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/2289/1110

Full metadata record

DC Field	Value	Language
dc.contributor.author	Subramanian, K.R.	-
dc.contributor.author	Sastry, Ch.V.	-
dc.date.accessioned	2006-01-06T05:53:06Z	-
dc.date.available	2006-01-06T05:53:06Z	-
dc.date.issued	1988	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1988, Vol. 9, p 225-229.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/1110	-
dc.description.abstract	The low-frequency radio spectrum of the continuum emission from the undisturbed sun is determined for 24 days during the period May-September 1985. 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.format.extent	484957 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	Sun	en
dc.subject	Low-frequency radio observation	en
dc.subject	Sun, Corona	en
dc.title	The low-frequency radio spectrum of the continuum emission from the undisturbed Sun	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

Files in This Item:

File	Description	Size	Format
1988_JAA_V9_p225-229.pdf	5p.	473.59 kB	Adobe PDF	View/Open