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http://hdl.handle.net/2248/237
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DC Field | Value | Language |
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dc.contributor.author | Singh, J | - |
dc.contributor.author | Cowsik, R | - |
dc.contributor.author | Venkatakrishnan, P | - |
dc.contributor.author | Srinivasan, R | - |
dc.contributor.author | Chinnappan, V | - |
dc.contributor.author | Raju, K. P | - |
dc.contributor.author | Srikanth, R | - |
dc.date.accessioned | 2005-01-17T10:41:49Z | - |
dc.date.available | 2005-01-17T10:41:49Z | - |
dc.date.issued | 1997 | - |
dc.identifier.citation | Kodaikanal Observatory Bulletins Series A, Vol. 13, pp. 37-39 | en |
dc.identifier.issn | 0374-3632 | - |
dc.identifier.uri | http://hdl.handle.net/2248/237 | - |
dc.description.abstract | To investigate the spatial variation of tempereture and density within coronal strucures, narrow band photometry in three coronal emission lines was done during this eclipse. The emission lines 6374 (FeX), 7892 (Fe XI) and 5303 Armstrong (Fe XIV) represented temperatures in the Armstrong range of 1-2 million degrees. Peltier cooled CCD camera was used to record the coronal images thorugh 5 Armstrong interference filters with pixel resolution of 11 arcsec. | en |
dc.format.extent | 53112 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | - |
dc.publisher | Indian Institute of Astrophysics, Bangalore | en |
dc.subject | Narrow band photometry | en |
dc.subject | Emission lines | en |
dc.subject | Electron density | en |
dc.subject | Coronal structure | en |
dc.title | Narrow Band Photometry in Emission Lines during the Total Solar Eclipse of October 24, 1995 | 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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Narrow Band Photometry in Emission Lines during the Total Solar Eclipse.pdf | 51.87 kB | Adobe PDF | View/Open |
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