Nomenclature#
There is a convention on consistent variable names throughout the library:
- airmass#
- Airmass 
- airmass_absolute#
- Absolute airmass 
- airmass_relative#
- Relative airmass 
- albedo#
- Ratio of reflected solar irradiance to global horizontal irradiance [unitless] 
- aoi#
- Angle of incidence. Angle between the surface normal vector and the vector pointing towards the sun’s center. [°] 
- aoi_projection#
- cos(aoi). When the sun is behind the surface, the value is negative. For many uses, negative values must be set to zero. 
- ape#
- Average photon energy 
- apparent_zenith#
- Refraction-corrected solar zenith angle. The solar zenith angle describes the position of the sun relative to the vertical and is defined as the angle between a vector pointed straight up and a vector pointed at the sun, from the observer. [°] 
- apparent_elevation#
- Refraction-corrected solar elevation angle. This is the complement of apparent_zenith (90 - apparent_zenith). [°] 
- bhi#
- Beam/direct horizontal irradiance 
- cross_axis_slope#
- Cross-axis tilt angle. [°] Consider two parallel rows of modules at different height; - cross_axis_slopeis the angle formed the line formed by the intersection between the slope containing the tracker axes and a plane perpendicular to the tracker axes, and the horizontal plane. Cross-axis tilt is measured by using a right-handed convention. For example, trackers with axis azimuth of 180° (heading south) will have a negative cross-axis tilt if the tracker axes plane slopes down to the east and positive cross-axis tilt if the tracker axes plane slopes up to the east. Use- calc_cross_axis_slope()to calculate- cross_axis_slope
- dhi#
- Diffuse horizontal irradiance 
- dni#
- Direct normal irradiance [Wm⁻²]. Irradiance received per unit area by a surface perpendicular (normal) to the sun’s rays that propagate in a straight line from the sun. 
- dni_clear#
- Clear sky direct normal irradiance 
- dni_extra#
- Direct normal irradiance at top of atmosphere (extraterrestrial) 
- effective_irradiance#
- Effective irradiance 
- eta_inv#
- Inverter efficiency 
- eta_inv_nom#
- Nominal inverter efficiency 
- eta_inv_ref#
- Reference inverter efficiency 
- g_poa_effective#
- Broadband plane of array effective irradiance 
- gamma_pdc#
- Module temperature coefficient. Typically in units of 1/C. 
- ghi#
- Global horizontal irradiance 
- ghi_clear#
- Clearsky global horizontal irradiance [Wm⁻²] 
- ghi_extra#
- Horizontal irradiance at top of atmosphere (extraterrestrial) 
- gri#
- Ground-reflected irradiance 
- i_sc#
- Short circuit module current 
- i_x, i_xx#
- Sandia Array Performance Model IV curve parameters 
- latitude#
- Latitude in decimal degrees. Positive north of equator, negative to south. 
- longitude#
- Longitude in decimal degrees. Positive east of prime meridian, negative to west. 
- pac, ac#
- AC power 
- pdc, dc#
- DC power 
- pdc0#
- Nameplate DC rating 
- photocurrent#
- Photocurrent 
- poa_diffuse#
- Total diffuse irradiance in plane [Wm⁻²]. Sum of ground and sky diffuse components of global irradiance. 
- poa_direct#
- Direct/beam irradiance in plane [Wm⁻²]. 
- poa_global#
- Global irradiance in plane. Sum of diffuse and beam projection [Wm⁻²]. 
- poa_ground_diffuse#
- In plane ground reflected irradiance [Wm⁻²]. 
- poa_sky_diffuse#
- Diffuse irradiance in plane from scattered light in the atmosphere (without ground reflected irradiance) [Wm⁻²]. 
- precipitable_water#
- Total precipitable water contained in a column of unit cross section from earth to top of atmosphere 
- pressure#
- Atmospheric pressure 
- relative_humidity#
- Relative humidity 
- resistance_series#
- Series resistance 
- resistance_shunt#
- Shunt resistance 
- saturation_current#
- Diode saturation current 
- solar_azimuth#
- Azimuth angle of the sun in degrees East of North. The solar azimuth angle describes the sun’s position along the horizon relative to the observer. The pvlib-python convention is defined as degrees East of North, so North = 0°, East = 90°, South = 180°, West = 270°. 
- solar_zenith#
- Zenith angle of the sun in degrees. This is the angle between is between a vector pointed straight up and a vector pointed at the sun, from the observer. This is the complement of solar elevation (90 - elevation). [°] 
- spectra#
- spectra_components#
- Spectral irradiance (components) [Wm⁻²nm⁻¹]. The amount of energy incident on a unit area per unit time and per unit wavelength. As with broadband irradiance, global spectral irradiance is composed of direct and diffuse components. 
- surface_azimuth#
- Azimuth angle of the surface in degrees East of North. This angle describes the horizontal projection of the normal vector from the surface. The pvlib-python convention is defined as degrees East (clockwise) of North, so North = 0°, East = 90°, South = 180°, West = 270°. 
- surface_tilt#
- Tilt from horizontal [°]. The surface tilt angle is defined as degrees from the horizontal such that a surface facing up would have a surface tilt of 0°, and one facing the horizon would be 90°. [°] 
- temp_air#
- Temperature of the air 
- temp_cell#
- Temperature of the cell 
- temp_dew#
- Dewpoint temperature 
- temp_module#
- Temperature of the module 
- tz#
- Timezone 
- v_mp, i_mp, p_mp#
- Module voltage, current, power at the maximum power point 
- v_oc#
- Open circuit module voltage 
- wind_direction#
- Wind direction 
- wind_speed#
- Wind speed 
For further explanation of the variables, common symbols, and units, refer to the following sources from SoDa Service:
Note
These further references might not use the same terminology as pvlib. But the physical process referred to is the same.
