Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/639Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Punetha, L. M | - |
| dc.contributor.author | Joshi, G. C | - |
| dc.date.accessioned | 2005-12-07T05:32:02Z | - |
| dc.date.available | 2005-12-07T05:32:02Z | - |
| dc.date.issued | 1984-12 | - |
| dc.identifier.citation | BASI, Vol. 12, No. 4, pp. 393-397 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/639 | - |
| dc.description.abstract | The Doppler widths of 0-1, 1-2 and 2-3 vibrational bands of the violet system of CN molecule in the solar atmosphere increase linearly with equivalent width upto approximately equal to 20 mA | en |
| dc.format.extent | 358193 bytes | - |
| dc.format.mimetype | application/pdf | - |
| dc.language.iso | en | - |
| dc.publisher | Astronomical Society of India | en |
| dc.subject | CN molecule | en |
| dc.subject | Doppler width | en |
| dc.subject | The Sun | en |
| dc.title | Doppler width of CN lines in the Sun | en |
| dc.type | Article | en |
| Appears in Collections: | BASI Publications | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| PUNETHA.pdf | 349.8 kB | Adobe PDF | ![]() View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.
