62 citations · 212 across the 6 of their papers we have counts for
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Magnetic field amplification by the Weibel instability at planetary and astrophysical high-Mach-number shocks
Artem Bohdan, Martin Pohl, Jacek Niemiec +5
Collisionless shocks are ubiquitous in the Universe and often associated with strong magnetic field. Here we use large-scale particle-in-cell simulations of non-relativistic perpen…
An in situ comparison of electron acceleration at collisionless shocks under differing upstream magnetic field orientations
A. Masters, A. H. Sulaiman, Ł. Stawarz +6
A leading explanation for the origin of Galactic cosmic rays is acceleration at high-Mach number shock waves in the collisionless plasma surrounding young supernova remnants. Evide…
Suprathermal electrons at Saturn's bow shock
A. Masters, A. H. Sulaiman, N. Sergis +4
The leading explanation for the origin of galactic cosmic rays is particle acceleration at the shocks surrounding young supernova remnants (SNRs), although crucial aspects of the a…