Observations and interpretation of solar flares at microwave frequencies |
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| Authors: | C J Crannell G A Dulk T Kosugi A Magun |
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| Institution: | (1) Laboratory for Astronomy and Solar Physics, NASA/Goddard Space Flight Center, 20771 Greenbelt, MD, U.S.A.;(2) Department of Astrophysical, Planetary and Atmospheric Sciences, University of Colorado, CB 391, 80309 Boulder, CO, U.S.A.;(3) Tokyo Astronomical Observatory, Mitaka, 181 Tokyo, Japan;(4) Institute for Applied Physics, University of Bern, CH-3012 Bern, Switzerland |
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| Abstract: | The physical processes responsible for microwave emission in solar flares are outlined, and examples of how microwave observations have been interpreted in terms of physical parameters are described. Selected results obtained during Solar Cycle 21 with the microwave observatories dedicated to synoptic observations of the Sun are summarized. The status and future plans for these facilities at Bern and in Japan are presented. Also discussed are the instrument capabilities required at microwave frequencies to achieve the objectives of a future facility for high-energy solar physics. |
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