Electrical conductivity in the solar photosphere and chromosphere

Details Electrical conductivity in the solar photosphere and chromosphere Electrical conductivity in the solar photosphere and chromosphere

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986baicz..37..155k&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 37, no. 3, 1986, p. 155-163.

Astronomy and Astrophysics

Astronomy

14

Chromosphere, Photosphere, Plasma Conductivity, Solar Atmosphere, Solar Wind, Electrical Resistivity, Solar Magnetic Field, Stellar Models

Scientific paper

The method of computing of isotropic, Pedersen, Hall and Cowling conductivities for the model of a quiet photosphere and chromosphere (C-model of VAL) is developed. Numerical results and graphs are calculated for magnetic fields of 10-2T and 10-4T using new values of the proton-hydrogen scattering cross-section. In addition, the graph of conductivities in the solenoid magnetic field model is presented. A table of the Braginski coefficients calculated from VAL is also presented.

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