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VLA observations of angular broadening close to the sun

dc.contributor.authorGothoskar, Pradeep
dc.contributor.authorAnantharamaiah, K R
dc.contributor.authorDesai, Ketan
dc.contributor.authorRao, A P
dc.date.accessioned2006-12-14T10:38:36Z
dc.date.available2006-12-14T10:38:36Z
dc.date.issued2001
dc.descriptionRestricted Access.en
dc.description.abstractWe 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.extent8338 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationAstrophysics and Space Science, 2001, Vol.278, p193-196en
dc.identifier.issn0004-640X
dc.identifier.urihttp://hdl.handle.net/2289/1585
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2001Ap&SS.278..193Gen
dc.relation.urihttp://dx.doi.org/10.1023/A:1013110930964en
dc.rights(2001) Kluwer Academic Publishers.en
dc.titleVLA observations of angular broadening close to the sunen
dc.typeArticleen

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