EGU2020-8731, updated on 09 Jan 2024
https://doi.org/10.5194/egusphere-egu2020-8731
EGU General Assembly 2020
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Observations of Plasma Waves in the Multiple X-line Reconnection at the Magnetopause

Zhihong Zhong1,2, Daniel B. Graham2, Yuri V. Khotyaintsev2, Meng Zhou1, Rongxin Tang1, and Xiaohua Deng1
Zhihong Zhong et al.
  • 1Nanchang University, Nanchang, China
  • 2Swedish Institute of Space Physics, Uppsala, Sweden

Plasma waves are one of the important products of the magnetic reconnection process.  Plasma waves can produce particle heating, diffusion, and anomalous effects, which can potentially affect magnetic reconnection. We investigate the evolution and properties of plasma waves during a multiple X-line reconnection event at the magnetopause using measurements from the Magnetospheric Multiscale (MMS) mission. Both whistler waves and large-amplitude electrostatic waves were observed around the reconnecting current sheet. In these regions, the electron velocity distribution functions consist of a combination of a cold beam at low energies with an anisotropic population or a loss-cone at high energies. The electrostatic waves corresponded to regions where the cold beams are accelerated, while the whistlers corresponded to regions with significant anisotropies or loss cones. When the cold beams were accelerated to higher energies, the whistlers disappeared since the anisotropy or loss-cone distributions became less apparent. These results present the detailed evolution of the plasma waves reflecting the electron dynamics during magnetic reconnection.

How to cite: Zhong, Z., Graham, D. B., Khotyaintsev, Y. V., Zhou, M., Tang, R., and Deng, X.: Observations of Plasma Waves in the Multiple X-line Reconnection at the Magnetopause, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-8731, https://doi.org/10.5194/egusphere-egu2020-8731, 2020.

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