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Section: H1
Task: IOO
It will probably register as an IMC lockloss, just wanted to make sure people know it was caused by an injection.
Craig mentioned yesterday that we might want to walk our IMC uncontrolled degree of freedom: the spot position on MC1 and MC3. I made a short script which should step the sliders of MC1 and MC3 in the correct configuration (differential step in pit, common step in yaw). If you want to run it is in
/ligo/gitcommon/labutils/imc_walk
To step both mirrors by eg 0.1 microradians, run python walk_imc_dof_4.py P 0.1
This might not end up being used since Robert suspects much of our jitter could be caused by the multiple roughing pumps running in the LVEA.
Jennie W, Camilla,
This morning Camilla and I went into HAM1 on the +Y side and measured the beam height of the beam from the PSL above the table. This is to aid in the design for the JAC periscope.
First we measured the beam height near the septum window to HAM2. We had to use a metre stick that had been wiped down as the beam height was slightly too high for the 12 inch class-B ruler from the tool pan. This ruler had to be bent at the top as it reaches the sloping part of the edge of the chamber roof. Camilla and I took several measurements in case the bottom of the ruler was not straight up from the table.
+X (HAM2 side)
My measurements of this height are here and here - loks about 315mm above the table.
Camilla's measurements are here and here with three zoom outs so the bolt hole we lined the ruler up with and the surrounding components can be seen. Hers suggets 313 -314mm above the table.
We were both measuring in the same spot along the beam.
-X (PSL side)
My measurement on the -Y side suggests 317 mm above the table. The two following pictures are where I had the ruler in front of the balance mass.
This is another measurement with the ruler behind the balance mass but its too hard to see the numbers, I think it is still about 320 mm high here.
There are Camilla's measurements on the same side. The first looks like 317mm above the table, 311mm above the table. The third image shows Camilla had the ruler behind the balance mass (so in a different place from my first -X measurement).
Tagging EPO for photos.
[Betsy, Keita, Camilla, Richard M., Elenna]
After the power outage, we wanted to get some confirmation of PZT pointing out of the PSL. Betsy, Keita and Camilla went in the cleanroom with the IR viewer and indicator cards and took the covers off the IMC refl and trans viewports on HAM2. Keita found the beam out of the IMC REFL viewport, and I adjusted the IMC PZT in pitch and yaw under direction from Keita. I accidentally moved the pitch slider a bit at the beginning due to user error. Then, we took large steps of 1000 or 2000 counts to move the offsets in pitch and yaw.
Start values: pitch: 22721, yaw: 5488
End values: pitch: 21192, yaw: 6488
Then, Betsy found the beam out of the IMC TRANS viewport and Richard marked the beam spot approximately on the outside of the cleanroom curtain with a red sharpie. This is super rough but gives us a general location of the beam. We think this is a good enough pointing recovery to proceed with vent activities.
During this work, PSL waveplate rotetor was set to 200mW and then de-energized. I haven't re-energized as we don't need higher power for a long time.
PSL laser pipe was temporarily opened for this task and was closed after.
Attached video shows the flashing of the beam in MC TRANS path. The alignment from the PSL through the IMC is not crazy. Any further refinement should be done after we start pumping down the corner before we install HAM1 optics.
Accepting PZT offsets in h1ascimc SAFE.snap table.
Jennie Siva Keita Mayank
Following our previous attempt here . We opened a new ISS PD array (S.N. 1202965).
This unit is in great condition. i.e.
1) No sign of contamination.
2) All the optics are intact (No chipping)
We tried interfacing the QPD-cable S1203257 with the QPD but it turned out that they are not compatible.
We will look for the updated version of the QPD cable.
More photos I took of the unboxed unit,
Keita holding part of QPD connector that connects to cable,
zoom in of part of prisms close to PD array to show they don't look damaged like the previous one we unboxed,
dcc and serial number of baseplate (this is different part for each observatory due to differing beam heights).
Keita explaining the QPD cable clamp to Shiva (right) and Mayank (left).
View of optics with periscope upper mirror on the left.
View of part of prisms close to periscope.
View of back of array and strain relief.
plus a picture of an packaged coptic that was sitting on top of this capsule while it was in the storage cupboard.
For future reference all the ISS arrays and there serial numbers are listed in the dcc entry for the assembly drawing LIGO-D1101059-v5.
