dc.contributor.author |
Gopalswamy, N |
|
dc.date.accessioned |
2005-02-11T05:47:17Z |
|
dc.date.available |
2005-02-11T05:47:17Z |
|
dc.date.issued |
1986 |
|
dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol. 6, pp. 77-85 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/370 |
|
dc.description.abstract |
A brief review of the recent work done on Type-I radio emission in the Indian Institute of Astrophysics is presented. The most plausible low frequency turbulence needed to generate the type-I bursts is shown to be ion-sound turbulence. A method is presented to evaluate the coronal magnetic field using type-I radio emission data. |
en |
dc.format.extent |
322979 bytes |
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dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
|
dc.publisher |
Indian Institute of Astrophysics, Bangalore |
en |
dc.subject |
Radio Bursts |
en |
dc.subject |
Solar Radio Bursts |
en |
dc.subject |
Type-I Solar Radio Bursts |
en |
dc.title |
Type-I Solar Radio Bursts |
en |
dc.type |
Article |
en |