Reconnection rates and X line motion at the magnetopause: Global 2D‐3V hybrid‐Vlasov simulation results-Reference-Cited by-同舟云学术

Reconnection rates and X line motion at the magnetopause: Global 2D‐3V hybrid‐Vlasov simulation results

Published:2017-03 Issue:3 Volume:122 Page:2877-2888
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Hoilijoki Sanni¹^ORCID,Ganse Urs¹,Pfau‐Kempf Yann¹,Cassak Paul A.²^ORCID,Walsh Brian M.³^ORCID,Hietala Heli⁴^ORCID,Alfthan Sebastian⁵,Palmroth Minna¹⁶^ORCID

Affiliation:

1. Department of Physics University of Helsinki Helsinki Finland

2. Department of Physics and Astronomy West Virginia University Morgantown West Virginia USA

3. Mechanical Engineering and Center for Space Physics Boston University Boston Massachusetts USA

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

5. CSC‐IT Center for Science Ltd. Espoo Finland

6. Finnish Meteorological Institute Helsinki Finland

Funder

Suomen Akatemia

European Research Council

National Science Foundation

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016JA023709

Reference56 articles.

1. Scaling of asymmetric reconnection in compressible plasmas

2. ULF waves and their influence on bow shock and magnetosheath structures

3. Global hybrid simulations: Foreshock waves and cavitons under radial interplanetary magnetic field geometry

4. What determines the reconnection rate at the dayside magnetosphere?

5. Scaling of the magnetic reconnection rate with symmetric shear flow

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