Two-dimensional partially ionized magnetohydrodynamic turbulence
© Ionization occurs in the upper atmospheres of hot Jupiters and in the interiors of gas giant planets, leading to magnetohydrodynamic (MHD) effects that couple the momentum and the magnetic field, thereby significantly altering the dynamics. In regions of moderate temperatures, the gas is only par...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Cambridge University Press (CUP)
2021
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| Online Access: | https://hdl.handle.net/1721.1/133786 |