[Sheila, Kiwamu]
Looking at the ITMX camera, Sheila found a good alignment of PR3 which centers the beam on ITMX. The below is the slider settings:
PR3 (to get the beam centered on ITMX)
It seems that this alignment also kind of centers the beam on ITMY without touching BS. Indeed the biases look similar to what Keita had when he got it centered on ITMY (see alog 8978). However, with this alignment, we were unable to get the PRX fringes even with ITMX steered. To study what is happening, I looked at the PR3 camera which is an analog camera (see alog 8937) attached on the MC spool. Then I realized that the ITMX return beam was hitting the swiss cheese baffle. This was the beam propagating from PR2 to PRM. I tried to steer it with ITMX, but the actuation range was not big enough and also the spot tended to disappear as I steered ITMX. So instead, I steered PR3 to let the beam hit the PRM.
As a result, currently multiple bounces is happening in the PRX cavity. A clear beam spot is visible on the BS baffle of its HR side and the spot is sensitive to both PRM and ITMX, indicating that this is a multiple-bounces beam. Note that I didn't change the ITMX biases so that both pitch and yaw sliders are zero. Apparently the horizontal alignment is not good because I can see the beam is slightly hitting the BS baffle on its right side. I am guessing that we need to re-tweak PR2 horizontally to clear BS.
PR3 (to get multiple bounces in the PRX cavity)
Blue bolts bad - see picture. Swap these out if there is an opertunity.
I reworked the IO_AB_* path on the PSL. This incuded a small change to the layout to accomodate a 2" mirror mount. The beam is routed to IO AB_PD2, and the PD is powered. IO_AB_PD3 is not yet on the table. IO_AB_PD1 is on the table but not hooked up.
Moved one inch away from the periscope foot:
IO_AB_M8
IO_AB_BS2
IO_AB_M9 - also moved one inch toward the center of the table to keep the path length from the lens 15"
IO_AB_PD - also moved one inch toward the center of the table
IO_AB_M10
IO_AB_CCD1 - not yet on the table
Need for DC PDs:
- power cable for IO_AB_PD3
- BNC cable for IO_AB_PD3
- connection to DAC for PD2 and PD3
Need for camera:
- camera - didn't find a WATEC
- power cable
- BNC
Other to do:
- swap optic from manual rotation stage to powered rotation stage for IO_MB_HWP2
- install and test the rotation stage in the main beam
What has been done so far :
- Filters were installed in the lockin demodulator and were tuned for a 10Hz signal excitation.
*9:11Hz bandpass for the optical lever signal
*1Hz ellip low pass and 20Hz notch for the demodulated I and Q signals
- Lock2Osem matrix filled to excite the pringle mode of the second mass from the pitch oscillator (UL, LR = 1 LL, UR=-1)
- Sent a 10Hz, 50000cts signal from the oscillator, to excite the pringle mode of M2, but I couldn't see the demod Q and I changing when modifying the coil gains, so I quit after few iterations
- M2 length to M3 Pitch transfer functions, without coil balancing. It matches the model below 2Hz, cf attachement. The signal/noise ratio of the tf is too low above that. I had to divide the model supposed to be in rad/N.m by 100 to match with the op lev TF, and I'm not sure where this factor comes from. The red curve is a fit of the modeled tf, and the cyan is the inverted tf.
What I intented to do this evening is to install this inverted filter in the L2P M2 drivealign matrix, take a new L2P TF and compare it with the previous one, to see the improvement., but didn't have time to finish.
If anyone wants to take over :
Script live in /SusSVN/trunk/BSFM/H1/BS/Common/Scripts/L2Pdecouplingfiltersdesign.m
TF data is in /ligo/svncommon/SusSVN/sus/trunk/BSFM/H1/BS/SAGM3/Data
Hugh, Mitch, Jim
After TMS removed their lower half this morning, SEI went to EY to remove our mass stacks from the optical table. Relatively painless, we were done by 3pm. Our parts are currently stored in foil the AOS cleanroom over the gate valve. NEXT!
Today, Travis and rerouted the SUS testing cables from the SRM satellite boxes to the SR2 satellite boxes and cleaned up all the riff raff cabling left over from OMC work in the area. We labeled the cables and the SR2 sat boxes. Note, currently SRM is still plugged into the table end of the cables so we need to just move them the the SR2 suspension on the table. I also moved the SR2 optic (in a special holder) to the table so be aware.