[Matthew Mayank Siva Keita]
On Friday (2025-02-28) we moved the optics onto taller posts so that we did not have to pitch the beam up to much (in hind-sight, we probably would've been okay doing this) when we align the beam into the input port of the ISS array. We have not aligned the beam yet and most likely should re-profile it(may not need to) to ensure that the planned lens position is correct.
We also spent some time checking the electronics box for proper connections and polarity; then we tested the upper row of PDs (4 top ones) by plugging in each cathode/anode to the respective port. The output DSUB we used a breakout board and threw each channel onto an oscilloscope -- it seems that all four of the top row of PDs are functioning as anticipated.
Important Note:
Keita and I looked at the "blue glass" plates that serve as beam dumps, but just looking at the ISS array we do not know how to mount them properly. We think there may be some component missing that clamps them to the array. So we repackaged the blue-glass in its excessive lens paper.
Jennie W, Rick S, Mayank C, Keita K
We went into the optics lab today with the intent for Rick to review the ISS array assembly we unboxed the other day (LHO alog #82731) on which we found some particulate contaminsation and some detached parts.. Rick and Keita are unsure how the support rods (first picture) were bent during transit and they appear to have bent at the top and deformed the cover piece (D1300717) they were attached to as they came unfixed at the other end and so were just resting on the top of the QPD mount plate (D1300719). They appear to have moved around and scored the surface of this platform. Maybe this happened in transit or storage but it seems like it would have had to be a large force and Rick says the storage containers were packed in form during transit.
1st package: Base piece (D1101074-v2 S/N 004) is double-bagged in my office and I have put in a clean and bake order as this spacer is site specific in height and some of our ISS spares will have a spacer set to the L1 beam height instead so we may need to swap it out.
2nd package: Cover piece D1300717 with the spacing posts attached is not bagged properly as we probably do not want to reuse this and so it is in Keita's office.
3rd package: Array and mirror assembly with PDs still attached was wrapped in foil with dry sealed clean room wipes protecting top optic in periscope, then double-bagged. Shown in center left of this image. This will need re-cleaned if we want ot scavenge parts form it.
4th package: All the other parts from assembl y shown in this image ( apart from PD assembly, baseplate, tool pan and top cover) have been packaged up in foil and double bagged in one package. These will also need recleaned if reused.
These last two packages are stored in the cabinet that the spare ISS array units are in, situated in the vacuum bake prep area next to the PCal lab. The shipping cover and base plate for the array are also back in this cupboard.
For reference the assembly drawing can be found here.
The assembly we worked on has the dcc ref S12020967
I don't have access to the entries for serial numbers but the ISS array assembly dcc entry is here. https://dcc.ligo.org/LIGO-D1101059
To rebuild the spare ISS PD Array unit (D1101059 S1202967, note that I myself don't have an access right for the S-number document on DCC) and align the PDs, we opened the transport container (D1400368) in the optics lab.
We initially had a hard time to open the container as the viton gasket (D1400366) was REALLY firmly stuck to the container lid (D1400367) and the container base (D1400365). We put the container on top of small stainless steel cart and used screwdrivers to pry the cover off from the base plate. Even after two corners were freed, we could not lift the lid just by hand, and we had to continue prying the lid until all four corners were freed.
Contamination:
After finally removing the lid, we found two bases for concern, the first is the contamination.
The first two pictures shows the container assembly before and after removing the lid.
Note that the second picture shows the class A "cover" for the assembly tilted back. It turns that the cover was just put there, free to rattle. Connection rods that are supposed to attach the cover to the cage structure were not bolted to the cage.
The third picture shows how filthy the container base plate was. It also shows a half of QPD retainer parts that were found there, next to a swagelock fitting attached to the base plate.
Fourth picture shows the pre-soaked wipe I used to lightly clean the top surface of the PD array base plate. I immediately picked up some black stuff. You can also see that the PEEK parts are covered with black stuff.
Fifth picture shows the PEEK parts. I wiped the top parts but the bottom one is yet to be cleaned. You can easily see the difference.
6th and 7th picture shows deep scuff on the class A surface of the array PD structure, which seemed to have most accumulated the black stuff.
Glass chipping
We also found what seemed like tiny pieces of glass on the container base plate as well as the ISS PD base plate.
We inspected plate optics and found that all of them have chips. The worst one is one of the high reflectors.
