Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-02-11
Astronomische Nachrichten, Volume 328, Issue 3, page 292, 2007
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
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.
Braun Doug C.
Cally Paul S.
Schunker Hannah
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