Understanding the convective Sun

Details Understanding the convective Sun Understanding the convective Sun

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.517..195t&link_type=abstract

In: Proceedings of SOHO 12 / GONG+ 2002. Local and global helioseismology: the present and future, 27 October - 1 November 2002,

Physics

Convection, Solar Atmosphere, Solar Structure, Helioseismology

Scientific paper

Hydrodynamical simulations of the surface layers of the Sun, has greatly improved our understanding and interpretation of solar observations. I review some past successes in matching spectral lines, improving the agreement with high-degree p-mode frequencies and matching the depth of the solar convection zone without adjustable convection-parameters. Our solar simulations contain p-modes, and are used for studying the asymmetry of p-mode peaks and to calibrate the conversion between the observed velocity proxies and the actual velocities.

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