Detailed characterization of a laboratory magnetized supercritical collisionless shock and of the associated proton energization

Yao W.; Fazzini A.; Chen S. N.; Burdonov K.; Antici P.; Béard J.; Bolaños S.; Ciardi A.; Diab R.; Filippov E. D.; Kisyov S.; Lelasseux V.; Miceli M.; Moreno Q.; Nastasa V.; Orlando S.; Pikuz S.; Popescu D. C.; Revet G.; Ribeyre X.; d’Humières E.; Fuchs J.

doi:10.1063/5.0055071

Volume 7 Issue 1

Jan. 2022

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Yao W., Fazzini A., Chen S. N., Burdonov K., Antici P., Béard J., Bolaños S., Ciardi A., Diab R., Filippov E. D., Kisyov S., Lelasseux V., Miceli M., Moreno Q., Nastasa V., Orlando S., Pikuz S., Popescu D. C., Revet G., Ribeyre X., d’Humières E., Fuchs J.. Detailed characterization of a laboratory magnetized supercritical collisionless shock and of the associated proton energization[J]. Matter and Radiation at Extremes, 2022, 7(1): 014402. doi: 10.1063/5.0055071

Citation:

Yao W., Fazzini A., Chen S. N., Burdonov K., Antici P., Béard J., Bolaños S., Ciardi A., Diab R., Filippov E. D., Kisyov S., Lelasseux V., Miceli M., Moreno Q., Nastasa V., Orlando S., Pikuz S., Popescu D. C., Revet G., Ribeyre X., d’Humières E., Fuchs J.. Detailed characterization of a laboratory magnetized supercritical collisionless shock and of the associated proton energization[J]. Matter and Radiation at Extremes, 2022, 7(1): 014402. doi: 10.1063/5.0055071

Citation:

Yao W., Fazzini A., Chen S. N., Burdonov K., Antici P., Béard J., Bolaños S., Ciardi A., Diab R., Filippov E. D., Kisyov S., Lelasseux V., Miceli M., Moreno Q., Nastasa V., Orlando S., Pikuz S., Popescu D. C., Revet G., Ribeyre X., d’Humières E., Fuchs J.. Detailed characterization of a laboratory magnetized supercritical collisionless shock and of the associated proton energization[J]. Matter and Radiation at Extremes, 2022, 7(1): 014402. doi: 10.1063/5.0055071

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Detailed characterization of a laboratory magnetized supercritical collisionless shock and of the associated proton energization

doi: 10.1063/5.0055071

Yao W.^{1, 2
,
,
,},
Fazzini A.¹,
Chen S. N.³,
Burdonov K.^{1, 2, 4},
Antici P.^5
,,
Béard J.^6
,,
Bolaños S.^1
,,
Ciardi A.^2
,,
Diab R.^1
,,
Filippov E. D.^{7, 4
,},
Kisyov S.³,
Lelasseux V.^1
,,
Miceli M.^{8, 9
,},
Moreno Q.^{10, 11
,},
Nastasa V.³,
Orlando S.⁹,
Pikuz S.^{7, 12},
Popescu D. C.^3
,,
Revet G.¹,
Ribeyre X.^{10
,},
d’Humières E.¹⁰,
Fuchs J.¹

1.
LULI–CNRS, CEA, UPMC Univ Paris 06: Sorbonne Université, Ecole Polytechnique, Institut Polytechnique de Paris, F-91128 Palaiseau Cedex, France
2.
Sorbonne Université, Observatoire de Paris, Université PSL, CNRS, LERMA, F-75005 Paris, France
3.
ELI-NP, “Horia Hulubei” National Institute for Physics and Nuclear Engineering, 30 Reactorului Street, RO-077125 Bucharest-Magurele, Romania
4.
IAP, Russian Academy of Sciences, 603155 Nizhny Novgorod, Russia
5.
INRS-EMT, 1650 Blvd. Lionel-Boulet, Varennes, Quebec J3X 1S2, Canada
6.
LNCMI, UPR 3228, CNRS-UGA-UPS-INSA, F-31400 Toulouse, France
7.
JIHT, Russian Academy of Sciences, 125412 Moscow, Russia
8.
Università degli Studi di Palermo, Dipartimento di Fisica e Chimica E. Segrè, Piazza del Parlamento 1, 90134 Palermo, Italy
9.
INAF–Osservatorio Astronomico di Palermo, Palermo, Italy
10.
University of Bordeaux, Centre Lasers Intenses et Applications, CNRS, CEA, UMR 5107, F-33405 Talence, France
11.
ELI-Beamlines, Institute of Physics, Czech Academy of Sciences, 5 Kvetna 835, 25241 Dolni Brezany, Czech Republic
12.
NRNU MEPhI, 115409 Moscow, Russia

More Information

Corresponding author: a)Author to whom correspondence should be addressed: yao.weipeng@polytechnique.edu
Received Date: 2021-04-25
Accepted Date: 2021-09-26

Available Online: 2022-01-01

Publish Date: 2022-01-01

Abstract

Abstract

Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of nonthermal particles and high-energy radiation. In the absence of particle collisions in the system, theory shows 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 shock formation. Shock formation can alternatively take place when two plasmas interact, through microscopic instabilities inducing electromagnetic fields that are able in turn to mediate energy dissipation and shock formation. Using our platform in which we couple a rapidly expanding plasma induced by high-power lasers (JLF/Titan at LLNL and LULI2000) with high-strength magnetic fields, we have investigated the generation of a magnetized collisionless shock and the associated particle energization. We have characterized the shock as being collisionless and supercritical. We report here on measurements of the plasma density and temperature, the electromagnetic field structures, and the particle energization in the experiments, under various conditions of ambient plasma and magnetic field. We have also modeled the formation of the shocks using macroscopic hydrodynamic simulations and the associated particle acceleration using kinetic particle-in-cell simulations. As a companion paper to Yao et al. [Nat. Phys. 17 , 1177–1182 (2021)], here we show additional results of the experiments and simulations, providing more information to allow their reproduction and to demonstrate the robustness of our interpretation of the proton energization mechanism as being shock surfing acceleration.

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References(65)

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