Introduction of the solar broadband microwave spectrometer.

Details Introduction of the solar broadband microwave spectrometer. Introduction of the solar broadband microwave spectrometer.

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arbes...4...26l&link_type=abstract

Astrophysics Reports, Special Issue, No. 4, p. 26 - 32

Astronomy and Astrophysics

Astrophysics

Spectrometers: Solar Flares, Spectrometers: Solar Microwave Radiation

Scientific paper

The solar radio spectrometers in 1.0 - 2.0 GHz and 2.6 - 3.8 GHz which are working and the 5.2 - 7.6 GHz spectrometer which will come into operation in 1999, are introduced. 171 and 146 bursts in 1.0 - 2.0 GHz and 2.6 - 3.8 GHz, respectively, with a wealth of fine structures in time and frequency in different types has been registered. The solar radio bursts at different frequencies reflect the evolving processes of solar flares in time and height, and provide much basis for the research on solar flares.

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