z-logo
open-access-imgOpen Access
Comparison and analysis of 2-D simulation results with two implosion radiation experiments on the Los Alamos Pegasus I and Pegasus II capacitor banks
Author(s) -
Darrell L. Peterson,
R.L. Bowers,
C. Lebeda,
W. Matuska,
J.F. Benage,
G. C. Idzorek,
H. Oona,
John Stokes,
N. F. Roderick
Publication year - 1995
Language(s) - English
Resource type - Reports
DOI - 10.2172/102223
Subject(s) - implosion , physics , z pinch , radiation , optics , national ignition facility , hohlraum , nuclear physics , plasma , inertial confinement fusion , laser
Two experiments, PegI-41, conducted on the Los Alamos Pegasus I capacitor bank, and PegII-25, on the Pegasus II bank, consisted of the implosions of 13 mg (nominal), 5 cm radius, 2 cm high thin cylindrical aluminum foils resulting in soft x-ray radiation pulses from the plasma thermalization on axis. The implosions were conducted in direct-drive (no intermediate switching) mode with peak currents of about 4 MA and 5 MA respectively, and implosion times of about 2.5 {micro}s and 2.0 {micro}s. A radiation yield of about 250 kJ was measured for PegII-25. The purpose of these experiments was to examine the physics of the implosion and relate this physics to the production of the radiation pulse and to provide detailed experimental data which could be compared with 2-D radiation-magnetohydrodynamic (RMHD) simulations. Included in the experimental diagnostic suites were faraday rotation and dB/dt current measurements, a visible framing camera, an x-ray stripline camera, time-dependent spectroscopy, bolometers and XRD`S. A comparison of the results from these experiments shows agreement with 2-D simulation results in the instability development, current, and radiation pulse data, including the pulsewidth, shape, peak power and total radiation yield as measured by bolometry. Instabilities dominate the behavior of the implosion and largely determine the properties of the resulting radiation pulse. The 2-D simulations can be seen to be an important tool in understanding the implosion physics

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here