Turbulence Properties of Interplanetary Coronal Mass Ejections in the Inner Heliosphere: Dependence on Proton Beta and Flux Rope Structure

Interplanetary coronal mass ejections (ICMEs) have low proton beta across a broad range of heliocentric distances and a magnetic flux rope structure at large scales, making them a unique environment for studying solar wind fluctuations. Power spectra of magnetic field fluctuations in 28 ICMEs observ...

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Detalles Bibliográficos

Principais autores:	S. W. Good, O. K. Rantala, A.-S. M. Jylhä, C. H. K. Chen, C. Möstl, E. K. J. Kilpua
Formato:	Artigo
Idioma:	Inglês
Publicado:	IOP Publishing 2023-01-01
Series:	The Astrophysical Journal Letters
Assuntos:	Solar coronal mass ejections Interplanetary magnetic fields Interplanetary turbulence Solar wind
Acceso en liña:	https://doi.org/10.3847/2041-8213/acfd1c
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