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SMU FCO

Functional Checkout of the Secondary Mirror

Draft - a work in progress

This is a draft plan for the SMU FCO of July 2003 following its complete overhaul. It assumes passage of an electro-mechanical checkout on 22 July.

Participation of many JCMT staff is anticipated and appreciated. This document already contains contributions from JW and CW.

The document was written in advance of the completion of the repairs and has been updated in blue with the reality that followed.

Preliminaries

  1. Settings prior to the overhaul are as described in smu.ifl (in mt_smudir), and in the SMU focus document in this tree.
  2. It may be anticipated that nominal settings (zero-points) and limits will all change, but that relative positions may remain unchanged. For example :
    • the default Z focus position for SCUBA will change, but the relative offsets between SCUBA and other receivers will remain the same,
    • the values assigned to the soft limits will change, but (given the same screw pitch) the difference between the upper and lower limits should remain the same.
    Nonetheless, and to repeat, the FCO plan must anticipate 'all change'.
  3. It is anticipated that Chopper functionality has not been changed - i.e. that the subreflector and Chopping hardware have not been separated - although a cautious FCO would include one perfunctory check.
Daytime plan
  1. Determine hard limits on X,Y and Z tables (TCC, NTM), and set soft limits.
    • A May 2000 document ( /JACdocs/JCMT/a/003/17) describes the limits, ranges and hard stops of the X, Y and Z axes as follows :

      Axis
      limits
      (mm)
      range (mm)
      encoder units
      hard stops
      (mm)
      range (mm)
      encoder units
      current soft
      limits range
      X
      +23.5
      47.0
      12866
      +24.0
      48.0
      13140
      12900
      Y
      +23.5
      47.0
      12080
      +24.0
      48.0
      12337
      12975
      Z
      +22.8
      45.6
      12486
      +23.3
      46.6
      12760
      12600

    • Set X soft limits such that range again = 12900 units.
    • Set Y soft limits such that range again = 12975 units.
    • Set Z soft limits such that range again = 12600 units.

      Set zero-points using the similarity arguments above :

    • Set new X-zero-point = XLSL + 7262
    • Set new Y-zero-point = YLSL + 5585
    • Set new Z-zero-point = ZLSL + 6570

      (XLSL = X axis lower soft limit, etc.).

    The reality :

Nighttime Plan
  1. Start optimistically :
    • Configure telescope for SCUBA observing.
    • Set (dX,dY,dZ) = (0,0,0), (uaz,uel) = (0,0)
    • Take a jiggle map of a bright source (Jupiter early evening, G34.3 mid-evening-shift, Mars 2nd shift).
    • If source is seen on the array : skip to 5.

  2. Configure RxH3 as front end and point at HOLO, with offsets = (0,0) and a Z-focus setting of +31mm. (dZ should show on screen s0 as +31.00) (Ensure that the source at UKIRT is switched ON).
    The entry to watch is     Lo Sig Pwr, the signal strength.
    It may be possible to 'peak-up' on this signal using appropriate setoff commands, but if in doubt take a small (1000x1000 point) holography map : this should only take a few minutes, and will cover enough space to catch the signal. Jan will reduce offline (thank you) and provide 'pointing' offsets. The technique is insensitive to the focus offset.

  3. However, such pointing offsets are not due to pointing/collimation changes (for there have been none) so they must be due to a change in the configuration of the SMU tables. It is not anticipated that the optical-table-quality tables will be restored to a configuration too different from that prior to the shutdown so these 'pointing errors' ought to be small (and steps 3 & 4 ought to be unnecessary !).
    The offsets must be due to an error in the orientation of the tables w.r.t. the optical axis, either in translation or tilt. The optical precision of the SMU hopefully eliminates the latter. A translation error in X or Y of 1mm generates a displacement of the best image by 7mm, or 8" (calculations by IMC). Adjust the X & Y zero points accordingly to move the peak holography signal to the centre of the map. (Repeat the map and repeat . . .)

    Actually, the most recent RxH3 map of 30 June 2003 had pointing offsets of (-1",+7") (in (daz,del) = (Y,X) in SMU coordinates).

  4. Repeat step 1.

  5. On a more point-like source perform focus measurements and determine total offsets (dX,dY,dZ).

  6. Add these to (X_ZERO, Y_ZERO, Z_ZERO) in smu.ifl and mt_compifl (FJO). Repeat step 5 to ensure signs are OK - (dX,dY,dZ) should now be (0,0,0)


Iain Coulson
24 Jul 2003
Contact: Iain Coulson. Updated: Sat Nov 6 19:06:29 HST 2004

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