U.S.-Japan Seminar on the Recent Advances in the Understanding of Solar Flares, Tokyo, Japan, October 5-8, 1982, Proceedings

Details U.S.-Japan Seminar on the Recent Advances in the Understanding of Solar Flares, Tokyo, Japan, October 5-8, 1982, Proceedings U.S.-Japan Seminar on the Recent Advances in the Understanding of Solar Flares, Tokyo, Japan, October 5-8, 1982, Proceedings

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86.....k&link_type=abstract

Seminar sponsored by the Japan Society for the Promotion of Science and National Science Foundation. Solar Physics (ISSN 0038-09

Physics

24

Conferences, Solar Flares, Solar Physics, Chromosphere, Energetic Particles, Energy Transfer, Japanese Spacecraft, Nuclear Reactions, Particle Acceleration, Plasma Heating, Solar Atmosphere, Solar Corona, Solar Corpuscular Radiation, Solar Electrons, Solar Instruments, Solar Magnetic Field, Solar Maximum Mission, Solar Radio Bursts, Solar Spectra, Solar X-Rays, Thermal Plasmas

Scientific paper

Papers are presented on recent research concerning the understanding of solar flares, including the general characteristics of flares; energy transport, and chromospheric heating and evaporation; emission processes and source structure; and high energy photons, nuclear processes, and particle acceleration. Topics addressed include magnetic theories of solar flares, nonthermal and nonequilibrium effects in soft X-ray flare spectra, the thermal evolution of flare plasmas, upper limits on the total radiant energy of solar flares, energetic electrons as an energy transport mechanism in solar flares, the spatial characteristics of microwave bursts, and the relation between hard X-ray spectra and electron energy spectra. Also examined are the pre-flare and post-flare X-ray variations in active regions, the imaging of impulsive solar flare phenomena, the vertical structure of hard X-ray flares, the spatial structure of high energy photon sources, gamma-ray lines and neutrons from solar flares, and a dynamical interpretation of the very hot region appearing at the top of a loop. For individual items see A83-47659 to A83-47701

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