The active solar corona

Details The active solar corona The active solar corona

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983sciam.248..104w&link_type=abstract

Scientific American, vol. 248, Feb. 1983, p. 104-106, 108, 110-112(3ff.).

Computer Science

Sound

Solar Activity, Solar Corona, Solar Prominences, Astronomical Photography, Digital Data, Photosphere, Solar Eclipses, Solar Maximum Mission, Solar Terrestrial Interactions, Solar Wind, X Ray Imagery

Scientific paper

Progress in solar corona research is discussed. Coronal observations using X-ray telescopes, radio telescopes, and coronagraphs are described. The interactions of magnetic fields, electric currents, and gas pressure to produce coronal phenomena are considered, reporting on the use of models to explain some of the phenomena. The heating of the corona by sound waves or MHD waves is addressed. The effects of changes in the solar wind emanating from the corona on the earth, mediated by the wind's interaction with the earth's magnetosphere, are described.

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