Estimation of magnetic field in the solar coronal streamers through low frequency radio observations

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5057

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DC Field	Value	Language
dc.contributor.author	Ramesh, R	-
dc.contributor.author	Kathiravan, C	-
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2010-03-08T14:23:20Z	-
dc.date.available	2010-03-08T14:23:20Z	-
dc.date.issued	2010-03	-
dc.identifier.citation	The Astrophysical Journal, Vol. 711, No. 2, pp. 1029 – 1032	en
dc.identifier.issn	0004-637X	-
dc.identifier.uri	http://hdl.handle.net/2248/5057	-
dc.description	Open Access	en
dc.description.abstract	The observations of circularly polarized thermal radio emission from solar coronal streamers at two low frequencies, viz., 77 and 109 MHz, are used to estimate the magnetic field strength (B) at their corresponding radial distances r≈ 1.7 and 1.5 solar radii given by the electron density model of Newkirk. The estimated values of B at the above two distances are ≈5 ± 1 G and 6 ± 2 G, respectively.	en
dc.language.iso	en	en
dc.publisher	Institute of Physics	en
dc.relation.uri	http://www.iop.org/EJ/abstract/0004-637X/711/2/1029	en
dc.rights	© Institute of Physics	en
dc.subject	Sun: Activity	en
dc.subject	Sun: Corona	en
dc.subject	Sun: Magnetic Topology	en
dc.subject	Sun: Radio Radiation	en
dc.title	Estimation of magnetic field in the solar coronal streamers through low frequency radio observations	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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