Local time asymmetry of Saturn's magnetosheath flows
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DOI: 10.1002/2017gl073031
Abstract: Using gross averages of the azimuthal component of flow in Saturn's magnetosheath, we find that flows in the pre-noon sector reach a maximum value of roughly half that of the post-noon side. Corotational magnetodisc plasma… read more here.
Keywords: magnetosheath; time asymmetry; magnetosheath flows; asymmetry saturn ... See more keywords