D. Graham, Y. Khotyaintsev, M. André, A. Vaivads, A. Chasapis, W. Matthaeus, A. Retinò, F. Valentini, D. Gershman
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Non-Maxwellianity of electron distributions near Earth's magnetopause
Plasmas in Earth's outer magnetosphere, magnetosheath, and solar wind are essentially collisionless. This means particle distributions are not typically in thermodynamic equilibrium and deviate sig...
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