Is the sky_diffuse_passias
model conceptually correct?
#1825
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kandersolar
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pvlib.shading.sky_diffuse_passias
implements a row-to-row diffuse irradiance reduction model given in Passias & Kallback 1984. The reference uses the term "masking" to refer to row-to-row diffuse shading and claims that "the relative reduction in the diffuse irradiance due to the masking effect" is given byI see that$1 - \cos^2(\psi/2)$ is equivalent to $(1 - \cos(\psi))/2$ and thus can be understood as a case of the B-71 view factor where the obstruction is not somewhere in the middle of the field of view like the above figure suggests but rather at the edge of the field of view as shown in pink here:
So it seems to be accounting for shading from some other obstruction rather than the adjacent row. I also don't understand how it could account for row-row shading without taking the surface tilt into account.
I find myself even more skeptical after comparing the equation with the VF calculations elsewhere in pvlib and not getting the values I expect:
Am I misunderstanding how to use the Passias equation? How can it be used correctly?
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