Langmuir-wave Excitation in Solar Wind Magnetic Holes

Langmuir-wave Excitation in Solar Wind Magnetic Holes

Magnetic holes (MHs) are structures commonly observed in various space plasma environments throughout the solar system, including the solar wind. These structures are characterized by a localized decrease in magnetic field strength, coincident with an increase in plasma density. Previous observation...

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Bibliographic Details
Main Authors: Jingting Liu, Daniel Verscharen, Jesse Coburn, Georgios Nicolaou, Xiangyu Wu, Wence Jiang, Oreste Pezzi, Francesco Pucci, Matteo Zuin, Christopher J. Owen, Hamish Reid
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Subjects:
Solar wind
Space plasmas
Online Access:https://doi.org/10.3847/2041-8213/adea4f
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