[Dire warning][TTF control system][Physical scan range][Fixing the resolution][Table of values]
However, several observers have demanded to know more so here we go. Please completely absorb this material before even contemplating a change in bandpass. . . .

The CS100 controller is central to the operation of the TTF. Our Mark I version of the CS100 can be operated manually from front panel controls, or under computer control using an RS232 interface. This expensive machine keeps the TTF plates parallel and allows the plate spacing to be tuned - from an optical point of view - over a very large physical range. The CS100 is attached to the exterior of TAURUS-2 in the Cass cage (bottom right). If you lie on the floor and look up, you should see it.
The front panel of the CS100 has a number of analogue dials and switches shown in the figure below. The X, Y and Z settings for the TTF are controlled through these analogue switches, although of course we have limited software control through the SMS window in the control room.
In the figure, the manual switches to the left are:

For our antiquated CS100, there are rather more switches below the meters than shown here but do not worry. Below, we use the subscript "f" for "fine" and "c" for "coarse".
You may have seen your support astronomer tweaking X and Y to check whether the TTF plates are roughly parallel. This is best done either (a) through the quadrant check under SMS, or (b) by eye at the access port using the Ne lamp when Zc = +5. For the purposes of tuning the bandpass, we can forget about X and Y, since Z is the variable that relates linearly to the spacing of the TTF plates.
The software variables under SMS which control X, Y and Z are called Xs, Ys and Zs. The next section explains the all important relations between the analogue coarse and fine dials, and the software variables.

