Smoke detector

Information

  • Patent Grant
  • 6326897
  • Patent Number
    6,326,897
  • Date Filed
    Monday, March 12, 2001
    23 years ago
  • Date Issued
    Tuesday, December 4, 2001
    23 years ago
Abstract
A smoke detector includes a housing defining a dark chamber admitting test atmosphere. A light receiver is disposed within the chamber. A scatter emitter is positioned within the chamber such that light strikes the receiver when reflected off particles suspended in the test atmosphere. An obscuration emitter is positioned within the chamber such that light emitted is directed to the receiver unless obstructed by particles suspended in the test atmosphere. A smoke detect signal is generated responsive to a measurement made responsive to the scatter emitter and/or the obscuration emitter.
Description




BACKGROUND OF THE INVENTION




The present invention relates to systems and methods for detecting smoke. Smoke detectors detect the presence of smoke particles as an early indication of fire. Smoke detectors are used in closed structures such as houses, factories, offices, shops, ships, aircraft, and the like. Smoke detectors may include a chamber that admits a test atmosphere while blocking ambient light. A light receiver within the chamber receives a level of light from an emitter within the chamber, which light level is indicative of the amount of smoke contained in the test atmosphere.




Several types of fires need to be detected. A first type is a slow, smoldering fire that produces a “gray” smoke containing generally large particles, which may be in the range of 0.5 to 1.2 microns. A second type is a rapid fire that produces “black” smoke generally having smaller particles, which may be in the range of 0.05 to 0.5 microns. Fires may start as one type and convert to another type depending on factors including fuel, air, confinement, and the like.




Two detector configurations have been developed for detecting smoke particles. Direct, or obscuration, detectors align the emitter and receiver such that light generated by the emitter shines directly into the receiver. Smoke particles in the test atmosphere interrupt a portion of the beam thereby decreasing the amount of light received by the emitter. Obscuration detectors typically work well for black smoke but are less sensitive to gray smoke. Additionally, obscuration detectors typically are not within a chamber, as they have an emitter and a receiver spaced at a substantial distance, such as one meter or across a room, whereas smoke detector chambers are preferably located within a compact housing. Indirect or reflected detectors, commonly called scatter detectors, have an emitter and receiver positioned on non-colinear axes such that light from the emitter does not shine directly onto the receiver. Smoke particles in the test atmosphere reflect or scatter light from the emitter into the receiver. Reflected detectors generally work well for gray smoke but have a decreased sensitivity to black smoke.




Smoke detectors typically use solid-state optical receivers such as photodiodes due to their low cost, small size, low power requirements, and ruggedness. One difficulty with solid-state receivers is their sensitivity to temperature. Additional circuitry that increases photo emitter current with increasing temperature partially compensates for temperature effects. Typical detectors also require complicated control electronics to detect the light level including analog amplifiers, filters, comparators, and the like. These components may be expensive if precision is required, may require adjustment when the smoke detector is manufactured, and may exhibit parameter value drift over time.




What is needed is a smoke detector with good sensitivity to both gray smoke and black smoke. The smoke detector should use a minimum of analog components to reduce cost and the possibility for component value drift over time. The smoke detector should also compensate for the effects of ambient temperature.











BRIEF DESCRIPTION OF DRAWINGS




The subject matter that is regarded as the invention is particularly pointed out and distinctly claimed in the claim portion that concludes the specification. The invention, together with further objects and advantages thereof, may best be understood by reference to the following description taken in conjunction with the accompanying drawings, where like numerals represent like components, and in which:





FIG. 1

is a schematic diagram illustrating a dual emitter smoke detector;





FIG. 2

is a schematic diagram illustrating emitter placement within a dual emitter smoke detector;





FIG. 3

is a schematic diagram illustrating the use of baffles in a dual emitter smoke detector;





FIG. 4

is a schematic diagram illustrating emitter placement having an increased effective path for direct light;





FIG. 5

is a schematic diagram illustrating opposing reflectors for increasing effective path for direct light;





FIG. 6

is a schematic diagram of a control circuit for a dual emitter smoke detector;





FIG. 7

is a timing diagram illustrating operation of a dual emitter smoke detector;





FIG. 8

is a schematic diagram of a light receiver driving and sensing circuit;





FIG. 9

is a schematic diagram of a light receiver circuit with a combined driving and sensing port;





FIG. 10

is a schematic diagram of a dual emitter smoke detector including an optional reference receiver;





FIG. 11

is a chart illustrating the operation of the dual emitter smoke detector when gray smoke is present;





FIG. 12

is a chart illustrating the operation of a dual emitter smoke detector when black smoke is present;





FIG. 13

is a flow chart illustrating operation of the controller for a smoke detector;





FIG. 14

is a circuit schematic illustrating the electrical connection for an optional reference receiver according to

FIG. 10

; and





FIG. 15

is a chart illustrating a smoke detector including additional dynamic scatter detector measurement thresholds.











DETAILED DESCRIPTION OF THE DRAWINGS




A smoke detector detects both black and gray smoke with good sensitivity and reduced temperature sensitivity. The smoke detector has simplified control elements and is inexpensive to produce. The smoke detector includes a housing defining a dark chamber, the chamber admitting a test atmosphere. A light receiver is disposed within the chamber. A scatter emitter within the chamber is positioned such that light from the scatter emitter strikes the receiver when reflected off particles suspended in the test atmosphere. An obscuration emitter disposed within the chamber is positioned such that light emitted by the obscuration emitter is directed to the receiver unless obstructed by particles suspended in the test atmosphere. In one embodiment, the scatter emitter emits light with a first principal emission wavelength and the obscuration emitter emits light at a second principal emission wavelength less than the first principal emission wavelength. The presence of smoke may be determined based on the amount of reflected light received and the amount of directed light received. The smoke detector may include a controller having a discrete output and a sense input. A capacitor may be connected to the discrete output and to a current path extending from the light receiver. A voltage sense path connects the capacitor to the sense input. The controller turns on an emitter, asserts the discrete output to charge the capacitor, and deasserts the discrete output. The elapsed time between when the discrete output is deasserted and when the sensed voltage crosses a threshold voltage level is determined. The amount of light from the asserted emitter is determined based on the elapsed time. In a refinement, the controller turns off all emitters and determines one or more dark reference levels. The dark reference levels can be used to determine the amount of light received from the asserted emitters.




Referring to

FIG. 1

, a schematic diagram illustrating a dual emitter smoke detector, is shown. A smoke detector, shown generally by


20


, includes housing


22


defining a dark chamber. The chamber admits test atmosphere


24


which may include smoke particles, some of which are shown and indicated by reference numeral


26


. Smoke detector


20


includes receiver


28


generating a signal on receiver output


30


based on the intensity of light striking receiver


28


. Scatter emitter


32


is positioned within the chamber such that emitted light


34


strikes receiver


28


if reflected off smoke particles


26


suspended in test atmosphere


24


. Scatter emitter


32


is controlled by scatter emitter signal


36


. Obscuration emitter


38


is positioned within housing


22


to generate light


40


that strikes receiver


28


unless obstructed by smoke particles


26


suspended in test atmosphere


24


. Obscuration emitter


38


is controlled by obscuration emitter signal


42


.




