Thermal forces and the coronal helium abundance

Details Thermal forces and the coronal helium abundance Thermal forces and the coronal helium abundance

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..620h&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 620-6

Computer Science

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

Scientific paper

The interaction between protons and minor ions in the chromosphere-corona transition region produces an upward force on the minor ions and an enhanced coronal abundance. In this presentation we compare a ``classical'' hydrodynamical model of a hydrogen - helium solar wind and a model based on a 16-moment fluid description where the heat flux is treated in a self-consistent manner.

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