Extended Cyclotron Resonant Heating of the Turbulent Solar Wind

Extended Cyclotron Resonant Heating of the Turbulent Solar Wind

Circularly polarized, nearly parallel propagating waves are prevalent in the solar wind at ion-kinetic scales. At these scales, the spectrum of turbulent fluctuations in the solar wind steepens, often called the transition range, before flattening at sub-ion scales. Circularly polarized waves have b...

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Bibliographic Details
Main Authors: Trevor A. Bowen, Ivan Y. Vasko, Stuart D. Bale, Benjamin D. G. Chandran, Alexandros Chasapis, Thierry Dudok de Wit, Alfred Mallet, Michael McManus, Romain Meyrand, Marc Pulupa, Jonathan Squire
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Letters
Subjects:
Plasma astrophysics
Space plasmas
Plasma physics
Interplanetary turbulence
Solar wind
Fast solar wind
Online Access:https://doi.org/10.3847/2041-8213/ad6b2e

Internet

https://doi.org/10.3847/2041-8213/ad6b2e

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