The combination of scatter emitter


32


and receiver


28


implements a scatter detector. The combination of obscuration emitter


38


and detector


28


effects an obscuration detector. Due to the generally differing sizes of black and gray smoke particles, smoke detection may be enhanced when obscuration emitter light


40


and scatter emitter light


34


have different principle emission wavelengths. For example, scatter emitter light


34


may be in the infrared range, or possibly a visible color light range, and obscuration emitter light


40


may be in a colored visible light range, such as blue, green, blue-green, red or violet light range. A visible color light emitter is preferable for the obscuration detector because the wavelength of such light is close to, or smaller than, the size of the black smoke particles, making the light easier for the black smoke particles to block, which is particularly advantageous for obscuration detectors having a short distance between the emitter


38


and the receiver


28


. Whereas known obscuration detectors typically use white light transmitted over a substantial distance, such as one meter or the width of a room, the obscuration detector comprising emitter


38


and receiver


28


can be implemented in a small area, such as a smoke detector housing having a length, height and width, each substantially less than 12 inches, and preferably the longest dimension of such housing is less than 7 inches.




Smoke detector


20


includes control unit


44


. Control unit


44


is coupled to receive output


30


, and generates scatter emitter signal


36


and obscuration emitter signal


42


. Control unit


44


is responsive to the receiver output


30


to generate a smoke detect signal at smoke detect signal output


46


, based on receiver output


30


, indicating the presence of smoke within test atmosphere


24


. Smoke detect signal


46


may be used to activate one or more fire alarm devices, not shown, such as audible warning devices, warning lamps, fire department notification devices, and the like.




In operation, control unit


44


turns on scatter emitter


32


. A first signal is received from receiver


28


indicating the amount of scatter emitter light


34


reflected from smoke particles


26


. Control unit


44


is responsive thereto to determine the amount of reflected light received. Control unit


44


turns on obscuration emitter


38


and receives a second output signal from receiver


28


indicating the amount of directed light from obscuration emitter light


40


not blocked by smoke particles


26


. Control unit


44


is responsive thereto to determine the amount of directed light received. Control unit


44


then determines the presence of smoke particles


26


in test atmosphere


24


based on the amount of reflected light received and/or the amount of directed light received. The duration of time that scatter emitter


32


is on may be dependent upon the amount of scatter emitter light


34


reflected to receiver


28


. Likewise, the duration of time obscuration emitter


38


is on may be dependent upon the amount of obscuration emitter light


40


striking receiver


28


. It is also envisioned that the scatter emitter and obscuration emitter can be controlled differently. For example, the scatter emitter may be on an amount of time dependent upon the amount of scatter emitter light


34


reflected to receiver


28


whereas the obscuration emitter on-time may be independent of the amount of obscuration emitter light


40


striking receiver


28


.




Referring now to

FIG. 2

, a schematic diagram illustrating emitter placement within a dual emitter smoke detector is shown. Smoke detector


20


includes a chamber, shown generally by


50


, formed by overlapping light baffle


52


defining side walls and front and back walls (not shown), which together form a dark chamber for test atmosphere


24


. Receiver


28


and scatter emitter


32


are held in receiver housing


54


. Receiver housing


54


establishes the spacing and angle between receiver


28


and scatter emitter


32


. Receiver housing


54


includes lip


56


at least partially blocking light from scatter emitter


32


so that none of scatter emitter light


34


directly strikes receiver


28


. Emitter housing


58


holds obscuration emitter


38


across from receiver


28


. The receiver housing


54


may be integrally molded with the front or back walls defining chamber


50


.




Several design variations can optionally be employed to reduce the amount of direct light from scatter emitter


32


striking receiver


28


. First, lens


59


may be used to focus light leaving scatter emitter


32


. Lens


59


may be a separate element as shown, or it may be molded as part of the housing for scatter emitter


32


. Second, scatter emitter


32


may be recessed in housing


54


, as shown. Third, receiver


28


may be recessed in housing


54


, as shown.




Referring now to

FIG. 3

, a schematic diagram illustrating the use of baffles in a dual emitter smoke detector is shown. One or more baffles


60


are placed between receiver


28


and obscuration emitter


38


. Each baffle


60


includes aperture


62


limiting the amount of obscuration emitter light striking receiver


28


. Each aperture


62


may include lens


64


operative to focus light emitted by obscuration emitter


38


onto light receiver


28


. The baffles


60


may be of any suitable construction, and may for example be plastic molded integrally with the housing comprising baffles


52


, a front wall (not shown) and a back wall (not shown). These baffles


60


enhance the obscuration detector by reducing the amount of forward scatter reaching the receiver


28


.




Referring now to

FIG. 4

, a schematic diagram illustrating emitter placement providing an increased effective path for direct light is shown. Receiver housing


70


holds receiver


28


, scatter emitter


32


, and obscuration emitter


38


. The length of the effective path that emitter light


40


travels in dark chamber


24


is approximately doubled using right angle mirror


72


to reflect light generated by the obscuration emitter


38


back to the adjacent receiver


28


. The longer effective path length for obscuration emitter light


40


increases the smoke detector's sensitivity to black smoke. In the presence of smoke, light emitted by obscuration emitter


38


will be blocked by some smoke particles and reflected off of other smoke particles. The amount of light reflected will depend on the color of the smoke and the size of the smoke particles, as gray smoke will reflect more light than black smoke, for example. By increasing the length of the light path from emitter


38


to receiver


28


, and selection of the emitter


38


to produce a desired light color, more light will be blocked by smoke particles and less reflected light will reach receiver


28


. The resulting obscuration detector thus has an increased sensitivity to smoke. Housing


70


includes optional diffusing and collimating lens


74


positioned in front of obscuration emitter


38


. Lens


74


smoothes the angular disparity of light leaving obscuration emitter


38


and controls the amount of obscuration emitter light


40


directed toward mirror


72


. A vertical wall


73


may advantageously be inserted in parallel with the direct path traveled by light


40


to reduce the amount of light from emitter


32


reflected by mirror


72


that strikes receiver


28


during scatter detector operation.




Referring to

FIG. 5

, a schematic diagram illustrates opposing reflectors to increase the effective path length for direct light through the dark chamber


24


. First reflective surface


76


includes a sequence of right angle reflectors. Opposing reflective surface


77


also includes a sequence of right angle reflectors. Reflective surfaces


76


,


77


are positioned such that light from obscuration emitter


38


bounces alternately off first reflective surface


76


and opposing reflective surface


77


, increasing the effective path of obscuration emitter light


40


. Additionally, lens


78


controls the pattern of light


34


leaving scatter emitter


32


.




