Radiative transfer is one of the most fundamentally important concepts in astrophysics.
Radiative Transfer
The process by which radiation travels through a medium.
Radiative Viscosity ...
Radiative transfer is the physical phenomenon of energy transfer in the form of electromagnetic radiation. The propagation of radiation through a medium is affected by Absorption , Emission and scattering processes....
Radiative Transfer - The transport of energy by electromagnetic radiation
Radio Galaxy - A galaxy that is a strong source of radio radiation
Radioactivity - The spontaneous disintegration of an unstable nucleus of an atom ...
Radiative Transfer. New York: Dover. ISBN 0486605906.
Chandrasekhar, S. (1975) [1960]. Plasma Physics. Chicago: The University of Chicago Press. ISBN 0226100847.
Chandrasekhar, S. (1981) [1961]. Hydrodynamic and Hydromagnetic Stability.
The radiation zone is the region within the stellar interior where radiative transfer is sufficiently efficient to maintain the flux of energy. In this region the plasma will not be perturbed and any mass motions will die out.
(where r is a vector position); which expression is, like the equation of radiative transfer, complete but practically useless.
An approximation used in the study of radiative transfer. It is the assumption that the ratio of the second moment of the radiation field to the mean intensity is everywhere equal to 1/3, the value of this ratio for an isotropic field. [H76] ...
Ground-Truth Analysis of Radiative Transfer in the Jovian Atmosphere (IDS)
Dr. Glenn S. Orton
Composition of the Jovian Atmosphere (IDS) ...
Introduction to the Study of Stellar Structure Hydrodynamic and Hydromagnetic StabilityRadiative Transfer
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Astronomy Dictionary ...
Cloud physics, broadly considered, embraces not only the study of condensation and precipitation processes in clouds, but also radiative transfer, optical phenomena, electrical phenomena, ...
 See also: Atmosphere, Temperature, Time, Emission, Model
  
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