Atmospheric Window and TOA Net CRE
This chapter deals with some features regarding the longwave and the net CRE, makes explicit an expectation about TSI (menationed already above), and places a non-observable (only computable) energy flow component, atmospheric window radiation, into the integer system.
On this page:
[Kopp, G. (2020), TSIS TIM Level 3 Total Solar Irradiance 24-hour Means, version 03,
Greenbelt, MD, USA: NASA Goddard Earth Science Data and Information Services Center (GES DISC),
Accessed <August 11, 2023 at https://doi.org/10.5067/TSIS/TIM/DATA306]
Costa and Shine (2012) performed LBL-computation of the global mean clear-sky atmospheric window radiation (STI, surface transmitted irradiance, without assumption on the wavelengths), and found it as 65 Wm-2, with regard to their model-OLR = 259 Wm-2. With proportionality, using our theoretical OLR(clear) = 266.8 Wm-2, this would result in WIN(clear) = 66.96 Wm-2.
Notice that 66.70 Wm-2 is an integer position = 10/4 units (with 51/4 incoming, 8/4 reflected, 40/4 LW-emitted and 3/4 clear-sky TOA net imbalance). This means that on the disk, 40 units outgoing LW is the sum of 10 units window radiation and 30 units atmospheric upward emission. Surface upward LW (ULW) on the sphere is 15 units, that is, 60 units on the disk. ATM up = ULW/2.
This of course reinforces the Clear-sky net imbalance at TOA = 3/4 units = 20.01 Wm-2 we were using in TSI calibration in the Geometric deduction.