Referring to

FIG. 6

, a schematic diagram of a control circuit for a dual emitter smoke detector. Control unit


44


includes a controller


80


which may be a microcontroller, a microprocessor, a digital signal processor, a programmable logic unit, or the like, and may, for example, be provided by part number PIC16CE624 commercially available from Microchip Technology Inc. of Chandler, Ariz. Scatter emitter


32


, implemented as light emitting diode D


1


, is connected between a 9 Volt supply potential and the collector of transistor Q


1


. The base of transistor Q


1


is connected to output GP


1


of controller


80


. The emitter of transistor Q


1


is connected through resistor R


1


to ground. Hence, output GP


1


generates scatter emitter signal


36


. Similarly, obscuration emitter


38


, implemented as light emitting diode D


2


, is connected between a 9 Volt supply and the collector of transistor Q


2


. The base of transistor Q


2


is connected to output GP


0


of controller


80


. The emitter of transistor Q


2


is connected through resistor R


2


to ground. Hence, output GPO generates obscuration emitter signal


42


. Each of transistors Q


1


and Q


2


may comprise NPN, PNP, FET or MOSFET elements, or the like, and may for example be a part number MPSA13 Darlington pair commercially available from Motorola, Inc. of Schaumburg, Ill. Heat sinking each transistor Q


1


, Q


2


with its respective controlled emitter D


1


, D


2


results in temperature compensation such that the amount of light generated by emitter D


1


, D


2


is less dependent upon ambient temperature.




Receiver


28


, implemented by photodiode PD


1


, is connected between supply voltage V


DD


and connection point


82


. Capacitor C


1


, indicated by


84


, is connected across receiver


28


. Resistor R


3


, indicated by


86


, joins connection point


82


with discrete output GP


2


of controller


80


, indicated by


88


. Connection point


82


is also connected to sense input


90


of controller


80


, labeled GP


3


. Preferably, sense input


90


is connected to a comparator, having an adjustable reference threshold, within controller


80


. Although the receiver


28


and capacitor C


1


are described as being connected between supply voltage V


DD


and connection point


82


, it will be recognized that the capacitor C


1


and receiver


82


can alternatively be connected in parallel between connection point


82


and ground.




In one embodiment, scatter emitter


32


has a principle wavelength between 850 and 950 nanometers and obscuration emitter


38


has a principle emission wavelength between 430 and 575 nanometers. For example, light emitting diode D


1


can be implemented using an MIE-546A4U, emitting light at a principal wavelength of 940 nanometers, available from Unity Optoelectronics Technology of Taipei, Taiwan. Light emitting diode D


2


may be an MVL-504B, emitting light at a principal wavelength of 470 nanometers, also available from Unity Optoelectronics Technology. The intensity of scatter emitter light


34


and obscuration emitter light


40


are dependent upon the values of resistors R


1


and R


2


, respectively. In this example, the resistance of resistor R


1


may be 7 Ω and the resistance of resistor R


2


may be 16 Ω


0


. Photodiode PD


1


may be, for example, a MID-56419, also available from Unity Optoelectronics Technology.




Referring now to

FIG. 7

, a timing diagram illustrates operation of a dual emitter smoke detector. The timing diagram shows one cycle during which the following timing measurements are made: a dark scatter reference; an elapsed scatter time that is based on scatter emitter light


34


impacting receiver


28


; a dark obscuration reference; and an elapsed obscuration time that is based on the amount of obscuration emitter light


40


impacting receiver


28


. The cycle is repeated periodically. Discrete output


88


toggles between supply voltage V


DD


and ground, and the sense input


90


toggles between floating and ground states. For convenience, asserting will refer to applying supply voltage V


DD


and deasserting will refer to grounding the terminal.




More particularly, discrete output


88


and sense input


90


are deasserted by connection to ground potential at time


100


. This causes capacitor


84


to charge to approximately voltage V


DD


. Discrete output


88


is asserted at time


104


, at which time sense input


90


is allowed to float, allowing the voltage across capacitor


84


to discharge through resistor


86


. Discharge will also occur due to the dark current produced by receiver


28


, connected in parallel to capacitor


84


. Asserting discrete output


88


, and permitting terminal


90


to float, triggers a counter within controller


80


to begin counting clock pulses, as indicated by counter signal


106


. The counter is halted when sense input


90


crosses threshold voltage level


108


. A comparator (not shown) internal to the controller compares the signal level on sense input


90


to a programmable reference level


108


, which is set to a default level during most of the measurement cycle. The dark scatter reference


110


is the elapsed time between when discrete output


88


is asserted and when sense input


90


crosses threshold voltage level


108


, and indicates a dark current reference level of receiver


28


. This dark scatter reference


110


is used in the scatter detector measurement as described herein below.




Discrete output


88


and sense input


90


are deasserted at time


112


, causing charging of capacitor


84


. Discrete output


88


is asserted at time


116


, at which time sense input


90


is permitted to float. At the same time, scatter emitter signal


36


is asserted, turning on scatter emitter


32


. The rate of discharge of capacitor


84


is dependent upon the amount of scatter emitter light


34


striking receiver


28


, as the capacitor


84


will discharge both through resistor


86


and due to the current through receiver


28


. Asserting discrete output


88


begins a counter within controller


80


, as indicated by counter signal


106


. The counter is turned off when sense input


90


crosses threshold voltage level


108


. The elapsed scatter time


118


, which is the elapsed time between asserting discrete output


88


and when sense input


90


crosses threshold voltage level


108


, is dependent upon the amount of scatter emitter light


34


striking receiver


28


. The more reflective smoke particles that are present, the more light from scatter emitter


32


that will strike receiver


28


, the more current that will be drawn through the receiver


28


, and the shorter the time required to discharge the capacitor


84


to the point that the sense input


90


crosses threshold voltage level


108


. Scatter emitter signal


36


may be deasserted at time


120


, following the elapsed scatter time


118


, such that the scatter emitter is turned off when the sense input


90


crosses threshold


108


.




At time


122


the output


88


is deasserted and the sense input


90


continues to float. The voltage level on the sense input


90


will drop to a level


121


, which is proportional to the magnitude of the dark current present at receiver output


30


, after an appropriate settling time for capacitor


84


. The settling time is selected to be the maximum amount of time expected for the capacitor to become substantially settled, and may for example be approximately 10 to 15 milliseconds. The internal comparator's reference threshold


108


is programmable to 1 of 32 different voltage levels. The magnitude range for the dark current is determined using this programmable threshold. Initially, threshold


108


is set to its lowest programmable value, and once the capacitor settling time has elapsed, a comparison is made to determine whether the voltage present on input


90


is higher than this lowest programmable level. If it is not, then the dark current magnitude is in the lowest range. If, however, the voltage present at input


90


is higher than the lowest programmable level, the reference level


108


is incremented to its next level. If the voltage present on sense input


90


is higher than the incremented reference level


108


, the reference level is incremented again, to the next programmable reference level. The sense input is then compared to that reference level. The process of incrementing the reference level to its next sequential level, and comparing the voltage on sense input


90


to that incremented sequential reference level, will be repeated until the level on input


90


is lower than the reference level


108


or the highest reference voltage is reached. The level to which threshold


108


must be raised in order to exceed the signal level on input


90


is the obscuration dark current reference level, and it is stored for later use in selecting an adjustment factor as described in greater detail herein below. The adjustment factor is used to compensate for temperature variations, thereby enhancing the accuracy of obscuration detector measurements made over a wide temperature range.




