%0 Journal Article %T Detailed characterization of laboratory magnetized super-critical collisionless shock and of the associated proton energization %+ Laboratoire pour l'utilisation des lasers intenses (LULI) %+ Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères = Laboratory for Studies of Radiation and Matter in Astrophysics and Atmospheres (LERMA) %+ Horia Hulubei National Institute for Physics and Nuclear Engineering %+ IAP, Russian Academy of Sciences, 603155, Nizhny Novgorod, Russia %+ Énergie Matériaux Télécommunications - INRS (EMT-INRS) %+ Laboratoire national des champs magnétiques intenses - Toulouse (LNCMI-T) %+ Joint Institute for High Temperatures of the RAS (JIHT) %+ Università degli studi di Palermo - University of Palermo %+ INAF - Osservatorio Astronomico di Palermo (OAPa) %+ Centre d'Etudes Lasers Intenses et Applications (CELIA) %+ Institute of Physics of the Czech Academy of Sciences (FZU / CAS) %+ Moscow State Engineering Physics Institute (MEPhI) %A Yao, W. %A Fazzini, A. %A Chen, S., N. %A Burdonov, K. %A Antici, P. %A Béard, J. %A Bolaños, S. %A Ciardi, A. %A Diab, R. %A Filippov, E., D. %A Kisyov, S. %A Lelasseux, V. %A Miceli, M. %A Moreno, Q. %A Nastasa, V. %A Orlando, S. %A Pikuz, S. %A Popescu, D., C. %A Revet, G. %A Ribeyre, X. %A D’humières, E. %A Fuchs, J. %< avec comité de lecture %@ 2468-080X %J Matter and Radiation at Extremes %I AIP Publishing %V 7 %N 1 %P 014402 %8 2022 %D 2022 %R 10.1063/5.0055071 %Z Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Journal articles %X Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of non-thermal particles and high-energy radiation.In the absence of particle collisions in the system, theoretical works show that the interaction of an expanding plasma with a pre-existing electromagnetic structure (as in our case) is able to induce energy dissipation and allow for shock formation. Shock formation can alternatively take place when two plasmas interact, throughmicroscopic instabilities inducing electromagnetic fields which are able in turn to mediate energy dissipation and shock formation. Using our platform where we couple a fast expanding plasma induced by high-power lasers (JLF/Titan at LLNL and LULI2000) with high-strength magnetic fields, we have investigated the generation of magnetized collisionless shock and the associated particle energization. We have characterized the shock to be collisionless and super-critical.We report here on measurements of the plasma density, temperature, the electromagnetic field structures, and particle energization in the experiments, under various conditions of ambient plasma and B-field. We have also modelled the formation of the shocks using macroscopic hydrodynamic simulations and the associated particle acceleration using kinetic particle-in-cell simulations. As a companion paper of \citet{yao2020laboratory}, here we show additional results of the experiments and simulations, providing more information to reproduce them and demonstrating the robustness of our interpreted proton energization mechanism to be shock surfing acceleration. %G English %2 https://hal.science/hal-03355441/document %2 https://hal.science/hal-03355441/file/magnetized_collisionless_shock_long_MRE.pdf %L hal-03355441 %U https://hal.science/hal-03355441 %~ OBSPM %~ CEA %~ INSU %~ X %~ ENS-PARIS %~ UNIV-TLSE3 %~ UGA %~ CNRS %~ UNIV-CERGY %~ INSA-TOULOUSE %~ LERMA %~ X-LULI %~ X-DEP %~ X-DEP-PHYS %~ DAM %~ PSL %~ LNCMI %~ INSA-GROUPE %~ SORBONNE-UNIVERSITE %~ SORBONNE-UNIV %~ SU-SCIENCES %~ IP_PARIS %~ IP_PARIS_COPIE %~ TEST-HALCNRS %~ ENS-PSL %~ OBSPM-PSL %~ UGA-EPE %~ SU-TI %~ FERMI %~ ALLIANCE-SU %~ UNIV-UT3 %~ UT3-INP %~ UT3-TOULOUSEINP