DOE PAGES title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Time evolution and asymmetry of a laser produced blast wave

Abstract

Studies of a blast wave produced from carbon rods and plastic spheres in an argon background gas have been conducted using the Vulcan laser at the Rutherford Appleton Laboratory. A laser of 1500 J was focused onto these targets, and rear-side observations of an emission front were recorded using a fast-framing camera. The emission front is asymmetrical in shape and tends to a more symmetrical shape as it progresses due to the production of a second shock wave later in time, which pushes out the front of the blast wave. Plastic spheres produce faster blast waves, and the breakthrough of the second shock is visible before the shock stalls. Furthermore the results are presented to demonstrate this trend, and similar evolution dynamics of experimental and simulation data from the FLASH radiation-hydrodynamics code are observed.

Authors:
ORCiD logo [1];  [2];  [3];  [3];  [4]; ORCiD logo [1];  [3];  [3];  [1]; ORCiD logo [4];  [5];  [4];  [2];  [5];  [4];  [3]; ORCiD logo [1]
  1. Univ. of York, York (United Kingdom)
  2. STFC Rutherford Appleton Lab., Didcot (United Kingdom)
  3. Univ. of Oxford, Oxford (United Kingdom)
  4. Queen's Univ., Belfast (United Kingdom)
  5. Univ. of Chicago, Chicago, IL (United States)
Publication Date:
Research Org.:
Univ. of Chicago, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1502089
Alternate Identifier(s):
OSTI ID: 1399292
Grant/Contract Number:  
SC0016566; FWP 57789
Resource Type:
Accepted Manuscript
Journal Name:
Physics of Plasmas
Additional Journal Information:
Journal Volume: 24; Journal Issue: 10; Journal ID: ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; Plasmas; Computer simulation; Volcanology; Plasma diagnostics; Shock waves; Data analysis; Chemical elements; Lasers; Electromagnetism; Hydrodynamics simulations

Citation Formats

Tubman, E. R., Scott, R. H. H., Doyle, H. W., Meinecke, J., Ahmed, H., Alraddadi, R. A. B., Bolis, R., Cross, J. E., Crowston, R., Doria, D., Lamb, D., Reville, B., Robinson, A. P. L., Tzeferacos, P., Borghesi, M., Gregori, G., and Woolsey, N. C. Time evolution and asymmetry of a laser produced blast wave. United States: N. p., 2017. Web. doi:10.1063/1.4987038.
Tubman, E. R., Scott, R. H. H., Doyle, H. W., Meinecke, J., Ahmed, H., Alraddadi, R. A. B., Bolis, R., Cross, J. E., Crowston, R., Doria, D., Lamb, D., Reville, B., Robinson, A. P. L., Tzeferacos, P., Borghesi, M., Gregori, G., & Woolsey, N. C. Time evolution and asymmetry of a laser produced blast wave. United States. https://doi.org/10.1063/1.4987038
Tubman, E. R., Scott, R. H. H., Doyle, H. W., Meinecke, J., Ahmed, H., Alraddadi, R. A. B., Bolis, R., Cross, J. E., Crowston, R., Doria, D., Lamb, D., Reville, B., Robinson, A. P. L., Tzeferacos, P., Borghesi, M., Gregori, G., and Woolsey, N. C. Fri . "Time evolution and asymmetry of a laser produced blast wave". United States. https://doi.org/10.1063/1.4987038. https://www.osti.gov/servlets/purl/1502089.
@article{osti_1502089,
title = {Time evolution and asymmetry of a laser produced blast wave},
author = {Tubman, E. R. and Scott, R. H. H. and Doyle, H. W. and Meinecke, J. and Ahmed, H. and Alraddadi, R. A. B. and Bolis, R. and Cross, J. E. and Crowston, R. and Doria, D. and Lamb, D. and Reville, B. and Robinson, A. P. L. and Tzeferacos, P. and Borghesi, M. and Gregori, G. and Woolsey, N. C.},
abstractNote = {Studies of a blast wave produced from carbon rods and plastic spheres in an argon background gas have been conducted using the Vulcan laser at the Rutherford Appleton Laboratory. A laser of 1500 J was focused onto these targets, and rear-side observations of an emission front were recorded using a fast-framing camera. The emission front is asymmetrical in shape and tends to a more symmetrical shape as it progresses due to the production of a second shock wave later in time, which pushes out the front of the blast wave. Plastic spheres produce faster blast waves, and the breakthrough of the second shock is visible before the shock stalls. Furthermore the results are presented to demonstrate this trend, and similar evolution dynamics of experimental and simulation data from the FLASH radiation-hydrodynamics code are observed.},
doi = {10.1063/1.4987038},
journal = {Physics of Plasmas},
number = 10,
volume = 24,
place = {United States},
year = {Fri Oct 13 00:00:00 EDT 2017},
month = {Fri Oct 13 00:00:00 EDT 2017}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record

