.BuildSysPro.BaseClasses.HeatTransfer.Components.LinearExtLWR

Echanges thermique par rayonnement en grande longueur d'onde

Information

Calculation of linearized long wavelength radiation exchanges with the sky and the environment.

Hypothesis and equations

The solar flux with long wavelength radiation has two sources : the environment and the sky. Different hypothesis have been made :

The radiative net fux exchanged between a wall and the outside is linearized with the function below :

Where :

sigma and epsilon are respectively the Stefan-Boltzmann constant and the emissivity of the wall. Furthermore T_cielConst, T_envConst and T_surfConst are representatives constants of the sky, environment and outside surface temperatures. Using the values :

it gives :

Finally, we get :

Flux_GLO=Flux_GLOEnvironnement + Flux_GLOCiel

Bibliography

TF1 CLIM2000

Instructions for use

Typical values for epsilon (from BodyRadiation model) :

   aluminium, polished    0.04
   copper, polished       0.04
   gold, polished         0.02
   paper                  0.09
   rubber                 0.95
   silver, polished       0.02
   wood                   0.85..0.9

Known limits / Use precautions

Verify that the conditions of use are close enough to T_envConst=283.15 K and T_cielConst=T_extConst-20 = 263.15 K.

Validations

Modèle validé - Gilles PLESSIS 12/2012

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Licensed by EDF under a 3-clause BSD-license
Copyright © EDF 2009 - 2023
BuildSysPro version 3.6.0
Author : Gilles PLESSIS, EDF (2012)
Initial model : BodyRadiation, Anton Haumer, Copyright © Modelica Association, Michael Tiller and DLR.
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