dc.contributor.author |
Sinha, K. |
|
dc.date.accessioned |
2010-07-27T08:34:33Z |
|
dc.date.available |
2010-07-27T08:34:33Z |
|
dc.date.issued |
1984 |
|
dc.identifier.citation |
This article downloded from ADS Free Online Journal |
en_US |
dc.identifier.uri |
http://hdl.handle.net/123456789/714 |
|
dc.description.abstract |
Utilizing the KPNO altas (Brault & Teserman 1972) for the (0-0) band of the Swan system of the C₂ molecules, we determine rotational temperatures Trot, for µ = 1.0 and µ = 0.2. When saturation in the observed equivalent widths is accounted for, the model-based result for Trot comes out slightly lower than observations at a near limb position (µ = 0.2). There is no evidence for an increase in temperature towards the solar limb discussed earlier (Sinha 1979a, b). |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
basi12-172 |
|
dc.subject |
Solar spectrum, C₂ molecules, Rotational temperature, Model atmosphere |
en_US |
dc.title |
Centre-to-limb behaviour of molecular rotational temperatures III |
en_US |
dc.type |
Article |
en_US |