Published 1991 | Version v1
Book

Analysis of time- and space-resolved Na-, Ne-, and F-like emission from a laser-produced bromine plasma

  • 1. Lawrence Livermore National Lab., Livermore, CA (United States)
  • 2. Nuclear Research Center of the Negev, Beer Sheva (Israel)
  • 3. Lawrence Berkeley Lab., CA (United States)

Description

Advance in the efficiency and accuracy of computational atomic physics and collisional radiative modeling promise to place the analysis and diagnostic application of L-shell emission on a par with the simpler K-shell regime. Coincident improvements in spectroscopic plasma measurements yield optically thin emission spectra from small, homogeneous regions of plasma, localized both in space and time. Together, these developments can severely test models for high-density, high-temperature plasma formation and evolution, and non-LTE atomic kinetics. In this paper they present highly resolved measurements of n = 3 to n = 2 X-ray line emission from a laser-produced bromine micro plasma. The emission is both space- and time-resolved, allowing them to apply simple, steady-state, 0-dimensional spectroscopic models to the analysis. These relativistic, multi-configurational, distorted wave collisional-radiative models were created using the HULLAC atomic physics package. Using these models, the authors have analyzed the F-like, Ne-like and Na-like (satellite) spectra with respect to temperature, density, and charge-state distribution. This procedure leads to a full characterization of the plasma conditions

Part of:
Radiative properties of hot dense matter

Additional details

Publishing Information

Publisher
World Scientific Publishing Co. Pte. Ltd.
Imprint Place
River Edge, NJ (United States)
ISBN
981-02-0665-8
Imprint Title
Radiative properties of hot dense matter
Imprint Pagination
392 p.
Journal Page Range
p. 215-220.

Conference

Title
4. international workshop on radiative properties of hot dense matter.
Dates
22-26 Oct 1990.
Place
Sarasota, FL (United States).

Optional Information

Secondary number(s)
CONF-9010298--.