Characterizing lunar 1 Hz whistler waves across a solar cycle using ARTEMIS observationsOA
Characterizing lunar 1 Hz whistler waves across a solar cycle using ARTEMIS observations
LongFei Jia;BinBin Ni;Song Fu;YueQun Lou;TaiFeng Jin;XiaoTong Yun;ShaoTing Cheng;ShuYue Pang;XiangYuan Tong;Xin Ma
School of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,ChinaSchool of Earth and Space Science and Technology,Wuhan University,Wuhan 430072,China
Moonwhistler wavessolar windstatistical analysissolar activity cycle
Moonwhistler wavessolar windstatistical analysissolar activity cycle
《地球与行星物理（英文）》 2026 (3)
385-399,15
This research was supported by the National Natural Science Foundation of China(Grant Nos.42474217,U2541290,42174188,42188101,42025404,42330207,and 42578015),the National Key R&D Program of China(Grant Nos.2022YFF0503700,2022YFF0503900,and 2025YFF0512500),the Fundamental Research Funds for the Central Universities(Grant No.242025kf0008),and the Natural Science Foundation of Hubei Province,China(Grant No.2025AFA030).We acknowledge K.H.Glassmeier,U.Auster,and W.Baumjohann for the use of FGM data and C.W.Carlson and J.P.McFadden for use of ESA data.All ARTEMIS data used are available at http://artemis.ssl.berkeley.edu.We further thank Lianghai Xie for providing the modeled lunarmagnetic field results.
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