dc.contributor.author |
Ramesh, R |
|
dc.contributor.author |
Satya Narayanan, A |
|
dc.contributor.author |
Kathiravan, C |
|
dc.contributor.author |
Sastry, Ch. V |
|
dc.contributor.author |
Shankar, N. U |
|
dc.date.accessioned |
2008-09-11T16:10:28Z |
|
dc.date.available |
2008-09-11T16:10:28Z |
|
dc.date.issued |
2005-02 |
|
dc.identifier.citation |
Astronomy and Astrophysics, Vol. 431, No. 1, pp. 353 - 357 |
en |
dc.identifier.issn |
0004-6361 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3554 |
|
dc.description.abstract |
We report radio observations of quasi-periodic type III burst emission from the solar corona in close association with the 2B/X2.8 flare of December 11, 2001 at two frequencies (151.5 and 109 MHz). The measured mean period was ≈11.6 s. We attempted to infer the plasma parameters of the region where the electron beams responsible for the observed type III emission were accelerated/injected using our data, and the values are the following: the Alfvén speed (v/sub A) = 873± 427 km s-1; the electron density (N/sube) ≈ 3.09 × 10/subp9 cm/sub-3; the magnetic field strength (B) = 22 ± 11 G. |
en |
dc.language.iso |
en |
en |
dc.publisher |
EDP Sciences |
en |
dc.relation.uri |
http://dx.doi.org/10.1051/0004-6361:20041130 |
en |
dc.subject |
Sun: activity |
en |
dc.subject |
Sun: flares |
en |
dc.subject |
Sun: oscillations |
en |
dc.subject |
Sun: radio radiation |
en |
dc.title |
An estimation of the plasma parameters in the solar corona using quasi-periodic metric type III radio burst emission |
en |
dc.type |
Article |
en |