Next up: Level and suspend the SR2 all metal sus and pull back all of the OSEMs in order to take open light gain/offsets.
900 Corey doing TMS work at both EX and EY
1000 RCG upgrades begin
1020-1600 Cheryl working in PSL enclosure
1040 Fil and Aaron doing cable survey at ISCH1TL
1120 Townsend onsite
1140 Jim/Cyrus working MX
1240 Praxair delivery
Today, TMS removed the lower TMS structure.
SEI shuffled weights and cleared the table of the H2 weights.
SUS located the ETMy SUS cookie cutters and assisted in the hunt for the BSC10 TMSy cookie cutter. We'll plan to reposition the SUS QUAD upper structure on the table tomorrow unless the TMS cookie cutter pops up and TMS wants to press on.
Aha - Travis found the TMS cookie cutters.
After the rcg update and front end restart, hepi, isi and suspension systems have been restored back to their automatically generated snap from 8:00 am this morning.
I used the following commands :
for optic in mc1 mc2 mc3 prm pr2 pr3 itmx itmy bs im htts etmx etmy srm tmsx
do
burtrestore h1sus${optic}epics 08:00
done
for isi in ham2 ham3 bs itmy
do
burtrestore h1isi${isi}epics 08:00
done
for hpi in ham2 ham3 bs itmy
do
burtrestore h1hpi${hpi}epics 08:00
done
I noticed that we no longer had a retro-reflected green beam even though we were aligned onto the QPDs. TMSX was as follows: PIT: -103, YAW: -297. In order to get the retro-reflected beam back, I had to move TMSX to: PIT: 13. YAW: -323. I am not sure what would have caused the offset to drift so much. I have turned the clean room fans back ON to see if this caused a drift in anything.
Jim, Cyrus, Dan and Dave
We recompiled all front end models against RCG tag-2.8.2 with the execption of h1susim and h1sushtts which were left back at tag-2.8 (current models do not compile).
We first upgraded h1seib1 and h1asc0 because slow data errors were easily evident in the h1hpiitmy and h1ascimc models (due to EzCa and Phase parts respectively). These systems slow data was found to be correct, so we went ahead and restarted all user models and restarted the DAQ. The h1pemmx system did not restart, even after many attempts. Jim went to MX and power cycled h1pemmx and its chassis, it then restarted correctly but the return timing signal to the MSR master continues to have problems (started 22Nov2013).
Cyrus and Jim revisited MX and found that the return single mode timing line was loose at the IO Chassis timing slave SFP. The fiber was reseated and the return timing diagnostic signal is now good at the MSR master.
We added two new EDCU ini files into the DAQ: H1EDCU_GRD.ini and H1EDCU_PSLCENTROID.ini (Guardian and PSL image centroid channels). I also updated the H1EDCU_ECATX1PLC2.ini file against the latest Beckhoff file.
We reconfigured h1nds0 to serve commissioning frames (it was serving science frames as a check of this frame type). This gives the users full look back over the past weekend when h1fw1 was down due to disk issues.
Dan upgraded the h1ldasgw0 QFS file server. h1fw0 was down for about an hour.
We timed the recover time of the PSL when the h1psl0 models were stopped and restarted. We recovered the reference cavity in a record 2 minutes. Opening the diode room shutter via MEDM posed no problems today.
Attached are plots of dust counts at end Y requested from Dec. 13 20:00 - Dec. 16 20:00 UTC.
We finished welding ETMY on Friday evening. It was hanging with about 5 or 6 mrad of differential pitch wrt the PUM. It was left hanging over the weekend. When we looked at it this morning, two fibres had broken and the other two were lying against one of the earthquake stop rails. All the horns and stock were still intact. We scribed off the stock from all 8 horns and filed them back to 6mm above the ears. Work is ongoing to clean up the remains of the two shattered fibres and to pull enough fibres to allow welding again first thing in the New Year. Angus, Travis & Betsy
After cleaning, we stowed the lower sections of the QUAD in the welding cleanroom and covered them with C3 covers. 2 Genie lifts are now at EY for the TMS and SUS cartridge rearrangement. SEI and TMS are free to go start their work.
