The Madurai solar radio spectrograph

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3372

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DC Field	Value	Language
dc.contributor.author	Shanmugaraju, A	-
dc.contributor.author	Umapathy, S	-
dc.date.accessioned	2008-09-04T17:28:09Z	-
dc.date.available	2008-09-04T17:28:09Z	-
dc.date.issued	1998	-
dc.identifier.citation	BASI, Vol. 26, pp. 305 - 310	en
dc.identifier.uri	http://hdl.handle.net/2248/3372	-
dc.description.abstract	The solar radio spectrograph has been constructed at our School of Physics to study the dynamic activities of the sun in metre wavelenght which is quite important for understanding the physics of the outer solar corona. In this paper, the salient features of the spcetrograph are highlighted and the current observations programmes and some of the observational results are described. The desirable improvements in the spectrograph before the next solar maximum and some of the theoretical aspects in connection with the coronal events attempted are summarised at the end.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1998BASI...26..305S	en
dc.subject	Radio spectrograph	en
dc.subject	Coronal emissions	en
dc.subject	Observations	en
dc.title	The Madurai solar radio spectrograph	en
dc.type	Article	en
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