Post-flare pulsations in the 54–78 MHz frequency band

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3603

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DC Field	Value	Language
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
Appears in Collections:	IIAP Publications

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