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Eddington approximation | ||||
subject | fact |
Eddington approximation | has definition 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. | |
is a kind of stellar theory | ||
stellar theory | has domain star | |
theory | has validity correct or incorrect with caveats | |
has author or reasearch group | ||
has date or a range of dates for which the theory was active |