0000000000190875

AUTHOR

S. N. Chen

showing 3 related works from this author

Detailed characterization of laboratory magnetized super-critical collisionless shock and of the associated proton energization

2021

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…

Nuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesmagnetic fieldQC770-798shock waves01 natural sciencesAtomic and Molecular Physics and OpticsPhysics - Plasma Physics010305 fluids & plasmasPlasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E AstrofisicaNuclear Energy and Engineering[PHYS.PHYS.PHYS-PLASM-PH]Physics [physics]/Physics [physics]/Plasma Physics [physics.plasm-ph]Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesPhysics::Space PhysicsElectrical and Electronic Engineering010306 general physics
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Laboratory evidence for asymmetric accretion structure upon slanted matter impact in young stars

2020

Aims. Investigating the process of matter accretion onto forming stars through scaled experiments in the laboratory is important in order to better understand star and planetary system formation and evolution. Such experiments can indeed complement observations by providing access to the processes with spatial and temporal resolution. A previous investigation revealed the existence of a two-component stream: a hot shell surrounding a cooler inner stream. The shell was formed by matter laterally ejected upon impact and refocused by the local magnetic field. That laboratory investigation was limited to normal incidence impacts. However, in young stellar objects, the complex structure of magne…

Shock wavestarsAccretionMagnetohydrodynamics (MHD)Young stellar objectFOS: Physical sciencesX-rays: starsAstrophysics01 natural sciencesShock wavesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsEjecta010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicspre-main sequence -X-raysAstronomy and AstrophysicsPlasmaPlanetary system[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]accretion disks -instabilities -magnetohydrodynamics (MHD) -shock waves -starsAccretion (astrophysics)StarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceInstabilitiesAccretion disksStars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Particle energization in colliding subcritical collisionless shocks investigated in the laboratory

2022

Context. Colliding collisionless shocks appear across a broad variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. Aims. The main goal of our experimental and computational work is to understand the effect of the interpenetration between two subcritical collisionless shocks on particle energization. Methods. To investigate the detailed dynamics of this phenomenon, we performed a dedicated laboratory experiment. We generated two counter-streaming subcritical collisionless magnetized shocks by irradiating two Teflon (C2F4) targets with 100 J, 1 ns laser beams on the LULI2000 laser facility. The interaction region between the plasm…

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E Astrofisica[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU]Sciences of the Universe [physics]Space and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsshock wavesinterplanetary mediumPhysics - Plasma Physicsacceleration of particles
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