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Lack of Detailed Balance at Sub-ion Scales in Turbulent Solar Wind

A notable feature of turbulence in solar wind is the presence of an additional power-law spectral domain at scales below the ion inertial length. This spectral domain has been attributed to a distinct turbulent regime involving alternative wave modes. However, this interpretation is still up for deb...

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Autors principals: Giuseppe Consolini, Elettra Consolini
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2026-01-01
Col·lecció:The Astrophysical Journal Letters
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Accés en línia:https://doi.org/10.3847/2041-8213/ae3d32
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