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Statistical Properties of Alfvén Ion Cyclotron Waves and Kinetic Alfvén Waves in the Inner Heliosphere
作者姓名:Chang Sun  Lei Yang  Qiu-Huan Li  Cun-Li Dai  Jian-Ping Li  Zheng-Wei Cheng  De-Jin Wu
作者单位:1. Key Laboratory of Planetary Sciences, Purple Mountain Observatory, CAS;2. School of Astronomy and Space Sciences, University of Science and Technology of China;3. State Key Laboratory of Space Weather, National Space Science Center, CAS;4. Institute of Space Physics, Luoyang Normal University;5. Henan Key Laboratory of Electromagnetic Transformation and Detection, Luoyang Normal University;6. College of Sciences, Nanjing Agricultural University;7. Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, CAS
基金项目:supported in part by the National Natural Science Foundation of China (NSFC, grant Nos. 41874201, 12250014, 11790302, 42174195, and 11873018);;the Specialized Research Fund for State Key Laboratories;
摘    要:Alfvén ion cyclotron waves(ACWs) and kinetic Alfvén waves(KAWs) are found to exist at <0.3 au observed by Parker Solar Probe in Alfvénic slow solar winds. To examine the statistical properties of the background parameters for ACWs and KAWs and related wave disturbances, both wave events observed by Parker Solar Probe are selected and analyzed. The results show that there are obvious differences in the background and disturbance parameters between ACWs and KAWs. ACW events have a relatively hi...

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