White emission of the hydrostatic corona

Details White emission of the hydrostatic corona White emission of the hydrostatic corona

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..132b&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, Jan.-Feb. 1985, p. 132-140) Soviet Astronomy (ISSN 0038-5301), vol. 29, Jan.-Feb. 1985, p. 7

Astronomy and Astrophysics

Astronomy

12

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

Scientific paper

The analytical expression for the brightness distribution of the K corona as a function of the distance from the centre of the solar disk, B(ρ), is obtained under the assumption of the hydrostatic density distribution at T = const. It is shown that the standard form of numerous observed dependences ln B(ρ) is connected mainly with the validity of the above-mentioned simple assumptions in the layers above the inner corona which consists of closed loops. A convenient method is suggested for the determination of the temperature in the corona at the levels (1.2 - 2.5)R_sun; from the centre; the values T ≈ 1.5×106K at equatorial latitudes and T ≈ 1.1×106K in polar regions of the "minimum" corona are obtained.

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