At time


123


, threshold


108


is returned to its default value, discrete output


88


is asserted, permitting capacitor


84


to discharge, and the counter begins counting, as indicated by counter signal


106


, while obscuration emitter signal


42


remains deasserted (i.e., emitter


38


is off). The counter is turned off when sense input


90


crosses voltage threshold


108


. The dark obscuration reference


127


, which is the elapsed time between asserting discrete output


88


and when sense input


90


crosses threshold


108


, is a reference dark current time count for obscuration emitter


38


. This dark obscuration reference


127


is used in the obscuration detector measurement as described herein below.




At time


124


, discrete output


88


is deasserted, the sense input


90


continues to float, and obscuration emitter signal


42


is asserted. Consequently, capacitor


84


begins charging at the same time as obscuration emitter


38


turns on. The capacitor


84


will charge to a potential such that the sense input


90


settles at voltage level


125


, which voltage level is dependent upon the amount of light striking the light receiver


28


. If no smoke is present, the emitter light


40


reaches receiver


28


without substantial blockage, inducing a large current in receiver


28


, resulting in a high voltage level


125


at time


126


. When more smoke is present, less emitter light


40


reaches receiver


28


, allowing the sense input


90


to reach a lower voltage


125


at time


126


. At time


126


, discrete output


88


is asserted, while sense input


90


floats, and the obscuration emitter is turned off, causing capacitor


84


to discharge through resistor


86


and receiver


28


. The time required for the capacitor to discharge to the point that sense input


90


crosses threshold


108


is inversely related to the amount of emitter light


40


striking receiver


28


between time


124


and time


126


. As noted above, the more smoke present while the obscuration emitter is on, the lower the voltage


125


at sense input


90


. The lower the voltage at time


126


, the more time will be required to discharge capacitor


84


to the point that the sense input


90


crosses above threshold voltage level


108


. The measurement of elapsed obscuration time


128


is initiated upon deasserting discrete output


88


. At that time, a counter within controller


80


begins counting, as indicated by counter signal


106


. The counter is turned off when sense input


90


crosses threshold voltage level


108


. The elapsed obscuration time


128


, between asserting discrete output


88


and when sense input


90


crosses over threshold voltage level


108


, indicates the amount of obscuration emitter light


40


striking receiver


28


during the interval from time


124


to time


126


. Preferably, measurements


110


,


118


,


127


and


128


are taken within a short period of time to properly compensate for dark current in receiver


28


. Elapsed obscuration time


128


is used in the obscuration detector measurement as described herein below.




Although not illustrated, it will be recognized that the length of time required to complete each measurement cycle can be reduced. Those skilled in the art will appreciate that if the times


112


,


122


,


124


and


129


are preset, the time period between asserting and deasserting the output


88


must be longer than the longest expected time required for the voltage on sense input


90


to cross threshold


108


. To reduce the cycle time, the time periods


112


,


122


,


124


and


129


are set dynamically as follows. As soon as the sense input


90


crosses the threshold


108


, the control input


88


is deasserted. As a consequence, the times


112


,


122


,


124


and


129


need not be set in advance, and they will occur at the earliest possible time for actual measurement conditions.




The operation of smoke detector


20


will now be described with reference to

FIGS. 6

,


7


, and


11


through


13


.

FIGS. 11 and 12

graphically illustrate the operation of the obscuration detector, using emitter


38


and receiver


28


, and the scatter detector, using emitter


32


and receiver


28


, when gray smoke and black smoke are present in the dark chamber.

FIG. 13

is a flow chart illustrating a smoke detector sensor cycle implemented under the control of controller


80


. The trapezoid boxes that are not numbered are comments provided to assist understanding, and are not steps in the operation of controller


80


. In each sensor cycle, the dark scatter time


110


is measured, as described above, in step


1300


. The scatter emitter


32


is energized at time


116


, as indicated in step


1302


, and the elapsed scatter time


118


is then measured, as described above, as indicated in step


1304


. The scatter ratio, which is the ratio of the elapsed scatter time


118


to the dark scatter reference


110


, is compared to a threshold TH


3


. As can be seen in

FIG. 11

, in the presence of gray smoke, the time required for the capacitor


84


to discharge while scatter emitter


32


generates light quickly decreases as the density of the smoke particles increases. This occurs because the amount of light from emitter


32


that strikes the receiver


28


after being reflected off of the smoke particles increases with increasing gray smoke density. This comparison to threshold TH


3


is made to determine whether the obscuration level is expected to be above or below 0.6%. If the scatter detector measurement is above threshold TH


3


, the cycle interval will be set to a long interval as indicated in step


1320


, and the cycle ends.




If the scatter emitter is below threshold TH


3


(point C in

FIGS. 11 and 12

) as determined in step


1306


, the dark obscuration reference


127


is measured, as indicated in step


1309


. The initial conditions are set using obscuration emitter


38


, as indicated in step


1310


. The initial conditions are set by turning the obscuration emitter


38


on and letting the capacitor


84


settle to a level


125


. The elapsed obscuration time


128


is measured, in step


1312


, by turning the emitter


38


off and measuring how long it takes for the voltage at terminal


82


to cross threshold


108


. In step


1314


, the state of the cycle interval is evaluated. If the cycle interval is long, the obscuration reference is set to the difference between the elapsed obscuration time


128


and the dark obscuration reference


127


, as indicated in step


1317


. This is the reference level taken at point C, as it is the first time the obscuration measurement is made after the scatter ratio crosses threshold TH


3


. Additionally, the short cycle interval is set in step


1318


, so that measurements will be taken more often. The controller


80


then determines whether the obscuration percentage change is below threshold TH


2


in step


1322


. If it is, the controller


80


will determine whether the scatter ratio dropped below the threshold TH


1


, as indicated in step


1308


, while emitter


32


is generating light. If it has dropped below TH


1


, the smoke detect signal is generated as indicated in step


1316


. A suitable alarm, such as an audible, visual, and/or electrical signal can then be generated.




If it is determined in step


1308


that the scatter ratio has not dropped below threshold TH


1


, although it is below TH


3


, and the obscuration measurement is below threshold TH


2


as determined in steps


1306


and


1322


, the smoke detector enters a pending alarm state and the cycle ends.




If it is determined in step


1322


that the obscuration percentage change is greater than threshoMarch 12, 2001ld TH


2


, the scatter emitter ratio is compared to a threshold TH


4


, in step


1324


. If the scatter time ratio is above TH


4


, the alarm condition continues to be pending, such that the measurement cycle is repeated more often, and the cycle ends. If the scatter ratio is below threshold TH


4


, an alarm detect signal is made, as indicated in step


1326


, and the cycle ends. As can be seen from

FIGS. 11 and 12

, when gray smoke is present, the time required for capacitor


84


to discharge while emitter


32


is generating light decreases much more quickly than when black smoke is present. As a consequence, the scatter detector will require a greater smoke density to cross the threshold TH


1


in the presence of black smoke, as compared to gray smoke. The smoke detector


20


uses the obscuration detector measurement to alter the scatter emitter threshold to TH


4


to enable the smoke detector to react more quickly. In the presence of gray smoke, the scatter ratio will cross threshold TH


1


well before the obscuration difference crosses threshold TH


2


. In the presence of black smoke, however, the obscuration difference crosses threshold TH


2


for a lower smoke density than that where the scatter ratio crosses threshold TH


1


. The smoke detector thus permits dynamic adjustment of the scatter emitter threshold from TH


1


to TH


4


to allow faster reaction by the scatter detector in the presence of black smoke.




