Astronomy and Astrophysics – Astronomy
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.0707g&link_type=abstract
American Astronomical Society, SPD meeting #40, #7.07; Bulletin of the American Astronomical Society, Vol. 41, p.813
Astronomy and Astrophysics
Astronomy
Scientific paper
Seismic maps of the non-visible side of the Sun (far side) have been used for almost a decade to follow large active regions before they rotate to face the Earth. Preliminary efforts to quantify the success rate of the used technique (seismic holography) have been published with limited data. However, a thorough study is needed to further understand the limitations of the technique in terms of size and strength of the active regions detected and to reveal clues as to how to improve it.
We have analyzed three complete years of far-side seismic maps calculated using both Global Oscillation Newtwork group (GONG) and Michelson Doppler Imager (MDI) data and matched the far-side candidates with associated active regions as recorded by the NOAA database. Here we present the results.
Braun Daniel
Gonzalez-Hernandez Irene
Hill F. F.
Lindsey Charles
Scherrer Phil
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