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• W2098202352 endingPage "77" @default.
• W2098202352 startingPage "77" @default.
• W2098202352 abstract "We compare helioseismic travel-time shifts measured from a realistic magnetoconvective sunspot simulation using both helioseismic holography and time–distance helioseismology, and measured from real sunspots observed with the Helioseismic and Magnetic Imager instrument on board the Solar Dynamics Observatory and the Michelson Doppler Imager instrument on board the Solar and Heliospheric Observatory. We find remarkable similarities in the travel-time shifts measured between the methodologies applied and between the simulated and real sunspots. Forward modeling of the travel-time shifts using either Born or ray approximation kernels and the sound-speed perturbations present in the simulation indicates major disagreements with the measured travel-time shifts. These findings do not substantially change with the application of a correction for the reduction of wave amplitudes in the simulated and real sunspots. Overall, our findings demonstrate the need for new methods for inferring the subsurface structure of sunspots through helioseismic inversions." @default.
• W2098202352 created "2016-06-24" @default.
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• W2098202352 date "2011-12-14" @default.
• W2098202352 modified "2023-09-27" @default.
• W2098202352 title "HELIOSEISMOLOGY OF A REALISTIC MAGNETOCONVECTIVE SUNSPOT SIMULATION" @default.
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• W2098202352 doi "https://doi.org/10.1088/0004-637x/744/1/77" @default.
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