No CrossRef data available.
Article contents
Low Frequency (30-110 MHz) Radio Imaging Observations Of Solar Coronal Mass Ejections
Published online by Cambridge University Press: 03 June 2005
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
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
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 83 - 94
- Copyright
- © 2005 International Astronomical Union
You have
Access