Although the scatter detector and obscuration detector can operate independently, several advantages are gained by using them together as described above. For example, the short length of the obscuration detector light path from emitter


38


to receiver


28


affects its sensitivity. By using the scatter detector threshold TH


3


as a precondition to using the obscuration detector, the reliability of the obscuration detector is increased despite the relatively short length of the path for obscuration detector light


40


. Using the obscuration detector to reset the scatter emitter alarm threshold to TH


4


improves the scatter detector's sensitivity in the presence of black smoke while helping to avoid false alarms which would result if the scatter detector threshold is always low. Additionally, the scatter emitter can operate alone during most cycles as the obscuration detector need only be used after the scatter detector ratio reaches threshold TH


3


. This reduces the overall current drain of the smoke detector under non-alarm conditions, which is particularly important for battery-operated smoke detectors.




It is envisioned that the smoke detector sensor cycle will be repeated periodically, and that each cycle will last for a very short period of time. For example, the cycle may be repeated once every 5 to 45 seconds, and can for example occur once every 8 seconds. The cycle may last between 0.05 and 0.2 second, and may for example last approximately 0.1 second. The timing of the cycle is chosen to reduce power consumption without detrimentally impacting the response time of the smoke detector. Additionally, it is envisioned that the cycle will be repeated at a higher rate, set in step


1318


, such as once every 1 to 5 seconds, when the scatter ratio drops below threshold TH


3


, until the scatter ratio rises above threshold TH


3


, as determined in step


1306


, at which time the interval between sampling cycles will be reset to the longer interval in step


1320


, such as the exemplary once every 8 seconds interval described above.




An example of how the thresholds TH


1


-TH


4


can be selected will now be provided. The threshold TH


1


can be selected as follows. A scatter detector is placed in gray smoke having a density that causes a UL beam to detect approximately 2.5% obscuration/foot. “UL beam” refers to a beam detector test performed according to Underwriter's Laboratory (UL) test standards, such as UL268. The scatter detector measurement is made. The scatter detector measurement in that smoke density is used for the threshold TH


1


of the smoke detector. The threshold TH


3


is selected in a similar manner. The scatter detector is placed in gray smoke having a density such that UL beam will detect approximately 0.6% obscuration/foot. The scatter detector measurement in that density of smoke is threshold TH


3


. Threshold TH


4


is also selected in the same manner. The scatter detector is placed in gray smoke having a density such that a UL beam will detect approximately 1.25% obscuration/foot. The scatter detector measurement in that smoke density is the threshold TH


4


for the smoke detector. The threshold TH


2


is selected to correspond to approximately a 4% light reduction, which due to the short path length for light


40


, corresponds to approximately 6% obscuration/foot in the presence of black smoke as measured by a UL beam. For a new smoke detector operating using these thresholds in the presence of black smoke, the light from the obscuration emitter


38


is expected to be at approximately 98% of full intensity when it impacts receiver


28


at the time when the scatter detector ratio crosses threshold TH


3


. As long as the scatter detector detects at least this level of smoke, the obscuration emitter


38


will continue to operate, and the sensing cycle will be repeated at the higher repetition rate. When threshold TH


2


is exceeded the detector will change the scatter detector alarm threshold to be more sensitive, by using threshold TH


4


instead of threshold TH


1


. Those skilled in the art will recognize that the thresholds are merely exemplary, and that other thresholds could be used. Additionally, smoke detectors can be tailored for use in controlled environments by the selection of the threshold levels. For example, if the smoke detector is intended for use in a controlled environment where fuels (e.g., gasoline or kerosene) are stored, such that fires are expected to always have a high black smoke content, the thresholds TH


1


-TH


3


can be selected such that the smoke detector is more sensitive to black smoke without producing excessive false alarms. Those skilled in the art will also recognize that the actual smoke density thresholds for any particular smoke detector can vary due to aging of the smoke detector, environmental conditions, part tolerances, and the like.




It is further envisioned that instead of having two unique alarm thresholds, TH


1


and TH


4


, the alarm threshold could be proportionally adjusted by the amount of black smoke composition present, (i.e. TH


4


′=f(Scatter, Obscuration). To obtain an alarm at a consistent smoke density the function f(Scatter, Obscuration) can be implemented using a table-lookup. The following 5 point table 1 is provided as an example.















TABLE 1











Scatter




Obscuration



























1.25




4







1.56




3.16







1.87




2.5







2.18




1.78







2.5




1.1















The table represents the smoke detect threshold level TH


1


or TH


4


′ for the scatter detector as the obscuration detector % change measurements changes. Thus, when the obscuration measurement detects a 1.1 percent change, the scatter emitter threshold will be TH


1


. As mentioned above, TH


1


is the scatter emitter measurement taken in a smoke density that produces a 2.5 percent obscuration in a UL beam measurement. As the obscuration measurement rises, the smoke detect threshold for the scatter detector rises. When the obscuration detector measurement crosses 1.78 percent change, the scatter emitter threshold is raised to TH


4


′. For this obscuration measurement, TH


4


′ is a scatter emitter measurement taken in a smoke density that produces a 2.18 percent obscuration in a UL beam measurement. When the obscuration detector measurement crosses 2.5 percent change, the scatter emitter threshold is raised to the next threshold TH


4


′. For this obscuration measurement, TH


4


′ is a scatter emitter measurement taken in a smoke density that produces a 1.87 percent obscuration in a UL beam measurement. When the obscuration detector measurement crosses 3.16 percent change, the scatter emitter threshold is raised to the next threshold TH


4


′. For this obscuration measurement, TH


4


′ is a scatter emitter measurement taken at a smoke density that produces a 1.56 percent obscuration in a UL beam measurement. When the obscuration detector measurement crosses 4 percent change, the scatter emitter threshold is raised to the next threshold TH


4


′. For this obscuration measurement, TH


4


′ is a scatter emitter measurement taken in a smoke density that produces a 1.25 percent obscuration in a UL beam measurement. Thus it can be seen that as the obscuration measurement rises, the scatter detector smoke detect threshold rises proportionally. In operation, if the scatter measurement corresponds to a smoke level of greater than 2.5% obscuration/foot as measured by the UL beam, then an alarm would be generated regardless of the obscuration detector measurement as the threshold for the scatter detector measurement will be TH


1


. For scatter measurements that indicate a smoke level of less than 2.5% obscuration/ft, as measured by the UL beam, the alarm would be generated based on the evaluation of TH


4


′=f (Scatter, Obscuration). The different measurement thresholds TH


4


′ permit the smoke detector to produce a smoke detect signal in approximately the same smoke density (reference B in

FIG. 15

) regardless of the percentage of black and gray smoke. The reference levels are selected such a smoke detect signal will be generated at point B for reference level TH


1


if the smoke has 0% black smoke. The respective reference levels for TH


4


′ are selected such a smoke detect signal will be generated at density B in

FIG. 15

for: 25% black smoke; 50% black smoke; 75% black smoke; and 100% black smoke. It will be recognized that scatter threshold can alternately be generated as a direct function of the slope of the obscuration detector measurement.




