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URLhttps://doi.org/10.18429/JACoW-EBIST2022-FR2WH03
TitleCharge-exchange factor in EBIT spectral analysis
Authors
  • Y. Yang, A. Hosier, E. Takacs
    Clemson University
  • A. Foster, A. Gall, N. Brickhouse, R. Smith
    Center for Astrophysics | Harvard & Smithsonian
  • A. Naing, D. Dipti, G. O'Neil, J. Tan, P. Szypryt, Y. Ralchenko
    National Institute of Standards and Technology
  • D. Schultz
    Northern Arizona University
AbstractSpectral analysis of an EBIT plasma requires an understanding of the ionization balance. Simulations require accurate atomic data (excitation, ionization, and recombination cross sections) and known operating conditions (electron beam density and energy, and trapped ion temperature). For highly charged ions in an EBIT, charge exchange (CX) recombination is significant despite the relatively low density of neutral ions. Uncertainties of the CX cross sections combined with the limited knowledge of the experimental parameters (neutral density, relative ion velocity) constrain the models of spectral emission. To combine the unknown factors into one free parameter, we introduce a charge exchange factor that can be accurately determined experimentally using measured line intensity ratios and theoretical cross sections. Using measured Fe spectra at multiple electron beam energies (9.21 kV x 18 kV), the charge exchange factor was determined in a measurement at NIST. The factor was used in our collisional-radiative (CR) model* to produce simulated spectra and line intensity ratios. The agreement demonstrates the usefulness of this approach for spectral modeling.
Paperdownload: FR2WH03.pdf
CiteBibTeX, LaTeX, Text/Word, RIS, EndNote
Conference14th International Symposium on EBIS/T
Series
LocationWhistler BC, Canada
Date14-17 Jun 2022
PublisherJACoW Publishing, Geneva, Switzerland
Editorial BoardOliver Kester, TRIUMF
Online ISBN978-3-95450-239-4
Online ISSNnone
Received29 November 2023
Revised19 December 2024
Accepted19 December 2024
Issued05 May 2025
DOI10.18429/JACoW-EBIST2022-FR2WH03
Pages30-33