High Mach Number Quasi‐Perpendicular Shocks: Spatial Versus Temporal Structure
Author:
Affiliation:
1. Solana Scientific Inc. Solana Beach CA USA
2. Southwest Research Institute San Antonio TX USA
3. University of California Los Angeles Los Angeles CA USA
4. University of Iowa Iowa City IA USA
Funder
Goddard Space Flight Center
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029287
Reference49 articles.
1. Magnetic pulsations from 0.1 to 4.0 Hz and associated plasma properties in the Earth's subsolar magnetosheath and plasma depletion layer
2. Microstructure in two- and three-dimensional hybrid simulations of perpendicular collisionless shocks
3. Direct evidence of nonstationary collisionless shocks in space plasmas
4. Ion anisotropy instabilities in the magnetosheath
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