The control system described with regards to

FIGS. 6 and 7

may be adapted to any number of emitters. The signal to noise ratio is an important consideration in selecting the threshold


108


. Threshold


108


is selected as permitted by the controller


80


so that substantial voltage changes do not produce small time differences. However, if the threshold voltage level


108


is too large, even very small variations in the voltage will result in substantial time differentials, such that the circuit will be highly susceptible to noise. It is envisioned that the threshold voltage


108


can be more than half of the supply voltage V


DD


used to charge the capacitor, and more particularly on the order of ⅞


th


of the voltage V


DD


. As noted above, the voltage is supplied to one input of an internal comparator, the other input of which is connected to sense input


90


. It is envisioned that a different threshold voltage level


108


may be used to determine the dark reference level and the light levels from each emitter


32


,


38


. For example, the threshold


108


for the scatter detector may be lower than the threshold


108


for the obscuration detector to account for the lower signal-to-noise ratio in the signal received from scatter emitter


32


.




In one embodiment a ratio of the received emitter light to the dark reference level at different times is used to compensate for variations in the value of capacitor


84


, and some of the affects of aging and temperature. A first ratio of the received emitter light


34


,


40


to the dark reference level under no smoke conditions is stored in controller


80


. During use, a new ratio of received emitter light


34


,


40


to the dark reference level is obtained. In particular, the calibrated measurement ratio used can be:






(T


118


/T


110


)/(T


118Ref


/T


110Ref


),






where T


118


is the measured elapsed scatter time


118


and T


110


is the measured dark scatter reference


110


time at a sampling time, and T


118Ref


is the elapsed scatter time


118


and T


110


Ref is the dark reference for a stored reference level. In particular, the reference ratio T


118Ref


/T


110Ref


is a stored calibration value representing a no smoke condition. This ratio of ratio represents the percentage of smoke present. An initial reference ratio value can be set and stored for the scatter and/or obscuration detector when the smoke detector is manufactured. Over time, the reference ratio can be altered to reflect changing performance characteristics of the smoke detector components, and to compensate for the presence of dirt, such as dust, in the dark chamber. These adjustments can be made by incremental compensation of the reference ratio in proportion to the gradual drift in measured ratios that do not produce an alarm indication. Thus, if the measured scatter and obscuration ratios at different sampling times drift up or down over a period of time, the associated reference thresholds can be adjusted to a higher or lower value to reflect that drift. Adjustments in the reference ratio would not be made for those measurement that result in a pending alarm or actual alarm condition. By using a ratio of the new received light-to-dark level ratio and the old light-to-dark level ratio removes the effects of long-range drift in capacitor


84


and compensates for temperature variations, which affects are cancelled by the ratio.




Variations in the characteristics of the obscuration detector may also be compensated for automatically. The obscuration detector uses a percent change calculation to detect a pending alarm condition. In particular, the following relationship is used:






(O


Ref


−O


Dif


)/O


Ref








where O


Ref


is an obscuration reference and O


Dif


is an obscuration difference. The obscuration difference is T


127


−T


128


. The obscuration reference is the obscuration difference recorded when the scatter measurement crosses threshold TH


3


. By using a percentage change threshold, instead of an absolute measurement, variations in the performance of the emitter


38


and the receiver


28


, whether caused by temperature variations, aging, dirt, or the like, can be compensated for during measurement.




Many configurations for sensing received light are possible. Each of these configurations includes controller


80


having discrete output


88


and sense input


90


. In some implementations, discrete output


88


and sense input


90


share a common input/output port. Capacitor


84


is connected to discrete output


88


. A path for current extends between capacitor


84


and light receiver


28


. A voltage sense path extends from capacitor


84


to sense input


90


. In these embodiments, the sense input is allowed to float while the discrete output changes from V


DD


to ground, for example.




Referring now to

FIG. 8

, a schematic diagram of a light receiver driving and sensing circuit according to an alternate embodiment is shown. Resistor RA is connected in parallel with receiver


28


between discrete output


88


and capacitor


84


. Capacitor


84


is directly connected to sense input


90


. Capacitor


84


is connected to ground. It will be recognized that the signals


88


and


90


will be inverted relative to the signals in

FIG. 7

, and further that the sense input


90


can float throughout the sensing cycle.




Referring now to

FIG. 9

, a schematic diagram illustrates a light receiver circuit with a combined driving and sensing port according to another embodiment. Resistor RB is connected between combined discrete output


88


and sense input


90


and the parallel combination of resistor RC, receiver


28


, and capacitor


84


. In this embodiment, it is envisioned that the voltage V


DD


will be applied to terminal


88


,


90


during charging and that terminal


88


,


90


will float otherwise. Thus, terminal


88


,


90


is indicative of the capacitor voltage, which over time is dependent upon the rate at which current is discharged by the capacitor


84


, which is in turn dependent on the current in the receiver


28


.




Referring now to

FIG. 10

, a schematic diagram of an embodiment of a dual receiver smoke detector is shown. Second receiver


140


is positioned such that light


142


from obscuration emitter


38


travels along an isolated path different from light


40


, the isolated path free from smoke in test atmosphere


24


. This may be accomplished by producing a sealed cavity in housing


144


between obscuration emitter


38


and receiver


140


, by inserting a light pipe between obscuration emitter


38


and receiver


140


, or the like. The receiver


140


is connected in parallel with resistor RA′ (

FIG. 14

) between output


88


′ of controller


80


and terminal


82


′. A capacitor


84


′ is connected between ground and terminal


82


′. A sense input


90


′ is connected to terminal


82


′. The capacitor


84


′, resistor RA′ and receiver


140


may be identical to capacitor


84


, resistor RA and receiver


28


, respectively. The Controller


80


determines the intensity of light


142


emitted by obscuration emitter


38


by monitoring sense input


90


′. Controller


80


then uses the determined intensity of light


142


emitted by obscuration emitter


38


and the intensity of light


40


passing through test atmosphere


28


to more accurately determine the presence of smoke as detected by the obscuration detector. Responsive to obscuration emitter


38


, the difference between the time measurements made from receiver


140


and the time measurements made from receiver


28


is indicative of the amount of smoke particles in the dark chamber. Such an arrangement compensates for variations in the performance of emitter


38


and receiver


140


.




It is envisioned that improved performance can also be obtained by normalizing for dark current, as an alternative to the ratio-of-ratios technique described above, for those measurements made responsive to the scatter emitter


32


, using the dark current voltage


121


range measurement made during the time interval


122


to


123


(FIG.


