Temporary decrease in the normal solar radio intensity level and its association with an impulsive burst

Details Temporary decrease in the normal solar radio intensity level and its association with an impulsive burst Temporary decrease in the normal solar radio intensity level and its association with an impulsive burst

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975erp..rept.....p&link_type=abstract

Environmental Research Papers Air Force Cambridge Research Labs., Hanscom AFB, MA.

Physics

Radio Attenuation, Solar Flares, Solar Radio Bursts, Solar Radio Emission, Kirchhoff Law Of Radiation, Models, Plasma Turbulence, Solar Flux Density

Scientific paper

Solar radio phenomena designated as post-burst decreases, absorptions, and negative-burst events are extremely rare and seem to be the only evidence of temporary decreases in the sun's radio emission. The presence of optically identified material in the flare/burst region is merely an association and not the cause of the observed radio decreases as has been suggested by earlier investigators. A theoretical model for the decreases is presented which invokes plasma turbulence effects of an electron beam in the radio-emissive region with absorption effects taking place in accordance with Kirchoff's law.

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