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Using Jupiter’s gravitational field to probe the Jovian convective dynamo
Convective motion in the deep metallic hydrogen region of Jupiter is believed to generate its magnetic field, the strongest in the solar system. The amplitude, structure and depth of the convective motion are unknown. A promising way of probing the Jovian convective dynamo is to measure its effect o...
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| Veröffentlicht in: | Sci Rep |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artigo |
| Sprache: | Inglês |
| Veröffentlicht: |
Nature Publishing Group
2016
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| Schlagworte: | |
| Online Zugang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4804308/ https://ncbi.nlm.nih.gov/pubmed/27005472 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/srep23497 |
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