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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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Effective temperature for late type stars with or without water vapor opacity calculated for several masses, determining convective energy transport efficiency
FORTRAN program for computing stellar opacity from absorption spectra, electron scattering, and electron conduction data
Infrared opacity of hot water vapor based on stratoscope telescope observations of cool stars
Hot water vapor opacity effects on dispersion spectra of red giant stars, constructing stellar atmospheric models
Contribution of collision induced Fermi resonance band of carbon dioxide to Venus atmosphere opacity
Interim absorption coefficients and opacities for hydrogen plasma at high pressure
Lyman alpha wing opacity effect on temperature scale and helium content in F and G subdwarf atmospheres
Surface dielectric constant and microwave opacity of Venus atmosphere as function of wavelength determined by radar observations
Autoionization lines effect on stellar structure by computing contributions to Rosseland mean opacity
Photospheric radiation field role in temperature inversion of stellar chromospheres with dominant H ion opacity, postulating mechanical energy dissipation
Ballistic piston compressor for opacity measurements of hot compressible gases
Collective interactions effect on electron scattering opacity in stellar interiors, using Debye-Huckel radial distribution function and neglecting collisions
Opacity-probability distributions for CO, computing theoretical spectra of line absorption coefficient, discussing effects of temperature and/or turbulent velocity
Electrical conductivity and conductive opacity for relativistic electron gas in presence of ions taking into account ion-ion interaction
Free-free opacity of stellar interiors by ion correlations applied to red giant degenerate cores
Triatomic hydrogen ion role in solar photosphere opacity implied from limb darkening and specific intensity data
Massive homogeneous star pulsation stability, determining maximum mass by opacity formula
Magnetic field effects on Compton scattering and radiative opacity, considering longitudinal and transverse propagation with circular polarization