Direct observations of cross-scale wave-particle energy transfer in space plasmas

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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Publication Details

Journal
Science Advances
Published
2025-02-07
DOI
https://doi.org/10.1126/sciadv.adr8227
Citations
9
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
10.39
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article

Direct observations of cross-scale wave-particle energy transfer in space plasmas

C. T. Russell, J. L. Burch, Jing‐Huan Li, Chao Yue et al.
9 citations
Science Advances
Ionosphere and magnetosphere dynamics
10.39
article

Direct observations of cross-scale wave-particle energy transfer in space plasmas

C. T. Russell, J. L. Burch, Jing‐Huan Li, Chao Yue, Xu‐Zhi Zhou, Qiugang Zong, Zhi‐Yang Liu, Yoshiharu Omura, G. Le, Li Li, Shan Wang
article en
9 citations

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.

Science AdvancesVol. 11(6)
Macau University of Science and Technology (MO), Southwest Research Institute (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), Goddard Space Flight Center (US), Swedish Institute of Space Physics (SE), Université Toulouse III - Paul Sabatier (FR), University of California, Los Angeles (US), Peking University (CN), Kyoto University (JP), Institut de Recherche en Astrophysique et Planétologie (FR)
Affordable and clean energy
Openalex Percentile: Top 2%
Ionosphere and magnetosphere dynamics
10.39
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