skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: On the transparency of foam in low-density foam {ital Z}-pinch experiments

Journal Article · · Review of Scientific Instruments
DOI:https://doi.org/10.1063/1.1149476· OSTI ID:295613
 [1]; ; ;  [2];  [3]
  1. Prism Computational Sciences, Inc., Madison, Wisconsin 53703 (United States)
  2. Sandia National Laboratories, Albuquerque, New Mexico 87185 (United States)
  3. Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)

{ital Z}-pinch experiments have been performed on the SATURN and {ital Z} machines at Sandia National Laboratories to study physics issues related to x-ray radiation generation and inertial confinement fusion. Some of these experiments utilize a CH foam located on-axis to convert energy to radiation and act as a radiative transfer volume. A significant issue for foam {ital Z}-pinch experiments is the transparency of the heated foam as a function of time and wavelength. Foam transparency will be important in future foam {ital Z}-pinch experiments both because it influences the time-dependent radiation field seen by an inertial confinement fusion capsule embedded in the foam, and because it is an important factor in making high-resolution spectral measurements of a capsule or tracers embedded in the foam. In this article, we describe results from simulations and experiments which address the issue of foam transparency. We discuss imaging data from one {ital Z} experiment in which x-ray emission from a half-Au/half-CH disk located at the bottom of a 1-cm-tall, 14 mg/cc TPX foam is observed. Simulation results predicting CH foam optical depths as a function of plasma conditions are presented. In addition, we present results from spectral calculations which utilize 2D magnetohydrodynamic (MHD) simulation predictions for the time-dependent foam conditions. Our results indicate that the observed x-ray framing camera images are consistent with early-time (several ns prior to stagnation) foam electron temperatures of {approx_gt}30 eV, which is somewhat hotter than the foam electron temperatures predicted from the 2D MHD simulations at early times. {copyright} {ital 1999 American Institute of Physics.}

OSTI ID:
295613
Report Number(s):
CONF-980605-; ISSN 0034-6748; TRN: 99:001799
Journal Information:
Review of Scientific Instruments, Vol. 70, Issue 1; Conference: 12. topical conference on high-temperature plasma diagnostics, Princeton, NJ (United States), 7-11 Jun 1998; Other Information: PBD: Jan 1999
Country of Publication:
United States
Language:
English