dc.contributor.author |
Peraiah, A |
|
dc.contributor.author |
Raghunath, G |
|
dc.date.accessioned |
2005-03-03T06:26:27Z |
|
dc.date.available |
2005-03-03T06:26:27Z |
|
dc.date.issued |
1980 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 3, pp. 21-25 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/374 |
|
dc.description.abstract |
The effects of rotation are investigated on the source functions in an expanding atmosphere. We have considered a non-LTE two-level atom in an extended atmosphere. We have also made use of von Zeipel`s theorem in giving the incident radiation at Tou = Toumax. Uniform rotation is assumed and the values of the ratios of the centrifugal force and gravity force at the equator are taken to be 0.1, 0.4, 0.8 corresponding to a uniform rotational velocity of 1, 4 and 8 mtu. It is found that rotation will dilute the rotation field which is similar to the effects of expansion. |
en |
dc.format.extent |
102484 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Source Function |
en |
dc.subject |
Von Zeipel`s theorem |
en |
dc.title |
Rotational Effects on line Source Function |
en |
dc.type |
Article |
en |