Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind

Ion cyclotron waves (ICWs) are prevalent in the near-Sun solar wind and play a significant role in the nonadiabatic heating of plasma. Recent observations from the Parker Solar Probe have revealed the simultaneous presence of antisunward and sunward ICWs in the vicinity of the Alfvén surface. Howeve...

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Main Authors: Yifan Wu, Chen Shi, Xin Tao, Jinsong Zhao
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adbc6a
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author Yifan Wu
Chen Shi
Xin Tao
Jinsong Zhao
author_facet Yifan Wu
Chen Shi
Xin Tao
Jinsong Zhao
author_sort Yifan Wu
collection DOAJ
description Ion cyclotron waves (ICWs) are prevalent in the near-Sun solar wind and play a significant role in the nonadiabatic heating of plasma. Recent observations from the Parker Solar Probe have revealed the simultaneous presence of antisunward and sunward ICWs in the vicinity of the Alfvén surface. However, single-satellite observations cannot effectively trace the generation and evolution of these observed waves. To address this limitation, we employ kinetic-hybrid simulations to replicate the generation and evolution of counterpropagating ICWs under typical plasma conditions in the near-Sun solar wind. Following the linear growth phase, the simulated waves exhibit amplitude and polarization characteristics that closely match the observations. Additionally, our simulation illustrates proton scattering induced by the counterpropagating waves. These results underscore the significance of locally generated ICWs in influencing solar wind ion dynamics.
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series The Astrophysical Journal
spelling doaj-art-e297f8fd27bf474c9864b2c0658b607a2025-08-20T03:08:20ZengIOP PublishingThe Astrophysical Journal1538-43572025-01-01983210710.3847/1538-4357/adbc6aKinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar WindYifan Wu0https://orcid.org/0000-0002-2039-0590Chen Shi1https://orcid.org/0000-0002-9166-1036Xin Tao2https://orcid.org/0000-0002-4676-8133Jinsong Zhao3https://orcid.org/0000-0002-3859-6394CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China , Hefei, People’s Republic of China ; xtao@ustc.edu.cn; CAS Center for Excellence in Comparative Planetology , Hefei, People’s Republic of ChinaSchool of Physics and Electronic Sciences, Changsha University of Science and Technology , Changsha, People’s Republic of ChinaCAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China , Hefei, People’s Republic of China ; xtao@ustc.edu.cn; CAS Center for Excellence in Comparative Planetology , Hefei, People’s Republic of ChinaPurple Mountain Observatory, Chinese Academy of Sciences , Nanjing, People’s Republic of China ; js_zhao@pmo.ac.cn; School of Astronomy and Space Science, University of Science and Technology of China , Hefei, People’s Republic of ChinaIon cyclotron waves (ICWs) are prevalent in the near-Sun solar wind and play a significant role in the nonadiabatic heating of plasma. Recent observations from the Parker Solar Probe have revealed the simultaneous presence of antisunward and sunward ICWs in the vicinity of the Alfvén surface. However, single-satellite observations cannot effectively trace the generation and evolution of these observed waves. To address this limitation, we employ kinetic-hybrid simulations to replicate the generation and evolution of counterpropagating ICWs under typical plasma conditions in the near-Sun solar wind. Following the linear growth phase, the simulated waves exhibit amplitude and polarization characteristics that closely match the observations. Additionally, our simulation illustrates proton scattering induced by the counterpropagating waves. These results underscore the significance of locally generated ICWs in influencing solar wind ion dynamics.https://doi.org/10.3847/1538-4357/adbc6aSolar windPlasma physicsSpace plasmas
spellingShingle Yifan Wu
Chen Shi
Xin Tao
Jinsong Zhao
Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind
The Astrophysical Journal
Solar wind
Plasma physics
Space plasmas
title Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind
title_full Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind
title_fullStr Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind
title_full_unstemmed Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind
title_short Kinetic-hybrid Simulations of Counterpropagating Ion Cyclotron Waves and Proton Scattering in the Near-Sun Solar Wind
title_sort kinetic hybrid simulations of counterpropagating ion cyclotron waves and proton scattering in the near sun solar wind
topic Solar wind
Plasma physics
Space plasmas
url https://doi.org/10.3847/1538-4357/adbc6a
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AT chenshi kinetichybridsimulationsofcounterpropagatingioncyclotronwavesandprotonscatteringinthenearsunsolarwind
AT xintao kinetichybridsimulationsofcounterpropagatingioncyclotronwavesandprotonscatteringinthenearsunsolarwind
AT jinsongzhao kinetichybridsimulationsofcounterpropagatingioncyclotronwavesandprotonscatteringinthenearsunsolarwind