Recipe for a Saturn‐Like Dynamo
Abstract The Cassini Grand Finale orbits provided detailed observations of Saturn’s internal magnetic field. Unique characteristics of the observed field, such as its axisymmetry and power spectrum, provide constraints on dynamo processes deep in Saturn’s interior. Here, we use numerical dynamo simu...
| Published in: | AGU Advances |
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| Main Authors: | , |
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2021-06-01
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| Subjects: | |
| Online Access: | https://doi.org/10.1029/2020AV000318 |