Japan Geoscience Union Meeting 2021

Presentation information

[E] Poster

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM12] Dynamics of the Inner Magnetospheric System

Sat. Jun 5, 2021 5:15 PM - 6:30 PM Ch.04

convener:Kunihiro Keika(Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo), Yoshizumi Miyoshi(Institute for Space-Earth Environmental Research, Nagoya University), W Lauren Blum(University of Colorado Boulder), Yuri Shprits(Helmholtz Centre Potsdam GFZ German Research Centre for Geosciences)

5:15 PM - 6:30 PM

[PEM12-P05] Global characteristics of cold protons in the near-Earth magnetotail: MMS/HPCA observations

*Kunihiro Keika1, Masahiro Hoshino1, Ryuta Asami1 (1.Graduate School of Science, The University of Tokyo )

Keywords:plasma transport in the magnetosphere, origin of plasma sheet populations, two-component plasma

We conduct a statistical study of cold protons in the near-Earth magnetotail under quiet magnetotail conditions. Performing two-component Maxwellian fits to velocity distributions, we extract densities and temperatures of cold protons. Cold protons are separated into three distinct populations in the density-plasma b space. We interpret that Population I, characterized by a positive correlation of density to b, is solar-wind origin plasma transported over the polar regions. Population II, seen only in the high-b (>0.1) and tailward region (r > 20 Re) particularly on the dusk side, is solar-wind origin plasma entering through the flank magnetopauses and remains cold. Population III, clearly identified in the near-Earth region (r < 10 Re), is of ionospheric origin. The results also suggest that plasma supply to the plasma sheet is dominated by Population I and that cold plasma in the near-Earth magnetotail is mostly of ionospheric origin.