instability at the magnetic field reconnection. In the case of ion-acoustic turbulence, the high temperature current sheet model must adopt the aromalous conductivity instead of the Coulomb conductivity. The numerical results are consistent with the observations obtained by Hanaoka (1994). Thus the flare caused by X-ray loop coalescence can be basically interpreted by this model of magnetic field reconnection driven by ponderomotive force.

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