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20  (FG5)  or  33(FG5-X)  centimetres.  The  dropping  chamber  is
                  maintained at vacuum by use of an ion pump and sits upon its own
                  tripod,  to  isolate  it  from  the  other  components  of  the  FG5,  most
                  importantly  from  the  super-spring  component,  as  the  vibrations

                  created in the movement of the cart within the chamber are significant,
                  but even so the recoil from the floor of from the tripod can be easily
                  detected in the individual drop residuals.

                        Below the dropping chamber and central to the design of the FG-
                  5 is a modified Mach-Zender interferometer. A collimated continuous
                  wave 633nm laser beam enters into the side of the interferometer and
                  is  split  into  two  optical  arms,  one  arm  straight  through  the  beam

                  splitter to generate a reference arm whilst the other is reflected up into
                  the dropping chamber to reflect off  of the corner cube before being
                  reflected  down  to  another  corner  cube  within  the  ‘super-spring’

                  assembly which is then recombined inside the interferometer with the
                  reference arm of light. These recombined arms of laser light generate
                  the interference fringes which form the basis of the determination of

                  gravity.
                        To  provide  an  inertial  reference  frame  and  vibration  isolation
                  from the high frequency natural micro-seismic activity of the planet,

                  the  FG-5  (Figure  13.2.)  has  a  unique  super-spring  component  (or
                  assembly) which is coupled to the interferometer above it. The free-
                  fall  trajectory  of  the  dropped  object  is  referenced  to  a  very  stable
                  activespring system called a “Superspring”. The Superspring provides

                  seismic-isolation  for  the  reference  optic  to  improve  the  noise
                  performance of the FG5.




























                                Figure 13.2. Image courtesy of Micro-G LaCoste
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