XY physical movement. The
maximum allowed XY amplitude is 3.21
m.
The analogue Coarse range at the controller is (-5,+5) which corresponds
to (-1,+1)
m.
The Fine control gives an additional (0
10)
or 0.21
m.
The SMS control interface allows for (-2048,+2048) which corresponds
to (-0.5,0.5)
m.
Since the Fine control gives only a positive voltage, the total physical
scan range is (-1.5,+1.71)
m.
Z physical movement.The maximum
allowed Z amplitude is 13.05
m.
The analogue Coarse range at the controller is (-5,+5)
which corresponds to (-5,+5)
m.
The Fine control gives an additional (0
10)
or 1.05
m.
The SMS control interface allows for (-2048,+2048)
which corresponds to (-1,1)
m.
Since the Fine control gives only a positive voltage, the total physical
scan range is (-6,+7.05)
m.
An
illustration of the different instrumental response profiles for a range
of gap spacings (shown on the left hand side). The integer series indicates
the order of interference. For comparison, the RTTF filter set is shown
above to the same wavelength scale.
Note from the equation for
that each order of interference corresponds to a
physical displacement of the plates. This is how far the plates move when
they are scanned over a free spectral range. By now, you will know that
the instrumental response repeats over a free spectral range, as you will
have seen when scanning the plates using the variable Zs
under the SMS control window.
Remember that, in software, regardless of what resolution you are working
at, the free spectral range in Zs is always the same.
At
H
,
this is about 340.
The
free spectral range in Z scales linearly with wavelength, i.e. FSR(Zs)
corresponds to about 205 at 400nm.
The resolving power at any wavelength is
,
in other words,
.
This leads to a nice mnemonic at H
:
the
gap in microns is 1% of the resolving power. The available range
of resolving powers at every wavelength is shown here.
Therefore, for a chosen bandpass
,
the gap you want is
.
Below, we have determined a complete set of physical gaps for the primary
settings of Zc, Zf and Zs.
For convenience, choose a setting with Zf set to 0.
Note something fundamental to a fixed interferometric spacing. The bandpass
goes like
which can be a real problem. At any specific analogue setting, the software
control allows you to tune over a 2
m
range. So at small gap spacings, tuning over the full Zs
range can partly offset the effect. In other words, if you have set up
the BTTF to work at H
and [OII]3727, observe the former at high Zs and the
latter at low Zs. At large gap spacings, the
effect will be a problem until the new automatic control system is commissioned,
at which time you will be able to tune over the full physical range in
software.
! After you have dialed up the required settings from the table below, it is crucial that you force the software environment to accept these values. This is trivial to do. Simply turn off the external control and open the CS100 loop in software, then turn external control back on, and close the loop again. To wit, if you are familiar with the SMS key pad -- which I presume you are otherwise you wouldn't have come this far -- hit "." and then type
obeyw taurus EXTERNAL falseand after a few seconds or so, type
obeyw taurus CLOSE_LOOP false
obeyw taurus EXTERNAL trueIf you prefer to mess with the SMS window system, go to setup / change_cs100 and do the equivalent operations there.
obeyw taurus CLOSE_LOOP true
You must never turn Zc below -2 (`below' means `more negative') in case you squash the plates together. For the expert, please do not attempt to access a setting in (Zc, Zf, Zs) smaller than 3 microns.
Zc Zf Zs gap (um) 1 -5. 0.00 -2048. -0.51 (negative gaps do exist!) 2 -5. 0.00 0. 0.49 DO NOT USE 3 -5. 0.00 2048. 1.49 DO NOT USE 4 -5. 5.00 -2048. 0.01 DO NOT USE 5 -5. 5.00 0. 1.01 DO NOT USE 6 -5. 5.00 2048. 2.01 DO NOT USE 7 -5. 10.00 -2048. 0.54 DO NOT USE 8 -5. 10.00 0. 1.54 DO NOT USE 9 -5. 10.00 2048. 2.54 DO NOT USE 10 -4. 0.00 -2048. 0.49 DO NOT USE 11 -4. 0.00 0. 1.49 DO NOT USE 12 -4. 0.00 2048. 2.49 DO NOT USE 13 -4. 5.00 -2048. 1.01 DO NOT USE 14 -4. 5.00 0. 2.01 DO NOT USE 15 -4. 5.00 2048. 3.01 DO NOT USE 16 -4. 10.00 -2048. 1.54 DO NOT USE 17 -4. 10.00 0. 2.54 DO NOT USE 18 -4. 10.00 2048. 3.54 19 -3. 0.00 -2048. 1.49 DO NOT USE 20 -3. 0.00 0. 2.49 DO NOT USE 21 -3. 0.00 2048. 3.49 22 -3. 5.00 -2048. 2.01 DO NOT USE 23 -3. 5.00 0. 3.01 DO NOT USE 24 -3. 5.00 2048. 4.01 25 -3. 10.00 -2048. 2.54 DO NOT USE 26 -3. 10.00 0. 3.54 27 -3. 10.00 2048. 4.54 28 -2. 0.00 -2048. 2.49 DO NOT USE 29 -2. 0.00 0. 3.49 30 -2. 0.00 2048. 4.49 31 -2. 5.00 -2048. 3.01 DO NOT USE 32 -2. 5.00 0. 4.01 33 -2. 5.00 2048. 5.01 34 -2. 10.00 -2048. 3.54 35 -2. 10.00 0. 4.54 36 -2. 10.00 2048. 5.54 37 -1. 0.00 -2048. 3.49 38 -1. 0.00 0. 4.49 39 -1. 0.00 2048. 5.49 40 -1. 5.00 -2048. 4.01 41 -1. 5.00 0. 5.01 42 -1. 5.00 2048. 6.01 43 -1. 10.00 -2048. 4.54 44 -1. 10.00 0. 5.54 45 -1. 10.00 2048. 6.54 46 0. 0.00 -2048. 4.49 47 0. 0.00 0. 5.49 48 0. 0.00 2048. 6.49 49 0. 5.00 -2048. 5.01 50 0. 5.00 0. 6.01 51 0. 5.00 2048. 7.01 52 0. 10.00 -2048. 5.54 53 0. 10.00 0. 6.54 54 0. 10.00 2048. 7.54 55 1. 0.00 -2048. 5.49 56 1. 0.00 0. 6.49 57 1. 0.00 2048. 7.49 58 1. 5.00 -2048. 6.01 59 1. 5.00 0. 7.01 60 1. 5.00 2048. 8.01 61 1. 10.00 -2048. 6.54 62 1. 10.00 0. 7.54 63 1. 10.00 2048. 8.54 64 2. 0.00 -2048. 6.49 65 2. 0.00 0. 7.49 66 2. 0.00 2048. 8.49 67 2. 5.00 -2048. 7.01 68 2. 5.00 0. 8.01 69 2. 5.00 2048. 9.01 70 2. 10.00 -2048. 7.54 71 2. 10.00 0. 8.54 72 2. 10.00 2048. 9.54 73 3. 0.00 -2048. 7.49 74 3. 0.00 0. 8.49 75 3. 0.00 2048. 9.49 76 3. 5.00 -2048. 8.01 77 3. 5.00 0. 9.01 78 3. 5.00 2048. 10.01 79 3. 10.00 -2048. 8.54 80 3. 10.00 0. 9.54 81 3. 10.00 2048. 10.54 82 4. 0.00 -2048. 8.49 83 4. 0.00 0. 9.49 84 4. 0.00 2048. 10.49 85 4. 5.00 -2048. 9.01 86 4. 5.00 0. 10.01 87 4. 5.00 2048. 11.01 88 4. 10.00 -2048. 9.54 89 4. 10.00 0. 10.54 90 4. 10.00 2048. 11.54 91 5. 0.00 -2048. 9.49 92 5. 0.00 0. 10.49 93 5. 0.00 2048. 11.49 94 5. 5.00 -2048. 10.01 95 5. 5.00 0. 11.01 96 5. 5.00 2048. 12.01 97 5. 10.00 -2048. 10.54 98 5. 10.00 0. 11.54 99 5. 10.00 2048. 12.54 Zc Zf Zs gap (um)
The next generation control system. One could increase this
scan range with an analogue switch summation point in the circuitry. The
new look TTF interface will circumvent the CS100 control panel and allow
the full physical range to be scanned with an 18-bit bus, or a unique step
of
m,
equivalent to 0.5Å. The commissioning should be complete by the end
of the millenium.