dc.contributor.author |
Ramesh, R |
|
dc.date.accessioned |
2008-08-14T11:24:14Z |
|
dc.date.available |
2008-08-14T11:24:14Z |
|
dc.date.issued |
2000-09 |
|
dc.identifier.citation |
Solar Physics, Vol. 196, No. 1, pp. 213 - 220 |
en |
dc.identifier.issn |
0038-0938 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3146 |
|
dc.description.abstract |
We report low-frequency observations of an enhancement in the solar corona prior to the halo coronal mass ejection of 23 October 1997, with the Gauribidanur radioheliograph. The Sun was `quiet' and no radio bursts were observed either prior to or in the aftermath of the event. The radio method would be useful in studying the pre-event structures associated with the eruptive solar activity, particularly from the ground. |
en |
dc.format.extent |
98521 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://www.springerlink.com/content/k57018776036jv55/ |
en |
dc.subject |
Low-Frequency Observations |
en |
dc.subject |
Solar Corona |
en |
dc.subject |
Halo Coronal Mass Ejection |
en |
dc.subject |
Radio Bursts |
en |
dc.subject |
Solar Activity |
en |
dc.title |
The Halo CME Event Of 23 October 1997 - Low-Frequency Radio Observations Of The Pre-Event Corona |
en |
dc.type |
Article |
en |