Influence of the anomalous thermal conductivity on the structure of the solar atmosphere transition region

Details Influence of the anomalous thermal conductivity on the structure of the solar atmosphere transition region Influence of the anomalous thermal conductivity on the structure of the solar atmosphere transition region

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008astl...34..344b&link_type=abstract

Astronomy Letters, Volume 34, Issue 5, pp.344-352

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The generalized Wiedemann-Franz law for a nonisothermal quasi-neutral plasma with developed ion-acoustic turbulence and Coulomb collisions has been proven. The results obtained are used to explain the anomalously low thermal conductivity in the chromosphere-corona transition region of the solar atmosphere. Model temperature distributions in the lower corona and the transition region that correspond to well-known experimental data have been determined. The results obtained are useful for explaining the abrupt change in turbulent-plasma temperature at distances smaller than the particle mean free path.

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