Research study on dynamics of the solar atmosphere

Details Research study on dynamics of the solar atmosphere Research study on dynamics of the solar atmosphere

Jul 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hco..rept.....b&link_type=abstract

Final Report, 1 Jan. 1972 - 30 Jun. 1974 Harvard Coll. Observatory, Cambridge, MA.

Physics

Gravitational Fields, Magnetohydrodynamics, Solar Atmosphere, Solar Corona, Climate, Earth (Planet), Meteorology, Oso-5, Oso-6, Solar Activity Effects, Solar Wind, Sunspots

Scientific paper

This report summarizes studies carried out in magnetohydrodynamics and a new form of gravitational force. It describes coronal studies at two eclipses, reviews an attempt to verify (with negative results) a finding by Gnevyshev that the sunspot cycle on the average has a double maximum, and covers research in the general area of solar-terrestrial relations. Relationships between the intensity of the extreme ultraviolet (EUV) emission-line corona, the level of geomagnetic activity, and the velocity of the solar wind are discussed.

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