Other
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989sao..reptr....g&link_type=abstract
Semiannual Report Nos. 12-17, 1 May 1986 - 30 Apr. 1989 Smithsonian Astrophysical Observatory, Cambridge, MA.
Other
Coronal Holes, Solar Activity, Solar Corona, Stellar Activity, Stellar Coronas, Chromosphere, Geomagnetic Tail, Magnetohydrodynamic Waves, Photosphere, Radio Emission, Radio Observation, Solar Flares, Solar Prominences, Solar Wind, Stellar Magnetic Fields, Stellar Rotation, Stellar Winds, Tearing Modes (Plasmas), Very Large Array (Vla)
Scientific paper
Progress in observational, theoretical, and radio studies of coronal plasmas is summarized. Specifically work completed in the area of solar and stellar magnetic fields, related photospheric phenomena and the relationships between magnetism, rotation, coronal and chromospheric emission in solar-like stars is described. Also outlined are theoretical studies carried out in the following areas, among others: (1) neutral beams as the dominant energy transport mechanism in two ribbon-flares; (2) magneto hydrodynamic and circuit models for filament eruptions; and (3) studies of radio emission mechanisms in transient events. Finally, radio observations designed for coronal activity studies of the sun and of solar-type coronae are described. A bibliography of publications and talks is provided along with reprints of selected articles.
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