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RHESSI and Microwave Imaging Observations of Two Solar Flares

Published online by Cambridge University Press:  14 March 2005

M.R. Kundu ,
E.J. Schmahl  and
V.I. Garaimov
M.R. Kundu
Affiliation:
Astronomy Department, University of Maryland, College Park, MD 20742
E.J. Schmahl
Affiliation:
Astronomy Department, University of Maryland, College Park, MD 20742 Lab for Astronomy and Solar Physics, NASA/GSFC, Greenbelt, MD 20771
V.I. Garaimov
Affiliation:
Astronomy Department, University of Maryland, College Park, MD 20742
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Abstract

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We describe two flares of GOES class M5.7 and 1.5 which were observed simultaneously by RHESSI (Ramaty High Energy Solar Spectroscopic Imager) and NoRH (Nobeyama Radio Heliograph). Both flares exhibit slow motions suggestive of changing magnetic shear, loop expansion, or gradual reconnection. One flare is clearly a coronal hard X-ray and microwave flare.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS223 , June 2004 , pp. 425 - 428
Copyright
© 2004 International Astronomical Union