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Paper: Interaction of Helioseismic Waves with Sunspots: Observations and Numerical MHD Simulations
Volume: 462, Progress in Solar/Stellar Physics with Helio- and Asteroseismology
Page: 277
Authors: Zhao, J.; Parchevsky, K. V.; Kosovichev, A. G.
Abstract: We investigate how helioseismic waves that originate from effective point sources interact with sunspots. For observations, the waves from point sources are reconstructed by cross-correlating observed photospheric Doppler signals. For numerical simulations, the waves are generated by simulating perturbation propagation from a pulse near the surface and propagate through magnetostatic and magnetohydrodynamic (MHD) sunspot models. For both cases, we study f-mode and p-mode waves separately. We also study different cases when the point source is located outside the sunspot, and when the source is located inside the sunspot. Our results nicely visualize how the waves, including both wave amplitudes and phases, interact with the magnetic field, thermodynamic and flow structure of sunspots, and how the waveform evolves before, during, and after the propagation through sunspots. Our analysis of wave–magnetic-field interactions also extends below the sunspot's surface. This brings us new rich information of how the waves respond to the magnetic field below the surface, but also poses new challenges for local helioseismology to infer the sunspot's interior properties from waveform observations.
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