Fine structure in solar microwave bursts

Details Fine structure in solar microwave bursts Fine structure in solar microwave bursts

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130..183a&link_type=abstract

(Committee of European Radio Astronomers, SNSF, URSI, et al., Workshop on Particle Beams in the Solar Atmosphere, Braunwald, Swi

Physics

47

Circular Polarization, Fine Structure, Microwave Emission, Solar Radio Bursts, Microwave Interferometers, Microwave Spectra, Temporal Resolution

Scientific paper

A new multichannel radio spectrograph has been constructed for the study of short-lived structures in solar microwave bursts. It measured the integrated flux over the whole solar disk in two circular polarizations at 36 frequencies between 4 and 8 GHz, with a time constant of 0.5 ms. All 119 recorded bursts observed in 1981 and 1983 are analyzed. Attention is focused on events with a lifetime of less than 1 s.

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