EGU24-2562, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-2562
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Banana Current in the Inner Magnetosphere Observed by Van Allen Probes

Xiao-Xin Zhang1, Tonghui Wang1, Fei He2, Jingtian Lv1, Qiugang Zong3, and Huishan Fu4
Xiao-Xin Zhang et al.
  • 1National Satellite Meteorological Center, CMA, Beijing, China (xxzhang@cma.gov.cn)
  • 2Institute of Geology and Geophysics, Chinese Academy of Sciences
  • 3Peking University
  • 4Beihang University

By using the magnetic field data from Van Allen Probes, we analyzed the distribution characteristics of the electromagnetic environment in the inner magnetosphere on different Dst* index and magnetic local time. Our results show that for the response of different current systems, the dawn-dusk and noon-midnight asymmetry distribution of the residual magnetic field δB increases with Dst* index. When Dst* < −60 nT, a “banana”-shaped geomagnetic field negative disturbance peak region appears in the sector from midnight to dusk. Then, we obtained the azimuthal current density and found the asymmetric internal eastward and external westward ring current. Through the vector analysis of three-dimensional current density, the current density vector distribution in the magnetic equatorial plane is completely displayed for the first time, which directly proves the existence of banana current near r = 3.0–4.0 RE during strong geomagnetic storms.

How to cite: Zhang, X.-X., Wang, T., He, F., Lv, J., Zong, Q., and Fu, H.: Banana Current in the Inner Magnetosphere Observed by Van Allen Probes, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-2562, https://doi.org/10.5194/egusphere-egu24-2562, 2024.