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A Simplified Model Solar Atmosphere
Solar Physics, 1968A simplified representation of the temperature distribution in the solar photosphere is proposed: θ (τ 0) = θ 0 – θ 1 logτ 0. An expression is derived for the emergent continuous spectrum from the simple model. The limitations and applications of the simple model are discussed.
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Solar photo rates for planetary atmospheres and atmospheric pollutants
Astrophysics and Space Science, 1992Unattenuated solar photo rate coefficients and excess energies for dissociation, ionization, and dissociative ionization are presented for atomic and molecular species that have been identified or are suspected to exist in the atmospheres of planets, satellites (moons), comets, or as pollutants in the Earth atmosphere.
W. F. Huebner, J. J. Keady, S. P. Lyon
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Electrodynamics of the Outer Solar Atmosphere
Space Science Reviews, 1983The structure of the outer solar atmosphere and its magnetic coupling to the photospheric motions indicate the existence of large-scale current systems. The heating and the dynamics of coronal structures is therefore governed by electrodynamic coupling of these structures to the underlying photosphere.
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Degradation mechanisms of perovskite solar cells under vacuum and one atmosphere of nitrogen
Nature Energy, 2021Richard Henry Friend +2 more
exaly
Atmospheric and solar neutrinos
Nuclear Physics B - Proceedings Supplements, 2000openaire +2 more sources
Metal-organic frameworks for solar-driven atmosphere water harvesting
Chemical Engineering Journal, 2023Zhizhen Ye, Xinsheng Peng
exaly
Solar and Atmospheric Neutrinos
Particles, Strings and Cosmology (PASCOS 99), 2000openaire +1 more source
Philosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2021
Bernhard Fleck +2 more
exaly
Bernhard Fleck +2 more
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