The Solar Maximum Year program - Main results

Details The Solar Maximum Year program - Main results The Solar Maximum Year program - Main results

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983prir.....q..82s&link_type=abstract

Priroda (ISSN 0032-874X), Dec. 1983, p. 82-90. In Russian.

Physics

Satellite Observation, Solar Atmosphere, Solar Flares, Solar Maximum Mission, Electron Acceleration, Solar Activity, Solar Magnetic Field, Solar Wind, Solar X-Rays

Scientific paper

After a brief review of the physics of solar activity and flares, the paper describes the objectives and organization of the Solar Maximum Year (SMM) program. The main results are briefly discussed, with attention given to X-ray studies from the SMM satellite, VLA observations of the rapid quadrupole-to-dipole transition of magnetic fields, the existence of magnetic transients, the chromospheric 'evaporation' phenomenon, and the existence of accelerated-electron beams.

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