Citation Metrics:
Cited by: 4 works
Citation information provided by
Web of Science

Figures / Tables:

FIG. 1. FIG. 1. : A diagram of the experimental set-up for producing a blast wave from a carbon rod and propagating out into an ambient background gas.

Save / Share:

Works referenced in this record:

Instability of Taylor-Sedov blast waves propagating through a uniform gas
journal, May 1991


Extensible component-based architecture for FLASH, a massively parallel, multiphysics simulation code
journal, October 2009


FLASH magnetohydrodynamic simulations of shock-generated magnetic field experiments
journal, December 2012


On the origin of cosmic magnetic fields
journal, March 2008


FLASH: An Adaptive Mesh Hydrodynamics Code for Modeling Astrophysical Thermonuclear Flashes
journal, November 2000

  • Fryxell, B.; Olson, K.; Ricker, P.
  • The Astrophysical Journal Supplement Series, Vol. 131, Issue 1
  • DOI: 10.1086/317361

Scaling of Magneto-Quantum-Radiative Hydrodynamic Equations: from Laser-Produced Plasmas to Astrophysics
journal, October 2014


Generation of scaled protogalactic seed magnetic fields in laser-produced shock waves
journal, January 2012

  • Gregori, G.; Ravasio, A.; Murphy, C. D.
  • Nature, Vol. 481, Issue 7382
  • DOI: 10.1038/nature10747

Laboratory observation of secondary shock formation ahead of a strongly radiative blast wave
journal, February 2006

  • Hansen, J. F.; Edwards, M. J.; Froula, D. H.
  • Physics of Plasmas, Vol. 13, Issue 2
  • DOI: 10.1063/1.2168157

Magnetohydrodynamic scaling: From astrophysics to the laboratory
journal, May 2001

  • Ryutov, D. D.; Remington, B. A.; Robey, H. F.
  • Physics of Plasmas, Vol. 8, Issue 5
  • DOI: 10.1063/1.1344562

Astrophysical blastwaves
journal, January 1988

  • Ostriker, Jeremiah P.; McKee, Christopher F.
  • Reviews of Modern Physics, Vol. 60, Issue 1
  • DOI: 10.1103/RevModPhys.60.1

The spectrum of the Sedov–Taylor point explosion linear stability
journal, June 2016

  • Sanz, J.; Bouquet, S. E.; Michaut, C.
  • Physics of Plasmas, Vol. 23, Issue 6
  • DOI: 10.1063/1.4953424

Similarity Criteria for the Laboratory Simulation of Supernova Hydrodynamics
journal, June 1999

  • Ryutov, D.; Drake, R. P.; Kane, J.
  • The Astrophysical Journal, Vol. 518, Issue 2
  • DOI: 10.1086/307293

The dynamics of the combustion products behind plane and spherical detonation fronts in explosives
journal, January 1950

  • Taylor, Geoffrey Ingram
  • Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences, Vol. 200, Issue 1061, p. 235-247
  • DOI: 10.1098/rspa.1950.0014

FLASH MHD simulations of experiments that study shock-generated magnetic fields
journal, December 2015


Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.