sunset
The sunset function determines the Coordinated Universal Time when the sun just sets below the horizon.
The sunset function determines the Coordinated Universal Time when the sun just sets below the horizon.
The sunrise function determines the Coordinated Universal Time when the sun just rises above the horizon.
The sundiagram function creates an illustration of the sun path over the year for a specific geographic location.
The suntime function calculates the Coordinated Universal Time or local time for a given sun position and geographic location.
Creates spectral radiance data for a Tregenza hemisphere with 145 patches for CIE sky types 3 and 12
Calculates and plots the resulting horizontal and vertical Correlated Colour Temperatures from the Tregenza luminance distribution with 145 patches
Calculates the resulting horizontal and vertical illuminances for a given Tregenza luminance distribution with 145 patches
Calculates the sun position according to DIN EN 17037 from UTC
Determines the CIE general standard sky type for a given luminance distribution of a Tregenza hemisphere
Calculates the corresponding luminance distribution for a Tregenza hemisphere with 145 patches according to the CIE procedure described in ISO 15469
Determines the α-opic equivalent daylight D65 quantity for a given spectrum
Determines the melanopic equivalent daylight D65 illuminance for a given spectrum
Determines the nearest neighbour patches and the angular distance to a given tregenza hemisphere patch
Calculates the True Solar Time (TST) according to DIN EN 17037 from Coordinated Universal Time (UTC)
Determines the CIE general standard sky type for a given luminance distribution of a Tregenza hemisphere
Calculates the resulting horizontal and vertical Correlated Colour Temperatures from the Tregenza radiance distribution with 145 patches and the colour coordinates x and y
Returns the (UTC) for True Solar Time (TST) 12:00 according to DIN EN 17037
Determines the CIE general standard sky type for a given luminance distribution of a Tregenza hemisphere as described by Kobav et al.
Calculates the resulting horizontal and vertical illuminances for a given Tregenza luminance distribution
Creates a directogram plot of a Tregenza sky hemisphere