Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2416
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dc.contributor.authorSastry, Ch.V.-
dc.contributor.authorShevgaonkar, R.K.-
dc.contributor.authorRamanuja, M.N.-
dc.date.accessioned2007-05-25T08:32:55Z-
dc.date.available2007-05-25T08:32:55Z-
dc.date.issued1983-09-
dc.identifier.citationSolar Physics, 1983, Vol.87, p391-399en
dc.identifier.issn0038-0938-
dc.identifier.issn1573-093X (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/2416-
dc.descriptionOpen Access.en
dc.description.abstractTwo-dimensional maps have been made of the slowly varying component (SVC) of solar radio emission at a frequency of 34.5 MHz, with half-power beam width of 26/40 arcmin. It is found that a majority of SVC sources have brightness temperatures of the order of 500.000 K, and half-power widths of about 4 solar radii. The shifts in the positions of the centroids of the SVC sources from the center of the sun were in the range 1.5 to 2 solar radii. These observations can be explained in terms of thermal emission from coronal regions of enhanced density and temperature located at distances of 1.5 to 2 solar radii from the center of the sun.en
dc.format.extent728897 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1983SoPh...87..391Sen
dc.relation.urihttp://dx.doi.org/10.1007/BF00224848en
dc.rights1983 Springeren
dc.subjectBRIGHTNESS TEMPERATUREen
dc.subjectDECAMETRIC WAVESen
dc.subjectSOLAR CORONAen
dc.subjectSOLAR RADIO EMISSIONen
dc.subjectTHERMAL EMISSIONen
dc.subjectRADIAL DISTRIBUTIONen
dc.subjectTEMPERATURE DISTRIBUTIONen
dc.titleObservations on the slowly varying component of solar radio emission at decameter wavelengthsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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