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Li JH, Zhou XZ, Liu ZY, Wang S, Omura Y, Li L, Yue C, Zong QG, Le G, Russell CT, Burch JL. Direct observations of cross-scale wave-particle energy transfer in space plasmas. SCIENCE ADVANCES 2025; 11:eadr8227. [PMID: 39919183 PMCID: PMC11804927 DOI: 10.1126/sciadv.adr8227] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/17/2024] [Accepted: 01/08/2025] [Indexed: 02/09/2025]
Abstract
The collisionless plasmas in space and astrophysical environments are intrinsically multiscale in nature, behaving as conducting fluids at macroscales and kinetically at microscales comparable to ion and/or electron gyroradii. A fundamental question in understanding the plasma dynamics is how energy is transported and dissipated across scales. Here, we present spacecraft measurements in the terrestrial foreshock, a region upstream of the bow shock where the solar wind population coexists with the reflected ions. In this region, the fluid-scale, ultralow-frequency waves resonate with the reflected ions to modify the velocity distributions, which in turn cause the growth of the ion-scale, magnetosonic-whistler waves. The latter waves then resonate with the electrons, and the accelerated electrons contribute to the excitation of electron-scale, high-frequency whistler waves. These observations demonstrate that the chain of wave-particle resonances is an efficient mechanism for cross-scale energy transfer, which could redistribute the kinetic energy and accelerate the particles upstream of the shocks.
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Affiliation(s)
- Jing-Huan Li
- School of Earth and Space Sciences, Peking University, Beijing, China
- State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China
- Swedish Institute of Space Physics, Uppsala, Sweden
| | - Xu-Zhi Zhou
- School of Earth and Space Sciences, Peking University, Beijing, China
| | - Zhi-Yang Liu
- Institut de Recherche en Astrophysique et Planetologie, CNES-CNRS, Universite Toulouse III, Paul Sabatier, Toulouse, France
| | - Shan Wang
- School of Earth and Space Sciences, Peking University, Beijing, China
| | - Yoshiharu Omura
- State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China
- Research Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japan
| | - Li Li
- School of Earth and Space Sciences, Peking University, Beijing, China
| | - Chao Yue
- School of Earth and Space Sciences, Peking University, Beijing, China
| | - Qiu-Gang Zong
- School of Earth and Space Sciences, Peking University, Beijing, China
- State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China
| | - Guan Le
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Christopher T. Russell
- Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA, USA
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Xie ZK, Zong QG, Yue C, Zhou XZ, Liu ZY, He JS, Hao YX, Ng CS, Zhang H, Yao ST, Pollock C, Le G, Ergun R, Lindqvist PA. Electron scale coherent structure as micro accelerator in the Earth's magnetosheath. Nat Commun 2024; 15:886. [PMID: 38286824 PMCID: PMC10824732 DOI: 10.1038/s41467-024-45040-5] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/19/2023] [Accepted: 01/10/2024] [Indexed: 01/31/2024] Open
Abstract
Turbulent energy dissipation is a fundamental process in plasma physics that has not been settled. It is generally believed that the turbulent energy is dissipated at electron scales leading to electron energization in magnetized plasmas. Here, we propose a micro accelerator which could transform electrons from isotropic distribution to trapped, and then to stream (Strahl) distribution. From the MMS observations of an electron-scale coherent structure in the dayside magnetosheath, we identify an electron flux enhancement region in this structure collocated with an increase of magnetic field strength, which is also closely associated with a non-zero parallel electric field. We propose a trapping model considering a field-aligned electric potential together with the mirror force. The results are consistent with the observed electron fluxes from ~50 eV to ~200 eV. It further demonstrates that bidirectional electron jets can be formed by the hourglass-like magnetic configuration of the structure.
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Affiliation(s)
- Zi-Kang Xie
- Institute of Space Physics and Applied Technology, Peking University, Beijing, 100871, China
| | - Qiu-Gang Zong
- Institute of Space Physics and Applied Technology, Peking University, Beijing, 100871, China.
- State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Taipa, Macau, China.
| | - Chao Yue
- Institute of Space Physics and Applied Technology, Peking University, Beijing, 100871, China
| | - Xu-Zhi Zhou
- Institute of Space Physics and Applied Technology, Peking University, Beijing, 100871, China
| | - Zhi-Yang Liu
- Institute of Space Physics and Applied Technology, Peking University, Beijing, 100871, China
| | - Jian-Sen He
- Institute of Space Physics and Applied Technology, Peking University, Beijing, 100871, China
| | - Yi-Xin Hao
- Max Planck Institute for Solar System Research, Göttingen, Germany
| | - Chung-Sang Ng
- Geophysical Institute, University of Alaska Fairbanks, Fairbanks, AK, USA
| | - Hui Zhang
- Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, 264209, China
| | - Shu-Tao Yao
- Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, 264209, China
| | - Craig Pollock
- Denali Scientific, 3771 Mariposa Lane, Fairbanks, AK, 99709, USA
| | - Guan Le
- Heliophysics Science Division, NASA, Goddard Space Flight Center, Greenbelt, MD, 20771, USA
| | - Robert Ergun
- Department of Astrophysical and Planetary Sciences, University of Colorado LASP, Boulder, CO, USA
| | - Per-Arne Lindqvist
- Department of Space and Plasma Physics, KTH Royal Institute of Technology, Stockholm, Sweden
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