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Advanced  Problems                                                    45











                        Light  Iron-
                        snai  oojeci                         MEMS actuator
                                                      Kv     (not  10 scale)

                        rVfnTmaMp.  ,      ^ ^
                            mirror
                                              Wavefront sensor
                                                                    Controller
                                               and algorithms
                      FIGURE AP1.4  Extremely large optical telescope with deformable  mirrors
                     for atmosphere compensation.



      AP1.4  Adaptive optics has applications to a wide variety of   control one of the deformable mirrors to compensate for
          key  control  problems, including  imaging  of  the  human  the distortions in the incoming light. Figure AP1.4 shows
          retina  and  large-scale,  ground-based  astronomical  a diagram of the telescope with a single deformable mir-
          observations [98]. In both cases, the approach is to use a   ror. Suppose  that  the  mirror  has  an  associated  MEMS
          wavefront sensor to measure distortions in the incoming   actuator  that can be used  to vary the orientation. Also,
          light and  to  actively control and compensate to the er-  assume  that the  wavefront  sensor  and  associated  algo-
          rors induced  by the distortions. Consider  the case  of an   rithms  provide  the  desired  configuration  of  the  de-
          extremely  large  ground-based  optical  telescope, possi-  formable  mirror to the feedback  control system.
          bly  an  optical  telescope  up  to  100 meters  in  diameter.
          The  telescope components include deformable  mirrors  AP1.5  The Burj  Dubai  is the tallest  building in the world
          actuated by micro-electro-mechanical  (MEMS) devices   [94]. The  building,  shown  in  Figure API.5, stands  at
          and sensors  to measure  the  distortion  of  the  incoming
          iight as it passes through the turbulent and uncertain at-
          mosphere of Earth.
            There  is  at  least  one  major  technological  barrier
          to constructing a  100-m optical telescope.The numeri-
          cal  computations  associated  with  the  control  and
          compensation  of the extremely large optical  telescope
                            10
          can be on the order  of 10  calculations each  1.5 ms.To
          date, this computational  power  is unachievable. If  we
          assume  that  the  computational  capability  will  ulti-
          mately  be available, then  one can consider  the  design
          of  a  feedback  control  system  that  uses  the  available
          computational  power. We  can  consider  many  control
          issues  associated  with  the  large-scale  optical  tele-
          scope. Some  of  the  controls  problems  that  might  be
          considered  include  controlling  the  pointing  of  the
          main  dish, controlling the  individual  deformable  mir-
          rors, and  attenuating  the deformation  of the  dish  due
          to changes  in outside temperature.
            Employing  Figure  1.3 as a  model  for  the block  dia-  FIGURE AP1.5  The world's tallest  building in
          gram, describe a closed-loop feedback  control system to   Dubai. (Photo courtesy of Alamy  Images.)
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