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91探花
First HED experiment at XFEL

Professor Justin Wark

Professor of Physics

Sub department

  • Atomic and Laser Physics

Research groups

  • 91探花 Centre for High Energy Density Science (OxCHEDS)
Justin.Wark@physics.ox.ac.uk
Telephone: 01865 (2)72251
Clarendon Laboratory, room 029.9
  • About
  • Publications

X-Ray Line Transfer in Plasmas with Large Velocity Gradients

Chapter in High Energy Density Laboratory Astrophysics, Springer Nature (2005) 171-176

Authors:

FM Kerr, A Gouveia, RW Lee, PK Patel, O Renner, SJ Rose, HA Scott, JS Wark

Materials science under extreme conditions of pressure and strain rate

METALL MATER TRANS A 35A:9 (2004) 2587-2607

Authors:

BA Remington, G Bazan, J Belak, E Bringa, M Caturla, JD Colvin, MJ Edwards, SG Glendinning, DS Ivanov, B Kad, DH Kalantar, M Kumar, BF Lasinski, KT Lorenz, JM McNaney, DD Meyerhofer, MA Meyers, SM Pollaine, D Rowley, M Schneider, JS Stolken, JS Wark, SV Weber, WG Wolfer, B Yaakobi, LV Zhigilei

Abstract:

Solid-state dynamics experiments at very high pressures and strain rates are becoming possible with high-power laser facilities, albeit over brief intervals of time and spatially small scales. To achieve extreme pressures in the solid state requires that the sample be kept cool, with T-sample < T-melt. To this end, a shockless, plasma-piston "drive" has been developed on the Omega laser, and a staged shock drive was demonstrated on the Nova laser. To characterize the drive, velocity interferometer measurements allow the high pressures of 10 to 200 GPa (0.1 to 2 Mbar) and strain rates of 10(6) to 10(8) s(-1) to be determined. Solid-state strength in the sample is inferred at these high pressures using the Rayleigh-Taylor (RT) instability as a "diagnostic." Lattice response and phase can be inferred for single-crystal samples from time-resolved X-ray diffraction. Temperature and compression in polycrystalline samples can be deduced from extended X-ray absorption fine-structure (EXAFS) measurements. Deformation mechanisms and residual melt depth can be identified by examining recovered samples. We will briefly review this new area of laser-based materials-dynamics research, then present a path forward for carrying these solid-state experiments to much higher pressures, P > 10(3) GPa (10 Mbar), on the National Ignition Facility (NIF) laser at Lawrence Livermore National Laboratory.

Time Resolved X鈥恟ay Diffraction and Non鈥怲hermal Inelastic X鈥恟ay Scattering

AIP Conference Proceedings AIP Publishing 705:1 (2004) 1387-1390

Authors:

P Sondhauss, M Harbst, J Larsson, GA Naylor, A Plech, K Scheidt, O Synnergren, JS Wark, M Wulff

Simulations of a photopumped X-ray laser using the H-like Cl - Li-like Se scheme

Journal of Quantitative Spectroscopy and Radiative Transfer 83:2 (2004) 203-213

Authors:

IR Al'Miev, X Lu, SJ Rose, J Zhang, JS Wark

Abstract:

Calculations of the modal photon densities and gain in a photopumped Cl XVII-Se XXXII X-ray laser are presented. In this paper we undertake a realistic simulation of the generation of both Cl and Se plasmas, using a high-power optical laser, which includes radiation from both Ly-伪 fine-structure components of H-like Cl pumping the 2p3/2-5d5/2 transition in Li-like Se. The calculations are performed in two dimensions in a realistic geometry taking into account plasma gradients. This gives information about the spatial extent and time evolution of X-ray lasing gain on the 5-4 transitions (39.5 脜) in Li-like Se. We find that gain (about 200 cm-1) is expected only when the optical laser includes a pre-pulse. Calculations show that the absorption of pumping radiation in the pumped plasma can reduce the gain by 20%. Time-dependent calculations have shown that the gain is reduced by 30% in comparison to the steady-state calculations. The effect of the spectral profile and self-radiation of 5d5/2-2p3/2 transition in Li-like Se reduces the gain by about 2%. 漏 2003 Elsevier Ltd. All rights reserved.

Enhancement of optically thick to thin line intensities in solar and stellar coronal plasmas through radiative transfer effects: An angularly resolved study

ASTROPHYSICAL JOURNAL 613:2 (2004) L181-L184

Authors:

FM Kerr, SJ Rose, JS Wark, FP Keenan

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