Loss of magnetic tension in pre-flare magnetic configurations
โ Scribed by P. Venkatakrishnan
- Publisher
- Springer
- Year
- 1990
- Tongue
- English
- Weight
- 378 KB
- Volume
- 128
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
On the assumption that solar flares are due to instabilities which occur in current sheets in the Sun's atmosphere, one may classiC, magnetic-field configurations associated with [lares into two types. One is characterized by 'closed' current sheets, magnetic-field lines adjacent to these sheets beg
Observations of radio emission at 3.3 mm wavelength associated with magnetic fields in active regions are reported. Results of more than 200 regions during the years 1967-1968 show a strong correlation between peak enhanced millimeter emission, total flux of the longitudinal component of photospheri