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Secondar Mirror : Focus Settings

JCMT - Secondary Mirror : Focus Settings



CONTENTS


The SMU.IFL file describes the calculation of the three focus positions as follows :

(X + DX + SX + X_ZERO) * X_SCALE
(Y + DY + SY + Y_ZERO) * Y_SCALE
(Z + DZ + SZ + Z_ZERO) * Z_SCALE.

where

          X = XB + XA * COS (ELEVATION)
          Y = YB
          Z = ZB + ZA * SIN (ELEVATION) + ZC*SIN(ELEVATION)**2

Current (July 2003) values of these coefficients are

X
 
Y
 
Z
 
Notes
XA
5.791
 
 
 
 
ZA
0.54
 
 
XB
-5.838
 
YB
3.73
 
ZB
-12.53
 
 
 
 
 
 
 
 
ZC
0.845
 
 
DX
0.0
 
DY
0.0
 
DZ
0.0
 
(1)
SX
0.0
 
SY
0.0
 
SZ
0.0
 
(2)
X_ZERO
-27.99
 
Y_ZERO
+22.88
 
Z_ZERO
+25.09
 
(3)
X_SCALE
-273.756
 
Y_SCALE
+257.02
 
Z_SCALE
+273.817
 
(4)

Notes:
  1. default value; updated as a result of focus observation
  2. an increment applied only during observations
  3. encoder zero in mm
  4. encoder units per mm

Receiver-dependent offsets also apply and are as follows (July 2003, in mm) :

FE
X
Y
Z
SCUBA
-0.09
0.15
-5.27
RXA3I
0.33
-0.26
-1.01
RXB
0.16
-0.12
-0.96
RXW_C
0.74
-0.44
-1.00
RXW_D
0.18
0.14
-0.77
FTS
0
0
0


NB: Focus offsets are now (2006) kept in Rx/FE-specific files like
/jac_sw/itsroot/src/wrappers/rxa/initialise/instrument_rxa.ent

The Z focus is also a function of temperature :
          DZT = DZT_CONST + ( DZT_COEFF * MEAN_TEMPERATURE )
where


(DX, DY, DZ) may be seen in the lower left of the 's0' screen (as dX, dY, dZ), while X, Y, Z (before the addition of the zero-points) are shown in the top few lines of the 's3' screen. X_encoder, Y_encoder, Z_encoder lie a few lines below this.

Potentially the following range of values may occur for SCUBA at a temperature of 4oC :

Axis
Elevation = 0
Elevation = 90
Elevation = 0
Elevation = 90
soft
lower
limit
soft
upper
limit
(mm)
(encoder units)
X
-0.14
-5.93
7700
9286
400
13300
Y
+3.88
+3.88
6878
6878
275
13250
Z
-17.80
-16.41
1996
2375
300
12900

The last 2 columns show the 'soft' limits for these travels, and the expected demand values are seen to be well away from these limits. Even a +5.9mm change (as suggested by obsn. #0028 on UT20030706 that preceded the reported SMU tables failure) would only change the demand by -1615 units : still not enough to reach these soft limits.

In the event of an SMU fault that effectively disables one axis, it is obvious that the axis to best cope with this is Y, since it is unaffected by changes in elevation. If it can be set to one particular value before being disabled then set it to
  • DY = 0.0 mm, or an encoder value of 6878 for SCUBA.
If you must fix X or Z to one value, then you must effectively optimize the setting for one elevation, and accept focus errors at other elevations. Optimal values for SCUBA are :

Elevation
X
Z
mm
encoder
units
mm
encoder
units
15
-0.33
7779
7.49
2049
30
-0.91
7912
7.77
2128
40
-1.49
8071
7.99
2187
50
-2.21
8268
8.20
2245
60
-3.03
8493
8.39
2298
70
-3.95
8744
8.54
2339
80
-4.92
9010
8.64
2366
90
-5.93
9287
8.68
2375


These values may be seen in appropriate parts of the 's3' screen.

For other receivers add the following amounts :

Receiver
Axis
mm
enc.units
RxA3i
X
0.44
-120
Z
4.26
1166
RxB
X
0.25
-68
Z
4.31
1180
RxW_C
X
0.83
-227
Z
4.27
1169
RxW_D
X
0.27
-74
Z
4.50
1232
FTS
X
0.09
-25
Z
5.27
1443


Default increments (SX,SY,SZ) during focus measurements are 0.3mm in Z and 1.0mm in X & Y. Fluxes drop to about 70% of peak flux at 2 increments away in all axes. So having the X or Z axis optimized for eg 50 degrees elevation and observing at 70 degrees elevation incurs a focussing error of less than 2 increments (0.6mm in Z, 2.0mm in X). For most observing therefore you may wish to adopt the el=50 or el=60 values above as most useful - or tailor the optimization to match your specific future observing needs, i.e. the likely elevations.

Contact: Iain Coulson. Updated: Wed Sep 6 12:18:53 HST 2006

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