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

Title:	Low frequency (< 100 MHz) thermal radio emission from the solar corona and the effect of radial magnetic field
Authors:	Ramesh, R Sastry, Ch. V
Keywords:	Thermal Radio Emission Solar Corona Radial Magnetic Field
Issue Date:	Dec-2005
Publisher:	Astronomical Society of the Pacific
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.
Series/Report no.:	ASP Conference Series, Vol. 346
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.
URI:	http://hdl.handle.net/2248/578
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Low frequency thermal radio emission		279.14 kB	Adobe PDF	View/Open

DSpace JSPUI