Interpret every logarithm in the empirical profile as base ten with the dimensionless argument . PutThe upper atmosphere has for , while integration of below it givesAssume that the stated planetary equilibrium temperature is a reasonable brightness temperature at the photosphere. ThenAt , , and thereforeThis estimate neglects day-night variation, wavelength-dependent photospheric pressure, and a possible radiative-convective boundary; it treats the retrieved profile as representative of the dayside disk.
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