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Excitation of high-mtearing modes at the solar flare site

✍ Scribed by V. Krishan


Publisher
Springer
Year
1982
Tongue
English
Weight
209 KB
Volume
80
Category
Article
ISSN
0038-0938

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✦ Synopsis


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.