Solar type I radio bursts - Shock model

Details Solar type I radio bursts - Shock model Solar type I radio bursts - Shock model

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...100...20w&link_type=abstract

Astronomy and Astrophysics, vol. 100, no. 1, July 1981, p. 20-23. NSF-supported research.

Astronomy and Astrophysics

Astronomy

19

Electric Current, Plasma Radiation, Plasma Waves, Shock Waves, Solar Corona, Solar Radio Bursts, Brightness Temperature, Radio Astronomy

Scientific paper

The brief intense emission of type I bursts is taken to be evidence for localized strong electrical currents in the corona. The radiation mechanism is considered to be the combination of upper-hybrid and lower-hybrid waves. The upper-hybrid waves, driven by the loss-cone of trapped fast electrons, are highly directional and can yield the observed high brightness temperature. The lower-hybrid waves provide a high radiative opacity and are most probably generated by shocks.

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