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Home > Research > Ifsdocs > PHYSICS >  
   

Chapter 2. Radiation

IFS documentation Front Page


Table of contents



Chapter 1. Overview

Chapter 2. Radiation

Chapter 3. Turbulent diffusion and interactions with the surface

Chapter 4. Subgrid-scale orographic drag

Chapter 5. Convection

Chapter 6. Clouds and large-scale precipitation

Chapter 7. Land suface parametrization

Chapter 8. Methane oxidation

Chapter 9. Climatological data

REFERENCES


 
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2.1 Radiative heating




The radiative heating rate is computed as the divergence of net radiation fluxes :

 
,
(2.1)


where is the specific heat at constant pressure of moist air
,


and and are the specific heats at constant pressure of dry air and water vapour, respectively. Sections 2.2 and 2.3 describe the computation of the longwave and shortwave radiative fluxes respectively. The solution of the radiative transfer equation to obtain the fluxes is unfortunately very expensive, and we cannot afford to do it more than every 3 hours at every fourth grid point. The interpolation scheme used for obtaining the radiative fluxes at every grid point and every time step for the relevant instantaneous temperature profile and solar zenith angle is described in Section 2.4.


A description of the inputs, in particular the climatologically defined quantities of radiative importance is given in Section 2.5. Finally, an alphabetical list of the subroutines of the radiation scheme is given in Section 2.6.


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