Thank you for your response. I understand your point, but I find myself going down a bit of a rabbit hole. I initially tried a rough estimation by multiplying the g-values of the film (0.2) and the glazing assembly (0.45), based on the technical datasheets previously shown. However, this results in a combined g-value of 0.2x0.45= 0.09, which seems unrealistically low. Interestingly, using this value in my simulations eliminates any overheating issues. Yet, the occupants, based on real-world experience, report significant overheating during summer evenings, particularly on the west façade, which receives intense direct solar radiation (near-normal to the glazing plane). This contradicts the simulation results.
Given that the building is around 20 years old and lacks spectral data for the glazing and film, I’ve been trying to find a more realistic way to model their combined behavior. My current workaround involves creating an equivalent layer in Window 7 and simulating an equivalent film in Optics, but I recognize this is just a temporary hack.
From my understanding, two key factors might be contributing to the discrepancy:
The film appears to be mirror-like and likely contains aluminum, which typically has a low emissivity (around 0.1–0.2). This means that once solar radiation is absorbed (about 0.26 in this case), very little longwave radiation is emitted outward. If the assembly cannot effectively radiate this heat back outside, it may lead to internal heat buildup, raising the mean radiant temperature, consistent with the occupants observations.
Outdoor air temperatures in Zaragoza during summer evenings often exceed 30°C, which reduces the glazing’s ability to dissipate heat via conduction and convection.
In essence, it seems the glazing assembly is acting as a heat trap for the absorbed solar energy component.
Does this interpretation make sense to you? And do you have any suggestions for a more accurate way to simulate this behavior given the limited data?
Thanks