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Candela Seconds or Candlepower Seconds<br />
This quantity is the actual light energy contained in a pulse of<br />
light. Candela seconds is used by the Society of Automotive<br />
Engineers SAE) and the California Highway Patrol to specify<br />
the minimum requirements for light output from a flashing<br />
light because flash energy has been shown to be a relatively<br />
accurate and fair way of comparing radically different types of<br />
lights such as incandescent rotators and xenon strobe lights.<br />
Candela seconds is merely a relative measure of how bright a<br />
flash of light will appear to a human eye. A light with a higher<br />
candela second rating will appear brighter than a light with a<br />
lower candela second rating even if the lower rated light has<br />
a much higher peak candela rating.<br />
Effective Candela or Effective Candlepower<br />
Effective Candela is based on candela seconds and attempts<br />
to equate the brightness of a flashing light source to the<br />
brightness of a steady burning source. If a flashing light has<br />
a candela effective rating of 100 then it will be visible at the<br />
same distance as a 100 candela steady burning source. The<br />
National Bureau of Standards, the FAA, and the Illuminating<br />
Engineering Society use effective candela in specifying<br />
intensities of flashing light source because this rating is the<br />
most meaningful when it becomes necessary to predict the<br />
visible range of flashing warning lights versus steady burning<br />
light sources.<br />
Please note that the actual perceived light output of a visual<br />
signal depends on a number of interdependent factors which<br />
can vary the light output by a factor of 10 or more for a given<br />
amount of energy per flash.<br />
Some of these factors are:<br />
• Viewing Distance<br />
• Viewing Angle<br />
• Flash Rate<br />
• Pulse Width or Duration<br />
• Ambient Light Conditions<br />
• Chromaticity or Color Saturation<br />
• Lens or LED Light Source Color<br />
• Lens Optics<br />
• Physical shape of Light Source and positioning<br />
relative to Lens (optical coupling)<br />
• Light Source Efficiency<br />
• Voltage Variation<br />
Linear Perspective<br />
When selecting a visual signal it is also important to keep in<br />
mind that as objects are viewed from a greater distance, they<br />
appear smaller because their visual angle decreases. The<br />
visual angle of an object is the angle subtended at the eye by<br />
a triangle with the object at its base. The greater the distance<br />
of the object from the eye, the greater the height of this<br />
triangle, and the less the visual angle. This follows simply from<br />
Euclidean geometry.<br />
You already know this from everyday life: buildings look<br />
smaller as they are further away. So do people. If you know<br />
approximately how big something is (its physical size) -<br />
for example, a person of average height is<br />
usually around 5 or 6 feet tall) and you<br />
observe that person to be a certain<br />
apparent size, you are able to automatically<br />
estimate roughly how far away they are.<br />
The relationship between distance and<br />
apparent height of objects is an<br />
inverse-linear function:<br />
h= a – d<br />
where h is the apparent height,<br />
d is the distance of the object, and<br />
a is the actual size of the object.<br />
For example: A 94PLEDMR120A<br />
Polaris Beacon has an<br />
“Actual Size” of 7.75” high.<br />
One does not have to actually do the<br />
math to realize that regardless of how<br />
bright this beacon actually is, at a great<br />
distance away (1000’), to the viewer, it<br />
would appear a small point of light.<br />
TM<br />
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