Some statistics of solar radio bursts of spectral types II and IV

Details Some statistics of solar radio bursts of spectral types II and IV Some statistics of solar radio bursts of spectral types II and IV

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...325..901c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 325, Feb. 15, 1988, p. 901-904.

Astronomy and Astrophysics

Astrophysics

17

Radio Waves, Solar Radio Bursts, Solar Spectra, Solar X-Rays, Type 2 Bursts, Type 4 Bursts, H Alpha Line, Particle Acceleration, Solar Flares, Solar Radiation, Statistical Analysis

Scientific paper

The properties of meter wavelength solar emissions are studied using a sample of all type II and type IV radio bursts detected by the Culgoora radio observatory during 1968-1983. It is found that type IV emission generally occurs in conjunction with type II emission. For type III bursts preceding type II bursts, the delay to type II onset is 6.5 min on average. The intensities and durations of type II bursts are not dependent on the heliolongitude of the associated flares.

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