Search for a self-consistent solar wind model

Details Search for a self-consistent solar wind model Search for a self-consistent solar wind model

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216...24g&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 24-27 (2010).

Physics

1

Solar Wind, Photosphere, Solar Corona, Hydrodynamics, Particle Emission, Solar Wind, Photosphere, Corona, Hydrodynamics

Scientific paper

We describe here a solar wind 1-fluid 1D model which is (1) time-dependent (2) includes transition region down to solar surface (3) uses a moderate number of grid points to enable further generalization to 2D/3D. The present model enables to study the response of the transition region and corona to photospheric pressure perturbations, including the solar wind up to ten solar radii. A simple chromosphere model with uniform temperature is used, in two different forms, either taking into account partial ionization or not. We show here how the amplitude of the response and associated viscous heating vary when attempting to decreasing the dynamical viscosity to approach realistic values.

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