Simultaneous macroscale and microscale wave–ion interaction in near-earth space plasmas

Z.-Y. Liu, Q.-G. Zong (), R. Rankin, H. Zhang, Y. F. Wang, X.-Z. Zhou, S.-Y. Fu, C. Yue, X.-Y. Zhu, C. J. Pollock, S. A. Fuselier and G. Le
Additional contact information
Z.-Y. Liu: Peking University
Q.-G. Zong: Peking University
R. Rankin: University of Alberta
H. Zhang: University of Alaska Fairbanks
Y. F. Wang: Peking University
X.-Z. Zhou: Peking University
S.-Y. Fu: Peking University
C. Yue: Peking University
X.-Y. Zhu: Peking University
C. J. Pollock: Denali Scientific
S. A. Fuselier: Southwest Research Institute
G. Le: NASA Goddard Space Flight Center

Nature Communications, 2022, vol. 13, issue 1, 1-9

Abstract: Abstract Identifying how energy transfer proceeds from macroscales down to microscales in collisionless plasmas is at the forefront of astrophysics and space physics. It provides information on the evolution of involved plasma systems and the generation of high-energy particles in the universe. Here we report two cross-scale energy-transfer events observed by NASA’s Magnetospheric Multiscale spacecraft in Earth’s magnetosphere. In these events, hot ions simultaneously undergo interactions with macroscale (~ $${10}^{5}$$ 10 5 km) ultra-low-frequency waves and microscale ( $$\sim {10}^{3}$$ ~ 10 3 km) electromagnetic-ion-cyclotron (EMIC) waves. The cross-scale interactions cause energy to directly transfer from macroscales to microscales, and finally dissipate at microscales via EMIC-wave-induced ion energization. The direct measurements of the energy transfer rate in the second event confirm the efficiency of this cross-scale transfer process, whose timescale is estimated to be roughly ten EMIC-wave periods about (1 min). Therefore, these observations experimentally demonstrate that simultaneous macroscale and microscale wave-ion interactions provide an efficient mechanism for cross-scale energy transfer and plasma energization in astrophysical and space plasmas.

Date: 2022
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DOI: 10.1038/s41467-022-33298-6

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