The primary cosmic-ray electron spectrum between 0.09 and 8.4 Bev in 1965.
Primary cosmic ray electron energy spectrum from high altitude balloon measurements
Fanselow, J. L.↗
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Origin of primary cosmic radiation and its antiproton component.
Primary cosmic ray origin and acceleration and antiproton energy spectrum, using Fokker-Planck diffusion equation
Bowen, T.↗
The primary cosmic-ray electron spectrum in the energy range from 300 Mev to 4 Bev from 1964 to 1966.
Primary cosmic ray electron energy spectrum and flux density variations from balloon-borne counter telescope data
L'Heureux, J.↗
Long-term variations of the primary cosmic-ray electron component.
Long term variations of primary cosmic ray electron flux density from balloon-borne counter telescope data, noting absence of solar modulation
Dev Verma, S.↗
Primary protons and alpha particles in the energy range 70-240 Mev/nucleon observed during 1966.
Differential energy spectra of high energy primary cosmic ray protons and alpha particles from balloon flight data, noting solar activity effects
Badhwar, G. D.↗
Calculation of primary product quantum yields for photolysis reactions of glassy polymers
Calculating primary product quantum yields for photolysis reactions of irradiated glassy polymers
Gloria, H. R.↗
Hydrodynamics of a new concept of primary containment by energy absorption
Fluid dynamical analysis for idealized reactors system with spherical symmetry determines the effect which the destructive component of a nuclear accident produces on primary containment structures. Steel strands surrounding the reactor cavity in the biological shield exhibit plastic deformation to achieve the energy absorption.
Fistedis, S. H.↗
Primary radical yields in pulse irradiated alkaline aqueous solution
Primary radical yields of hydrated electrons, H atoms, and OH radicals are determined by measuring hydrated electron formation following a 4 microsecond pulse of X rays. The pH dependence of free radical yields beyond pH 12 is determined by observation of the hydrated electrons.
Fielden, E. M.↗
Evidence for a change of chemical composition of the primary cosmic radiation and a possible cause
Evidence for chemical composition changes in primary cosmic ray flux at high energies
Wayland, J. R.↗
Primary cosmic radiation Status report for period ending Aug. 1968
High altitude balloon flights for detecting primary cosmic rays
Friedlander, M. W.↗
Experimental investigation of a 10 deg conical turbojet plug nozzle with iris primary and translating shroud at Mach numbers from 0 to 2.0
Performance of 10 deg conical turbojet plug nozzle with iris primary and translating shroud for supersonic cruise applications
Bresnahan, D. L.↗
Primary cosmic-ray electrons between 17 MeV and 1 GeV in 1967
Balloon-borne detector observations of primary cosmic ray electrons between 17 MeV and 1GeV
Israel, M. H.↗
Experimental investigation of a 10 deg conical turbojet plug nozzle with translating primary and secondary shrouds at Mach numbers from 0 to 2.0
Static tests of nozzle efficiency and pumping characteristics of conical turbojet plug nozzle with translating primary and secondary shrouds at Mach 0 to 2.0
Bresnahan, D. L.↗
Development of high energy density primary batteries Final report, 31 May 1967 - 30 Apr. 1968
High energy density copper fluoride-lithium primary batteries
Abens, S. G.↗
Separation of primary and secondary particles in mass spectrometric investigations of the upper atmosphere
Primary and secondary particle separation in mass spectroscopy of upper atmosphere
Martykevich, G. M.↗
The relative energy spectra of carbon and oxygen nuclei in the primary cosmic radiation.
Energy spectra of carbon and oxygen nuclei in primary cosmic radiation, comparing results to earlier measurements and satellite observation
Ormes, J. F.↗
Problems in planning for the introduction of primary electric propulsion.
NASA long range planning of primary electric propulsion for automated space program
Edgecombe, D. S.↗
Vacuum-ultraviolet photochemistry. IX - Primary and chain processes in the photolysis of hydrogen peroxide.
Primary processes leading to atomic and molecular hydrogen formation in hydrogen peroxide photolysis at 1236 A, noting OH formation
Decarlo, V. J.↗