Variability of the pitch angle distribution of radiation belt ultrarelativistic electrons during and following intense geomagnetic storms: Van Allen Probes observations-Reference-Cited by-同舟云学术

Variability of the pitch angle distribution of radiation belt ultrarelativistic electrons during and following intense geomagnetic storms: Van Allen Probes observations

Published:2015-06 Issue:6 Volume:120 Page:4863-4876
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Ni Binbin¹²,Zou Zhengyang¹^ORCID,Gu Xudong¹,Zhou Chen¹,Thorne Richard M.³,Bortnik Jacob³,Shi Run¹,Zhao Zhengyu¹,Baker Daniel N.⁴,Kanekal Shrikhanth G.⁵,Spence Harlan E.⁶,Reeves Geoffrey D.⁷^ORCID,Li Xinlin⁴

Affiliation:

1. Department of Space Physics, School of Electronic InformationWuhan University Wuhan China

2. State Key Laboratory of Space WeatherChinese Academy of Sciences Beijing China

3. Department of Atmospheric and Oceanic SciencesUniversity of California Los Angeles California USA

4. Laboratory for Atmospheric and Space PhysicsUniversity of Colorado Boulder Boulder Colorado USA

5. NASA Goddard Space Flight Center Greenbelt Maryland USA

6. Institute for the Study of Earth, Oceans, and SpaceUniversity of New Hampshire Durham New Hampshire USA

7. Space Science and Applications GroupLos Alamos National Laboratory Los Alamos New Mexico USA

Funder

NSFC

Fundamental Research Funds for the Central Universities

JHU/APL

NASA's

ECT

NASA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021065

Reference48 articles.

1. Electron scattering loss in Earth's inner magnetosphere: 2. Sensitivity to model parameters

2. A Long-Lived Relativistic Electron Storage Ring Embedded in Earth’s Outer Van Allen Belt

3. 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

4. Gradual diffusion and punctuated phase space density enhancements of highly relativistic electrons: Van Allen Probes observations

5. An impenetrable barrier to ultrarelativistic electrons in the Van Allen radiation belts

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