Cold Plasmaspheric Electrons Affected by ULF Waves in the Inner Magnetosphere: A Van Allen Probes Statistical Study
Abstract
Six years of Van Allen Probes data are used to investigate cold plasmaspheric electrons affected by ultralow-frequency (ULF) waves in the inner magnetosphere (L<7) including spatial distributions, occurrence conditions, and resonant energy range. Events exhibit a global distribution within L= 4–7 but preferentially occur at L~5.5–7 in the dayside, while there is higher occurrence rate in the duskside than dawnside. They can occur under different geomagnetic activities and solar wind velocities (VS), but the occurrence rates are increasing with larger AE, |SYMH|, and VS. These features are closely associated with the generation and propagation of ULF waves in Pc4 (45–150 s) and Pc5 (150–600 s) bands. Combined with electron observations from HOPE instrument, the resonant energies inferred from wave power indicate that cold electrons at ones to hundreds of electron volts can be affected by ULF waves. Finally, this study may shed new light on further investigations on the acceleration and transportation of cold plasmaspheric particles that would affect plasmaspheric material release to the Earth's magnetosphere and instabilities for exciting various waves.
- Authors:
-
- Peking Univ., Beijing (China)
- Univ. of New Hampshire, Durham, NH (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Univ. of Minnesota, Minneapolis, MN (United States)
- Univ. of Alberta, Edmonton, AB (Canada)
- Publication Date:
- Research Org.:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Org.:
- USDOE; National Aeronautics and Space Administration (NASA); National Postdoctoral Program for Innovative Talents; China Postdoctoral Science Foundation; National Natural Science Foundation of China (NSFC)
- OSTI Identifier:
- 1818105
- Report Number(s):
- LA-UR-20-20738
Journal ID: ISSN 2169-9380; TRN: US2213917
- Grant/Contract Number:
- 89233218CNA000001; BX20180002; 41904145; 41421003; 41627805; NAS5-01072
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Journal of Geophysical Research. Space Physics
- Additional Journal Information:
- Journal Volume: 124; Journal Issue: 10; Journal ID: ISSN 2169-9380
- Publisher:
- American Geophysical Union
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cold plasmaspheric electrons; ULF waves; wave-particle interaction; drift-bounce resonance
Citation Formats
Ren, Jie, Zong, Q. G., Zhou, X. Z., Spence, H. E., Funsten, H. O., Wygant, J. R., and Rankin, R. Cold Plasmaspheric Electrons Affected by ULF Waves in the Inner Magnetosphere: A Van Allen Probes Statistical Study. United States: N. p., 2019.
Web. doi:10.1029/2019ja027009.
Ren, Jie, Zong, Q. G., Zhou, X. Z., Spence, H. E., Funsten, H. O., Wygant, J. R., & Rankin, R. Cold Plasmaspheric Electrons Affected by ULF Waves in the Inner Magnetosphere: A Van Allen Probes Statistical Study. United States. https://doi.org/10.1029/2019ja027009
Ren, Jie, Zong, Q. G., Zhou, X. Z., Spence, H. E., Funsten, H. O., Wygant, J. R., and Rankin, R. Wed .
"Cold Plasmaspheric Electrons Affected by ULF Waves in the Inner Magnetosphere: A Van Allen Probes Statistical Study". United States. https://doi.org/10.1029/2019ja027009. https://www.osti.gov/servlets/purl/1818105.
@article{osti_1818105,
title = {Cold Plasmaspheric Electrons Affected by ULF Waves in the Inner Magnetosphere: A Van Allen Probes Statistical Study},
author = {Ren, Jie and Zong, Q. G. and Zhou, X. Z. and Spence, H. E. and Funsten, H. O. and Wygant, J. R. and Rankin, R.},
abstractNote = {Six years of Van Allen Probes data are used to investigate cold plasmaspheric electrons affected by ultralow-frequency (ULF) waves in the inner magnetosphere (L<7) including spatial distributions, occurrence conditions, and resonant energy range. Events exhibit a global distribution within L= 4–7 but preferentially occur at L~5.5–7 in the dayside, while there is higher occurrence rate in the duskside than dawnside. They can occur under different geomagnetic activities and solar wind velocities (VS), but the occurrence rates are increasing with larger AE, |SYMH|, and VS. These features are closely associated with the generation and propagation of ULF waves in Pc4 (45–150 s) and Pc5 (150–600 s) bands. Combined with electron observations from HOPE instrument, the resonant energies inferred from wave power indicate that cold electrons at ones to hundreds of electron volts can be affected by ULF waves. Finally, this study may shed new light on further investigations on the acceleration and transportation of cold plasmaspheric particles that would affect plasmaspheric material release to the Earth's magnetosphere and instabilities for exciting various waves.},
doi = {10.1029/2019ja027009},
journal = {Journal of Geophysical Research. Space Physics},
number = 10,
volume = 124,
place = {United States},
year = {Wed Oct 23 00:00:00 EDT 2019},
month = {Wed Oct 23 00:00:00 EDT 2019}
}
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