The low-frequency radio spectrum of the continuum emission from the undisturbed sun

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3666

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DC Field	Value	Language
dc.contributor.author	Subramanian, K. R	-
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2008-09-16T15:48:35Z	-
dc.date.available	2008-09-16T15:48:35Z	-
dc.date.issued	1988-12	-
dc.identifier.citation	Journal of Astrophysics and Astronomy , Vol. 9, No. 4, pp. 225 - 229	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2248/3666	-
dc.description.abstract	The low-frequency radio spectrum of the continuum emission from the undisturbed Sun is determined for 24 days during the period 1985 May - September. It is found that the spectral index varied from +1.6 to +3.6 during this period. It is suggested that the large positive spectral indices are due to the existence of temperature gradients in the outer corona.	en
dc.language.iso	en	en
dc.publisher	Indian Academy Sciences	en
dc.relation.uri	http://ads.ari.uni-heidelberg.de/abs/1988JApA....9..225S	en
dc.subject	Continuous Spectra	en
dc.subject	Radio Spectra	en
dc.subject	Solar Corona	en
dc.subject	Solar Radio Emission	en
dc.subject	Solar Spectra	en
dc.subject	Emission Spectra	en
dc.subject	Low Frequencies	en
dc.subject	Spectrum Analysis	en
dc.subject	Temperature Distribution	en
dc.title	The low-frequency radio spectrum of the continuum emission from the undisturbed sun	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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