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Article Dans Une Revue High Energy Density Physics Année : 2015

Structure of a laser-driven radiative shock

Résumé

Radiative shocks are ubiquitous in stellar environments and are characterized by high temperature plasma emitting a considerable fraction of their energy as radiation. The physical structure of these shocks is complex and experimental benchmarks are needed to provide a deeper understanding of the physics at play. In addition, experiments provide unique data for testing radiation hydrodynamics codes which, in turn, are used to model astrophysical phenomena.
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Dates et versions

hal-03743110 , version 1 (02-08-2022)

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Uddhab Chaulagain, Chantal Stehle, Jean Larour, Michaela Kozlová, Francisco Suzuki-Vidal, et al.. Structure of a laser-driven radiative shock. High Energy Density Physics, 2015, 17, pp.106-113. ⟨hal-03743110⟩
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