F-mode Seismology Of Solar Simulations

Details F-mode Seismology Of Solar Simulations F-mode Seismology Of Solar Simulations

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1613d&link_type=abstract

American Astronomical Society, SPD meeting #42, #16.13; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

Time-distance helioseismology using f-mode travel times is used to study near-surface regions of realistic numerical magnetohydrodynamic simulations. A fully-consistent inversion procedure is used to analyze the simulation flow field outside of a sunspot. This approach is carried out to validate the time-distance technique, as well as the sensitivity kernels and the inversion algorithm. This work is supported by NASA under the SDO Science Center project (contract NNH09CE41C) as well as well as a NASA EPSCoR award.

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