Spatiotemporal Properties of Compressible Magnetohydrodynamic Turbulence from Space Plasma

It is well established that Alfvénic turbulence undergoes a weak-to-strong transition as energy cascades to smaller scales, but whether this occurs in compressible magnetohydrodynamic (MHD) turbulence remains unclear. Using multispacecraft measurements from Cluster and an improved polarization-based...

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Detalhes bibliográficos

Principais autores:	Siqi Zhao, Huirong Yan, Terry Z. Liu, Chuanpeng Hou, Ka Ho Yuen
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2026-01-01
coleção:	The Astrophysical Journal
Assuntos:	Interplanetary turbulence Magnetohydrodynamics Plasma physics
Acesso em linha:	https://doi.org/10.3847/1538-4357/ae7e87
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