EGU2020-4003
https://doi.org/10.5194/egusphere-egu2020-4003
EGU General Assembly 2020
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Roles of electrons and ions in formation of the current in mirror mode structures in the terrestrial plasma sheet: MMS observations

Guoqiang Wang1, Tielong Zhang1, Mingyu Wu1, Daniel Schmid2, Yufei Hao3, Zonghao Pan4, and Martin Volwerk2
Guoqiang Wang et al.
  • 1Harbin Institute of Technology (Shenzhen), Shenzhen, China
  • 2Space Research Institute, Austrian Academy of Sciences, Graz, Austria
  • 3Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
  • 4CAS Key Laboratory of Geospace Environment, University of Science and Technology of China, Hefei, China

Currents are believed to exist in mirror mode structures and to be self-consistent with the magnetic field depression. Here, we investigate a train of mirror mode structures in the terrestrial plasma sheet on 11 August 2017 measured by the Magnetospheric Multiscale mission. We find that bipolar current densities exist in the cross-section of two hole-like mirror mode structures, referred to as magnetic dips. The bipolar current in the magnetic dip with a size of ~2.2 ρi (the ion gyro radius) is mainly contributed by variations of the electron velocity, which is mainly formed by the magnetic gradient-curvature drift. For another magnetic dip with a size of ~6.6 ρi, the bipolar current is mainly caused by an ion bipolar velocity, which can be explained by the collective behaviors of the ion drift motions. These observations suggest that the electrons and ions play different roles in the formation of currents in magnetic dips with different sizes.

How to cite: Wang, G., Zhang, T., Wu, M., Schmid, D., Hao, Y., Pan, Z., and Volwerk, M.: Roles of electrons and ions in formation of the current in mirror mode structures in the terrestrial plasma sheet: MMS observations, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-4003, https://doi.org/10.5194/egusphere-egu2020-4003, 2020