Ohmic heating from a time-varying stellar magnetic field can rival or exceed XUV heating in the upper atmospheres of close-in exoplanets and can screen the field above the 1 microbar level.
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Ohmic heating in the upper atmosphere of hot exoplanets The influence of a time-varying magnetic field
Ohmic heating from a time-varying stellar magnetic field can rival or exceed XUV heating in the upper atmospheres of close-in exoplanets and can screen the field above the 1 microbar level.