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Laser-Produced Plasmas as Drivers of Quasi-Parallel Collisionless Shock Formation in the Laboratory
2020
Zenodo
Quasi-parallel collisionless shocks are objects of considerable interest in space and astrophysics, most notably as possible sites of cosmic ray acceleration. Such shocks occur naturally in systems such as supernova remnants and planetary bow shocks, where the complex and turbulent structures they form are commonly observed by spacecraft. However, \textit{in situ} spacecraft measurements have some inherent limitations, such as a moving reference frame and non-repeatable measurements. Generating
doi:10.5281/zenodo.3875148
fatcat:ry7wu4q47resbiw4fa7nnbcz7m