The Influence of Magnetism on p-Mode Surface Amplitudes

Astronomy and Astrophysics – Astronomy

Scientific paper

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Sun: Activity, Sun: Magnetic Fields, Sun: Oscillations

Scientific paper

We propose a mechanism to explain the observed suppression of p-mode surface velocities in solar active regions. We show that a horizontal magnetic field can lower the upper turning point and change the skin depth for a simple plane-parallel adiabatically stratified polytrope. In addition to power suppression, the magnetic field alters the phase of p-modes. Simultaneous measurements of phase as well as amplitude in the active and quiet regions would provide an additional diagnostic for probing the structure of active region magnetic fields.

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