Normalize >aT~ G!y
Normalize the map data to the total emitted flux from all sources. I "HEXsSe
This option allows you to have the flux and irradiance normalized to the total (};/,t1#$
emitted flux. When this box is checked, TracePro divides the values in the +|qw >1J(
irradiance map and the total flux by the emitted flux. This is especially useful for 6t3Zi:=I
calculating system transmittance for an optical system, or lighting efficiency for a ; jrmr`l=
lighting calculation. aX?
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Example 1: System Transmittance \"b'Z 2 g
Suppose you need to calculate the system transmittance of an optical system. lQpl8>
You would probably use the grid raytrace option, and the emitted flux is equal to gn lU
the sum of the flux in all the emitted rays. When you display an irradiance map, [`' K.-?#
the system transmittance is equal to the total flux, displayed at the bottom of the VyWzb
irradiance map window, divided by the emitted flux. To get the system WQsu}_g5y
transmittance, check the Normalize to emitted flux box and press the Apply aVp-Ps|r
button. The map will be redisplayed, and the Normalized Flux value will be equal r- ,u)zf"
to the system transmittance. \pXo~;E\
Example 2: Lighting Efficiency 0F 6 ~S
Suppose you need to calculate the lighting efficiency of a luminaire in illuminating @4$la'XSx
a plane. You would probably choose the Surface Source raytrace option, and the TP mb]j
emitted flux is equal to the flux you specified when you defined the sources. When p5J!j I=
you display an irradiance map, the total flux incident on the observation plane is c| X }[
displayed at the bottom of the window. The lighting efficiency is equal to the total l_pf9 !z
flux divided by the emitted flux. To get the lighting efficiency directly, check the YwZ ]J
Normalize to emitted flux box and press the Apply button. The map will be X? Or.
redisplayed, and the Normalized Flux value will be equal to the lighting efficiency lD $\t/8B
of the luminaire.
