Asymmetric Reconnection Within a Flux Rope‐Type Dipolarization Front-Reference-Cited by-同舟云学术

Asymmetric Reconnection Within a Flux Rope‐Type Dipolarization Front

Published:2020-01 Issue:1 Volume:125 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Marshall A. T.¹,Burch J. L.²,Reiff P. H.¹,Webster J. M.¹,Torbert R. B.²³,Ergun R. E.⁴,Russell C. T.⁵,Strangeway R. J.⁵,Giles B. L.⁶,Nakamura R.⁷,Hwang K. ‐J.²,Genestreti K. J.³

Affiliation:

1. Department of Physics and Astronomy Rice University Houston TX USA

2. Southwest Research Institute San Antonio TX USA

3. Space Science Center University New Hampshire Durham NH USA

4. Department of Astrophysical and Planetary Sciences University of Colorado Boulder Boulder CO USA

5. Department of Earth, Planetary, and Space Sciences University of California, Los Angeles Los Angeles CA USA

6. Goddard Space Flight Center NASA Greenbelt MD USA

7. Space Research Institute Austrian Academy of Sciences Graz Austria

Funder

Southwest Research Institute

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA027296

Reference43 articles.

1. Bursty bulk flows in the inner central plasma sheet

2. Tail Reconnection Triggering Substorm Onset

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

4. Characteristics of high-speed ion flows in the plasma sheet

5. Multispacecraft analysis of dipolarization fronts and associated whistler wave emissions using MMS data

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