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http://hdl.handle.net/2248/206
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DC Field | Value | Language |
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dc.contributor.author | Uddin, W | - |
dc.contributor.author | Pande, M. C | - |
dc.contributor.author | Verma, V. K | - |
dc.date.accessioned | 2005-01-08T08:44:16Z | - |
dc.date.available | 2005-01-08T08:44:16Z | - |
dc.date.issued | 1988 | - |
dc.identifier.citation | Kodaikanal Observatory Bulletins Series A, Vol. 9, pp. 223 | en |
dc.identifier.issn | 0374-3632 | - |
dc.identifier.uri | http://hdl.handle.net/2248/206 | - |
dc.description.abstract | In the present investigation we have studied the relation between solar proton flares and associated optical, radio and x-ray events. It is found that optical flares are usually associated with large optical flares in H-alpha (≥ 2B) and long duration type II and IV, microwave and hard X-ray bursts. The results obtained in the present analysis may be used for the prediction of solar proton flares. | - |
dc.format.extent | 32536 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | - |
dc.publisher | Indian Institute of Astrophysics, Bangalore | en |
dc.subject | Solar flares | en |
dc.title | Possibility of occurrence of solar proton flares in relation to other phenomena | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 ) |
Files in This Item:
File | Description | Size | Format | |
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Possibility of occurrence of solar proton flares in relation to other phenomena.pdf | 31.77 kB | Adobe PDF | View/Open |
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