Last updated on 19-Jun-2001 12:25 AM

 

 

Warm Up Procedure

1   Warming Up

2   Cooldown Record

1   Warming Up (2 days)

DATE/TIME:
The detector should not be the coldest part of the instrument during the warm-up procedure. This is to avoid it collecting ice if there is a leak. It can be heated using the the Lakeshore LS330 Temperature Controller, but be sure to avoid shock heating the array (temperature change > 1K per minute), by using the 'Low' heater setting when the detector is below ~120K, and only the 'Medium' heater setting at higher temperatures. Additional heaters are attached to the 4K (nominally 5 Watt dissipation) and first (20W nominal dissipation) stages of the Joule-Thomson cooler.
The bulk of the cryostat is warmed back up to room temperature using heater panels attached to the optics box and the radiation shield, with fixed heating powers of 450 Watts and 150 Watts respectively.   Typical warm-up curves are shown in Figure 1.

 

Figure 1. Warming up Michelle. The cryostat can be backfilled with dry nitrogen gas once the temperatures have risen above 120K.

Make the Array safe by loading the "Protect_Array" waveform via the waveform Generator control screen (LINK TO DJI STUFF)
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Open the JT and Bypass valves (clockwise) to 5 turns and close again immediately to 4 turns ( to remove backlash). Switch off the JT Compressor followed by the associated GM motor and finally the compressor (see below re Gemini).
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If the Instrument is remaining on UKIRT to warm-up completely no further action is needed with the JT Helium system. If, however, the cryostat is to be removed from UKIRT during the warm-up, the disconnection of the JT Helium supply lines (with system pressures equalized) will result in a pressure build-up within the cooler which will vent via the pressure relief valves.

On the Gemini Telescope the compressors will run permanently and all the Helium supply lines will have to be disconnected at the Cassegrain wrap interface once the GM coldheads are depowered.

In both cases some system recharging with N6 Helium will be required once the Instrument is warm. At UKIRT only the JT pipework will need recharging to 150psi whilst on Gemini all three manifolds will probably need to be done.

The heater at the Detector is controlled via the Lakeshore LS330 controller. Check/adjust the setpoint to 300K and switch on the heater at the 'Low' setting.
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Using a dual DC Power supply apply the following voltages to the first and third stages of the Joule-Thomson cooler:-

First (70K) Stage:

~23V giving ~20W power input (25.7 ohm resistor)

Third (4K) Stage:

11.3V giving 5W power input (25.7 ohm resistor)

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Switch off the Main GM Coldhead motor and subsequently the Compressor (see note above re Gemini). The GM Coldhead can be safely disconnected from the Helium pipework without subsequent recharging.

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1.2   Apply heat to the Main Optical Bench and Radiation Shield using the Heater Control Unit. Position the unit near the cryostat and terminate to the Heater connector. By setting "setpoint 1" on each channel to 25 deg C and "enabling" each channel 300W input is provided to the MOB and 150W to the Radiation Shield
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1.3   When the coldest temperature anywhere inside the cryostat is above 120K the cryostat can be backfilled. First, however, the bolts securing the two main Vacuum covers should be loosened to slightly more than finger tight. If not these bolts will be virtually impossible to undo when the vacuum is removed. Backfill the cryostat with clean, dry nitrogen. For the volume to be filled this can take over 30 mins and is only terminated when the pop-off plate on the motor connector plate has operated. (i.e. DO NOT RELY ON VACUUM GAUGE MONITOR!)

.   Ensure that you have an adequate supply of gas before starting - remember that the volume of the cryostat is ~2 cubic metres.

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1.4   With backfilling complete and the detector temperature above 120K, set the LS330 controlled heater to the 'Medium' setting.
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When all temperatures have reached approximately 290 K (15 deg C) the warm-up heaters can be switched off and the cryostat prepared for opening. Log the timing to update the Instrument cooldown log
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Recharge or purge teh Helium system as required to 150 psi.

 

2   Cooldown Record

  The following table records the dates when the main Michelle optical bench was cooled to <100K.

 
Cooldown Warmup Period Cold [weeks] Notes
24/8/98 30/8/98

1.0

Mechanism tests. No filters or detector installed.
28/9/98 12/10/98 2.0 Mechanism tests. No filters or detector installed.
12/11/98 21/11/98 1.5 Detector and filter wheels fitted for this cooldown
11/12/98 5/2/99 8.0 System testing with warm (but operable) detector and grating drum stuck at LOW_N
22/3/99 24/3/99 0.3 Grating drum jammed
21/4/99 5/5/99 2.0 Detector electronics fault
8/9/99 8/10/99 4.5 Grating drum jammed
1/1/00 24/3/00 11.5 System tests. High background - Excessive flexure - Grating Drum Operates Erratically.
14/6/00 18/8/00 9.2 Imager Only
18/10/00 20/1/01 13.5 New Grating drum
9/3/01 23/3/01 2.0 Gemini Fore-optics fitted - blockage in Spectrometer path
6/4/01 16/5/01 6.0 Acceptance Cooldown
       
    56.5 TOTAL PERIOD COLD WITH DETECTOR FITTED