The heating mechanism and stability of the giant POST flare arch of 21-22 May, 1980

Details The heating mechanism and stability of the giant POST flare arch of 21-22 May, 1980 The heating mechanism and stability of the giant POST flare arch of 21-22 May, 1980

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992chjss..12..161t&link_type=abstract

Chinese Journal of Space Science (ISSN 0254-6124), vol. 12, no. 3, p. 161-170.

Physics

Magnetohydrodynamic Stability, Solar Corona, Solar Flares, Tearing Modes (Plasmas), Cylindrical Plasmas, Solar Magnetic Field

Scientific paper

It is proposed here that the fast tearing modes in cylindrical geometry are an effective heating mechanism for postflare coronal arch of May 21-22, 1980, which remained visible for more than 10 hrs after onset. The magnetic energy supplied by the tearing modes is calculated along with the corresponding fast tearing modes growth rate and time. The MHD equilibrium and the stability of the arch are discussed.

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