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Low Frequency (30-110 MHz) Radio Imaging Observations Of Solar Coronal Mass Ejections

Published online by Cambridge University Press:  03 June 2005

R. Ramesh
R. Ramesh
Affiliation:
Centre for Research and Education in Science and Technology, Indian Institute of Astrophysics, Hosakote 562 114, Bangalore, INDIA email: [email protected]
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Abstract

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Ground based radio imaging observations play an useful role in the study of mass ejections from the solar corona since they do not have the limitation of an occulter and both the disk/limb events can be detected early in their development, particularly via the thermal bremmstrahlung emission from the frontal loop of the CME. I present here some of the recent results on the above topic using data obtained with the Gauribidanur radioheliograph, near Bangalore in India.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: generalSun: coronaSun: coronal mass ejections (CMEs)Sun: radio radiation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 83 - 94
Copyright
© 2005 International Astronomical Union