between the detector and the sources of potential fires. Small concentrations of these types of gases may not absorb enough UV radiation to cause a problem, but when higher concentrations of these gases are present the detectors may become blind as not enough
False Alarms
Arc Welding, long duration lightning flashes, cracked mercury lamps, cracked halogen lamps, and
NOTE:
Ultraviolet detectors are sensitive to arc welding and if this type of radiation can be expected, nuisance alarms must be controlled through proper application including careful positioning and shielding of the detectors. Some applications may require a UV/IR system.
CAUTION:
Caution must be exercised if the detection system is turned off, as the hazardous area will not be protected. .
Lightning strikes can trigger the detector but this can be solved by pointing the sensor cone of vision below the horizon and setting the time delay to 7 seconds.
Cracked mercury or halogen lamps in the vicinity of the fire detector should be replaced as soon as they are discovered.
UV radiation other than that produced by an actual fire is referred to as “background UV”. An example of a high level of background UV could be a flare stack situated outside of a building. The UV radiation produced by this flare may be detected when a door to the building is opened. Windows or other reflective surfaces may also cause unusually high levels of UV radiation to enter the building from the flare. In a situation like this, the fire detection system response must be carefully checked and the sensitivity level adjusted high enough, so that this “background UV” will not cause false alarms.
UV fire detectors respond to radiation other than ultraviolet.
Position and Density of Detectors
The
NOTE:
Do not mount UV detectors close to the ceiling of enclosed buildings if smoke might accumulate before the
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