Physics
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..128..399b&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 128, Aug. 1990, p. 399-414.
Physics
Noise Storms, Polarized Electromagnetic Radiation, Radio Spectra, Solar Spectra, Solar Storms, Continuous Spectra, Solar Radio Emission, Type 3 Bursts
Scientific paper
Based on single-frequency records from the Tremsdorf Observatory, a method to discriminate type I and type III continua from polarization measurements was derived. Intense 40 MHz continua identified by spectral criteria as a type III continuum are more weakly polarized than type I continua. The increase in the number of intense continua at frequencies not above 64 MHz during the second, compared to the first, activity maximum of cycle No. 20 was due to an enhanced number of continua with a significant contribution of type I continuum. Relations between the parameters of the continua and the concurrent storm bursts confirm the validity of the above-mentioned ideas and may be useful to test models which try to explain the generation of type I and type III storms under common aspects.
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