The first three pictures show the damage of the leftmost HR optic seen from the beam entry point (i.e. array PDs are facing you). There appears to be a big chip where the adjustment cam is supposed to touch, but the cam was found detatched from the assembly and was on the transport container base plate.
The fourth picture shows the chip at the corner of the middle optic (BS). It also highlights that what seems to be the deep scuff marks or maybe grinding marks from the manufacturing process on the high reflector to the left (which is a different optics from the first three pictures as you're looking at the assembly from the array PD position so to speak) seem to have accumulated black stuff. That optic also has bad chipping on the front edge, which is more clear on the fifth picture.
The 6th picture shows one of the bigger glass pieces found on the surface of the transport container base plate. Note the black smudge on the glass (if it is glass).
I've used the pico to center IM4 trans QPD. See alogs about this history: 80604 78962 78943 78856
After difficulty with input alignment shifts in the spring, we centered IM4 with the hopes that we could use that as a reference for any future input alignment shifts to reset the IMs. However this didn't work well when the PMC was swapped. Now we are recentering IM4 trans to get this new reference since we've been operating here for a while.
Had about 20hrs with no IMC/FSS glitches from 9pm Thurs night until about 340pmPT Fri afternoon. But have now had several for the last 5hrs.
Also for one ~60min stretch, H1 almost made it to NLN, but had rung up violins which kept us at OMC Whitening for 20min until the next IMC glitch.
Here are some running notes for the rough 5hrs filled with glitches (currently have H1 in IDLE).
Notes During Return of IMC/FSS Glitch Locklosses
2340utc (340pmPT) LOCKLOSS with IMC tag was the beginning of IMC/FSS glitch locklosses (where we went almost 20hrs since the last glitch around 5utc (9pmPT).
0111-0208: OBSERVING
0208utc (608pmPT): Attached screenshot shows a coincident glitch lockloss seen on FSS & IMC. Here is the LOCKLOSS page also tagged with IMC glitch.
Starting an FRS Ticket to mark the DOWNTIME (FRS-32644) for 3.5hrs of DOWNTIME so far. Where there was notable part of downtime due to IMC not locking easily.
VIOLINS Rung Up A Bit: (haven't had this since my shift on Tues night!) So were stuck at OMC WHITENING for over 20min before H1 had....
So for the last 3hrs:
Not sure what is more useful. Keep having ISC LOCK continue to locking, or to leave it in IDLE for IMC/PMC/FSS monitoring....
I took the opportunity to center the IMC WFS this morning since we've been getting the notification on DIAG_MAIN for some time. The process was as follows:
Looking at the OFI TEC servo we noticed that the response was much slower than what one could expect from the given ugf frequency. The gain was increased fomr -1 to -15, whereas the ugf frequency was decreased from 50mHz to 10mHz. This resulted in a response time around 10s, which is about 3x faster than when we started. Increasing the ugf beyond this can make the servo unstable.
As a side note: The applied voltage at the driver was about 3x higher than the voltage readback from the TEC, indicating a rather large voltage drop in the cable.
Sheila, Betsy, Camilla
With the HAM6 +X door off we did an initial inspection of HAM6, looking for anything that could have caused the pressure spikes seen in 78346, 78432.
There was discoloration on the fast shutter, see lower half of the -X part of the "fast shutter cap" and viton piece: part (4) and (10) of D1003318. Photos attached. This was the only thing we could see out of the ordinary.
From the Feb 2024 HAM6 closeout photos in 75791, this photo shows the fast shutter and no discoloration can be seen.
We'll plan to inspect the fast shutter when closed today.
Tagging for EPO.
Looks like there is visible damage on the KTP optic of the OFI.
TBC...
Betsy, Sheila, TJ, Mitchell, Camilla
On second inspection, after TJ and Mitch removed some of the OFI shroud 79227, you can clearly see two crater holes in the KTP wedge on the input (SRM) sideG2100316 OFI doc. The output (OMC) side of the KTP wedge looked smooth. Photo and photo.
There is splatter on the Fused Silica wedge optic, holder and surrounding beam dumps facing the KTP crater holes. Photo and photo. Maybe there was more splatters on the KTP holder too.
Photos of the SRM AR surface looked fine, but it was hard to see: photo
Zoomed out photos of the OFI with shroud removed to aid with planning: here and here.
Additional photos from everyone on googledrive here.
Attached is a view looking through the OFI from the SRM side back towards HAM6. As well as the two crater spots, you can see the black dots of splatter on the FS wedge.
