Radiative heat exchange in the atmosphere by K. IНЎA KondratК№ev

Cover of: Radiative heat exchange in the atmosphere | K. IНЎA KondratК№ev

Published by Pergamon Press in Oxford, New York .

Written in English

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Subjects:

  • Atmosphere temperature.,
  • Energy budget (Geophysics)

Edition Notes

Bibliography: p. 383-406.

Book details

Statement[by] K. Ya. Kondratʹyev.
Classifications
LC ClassificationsQC880 .K6313 1965
The Physical Object
Paginationx, 411 p.
Number of Pages411
ID Numbers
Open LibraryOL5879421M
LC Control Number63010047

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Radiative transfer in the cloudy atmosphere B. Mayer a Deutsches Zentrum f¨ ur Luft- und Raumfahrt (DLR), Oberpfaenhofen, Wessling, Germany Abstract. Radiative transfer in clouds is a challenging task, due to their high spa-tial and temporal variability which is unrivaled by any other atmospheric Size: 1MB.

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The text first covers the basic definitions and concepts, and then proceeds to discussing. Radiation heat transfer is the mode of transfer of heat from one place to another in the form of waves called electromagnetic waves. Convection and conduction require the presence of matter as a medium to carry the heat from the hotter to the colder region.

Some common examples of Radiation are Ultraviolet light from the sun, heat from a stove burner, visible light from a candle, x-rays from. Radiative heat exchange of bodies in the atmosphere at large flight velocities was reported.

The results of calculations of the degree of blackness of the homogeneous flat air layer at the. The present paper considers the optical properties of the Venusian atmosphere (including the gaseous components, cloud formations and haze) and their effect on radiative heat exchange.

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Energy balance in the other hand, account for energy transfers trough all possible processes, namely radiation, conduction, sensible heat, latent heat. The problem of the influence of radiative flux divergence and turbulent heat exchange on temperature of the near-ground layer of the atmosphere is considered.

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The main difference between conduction, convection and radiation is Conduction is nothing but the heat transfer from the hotter part to the colder one. Convection is the heat transfer by up and down motion of the fluid. Radiation occurs when heat travels through empty space. For example using the emissivity of CO2 to calculate radiative heat transfer in the atmosphere with the standard Stefan-Boltzmann equation when you know the concentration of CO2 is, say, ppmV.

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I'm actually trying to create a benchmark problem for some FE calculations and I add increasingly complexity. The problem with my current PDE is that I really get unmeaningful results (negative temperature at t=0 on the surface) $\endgroup$ – .

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