2014
DOI: 10.1016/j.hedp.2013.10.004
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Determination of magnetic fields based on the Zeeman effect in regimes inaccessible by Zeeman-splitting spectroscopy

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Cited by 20 publications
(12 citation statements)
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“…In the two methods described, B is obtained from comparison between line widths. This limits the minimum field magnitude measurable and requires high-accuracy line shape measurements and a high signal-to-noise ratio [5]. The third method, also applicable only when a dominant direction of ì B exists, is based on independently recording the full line shapes of the left-and right-handed circularly polarized components of Zeeman-split emissions observed along multiple chords through the plasma [21].…”
Section: The Two-polarizations Methodsmentioning
confidence: 99%
“…In the two methods described, B is obtained from comparison between line widths. This limits the minimum field magnitude measurable and requires high-accuracy line shape measurements and a high signal-to-noise ratio [5]. The third method, also applicable only when a dominant direction of ì B exists, is based on independently recording the full line shapes of the left-and right-handed circularly polarized components of Zeeman-split emissions observed along multiple chords through the plasma [21].…”
Section: The Two-polarizations Methodsmentioning
confidence: 99%
“…Here, we present an experimental determination of B θ throughout the magnetized plasma implosion, achieved using a noninvasive spectroscopic technique that provides a high sensitivity for the Zeeman effect [26]. This technique is based on the polarization properties of the Zeeman components for light emission viewed parallel to the B-field, as described in [27][28][29][30], and recently implemented for Z-pinch implosions [24].…”
mentioning
confidence: 99%
“…Since, the Zeeman splitting within each of the σ components is small ( 0.025Å for B = 1 T), each of the σ + and σ − line shapes is fitted with a Voigt profile, where the Gaussian part accounts for instrumental and Doppler broadening, and the Lorentzian part is due to the Stark broadening. B θ is then extracted from the wavelength difference between the peaks (∆λ) of the best fits (where B θ (T)= 5 × ∆λ(Å) [26], for the Ar III line), and n e is obtained from the Lorentzian width. Figures 2c,d are the same as Figs.…”
mentioning
confidence: 99%
“…Contrary to what had been believed, at most 1/3 of the discharge current was found to flow within the highly compressed stagnating plasma (SP). The direct confirmation of this study requires experimental measurements of B θ during the stagnation and close to the SP, a task that is extremely difficult due to the high electron density n e , the high ion velocities, and the transient nature of the plasma [21].…”
Section: Introduction -mentioning
confidence: 78%