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Computer simulations of Jupiter’s deep internal dynamics help interpret what Juno sees
We describe computer simulations of thermal convection and magnetic field generation in Jupiter’s deep interior: that is, its convective dynamo. Results from three different simulations highlight the importance of including the dynamics in the very deep interior, although much of the convection and...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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National Academy of Sciences
2018
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6142197/ https://www.ncbi.nlm.nih.gov/pubmed/29941563 http://dx.doi.org/10.1073/pnas.1709125115 |