Infrared transmission properties of CO, HCl, and SO2 and their significance for the greenhouse effect on Venus
IR absorption properties of CO, HCl and sulfur dioxide measured for role in Venus greenhouse effect
Eberstein, I. J.↗
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The perturbation spectrum of CO
Perturbation rotational levels in triplet states of CO emission spectra attributed to resonance fluorescence process involving optically forbidden transitions
Black, G.↗
Measurement of the lifetime of the A super 1 pi state of CO by level-crossing spectroscopy
APi state lifetime of CO measured using molecular level crossing spectroscopy
Isler, R. C.↗
Oxidation of Co-10 w/o Cr interrupted by vacuum annealing
Vacuum annealing treatments effect on oxidation rate of Co-Cr alloy at high temperatures
Hed, A. Z.↗
Structured variations of the plasmapause - Evidence of a co-rotating plasmatail
Structured variations of plasmapause observed by OGO-D and evidence of co-rotating plasmatail
Grebowsky, J. M.↗
Production of CO(a 3 Pi) and other metastable fragments by electron impact dissociation of CO2
Dissociative excitation of CO(a 3 Pi) and other metastable fragments such as O(5S) produced by electron impact on CO2
Wells, W. C.↗
Spectra of Fe, Co, Ni, and Cu isoelectronic with Na I and Mg I
Highly ionized line spectra of Fe, Co, Ni and Cu belonging to Na I and Mg I isoelectronic sequences
Behring, W.↗
Lifetimes of metastable CO and N2 molecules
Metastable radiative lifetimes of molecular states of nitrogen and CO, using time of flight and high resolution electron gun techniques
Borst, W. L.↗
Photocatalytic production of organic compounds from CO and H2O in a simulated Martian atmosphere
Organic compounds biosynthesis in simulated Mars atmosphere, using UV irradiation for photocatalytic production from CO and water mixtures
Hardy, J. P.↗
The influence of manganese and silicon on the oxidation behavior of Co-20Cr
Manganese and silicon effects on oxidation and scale mechanisms of Co-Cr alloys, using thermogravimetric, metallographic and microprobe techniques
Armijo, J. S.↗
Interpretation of high resolution spectra of Mars. III - Calculations of CO abundance and rotational temperature
Mars atmospheric CO abundances and rotational temperature from Voigt line profiles
Young, L. D. G.↗
Excitation of the CO Fourth Positive band system by electron impact on carbon monoxide and carbon dioxide
CO Fourth Positive band system excitation cross sections by electron impact on carbon monoxide and carbon dioxide
Mumma, M. J.↗
Mapping of the oxidation products in the ternary Co-Cr-Al system
Ternary Co-Cr-Al alloy oxidation data, detailing kinetics, products, mechanisms, resistance behavior and rate
Hed, A. Z.↗
Selection of an alloy composition in the ternary Co-Cr-Al system for oxidation resistance
Ternary Co-Cr-Al alloy oxidation resistant composition selection, using oxide maps superimposed on phase diagram
Hed, A. Z.↗
Interstellar CO in the ultraviolet spectrum of zeta Ophiuchi
Optical methods in the vacuum ultraviolet were used to detect interstellar H2 in the spectrum of epsilon Persei; CO in the spectrum of zeta Ophiuchi was also observed. By contrast with radio results, the regions sampled are small, being one or a few clouds in the line of sight, and isotopic effects are detected in the spectrum.
Smith, A. M.↗
A curve of growth determination of the f-values for the fourth positive system of CO and the Lyman-Birge-Hopfield system of N2.
The curve of growth method has been employed to determine f-values for the fourth positive system of CO and the magnetic dipole and electric quadrupole components of the Lyman-Birge-Hopfield system of N2. No significant dependence on r-centroid was found. The mean value of the ratio of the electric quadrupole to magnetic dipole f-values was 0.076.
Pilling, M. J.↗
Transition moments, Franck-Condon factors, and lifetimes of forbidden transitions - Calculation of the intensity of the Cameron system of CO.
Discussion of the factors affecting the intensity of forbidden transitions in diatomic molecules. It is shown that using Franck-Condon factors to predict relative band intensities is less reliable for forbidden transitions than it is for allowed transitions. The intensity of the 0,0 and 1,0 bands of the a super 3 pi-super 1 sigma Cameron system of CO are calculated using perturbation theory. The intensity arises from spin-orbit mixing of the A super 1 pi state with the a super 3 pi state. From the known spin-orbit coupling constant of the a super 1 pi state and the known intensity of the fourth positive A super 1 pi-super 1 sigma transition, the oscillator strengths of the 0,0 and 1,0 bands are calculated to be 1.63 x 10 to the minus 7th power and 1.99 x 10 to the minus 7th power. Lifetimes of various rotational levels are shown to range from 2.9 to several hundred milliseconds.-
James, T. C.↗
Intensity measurements of the 0,0 band of the a/3 Pi/-Chi/1 Sigma/ Cameron system of CO.
The band strength of the 0,0 band of a CO Cameron system has been determined from measurements of the equivalent widths of a number of resolved rotational lines. Equivalent widths were converted to line strengths using a Doppler curve of growth. The result obtained agrees almost exactly with that of Fairbairn (1970).
James, T. C.↗