S. Dwyer, P. King, J. Kissel Shiela reduced the 1064 nm laser power coming from the PSL going into the vacuum system via the PSL's rotation stage down to 108 mW (measured down stream of the PSL rotation stage, H1:IMC-PWR_IN_OUT16) to 108 mW, then Peter and I locked out the rotation stage controller. We've confirmed that requesting adjusting rotation stage angle does not change the power after locking out the controller. It's currently laser SAFE (the PSL light pipe has been shuttered as normal), but in case we need the PSL light for alignment later, I figured we'd get the procedural stuff done before we need it. Due to IMC particulate concerns, we wish not to have higher than ~100 mW in-chamber while in air, so as to not burn stuff into a flashing IMC (see M1300464).
J. Kissel I gathered a dust count reading before doors were removed this morning. Counts are zero and zero!
J. Kissel, J. Warner In prep for today's vent, Jim and I locked HAM5 HEPI. Displacements between locked and unlocked are on the order of ~20-30 um, and 5-10 urad from nominal floating position with IPS-only, "position" loops closed. See attached screenshots, but I recap pertinent info below. dX -2.3 um dY +17.6 um dZ +23.7 um dRX +1.2 urad dRY +4.1 urad dRZ -8.7 urad I also attach pictures of the locking bolts / set screws. To lock HEPI (while attempting to preserve alignment): - Procure a CDS laptop, and open MEDM to get the DC BIAS screen of the given HEPI you want to lock - Take a screen cap of the screen before you get started. - Run all set screws and bolts into such that they're barely contacting the floating cube in each / every corner. - Using the appropriate allen wrenches (you'll need two sizes, 3/16" and 1/4"), and while watching the attached displacement screen, gently nudge the bolts further into contact until tool tight, rotating between bolts / set screws so as to not crank on any one bolt more than the others for a given tightening iteration. It's fine to do this sequentially around the corners. - Displacements from nominal on the order of a few 10s of um / urad are the precision you'll be able to lock the position. - Take another screenshot of the position and displacement once done and record. This process takes about 20-30 minutes.
Minute trend plot of PT246B for the last 12 hours attached per Gerardo's request.
Gerardo, Mark D. Tyler, Chandra
Corner
EY
We will start roughing down EY tomorrow.
Checked on CP4 at MY.
We have an aux cart running at Y-End right next to the BRS, it will be there until pressure at the BSC10 annulus system is kept at nominal by its ion pump.
Prior to corner station vent, high voltage has been turned off (as per items mentioned in M1300464). - ESD driver - Fast shutter de-energized - OMC's PZT actuator drive - Picomotors ITM Ring heater's measured power is zero (power is off at chassis), and I've changed the requested power to zero via MEDM.
The net pump speed of this diaphragm backing pump is "much" less than what we are used to. I used this portable pump station for the first time the other day to evacuate 4 lengths of 1.5" flex line + the volume between IP6's closed GV and the zero-length reducer and it took "minutes" not seconds.
J. Kissel I've taken standard close-out transfer functions for H1 SUS TMSY. It's free and clear of rubbing, and results looking strikingly similar to before. OK for pump down! Raw data is committed here: /ligo/svncommon/SusSVN/sus/trunk/TMTS/H1/TMSY/SAGM1/Data 2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_L_0p01to50Hz.xml 2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_P_0p01to50Hz.xml 2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_R_0p01to50Hz.xml 2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_T_0p01to50Hz.xml 2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_V_0p01to50Hz.xml 2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_Y_0p01to50Hz.xml
The DMT test box, h1dmt3, was patched and rebooted today at about 2 pm PDT. This should have no impact on the control room.
