Hybrid Simulations of Magnetodisc Transport Driven by the Rayleigh‐Taylor Instability
Author:
Affiliation:
1. Geophysical Institute University of Alaska Fairbanks Fairbanks AK USA
2. Department of Physical Sciences Embry‐Riddle Aeronautical University Bunnell 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/10.1029/2018JA026420
Reference39 articles.
1. 1. Transport of Mass, Momentum and Energy in Planetary Magnetodisc Regions
2. Dynamics of the Saturnian inner magnetosphere: First inferences from the Cassini magnetometers about small-scale plasma transport in the magnetosphere
3. Interchange Injections at Saturn: Statistical Survey of Energetic H + Sudden Flux Intensifications
4. The magnetosphere of Jupiter: Coupling the equator to the poles
5. Flow of mass and energy in the magnetospheres of Jupiter and Saturn
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1. The Roles of Flux Tube Entropy and Effective Gravity in the Inward Plasma Transport at Saturn;The Astrophysical Journal;2022-09-01
2. The Kelvin-Helmholtz Instability From the Perspective of Hybrid Simulations;Frontiers in Astronomy and Space Sciences;2021-12-13
3. Kelvin–Helmholtz‐Related Turbulent Heating at Saturn's Magnetopause Boundary;Journal of Geophysical Research: Space Physics;2021-02
4. On The Nature of Turbulent Heating and Radial Transport in Saturn's Magnetosphere;Journal of Geophysical Research: Space Physics;2021-01
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