Rotational Effects on line Source Function

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/374

Full metadata record

DC Field	Value	Language
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	-
dc.format.mimetype	application/pdf	-
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
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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