Acceleration of radiation belt electrons and the role of the average interplanetary magnetic field B z component in high‐speed streams-Reference-Cited by-同舟云学术

Acceleration of radiation belt electrons and the role of the average interplanetary magnetic field B z component in high‐speed streams

Published:2017-10 Issue:10 Volume:122 Page:10,084-10,101
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Souza V. M.¹^ORCID,Lopez R. E.²^ORCID,Jauer P. R.¹,Sibeck D. G.³^ORCID,Pham K.⁴,Da Silva L. A.¹,Marchezi J. P.¹^ORCID,Alves L. R.¹^ORCID,Koga D.¹^ORCID,Medeiros C.¹^ORCID,Rockenbach M.¹,Gonzalez W. D.¹^ORCID

Affiliation:

1. National Institute for Space Research/INPE São Paulo Brazil

2. Department of PhysicsUniversity of Texas at Arlington Arlington Texas USA

3. NASA/Goddard Space Flight Center Greenbelt Maryland USA

4. Department of Physics and AstronomyWest Virginia University Morgantown West Virginia USA

Funder

Fundação de Amparo à Pesquisa do Estado de São Paulo

Primate Conservation

Conselho Nacional de Desenvolvimento Científico e Tecnológico

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017JA024187

Reference58 articles.

1. Bursty bulk flows in the inner central plasma sheet

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

3. A strong CME-related magnetic cloud interaction with the Earth's Magnetosphere: ISTP observations of rapid relativistic electron acceleration on May 15, 1997

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