Dear Marcello, yes, the star-node model work has same limitations especially for extreme geometries and temperature deviations .
The “detailed” model is able to handle these extreme cases correctly. For ordinary space shapes the star-rnode model does a good job as shown in several comparisons. If you aren’t sure if the star-node model performs well for your geometry/temperatures you can check the results with the detailed model based on Gebhart factors. Personally, I simulate 4 surfaces at least in a zone. Dipl.-Ing.
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Dear TRNSYS users, I have a very simple non-geometrical type 56 model with one zone with two surfaces: one boundary surface of 40 m2 and an external surface of 400 m2. External condition
and boundary temperature are held constants. When I plott surface temperatures and heat exchange between the two surfaces, I found a very large long wave radiation exchange between the two surfaces.
By hand calculation (Q=sigma S (T1^4 – T2^4), whit S = area of the little surface), I found that the value given of heat exchange by radiation by TRNSYS is about
ten times larger than what I expected. Indeed, it seems that value given by TRNSYS is near to the value given by the same equation but considering the largest surface area. However, if I split the external surface in two surfaces of half the area, the value calculated by TRNSYS is reduced of about 7 times. If I split again these surfaces,
radiation exchange continue to drop but more slightly, tending to a value near the one calculated by hand.
My question is : have you already found the same behavior? Is there a recommendation to define at least three surfaces in a zone in order to calculate properly
heat exchange by radiation? Thank you for your help! Best regards, Marcello Caciolo
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