Calibrations
9:30: start of operations
HEXA |
-2.03 |
-7.25 |
4.47 |
-31.74 |
187 |
0 |
We have a problem with
BCU: when we change subapertures the HVC goes to limit. We stop the update to HVC before configuring:
slopeComputer.disableHVCUpdate()
We open the jitter & pupil loops, we take snapshots to check swing arm vibrations:
TN |
Notes |
Res |
20141104_173522 |
" |
179 |
20141104_174007 |
JCL |
139 |
20141104_173448 |
swing arm vibrations check, JOL |
179 |
10:30: we restore the 10modes recontructor for the blue pupil. Loop frequency = 320Hz. Offload to Hexapod is disabled. Modes 2-10, gain= 0.3.
Then we increase the loop frequency to 1kHz, gain >0.28 oscillates. JCL + correcting TT on LGSW are conflicting.
PI |
X |
Y |
Blue |
-0.72 |
-2.21 |
Yellow |
-4.12 |
0.25 |
Red |
2.60 |
-4.47 |
Setting the PI offset to a static value seems to increase the loop stability. We rise the mode number up to 10 and gain= 0.2.
Problem with offload...
We generate a new rec from the 300Hz IM:
REC: 10modes_ryb_300Hz and we close the loop with gain= 0.3.
TN |
Notes |
Res |
20141104_184331 |
g(2-10)=0.3, POL |
295 |
20141104_184527 |
bad, pupil loop was converging |
366 |
20141104_184557 |
PCL |
365 |
20141104_184812 |
g(TT+10modes)=0.3 |
530 |
20141104_185107 |
g(2-10)=0.3, JCL |
563 |
We record a new IM with the 10modes loop closed at low gain (0.05).
IM: 20141104_181359 shift=2
REC: 50modes_ryb_300Hz
we close the loop with 50modes and a gain up to 0.65. It works, so we load also a disturb equivalent to
0.8" (oversampling=300Hz, wind = 5m/s).
TN |
Notes |
Res |
20141104_193819 |
OL |
480 |
20141104_193906 |
OL |
479 |
20141104_194000 |
OL |
480 |
20141104_194215 |
g=0.1 |
82 |
20141104_194340 |
g=0.3 |
54 |
20141104_194601 |
g=0.7 |
97 |
12:50: new REC, just yellow pupil
REC: 50modes_y_300Hz
We record an IM at 150modes closing the loop on 50 with the old rec (ryb).
IM: 20141104_195640 wrong, the shell was not flattened...
IM: 20141104_195926 OK
REC: 150modes_y_300Hz
TN |
Notes |
Res |
20141104_201015 |
Y, g(0-50)=0.6, g(50-150)=0.3 |
138 |
20141104_201306 |
Y, g(0-50)=0.65, g(50-150)=0.6 |
176 |
Now we set the loop frequency to 1kHz, diodes current to 0.2A (equivalent to 4000 ADU/subap), we load disturb equivalent to
0.8".
NB: until now we used OVS disturbance function to load the disturb, this is correct only if the WFS is running at slower speed than the disturb. In this case (WFS @ 1kHz) we should use WFS disturbance
TN |
Notes |
Res |
20141104_202230 |
Y, g(0-50)=0.3, g(50-150)=0.2 |
122 |
20141104_202309 |
Y, g(0-50)=0.5, g(50-150)=0.3 |
251 |
REC: 150modes_ryb_300Hz
13:30: stop to refill LBC
13:45: we start FLAO board
DARK: 20141104_204154
TN |
Notes |
20141104_205523 |
after rebooting arbitrator |
14:21: light is back on LGSW
PI |
X |
Y |
Blue |
-3.47 |
-0.56 |
Yellow |
-5 |
3.45 |
Red |
0.14 |
-5.76 |
TN |
Notes |
Res |
20141104_213058 |
OL |
470 |
20141104_213135 |
OL |
471 |
20141104_213340 |
OL |
471 |
20141104_213552 |
g(0-50)=0.5, g(50-150)=0.3 |
70 |
20141104_213632 |
g(0-50)=0.3, g(50-150)=0.2 |
70 |
Now we load disturb equivalent to
1.2", v=15m/s,
TN |
Notes |
Res |
20141104_214012 |
OL |
609 |
20141104_214042 |
OL |
609 |
20141104_214203 |
g(0-50)=0.3, g(50-150)=0.2 |
80 |
We remove disturb, we flatten the mirror and we acquire slope offset:
SO: 20141104_214442
TN |
Notes |
Res |
20141104_214643 |
g(0-50)=0.3, h(50-150)=0.2 |
80 |
20141104_214756 |
OL |
608 |
20141104_214942 |
g(0-50)=0.6, h(50-150)=0.4 |
83 |
20141104_215002 |
" |
80 |
20141104_215638 |
noTT, JOL, g(2-50)=0.6, h(50-150)=0.4 |
82 |
20141104_215734 |
noTT, JCL, g(2-50)=0.6, h(50-150)=0.4 |
81 |
15:00: we close the loop on FLAO, correcting 400modes. We set PIs to the following static position:
PI |
X |
Y |
Blue |
-3.87 |
1.46 |
Yellow |
-3.23 |
4.49 |
Red |
-2.57 |
-4.14 |
We focus the Z stage on FLAO: Z= 37mm
SO: 20141104_221601 optimized for CCD47 and IRTC images
TN |
Notes |
Res |
20141104_221740 |
FLAO CL |
60 |
20141104_221811 |
" |
75 |
20141104_222248 |
ARGOS CL, g(0-50)=0.6, g(50-150)=0.4 |
85 |
20141104_222316 |
" |
87 |
15:25: stop operation with
CalUnit
Pockels cells test with IS
15:30: after operations on the first half of the day we perform a
PockelsCellsTransmission test using the Internal Sources. The system configuration is the following:
TN |
Sup |
'20141104_223443', '20141104_223759' |
B=75, Y=113, R=95 |