Quasi-Parallel Shock Reformation Seen by Magnetospheric Multiscale and Ion-Kinetic Simulations
Authors/Creators
- 1. Swedish Institute of Space Physics; Department of Physics, University of Helsinki
- 2. Department of Physics, University of Helsinki
- 3. Department of Physics, University of Helsinki; Finnish Meteorological Institute
Description
Shock waves in collisionless plasmas are among the most efficient particle accelerators in space. Shock reformation is a process important to plasma heating and acceleration, but direct observations of reformation at quasi-parallel shocks have been lacking. Here, we investigate Earth's quasi-parallel bow shock with observations by the four Magnetospheric Multiscale spacecraft. The multi-spacecraft observations provide evidence of short large-amplitude magnetic structures (SLAMS) causing reformation of the quasi-parallel shock. We perform an ion-kinetic Vlasiator simulation of the bow shock and show that SLAMS reforming the bow shock recreates the multi-spacecraft measurements. This provides a method for identifying shock reformation in the future.
Files
Geophysical Research Letters - 2022 - Johlander - Quasi‐Parallel Shock Reformation Seen by Magnetospheric Multiscale and.pdf
Files
(1.8 MB)
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