Low‐Energy (<200 eV) Electron Acceleration by ULF Waves in the Plasmaspheric Boundary Layer: Van Allen Probes Observation-Reference-Cited by-同舟云学术

Low‐Energy (<200 eV) Electron Acceleration by ULF Waves in the Plasmaspheric Boundary Layer: Van Allen Probes Observation

Published:2017-10 Issue:10 Volume:122 Page:9969-9982
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Ren Jie¹²^ORCID,Zong Q.‐G.¹^ORCID,Miyoshi Y.²^ORCID,Zhou X. Z.¹^ORCID,Wang Y. F.¹,Rankin R.³^ORCID,Yue C.⁴⁵^ORCID,Spence H. E.⁶^ORCID,Funsten H. O.⁷^ORCID,Wygant J. R.⁸^ORCID,Kletzing C. A.⁹^ORCID

Affiliation:

1. Institute of Space Physics and Applied TechnologyPeking University Beijing China

2. Solar‐Terrestrial Environmental LaboratoryNagoya University Nagoya Japan

3. Department of PhysicsUniversity of Alberta Edmonton Alberta Canada

4. Department of Atmospheric and Oceanic SciencesUniversity of California, Los Angeles Los Angeles CA USA

5. University Corporation for Atmospheric Research Boulder CO USA

6. Department of Physics Institute for Earth, Oceans and SpaceUniversity of New Hampshire Durham NH USA

7. Los Alamos National Laboratory Los Alamos NM USA

8. School of Physics and AstronomyUniversity of Minnesota Minneapolis MN USA

9. Department of Physics and AstronomyUniversity of Iowa Iowa City IA USA

Funder

National Natural Science Foundation of China

Natural Sciences and Engineering Research Council of Canada

Canadian Space Agency

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017JA024316

Reference69 articles.

1. IMAGE EUV observation of radially bifurcated plasmaspheric features: First observations of a possible standing ULF waveform in the inner magnetosphere

2. ULF waves-their relationship to the structure of the Earth's magnetosphere

3. Magnetospheric Multiscale Overview and Science Objectives

4. A theory of long-period magnetic pulsations: 2. Impulse excitation of surface eigenmode

5. Giant pulsations: An explanation for their rarity and occurrence during geomagnetically quiet times

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