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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...

Deskribapen osoa

Gorde:
Egile Nagusiak: Jingting Liu, Daniel Verscharen, Jesse Coburn, Georgios Nicolaou, Xiangyu Wu, Wence Jiang, Oreste Pezzi, Francesco Pucci, Matteo Zuin, Christopher J. Owen, Hamish Reid
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2025-01-01
Saila:The Astrophysical Journal Letters
Gaiak:
Solar wind
Space plasmas
Sarrera elektronikoa:https://doi.org/10.3847/2041-8213/adea4f
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