7


). Each of the voltages ranges of the comparator is associated with a respective calibration factor stored in the memory of controller


80


. These calibration factors are stored at the factory and are preselected based on measurements taken using a smoke detector under test conditions. The calibration factor for one of the voltage ranges, the normal voltage range, has a value of 1. The calibration factors for each of the other voltage ranges are selected to compensate for the amount that the dark current is expected to vary the actual measurement of elapsed scatter time


118


relative to measurement of elapsed scatter time


118


in the normal voltage range. By multiplying the stored calibration factor by the measured ratio of T


118


/T


110


, the measured result can be normalized to compensate for the affects of dark current. This is particularly important since the dark current in receiver


28


is highly sensitive to temperature, which significantly impacts on the discharge time of the capacitor


84


.




Alternatively, it is envisioned that the stored factor can be multiplied by threshold


108


, to vary the threshold


108


such that the larger the dark current voltage


121


measured during period


122


to


123


, the higher the threshold


108


during the measurement of the elapsed scatter time


118


. It will be recognized that the dark current voltage


121


measurement taken during period


122


to


123


can be taken prior to time period


116


, if the threshold


108


is to be adjusted during measurement of the elapsed scatter time


118


.




It will be recognized by those skilled in the art that the PIC16CE624 microprocessor from Microchip Technology includes an internal comparator and a resistor network providing 32 reference levels for the internal comparator. The voltage at terminal


82


is compared to each of these reference levels to determine between which of the 32 reference voltages the dark current voltage


121


of the capacitor


84


settles as noted above. The PIC16CE624 microcontroller advantageously includes 32 reference levels that divide the overall voltage range between V


DD


and ground into non-uniform, contiguous ranges, the smaller ranges providing finer resolution where the dark current voltage


121


on capacitor


84


is likely to settle. However, the reference voltages could alternately be at uniform, contiguous intervals, if desired.




Thus it can be seen that an improved smoke detector is disclosed. The improved smoke detector provides a reliable smoke detect signal without excessive false alarm signals. While embodiments have been illustrated and described, it is not intended that these embodiments illustrate and describe all possible forms of the invention. For example, it is envisioned that the obscuration detector could cause the controller to issue a smoke detect signal when the percent change crosses threshold TH


2


, rather than changing the scatter detector threshold from TH


1


to TH


4


when the obscuration detector crosses threshold TH


2


. Accordingly, the words used in the specification are words of description rather than limitation, and it is understood that various changes may be made without departing from the spirit and scope of the invention.



Claims
  • 1. A particle detector, comprising:a housing defining a dark chamber, the chamber admitting test atmosphere; a scatter emitter/receiver combination disposed within the chamber, the scatter emitter positioned such that any portion of the light emitted by the scatter emitter that is reflected off of particles suspended in the atmosphere and received is proportional to the amount of high reflectivity particles present in the atmosphere; an obscuration emitter/receiver combination disposed within the chamber, the obscuration emitter positioned such that any portion of the light emitted by the obscuration emitter that is received is inversely proportional to the amount of low reflectivity particles present in the atmosphere; and a controller coupled to the scatter emitter/receiver combination and the obscuration emitter/receiver combination, the controller using the amount of particles sensed by the obscuration emitter/receiver combination to alter the sensitivity of the scatter emitter/receiver combination.
  • 2. The particle detector of claim 1, wherein the scatter emitter/receiver combination and the obscuration emitter/receiver combination share a common receiver.
  • 3. The particle detector of claim 1, wherein the controller is also configured to change a particle detector sensor cycle when a high reflectivity particle level crosses an initial scatter emitter threshold, and wherein the rate of the particle detector sensor cycle determines the frequency with which at least one of the scatter emitter and obscuration emitter emits light.
  • 4. The particle detector of claim 3, wherein the controller causes the obscuration emitter to generate light only after the high reflectivity particle level crosses the initial scatter emitter threshold.
  • 5. The particle detector of claim 4, wherein a scatter emitter alarm threshold is modified to occur at a lower high reflectivity particle level when an obscuration emitter threshold is exceeded thus altering the sensitivity of the scatter emitter/receiver combination.
  • 6. The particle detector of claim 3, wherein the controller determines the high reflectivity particle level by calculating an initial scatter ratio whose numerator is related to a scatter conduction current provided by the receiver of the scatter emitter/receiver combination in response to light from the scatter emitter and whose denominator is related to a scatter dark current provided by the receiver of the scatter emitter/receiver combination in response to no light from the scatter emitter.
  • 7. The particle detector of claim 6, wherein the controller compensates for changing environmental conditions and degraded performance of the particle detector by altering a scatter reference ratio that is used to provide a normalized scatter ratio that replaces the initial scatter ratio, wherein the normalized scatter ratio is used to determine the high reflectivity particle level, and wherein the scatter reference ratio corresponds to a no particle scatter ratio that is occasionally updated under a no particle condition.
  • 8. The particle detector of claim 7, wherein the controller determines the low reflectivity particle level by calculating a percentage change in obscuration from one particle detector sensor cycle to another particle detector sensor cycle, and wherein a detected obscuration is related to a difference between a conduction time in which an obscuration conduction current is provided by the receiver of the obscuration emitter/receiver combination in response to light from the obscuration emitter and an obscuration dark time in which a dark current is provided by the receiver of the obscuration emitter/receiver combination in response to no light from the obscuration emitter.
  • 9. The particle detector of claim 8, wherein the controller compensates for changing environmental conditions and degraded performance of the particle detector by setting an obscuration reference, and wherein the obscuration reference is utilized as a base for later determinations of percentage change in obscuration.
  • 10. The particle detector of claim 9, wherein the obscuration reference is set when the scatter measurement crosses the initial scatter emitter threshold.
  • 11. A smoke detector, comprising:a housing defining a dark chamber, the chamber admitting test atmosphere; a scatter emitter/receiver combination disposed within the chamber, the scatter emitter positioned such that any portion of the light emitted by the scatter emitter that is reflected off of particles suspended in the atmosphere and received is proportional to the amount of gray smoke present in the atmosphere; an obscuration emitter/receiver combination disposed within the chamber, the obscuration emitter positioned such that any portion of the light emitted by the obscuration emitter that is received is inversely proportional to the amount of black smoke present in the atmosphere; and a controller coupled to the scatter emitter/receiver combination and the obscuration emitter/receiver combination, the controller using the amount of smoke sensed by the obscuration emitter/receiver combination to alter the sensitivity of the scatter emitter/receiver combination.
  • 12. The smoke detector of claim 11, wherein the scatter emitter/receiver combination and the obscuration emitter/receiver combination share a common receiver.
  • 13. The smoke detector of claim 11, wherein the controller is also configured to change a smoke detector sensor cycle when a gray smoke level crosses an initial scatter emitter threshold, and wherein the rate of the smoke detector sensor cycle determines the frequency with which at least one of the scatter emitter and obscuration emitter emits light.
  • 14. The smoke detector of claim 13, wherein the controller causes the obscuration emitter to generate light only after the gray smoke level crosses the initial scatter emitter threshold.
  • 15. The smoke detector of claim 14, wherein a scatter emitter alarm threshold is modified to occur at a lower gray smoke level when an obscuration emitter threshold is exceeded thus altering the sensitivity of the scatter emitter/receiver combination.
  • 16. The smoke detector of claim 13, wherein the controller determines the gray smoke level by calculating an initial scatter ratio whose numerator is related to a scatter conduction current provided by the receiver of the scatter emitter/receiver combination in response to light from the scatter emitter and whose denominator is related to a scatter dark current provided by the receiver of the scatter emitter/receiver combination in response to no light from the scatter emitter.
  • 17. The smoke detector of claim 16, wherein the controller compensates for changing environmental conditions and degraded performance of the smoke detector by altering a scatter reference ratio that is used to provide a normalized scatter ratio that replaces the initial scatter ratio, wherein the normalized scatter ratio is used to determine the gray smoke level, and wherein the scatter reference ratio corresponds to a no smoke scatter ratio that is occasionally updated under a no smoke condition.
  • 18. The smoke detector of claim 17, wherein the controller determines the black smoke level by calculating a percentage change in obscuration from one smoke detector sensor cycle to another smoke detector sensor cycle, and wherein a detected obscuration is related to a difference between a conduction time in which an obscuration conduction current is provided by the receiver of the obscuration emitter/receiver combination in response to light from the obscuration emitter and an obscuration dark time in which a dark current is provided by the receiver of the obscuration emitter/receiver combination in response to no light from the obscuration emitter.
  • 19. The smoke detector of claim 18, wherein the controller compensates for changing environmental conditions and degraded performance of the smoke detector by setting an obscuration reference, and wherein the obscuration reference is utilized as a base for later determinations of percentage change in obscuration.
  • 20. The smoke detector of claim 19, wherein the obscuration reference is set when the scatter measurement crosses the initial scatter emitter threshold.
  • 21. A particle detector, comprising:a housing defining a dark chamber, the chamber admitting test atmosphere; at least one receiver disposed within the chamber; a first emitter disposed within the chamber, where a received portion of the light emitted by the first emitter is proportional to the amount of high reflectivity particles present in the atmosphere; a second emitter disposed within the chamber, where a received portion of the light emitted by the second emitter is inversely proportional to the amount of low reflectivity particles present in the atmosphere; and a controller coupled to the first emitter, the second emitter and the at least one receiver, the controller using the amount of particles sensed using one of the first and second emitters to alter an alarm threshold of the remaining emitter.
  • 22. The particle detector of claim 21, wherein the controller is also configured to change a particle detector sensor cycle when a high reflectivity particle level crosses an initial first emitter threshold, and wherein the rate of the particle detector sensor cycle determines the frequency with which at least one of the first and second emitters emits light.
  • 23. The particle detector of claim 22, wherein the controller causes the second emitter to generate light only after the high reflectivity particle level crosses the initial first emitter threshold.
  • 24. The particle detector of claim 23, wherein a first emitter alarm threshold is modified to occur at a lower high reflectivity particle level when a second emitter threshold is exceeded.
  • 25. The particle detector of claim 22, wherein the controller determines the high reflectivity particle level by calculating an initial first emitter ratio whose numerator is related to a first emitter conduction current provided by the receiver in response to light from the first emitter and whose denominator is related to a first emitter dark current provided by the receiver in response to no light from the first emitter.
  • 26. The particle detector of claim 25, wherein the controller compensates for changing environmental conditions and degraded performance of the particle detector by altering a first emitter reference ratio that is used to provide a normalized first emitter ratio that replaces the initial first emitter ratio, wherein the normalized first emitter ratio is used to determine the high reflectivity particle level, and wherein the first emitter reference ratio corresponds to a no particle first emitter ratio that is occasionally updated under a no particle condition.
  • 27. The particle detector of claim 26, wherein the controller determines the low reflectivity particle level by calculating a percentage change in obscuration from one particle detector sensor cycle to another particle detector sensor cycle, and wherein a detected obscuration is related to a difference between a conduction time in which a second emitter conduction current is provided by the receiver in response to light from the second emitter and a second emitter dark time in which a dark current is provided by the receiver in response to no light from the second emitter.
  • 28. The particle detector of claim 27, wherein the controller compensates for changing environmental conditions and degraded performance of the particle detector by setting an obscuration reference, and wherein the obscuration reference is utilized as a base for later determinations of percentage change in obscuration.
  • 29. The particle detector of claim 28, wherein the obscuration reference is set when the first emitter measurement crosses the initial first emitter threshold.
Parent Case Info

