Substorm occurrence rates, substorm recurrence times, and solar wind structure-Reference-Cited by-同舟云学术

Substorm occurrence rates, substorm recurrence times, and solar wind structure

Published:2017-03 Issue:3 Volume:122 Page:2973-2998
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Borovsky Joseph E.¹²^ORCID,Yakymenko Kateryna³⁴^ORCID

Affiliation:

1. Space Science Institute Boulder Colorado USA

2. CSSEUniversity of Michigan Ann Arbor Michigan USA

3. Department of Physics and Engineering PhysicsUniversity of Saskatchewan Saskatoon Saskatchewan Canada

4. Space Weather Summer SchoolLos Alamos National Laboratory Los Alamos New Mexico USA

Funder

NASA Heliophysics LWS TRT

NSF GEM

NSF Solar-Terrestrial

NASA Heliophysics Guest Investigator

NASA Geospace SR&T

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023625

Reference129 articles.

1. A statistical study of Pc 3–5 pulsations observed by the AMPTE/CCE Magnetic Fields Experiment, 1. Occurrence distributions

2. Bi-directional streaming of solar wind electrons >80 eV: ISEE evidence for a closed-field structure within the driver gas of an interplanetary shock

3. Hemispherical Joule Heating and theAEIndices

4. Superposed epoch analysis of the substorm plasma sheet

5. Belian R. D. J. E.Borovsky R. J.Nemzek andC. W.Smith(1994) Random and periodic substorms and their origins in the solar wind Proceedings of the Second International Conference on Substorms p. 463 Univ. of Alaska.

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