Displaying reports 1-20 of 88044.Go to page 1 2 3 4 5 6 7 8 9 10 End
Reports until 08:09, Wednesday 17 June 2026
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 08:09, Wednesday 17 June 2026 (90649)
HAM2 Doors Installation

(Randy, Jordan, Jake, Owen, Travis, Gerardo)

Both doors were installed on HAM2, no issues to report.  The usual dance, take one door off, to then move the cleanroom to be able to remove the other door, thank you all for the help moving this cleanroom.  

There are some pecularities that we like to note about the doors, we noted some rust on both flanges of HAM2 -Y and +Y, and some embeded particulate on some of the O-rings, metal type all over, the particles were removed with a clean wipe, however there was a "green" fiber on the +Y door O-ring, outer O-ring, around 11 O'clock, this fiber runs with the seal and not across, so we did not poke at it.

Then we connected an aux cart to the annulus system, and started the pump down, we will add second aux cart to help with pump down.

Next, we like to inspect the viewports on this chamber, but this job is going to require laser safe and no table near the door.  We did note something on the central high quality viewport and we like to take a closer look at it.

Images attached to this report
H1 SUS
betsy.weaver@LIGO.ORG - posted 07:43, Wednesday 17 June 2026 (90648)
BBSS Oplev back alive

On Tues Oli tracked down and made the final move step to get the BBSS (still now named the BS in controls) Oplev signal live.  I uncovered the Oplev and released any errant stops.  SInce the sum was 2k instead of it's nominal 20k, Oli tried driving the BBSS sliders around, no luck, so we went out and looked for the beam in the Oplev box with Jason.  The Oplev Beam is offset in Pitch by a beam diameter at at the diode and roughly centered in yaw.  We are chewing on this.  Since we did not restore the plane of the BBBS to the exact same spot as the BS was we should not have expected the beam to be on the Oplev even if it's pit/yaw is correct, due to translation of the beam.  That said, I would have expected more of a yeaw error, less pitch.  Today we are going to take a peek at the in-air PSL MC flashes to see if we can see anything heading to the output arm which gives us confidence in our IAS pointing alignment on the test stand (and can therefore ignore the oplev).

LHO General
thomas.shaffer@LIGO.ORG - posted 07:27, Wednesday 17 June 2026 (90647)
Ops Day Shift Start

TITLE: 06/17 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 7mph Gusts, 5mph 3min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.12 μm/s 
QUICK SUMMARY: The LVEA is in the laser safe bifurcated state at the moment. SPI, SQZ, BBS, FARO work continues.

H1 SPI
joshua.freed@LIGO.ORG - posted 17:07, Tuesday 16 June 2026 (90645)
SPI, ISIK Install Day 4

J. Freed, J. Kissel, J, Wright, F. Clara

Continuing from 90621 (Notes are stored here). Today we brought the SPI picomoters into play, got caught up on our backlog of alogs, and began probably our toughest opical alignment during install. The periscope...

In order we did:

H1 SPI
joshua.freed@LIGO.ORG - posted 16:57, Tuesday 16 June 2026 (90644)
SPI, Pathfinder Install, First hints of efficiency drift in IFO REF

J. Freed,

At 9:18:50 this morning our aligned REF IFO started to fluctuate in efficency. (SPI_REFIFO_Efficency_Oscilation_Start.png) This happened before while building SPI in the optics lab; however, then it was happening contiuously, while now our REF IFO was fine until it started happening. 

SPI_REFIFO_Efficency_Oscilation_Start_C.png At the exact same time as when this started, the REF PWR MON fliped to negative power for a split second. (The second time we have discovered negative power). I have no clue to what caused this flip
 
SPI_REFIFO_Efficency_Oscilation_Start_NC.png I checked other possible causes: (set frequency changes and pico moter movements) but they were minutes before this occured so unlikly to be the cause.
Images attached to this report
H1 SQZ
camilla.compton@LIGO.ORG - posted 16:53, Tuesday 16 June 2026 (90629)
HAM7 Vent - Tuesday June 16th - realigned to FC and swapped FC WFS A, co-alignment found bad
Ryan S, Madi, Camilla
 
Realign to FC
Yesterday we unlocked the OPO SUS 90623 but released this slightly shifted the alignment coming off the OPO SUS towards the FC. Today, we moved A:M3 to center on the ZM3 iris and ZM3 for the retro-reflection. Sliders attached. ZM3 went from P -150, Y -660 to  P -130, Y -620.  We mainly moved in YAW (A:M3 only in YAW) and double checked that the height at ZM3 and FC1 was around 6.25" still. After this, beam was centered on ZM4 iris, we did not touch B:M4. 
Once we did this, the beam was getting to the SQZT7 PD with minimal clipping dips, there were still some dips from max level but we compared this to nighttime June 2nd (with chamber open and OPO SUS unlocked) and it is the same.
 
Power through OPO SUS Check 
Similar to in 90573, where we measured between 2% and 5.5% power drop. Today, total of around 1.38 to 1.44mW out of OPO, before A:DC1. Measured drop of between 0.02 and 0.08mW though to off OPO after B:M4. This is between 2% and 5.8% power drop. We expect at least 3% (1% for each SFI and 1% at B:BS1) and our power budget  has 4.7% measured.
 
