TITLE: 03/23 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
Wind: 12mph Gusts, 9mph 5min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.27 μm/s
QUICK SUMMARY:
13:10 Peter is in the PSL continuing 70W alignment to the PMC
14:12 Chris is removing scaffolding from the optics lab to store at MX
Terry, Sheila, Arijit, TJ,
Today we made one more attempt to get the beam from the OPO aligned into HAM5 and out to HAM6, but we haven't found the beam.
Keita loaned us a Nikon D7100 which was much better for getting a clear picture of what we were looking at than the viewer we were using yesterday. Photos will be attached to this alog latter.
FIl also cabled the HAM5 illuminator up to the new beckhoff controls, so we could turn that on and off.
We started out by manually aligning the beam again through the apertures, doing a little bit more careful job this time by using the viewer to identify the edges of teh aperature and center the beam half way. We can still see the beam hitting ZM2 through the HAM5 viewport. We were also able to sometimes see the beam coming out the HAM5 viewport (perhaps going under the fly-offf mirror on the OFI), but latter this afternoon we weren't able to repeat that. We were never able to see a beam in HAM6.
We are leaving the OPO locked and generating a beam (we again have two soft door covers with a small gap to let the beam out). We have ZM1+ZM2 scanning with an amplitude of 10,000 counts for both pitch and yaw, and SRM scanning 1000 urad.
If this does not work, we may wait for a beam from the PSL to become available and try to see the rejected scatter from the OFI polarizer in the path towards the squeezer.
Valved out X-beam manifold turbo and spun it down, so expect vertex pressure to rise. Tomorrow I plan to hard close GV2, vent XBM volume, and start loosening bolts on 10" gate valve.
The mode matched output of the front end laser was aligned into the power amplifier. After the mechanical alignment, the power amplifier was turned on at a low diode current to check that nothing was grossly wrong. When the diode current was increased to 45 A, an output power of ~84 W was measured. The beam propagation was measured and found to be consistent with data provided by neoLASE. The measurement is partly messed up by the presence of pump light and a ghost beam from the sampling mirror. An average beam diameter of 356 microns was used for the mode matching to the high power oscillator optical path. The beam path towards the pre-modecleaner was roughly aligned. Minor problems were encountered with the fit of some parts. I hope to have the pre-modecleaner locked tomorrow. Ed / Peter
It is with a somewhat heavy heart that I cut the fibers out of the final Hanford ETM to detect the first gravitational waves ever. We removed the ETMx from the lower structure and stowed it in its cake tin. The new ETMx will be installed tomorrow in prep for a fresh weld next week.
TITLE: 03/22 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
SHIFT SUMMARY:
LOG:
13:36 Peter into PSL
14:30 M2 (aka Itchy & Scratchy) @ MY VEA
14:38 Jeff B out to EY/EX for photos, reinstall dust monitors for vent and rodent checks - contamination control
15:13 King Soft on site
16:40 Bubba out to EY - to the well
16:40 Jeff B back from Ends and heading out to LVEA
16:50 Betsy and Travis out to EX
16:55 Jeff B back
17:23 Kyle, with Apollo, arrived on site
17:24 Sheila, Arijit and Terry out to HAM6
17:33 Jeff B to ITMY for camera work
17:44 Mark out to LVEA
17:56 Marc back
18:31 Chandra out to MY
18:44 Betsy and Travis back
18:45 Peter out to PSL
18:55 Jeff B back from ITMY - LSO must be informed before transition to LASER HAZARD as the cover is OFF the viewport
20:35 Jeff B out to LVEA
21:08 Betsy and Travis back out to EX
21:45 Peter back
22:09 Jeff B back for the day
Per request, pictures attached of the cryopump bake enclosure installation. The installation took two days and several modifications were made before and after the bake commenced in an effort to create more uniform heat zones within the enclosure because the bottom is not achieving target temp. Modifications include:
Improvements for future designs:
The ISS box used to be dogged down using CL5 dog clamps, and is now dogged down with CL2 dog clamps, with CL5 dog clamps installed up side down against the base. One of the clamps installed against the base is a fork clamp, installed as the South fork clamp on the East side of the box, where the ISS box is up against the PMC box, so very difficult to access. Images attached show each side of the box, and the file names identify which clamp(s) and which side. In the images, the first clamp identified is the North clamp East side, and from there the clamps are identified in a counter clockwise direction, ending with the South clamp East side (which is shown in the last two images).
Vac - Chevron baffle work take place Monday contigent on proper valves come in tomorrow.
Sus - New acoustic mode damping device to be installed on ETMY after successful testing at LLO.
Sei - EX; H6 ISI remained locked. EY;EX;H6 HEPI remained locked. TJ reports guardian code is finished.
CDS ELE - POP90 issue still under investigation. Access System workers still working. ISS outer loop chassis to be installed either this afternoon or tomorrow.
PSL - Mode matching after 70W amp to drive back into the AOM/PMC beam path.
Bubba - Work Safely
Yesterday, Travis and Bubba's crew landed on a new VEA cleanroom configuration that allowed for better fiber welding equipment layout. This involved moving the large install platform staircase out of the VEA and bringing down a slightly bigger 8x10' cleanroom. We had to fix some panels, and rearrange the laser safety panels, and then the cleaning crew cleaned everything this morning.
