Nonthermal radio emission associated with a coronal disconnection event

Details Nonthermal radio emission associated with a coronal disconnection event Nonthermal radio emission associated with a coronal disconnection event

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...424l.135g&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 424, no. 2, p. L135-L138

Astronomy and Astrophysics

Astronomy

5

Interplanetary Magnetic Fields, Magnetic Field Reconnection, Radio Sources (Astronomy), Solar Corona, Solar Flares, X Rays, Astronomical Observatories, Coronagraphs, Plasma Density, Plasmas (Physics), Polarimeters, Solar Maximum Mission, Temperature

Scientific paper

We have found possible radio signatures of a coronal disconnection event observed by the Solar Maximum Mission Coronagraph/Polarimeter. The radio emission seems to be produced by charged particles accelerated during the same reconnection process which is responsible for the disconnection event. We discuss the implications of the radio emission characteristics to the reconnection process.

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