Observational Features of Charge distribution in Earth’s Inner Magnetosphere

Author:

Gao Lai1ORCID,Zhou Yufei1ORCID,Ji Yong1,Pu Zuyin2,Parks George3,Russell Christopher4,Zeng Gang5,Ma Lan1,Torbert Roy6ORCID,Yang Yanyan7,Burch James8ORCID,Shen Chao1

Affiliation:

1. School of Science, Harbin Institute of Technology

2. Peking University

3. University of California, Berkeley

4. University of California, Los Angeles

5. School of Mathematics and Physics, Jingchu University of Technology

6. University of New Hampshire

7. Institute of Crustal Dynamics, China Earthquake Administration

8. Southwest Research Institute

Abstract

Abstract Understanding the motion of charged particles in the electromagnetic field in the inner magnetosphere is essential for space science and space weather. Charge accumulation can occur due to the dipole magnetic and convective electric fields in this region. However, until the recent MMS mission, there were few means to detect charge distribution in situ. We report unambiguous in situ observation of the spatial distribution of the excess charge density in the inner magnetosphere by the magnetospheric multiscale (MMS) mission. We find that a positive (negative) charge accumulates in the dusk (dawn) side inner magnetospheres, which is contrary to the long assumed overall quasi-neutrality of space plasma. These observations and results offer insight into magnetosphere–ionosphere coupling.

Publisher

Research Square Platform LLC

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