dc.contributor.author |
Subramanian, K. R |
|
dc.contributor.author |
Ebenezer, E |
|
dc.date.accessioned |
2008-09-15T10:27:46Z |
|
dc.date.available |
2008-09-15T10:27:46Z |
|
dc.date.issued |
2003-12 |
|
dc.identifier.citation |
Solar Physics, Vol. 218, No. 1, pp. 221 - 226 |
en |
dc.identifier.issn |
0038-0938 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3603 |
|
dc.description |
Restricted Access |
en |
dc.description |
The original publication is available at springerlink.com |
en |
dc.description.abstract |
Quasi-periodic pulsations with periods mostly around 13 s in the frequency range of 54-78 MHz have been observed following the first X2 flare occurring on 24 November 2000. Assuming an impulsively generated propagating MHD wave in a coronal loop for the pulsations, the coronal magnetic field at 1.6 Rsolar is derived as ~6 G and the radius of cross section of the loop as ~13000 km. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Springer |
en |
dc.relation.uri |
http://www.springerlink.com/content/n541x4k3v6541141/ |
en |
dc.subject |
Coronal loop oscillations |
en |
dc.subject |
Solar corona |
en |
dc.title |
Post-flare pulsations in the 54–78 MHz frequency band |
en |
dc.type |
Article |
en |