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Counterpropagating Radiative Shock Experiments on the Orion Laser.
Suzuki-Vidal, F; Clayson, T; Stehlé, C; Swadling, G F; Foster, J M; Skidmore, J; Graham, P; Burdiak, G C; Lebedev, S V; Chaulagain, U; Singh, R L; Gumbrell, E T; Patankar, S; Spindloe, C; Larour, J; Kozlova, M; Rodriguez, R; Gil, J M; Espinosa, G; Velarde, P; Danson, C.
Affiliation
  • Suzuki-Vidal F; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Clayson T; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Stehlé C; Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères (LERMA), Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University, Université Pierre et Marie Curie (UPMC), Sorbonne University, 4 Place Jussieu, 75252 Paris, France.
  • Swadling GF; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Foster JM; Atomic Weapons Establishment (AWE), Aldermaston, Reading, West Berkshire RG7 4PR, United Kingdom.
  • Skidmore J; Atomic Weapons Establishment (AWE), Aldermaston, Reading, West Berkshire RG7 4PR, United Kingdom.
  • Graham P; Atomic Weapons Establishment (AWE), Aldermaston, Reading, West Berkshire RG7 4PR, United Kingdom.
  • Burdiak GC; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Lebedev SV; Blackett Laboratory, Imperial College London, London SW7 2BW, United Kingdom.
  • Chaulagain U; Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères (LERMA), Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University, Université Pierre et Marie Curie (UPMC), Sorbonne University, 4 Place Jussieu, 75252 Paris, France.
  • Singh RL; Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères (LERMA), Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University, Université Pierre et Marie Curie (UPMC), Sorbonne University, 4 Place Jussieu, 75252 Paris, France.
  • Gumbrell ET; Atomic Weapons Establishment (AWE), Aldermaston, Reading, West Berkshire RG7 4PR, United Kingdom.
  • Patankar S; Atomic Weapons Establishment (AWE), Aldermaston, Reading, West Berkshire RG7 4PR, United Kingdom.
  • Spindloe C; Science and Technology Facilities Council, Rutherford Appleton Laboratory, Harwell Campus, Chilton, Didcot, Oxon OX11 0QX, United Kingdom.
  • Larour J; Laboratoire de Physique des Plasmas (LPP), Centre National de la Recherche Scientifique (CNRS), Ecole Polytechnique, Université Pierre et Marie Curie, Université Paris-Saclay, Sorbonne University, PSL Research University, 4 Place Jussieu, 75252 Paris, France.
  • Kozlova M; Extreme Light Infrastructure (ELI), Institute of Plasma Physics, Czech Academy of Sciences, 182 00 Prague 8, Czech Republic.
  • Rodriguez R; Departamento de Fisica, Universidad de Las Palmas de Gran Canaria, 35003 Las Palmas de Gran Canaria, Las Palmas, Spain.
  • Gil JM; Departamento de Fisica, Universidad de Las Palmas de Gran Canaria, 35003 Las Palmas de Gran Canaria, Las Palmas, Spain.
  • Espinosa G; Departamento de Fisica, Universidad de Las Palmas de Gran Canaria, 35003 Las Palmas de Gran Canaria, Las Palmas, Spain.
  • Velarde P; Instituto de Fusion Nuclear, Universidad Politecnica de Madrid, 28040 Madrid, Spain.
  • Danson C; Atomic Weapons Establishment (AWE), Aldermaston, Reading, West Berkshire RG7 4PR, United Kingdom.
Phys Rev Lett ; 119(5): 055001, 2017 Aug 04.
Article in En | MEDLINE | ID: mdl-28949745
ABSTRACT
We present new experiments to study the formation of radiative shocks and the interaction between two counterpropagating radiative shocks. The experiments are performed at the Orion laser facility, which is used to drive shocks in xenon inside large aspect ratio gas cells. The collision between the two shocks and their respective radiative precursors, combined with the formation of inherently three-dimensional shocks, provides a novel platform particularly suited for the benchmarking of numerical codes. The dynamics of the shocks before and after the collision are investigated using point-projection x-ray backlighting while, simultaneously, the electron density in the radiative precursor was measured via optical laser interferometry. Modeling of the experiments using the 2D radiation hydrodynamic codes nym and petra shows very good agreement with the experimental results.

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Phys Rev Lett Year: 2017 Document type: Article

Full text: 1 Collection: 01-internacional Database: MEDLINE Language: En Journal: Phys Rev Lett Year: 2017 Document type: Article