Surface magnetic field effects in local helioseismology

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics

Scientific paper

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6 pages, 8 figures

Scientific paper

10.1002/asna.200610732

Using helioseismic holography strong evidence is presented that the phase (or equivalent travel-time) of helioseismic signatures in Dopplergrams within sunspots depend upon the line-of-sight angle in the plane containing the magnetic field and vertical directions. This is shown for the velocity signal in the penumbrae of two sunspots at 3, 4 and 5 mHz. Phase-sensitive holography demonstrates that they are significantly affected in a strong, moderately inclined magnetic field. This research indicates that the effects of the surface magnetic field are potentially very significant for local helioseismic analysis of active regions.

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