Modeling the Dynamics of Radiation Belt Electrons With Source and Loss Driven by the Solar Wind-Reference-Cited by-同舟云学术

Modeling the Dynamics of Radiation Belt Electrons With Source and Loss Driven by the Solar Wind

Published:2021-05-27 Issue:6 Volume:126 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Xiang Zheng¹²^ORCID,Li Xinlin²³^ORCID,Kapali Sudha⁴,Gannon Jennifer⁴^ORCID,Ni Binbin¹⁵^ORCID,Zhao Hong²⁶^ORCID,Zhang Kun²³⁷^ORCID,Khoo Leng Ying²³^ORCID

Affiliation:

1. Department of Space Physics School of Electronic Information Wuhan University Wuhan Hubei China

2. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA

3. Department of Aerospace Engineering Sciences University of Colorado Boulder Boulder CO USA

4. Computational Physics, Inc. Boulder Colorado USA

5. CAS Center for Excellence in Comparative Planetology Hefei Anhui China

6. Physics Department Auburn University Auburn AL USA

7. Space Science Institute Boulder CO USA

Funder

National Science Foundation

National Aeronautics and Space Administration

National Natural Science Foundation of China

China Postdoctoral Science Foundation

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA028988

Reference71 articles.

1. Electron scattering loss in Earth's inner magnetosphere: 1. Dominant physical processes

2. Baker D. N.(2001). Satellite anomalies due to space storms. InSpace storms and space weather hazards(pp. 285–311). Springer.https://doi.org/10.1007/978-94-010-0983-6_11

3. Disturbed space environment may have been related to pager satellite failure

4. The Relativistic Electron-Proton Telescope (REPT) Instrument on Board the Radiation Belt Storm Probes (RBSP) Spacecraft: Characterization of Earth’s Radiation Belt High-Energy Particle Populations

5. Coronal mass ejections, magnetic clouds, and relativistic magnetospheric electron events: ISTP

Cited by 15 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Influences of Solar Wind Parameters on Energetic Electron Fluxes at Geosynchronous Orbit Revealed by the Deep SHAP Method;Space Weather;2024-06

2. Statistical Analysis of Distributions of Electron Energy Spectra in the Earth’s Radiation Belts Based on Van Allen Probes Observations;Chinese Journal of Space Science;2024

3. Observations of different populations of radiation belt electrons by FengYun 3C: An analysis of the 17 March 2015 geomagnetic storm event;CHINESE J GEOPHYS-CH;2023

4. Three‐Dimensional Simulations of Ultra‐Relativistic Electron Acceleration During the 21 April 2017 Storm;Journal of Geophysical Research: Space Physics;2023-04

5. Prediction of geosynchronous electron fluxes using an artificial neural network driven by solar wind parameters;Advances in Space Research;2023-01