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• W2158045884 endingPage "136" @default.
• W2158045884 startingPage "136" @default.
• W2158045884 abstract "The helioseismic properties of the wave scattering generated by monolithic and spaghetti sunspots are analyzed by means of numerical simulations. In these computations, an incident f- or p1-mode travels through the sunspot model, which produces absorption and phase shift of the waves. The scattering is studied by inspecting the wavefield, computing travel-time shifts, and performing Fourier–Hankel analysis. The comparison between the results obtained for both sunspot models reveals that the differences in the absorption coefficient can be detected above noise level. The spaghetti model produces a steep increase of the phase shift with the degree of the mode at short wavelengths, while mode mixing is more efficient for the monolithic model. These results provide a clue for what to look for in solar observations to discern the constitution of sunspots between the proposed monolithic and spaghetti models." @default.
• W2158045884 created "2016-06-24" @default.
• W2158045884 creator A5022784363 @default.
• W2158045884 creator A5045685072 @default.
• W2158045884 creator A5054381864 @default.
• W2158045884 date "2014-06-02" @default.
• W2158045884 modified "2023-09-23" @default.
• W2158045884 title "EVALUATION OF THE CAPABILITY OF LOCAL HELIOSEISMOLOGY TO DISCERN BETWEEN MONOLITHIC AND SPAGHETTI SUNSPOT MODELS" @default.
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• W2158045884 doi "https://doi.org/10.1088/0004-637x/788/2/136" @default.
• W2158045884 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/5901914" @default.
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• W2158045884 hasPublicationYear "2014" @default.
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