Physics
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ssrv...17..181d&link_type=abstract
(IAU, IUGG, URSI, IUPAP, COSPAR, and SCOSTEP, International Solar-Terrestrial Physics Symposium, Sao Paulo, Brazil, June 17-24,
Physics
3
Chromosphere, Magnetospheric Instability, Polar Substorms, Solar Flares, Auroras, Cosmic Plasma, Energy Dissipation, Magnetic Storms, Solar Magnetic Field, Solar Spectra
Scientific paper
A study of those processes that appear similar in solar flare and magnetospheric substorm phenomena is presented. Two categories of problems are considered: (1) the gradual build-up of an energy reservoir that is cataclysmatically released during a flare or a substorm; and (2) the physical processes that take place once the energy release has started. It is concluded that flares, like substorms, occur in a magnetoactive plasma; that photospheric layers probably supply mass to flare processes; that one of the most important processes occurring during some flares is the acceleration of charged particles; and that further study is required in this area.
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