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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Reconnection in transrelativistic AGN coronae can energize protons to tens of PeV, producing a neutrino spectrum consistent with NGC 1068 observations without tuning the proton spectral slope.
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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.
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Can magnetic reconnection power neutrino emission from AGN coronae?
Reconnection in transrelativistic AGN coronae can energize protons to tens of PeV, producing a neutrino spectrum consistent with NGC 1068 observations without tuning the proton spectral slope.