Depending on the radiation discretization method, the contribution to the heat balance is handled differently. For the definition of ntfluxInt, the Optically Thick Participating Medium subnode uses the Rosseland approximation and defines qr, the radiative flux, as an extra contribution to the conductive heat flux. The P1 approximation and Discrete ordinates method, however, include the radiative source ∇ ⋅ qr to Q on the domain, in the variable QInt.
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The heat balance can be evaluated assuming constant material properties using the following variables: heatBalance_cst, dEiInt_cst, ntfluxInt_cst, WstrInt_cst, and QInt_cst. The evaluation of these variables is faster and accurate for constant material properties or small temperature gradients.
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The heat and energy balance variables such as ht.ntfluxInt or ht.ntefluxInt do not take into account the flux contributions on thin structures. For example, if a Thin Layer node is applied on a boundary, the heat flux on this boundary is not included in ht.ntfluxInt. It is instead added to the variable ht.sls1.ntfluxInt, defined locally on the thin structure. Here, sls1 is the tag of the Thin Layer node.
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The energy balance can be evaluated assuming constant material properties using the following variables: energyBalance_cst, dEi0Int_cst, ntefluxInt_cst, WInt_cst, and QInt_cst. The evaluation of these variables is faster and accurate for constant material properties or small temperature gradients.
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