Tables Related to Radiation Emerging from a Planetary Atmosphere with Rayleigh Scattering. [By] K.L. Coulson, Jitendra V. Dave, Zdenek Sekera PDF Download
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Author: Kinsell L. COULSON
Publisher:
ISBN:
Category :
Languages : en
Pages : 548
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Author: Kinsell L. COULSON
Publisher:
ISBN:
Category :
Languages : en
Pages : 548
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Author:
Publisher: Univ of California Press
ISBN:
Category :
Languages : en
Pages : 564
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Author: Kinsell L. Coulson
Publisher:
ISBN:
Category : Radiation
Languages : en
Pages : 568
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Author: British Museum. Department of Printed Books
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ISBN:
Category : English imprints
Languages : en
Pages : 512
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Author: British Library
Publisher:
ISBN:
Category : English imprints
Languages : en
Pages : 538
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Author:
Publisher:
ISBN:
Category : Union catalogs
Languages : en
Pages : 630
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Includes entries for maps and atlases.
Author: Anne B. Kahle
Publisher:
ISBN:
Category : Astrophysics
Languages : en
Pages : 22
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Calculations of the total radiation emerging from planetary atmospheres optically thicker than those of the earth. For Rayleigh scattering and Lambert reflectivity, the flux is determined for a wide range of solar elevations, ground reflectivities, and optical depths. For very large surface reflectivities there is more radiation downward onto a planet at the bottom of a thick atmosphere than is received at the top because the radiation that does penetrate undergoes multiple reflection. The total radiation absorbed by the surface plus the corresponding diffuse upward radiation always equals the input flow. Bond albedo is determined by numericaly integration. It approaches the value of the ground reflectivity as optical thickness approaches zero, and approaches 1 as it becomes very large. (Author).
Author: British Library
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ISBN:
Category : Best books
Languages : en
Pages : 640
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Author: D. Deirmendjian
Publisher:
ISBN:
Category : Light
Languages : en
Pages : 398
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Author: K. L. Coulson
Publisher:
ISBN:
Category : Atmospheric radiation
Languages : en
Pages :
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