Low frequency (30-110 MHz) radio imaging observations of solar coronal mass ejections

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4490

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.date.accessioned	2009-05-22T16:15:49Z	-
dc.date.available	2009-05-22T16:15:49Z	-
dc.date.issued	2005	-
dc.identifier.citation	Dere, Kenneth, Wang, Jingxiu and Yan, Yihua, Eds., Coronal and Stellar Mass Ejections., Proceedings of IAU Symposium 226th held at Beijing, China. 13 - 17 Sept 2004., pp. 83 - 94	en
dc.identifier.isbn	0-521-85197-1	-
dc.identifier.uri	http://hdl.handle.net/2248/4490	-
dc.description	Restricted Access	-
dc.description.abstract	Ground based radio imaging observations play an useful role in the study of mass ejections from the solar corona since they do not have the limitation of an occulter and both the disk/limb events can be detected early in their development, particularly via the thermal bremmstrahlung emission from the frontal loop of the CME. I present here some of the recent results on the above topic using data obtained with the Gauribidanur radioheliograph, near Bangalore in India.	en
dc.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.ispartofseries	IAU Symposium and Colloquium Proceedings Series; Vol. 226	-
dc.relation.uri	http://dx.doi.org/10.1017/S1743921305000190	en
dc.subject	Sun: General	en
dc.subject	Sun: Corona	en
dc.subject	Sun: Coronal Mass Ejections (CMEs)	en
dc.subject	Sun: Radio Radiation	en
dc.title	Low frequency (30-110 MHz) radio imaging observations of solar coronal mass ejections	en
dc.type	Article	en
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