Astronomy and Astrophysics – Astronomy
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.0712i&link_type=abstract
American Astronomical Society, SPD meeting #40, #7.12; Bulletin of the American Astronomical Society, Vol. 41, p.814
Astronomy and Astrophysics
Astronomy
Scientific paper
The power of solar acoustic waves is reduced inside magnetic regions mainly due to absorption, emissivity reduction and local suppression. These coefficients were recently determined for one acoustic wave travel distance with the use of direction and phase-velocity filters. The purpose of this work is to determine all three parameters, absorption, emissivity reduction and local suppression, with a new method that does not include direction and phase-velocity filters. This method utilizes many active regions from SOHO / MDI observations to increase the signal-to-noise ratio. For each active region, we compute cross-covariances of outgoing and ingoing waves as well as double-skip waves that have the reflection located inside the active region. The exactly same procedures are applied to the quiet sun to obtain cross-covariances as references. The wide range of acoustic modes that are used in the absence of any filtering enables the determination of the above parameters as functions of the travel distance from the center of the magnetic region.
Ilonidis Efstathios
Zhao Jun
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