GC115-0013
Clear-sky, Cloudy-sky and All-sky Global Mean Energy Budgets as the Solution of Classic Theoretical Radiative Transfer Constraint Equations
Abstract:
The set of these equations has a solution for LWCRE = 1 as unit flux, and the whole system of the atmospheric energy flows can be described by small integers, in their own units, separately for the clear-sky, the cloudy sky and (as their result) for the global mean all-sky case. OLR(all) = 9, OLR(clear) = 10, ULW = 15, G(all) = 6, G(clear) = 5 units = 133.40 Wm-2 with TSI = 51 units = 1360.68 ± 0.5 Wm-2.
Here we introduce the cloudy version of the equations and present the all-sky global mean system as the weighted sum of the clear-sky and cloudy-sky structures. “Clouds” are regarded as a single IR-opaque layer, represented by an effective cloud area fraction. Essential characteristics of the climate (like the CREs and the greenhouse effect) are explained as the cooperation of the clear-sky and cloudy-sky geometric arrangements expressed in the transfer equations. This way, the theoretical description of the Earth’s global mean energy budget is complete.
In Figure 1, we use different colors to make the clear-sky, cloudy-sky and all-sky units evident. The fundamental fluxes on the intercepting disk to solar radiation are integers; fractions appear after spherical weighting, and as a result of the clear-cloudy energy transfer.