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The Composition of Plasma inside Geostationary Orbit Based on Van Allen Probes Observations
Author(s) -
Yue Chao,
Bortnik Jacob,
Li Wen,
Ma Qianli,
Gkioulidou Matina,
Reeves Geoffrey D.,
Wang ChihPing,
Thorne Richard M.,
Lui Anthony T. Y.,
Gerrard Andrew J.,
Spence Harlan E.,
Mitchell Donald G.
Publication year - 2018
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1029/2018ja025344
Subject(s) - plasmasphere , electrojet , atomic physics , ring current , physics , van allen probes , van allen radiation belt , magnetosphere , ion , plasma , electron , helium , geostationary orbit , earth's magnetic field , magnetic field , astronomy , nuclear physics , satellite , quantum mechanics
The composition of the inner magnetosphere is of great importance for determining the plasma pressure and thus the currents and magnetic field configuration. In this study, we perform a statistical survey of equatorial plasma pressure distributions and investigate the relative contributions of ions and electron with different energies inside of geostationary orbit under two auroral electrojet levels based on over 60 months of observations from the Helium, Oxygen, Proton, and Electron and Radiation Belt Storm Probes Ion Composition Experiment mass spectrometers onboard Van Allen Probes. We find that the total and partial pressures of different species increase significantly at high auroral electrojet levels with hydrogen pressure being dominant in the plasmasphere. The pressures of the heavy ions and electrons increase outside the plasmapause and develop a strong dawn‐dusk asymmetry with ion pressures peaking at dusk and electron pressure peaking at dawn. In addition, ring current hydrogen with energies ranging from 50 keV up to several hundred keV is the dominant component of plasma pressure during both quiet (>90%) and active times (>60%), while oxygen with 10 < E < 50 keV and electrons with 0.1 < E < 40 keV become important during active times contributing more than 25% and 20% on the nightside, respectively, while the helium contribution is generally small. The results presented in this study provide a global picture of the equatorial plasma pressure distributions and the associated contributions from different species with different energy ranges, which advance our knowledge of wave generation and provide models with a systematic baseline of plasma composition.