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Formation of H+ PUI Tails Downstream of Distant Interplanetary Shocks

New Horizons’ Solar Wind Around Pluto (SWAP) instrument has observed interplanetary shocks from ∼20 to 60 au from the Sun. Different studies have analyzed the effects of these shocks on the solar wind ion (SWI) and interstellar pickup ion (PUI) distributions. A key finding includes the observation o...

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Hoofdauteurs: E. J. Zirnstein, D. J. McComas, B. L. Shrestha, H. A. Elliott, P. C. Brandt, S. A. Stern, A. R. Poppe, J. Parker, E. Provornikova, K. Singer, A. Verbiscer, New Horizons Heliophysics Team
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2025-01-01
Reeks:The Astrophysical Journal
Onderwerpen:
Heliosphere
Solar wind
Interplanetary shocks
Particle physics
Interplanetary turbulence
Online toegang:https://doi.org/10.3847/1538-4357/addf45
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