Numerical simulation of the Zeeman effect in neutral xenon from NIR diode-laser spectroscopy

We present a numerical method for simulating neutral xenon absorption spectra from diode-laser spectroscopy of the Zeeman-split 6 S ′ [ 1 / 2 ] → 6 P ′ [ 1 / 2 ] line at 834.682 nm-air in a galvatron's plasma. To simulate the spectrum, we apply a Voigt profile to a spectrum of σ -transition lin...

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Veröffentlicht in:Journal of applied physics 2008-07, Vol.104 (2), p.023303-023303-14
Hauptverfasser: Ngom, Baïlo B., Smith, Timothy B., Huang, Wensheng, Gallimore, Alec D.
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container_issue 2
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container_title Journal of applied physics
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creator Ngom, Baïlo B.
Smith, Timothy B.
Huang, Wensheng
Gallimore, Alec D.
description We present a numerical method for simulating neutral xenon absorption spectra from diode-laser spectroscopy of the Zeeman-split 6 S ′ [ 1 / 2 ] → 6 P ′ [ 1 / 2 ] line at 834.682 nm-air in a galvatron's plasma. To simulate the spectrum, we apply a Voigt profile to a spectrum of σ -transition lines of even- and odd-numbered isotopes computed from anomalous Zeeman and nonlinear Zeeman hyperfine structure theories, respectively. Simulated spectra agree well with Zeeman-split spectra measured from 30 to 300 G. A commercial nonlinear least-squares solver (LSQNONLIN) returns field strengths and translational plasma kinetic temperatures that minimize the error between simulated and experimental spectra. This work is a preamble to computing magnetic field topology and the speed distribution of neutral xenon particles in the plume of a Hall thruster from diode laser-induced fluorescence.
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subjects ABSORPTION SPECTRA
APPROXIMATIONS
CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS
ELECTRON TEMPERATURE
FLUORESCENCE
HYPERFINE STRUCTURE
INFRARED SPECTRA
ION TEMPERATURE
LASER SPECTROSCOPY
LEAST SQUARE FIT
MAGNETIC FIELDS
NONLINEAR PROBLEMS
PLASMA
PLASMA DIAGNOSTICS
PLASMA SIMULATION
SEMICONDUCTOR LASERS
TOPOLOGY
XENON
ZEEMAN EFFECT
title Numerical simulation of the Zeeman effect in neutral xenon from NIR diode-laser spectroscopy
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