An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations

An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations

Solar radio bursts are strongly affected by radio-wave scattering on density inhomogeneities, changing their observed time characteristics, sizes, and positions. The same turbulence causes angular broadening and scintillation of galactic and extragalactic compact radio sources observed through the s...

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Bibliographic Details
Main Authors: Eduard P. Kontar, A. Gordon Emslie, Daniel L. Clarkson, Xingyao Chen, Nicolina Chrysaphi, Francesco Azzollini, Natasha L. S. Jeffrey, Mykola Gordovskyy
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Radio bursts
Interplanetary scintillation
Interplanetary turbulence
Solar corona
Solar wind
Online Access:https://doi.org/10.3847/1538-4357/acf6c1

Internet

https://doi.org/10.3847/1538-4357/acf6c1

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