Radial Distribution of Electron Quasi-thermal Noise in the Inner Heliosphere

Radial Distribution of Electron Quasi-thermal Noise in the Inner Heliosphere

The electron population in the solar wind plasma can be described with three different components: a core, a halo, and a magnetic field aligned strahl. The electron quasi-thermal noise (QTN) is investigated by using an electron population model consisting of a core with a Maxwellian distribution and...

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Bibliographic Details
Main Authors: Yi-Lun Li, Ling Chen, De-Jin Wu
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Solar wind
Interplanetary physics
Space plasmas
Online Access:https://doi.org/10.3847/1538-4357/ad85d6
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