New magnetic reconnection theory.

Details New magnetic reconnection theory. New magnetic reconnection theory.

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..338l&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 3, p. 338 - 342

Physics

Magnetohydrodynamics: Solar Corona, Magnetohydrodynamics: Instabilities

Scientific paper

The subtle interactions between magnetohydrodynamics and high-frequency plasma waves involving transverse and lontitudinal modes are investigated. It is shown that there is a resistive instability caused by transverse plasmon and the Langmuir solitons in a current sheet, which eventually turns into an eruptive instability at the magnetic field reconnection. In the case of enhanced ion-acoustic turbulence, the high temperature current sheet model must adopt the anomalous conductivity instead of the Coulomb conductivity. The estimated results are consistent with the observations. Thus the flare-like brightenings can be basically interpreted by use of this model of magnetic field reconnection with the ponderomotive force.

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