Design and simulation of the potential of lead-free Ag<sub>3</sub>Bi<sub>1.1</sub>I<sub>6.3</sub> perovskite solar cells with different charge transport for energy enhancement. [PDF]
Islam MA+11 more
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Study of the spectral opacities in the stellar radiative interiors
M. Le Pennec
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Tempests in the troposphere: Mapping the impact of giant storms on Jupiter's deep atmosphere. [PDF]
Moeckel C, Ge H, de Pater I.
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Expanding the Interface: Overlooked Dermatologic Disorders With Ocular Involvement
JEADV Clinical Practice, EarlyView.
A George
wiley +1 more source
The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets. [PDF]
Krissansen-Totton J+3 more
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Opacity and radiative power losses calculations
High Energy Density Physics, 2009In this contribution we present results on opacity and radiative power losses in laser-produced plasmas. We focus our attention on the inner shell transition array 1s-2p in an aluminum plasma. At high densities, electron, Doppler and ion Stark broadening play a role in line merging.
Benredjem, D., Calisti, A., Mosse, C.
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Scaling law of radiative opacities for ICF elements
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2001info:eu-repo/semantics ...
Mínguez, E.+5 more
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Radiative opacities for stellar envelopes
Physica Scripta, 1995Recent advances in the field of opacity calculations for stellar envelopes are summarized. The methods used and the results obtained in the last decade by two independent groups are discussed briefly. Some of the important effects of the new data on astrophysical studies are outlined.
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The Effect of Degeneracy on the Scattering Contribution to the Radiative Opacity [PDF]
The effect of partial free electron degeneracy on the scattering contribution to the radiative opacity is of interest in calculations of the structure and evolution of stars, particularly the Sun, where the plasma at the Sun's center is partially degenerate and scattering is a major contribution to the opacity.
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