Observations of radio continua and terminology

Details Observations of radio continua and terminology Observations of radio continua and terminology

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104...19p&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

21

Continuous Spectra, Radio Spectra, Solar Flares, Type 4 Bursts, Centimeter Waves, Decametric Waves, Particle Acceleration, Polarization Characteristics, Temporal Distribution, Terminology

Scientific paper

Different components and successive stages of type IV bursts are discussed, and modifications to the schematic representation of well developed type IV bursts are proposed. It is shown that different components do not necessarily correspond to different electron populations. Consideration is given to the possible existence of two physically distinct acceleration mechanisms and it is noted that there may be one corresponding to an injection/acceleration site located relatively low in the corona producing electrons continuously or repetitively throughout the event's development while there may be another one corresponding to in situ acceleration during shock wave passage.

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