Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..130......&link_type=abstract
Workshop sponsored by the Committee of European Radio Astronomers, SNSF, URSI, et al. Solar Physics (ISSN 0038-0938), vol. 130,
Astronomy and Astrophysics
Astronomy
Conferences, Particle Beams, Solar Atmosphere, Solar Flares, Solar Radio Bursts, Electron Beams, Magnetic Field Configurations, Noise Storms, Radio Astronomy, Solar Magnetic Field, Solar Physics, Solar Radiation, Solar X-Rays
Scientific paper
Papers included in this issue discuss particle beams in the solar atmosphere, the role of magnetic field in the intensity and geometry of the type II burst generation, hard X-rays and associated weak decimetric bursts, the observations of beam propagation, and the type III radio burst productivity of solar flares. Consideration is given to interplanetary particle beams, the fine structures in solar radio bursts at 21-cm wavelength and pulsation modulation, spike observations in flares in China, simulation studies of electron acceleration by ion-ring distributions in solar flares, and the production of hard X-rays in solar flares. Attention is also given to the solar surface velocity fields determined from small magnetic features, the H-alpha line profile observations of a limb flare with a high temporal resolution, the pulse beam heating of solar atmosphere, the meter-decameter observations of the dMe flare stars with the Clark Lake Radio Telescope, and the magnetic field configurations which can produce prominences with inverse polarity.
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