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- W3131485357 abstract "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⊙ 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." @default.
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- W3131485357 date "1986-01-01" @default.
- W3131485357 modified "2023-09-28" @default.
- W3131485357 title "The K-corona under hydrostatic density distribution; relevance to solar wind" @default.
- W3131485357 hasPublicationYear "1986" @default.
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