pvlib.irradiance.perez_driesse

pvlib.irradiance.perez_driesse(surface_tilt, surface_azimuth, dhi, dni, dni_extra, solar_zenith, solar_azimuth, airmass=None, return_components=False)

Determine diffuse irradiance from the sky on a tilted surface using the continuous Perez-Driesse model.

The Perez-Driesse model [1] is a reformulation of the 1990 Perez model [2] that provides continuity of the function and of its first derivatives. This is achieved by replacing the look-up table of coefficients with quadratic splines.

Parameters:

• surface_tilt (numeric) – Surface tilt angle. See surface_tilt. [°]

• surface_azimuth (numeric) – Surface azimuth angle. See surface_azimuth. [°]

• dhi (numeric) – Diffuse horizontal irradiance, must be >=0. [Wm⁻²]

• dni (numeric) – Direct normal irradiance, must be >=0. [Wm⁻²]

dni_extranumeric

Extraterrestrial normal irradiance. [Wm⁻²]

solar_zenithnumeric

apparent (refraction-corrected) zenith angle. [°]

solar_azimuthnumeric

Solar azimuth angle. See solar_azimuth. [°]

airmassnumeric, optional

Relative (not pressure-corrected) airmass values. If airmass is a DataFrame it must be of the same size as all other DataFrame inputs. AM must be >=0 (careful using the 1/sec(z) model of AM generation). [unitless]

return_components: bool (optional, default=False)

Flag used to decide whether to return the calculated diffuse components or not.

Returns:

• numeric, OrderedDict, or DataFrame – Return type controlled by return_components argument. If return_components=False, sky_diffuse is returned. If return_components=True, diffuse_components is returned.

• sky_diffuse (numeric) – The sky diffuse component of the solar radiation on a tilted surface.

• diffuse_components (OrderedDict (array input) or DataFrame (Series input)) –

  Keys/columns are:

  • sky_diffuse: Total sky diffuse

  • isotropic

  • circumsolar

  • horizon

Notes

The Perez-Driesse model can be considered a plug-in replacement for the 1990 Perez model using the 'allsitescomposite1990' coefficient set. Deviations between the two are very small, as demonstrated in [1]. Other coefficient sets are not supported because the 1990 set is based on the largest and most diverse set of empirical data.

References

[1] (1,2)

Driesse, A., Jensen, A., Perez, R., 2024. A Continuous form of the Perez diffuse sky model for forward and reverse transposition. Solar Energy vol. 267. DOI: 10.1016/j.solener.2023.112093

[2]

Perez, R., Ineichen, P., Seals, R., Michalsky, J., Stewart, R., 1990. Modeling daylight availability and irradiance components from direct and global irradiance. Solar Energy 44 (5), 271-289.

See also

perez, isotropic, haydavies, klucher, reindl, king

Examples using pvlib.irradiance.perez_driesse

Modelling shading losses in modules with bypass diodes

Modelling shading losses in modules with bypass diodes