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

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F22%3A00556995" target="_blank" >RIV/68378271:_____/22:00556995 - isvavai.cz</a>

Výsledek na webu

<a href="http://hdl.handle.net/11104/0331121" target="_blank" >http://hdl.handle.net/11104/0331121</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1063/5.0055071" target="_blank" >10.1063/5.0055071</a>

Jazyk výsledku

angličtina

Název v původním jazyce

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

Popis výsledku v původním jazyce

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.

Název v anglickém jazyce

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

Popis výsledku anglicky

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.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10305 - Fluids and plasma physics (including surface physics)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2022

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Matter and Radiation at Extremes

ISSN

2468-2047

e-ISSN

2468-080X

Svazek periodika

7

Číslo periodika v rámci svazku

1

Stát vydavatele periodika

IN - Indická republika

Počet stran výsledku

14

Strana od-do

014402

Kód UT WoS článku

000729404600001

EID výsledku v databázi Scopus

2-s2.0-85121276879