Collisional filtration model in the solar transition region

Details Collisional filtration model in the solar transition region Collisional filtration model in the solar transition region

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..273g&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 273-2

Physics

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

In this work we will try to show the physical reasons for the steep temperature increase in the solar transition region, trying to look for a solution of the Boltzmann equation, which seems to be the most suitable tool for describing the plasma of the solar transition region. To solve the Boltzmann equation, we have used a Monte Carlo method; as a solution of this equation we have obtained a temperature enhancement and a density drop; besides, we have computed an electron heat flux towards the innersphere, showing a departure from the classical transport theory.

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