It is believed that radio type IVs, co-spatial with dense hot plasmoids, may be the result of a plasma radiation emission mechanism. The injection of mass into the corona was recently observed in chromospheric and coronal lines with magnetic field changes and also at very high speeds into loops. The start time of coronal loop transients, if extrapolated to the chromosphere, in most cases precedes flare H-alpha or X-ray emission. Observational inferences from polarization and other studies are seen as favoring the three-dimensional bubble over the planar loop as a description of coronal mass motions.
Serf studies of mass motions arising in flares
1982-01-01
Sonstige
Keine Angabe
Englisch
SERF studies of mass motions arising in flares
Elsevier | 1983
|Recent Trend in Serf-Tuning Technologies
British Library Online Contents | 1998
|Consecutive homologous flares and their relation to sunspot motions
Elsevier | 1984
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