Polarization of the thermal radio emission from outer solar corona

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4817

Full metadata record

DC Field	Value	Language
dc.contributor.author	Sastry, Ch. V	-
dc.date.accessioned	2009-09-11T16:52:00Z	-
dc.date.available	2009-09-11T16:52:00Z	-
dc.date.issued	2009-06	-
dc.identifier.citation	The Astrophysical Journal, Vol. 697, No. 2, pp. 1934 - 1939	en
dc.identifier.issn	0004-637X	-
dc.identifier.uri	http://hdl.handle.net/2248/4817	-
dc.description	Open Access	-
dc.description.abstract	The Haselgrove equations for radio-ray propagation in an anisotropic medium are used to determine the degree of circular polarization (dcp) of the low-frequency thermal radio emission from the outer solar corona with a magnetic field. The variation of dcp with frequency and magnetic field strength is investigated. It is found that weak magnetic fields can be detected by measuring the dcp at low frequencies.	en
dc.language.iso	en	en
dc.publisher	The American Astronomical Society	en
dc.relation.uri	http://dx.doi.org/10.1088/0004-637X/697/2/1934	en
dc.rights	© The American Astronomical Society	en
dc.subject	Sun: Activity	en
dc.subject	Sun: Corona	en
dc.subject	Sun: Magnetic Fields	en
dc.subject	Sun: Radio Radiation	en
dc.title	Polarization of the thermal radio emission from outer solar corona	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Polarization of the thermal radio emission	Open Access	157.77 kB	Adobe PDF	View/Open

DSpace JSPUI