Excitation cross section for some of the doubly ionized states of argon, neon, and krypton by fast electrons.
Excitation cross section for double ionized states of Ar, Ne and Kr due to fast electron impingement on neutral atom
Koozekanani, S. H.↗
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Noise mechanisms in the helium-neon laser
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Roberts, V.↗
Calculations of ionization equilibria for oxygen, neon, silicon, and iron.
O, Ne, Si and Fe ionization equilibria in low density plasma, including dielectronic recombination and autoionization processes in calculations
Allen, J. W.↗
Experimental observation of continuity-equation oscillations in slightly ionized deuterium, neon and helium gas.
LF oscillations in electron number density of ionized deuterium, Ne and He identified from particle continuity equation
Roth, J. R.↗
Shock-tube thermochemistry tables for high-temperature gases - Helium, neon, and argon, volume 3 Technical report
Shock tube thermochemistry tables for high temperature gases
Horton, T. E.↗
Field adsorption and desorption of helium and neon
He and Ne adsorption and desorption on field ion microscope tip, determining minimum required field strengths of gas films at different temperatures
Mclane, S. B.↗
Neutral neon in the visible solar spectrum
Neutral Ne emission line in visible solar spectrum during bright events in inner corona, noting 1958 outburst of RS Oph
Dietz, R. D.↗
Multistate impact-parameter calculation of atom-atom excitation cross sections - Excitation of atomic hydrogen by neon, argon, and krypton
Hydrogen and inert gas atoms collisional excitation cross sections calculated by multistate impact parameter approximation
Levy, H., II↗
GASP - A computer code for calculating the thermodynamic and transport properties for eight fluids - Helium, methane, neon, nitrogen, carbon monoxide, oxygen, argon, carbon dioxide
Computer programs for calculation of thermodynamic and transport properties of eight cryogenic fluids
Baron, A.↗
Born wave cross section calculations for the excitation of He/1 super 1 S/ to He/N super 1 L/ by helium, neon, argon and krypton
He excitation by He, Ne, Ar and Kr collisions, calculating first Born wave cross section
Levy, H., II↗
Measurement of the Stark broadening of the resonance lines of neutral argon and neon
Neutral Ar and Ne resonance lines Stark broadening constant from Stark width-oscillator strength product
Greig, J. R.↗
Single-electron capture by C/4 plus/ in helium, neon, and argon below 40 keV
Cross sections for single-electron capture by C/4 plus/ from He, Ne and Ar target gases
Koopman, D. W.↗
Isotope effects in the specific heat of solid neon
Solid Ne isotopes specific heat at constant pressure and volume, entropy, enthalpy and Gruneisen parameters
Fenichel, H.↗
Shock tube investigation of bromine dissociation rates in the presence of helium, neon, argon, krypton, and xenon
Bromine dissociation rates in presence of He, Ne, Ar, Kr and Xe, determining rate constant expressions from light absorption measurements behind incident shock waves
Warshay, W.↗
Distribution and origin of helium, neon, and argon isotopes in Apollo 12 samples measured by in situ analysis with a laser-probe mass spectrometer
He, Ne and Ar isotopic distribution and origin in Apollo 12 lunar samples, considering solar wind implantation
Megrue, G. H.↗
Short-range correlations in carbon-12, oxygen-16, and neon-20: Intrinsic properties
The Brueckner-Hartree-Fock (BHF) method has been applied to nuclei whose intrinsic structure is nonspherical. Reaction matrix elements were calculated as functions of starting energy for the Hamada-Johnston interaction using the Pauli operator appropriate to O-16 and a shifted oscillator spectrum for virtual excited states. Binding energies, single particle energies, radii, and shape deformations of the intrinsic state, in ordinary as well as renormalized BHF, are discussed and compared with previous HF studies and with experiment when possible. Results are presented for C-12, 0-16 and Ne-20. It is found that the binding energies and radii are too small, but that separation energies are well reproduced when the renormalized theory is used.
Braley, R. C.↗
Solar wind rare gas analysis: Trapped solar wind helium and neon in Surveyor 3 material
The He-4 and Ne-20 contents in sections of the Surveyor 3 support strut samples were determined by optical and scanning electron microscopy and are compared to the results of the Apollo solar wind composition (SWC) experiments. The He-4/Ne-20 ratio in the samples from the sunlit side of the strut was approximately 300; the ratios determined in Apollo 12 lunar fines and SWC foil were below 100. The He-4/He-3 ratios were also determined, and the ratio obtained from Surveyor 3 material is higher than those found with Apollo 11 and 12 SWC experiments. The effects of spallation by cosmic rays or solar protons, stripping by cosmic ray or energetic solar alpha particles, recycling of solar wind He and radiogenic Ne, He from terrestrial atmosphere, mass discrimination near the moon, mass dependence of trapping probability, diffusion, and contamination by lunar dust are considered.
Buehler, F.↗
New lines of neon ions in the range 50-200 A.
About 180 new spectral lines of Ne V, Ne VI, Ne VII, and Ne VIII have been measured and identified on spectrograms obtained from a large theta-pinch apparatus. The spectrograms covered the range from 50 to 200 A. The lines were classified by means of isoelectronic extrapolations and interpolations.
Hermansdorfer, H.↗