Detection of metastable atoms and molecules with continuous channel electron multipliers.
Detection of metastable He, H, Ne, Ar, Kr, Xe and molecular nitrogen with continuous channel electron multipliers
Donnelly, D. P.↗
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Experimental investigation of momentum exchange between argon and krypton beams incident on clean gold surfaces
Electromagnetic torsion balance measurement of forces exerted on clean Au surfaces by monoenergetic steady state Ar and Kr beams, calculating thermal accommodation coefficients
Mcginn, J. H.↗
White light laser
White light laser construction using Ar-Kr laser with suitable mixture and pressure of gases to provide equal output intensities of red, yellow, green and blue
Billman, K. W.↗
Radiation characteristics from high power noble gas arcs
Spectral radiation and polar distribution from high power Ar, Kr and Xe arcs
Decker, A. J.↗
Rare gases in Apollo 11 lunar material
Apollo 11 lunar fines, breccia and crystalline rocks rare gas data, emphasizing trapped and spallation Ne, Kr and Xe isotopic compositions
Black, D. C.↗
Gas chromatographic determination of hydrogen, nitrogen, oxygen, methane, krypton, and carbon dioxide at room temperature
Hydrogen, N, O, Kr methane and carbon dioxide gas chromatographic examination, discussing life detection device for Mars landing
Carle, G. C.↗
Noble gases in the atmosphere between 43 and 63 kilometers
Upper stratosphere and mesosphere concentrations of Ne, Ar, and Kr from rocket-borne cryogenic air sampler
Bieri, R. H.↗
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↗
New CW ion laser transitions in argon, krypton, and xenon
CW ion laser transitions in Ar, Kr and Xe, tabulating threshold data
Hodges, D. T.↗
Isotopic composition of xenon and krypton in the lunar soil and in the solar wind
Xe and Kr isotopes gas extraction and mass spectrometer analyses of Apollo 11 lunar soil, Murray carbonaceous chondrite and atmospheric Xe
Burnett, D. S.↗
Inert gases from Apollo 11 and Apollo 12 fines - Reversals in the trends of relative element abundances
Primordial Kr and Xe trapping as possible cause of element abundance trend reversal in Apollo 11 and 12 fines
Heymann, D.↗
Adsorption on the Martian regolith
Mars regolith carbon dioxide, water and Kr adsorption, explaining diurnal brightness phenomena
Cannon, W. A.↗
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.↗
Lunar fines and terrestrial rock powders - Relative surface areas and heats of adsorption
Apollo 11 lunar fines and ground terrestrial mafic rock powders effective surface areas and heats of adsorption, using Brunauer-Emmett-Teller Kr adsorption method
Cannon, W. A.↗
Stepwise heating analyses of rare gases from pile-irradiated rocks 10044 and 10057
Ar, Kr and Xe emanation during stepwise heating of lunar rocks under slow neutron irradiation in pile, using mass spectroscopy
Davis, P. K.↗
Visible and near ultraviolet spectra of low- pressure rare-gas microwave discharges
Visible and near UV spectra of vacuum Ar, Kr and Xe microwave discharge lamps with magnesium fluoride windows
Bowman, R. L.↗
Nuclear tracks in lunar samples
An attempt is made to relate the appearance of an etched tract to the atomic number and velocity of the ion that left it using 10 MeV/nucleon Kr beams and 6 MeV/nucleon Zn beams. It was found that the etching rate along a tract in minerals and glass is a monototonic function of ionization rate thus, making particle identification possible. Results show the following were present in lunar samples: superheavy elements, cosmic rays with z greater than 26, and solar flare particles in Surveyor glass.
Price, P. B.↗
A case for catastrophic early degassing of the earth.
Evidence is given for the occurrence in early earth history of massive escape of volatiles from the interior of the earth to its surface, which must have had catastrophic proportions. The mechanism and time of this event are inferred from the abundances and distribution of volatiles in the atmosphere, hydrosphere and crust, and from meteorite studies, and geophysical and astronomical observations. This event is linked to the melting of the earth during accretion which resulted in the concentration of U, Th, K and Pb in the outermost portion of the earth and in virtually complete expulsion of nonradiogenic Ar, Ne and Kr from its interior.
Fanale, F. P.↗