1981
DOI: 10.1016/0022-4073(81)90057-1
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Measurement of refractive indices of neon, argon, krypton and xenon in the 253.7–140.4 nm wavelength range. Dispersion relations and estimated oscillator strengths of the resonance lines

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Cited by 119 publications
(66 citation statements)
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“…We present in fig.10 the dispersive behaviour of A(ω) as a function of the photon energyhω. The open circles are the VUV measurements [18] obtained at low density (p ≈ 1 Atm). The dashed line is the fit to those points.…”
Section: Vuv Light Propagation In Liquid Xenonmentioning
confidence: 99%
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“…We present in fig.10 the dispersive behaviour of A(ω) as a function of the photon energyhω. The open circles are the VUV measurements [18] obtained at low density (p ≈ 1 Atm). The dashed line is the fit to those points.…”
Section: Vuv Light Propagation In Liquid Xenonmentioning
confidence: 99%
“…λ R vs n from equation (15) (black circles) is presented in fig.11. The input values for the refractive index n(ω) are the ones obtained from a fit to the low pressure VUV measurements [18]. The simple Clausius-Mossotti relation (4) (and its linearity as a function of ρ m ) is assumed to be valid.…”
Section: Vuv Light Propagation In Liquid Xenonmentioning
confidence: 99%
“…The linear medium properties were described in terms of tabulated frequency-dependent susceptibility based on Sellmeier formulas taken from Ref. [35] (and from refractiveindex.info for Ne).…”
Section: Simulation Of Optical Filamentsmentioning
confidence: 99%
“…We chose argon for this calibration procedure because its refractive index is known to be jð121:6 nmÞ ¼ 1:000502 at n R;0 ¼ 2:687 Â 10 19 cm À3 [8,9]. The corresponding Rayleigh crosssection for transverse observation amounts to dr= dX ¼ 6:265 Â 10 À25 cm 2 .…”
Section: Calibration With Rayleigh Scattered Radiation From Argonmentioning
confidence: 99%