The analysis of microwave recombination lines
Microwave recombination H lines, deriving electron temperature, electron density and emission measure sequentially
Cesarsky, D.↗
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Detection and identification of recombination lines from an H I region
Hydrogen I region anomalous alpha lines recombination in Orion B spectrum, identifying carbon emitter by measured frequency separation
Ball, J. A.↗
Recombination of iodine atoms in dilute solutions of argon
Recombination of iodine atoms in dilute argon solutions studied by flash photolysis
Blake, J. A.↗
Use of the third electrode and the recombination electrode in spacecraft batteries
Third electrode and recombination electrode in nickel cadmium battery system of spacecraft
Ford, F. E.↗
Characterization of control and recombination electrodes
Characterization and control of recombination electrodes in nickel cadmium cells
Seiger, H. N.↗
Effects of columnar recombination on conductivities of nuclear seeded plasmas
Nonlinear effects of recombination and collective diffusion associated with nuclear seeded plasmas using helium isotopes in gas cooled reactors
Dalton, G. R.↗
Ion-ion recombination total cross sections - Atomic species
Atomic ion-ion recombination total inelastic cross sections calculation by Landau-Zener method, noting agreement with experiment
Moseley, J.↗
Kinetics of electron reflection and ion recombination on insulator surfaces
Cs vapor filled cracks breakdown in thermionic trilayer insulators, calculating electron reflection and ion recombination kinetics on surfaces
Kniazzeh, A. G. F.↗
Yield of O/super 1 D/ by dissociative recombination of O2/plus/ from night airglow observations
Singlet-D atomic O yield per oxygen ion dissociative recombination from night airglow observations
Forbes, J. M.↗
Surface recombination of hydrogen molecules
Molecular hydrogen formation on dust grain surfaces, discussing recombination efficiency as function of surface temperature
Hollenbach, D.↗
Computer study of nonequilibrium excitation in recombining nitrogen plasma nozzle flows
Nonequilibrium excitation in recombining nitrogen plasma nozzle flows
Bowen, S. W.↗
Radiative electron-ion recombination into the first excited state of lithium
Li photoionization cross sections determined from spectral intensity measurements as function of threshold wavelength, discussing radiative electron-ion recombination into first excited state
Rothe, D. E.↗
Hydrogen recombination by nonactivated chemisorption on metallic grains
Hydrogen recombination and molecule formation by nonactivated chemisorption on iron grains surfaces
Arrhenius, G.↗
Output pulse amplitude from lithium-drifted detector-amplifier combination under conditions of carrier diffusion and bulk and surface recombination
Output pulse amplitude from lithium-drifted detector-amplifier combination under conditions of carrier diffusion and bulk and surface recombination
Tuzzolino, A. J.↗
Measurement of C/plus/ plus e/minus/ plus e/minus/ and CO/plus/ plus e/minus/ recombination in carbon monoxide flows
Carbon ion and free electrons three body recombination rate coefficient measurement in carbon monoxide flows
Dunn, M. G.↗
Measurements of recombination of electrons with H3O(plus)-(H2O)n series ions
Recombination coefficients of electrons with ions of the hydrated hydronium ion series (H3O(+))(H2O)n, where n = 0, 1, 2, 3, 4, 5, 6, were determined with a microwave afterglow/mass spectrometer apparatus. Afterglow measurements of electron density decays in helium-water vapor mixtures are correlated with the decay of mass-identified ion currents to the wall of the microwave cavity. By varying the temperature of the gas and the partial pressure of the water vapor in the mixture, different groups of hydronium series ions are made to dominate the afterglow.
Leu, M. T.↗
Radiofrequency recombination lines as diagnostics of the cool interstellar medium.
Quantitative details are given of a new diagnostic technique for the carbon and hydrogen (H I) recombination lines. Theoretical results are presented for conditions expected in H I clouds, and are compared with available observations for Orion A and NGC 2024.
Dupree, A. K.↗
6300 A quantum efficiency of the recombination mechanism in the night-time F layer.
Simultaneous airglow and electron content measurements made at Hawaii are used to infer the number of 6300 and 6364 A quanta produced per electron lost in the nighttime F layer of the ionosphere. The equation of continuity of electrons is then solved numerically to obtain the electron density profile, and the amount of quenching is estimated. This leads to the number of excitations of O(super-1 D) per O2(+) recombination (epsilon). We find, for an exospheric temperature of 1100 K, epsilon is equal to 1.1 plus or minus 0.6, in good agreement with Zipf's laboratory measurement at 300 K.
Brown, W. E.↗