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Plasma Motions and Compressive Wave Energetics in the Solar Corona and Solar Wind from Radio Wave Scattering Observations

Radio signals propagating via the solar corona and solar wind are significantly affected by compressive waves, impacting the properties of solar bursts as well as sources viewed through the turbulent solar atmosphere. While static fluctuations scatter radio waves elastically, moving, turbulent, or o...

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Autors principals: Francesco Azzollini, A. Gordon Emslie, Daniel L. Clarkson, Nicolina Chrysaphi, Eduard P. Kontar
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2024-01-01
Col·lecció:The Astrophysical Journal
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Accés en línia:https://doi.org/10.3847/1538-4357/ad4154
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