With sufficient warming, the same radiative
transfer equations show that upward IR will rise enough for sufficient quantities to escape to space, albeit at a higher altitude than before, warmed sufficiently so that its IR emissivity allows OLR to balance incoming absorbed radiation.
What the net
transfer equation show, is how kirchoff's law works in practice in relation to temperature.
Not exact matches
The amount of energy absorbed depends on the temperature of the absorber,
shown to be true by the stefan - boltzmann
equation for net
transfer of heat.
Previously I
showed an
equation that
showed the ratio of convective and radiative heat
transfer.
Physics of atmospheric radiation; theoretical techniques used to
show radiation
transfer equation
The implication that a modicum of ocean heat is needed to initiate a hurricane needs to be backed up by some back - of - envelope
equations that convey heat
transfer functions, latent heat, circulation rates etc., to
show that the hot ocean is capable to
transferring enough heat into a storm to make a difference.
And for the purists, the
equation as
shown relies on the temperature not changing as a result of the small
transfer of energy.
Steve I will ask you to
show the radiative heat
transfer equation in which you input an emission from another body, gas / solid or fluid and
show where it lowers the rate of cooling.
There is no input for back radiation in any heat
transfer equation so taking as if it does something can not be
shown via standard
equations.
To calculate this value, you need to solve the radiative
transfer equations, shown in Understanding Atmospheric Radiation and the «Greenhouse» Effect — Part Six — The E
equations,
shown in Understanding Atmospheric Radiation and the «Greenhouse» Effect — Part Six — The
EquationsEquations.