Solving the radiative
transfer equations through the atmosphere requires knowledge of the absorption spectra of each gas.
Not exact matches
In the classic heat -
transfer equation, the rate of temperature change depends on how uniformly the thermal energy is distributed
through an object.
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Well, the only way to work out the «expected» results — or what the theory predicts — is to solve the radiative
transfer equations (RTE) for that vertical profile
through the atmosphere.
To compute what happens quantitatively, one must solve the
equations for radiative
transfer absorption - line by absorption - line
through the atmosphere.
«Robert H. Essenhigh developed a comprehensive thermodynamic model of the lapse rate based on the Schuster - Schwarzschild integral (S - S)
Equations of
Transfer that govern radiation
through the atmosphere including absorption and radiation by greenhouse gases»