Adjustment and Maintenance
4
should be loosened slightly and the Superspring leveled. These M5 screws
have a M4 hex socket head. The Superspring should be unlocked
mechanically to let free the reference test mass. The translator plate
underneath the interferometer base (twiddler) should be put into its mid
range position so that the glass surface is normal to the beam. The top
mounting plate can be translated so that the beam travels cleanly through the
Superspring. Ideally, the test beam should overlap the reference beam in the
fringe viewer. Sometimes there is not enough range on the plate to get the
beams overlapped totally in the fringe viewer in the horizontal direction but
you should be able to get the two beams to have the same vertical position in
the fringe viewer. Finally, tighten the screws on the top mounting plate and
relevel the Superspring. Recheck the alignment after screws have been
tightened.
4.2.2.13.Final Mirror Translation-Getting Beams
Overlapped In Fringe Viewer
To move the test beam horizontally to overlap in the fringe viewer with the
reference beam it is sometimes necessary to translate the final adjustment
mirror underneath the interferometer base. Before doing so look through the
telescope and adjust the mirror until the two spots are coincident in the
telescope. This will ensure that the angle of the reference and test beams are
the same even though they may not yet be coaxial. Then you can turn all
three screws on the mirror mount in the same direction to translate the test
beam relative to the reference beam. Always watch the beam in the telescope
and make sure that you end up with the two beams overlapped in the
telescope. Once the reference and test beams overlap in the fringe viewer and
in the telescope they two beams are coincident and will produce good fringes.
4.2.2.14.Adjusting the APD signal detector
Preparations and Electrical hookups: Remove the dropper and tripod from
the interferometer base (IB) and remove the center section of the IB top cover
and the IB top cover containing the fringe viewer. Monitor the DC light level
from the avalanche photodiode (APD). It is usually best to do this using a
scope. The DC light level is available on the Analog Out port on the
interferometer base.
4-16
Summary of Contents for FG5
Page 22: ...Design Components and Function 2 Figure 2 10 The Superspring 2 14 ...
Page 31: ...Design Components and Function 2 Figure 2 13 Rotation Monitor 2 23 ...
Page 32: ......
Page 42: ...How to Set Up and Run the FG5 3 3 10 ...
Page 44: ...How to Set Up and Run the FG5 3 Figure 3 2 V Post 3 12 ...
Page 53: ...How to Set Up and Run the FG5 3 1 Backup the data 2 Shut off computer power 3 21 ...
Page 87: ...Adjustment and Maintenance 4 4 29 ...
Page 91: ...Adjustment and Maintenance 4 4 33 ...
Page 104: ...Troubleshooting 5 5 2 ...
Page 117: ...Troubleshooting 5 5 15 ...
Page 131: ...Checklists and Logs Appendix D 9 3 ...
Page 140: ...Checklists and Logs Appendix D Table 9 6 Replacing Drive Belt 9 12 ...
Page 145: ...Checklists and Logs Appendix D Table 9 10 Replace Linear Bearings 9 17 ...
Page 149: ...Checklists and Logs Appendix D Table 9 13 Replace Shaft Encoder 9 21 ...