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Méso Star authored
Now, the emissivity and specular fraction of the interface depend on the radiation source, whose identifier is an argument to their associated functor. At present, nothing has changed in the solver, which still queries these properties for the internal source. This commit is therefore an intermediary to correct the compilation of tests in relation to this API break.
Méso Star authoredNow, the emissivity and specular fraction of the interface depend on the radiation source, whose identifier is an argument to their associated functor. At present, nothing has changed in the solver, which still queries these properties for the internal source. This commit is therefore an intermediary to correct the compilation of tests in relation to this API break.
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