VLA observations of angular broadening close to the sun

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1585

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DC Field	Value	Language
dc.contributor.author	Gothoskar, Pradeep	-
dc.contributor.author	Anantharamaiah, K.R.	-
dc.contributor.author	Desai, Ketan	-
dc.contributor.author	Rao, A.P.	-
dc.date.accessioned	2006-12-14T10:38:36Z	-
dc.date.available	2006-12-14T10:38:36Z	-
dc.date.issued	2001	-
dc.identifier.citation	Astrophysics and Space Science, 2001, Vol.278, p193-196	en
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://hdl.handle.net/2289/1585	-
dc.description	Restricted Access.	en
dc.description.abstract	We present synthesis imaging of scatter-broadening of radio sources carried out using the Very Large Array (VLA) at six radio frequencies during the period of solar minimum. Three compact radio sources were observed from 2 to 16 solar radii around the sun. The data indicate highly anisotropic scattering. The scatter-broadening was estimated from the area of the scattered image and was found to be factor of two lower and orientation of magnetic fields was closer to the radial direction. Present observations confirm the variation of scatter-broadening with solar elongation.	en
dc.format.extent	8338 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2001Ap&SS.278..193G	en
dc.relation.uri	http://dx.doi.org/10.1023/A:1013110930964	en
dc.rights	(2001) Kluwer Academic Publishers.	en
dc.title	VLA observations of angular broadening close to the sun	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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