I would like Karen to do a floor cleaning of the test stand cleanroom as the floors are quite dirty. Also, the Genie that is not yet in the cleanroom needs a wipe down.
Note, I hand wiped the floor in the welding cleanroom and while I found dirt and some small metal particulate (from assembly of the cages around the suspension during welding), we did not find any "dead ringers" such as bugs or large objects which may have caused the fiber break.
I also carefully turned the C3 cover inside out and inspected for stray seams, fibers, particulate, etc. Other than bits of broken fibers, the cover was quite clean and secure looking.
[Arnaud, Kiwamu, Keita]
After HEPI work earlier, BS was restored using oplev.
POP beam yet to be found. PRY alignmnent was restored, PRY was locked, but couldn't see anything on MC tube baffle. Thinking that the beam is already clearing the baffle hole, we went to ISCT1 but couldn't find the beam (actually there was some beam but it didn't move when we misalign ITMY). We might have to go 10W before we can find anything.
PRY alignment is dubious. When PRY locks, the beam look low on BS AND ITMY. When we set the beam height on ITMY using ITMY video image, BS beam position came up and looked OK-ish (maybe still low). However, with this new alignment, we couldn't steer ITMY enough to re-establish the PRY cavity as F3 BOSEM output railed.
PRX scanning efforts. With PRY path aligned (to dubious alignment) and then ITMY misaligned, we scanned ITMX to see if we can see PRX cavity flash, but we weren't successful. We will set PR3 angle such that the beam hits the center of ITMY and scan ITMX tonight.
ITMX oplev is dubious. When we scanned ITMX, OSEMs (M0, L1 and L2) responded nicely but we got nothing from oplev.
ITMX camera should be zoomed out if possible. We cannot see any beam on the ITMX camera, but it's mostly looking at ITMX face.
Dubious PRY alignment:
PR3 | BS | ITMY | |
PIT slider [urad] | -96.9 | -159 | 253 |
YAW slider [urad] | 89.5 | -13 | -284 |
When the beam hight is OK-ish on ITMY:
PR3 | |
PIT | -715 |
YAW | 1079 |
We left ITMX scanned overnight last night with a hope that it finds a PRX fringe. However, there was no sign of fringing in ASC_POP_A_SUM or REFALIR_A_LF. See the attached plots. Note that the PR3 alignment was left such that the beam was centered on ITMY as Keita mentioned in his alog.
KiwamuI, ThomasV We aligned ITMX and ITMY optical levers to the position of the test masses at approximately 2013-12-16 12:00 PT. We may need to adjust the alignment if the pointing changes due to commissioning activities.
Also, we centered the PR3 opleve in this past Friday. Sorry for not alogging.
ITMX was reflecting off the compensation plate in the previous ALOG, we had shifted the alignment when trying to put the enclosure back on so we re-aligned receive the first bounce off the HR surface of the test mass. This is verified by actuating on the main chain and the reaction chain separately and verifying that the beam spot correlates to the main chain.
After an initial assessment that stated "not too bad, not too good" (https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=8919), which was based on just two data points (beam radius on WFSs), I added the third point further downstream of the WFS2 and it turns out that actually it's excellent.
In the attached plot, blue circles represent the measured beam width, blue crosses on both sides of blue circle represent the potential position error (Jamie claims +-1cm though probably it's too generous), red line is a fit over the three points, green is the curve generated by the design parameters.
As you can see, in both horizontal and vertical direction, the waist is very close to the middle of the WFSs, and the waist radius is very close to the designed 250um. Gouy separation for X (horizontal) and Y (vertical) are 82.6 and 87.1 degrees, respectively.