TITLE: 04/04 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
LOG:
14:39 (7:39) Tyler, Mark to EY
15:00 (8:00) Start of shift
15:15 (8:15) Bartlett to EX -- reset dust monitor #2
15:39 (8:39) Bartlett leaving EX
15:59 (8:59) Chris to EY -- delivering bolt
16:05 (9:05) Tyler, Mark back from EY
16:14 (9:14) Peter and Fil transitioning to laser safe
16:31 (9:31) Gerardo to EY -- vacuum work
18:14 (11:14) TVo, Sebastien, Dan, Alexei to LVEA
18:39 (11:39) Gerardo back from EY
19:02 (12:02) Gerardo to LVEA
19:29 (12:29) Fil to ISCT6 -- collect GIGE cameras
19:57 (12:57) TVo, Sebastien, Dan, Alexei out of LVEA
20:19 (13:19) TJ to HAM5 -- cleaning up
20:39 (13:39) Chandra, Tyler to LVEA -- craning work
20:43 (13:43) Gerardo to IP5
20:46 (13:46) Betsy to LVEA -- find something for Livingston
20:48 (13:48) Elizabeth to LVEA
21:02 (14:02) Jason to PSL enclosure -- grab materials
21:03 (14:03) Betsy out of LVEA
21:20 (14:20) TJ out from HAM5
21:29 (14:29) Jason out of PSL enclosure
21:37 (14:37) Elizabeth out of LVEA
22:01 (15:01) Betsy to LVEA -- investigate HAM5 HEPI
22:26 (15:26) Tyler out of LVEA
22:38 (15:38) Mark out of LVEA -- finished moving forklift
23:00 (16:00) End of shift
I spend most of the day taking transfer functions of the ETMY main and reaction chains intermittant with my other crazy business. Kissel took over after I exported all of the data but got a flag during the matlab processing of it and had wandered off with my patience.
Things look good with the plots now (as hinted via the quick looks at closeout yesterday), see attached.
Kissel has committed the new data to the SVN repository. Data can be found at the usual Data or Results directories at
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMY/SAG*/
FAMIS 6569
Added 70 mL to crystal chiller.
FAMIS 6944
Reported ETMX frequency noise as being high.
Started venting vertex this morning and spun up turbos on XBM and YBM. Looks like IP1 isn't going to make it - its isolation GV is probably leaking. The new GV on IP4 is sealing great!
Turned IP1 off.
another one bites the dust. i hear there's room in the dumpster...
There are very few more satisfying feelings.
We're replaced a 1" pico high reflector and a black glass behind with non-pico version in OMCR path. PSL beam was not available so no alignment.
We removed the following components from HAM6 (refer to D1000342):
We found that the black glass dump had some fogging on one of the two panels. Photos to follow.
Yesterday Terry, Nutsinee and I also prepared for tomorow's in chamber work by settings the apertures in their original places on the squeezer path, and aligning the beam produced by scanning the OPO through the apertures. We then moved the apertures out of the way.
1st attachment shows before the change. Green is uninstalled, red is replaced.
2nd is after.
3rd, 4th. Fogging apparent for left panel of the black glass V dump. The difference between these two is that I'm illuminating different part of the panel using a green flashlight.
5th. Right panel under the similar lighting. The fogging is much less severe.
6th, 7th. Outer side of the left panel also has fogging.
Note that I was able to wipe this off easily using a dry Vectra Alpha wipe, it didn't need any force, just wipe and it's off. I only wiped off the left 1/4 of the inside of the left panel that looks foggy in picture 4.
The dump is on the flow bench in the cleaning area next to optics lab in OSB, if somebody wants to inspect.
Between yesterday and today, Gerardo and I successfully bonded the ears to core optic mass ETM15, destined for LLO for post-O1 eventual replacement.
Ear s/n 195 bonded to S3 flat of mass June 29, 2016
Ear s/n 196 bonded to S4 flat of mass June 30, 2016
The first ear (s/n 195) has a series of bubbles along it's edge, but the surface area of these do not add up to more than the allowed amount as per E1000277, so it passes, see pix attached.
The second ear (s/n 196) has no bubbles and is nice full bond.
Inspection of the bonds this morning showed no change to the nice S4/Ear surface bond.
The small edge bubbles along the S3 Ear have migrated a bit (not worse, just moved a bit). Therefore, we decided to rewet the edge with solution to see if it would wick in and close some of the bubbles. This worked to close one of the larger bubbles, but one bubble continued to morph so we'll reinspect Monday. Note, none of the sizes of the bubbles got bigger, so the surface area of the bubble total remains the same and below spec.
Attached is a picture of what the bubbles in the ETM15 S3 Ear bond look like today (recall, it was bonded last Wed so it has now been over 5 days since initial bond). Apparently over the weekend, the bubbles ran inbound a bit further. I estimate the surface are of the bubbles to be near 20mm sq., still under the 50mm sq. spec. E1000278, although it isn't pretty. I measured the longest streaks to be almost 3mm long, with a width of 0.4mm. There are no bubbles inward from the edge near the center - anything shown in the picture is a camera reflection.
The S4 Ear bond looks unchanged from inspection last week, very good bond, very little bubbles.
Pictures of this ear bond taken by Danny at LLO just before use at LLO, indicate that the bubbles have not changed shape or size since the picture attached July 2016. Phew, said both Gerardo and I.