The thermal instability of the current sheet and the formation of coronal loops

Details The thermal instability of the current sheet and the formation of coronal loops The thermal instability of the current sheet and the formation of coronal loops

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980izssr..44.2465s&link_type=abstract

(Seminar po Vzaimodeistviiu Kosmicheskikh Luchei so Sredoi, Leningrad, USSR, Nov. 30-Dec. 2, 1979.) Akademiia Nauk SSSR, Izvesti

Physics

Coronal Loops, Current Sheets, Longitudinal Stability, Solar Corona, Thermal Instability, Directional Stability, Energy Dissipation, Magnetohydrodynamic Flow, Neutral Sheets, Small Perturbation Flow, Thermal Conductivity

Scientific paper

A theoretical study is presented of the longitudinal stability of a current sheet, homogeneous in the direction of the current, in the solar corona. The problem of the stability of the plane neutral sheet with respect to small perturbations with a wave vector parallel to the current is solved in the MHD approximation with allowance for heat conductivity and radiative energy losses.

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