Author： Subramanian Prasad Ananthakrishnan S. Janardhan P. Kundu M.R. White S.M. Garaimov V.I.
Publisher： Springer Publishing Company
ISSN： 0038-0938
Source： Solar Physics, Vol.218, Iss.1-2, 2003-12, pp. : 247-259
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
We present the first observations of a solar flare with the GMRT. An M2.8 flare observed at 1060 MHz with the GMRT on 17 November 2001 was associated with a prominence eruption observed at 17 GHz by the Nobeyama radioheliograph and the initiation of a fast partial halo CME observed with the LASCO C2 coronagraph. Towards the start of the eruption, we find evidence for reconnection above the prominence. Subsequently, we find evidence for rapid growth of a vertical current sheet below the erupting arcade, which is accompanied by the flare and prominence eruption.
Related content
Access to resources
Recommend
Eit and LASCO Observations of the Initiation of a Coronal Mass Ejection
By Dere K. Brueckner G. Howard R. Koomen M. Korendyke C. Kreplin R. Michels D. Moses J. Moulton N. Socker D. St. Cyr O. Delaboudinière J. Artzner G. Brunaud J. Gabriel A. Hochedez J. Millier F. Song X. Chauvineau J. Marioge J. Defise J. Jamar C. Rochus P. Catura R. Lemen J. Gurman J. Neupert W. Clette F. Cugnon P. Van Dessel E. Lamy P. Llebaria A. Schwenn R. Simnett G.
Solar Physics, Vol. 175, Iss. 2, 1997-10 ,pp. :