Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-11T09:35:51.704Z Has data issue: false hasContentIssue false
  • English
  • Français

Microwave and Hard X–ray Imaging of Energetic Electrons in Solar Flares: Event of 2003 June 17

Published online by Cambridge University Press:  01 November 2006

M. R. Kundu ,
E. J. Schmahl  and
S. M. White
M. R. Kundu
Affiliation:
Department of Astronomy, University of Maryland, College Park MD 20742
E. J. Schmahl
Affiliation:
Department of Astronomy, University of Maryland, College Park MD 20742 NASA Goddard Space Flight Center, Greenbelt, MD 20771
S. M. White
Affiliation:
Department of Astronomy, University of Maryland, College Park MD 20742
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We discuss a large flare that was observed simultaneously by RHESSI in hard X–rays and by the Nobeyama Radio Heliograph (NoRH) in microwaves. The imaging observations made both by RHESSI and NoRH show many interesting features which may be relevant for producing realistic flare models.

Keywords

Sun: flaresradio radiationX-raysgamma rays
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 334 - 342
Copyright
© 2006 International Astronomical Union