Behaviour of the polarization at dm-m wavelengths during the evolution of five two-ribbon flares

Details Behaviour of the polarization at dm-m wavelengths during the evolution of five two-ribbon flares Behaviour of the polarization at dm-m wavelengths during the evolution of five two-ribbon flares

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104..169r&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

6

Circular Polarization, Decimeter Waves, H Alpha Line, Solar Flares, Flux Density, Radio Spectra, Solar Magnetic Field, Temporal Distribution, X Ray Spectra

Scientific paper

The general behaviour of the circular polarization at dm - m wavelengths during the evolution of five two-ribbon flares is investigated. The changes of polarization, if present, occurred 10 to 20 min after the impulsive phases. Increases of the radio and X-ray fluxes occurred at the moments when the Hα ribbons started to extend over spot umbrae.

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