Ohmic and viscous damping of inner core translational oscillations
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arXiv
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| Hauptverfasser: | , , , , |
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| Format: | Preprint |
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2026
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| _version_ | 1866908989222027264 |
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| author | Personnettaz, Paolo Cébron, David Schaeffer, Nathanaël Deguen, Renaud Mandea, Mioara |
| author_facet | Personnettaz, Paolo Cébron, David Schaeffer, Nathanaël Deguen, Renaud Mandea, Mioara |
| contents | Large earthquakes can trigger translational oscillations of Earth's inner core (Slichter modes), yet their damping remains uncertain. Using simulations, we quantify viscous and Ohmic dissipation in the fluid outer core. Earth's rotation splits the motion into one polar and two equatorial modes. We explore all three and derive scaling laws for the quality factor with each dissipation mechanism. Viscous effects are negligible, confined to a thin layer at the inner core boundary. Ohmic dissipation dominates, with decay times of 3-16 years. Equatorial modes damp at least twice as fast as the polar mode. Our results suggest that Slichter modes can persist for years. Their continued non-detection is therefore more likely due to weak excitation than rapid damping. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2604_21417 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | Ohmic and viscous damping of inner core translational oscillations Personnettaz, Paolo Cébron, David Schaeffer, Nathanaël Deguen, Renaud Mandea, Mioara Geophysics Large earthquakes can trigger translational oscillations of Earth's inner core (Slichter modes), yet their damping remains uncertain. Using simulations, we quantify viscous and Ohmic dissipation in the fluid outer core. Earth's rotation splits the motion into one polar and two equatorial modes. We explore all three and derive scaling laws for the quality factor with each dissipation mechanism. Viscous effects are negligible, confined to a thin layer at the inner core boundary. Ohmic dissipation dominates, with decay times of 3-16 years. Equatorial modes damp at least twice as fast as the polar mode. Our results suggest that Slichter modes can persist for years. Their continued non-detection is therefore more likely due to weak excitation than rapid damping. |
| title | Ohmic and viscous damping of inner core translational oscillations |
| topic | Geophysics |
| url | https://arxiv.org/abs/2604.21417 |