Sentences with phrase «transfer equations»

"Transfer equations" refer to mathematical equations that are used to represent the movement or transfer of something from one place or state to another. It involves describing the changes or transition of variables or quantities in different contexts or conditions. Full definition
The radiative transfer equations as part of the modeled results have done a pretty good job of explaining the observed results but aren't exactly the same.
An example of two of the most fundamental of all heat transfer equations used by both chemical engineers and mechanical engineers will illustrate.
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.
This calculation includes solving the radiative transfer equations through the atmosphere (see CO2 — An Insignificant Trace Gas?
But the reason that the models are failing to reproduce what we see that they are based on an approximation of the radiative transfer equation which does not apply to the boundary layer where the ice is melting.
You correctly state that «less energy is needed to to raise one gram of CO2 one °C than one gram of air one °C» but you have simply ignored mass and the fundamental heat transfer equation Q = m x c x delta T.
Its main argument is that idealized blackbody calculations did not correctly predict the Moon's surface temperatures in the 1960s because other factors besides radiative heat transfer equations actually determine real surface temperatures.
Mishchenko, M.I., 2002: Vector radiative transfer equation for arbitrarily shaped and arbitrarily oriented particles: A microphysical derivation from statistical electromagnetics.
Is it not then fair to state that the link between tropopause and surface is given by the radiative transfer equations along with the proper input in terms of ghg concentrations and spectroscopic properties, and starting atmospheric temperatures?
Solving the radiative transfer equations through the atmosphere requires knowledge of the absorption spectra of each gas.
see fred «'' Jeff, the 1C value for a forcing of 3.7 W / m ^ 2 (the canonical value for doubled CO2 based on radiative transfer equations and spectroscopic data) is derived by differentiating the Stefan - Boltzmann equation that equates flux (F) to a constant (sigma) x the fourth power of temperature.
In the classic heat - transfer equation, the rate of temperature change depends on how uniformly the thermal energy is distributed through an object.
2.170) which is for blackbody radiation, they should be using the Microscopic Radiative Transfer Equation, which has terms for both spontaneous and stimulated emissions by greenhouse gases (Thomas and Stamnes [T&S], Eqn.
In this case you have the diffusion transfer equation, which similarly has a differential of hot and cold terms describing the heat flow, as does the radiation transfer equation, and we all understand that heat does not physically diffuse from cold to hot and that physical contact between a cold object and warm object does not make the warmer object warmer still.
The emissivity is combined with the surface effective temperature, sometimes called the skin temperature, in the radiative transfer equation.
Instead atmospheric physics uses the fundamental equations (the radiative transfer equations) which determine absorption and emission of radiation by water vapor, CO2, methane, and other trace gases.
If the model results of temperature and humidity profile vertically though the atmosphere were not correct then this would definitely affect the accuracy of the radiative transfer equations.
There is a reason why powerful computers are needed to solve the radiative transfer equations.
It's also the case that the results for the radiative transfer equations will have a certain amount of error using «band models» compared with the «line by line» (LBL) codes for all trace gases.
Well, the only way to work out the «expected» results — or what the theory predicts — is to solve the radiative transfer equations (RTE) for that vertical profile through the atmosphere.

Phrases with «transfer equations»

a b c d e f g h i j k l m n o p q r s t u v w x y z