Relation between solar narrow-band decimetre-wave bursts and associated X-ray bursts

Details Relation between solar narrow-band decimetre-wave bursts and associated X-ray bursts Relation between solar narrow-band decimetre-wave bursts and associated X-ray bursts

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.321..421e&link_type=abstract

Nature, Volume 321, Issue 6068, pp. 421-423 (1986).

Computer Science

10

Scientific paper

Theoretical models have been proposed, stimulated by a successful account of the jovian decametric radiation1, for a maser mechanism, or a normal relativistic cyclotron resonance mechanism, operating in solar flares, and for transport of energy across magnetic fields to the electron gas by maser-amplified radio waves2. Much effort has been directed towards observations of solar-flare radio spike bursts3-8. Here we compare solar narrow-band decimetre-wave spike bursts with corresponding X-ray events for 25 solar flares. We find that decimetre spike bursts are 102-103 times stronger than normal impulsive microwave bursts for the same observed amount of hard X-ray emission. This feature, along with the observation of 100% circular polarization, strongly supports a maser origin for the decimetre spike bursts.

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