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- W4386965364 abstract "Enceladus is an astrobiologically compelling target for scientific study and is predicted to have high seismic activity for its size, particularly at its south pole. We conduct ray-theoretical and full-waveform seismic simulations for three 1D models of Enceladus to compare the effects of ice shell and ocean thickness, as well as core structure and composition, on the waveforms recorded by a single seismometer. The 1D models are constructed using self-consistent modelling techniques to enable direct comparisons between the wavefields of each model. We investigate phases sampling the ice, ocean, and core layers at up to 8 Hz, complementing previous studies focussed on lower-frequency phases concentrated in the ice shell. We conclude that even at low epicentral distances (¡30°) from a source at the south pole, core-transmitted and -reflected phases can likely both be observed, providing constraints on ocean depth and core structure. We further confirm that a high-attenuation scenario for the ice shell does not preclude the generation of seismic signals above mission-candidate instrument sensitivity thresholds, and in fact may serve to remove unwanted signals from seismograms." @default.
- W4386965364 created "2023-09-23" @default.
- W4386965364 creator A5034938537 @default.
- W4386965364 creator A5079778433 @default.
- W4386965364 date "2024-01-01" @default.
- W4386965364 modified "2023-10-18" @default.
- W4386965364 title "Global seismology in the interior of Enceladus" @default.
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- W4386965364 doi "https://doi.org/10.1016/j.icarus.2023.115806" @default.
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