dc.contributor.author |
Sinha, K. |
|
dc.contributor.author |
Tripathi, B. M. |
|
dc.contributor.author |
Atalla, R. M. |
|
dc.contributor.author |
Singh, P. D. |
|
dc.date.accessioned |
2010-02-15T04:49:48Z |
|
dc.date.available |
2010-02-15T04:49:48Z |
|
dc.date.issued |
1988 |
|
dc.identifier.citation |
This article downloded from ADS Free Online Journal |
en_US |
dc.identifier.uri |
http://hdl.handle.net/123456789/505 |
|
dc.description.abstract |
Equivalent width calculations for some electronic and vibration-rotation transitions of the molecules PO, PH, MgH⁺, and CN have been carried out for a few umbral, photospheric, and facular model atmospheres. It appears that a few weak lines of these molecules might show up in the umbral spectrum. Le Blanc bands of CN are too weak for detection in the solar spectrum. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
sp115-221 |
|
dc.subject |
Faint molecules lines - PO, PH, MgH⁺ and CN |
en_US |
dc.title |
On the possibility of faint molecular lines of PO, PH, MgH⁺, and CN in the solar spectrum |
en_US |
dc.type |
Article |
en_US |