MMS data shows perpendicular electrons dominate j·E dissipation in magnetotail magnetic structures during turbulent reconnection, with bidirectional energy transfer and quantified mechanisms including parallel E, Fermi, betatron, and polarization effects.
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Statistical study of energy dissipation in magnetic structures during turbulent reconnection in the Earth's magnetotail
MMS data shows perpendicular electrons dominate j·E dissipation in magnetotail magnetic structures during turbulent reconnection, with bidirectional energy transfer and quantified mechanisms including parallel E, Fermi, betatron, and polarization effects.