Production spectrum of high-energy electrons from high-energy cosmic-ray collisions.
Production spectrum of high energy electrons from high energy cosmic ray pion decay and proton- proton collisions
PARTICLE PRODUCTION↗
SEARCH · Search NASA
Results for “ENERGY”
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.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
A diurnal variation of the intensity and energy spectrum of low energy electrons incident at Ft. Churchill, Canada
Diurnal variations in intensity and energy spectrum of low energy electrons measured at Ft. Churchill, Canada
Webber, W. R.↗
Fine structure in the energy spectrum of low energy auroral electrons
Energy spectrum fine structure of low energy auroral electrons
Evans, D. S.↗
Low-energy cosmic-ray composition and energy spectra measured in June 1965.
Low energy cosmic ray composition and energy spectra measured by sounding rockets carrying nuclear emulsions
Fichtel, C. E.↗
Energy fluxes of low-energy protons and positive ions in the earth's inner radiation zone.
Differential energy spectra of low energy protons and positive ions in earth inner radiation zone, using electrostatic analyzers aboard OGO-3 satellite
Frank, L. A.↗
Retarded interaction energies between like atoms in different energy states.
Retarded long range interaction energies between two like atoms in different energy states, noting selection rules for resonant interactions
Meath, W. J.↗
Energy dependence of energy partition in products of direct reactions - Crossed-beam studies and a new model.
Initial kinetic energy dependence of reaction energy distribution between direct ion-molecule reaction products internal and translational modes from crossed beam experiments
Herman, Z.↗
Diurnal variation of the intensity and energy spectrum of low-energy electrons incident at Fort Churchill, Canada.
Low energy incident electron intensity and energy spectrum diurnal variations, measuring cut-off values
Webber, W. R.↗
Possible conversion of rotational energy of the neutron star in the Crab Nebula into energy of relativistic electrons.
Rotational energy conversion of neutron star into relativistic electrons energy suggested by increasing period of pulsating radio source in Crab Nebula
Finzi, A.↗
The isotopic abundances and energy spectra of super 2 H, super 3 He, and super 4 He of cosmic-ray origin in the energy region 10-100 Mev nucleon super-1
Cosmic ray origin in high energy H and He isotropic abundances and energy spectra observed by IMP 4 satellite during solar quiet times
Hsieh, K. C.↗
Disintegration and energy degradation of very high-energy cosmic rays in intense photon fields
Very high energy cosmic rays disintegration and energy degradation by intense blue shifted photon fields of supernovae quasars and pulsar models
Pollack, J. B.↗
Energy climbs, energy turns, and asymptotic expansions
Asymptotic expansions and energy methods applied to three dimensional aircraft maneuvers involving energy climbs and turns
Edelbaum, T. N.↗
Energy dependence of the 4610- and 4765-A lines of Ar/plus/ excited in low-energy He/plus/ plus Ar collisions
Energy dependence and threshold behavior of ion Ar lines excited in low-energy He ion-Ar collisions
Lipeles, M.↗
Measurement of the distribution in energy and angle of high-energy albedo neutrons and determination of an upper limit for the solar neutron flux
High energy albedo neutrons energy and angular distributions, determining solar neutron flux upper limit
Heidbreder, E.↗
Correlation of excess energies of dissociative electron attachment processes with the translational energies of their products
Dissociative electron attachment excess energy correlation with fragment ion translational energies, determining radical affinity
Bafus, D. A.↗
Energy losses of low-energy photoelectrons to thermal electrons
Asymptotic expression for low energy photoelectron energy loss to ambient thermal electrons
Hays, P. B.↗
Conversion of magnetic-field energy into kinetic energy in the solar wind
Solar wind velocity increase by magnetic field energy conversion to kinetic energy, constructing steady state MHD one fluid model
Whang, Y. C.↗
An assessment of solar energy as a national energy resource
The applications are discussed of solar energy for thermal energy for buildings; chemical and biological conversion of organic materials to liquid, solid, and gaseous fuels; and the generation of electricity. It is concluded that if solar development programs are successful, building heating for public use is possible within 5 years, building cooling in 6 to 10 years, synthetic fuels from organic materials in 5 to 8 years, and electricity production in 10 to 15 years.
Donovan, P.↗