The Earthemitted thermal radiation has a spectrum of a black body with a characteristic average temperature of 288 K. The Earth infrared radiation also varies across the globe but less than the albedo. It also shows a diurnal variation which is small over the ocean but can amount to 20 % for desert areas.
The average infrared radiation emitted by Earth is 230 W m-2. For an orbiting spacecraft, it can vary from 150 W m-2 to 350 W m-2. The diurnal variations can amount to about 20 % over desert areas while being smaller over the oceans.
A model has been constructed for estimating the influence of latitude and longitude on Earth infrared variability (seasonal effect) [RD.34], given by:
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(F-2) |
where
t0 is the date
ω is the orbital pulsation (=2π/365,25)
ϕ is the equatorial latitude
JD is the Julian date of interest
Pn is the nth degree Legendre polynomial
and the following values are proposed:
e0= 0,68
e1 [k0=0, k1=-0,07, k2=0]
e2= -0,18