Progress of solar radio microwave bursts and fine structures

Details Progress of solar radio microwave bursts and fine structures Progress of solar radio microwave bursts and fine structures

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pabei..23..331l&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 23, No. 4, p. 331 - 345 (2005)

Astronomy and Astrophysics

Astrophysics

Astrophysics, Microwave Burst, Review, Solar Flare, Emission Mechanism

Scientific paper

The complicated radio spectrum detected in solar radio bursts contain a lot of important information on their source regions including physical environment and emission mechanisms. The emission of the microwave bursts is in higher frequency range (GHz) and often came from the magnetic reconnection region in lower corona. Especially, because of their morphologic features of short duration, rapid frequency drift, complicated types and so on, the microwave fine structures could bring out rich information on the source regions such as the complicated configuration of magnetic reconnection, the movement of energetic particle, etc. In this paper, three main stages of researches on the solar microwave bursts and the fine structures are reviewed. The main burst types, the mechanism researches and the observational instrument for each stage are summarized. The future proposals are discussed as well.

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