3D MHD modelling of a chromosphere above the sun's convective zone

Details 3D MHD modelling of a chromosphere above the sun's convective zone 3D MHD modelling of a chromosphere above the sun's convective zone

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..271..393p&link_type=abstract

Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 271,

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We report on the extension of the ASH code to include an atmospheric stable layer (i.e not convective). This layer is meant to model the sun's chromosphere within the anelastic approximation limits while coping with the wide range of densities, time and spatial scales between r = 0.7 Rsolar and r = 1.03 Rsolar. Convective overshoot into the stable atmospheric layer is observed in a region ~ 0.01 Rsolar thick, exciting waves which propagate upwards into the atmosphere.

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