Page 517 - Instrumentation Reference Book 3E
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500  Optical measurements
             improvements in performance may  be  expected.
             All may be made sensitive to visible or near infra-
             red  radiation.  The  usual  noise  considerations
             apply,  and  charge  leakage  between  elements
             implies that the scan interval must be  less than
             1 s. CIDs offer the possibility of very rapid read-
             out, so that they may be introduced for television
             purposes;  they  also  permit  sampling  patterns
             other than straightforward roster scanning. There
             is also the possibility that, by using two variants
             of CCDs in a single device, a CCD may develop
             with  dual  red  and blue  sensitivities. CCDs  are
             also commonly used in video cameras at the pres-
             ent time. The development  of these devices con-
             tinues to be intensive.                      motor                optical pick-up
               Outputs from array detectors may be displayed                   for phase-sensitive
             as a line scan on a CRO or as  a raster  display;                 detector
             alternatively, they may be fed into a microproces-   Figure 21.7  Chopperdisc.
             sor.  Their  applications  are numerous;  emission
             spectroscopy,  size measurement,  position  meas-
             urement,  robot  guidance,  facsimile recognition,   (2)  Cooling  the detector;
             and document  reading are amongst  them. With   (3)  Using  synchronized techniques.
             improvement in manufacturing technique it is to
             be expected that their cost will be greatly reduced   21.4.1  Detector circuit time constants
             in the next few years and their use become more
             widespread.                              Dark current  noise is due to random  events on
                                                      the atomic scale in the detector. Hence if the time
                                                      constant  of  the  detector  circuit  is  made  suffi-
             21.4  Detector techniques                ciently long the variations in the output current
                                                      will be smoothed out, and it will be of a correct
             In  nearly  all  optical  instruments  which  require   average value. The best  choice of  time constant
             a  measurement  of  light  intensity  we  rely  upon   will depend on the circumstances of any applica-
             the detector producing a signal (usually a current)   tion,  but  clearly  long  time  constants  are  not
             which  is  accurately  proportional  to  the  light   acceptable in many cases. Even in manually read
             intensity. However, all detectors, by their nature,   instruments a time constant as long as 1 s will be
             pass some current when in total darkness, and we   irritating to the observer.
             have to differentiate between the signal which is
             due to “dark current” and that due to “dark cur-
             rent plus light current.” A further problem arises if   21.4.2  Detector cooling
             we  try  to  measure  very  small  light  currents  or   It is  not possible to go into a full discussion of
             larger light currents very accurately. In all detec-   detector  noise  here  but  in  many  detectors  the
             tors there are small random variations of the dark   largest contribution to the noise is that produced
             current-i.e..   ”noise”-and  it  is  this noise which   by thermionic emission within the detector. Ther-
             limits the ultimate sensitivity of any detector.   mionic emission from metals follows Langmuir’s
               The differentiation  between “dark”  and “dark   law:
             plus light” signals is achieved by taking the differ-
             ence of  the signals when  the  light beam  falls on
             the  detector  and  when  it  is  obscured.  In  some   where Tis absolute temperature and i represents
             manually  operated  instruments  two  settings are
             made, one with and one without a shutter in the   the  emission  current.  Room  temperature  is
                                                      around 295 K  in terms  of  absolute temperature,
             beam. In most instruments a chopper disc (Figure   so a significant reduction in emission current and
             31.7) is made to rotate in the light beam so that the   noise can be achieved by cooling the detector.
             beam is interrupted at a regular frequency and the   Detectors  may  be  cooled by  the  use  of liquid
             signal  is  observed  by  as. circuits  that  do  not   nitrogen  (77K, -196”C),  solid  C02  (195K,
             respond to the continuous dark current. This tech-   -79°C).  or by Peltier effect cooling devices. The
             nique is called “beam chopping.”         use  of  liquid  nitrogen  or  solid  C02 is  cumber-
               The effects of noise can be reduced in three ways:
                                                      some; it usually greatly increases the complexity
             (1)  Prolonging  the time constant of the detector   of  the  apparatus  and  requires  recharging.
                circuitry;                            Another  problem  is  that  of  moisture  from  the
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