Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
First HED experiment at XFEL

Professor Justin Wark

Professor of Physics

Sub department

  • Atomic and Laser Physics

Research groups

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

Astrophysically relevant experiments on radiation transfer through plasmas with large velocity gradients

PHYS PLASMAS 4:5 (1997) 2004-2010

Authors:

JS Wark, SJ Rose, PK Patel, A Djaoui, O Renner, A Hauer

Abstract:

The transfer of radiation through plasmas with large velocity gradients is of relevance to several astrophysical situations, such as supernova explosions, maser operation, and stellar winds. Similar conditions often prevail in laser-produced plasmas, with velocity gradients of order 10(9) s(-1) significantly altering the effective optical depth and line shape. Some of the simplest cases to study experimentally are the hydrogenic resonance lines. Experiments performed in both planar and cylindrical geometry, comparing the observed line profiles with those modeled using a one-dimensional Lagrangian hydrocode, incorporating average-atom nonlocal thermodynamic equilibrium (non-LTE) atomic physics are described. The opacity effects on the ion populations an treated within the escape factor approximation, taking into account the effects of the velocity gradient. The hydrocode gives time- and space-dependent values of the electron and ion densities, excited state fractions, electron and ion temperatures, and velocities, The hydrodynamic output is post-processed with a radiative transfer routine to construct the simulated line shape. Details of the experiments and results are presented, and relevance to the astrophysical situations discussed. (C) 1997 American Institute of Physics.
More details from the publisher

Measurements of direct drive laser imprint in thin foils by radiography using an x-ray laser backlighter

PHYS PLASMAS 4:5 (1997) 1985-1993

Authors:

DH Kalantar, MH Key, LB DaSilva, SG Glendinning, BA Remington, JE Rothenberg, F Weber, SV Weber, E Wolfrum, NS Kim, D Neely, J Zhang, JS Wark, A Demir, J Lin, R Smith, GJ Tallents, CLS Lewis, A MacPhee, J Warwick, JP Knauer

Abstract:

In direct drive inertial confinement fusion, the residual speckle pattern remaining after beam smoothing plays an important role in the seeding of instabilities at the ablation front. An x-ray laser is used as an extreme ultraviolet backlighter to characterize the imprinted modulation in thin foils for smoothing by random phase plate and by spectral dispersion for both 0.35 and 0.53 mu m irradiation, and by induced spatial incoherence for 0.53 mu m irradiation. Measurements of the imprinted modulation due to a single optical mode generated by two beam interference, and modification of the imprint with a superposed smooth irradiation to study time dependence of the imprinting process are demonstrated. (C) 1997 American Institute of Physics.
More details from the publisher

Comparison of the semiclassical and modified semiempirical method of spectral calculation

Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics 56:1 (1997) 936-946

Authors:

DJ Heading, JS Wark, RW Lee, R Stamm, B Talin

Abstract:

In recent experiments the capacity has been developed to generate plasmas at high densities. Standard methods used to diagnose plasmas are difficult to apply at these conditions, since it is necessary to calculate the entire spectrum as there is significant overlap of spectral lines. However, for most elements, the number of individual spectral line profiles calculated using the semiclassical method is very small. We present a method to use an approximate line width formula, coupled with an accurate database to generate a large number of line profiles. We evaluate the accuracy and utility of such an approach by comparison with semiclassical calculations. © 1997 The American Physical Society.
More details from the publisher

Time-resolved x-ray diffraction from laser-irradiated crystals

Conference on Quantum Electronics and Laser Science (QELS) - Technical Digest Series 12 (1997) 31

Authors:

J Larsson, E Judd, PH Bucksbaum, PS Schuck, RW Falcone, PA Heimann, HA Padmore, Z Chang, MM Murnane, HC Kapteyn, A Asfaw, RW Lee, A Machacek, J Wark

Abstract:

A switch based on ultrashort pulse laser heating of diffraction crystals provide insights about x-ray diffraction that forms a synchrotron with sub-picosecond time resolution. A change is diffracted intensity results from thermal expansion of the crystal over an x-ray absorption depth. The reduction in diffracted intensity is limited by the laser fluence to about 15%. It also asserts that experiments using an ultrashort pulse Ti:Sapphire laser synchronized to the ring and a laser pump/x-ray probe are possible. With regards to temporal resolution, a higher level of it can be obtained by using an ultrafast streak camera synchronized to the laser.

Ultrafast x-ray diffraction of laser-irradiated crystals

AIP Conference Proceedings AIP Publishing (1997) 204-208

Authors:

PA Heimann, J Larsson, Z Chang, A Lindenberg, PJ Schuck, E Judd, HA Padmore, PH Bucksbaum, RW Lee, M Murnane, H Kapteyn, JS Wark, RW Falcone
More details from the publisher

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 65
  • Page 66
  • Page 67
  • Page 68
  • Current page 69
  • Page 70
  • Page 71
  • Page 72
  • Page 73
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet