Energy balance
Electromagnetic radiation
Greenhouse effect
Carbon cycle
Long term climate variation
Mass extinctions
Anthropogenic perturbation of carbon cycle
Nytrogen cycle
ν = c / λ
ν = frequency
c = speed of light
λ = wavelength
Energy of a photon:
E = h . ν = h . c / λ
h = Planck's constant
Wien's law
Stefan-Boltzmann law
\[F=\sigma T^4\]
F = W.m-2
T = Kelvins
σ = 5.67e-8 W.m-2.K-4
1] Some incoming shortwave radiation is not absorbed by the atmosphere and reaches the surface of the earth.
2] This radiation is absorbed by the surface of the earth and re-emitted at lower wavelengths (because the earth is much cooler than the sun)
3] This longwave radiation is absorbed by the atmosphere and re-emitted in all directions.
4] Some of this re-emitted longwave radiation is absorbed (again) by the surface and re-emitted.
"Keeping relative humidity constant"
How does carbon move through the spheres?