2022
DOI: 10.1007/s00340-022-07767-1
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Cross-calibration of a combined electrostatic and time-of-flight analyzer for energy- and charge-state-resolved spectrometry of tin laser-produced plasma

Abstract: We present the results of the calibration of a channeltron-based electrostatic analyzer operating in time-of-flight mode (ESA-ToF) using tin ions resulting from laser-produced plasma, over a wide range of charge states and energies. Specifically, the channeltron electron multiplier detection efficiency and the spectrometer resolution are calibrated, and count rate effects are characterized. With the obtained overall response function, the ESA-ToF is shown to accurately reproduce charge-integrated measurements … Show more

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Cited by 10 publications
(9 citation statements)
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References 33 publications
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“…Assuming an alignment of the grids where the grids are spaced such that they have minimal geometric overlap but the same orientation, the total transmission may be estimated to be 41 %. This figure was previously found to be consistent with an ion current comparison between the RFA and a grid-less Faraday cup [11].…”
Section: The Retarding Field Energy Analyzer (Rfa)supporting
confidence: 88%
See 3 more Smart Citations
“…Assuming an alignment of the grids where the grids are spaced such that they have minimal geometric overlap but the same orientation, the total transmission may be estimated to be 41 %. This figure was previously found to be consistent with an ion current comparison between the RFA and a grid-less Faraday cup [11].…”
Section: The Retarding Field Energy Analyzer (Rfa)supporting
confidence: 88%
“…Ions with higher charge may still be present but at negligible quantities. The individual charge-energy spectra follow trends similar to those seen previously using an electrostatic time-of-flight analyzer [11,22], with in particular the higher charge states bunching up to form the aforementioned high-energy peak.…”
Section: Rfa Spectrumsupporting
confidence: 79%
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“…The experimental measurements indicate a nearplateau in the ion energy distribution for kinetic energies in the 0.03-1 keV range, a peak near 2 keV followed by a sharp fall-off in the distribution for energies above 2 keV (red curve in figure 7). Charge-state resolved measurements, performed with a cross-calibrated electrostatic analyzer in time-of-flight mode (ESA-ToF) [107], attributed this peaked feature at 2 keV to the existence of peaks (centered near 2 keV) in the Sn 3+ − Sn 8+ ion energy distributions. To understand the physical origin of this peaked feature, Hemminga et al [106] performed two-dimensional simulations of the plasma initiation, growth and subsequent expansion using the radiation hydrodynamic code RALEF-2D.…”
Section: Plasma Expansion-'fast Ionic' Debrismentioning
confidence: 99%