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Origin and Properties of the Near-subsonic Solar Wind Observed by Parker Solar Probe

We identify and examine the solar wind intervals near the sonic critical point (i.e., M _S ∼ 1) observed by the Parker Solar Probe. The near-subsonic wind intervals show similar properties: a low density, an extremely low velocity, a low proton temperature, and essentially no magnetic field deflecti...

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Principais autores: Wenshuai Cheng, Ying D. Liu, Hao Ran, Yiming Jiao, Michael L. Stevens, Justin C. Kasper
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/ad3b98
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