Quantifying Turbulence as Captured in the Inner Corona in White-light Total Solar Eclipse Images

Turbulence is a fundamental process in astrophysical plasmas, playing a key role in energy transfer and dissipation. The solar corona is thought to be heated to temperatures exceeding 10 ^6  K in part by turbulent processes. Using the highest-resolution white-light total solar eclipse image obtained...

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Bibliografische Detailangaben

Hauptverfasser:	Zachary Bailey, Shadia Rifai Habbal, Riddhi Bandyopadhyay, Shaheda Begum Shaik
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	IOP Publishing 2026-01-01
Schriftenreihe:	The Astrophysical Journal Letters
Schlagworte:	Solar wind Solar physics Interplanetary turbulence Solar corona Solar eclipses Space plasmas
Online-Zugang:	https://doi.org/10.3847/2041-8213/ae4d16
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