Physics
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..114..347g&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 114, no. 2, 1987, p. 347-362.
Physics
11
Solar Corona, Solar Spectra, Stellar Mass Ejection, Particle Interactions, Radio Spectra, Visible Spectrum
Scientific paper
The authors present the two-dimensional imaging observations of radio bursts in the frequency range 25 - 50 MHz made with the Clark Lake multifrequency radioheliograph during a coronal mass ejection event (CME) observed on 1984, June 27 by the SMM Coronagraph/Polarimeter and Mauna Loa K-coronameter. The event was spatially and temporally associated with precursors in the form of meter-decameter type III bursts, soft X-ray emission and a Hα flare spray. The observed type IV emission in association with the CME (and the Hα spray) could be interpreted as gyrosynchrotron emission from a plasmoid containing a magnetic field of ≡2.5 G and nonthermal electrons with a number density of ≡105cm-3 and energy ⪆350 keV.
Gopalswamy Nat
Kundu Mukul R.
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