This was obtained from just two iterations of measurming at WFS1 and WFS2 and pushing RM2 toward RM1 based on the measurement. Downstream was measured just once after we were satisfied with WFS1 and WFS2.
relative position (mm) | position error (mm) | X diameter mean (um) | X diameter std | X goodness of fit | X goodness of fit std | Y diameter mean | Y diameter std | Y goodness of fit mean | Y goodness of fit std | |
WFS1 | 0 | +-10 | 746.79 | 4.6 | 0.01 | 0.000 | 688.9 | 4.2 | 0.00 | 0.000 |
WFS2 | 369 | +-10 | 746.25 | 10.1 | 0.00 | 0.000 | 758.18 | 4.4 | 0.00 | 0.000 |
downstream | 763.2 | +-10 | 1574.92 | 4.95 | 0.02 | 0.000 | 1666.38 | 1.79 | 0.01 | 0.000 |
Distance from RM3 to the first lens on the sled is, according to Jamie, between 48.0 and 48.25 inches.
Also, as noted earlier, the above data was obtained after having moved RM2 toward RM1 by 22.5mm. Everything else is the same as what Sheila reported much earlier.
We also measured at one point between RM3 and the sled (14.5" downstream of RM3). Together with upstream number measured yesterday (https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=8893), these are:
position | position error | X diameter (um) | X std | X goodness of fit mean | X goodness of fit std | Y diameter | Y std | Y goodness of fit | Y goodness of fit std | |
After RM3 | 14.5" downstream of RM3 | +-10mm | 3750.18 | 4.885 | 0.01 | 0.000 | 3923.63 | 2.137 | 0.00 | 0.000 |
Upstream of telescope | 44.7" downstream of 50:50BS right after the HWP | +-1" | 3851.01 | 1.982 | 0.01 | 0.000 | 3959.23 | 1.232 | 0.01 | 0.000 |
Upstream of telescope, head rotated 45 degrees | same as above | same as above | 4117.74 | 1.475 | 0.02 | 0.000 | 3845.62 | 0.763 | 0.00 | 0.000 |
In all of the above measurements, "Profile averages" was 10, "Rolling profile Averages" was 3, the actual number of measuremets (i.e. the number of scans performed before I stopped the measurement) were larger than 10 but I don't know if the software was taking more than 10 points into the statistics or not.
Several things to note.
We decided that we did NOT want to propagate the upstream measurements to downstream, because it was difficult to obtain more than one data points. (ModeMaster is supposed to overcome this, but in reality there are many caveats and you should know how to tell when which caveat applies.)
With NanoScan and limiting ourselves to the measurements with small beam, it was still difficult to obtain good data because of some kind of glitches. It's not clear if it was due to NanoScan or the beam, the beam was well damped and was not moving on the viewer card, there was no noticable intensity glitch either. But the symptom was that the statistics window shows nice steady data for anywhere from one second to 30 seconds, then there's some kind of glitch and the scan/fit image looked noticably different (not necessarily ugly), the diameter mean becomes larger and the stddev jumps to a big number (like 10% or more of the mean, VS up to a couple % when it's behaving nice), and the goodness of fit also becomes large. Somehow no glitch made the beam diameter number smaller. I just kept waiting for a good period and cherry-picked.
When the beam was moving it was impossible to obtain good data.
Another kind of glitch was "saturating" glitch where the software says there is a saturation. We disabled AGC of NanoScan and lowered the gain by 3dB in an attempt to eliminate saturation, it seemed to help but we couldn't kill that error completely.
We (I and Jamie) will go in HAM1 tomorrow to set the eddy current damper spacing (now that Bram wrote a procedure to do that, plus it turned out that Jamie didn't check the ECD spacing on the back plates).
Measurement apparatus. We flipped one steering mirror on the sled to direct the beam to Nanoscan that is placed at the same distance from the steering mirror as the WFS. Made measurement, flipped the mirror back, and moved to the next one.
Very nice! This will become version 12 in D1000313. It would be good to add the corresponding alamode file with the final distances here: https://dcc.ligo.org/T1300960-v1, I added a note to remind us that this is the relevant log entry.
A update on 2014.Jan.12:
Alexa, Koji and I changed the position of both WFSs to dump the reflected light off of the diode (see alog 9226).
The didgital cameras that are currently focues on an image are CAM10 (on 3 o'clock position on HAM3 side of MC spool) focused on one side of the swiss cheese baffle (wth holes for MC3 and pop) and CAM11 (mounted at 9 o'clock position on same baffle) focused on the other side of the same baffle (PRM and PR3 holes
The beam which is highest on the screen of CAM11 (above the PRM baffle if the camera was straight) is from an oplev.