The effect of the number of active nuclei on the rate of heat transfer in large-volume nucleate boiling
Effect of number of active nuclei on heat transfer rate in large-volume nucleate boiling
NUCLEATE BOILING↗
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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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The formation of thin continuous films from isolated nuclei.
Kinetics of formation of thin continuous films from isolated three-dimensional nuclei
THIN FILM↗
The energy spectrum of cosmic-ray heavy nuclei of charge Z greater than 10 during a solar quiet time in July 1961.
Energy spectrum of cosmic ray heavy nuclei, using stack of nuclear emulsions exposed during Quiet Sun on balloon flight
NUCLEAR EMULSION↗
The propagation of cosmic-ray nuclei in interstellar space and solar system.
Cosmic ray nuclei propagation in interstellar space and solar system examined from balloon, rocket and satellite soundings
BALLOON SOUNDING↗
Observations on nuclei heavier than iron in the primary by cosmic radiation.
Primary cosmic radiation abundance measurements on iron and heavier nuclei, using Cerenkov counter on balloon flights
CERENKOV COUNTER↗
An apparently high flux of primary cosmic-ray He-nuclei at 41 deg N mag.
Unexpected excess of primary cosmic ray helium nuclei flux value in nuclear photographic emulsions
HEAVY NUCLEUS↗
Nuclear matrix elements for forbidden beta decay of spheroidal-shaped nuclei.
Nilsson model used to derive expressions for nuclear matrix elements, considering forbidden beta decay of spheroidal-shaped nuclei
PARTICLE EMISSION↗
The intensity of heavy nuclei in the primary cosmic rays over Texas in March 1962 and the solar cycle modulation.
Heavy nuclei intensity in primary cosmic rays, long term solar cycle modulation and time lag in various phases
SOLAR CYCLE↗
The disintegration of heavy nuclei at elevated temperatures
Proton, neutron and alpha particle emission rates for heavy nuclei in elevated temperatures calculated and tabulated
HIGH TEMPERATURE ENVIRONMENT↗
Particle-Induced Electromagnetic De-Excitation of Nuclei in Stellar Matter
Excited nuclei electromagnetic de-excitation rate by inelastic scattering in stellar particles calculated as function of temperature, density, transition energy and multipole functions
ATOMIC EXCITATION↗
Secondary particle spectra from the interaction of 30- to 340-Mev protons on complex nuclei - Experimental data and comparison with theory.
Neutron and proton spectra anomalies from proton- nuclei interactions in 100 Mev region
PROTON ENERGY↗
Case of generation of heavy nuclei in the sun
Flux increase of heavy nuclei in composition of cosmic rays during solar burst periods
Suslov, A. A.↗
Indirect quadrupole-quadrupole interactions of nuclei in metals
Energy of indirect quadrupole-quadrupole nuclei interactions with metal conduction electrons
Kessel, A. R.↗
Proton and helium nuclei cosmic ray spectra and modulations between 100 and 2,000 MeV/nucleon
Combination Cerenkov and scintillation detector, and range scintillator for proton and helium nuclei cosmic ray spectra between 100 and 2000 MeV/nucleon
Ormes, J. F.↗
Cerebellar projections to the vestibular nuclei
Anatomical relationship of cerebellum to vestibular nuclear complex, and cytological features of nuclei in vestibular and fastigial regions
Eager, R. P.↗
The survival of heavy nuclei in Colgate's supernova cosmic ray acceleration model
Survival of heavy nuclei in Colgates supernova cosmic ray acceleration model
Kinsey, J. H.↗
Charge and energy spectrum of heavy nuclei during the solar minimum, 1965.
Heavy nuclei charge and energy spectrum during solar minimum measured by balloon flight, using nuclear emulsions
Durgaprasad, N.↗
Cerenkov-scintillation counter measurements of nuclei heavier than helium in the primary cosmic radiation. I.
Energy spectra and charge composition of nuclei heavier than helium in primary cosmic radiation from Cerenkov scintillation counter measurements
Ormes, J. F.↗