An eruptive prominence and associated cm-mm emission outside the solar limb

Details An eruptive prominence and associated cm-mm emission outside the solar limb An eruptive prominence and associated cm-mm emission outside the solar limb

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116...83z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 116, no. 1, 1988, p. 83-89. FINEP-supported research.

Astronomy and Astrophysics

Astronomy

6

Solar Flares, Solar Limb, Solar Prominences, Astronomical Maps, Radio Astronomy

Scientific paper

The authors present radio maps at 22 and 44 GHz which show the emission before and after the eruption of a quiescent prominence located at the west limb. The observed radiation following the eruption is not consistent with thermal bremsstrahlung mechanism. It can be interpreted as due to gyrosynchrotron emission of nonthermal electrons. The authors' observations appear to be similar to the microwave radiation observed in post-flare loops; this radiation is due to nonthermal electrons trapped in the closed magnetic structures formed after the prominence eruption.

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