Proton and Heavy Ion Acceleration by Magnetic Reconnection at the Near-Sun Heliospheric Current Sheet

Magnetic reconnection at the near-Sun heliospheric current sheet (HCS) dissipates the Parker spiral and converts magnetic energy into plasma kinetic energy. During Encounter 14 at a radial distance of $\sim $ 16.25 R​ _⊙ , Parker Solar Probe observed an HCS crossing where reconnection-driven acceler...

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Autori principali:	M. I. Desai, J. F. Drake, M. Swisdak, A. Fitzmaurice, D. J. McComas, S. D. Bale, T. Phan, G. Berland, D. G. Mitchell, C. M. S. Cohen, M. E. Hill, E. R. Christian, N. A. Schwadron, R. L. McNutt, W. H. Matthaeus, A. Rahmati, P. Whittlesey, R. Livi, D. Larson
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2026-01-01
Serie:	The Astrophysical Journal
Soggetti:	Solar magnetic reconnection
Accesso online:	https://doi.org/10.3847/1538-4357/ae48f2
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