The K-corona under hydrostatic density distribution Relevance to solar wind

Details The K-corona under hydrostatic density distribution Relevance to solar wind The K-corona under hydrostatic density distribution Relevance to solar wind

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..103..385b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 103, no. 2, 1986, p. 385-392.

Physics

14

Density Distribution, Hydrostatics, Solar Corona, Solar Wind, Brightness Distribution, Thomson Scattering

Scientific paper

An analytical expression is obtained for the K-corona brightness as a function of the distance from the solar limb. The agreement of the theory with the numerous observational data indicates that the density distribution at the levels located at 1.2 - 2.5 R_sun; heliocentric distances may be treated as hydrostatic with T = const. The deviation of the observed K-corona brightness from the expression obtained may be indicative of supersonic fluxes of matter. These concepts may be used to verify the various theoretical models for solar wind source.

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