Laboratory experiment is an attractive method of exploring the plasma physics that may occur in solar and astrophysical shocks. An experiment enables repeated and detailed measurements of a plasma as the input conditions are adjusted. To form a scaled experiment of an astrophysical shock a plasma physics model of the shock is required, and the important dimensionless parameters identified and reproduced in the laboratory. A laboratory simulation of a young supernova remnant is described. The experiment uses the interaction of two millimetre‐sized counter‐streaming laser‐produced plasmas placed in a strong transverse magnetic field to achieve this scaling. The collision‐free dynamics of the two plasmas and their interaction are studied with and without the magnetic field through spatially and temporally resolved optical measurements. Laboratory astroplasma physics experiments using high‐energy, high‐power laser technology enables us to reproduce in the laboratory the conditions of temperature and pressure that are met in extreme stellar environments.
Skip Nav Destination
,
,
,
,
,
,
Article navigation
7 April 2006
SUPERSTRONG FIELDS IN PLASMAS: Third International Conference on Superstrong Fields in Plasmas
19-24 September 2005
Varenna (Italy)
Research Article|
April 07 2006
Collisionless Plasma Astrophysics Simulation Experiments using Lasers Available to Purchase
N. C. Woolsey;
N. C. Woolsey
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
Search for other works by this author on:
A. D. Ash;
A. D. Ash
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
Search for other works by this author on:
C. Courtois;
C. Courtois
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
Search for other works by this author on:
R. O. Dendy;
R. O. Dendy
1UKAEA Culham Division, Culham Science Centre, Abingdon, OX14 3DB, United Kingdom
Search for other works by this author on:
C. D. Gregory;
C. D. Gregory
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
Search for other works by this author on:
I. M. Hall;
I. M. Hall
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
Search for other works by this author on:
J. Howe
J. Howe
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
Search for other works by this author on:
N. C. Woolsey
st
A. D. Ash
st
C. Courtois
st
R. O. Dendy
1
C. D. Gregory
st
I. M. Hall
st
J. Howe
st
*Department of Physics, University of York, York, Y010 5DD, United Kingdom
1UKAEA Culham Division, Culham Science Centre, Abingdon, OX14 3DB, United Kingdom
AIP Conf. Proc. 827, 365–375 (2006)
Citation
N. C. Woolsey, A. D. Ash, C. Courtois, R. O. Dendy, C. D. Gregory, I. M. Hall, J. Howe; Collisionless Plasma Astrophysics Simulation Experiments using Lasers. AIP Conf. Proc. 7 April 2006; 827 (1): 365–375. https://doi.org/10.1063/1.2195226
Download citation file:
Pay-Per-View Access
$40.00
Sign In
You could not be signed in. Please check your credentials and make sure you have an active account and try again.
Citing articles via
The implementation of reflective assessment using Gibbs’ reflective cycle in assessing students’ writing skill
Lala Nurlatifah, Pupung Purnawarman, et al.
Classification data mining with Laplacian Smoothing on Naïve Bayes method
Ananda P. Noto, Dewi R. S. Saputro
Effect of coupling agent type on the self-cleaning and anti-reflective behaviour of advance nanocoating for PV panels application
Taha Tareq Mohammed, Hadia Kadhim Judran, et al.
Related Content
Wakefield Acceleration in Relativistic Plasma Flows: Electron Acceleration to Cosmic Ray Energies
AIP Conf. Proc. (May 2007)
Scaling supernova hydrodynamics to the laboratory
Phys. Plasmas (May 1999)
Scaling laws for dynamical plasma phenomena
Phys. Plasmas (October 2018)
Collisionless Weibel shocks: Full formation mechanism and timing
Phys. Plasmas (July 2014)
Supernova Remnant Relevant Laser‐plasma Experiments
AIP Conf. Proc. (October 2004)