Survey of radiation belt energetic electron pitch angle distributions based on the Van Allen Probes MagEIS measurements-Reference-Cited by-同舟云学术

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Survey of radiation belt energetic electron pitch angle distributions based on the Van Allen Probes MagEIS measurements

Published:2016-02 Issue:2 Volume:121 Page:1078-1090
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Shi Run¹,Summers Danny¹,Ni Binbin²,Fennell Joseph F.³,Blake J. Bernard³,Spence Harlan E.⁴,Reeves Geoffrey D.⁵

Affiliation:

1. Department of Mathematics and StatisticsMemorial University of Newfoundland St. John's Newfoundland and Labrador Canada

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

3. Space Science Applications LaboratoryAerospace Corporation El Segundo California USA

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

5. Los Alamos National Laboratory Los Alamos New Mexico USA

Funder

Natural Sciences and Engineering Research Council of Canada

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021724

Reference44 articles.

1. The Magnetic Electron Ion Spectrometer (MagEIS) Instruments Aboard the Radiation Belt Storm Probes (RBSP) Spacecraft

2. Pitch angle distributions of energetic electrons at Saturn

3. An ISEE/whistler model of equatorial electron density in the magnetosphere

4. REPAD: An empirical model of pitch angle distributions for energetic electrons in the Earth's outer radiation belt

5. Van Allen Probes show that the inner radiation zone contains no MeV electrons: ECT/MagEIS data

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1. Variability of energetic proton flux and pitch angle distributions in the Earth's radiation belt modulated by geomagnetic storms;Physics of Fluids;2024-08-01

2. A New Model of Electron Pitch Angle Distributions and Loss Timescales in the Earth's Radiation Belts;Journal of Geophysical Research: Space Physics;2024-06

3. Chorus wave power at the strong diffusion limit overcomes electron losses due to strong diffusion;Nature Communications;2024-02-27

4. Why can the auroral-type sporadic E layer be detected over the South America Magnetic Anomaly (SAMA) region? An investigation of a case study under the influence of the high-speed solar wind stream;Frontiers in Astronomy and Space Sciences;2023-11-23

5. Comparison of radiation belt electron fluxes simultaneously measured with PROBA-V/EPT and RBSP/MagEIS instruments;Annales Geophysicae;2023-08-17

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