Excitation of high-m tearing modes at the solar flare site

Details Excitation of high-m tearing modes at the solar flare site Excitation of high-m tearing modes at the solar flare site

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...80..313k&link_type=abstract

Solar Physics, vol. 80, Oct. 1982, p. 313-316.

Physics

2

Solar Flares, Tearing Modes (Plasmas), Electron Energy, Solar Magnetic Field

Scientific paper

It is shown that high-m drift tearing modes can be excited under the conditions prevalent at the solar flare sites. Since the growth rate of the high-m tearing modes is larger than that for low-m macroscopic tearing modes and smaller than that of microscopic ion-acoustic instability, these modes warrant accommodation in the scheme of instabilities possibly operating in the hybrid model of solar flares suggested by Spicer.

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