EGU22-1678
https://doi.org/10.5194/egusphere-egu22-1678
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Simultaneous Generation of EMIC and MS Waves During the Magnetic Dip in the Inner Magnetosphere

Zheng Huang, Zhigang Yuan, Xiongdong Yu, Zuxiang Xue, and Zhihai Ouyang
Zheng Huang et al.
  • Wuhan University, Wuhan, China (zhenghuang@whu.edu.cn)

The Van Allen Probe B satellite simultaneously observed electromagnetic ion cyclotron (EMIC) and fast magnetosonic (MS) waves in a magnetic dip on April 29, 2017. During the magnetic dip, we found the coexistence of flux enhancements of ring current protons (∼11.2–∼51.7 keV) and flux reductions of relativistic electrons (∼1 MeV), which are identified as typical signatures of a magnetic dip in the inner magnetosphere. Based on linear theoretical calculations and observational analysis, the observed ring current protons show an anisotropic temperature distribution and partial shell distribution for different energies during the magnetic dip to provide free energies for the generation of EMIC and MS waves, respectively. Our findings indicate that the complex unstable distribution in the velocity phase space of ring current protons during the magnetic dip can trigger the simultaneous generation of EMIC and MS waves in the inner magnetosphere.

How to cite: Huang, Z., Yuan, Z., Yu, X., Xue, Z., and Ouyang, Z.: Simultaneous Generation of EMIC and MS Waves During the Magnetic Dip in the Inner Magnetosphere, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-1678, https://doi.org/10.5194/egusphere-egu22-1678, 2022.