The Densities and Compositions of Background Cold Ions Based on the Van Allen Probe Observations

Author:

Yue Chao1ORCID,Li Yuxuan1ORCID,Kistler Lynn2ORCID,Ma Qianli34ORCID,Fu Haobo1ORCID,Reeves Geoffrey D.56,Zhou Xuzhi1,Zong Qiugang1ORCID,Spence Harlan E.2ORCID

Affiliation:

1. Institute of Space Physics and Applied Technology Peking University Beijing China

2. Institute for the Study of Earth, Oceans, and Space University of New Hampshire Durham NH USA

3. Department of Atmospheric and Oceanic Sciences University of California, Los Angeles Los Angeles CA USA

4. Center for Space Physics Boston University Boston MA USA

5. Space Science and Applications Group Los Alamos National Laboratory Los Alamos NM USA

6. Space Sciences Division at the New Mexico Consortium Los Alamos NM USA

Abstract

AbstractThe cold ions, which are generally “invisible” to most instruments, have strong impacts on plasma wave and magnetic reconnection. Under particular situations, these cold ions could be accelerated and thus become detectable. In this study, we statistically investigated the properties of background cold ions based on Van Allen Probe observations. The cold ions could often be detected near the dusk sector, and a clear dawn‐dusk asymmetry is observed for all ion species with higher density at the dusk side, showing plasmaspheric plume‐like structures. Similar to the cold electrons, cold proton ions show a clear boundary of plasmapause with its location moving toward the Earth as geomagnetic activity increases. Furthermore, the percentage of oxygen increases, and the percentage of protons decreases as geomagnetic activity increases whereas the helium composition is generally small. Our results provide important information on ion compositions for the understanding of cold‐plasma dynamics in the inner magnetosphere.

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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