A revised solar model with a solar neutrino spectrum.
Solar interior analysis based on improved formulas for generation rate of nuclear energy in combination with los alamos opacity code, spectrum defining neutrino
STELLAR SPECTRUM↗
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Results for “opacity”
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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An analysis of the Mariner 2 microwave observations of Venus.
Mariner 2 limb darkening measurements of Venus at microwave range, discussing peak brightness temperature and opacity models
Pollack, J. B.↗
Model atmospheres for late-type stars.
Stellar atmosphere model constructed to test opacity effect due to water vapor on model atmosphere structures
Auman, J. R., Jr.↗
The dry massive model of the atmosphere of Venus.
Microwave and IR opacities of dry massive model of Venus atmosphere
Thaddeus, P.↗
Technique for predicting temperature distribution in gases
Simple algebraic equations enable calculation of the temperature distribution throughout a heat generating, radiation gas. They apply over the entire range of opacities, for any heat flux, for a temperature dependent absorption coefficient, and for a non-uniform distribution of volumetric heat sources.
Kascak, A.↗
Phenomenological analysis of reactive scattering.
Angular distribution of reactive elastic scattering analyzed by opacity function /reaction probability/
Bernstein, R. B.↗
Dynamical stability in pre-main-sequence stars.
Dynamical stability in premain sequence stars, discussing adiabatic models for pure hydrogen composition and collapse initiation by low opacity
Dworetsky, M. M.↗
Effect of line absorption of main-sequence model stars.
Line absorption effect on opacity and main sequence model stars noting luminosity, radius and mass of convective core
Cesarsky, C. J.↗
Limb darkening on the earth's night side at wavelengths of 1-3 mu and 3-7.5 mu.
Limb darkening on earth night side observed by Aerobee rocket, with explanation based on atmospheric opacity in water vapor and carbon dioxide bands
Feldman, P. D.↗
A nongray CO sub 2 H sub 2 O greenhouse model of Venus.
Nongray greenhouse model of Venus atmosphere possessing IR opacity due to carbon dioxide, water and diatomic N compatible with Mariner 5 and Venera 4 results
Pollack, J. B.↗
Age and initial helium abundance of globular cluster stars.
Globular cluster star age and initial He abundance from main sequence, horizontal branch and red giant tip models using radiative opacities
Iben, I., Jr.↗
The revised solar abundance of iron and the solar neutrino flux
Solar core opacity influence on revised photospheric iron abundances, discussing neutrino flux prediction doubling in solar models
Watson, W. D.↗
Interferometric investigations of the atmosphere of Venus
Venus atmosphere opacity law determination as function of wavelength, comparing interferometric and integrated brightness temperatures with model calculations for various atmospheric compositions
Muhleman, D. O.↗
Metal-poor stars. II - Initial horizontal- branch models
Initial horizontal branch metal poor star models, examining opacities, luminosity and cluster ages of RR Lyrae stars
Rood, R. T.↗
Venus - Determination of atmospheric parameters from the microwave spectrum
Venus atmospheric parameters from microwave spectrum, discussing brightness temperature, carbon dioxide content, opacity, water vapor, dust and models
Morrison, D.↗
Stellar structure theory
Stellar structure theory, examining particle aggregates gravitational and pressure forces, energy flow, generation and opacity and equations of state
Iben, I., Jr.↗
Partition functions in ionizing plasmas
Ionizing plasmas partition functions, determining opacities and equations of state
Fischel, D.↗
The importance of methane to pressure-induced absorption in the atmospheres of the outer planets
Pressure-induced absorption in planetary atmospheres from hydrogen-methane collisions, stressing resulting thermal opacity
Fox, K.↗