This application is a continuation of U.S. patent application Ser. No. 09/456,470, entitled “SMOKE DETECTOR,” by Applicants Brian J. Kadwell et al., filed on Dec. 8, 1999, now U.S. Pat. No. 6,225,910 the disclosure of which is hereby incorporated by reference.

US Referenced Citations (50)
Number Name Date Kind
3968379 Crane Jul 1976
3980997 Berns et al. Sep 1976
3982130 Trumble Sep 1976
4001800 Franks Jan 1977
4063227 Peterson Dec 1977
4131888 Galvin Dec 1978
4185278 Lintlemann et al. Jan 1980
4241282 Tresch et al. Dec 1980
4249169 Malinowski Feb 1981
4319234 Rice Mar 1982
4420746 Malinowski Dec 1983
4469953 Fujisawa et al. Sep 1984
4539556 Dederich et al. Sep 1985
4614968 Rattman et al. Sep 1986
4647785 Morita Mar 1987
4678921 Nakamura et al. Jul 1987
4680576 Bauer Jul 1987
4758733 Mochizuki Jul 1988
4769550 Dolnick Sep 1988
4851819 Kawai et al. Jul 1989
4857895 Kaprelian Aug 1989
4870394 Corl et al. Sep 1989
5053754 Wong Oct 1991
5103096 Wong Apr 1992
5117219 Tice et al. May 1992
5138562 Shaw et al. Aug 1992
5247283 Kobayashi et al. Sep 1993
5341214 Wong Aug 1994
5369397 Wong Nov 1994
5400014 Behlke et al. Mar 1995
5473314 Mochizuki et al. Dec 1995
5523743 Rattman et al. Jun 1996
5546074 Bernal et al. Aug 1996
5552765 Vane et al. Sep 1996
5576697 Nagashima et al. Nov 1996
5592147 Wong Jan 1997
5629671 Morita May 1997
5673020 Okayama Sep 1997
5691704 Wong Nov 1997
5699043 Vane et al. Dec 1997
5705988 McMaster Jan 1998
5708414 Peltier et al. Jan 1998
5719557 Rattman et al. Feb 1998
5721529 Vane et al. Feb 1998
5726633 Wiemeyer Mar 1998
5751218 Winterble et al. May 1998
5767776 Wong Jun 1998
5896088 Brooks, Jr. Apr 1999
5898377 Adachi Apr 1999
6049446 Ha et al. Apr 2000
Continuations (1)
Number Date Country
Parent 09/456470 Dec 1999 US
Child 09/804543 US