Código QR (código de barras bidimensional)

Constraints on Solar Wind Density and Velocity Based on Coronal Tomography and Parker Solar Probe Measurements

Previous work has established an empirical relationship between densities gained from coronal rotational tomography near the ecliptic plane with solar wind outflow speeds at heliocentric distance r _0 = 8 R _⊙ . This work aims to include solar wind acceleration, and thus velocity profiles out to 1 a...

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Detalhes bibliográficos
Principais autores: Kaine A. Bunting, Luke Barnard, Mathew J. Owens, Huw Morgan
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2024-01-01
coleção:The Astrophysical Journal
Assuntos:
Acesso em linha:https://doi.org/10.3847/1538-4357/ad1506
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