Equilibrium model of thin magnetic flux tubes

Details Equilibrium model of thin magnetic flux tubes Equilibrium model of thin magnetic flux tubes

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.207..277b&link_type=abstract

In ESA Plasma Astrophys. p 277-280 (SEE N85-22270 12-90)

Other

Astronomical Models, Magnetic Flux, Solar Atmosphere, Atmospheric Stratification, Beta Factor, Energy Transfer, Solar Magnetic Field

Scientific paper

The existence of a physically realizable domain in which approximations that lead to a self consistent solution for flux tube stratification in the solar atmosphere, without ad hoc hypotheses, is proved. The transfer equation is solved assuming that no energy transport other than radiative is present. Convective motions inside the tube are assumed to be suppressed by magnetic forces. Only one parameter, the plasma beta at tau = 0, must be specified, and this can be estimated from observations of spatially resolved flux tubes.

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