Today, Travis and I worked on moving the extracted ETMX lower QUAD unit to the chamberside staging cleanroom using the duct jack, separated the main and reaction chains, then mounted the main half on it's weld trolley. We removed all of the flags from PUM and UIM stages for safe keeping and re-install later. We rolled the main chain into the welding room and left the reaction chain to be reworked for the AERM install soon.
On another note, I reinspected the ETMX PUM mass which had a crack under one of it's prisms (FRS 4743) originating from the fiber welding many years ago - the good news is that the crack does not look any worse than it did in 2013, when comparing it now to pictures from then (see for yourself in the DCC link E1800076).
The illuminators can now be remotely operated. Under tab SYS in sitemap, select illuminators to enable/disable each individual illuminator.
F. Clara, R. McCarthy, P. Thomas
3 dust monitors not responding this morning. LVEA6; PSL101; EX VEA2;
EX VEA 2 was reset at 16:15 and showing high .5u counts
Yesterday afternoon Terry and I made another attempt at aligning the beam from the OPO into HAM5, but we weren't able to find a beam returning to HAM6.
We are able to see ZM2 from the east viewport on the north side of HAM5, and we can see the back side off the OFI kickoff mirror that the beam from ZM2 is supposed to hit. We can tell that for some alignments our beam is hitting the optic holder for ZM2, but other than that we don't really know where the beam is.
Today we will try with the HAM5 illuminator plugged in, and perhaps repeating the aperture alignment with more care.
TITLE: 03/22 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
Wind: 5mph Gusts, 4mph 5min avg
Primary useism: 0.08 μm/s
Secondary useism: 0.26 μm/s
QUICK SUMMARY:
TITLE: 03/21 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
SHIFT SUMMARY:
LOG: Attached
As we plan to re-open BSC10 on Monday morning, I have restarted the clean rooms at E Y. The cleaning crew will do a cleaning of these tomorrow.
Thanks for the time to the Squeezer crew! And to CoreyG for coming back for more everyday.
Pulled the feedthru again and just sitting in the area seemed to change the readout. I could do some minor manipulation of the cable and send it to the rail and put some pressure and a particular bend to get it to read reasonable values. Wasn't going to mess with fixing and end up worrying how long it would last--just pulled it and replaced it. New sensor worked fine and repeatably.
With three working vertical sensors, we got a new locked position, unlocked and quickly balanced the table. Relocked and only saw a slight shift. Did a payload consolidation and refloated. ISI damped and once things were really settled down, Isolated the platform. Left the ISI locked on stops so SQZ crew could climb around as needed.
CAVEATS:
Unable to milk the new cable through the copper braided shield, will need to disconnect from feed-thru to do that, once I find/get a milking fid. Need smaller kinder peek zip ties--the big ones we have are just too hard on the small CPS cable which could be contributing to shorting.
I still need to as-build the payload--it is different than last Thursday now.
We need to get an Isolated spectra for closeout.
See photo below--I'll try to get some pointers on it (it is fuzzy too) but you can see where the zip ties a couple inches from the ends have damaged the insulation exposing the inner shield. There is also some shield visible at the BNC connector--this is where I was able to make it work and fail repeatably.
Here are some images to help clarify what we saw.
I can't find an up to date drawing of the HAM5 layout, but here is a preliminary drawing https://dcc.ligo.org/DocDB/0121/D1500303/002/HAM5.PNG, which shows ZM2 much further in the +y direction than it really is placed. In reality the beam from the OFI to ZM2 runs nearly parallel to the septum.
Here are some photos taken from the easternmost viewport on the north side of HAM 5 (the -y viewport on the +x side of HAM5). The first photo is a blurry overview of what we can see, the fly off mirror for the squeezed beam is in the center (there is a black glass clip on the back of the mirror), behind that you can see the cage of ZM2. The violet looking thing that is just peaking over the black glass clip is our beam or scatter from our beam.
The second photo shows that at some alignments on ZM1/ZM2, we can see a quite bright thing in HAM5 which is probably our beam. The fourth photo shows an alignment for ZM1 for which the beam clips on the bracket for the eddy current damper on ZM2, while the third photo shows an alignment of ZM1 where we think the beam should be hitting ZM2. You can see some difuse IR light, and what looks like the outline of the black glass clip in that scattered light. This seems like a good candidate for our best alignment, you might think that this scatter means that the beam is hitting or nearly hitting the fly off mirror with the black glass clip, however, we saw nothing in HAM6 for this alignment.
A few images and notes to help
1) Photo of path from ZM2 to OFI bench, from LHO alog 39663 and "big picture 1" see links below.
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=39663
https://alog.ligo-wa.caltech.edu/aLOG/uploads/39663_20171206192338_ZM2_BigPicture_1.jpg
2) LIGO-D1500303 linked above is / was a temp (preliminary) layout. Refer now to SYS links below. We have added a note to D1500303.
a) LLO
LHAM5 - LIGO-D0900456
ZM2 - LIGO-D1600094
b) LHO
WHAM5- LIGO-D0901129 (please note this top level is pending, refer to D1700472 and D0900456 for now)
ZM2 - LIGO-D1700472
Hope these help. Corey A, Eddie and Calum