Magnetic Reconnection–driven Energization of Protons up to ∼400 keV at the Near-Sun Heliospheric Current Sheet

We report observations of direct evidence of energetic protons being accelerated above ∼400 keV within the reconnection exhaust of a heliospheric current sheet (HCS) crossing by NASA’s Parker Solar Probe (PSP) at a distance of ∼16.25 solar radii ( R _s ) from the Sun. Inside the exhaust, both the re...

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Váldodahkkit:	M. I. Desai, J. F. Drake, T. Phan, Z. Yin, M. Swisdak, D. J. McComas, S. D. Bale, A. Rahmati, D. Larson, W. H. Matthaeus, M. A. Dayeh, M. J. Starkey, N. E. Raouafi, D. G. Mitchell, C. M. S. Cohen, J. R. Szalay, J. Giacalone, M. E. Hill, E. R. Christian, N. A. Schwadron, R. L. McNutt Jr., O. Malandraki, P. Whittlesey, R. Livi, J. C. Kasper
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2025-01-01
Ráidu:	The Astrophysical Journal Letters
Fáttát:	Solar magnetic reconnection
Liŋkkat:	https://doi.org/10.3847/2041-8213/ada697
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