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

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8417104k&link_type=abstract

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Computer Science

Circular Polarization, Microwave Emission, Polarized Electromagnetic Radiation, Solar Activity, Solar Radio Bursts, Flux (Rate), Radio Telescopes

Scientific paper

The simplest solar microwave microbursts detected with high sensitivity may be the response to the simpler energetic injection. This systematic study suggests two classes of microbursts: microimpulsive (e-folding rise times 0.05s t 1s) and microgradual (0.5s t approx. 2s). 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 and in general is not correlated in time with flux.

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