Results 21 to 30 of about 34,429 (304)
A Table of the Radiative Opacities of a Number of Gas Mixtures.
Geoffrey Keller, R. E. Meyerott
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Radiative and Conductive Opacities for Eleven Astrophysical Mixtures.
A. N. Cox, John N. Stewart
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Radiative opacity tables for 40 stellar mixtures
Using improved methods, radiative opacities for 40 mixtures of elements are given for use in calculations of stellar structure, stellar evolution, and stellar pulsation. The major improvements over previous Los Alamos data are increased iron abundance in the composition, better allowance for the continuum depression for bound electrons, and corrections
A. N. Cox, J. E. Tabor
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The link between outgoing longwave radiation and the altitude at which a spaceborne lidar beam is fully attenuated [PDF]
According to climate model simulations, the changing altitude of middle and high clouds is the dominant contributor to the positive global mean longwave cloud feedback.
T. Vaillant de Guélis+6 more
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Adaptive Algorithm for the Generation of Superconfigurations in Hot-Plasma Opacity Calculations
In hot plasmas, such as the ones encountered in astrophysics or laser-fusion studies, the number of ionic excited states may become huge, and the relevant electron configurations cannot always be handled individually.
Jean-Christophe Pain
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Quantum Molecular Dynamics calculations of radiative opacities [PDF]
We show that Quantum Molecular Dynamics provides a powerful tool to extend and benchmark current opacities libraries into the complex regime of warm dense matter. In this regime, the medium can be constituted of electrons, protons, atoms and molecules, while plasma and many-body effects can not be treated as perturbations.
S. Mazevet+4 more
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Opacity Studies of Silicon in Radiatively Heated Plasma [PDF]
Measurements of the opacity of silicon at high temperature and high density are reported. A silicon dioxide foam was heated by eight nanosecond laser beams while a backlighter X-ray source was produced with a picosecond laser. Absorptions of the 1-2 transitions of Si XII through Si VI were observed in the wavelength range from 6.6 to 7.1 A.
Hui Wei+22 more
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The Radiative Transfer in Accretion Discs with Linear Plank Function: Role of Scattering Effect [PDF]
Radiative transfer in a geometrically thin accretion disc with fnite optical depth is considered under the plane-parallel approximation. The Eddington factor that is defned as the ratio of the mean intensity to radiation stress tensor, is assumed be ...
Fahimeh Habibi, Maryam Samadi
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Opacities and Atomic Diffusion
Opacity is a fundamental quantity for stellar modeling, and it plays an essential role throughout the life of stars. After gravity drives the collapse of interstellar matter into a protostar, the opacity determines how this matter is structured around ...
Georges Alecian, Morgan Deal
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Photoejection from Various Systems and Radiative-Rate Coefficients
Photoionization or photodetachment is an important process. It has applications in solar- and astrophysics. In addition to accurate wave function of the target, accurate continuum functions are required.
Anand K. Bhatia
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