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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Váldodahkkit:	Xiangyu Wu, Christopher J. Owen, Jesse Coburn, Georgios Nicolaou, Daniel Verscharen, Jingting Liu, Charalambos Ioannou, Hao Ran, Yeimy J. Rivera, Stephanie L. Yardley
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2026-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Solar wind Space plasmas Interplanetary physics
Liŋkkat:	https://doi.org/10.3847/1538-4357/ae3c7b
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