Observations on continuum emission from the Sun at 34.5 MHz

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DC Field	Value	Language
dc.contributor.author	Sastry, Ch.V.	-
dc.date.accessioned	2007-06-08T09:45:20Z	-
dc.date.available	2007-06-08T09:45:20Z	-
dc.date.issued	1984	-
dc.identifier.citation	Proceedings of the Indo-US workshop on solar terrestrial physics, New Delhi, 1984, p187	en
dc.identifier.uri	http://hdl.handle.net/2289/2642	-
dc.description	Restricted Access.	en
dc.description.abstract	We have made two-dimensional maps of the weak continuum emission from the Sun at 34.5 MHz during periods of little or no solar burst activity using the large Decameter Wave Radio Telescope at Gauribidanur. The half- power beam widths of the radio telescope are 26' x 40'. These observations showed that the centroid of the radio emission is some- times shifted in position from the center of the Sun by 1.5 to 2.0 R e . The maximum brightness temperatures are found to be of 6 the order of 0.5 x 10 K, and the half power widths of the brightness distributions are I 4 R , . 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 Re from the center of the Sun.	en
dc.format.extent	244500 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.title	Observations on continuum emission from the Sun at 34.5 MHz	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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