Evolution of Pitch Angle Distributions of Relativistic Electrons During Geomagnetic Storms: Van Allen Probes Observations
Author:
Affiliation:
1. NASA Goddard Space Flight Center Greenbelt MD USA
2. Space Science Institute Fort Atkinson WI USA
3. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JA028335
Reference66 articles.
1. 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
2. High-Resolution Energetic Particle Measurements at 6.6 RE, 3. Low-Energy Electron Anisotropies and Short-Term Substorm Predictions
3. Gradual diffusion and punctuated phase space density enhancements of highly relativistic electrons: Van Allen Probes observations
4. A Long-Lived Relativistic Electron Storage Ring Embedded in Earth’s Outer Van Allen Belt
5. The outer radiation belt response to the storm time development of seed electrons and chorus wave activity during CME and CIR driven storms;Bingham S. T.;Journal of Geophysical Research: Space Physics,2018
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1. Persistent Pitch Angle Anisotropies of Relativistic Electrons in the Outer Radiation Belts;Journal of Geophysical Research: Space Physics;2023-12-26
2. Statistical investigation on equatorial pitch angle distribution of energetic electrons in Earth’s outer radiation belt during CME- and CIR-driven storms;Frontiers in Astronomy and Space Sciences;2022-08-30
3. Differentiating Between the Leading Processes for Electron Radiation Belt Acceleration;Frontiers in Astronomy and Space Sciences;2022-06-13
4. Storm-Time Evolution of the Equatorial Electron Pitch Angle Distributions in Earth’s Outer Radiation Belt;Frontiers in Astronomy and Space Sciences;2022-03-23
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