On fast pulsations in flare continua

Details On fast pulsations in flare continua On fast pulsations in flare continua

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..104...43e&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

15

Continuous Spectra, Emission Spectra, Radio Spectra, Solar Flares, Solar Oscillations, Fine Structure, Power Spectra, Spectroheliographs, Temporal Distribution, Type 4 Bursts

Scientific paper

Pulsations with periods down to 0.05 s have been observed in continuum emission following flares. In pulsating events several frequencies may be excited, simultaneously or in time succession. Pulsations occur both in classical type IV events and in short-lasting continuum events. The power spectrum shows no large variation during one or two hours. Some implications of fast pulsations for the generation mechanism are discussed.

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