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Performance of Home Smoke Alarms - National Institute of ...

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Thus, within the range typical <strong>of</strong>ionization smoke alarms, the responseis within the limits <strong>of</strong> the UL 217 test.Residential photoelectric alarmstypically alarm at transmittances greaterthan 0.84 in the UL test. While theFE/DE smoke deviates outside the MIClimits at a transmittance <strong>of</strong> about 0.9,this observation is not by itself a causefor concern.Laser Light Transmittance(1.52 m pathlength)0.80.850.90.95The deviation between UL and FE/DEtest smoke results at lower lighttransmittance values suggests a smokesize distribution difference between thetwo smolder smokes. Since the UL11001790807060MIC output (pA)Figure 8. UL grey smoke (smolder smoke) sensitivitylimits and FE/DE datasmoke box is a re-circulating system, it can take between 12 min to 17 min to reach a lighttransmittance value <strong>of</strong> 0.8. The FE/DE is an open, single-pass flow system and the smoketransport time for these calibration tests is on the order <strong>of</strong> 30 s. Therefore, potentially moresmoke aging (i.e. coagulation growth <strong>of</strong>the smolder aerosol) can take place inthe smoke box relative to the FE/DE.Assuming that fresh smolder smokes areidentical in the smoke box and theFE/DE, additional coagulation growth inthe smoke box will tend to increase lightextinction while decreasing the MICoutput for a fixed amount <strong>of</strong> smoke.This could explain MIC differencebetween the two sources at lowertransmittances. The difference betweenrelative levels <strong>of</strong> obscuration and lightscattering <strong>of</strong> fresh and aged smoldersmokes should be less pronounced.There are two reasons for thissupposition. First, coagulation growthtends to incorporate the smallestparticles into bigger particles. TheLaser Light Transmittance(1.52 m pathlength)0.60.650.70.750.80.850.90.95110090807060MIC output (pA)Figure 9. UL black smoke sensitivity limits andcorresponding FE/DE datasmaller particles scatter little light, and contribute almost nothing to obscuration, thus they arenot missed. Second, the growth <strong>of</strong> particles that scatter significant amounts <strong>of</strong> light will tend to505040403030

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