Describe the bug
According to pvlib's source code, the model explores an empirical regression between DNI/I_0 and GHI/I_0 (i.e., Kt).
However, the original paper states
For direct normal radiation (noted I), we used as a reference, a calculated direct normal irradiation for cloudless skies (noted I_M), based on the model elaborated by A. Louche et al.[13].
Meaning that they use normalize DNI by a clear-sky version rather than the extraterrestrial.
I've looked at the [13] paper and it was not very clear, as it is mainly oriented to estimating turbidity. The only more similar thing I found was
There is also the fact that the current implementation does not saturate to 0 for Kt<0.17 as stated in the paper. As is, if Kt=0, it leads to one of the components being negative.
Lastly, maybe it could also be mentioned in the doc - assuming that the correct implementation is viable within pvlib -that this model was originally made for daily averages.
Describe the bug
According to pvlib's source code, the model explores an empirical regression between DNI/I_0 and GHI/I_0 (i.e., Kt).
However, the original paper states
Meaning that they use normalize DNI by a clear-sky version rather than the extraterrestrial.
I've looked at the [13] paper and it was not very clear, as it is mainly oriented to estimating turbidity. The only more similar thing I found was
There is also the fact that the current implementation does not saturate to 0 for Kt<0.17 as stated in the paper. As is, if Kt=0, it leads to one of the components being negative.
Lastly, maybe it could also be mentioned in the doc - assuming that the correct implementation is viable within pvlib -that this model was originally made for daily averages.