Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009apj...706..909c&link_type=abstract
The Astrophysical Journal, Volume 706, Issue 1, pp. 909-916 (2009).
Astronomy and Astrophysics
Astronomy
6
Sun: Activity, Sun: Helioseismology, Sun: Interior, Sunspots
Scientific paper
Observed acoustic power in magnetic regions is lower than the quiet Sun because of absorption, emissivity reduction, and local suppression of solar acoustic waves in magnetic regions. In the previous studies, we have developed a method to measure the coefficients of absorption, emissivity reduction, and local suppression of sunspots. In this study, we go one step further to measure the spatial distributions of three coefficients in two active regions, NOAA 9055 and 9057. The maps of absorption, emissivity reduction, and local suppression coefficients correlate with the magnetic map, including plage regions, except the emissivity reduction coefficient of NOAA 9055 where the emissivity reduction coefficient is too weak and lost among the noise.
Chou Dean-Yi
Liang Zhi-Chao
Sun Ming-Tsung
Yang Ming-Hsu
Zhao Hui
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