The simplest solar microbursts flux and circular polarization at 22 GHz

Details The simplest solar microbursts flux and circular polarization at 22 GHz The simplest solar microbursts flux and circular polarization at 22 GHz

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...95..155k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 95, Jan. 1985, p. 155-165. Research supported by the Financiadora de Estudos e Projetos of

Physics

9

Circular Polarization, Microwave Emission, Solar Flux, Solar Radio Bursts, Cassegrain Antennas, Flux Quantization, Time Response

Scientific paper

The simplest solar microwave microbursts detected with high sensitivity may be the response to the simpler energetic burst injections. Seventeen events from this category were identified in a series of more than 150 bursts recorded in 21-26 November, 1982. This first systematic study suggests that microbursts e-folding rise times concentrate into two classes of time scales, t greater than 0.05 s and much less than 1 s and t greater than about 0.05 s and less than about 2 s. Microbursts' circular polarization presents a dominant steady or slowly varying component that sets in before maximum emission. In some cases a faster component of polarization was found superimposed, which is not always well correlated in time with flux.

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