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First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR

We present a comprehensive analysis aimed at proving the hypothesis that a train of small-scale features observed by the Wide-field Imager (WISPR) onboard the Parker Solar Probe (PSP) are the signature of a Kelvin–Helmholtz instability (KHI). These features were seen near the flank of a Coronal Mass...

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Príomhchruthaitheoirí: Evangelos Paouris, Guillermo Stenborg, Mark G. Linton, Angelos Vourlidas, Russell A. Howard, Nour E. Raouafi
Formáid: Artigo
Teanga:Inglês
Foilsithe / Cruthaithe: IOP Publishing 2024-01-01
Sraith:The Astrophysical Journal
Ábhair:
Rochtain ar líne:https://doi.org/10.3847/1538-4357/ad2208
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