Modeled ocean convection in Ganymede produces a stationary magnetic field of about 5 nT, dominated by zonal jets, whose spatial pattern can identify the flow mode and, via peak-latitude shifts, constrain ocean thickness.
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Can the magnetic field induced by convective flow constrain the properties of Ganymede's subsurface ocean?
Modeled ocean convection in Ganymede produces a stationary magnetic field of about 5 nT, dominated by zonal jets, whose spatial pattern can identify the flow mode and, via peak-latitude shifts, constrain ocean thickness.