Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...464..476j&link_type=abstract
Astrophysical Journal v.464, p.476
Astronomy and Astrophysics
Astronomy
12
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.
Hindman Bradley W.
Jain Rekha
Zweibel Ellen G.
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