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
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/2005ASPC..346..153R
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Low frequency thermal radio emission 279.14 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.