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http://hdl.handle.net/2248/841
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DC Field | Value | Language |
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dc.contributor.author | Nirupama, Raghavan | - |
dc.date.accessioned | 2006-04-06T10:19:44Z | - |
dc.date.available | 2006-04-06T10:19:44Z | - |
dc.date.issued | 1968-09 | - |
dc.identifier.citation | KOB No 186 | en |
dc.identifier.uri | http://hdl.handle.net/2248/841 | - |
dc.description.abstract | Thirteen molecular lines of CN, C/sub2/ and CH have been photoelectrically observed at six disc positions each. The observed trends fall into two categories; one for strong lines and another for weak lines, irrespective of the molecule of their origin. Detailed profile calculations have been made for six selected lines. LTE methodology and an anisotropic model of turbulence have been assumed. | en |
dc.format.extent | 720352 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Kodaikanal Observatory | en |
dc.subject | Carbon Molecules | en |
dc.subject | Molecular Lines | en |
dc.title | Line Profile Analysis of Carbon Molecules in the Sun | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Raghavan.pdf | 703.47 kB | Adobe PDF | View/Open |
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