Low frequency (< 100 MHz) thermal radio emission from the solar corona and the effect of radial magnetic field

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/578

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2005-08-27T08:20:56Z	-
dc.date.available	2005-08-27T08:20:56Z	-
dc.date.issued	2005-12	-
dc.identifier.citation	K. Sankarasubramanian, M. Penn, and A. Pevtsov., eds., Large-scale Structures and their Role in Solar Activity ASP Conference Series, Vol. 346, Proceedings of the Conference held 18 - 22 October, 2004 in Sunspot, New Mexico, USA.	en
dc.identifier.uri	http://hdl.handle.net/2248/578	-
dc.description.abstract	We measured the degree of circular polarization of the thermal radiation from discrete structures in the solar corona at a frequency of 77 MHz and attempted to derive the magnetic field strength of these regions.	en
dc.format.extent	139097 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.ispartofseries	ASP Conference Series, Vol. 346	-
dc.relation.uri	http://adsabs.harvard.edu/abs/2005ASPC..346..153R	-
dc.subject	Thermal Radio Emission	en
dc.subject	Solar Corona	-
dc.subject	Radial Magnetic Field	-
dc.title	Low frequency (< 100 MHz) thermal radio emission from the solar corona and the effect of radial magnetic field	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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