| dc.contributor.author | Joshi, G. C. | |
| dc.contributor.author | Punetha, L. M. | |
| dc.contributor.author | Pande, M. C. | |
| dc.date.accessioned | 2011-09-16T05:40:41Z | |
| dc.date.available | 2011-09-16T05:40:41Z | |
| dc.date.issued | 1979 | |
| dc.identifier.citation | This article has been taken out from ADS | en_US |
| dc.identifier.uri | http://hdl.handle.net/123456789/836 | |
| dc.description.abstract | The calculated equivalents widths of some lines of SiO in the umbral spectrum suggest that strong lines of Si²⁸ O¹⁶ , Si²⁹ O¹⁶ , and Si³⁰ O¹⁶, may be present in the sunspot ultraviolet spectrum. We also find that between 37000 and 47000 cm ¯¹, the quasi-continuous absorption of SiO dominates all other absorptions. | en_US |
| dc.language.iso | en_US | en_US |
| dc.relation.ispartofseries | sp62-77 | |
| dc.subject | Sunspots, SiO lines | en_US |
| dc.title | (A-X) system of SiO in sunspots | en_US |
| dc.type | Article | en_US |