Correlation between Electron Temperature and Ion Charge-state Ratios in the Solar Wind at ∼0.5 au

Whether solar wind electrons expanding into the heliosphere can preserve information about their origin in the solar corona remains an open debate. The suprathermal strahl temperature has often been postulated as an indicator of source coronal electron temperature, while the core electron temperatur...

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Detalhes bibliográficos

Principais autores:	Xiangyu Wu, Christopher J. Owen, Jesse Coburn, Georgios Nicolaou, Daniel Verscharen, Jingting Liu, Charalambos Ioannou, Hao Ran, Yeimy J. Rivera, Stephanie L. Yardley
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2026-01-01
coleção:	The Astrophysical Journal
Assuntos:	Solar wind Space plasmas Interplanetary physics
Acesso em linha:	https://doi.org/10.3847/1538-4357/ae3c7b
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