Effects of Convection on Solar $p$ Modes

Physics

Scientific paper

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Solar Physics, Convection, $P$ Modes

Scientific paper

We are investigating how advective motions and structures such as magnetic flux tubes affect the propagation of $p$ modes in the Sun. We do this by means of a computer code which determines the eigenfrequencies of a ray with a given dispersion relation traveling through a plane-parallel medium with variations in the local wave velocity. By coupling this program to a numerical model of the solar convection zone, we plan to calculate shifts in eigenfrequencies as well as line widths and compare them to new high-quality data from the GONG project as well as from the MDI instrument on SOHO.

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