Observations and interpretation of solar flares at microwave frequencies

Details Observations and interpretation of solar flares at microwave frequencies Observations and interpretation of solar flares at microwave frequencies

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..118..155c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 118, no. 1-2, 1988, p. 155-183.

Astronomy and Astrophysics

Astronomy

19

Microwave Emission, Solar Flares, Solar Physics, Solar X-Rays, Cyclotron Radiation, H Alpha Line, Japan, Microwave Frequencies, Radio Astronomy, Solar Cycles

Scientific paper

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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