Plasma Transport Driven by the Three‐Dimensional Kelvin‐Helmholtz Instability
Author:
Affiliation:
1. Geophysical InstituteUniversity of Alaska Fairbanks Fairbanks AK USA
2. Now at Department of Physical SciencesEmbry‐Riddle Aeronautical University Daytona Beach FL USA
Funder
National Aeronautics and Space Administration
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/2017JA024394
Reference59 articles.
1. The Kelvin–Helmholtz instability under Parker-Spiral Interplanetary Magnetic Field conditions at the magnetospheric flanks
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3. Computer studies of the dynamic evolution of the geomagnetic tail
4. Entropy conservation in simulations of magnetic reconnection
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