Tagging for EPO.
Summary: We think that the sqz beam is seeing similar loss to the IFO beam in th alignment that we were running in until Friday, but double passed. The sqz beam transmission can be restored by moving the beam, and there should be enough power in this beam to be a useful diagnostic in chamber to distinguish between OFI and SRM damage.
Camilla and Noaki have measured 1.3mW coming from HAM7 towards HAM5 with the OPO locked on the seed. SRM transmission is 32.34%, ( 72680 ) so if nothing was damaged we should have something like 0.41mW of the OPO seed beam in transmission of SRM, which we should be able to measure with a power meter.
The table in 79101 indicates that the single bounce transmission to AS_C has dropped to 64% of what it was last Thursday. Here's a table of power predictions for the sqz beam arriving in HAM6:
no damage | sqz seed beam we expect at AS_C |
no damage | 1.3mW*(1-0.3234) * 0.99^2 = 0.86mW |
single pass of damaged optic with 0.64 transmission | 1.3*(1-0.3234)*0.99*0.99 * 0.64 = 0.55mW |
double pass of damaged optic with 0.64 tramission | 1.3*(1-0.3234)*0.99*0.99 * 0.64 *0.64 = 0.35mW |
With the alignment used for observing in recent weeks Naoki and Camilla measured 0.2 mW on AS_C QPD (not well centered on AS_C, but on the diode), which is calibrated into Watts arriving in HAM6. They moved ZM4 +5 to improve the transmission of the sqz beam to 0.9mW when centered on AS_C. These numbers don't agree super well with the predictions above, but they seem to suggest that the SQZ beam sees similar damage to the main IFO beam, but double passed.
Jennie, Jenne, Sheila, Keita
While the PSL team were preparing for a PSL in cursion, I started moving MC3 based on our plan to re-align onto the ISS array and IM4 TRANS QPD after the PMC swap last week.
We tried going up in yaw, saw some increase in power on IM4 trans QPD but then the ISS second loop QPD started to become further from the centre position as did the IM4_TRANS QPD (this is well centred enough that we could see the power drop whereas the ISS QPD started quite far off centre so that the nsum is quite close to zero).
We went back to the maximum value then tried IM3 alignment is both DOFs but this did not improve things in both QPDs so we tried MC3 pitch. Sheila then noticed that we were mazking the IMC relflected spot some horrible higher order mode so we decided to stop and think.
MC1 and MC3 changed in common yaw due to the WFS as we changed the uncorntolled differential DOF (MC1 - MC3), which we did not expect, to recover our alignment we would need MC1 and MC3 to change differentially as they did after the PMC swap, in this image.
The ndscope channels I used for this alignment walking session are attached with cusors before we changed anything and after we recovered the IMC alignment to pre-maintenance.
In conclusion we have reverted the IMC alignment back to before our changes as we think some action before the in-vacuum mirrors is needed.
Plan: To revert periscope PZT and MC1 back to their positions before the PMC swap and get Jason/Ryan to move steering mirrors in the PCAL enclosure to recover the prompt reflection from the IMC as witnessed by the MC WFS behind MC1. Then we can re-align the IMC.
Jennie W, Jenne, Keita, Sheila
Summary: The input alignment was changed due to the PMC (pre-mode cleaner) swap last week. Sheila et. al. tried to recover this with IM3 moves but the IM4 TRANS QPD, our main alignment reference into the main IFO, is still off in yaw and so we will need to walk mirror or mirrors in the IMC (input mode cleaner) tomorrow to recover this.
The other option is to move something upstream in the PSL but this is harder to do as it involves moving in air steering mirrors and so is harder to reverse. This is plan B for another maintenance Tuesday.
Attached you can see how the MC mirrors changed before (first cursor) and after (second cursor) the PMC swap and Jenne tweaking the periscope mirror (first two plots in bottom row show positioning into IMC via the pitch and yaw of the upper PSL periscope mirror).
Plan: Move MC3 in yaw in order to change the output spot position in the IMC. We will do this with the ASC for the IMC running so the alignment loops for the angle of MC2 and the differential yaw between MC1 and MC3 will still run, but I will increase the gain value of these loops to its old value from December 2014 (0.25).
For future reference, the triangular cavity DOFs are discussed here: DCC LIGO-P1000135
And the MC in particular here: DCC LIGO-G1301131