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DC Field | Value | Language |
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dc.contributor.author | Krishan, V | - |
dc.date.accessioned | 2008-12-16T09:58:48Z | - |
dc.date.available | 2008-12-16T09:58:48Z | - |
dc.date.issued | 1982-10 | - |
dc.identifier.citation | Solar Physics, Vol. 80, No.2, pp. 313 - 316 | en |
dc.identifier.issn | 0038-0938 (Print) 1573-093X (Online) | - |
dc.identifier.uri | http://hdl.handle.net/2248/4066 | - |
dc.description | Open Access | - |
dc.description.abstract | 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 | en |
dc.language.iso | en | en |
dc.publisher | D. Reidel Publishing Company | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1982SoPh...80..313K | en |
dc.relation.uri | http://www.springerlink.com/content/kn367772q447077v/ | en |
dc.rights | D. Reidel Publishing Company | - |
dc.subject | Solar Flares | en |
dc.subject | Tearing Modes (Plasmas) | en |
dc.subject | Electron Energy | en |
dc.subject | Solar Magnetic Field | en |
dc.title | Excitation of high-m tearing modes at the solar flare site | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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krishan.pdf | Open Access | 340.56 kB | Adobe PDF | View/Open |
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