期刊文献+
共找到4篇文章
< 1 >
每页显示 20 50 100
On the study of hydrodynamic instabilities in the presence of background magnetic fields in high-energy-density plasmas 被引量:2
1
作者 M.J.-E.Manuel B.Khiar +11 位作者 g.rigon B.Albertazzi S.R.Klein F.Kroll F.-E.Brack T.Michel P.Mabey S.Pikuz J.C.Williams M.Koenig A.Casner C.C.Kuranz 《Matter and Radiation at Extremes》 SCIE CAS CSCD 2021年第2期37-45,共9页
Blast-wave-driven hydrodynamic instabilities are studied in the presence of a background B-field through experiments and simulations in the high-energy-density(HED)physics regime.In experiments conducted at the Labora... Blast-wave-driven hydrodynamic instabilities are studied in the presence of a background B-field through experiments and simulations in the high-energy-density(HED)physics regime.In experiments conducted at the Laboratoire pour l’utilisation des lasers intenses(LULI),a laserdriven shock-tube platform was used to generate a hydrodynamically unstable interface with a prescribed sinusoidal surface perturbation,and short-pulse x-ray radiography was used to characterize the instability growth with and without a 10-T B-field.The LULI experiments were modeled in FLASH using resistive and ideal magnetohydrodynamics(MHD),and comparing the experiments and simulations suggests that the Spitzer model implemented in FLASH is necessary and sufficient for modeling these planar systems.These results suggest insufficient amplification of the seed B-field,due to resistive diffusion,to alter the hydrodynamic behavior.Although the ideal-MHD simulations did not represent the experiments accurately,they suggest that similar HED systems with dynamic plasma-β(=2μ_(0)ρv^(2)/B^(2))values of less than∼100 can reduce the growth of blast-wave-driven Rayleigh–Taylor instabilities.These findings validate the resistive-MHD FLASH modeling that is being used to design future experiments for studying B-field effects in HED plasmas. 展开更多
关键词 field. HYDRODYNAMIC INSTABILITIES
下载PDF
Development of new diagnostics based on LiF detector for pump-probe experiments
2
作者 T.Pikuz A.Faenov +25 位作者 NOzaki T.Matsuoka B.Albertazzi N.J.Hartley K.Miyanishi K.Katagiri S.Matsuyama K.Yamauchi H.Habara Y.Inubushi T.Togashi H.Yumoto H.Ohashi Y.Tange T.Yabuuchi M.Yabashi A.N.Grum-Grzhimailo A.Casner I.Skobelev S.Makarov S.Pikuz g.rigon M.Koenig K.A.Tanaka T.Ishikawa R.Kodama 《Matter and Radiation at Extremes》 SCIE EI CAS 2018年第4期197-206,共10页
We present new diagnostics for use in optical laser pump-X-ray Free Electron Laser(XFEL)probe experiments to monitor dimensions,intensity profile and focusability of the XFEL beam and to control initial quality and ho... We present new diagnostics for use in optical laser pump-X-ray Free Electron Laser(XFEL)probe experiments to monitor dimensions,intensity profile and focusability of the XFEL beam and to control initial quality and homogeneity of targets to be driven by optical laser pulse.By developing X-ray imaging,based on the use of an LiF crystal detector,we were able to measure the distribution of energy inside a hard X-ray beam with unprecedented high spatial resolution(~1 mm)and across a field of view larger than some millimetres.This diagnostic can be used in situ,provides a very high dynamic range,has an extremely limited cost,and is relatively easy to be implemented in pump-probe experiments.The proposed methods were successfully applied in pump-probe experiments at the SPring-8 Angstrom Compact free electron LAser(SACLA)XFEL facility and its potential was demonstrated for current and future High Energy Density Science experiments. 展开更多
关键词 XFEL Shock waves Pump-probe experiments High energy density science X-ray spectroscopy X-ray imaging
下载PDF
Analytical modelling of the expansion of a solid obstacle interacting with a radiative shock
3
作者 Th.Michel E.Falize +19 位作者 B.Albertazzi g.rigon Y.Sakawa T.Sano H.Shimogawara R.Kumar T.Morita C.Michaut A.Casner R Barroso P.Mabey Y.Kuramitsu S.Laffite L.Van Box Som G.Gregori R.Kodama N.Ozaki P.Tzeferacos D.Lamb M.Koenig 《High Power Laser Science and Engineering》 SCIE CAS CSCD 2018年第2期123-132,共10页
In this paper, we present a model characterizing the interaction of a radiative shock(RS) with a solid material, as described in a recent paper(Koenig et al., Phys. Plasmas, 24, 082707(2017)), the new model is then re... In this paper, we present a model characterizing the interaction of a radiative shock(RS) with a solid material, as described in a recent paper(Koenig et al., Phys. Plasmas, 24, 082707(2017)), the new model is then related to recent experiments performed on the GEKKO XII laser facility. The RS generated in a xenon gas cell propagates towards a solid obstacle that is ablated by radiation coming from the shock front and the radiative precursor, mimicking processes occurring in astrophysical phenomena. The model presented here calculates the dynamics of the obstacle expansion,which depends on several parameters, notably the geometry and the temperature of the shock. All parameters required for the model have been obtained from experiments. Good agreement between experimental data and the model is found when spherical geometry is taken into account. As a consequence, this model is a useful and easy tool to infer parameters from experimental data(such as the shock temperature), and also to design future experiments. 展开更多
关键词 high energy density physics laser–plasmas interaction modelling plasmas astrophysics plasma physics radiative hydrodynamics radiative shock
原文传递
Laboratory radiative accretion shocks on GEKKO XⅡlaser facility for POLAR project
4
作者 L.Van Box Som E.Falize +20 位作者 M.Koenig Y.Sakawa B.Albertazzi E Barroso J.-M.Bonnet-Bidaud C.Busschaert A.Ciardi Y.Hara N.Katsuki R.Kumar E Lefevre C.Michaut Th.Michel T.Miura T.Morita M.Mouchet g.rigon T.Sano S.Shiiba H.Shimogawara S.Tomiya 《High Power Laser Science and Engineering》 SCIE CAS CSCD 2018年第2期181-188,共8页
A new target design is presented to model high-energy radiative accretion shocks in polars. In this paper, we present the experimental results obtained on the GEKKO XII laser facility for the POLAR project. The experi... A new target design is presented to model high-energy radiative accretion shocks in polars. In this paper, we present the experimental results obtained on the GEKKO XII laser facility for the POLAR project. The experimental results are compared with 2 D FCI2 simulations to characterize the dynamics and the structure of plasma flow before and after the collision. The good agreement between simulations and experimental data confirms the formation of a reverse shock where cooling losses start modifying the post-shock region. With the multi-material structure of the target,a hydrodynamic collimation is exhibited and a radiative structure coupled with the reverse shock is highlighted in both experimental data and simulations. The flexibility of the laser energy produced on GEKKO XII allowed us to produce high-velocity flows and study new and interesting radiation hydrodynamic regimes between those obtained on the LULI2000 and Orion laser facilities. 展开更多
关键词 accretion processes high power laser HYDRODYNAMICS laboratory astrophysics
原文传递
上一页 1 下一页 到第
使用帮助 返回顶部