Source and seed populations for relativistic electrons: Their roles in radiation belt changes-Reference-Cited by-同舟云学术

Source and seed populations for relativistic electrons: Their roles in radiation belt changes

Published:2015-09 Issue:9 Volume:120 Page:7240-7254
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Jaynes A. N.¹,Baker D. N.¹,Singer H. J.²,Rodriguez J. V.³⁴^ORCID,Loto'aniu T. M.³⁴,Ali A. F.¹^ORCID,Elkington S. R.¹,Li X.¹,Kanekal S. G.⁵,Claudepierre S. G.⁶,Fennell J. F.⁶,Li W.⁷,Thorne R. M.⁷,Kletzing C. A.⁸,Spence H. E.⁹,Reeves G. D.¹⁰^ORCID

Affiliation:

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

2. NOAA Space Weather Prediction Center Boulder Colorado USA

3. Cooperative Institute for Research in Environmental SciencesUniversity of Colorado Boulder Boulder Colorado USA

4. NOAA National Centers for Environmental Information Boulder Colorado USA

5. NASA Goddard Space Flight Center Greenbelt Maryland USA

6. Space Sciences DepartmentAerospace Corporation Los Angeles California USA

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

8. Department of Physics and AstronomyUniversity of Iowa Iowa City Iowa USA

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

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

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2015JA021234

Reference63 articles.

1. Do Jovian electrons influence the terrestrial outer radiation zone?

2. Highly relativistic electrons in the Earth's outer magnetosphere: 1. Lifetimes and temporal history 1979–1984

3. Linear prediction filter analysis of relativistic electron properties at 6.6RE

4. Neutral line model of substorms: Past results and present view

5. Recurrent geomagnetic storms and relativistic electron enhancements in the outer magnetosphere: ISTP coordinated measurements

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