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Updated: May 26, 2026

Non-equilibrium Microwave Plasma for Efficient High Temperature Chemistry
Published on: August 1, 2017
Steven J Schwartz1, Edmund Henley, Jeremy Mitchell
1Blackett Laboratory, Imperial College London, South Kensington, United Kingdom. s.schwartz@imperial.ac.uk
This study reveals that electron heating in astrophysical shock waves occurs within narrow layers, a key factor limiting nonlinear steepening and influencing cosmic ray acceleration. Understanding these electron dynamics is crucial for space physics.
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