The characteristics of type IV-associated spikes at metric wavelengths

Details The characteristics of type IV-associated spikes at metric wavelengths The characteristics of type IV-associated spikes at metric wavelengths

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..111n&link_type=abstract

(CNR, Workshop on Radio Continua during Solar Flares, Duino, Italy, May 27-31, 1985) Solar Physics (ISSN 0038-0938), vol. 104, M

Physics

6

Polarization Characteristics, Type 4 Bursts, Fine Structure, Spikes, Temporal Distribution, Type 3 Bursts

Scientific paper

Out of 120 solar type IV events recorded at the Trieste Astronomical Observatory, 15 groups of spike bursts were selected. Their properties are analyzed with attention given to the characteristics of their polarization. It is found that the polarization of the spikes varies over a wide range, but that within a particular group of spikes it remains almost constant. Sometimes groups of spikes with different degrees of polarization occur almost contemporaneously, probably indicating that more than one source is active at nearly the same time. Occasionally spike bursts accompany type III bursts. Then, unlike the case with type IV-associated events, the polarization of the spikes varies greatly.

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