Green Misalignment 
Before we started we noticed that the green beam towards FC is grossly misaligned in Pitch, attached photos at ZM1 iris (green beam low) and ZM3 iris (green beam high). We are not sure when this happened, as the SK path was very off yesterday, it could have happened before the OPO was unlocked. We will check everything is secure and then attempt to use a single pico-motor to fix this as the is the most likely thing to have got bumped. 
 
Swapping FC WFS A 
When we started the beam was misaligned in pitch on the FC WFS, very low on the lens. We moved the picos in Pitch to get the beam on both A and B. The picos both still have plenty of range. We then verified which QPD was A, marked its location with a dog, and at the chassis turned off the +/- 18V for WFS before unplugging both WFS cables. We then unplugged the WFS A and removed it, removed the diode detector holder D2000384 from the enclosure D2000246 (marked part #4) and swapped it to the new diode housing (add ICS link) and reinstalled.
Ryan caught we needed to put H1:SQZ-RLF_QPD_A_SEG_C_OFFSET back to nominal (I'd changed it in March), then everything then seemed as expected. We need to better center onto these QPDs tomorrow. 
Images attached to this report
H1 SPI
joshua.freed@LIGO.ORG - posted 16:45, Tuesday 16 June 2026 - last comment - 09:05, Wednesday 17 June 2026(90642)
SPI, Pathfinder Install, Issues with Saturating Oscillating FBR_PWRIN_REF.

J. Freed,

WE HAVE DISCOVERED NEGATIVE POWER

The FBR_PWRIN_REF PD that monitors the Power coming from the REF beam of the interferometer has gains alot of noise during certain intervals. Sometimes the noise even goes negative power. The noise is corelated with the frequency difference between the ref beam and the meas beam we set. The lower the frequency difference the higher the noise

SPI_PW_REF_Noise_Pt3.png Shows the correlation between Set fequency and the noise
 
SPI_PW_REF_Noise_Pt1.png is a close up of the transition. Since we have a 1sec ramp time the noise starts one second after setting a new frequency difference.
 
SPI_PW_REF_Noise_Pt2.png Shows that the noise is sawtooth at a frequency double the set frequncy. 
 
I currently have no evidence of what this could be.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 09:05, Wednesday 17 June 2026 (90651)
Here's a screenshot of the oscillations stopping at 09:08:08 PDT (16:08:08 UTC).
There's something in the MEAS signal as well, but the amplitude is less (at least with this 32 kHz sampling rate).

Of course, nothing changed in the signal readout chains at this time. But lots of things are happening surrounding it.

Also, the oscillations are different frequency in the MEAS vs. REF path (again, with the "this is clearly aliasing" grain of salt).

But, since we're not saturating when the oscillations are NOT present, I don't think it's an issue with the transimpedance *resistor*; it's probably just that we need to double the capacitance, dropping the pole frequency from 13.5 kHz to 6.7 kHz.

We'll put an analog o-scope on the signal this morning to confirm.
Images attached to this comment
H1 General
oli.patane@LIGO.ORG - posted 16:39, Tuesday 16 June 2026 (90643)
Ops DAY Shift End

TITLE: 06/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

LVEA is LASER SAFE (Bifurcated)

HAM2 doors on!!!!


LOG:                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                          

Start Time System Name Location Lazer_Haz Task Time End
22:52 HAZ LVEA is  LASER HAZARD LVEA YES LVEA is  LASER HAZARD 20:14
14:34 FAC Randy LVEA YES Prep for HAM2 doors (in @ 1400) 15:03
15:02 FAC Chris, Eric, Randy LVEA YES Scaffolding for GV6 15:51
15:06 VAC Jordan LVEA YES Checking on GV6 scaffolding work 15:47
16:21 PCAL Tony PCAL Lab y(local) Setting up a measurement 16:39
16:44 SQZ RyanS LVEA YES HAM7 work 18:59
16:47 VAC Jordan, Owen, Jake LVEA YES Grabbing parts 17:47
16:48 FAC RyanC LVEA n Grabbign dust mon 16:52
16:48 SQZ Camilla LVEA YES HAM7 work 18:59
16:59 BBSS Betsy, Oli, Jason LVEA yes checking on the BS Oplev level. 17:21
17:06 FAC Christina Optics lab N Making Alcohol wipes under the fume hood 18:13
17:13 CRS Madi, Shoshana LVEA H2 PSL YES Building CRS (Madi out 17:48) 19:19
17:29 SPI Jeff LVEA YES Turning pico controller on 17:31
18:27 SPI Jeff, Jennie LVEA n SPI install 20:18
18:30 PCAL Tony PCAL Lab y(local) Turning computer on 18:37
18:43 EE Marc CER YES Looking for Fil 18:45
18:58 SPI Josh LVEA YES SPI install 20:13
19:45 FAC Randy LVEA n HAM2 door prep 22:44
19:51 CRS Shoshana H2 PSL y(local) CRS work 20:39
19:58 VAC Travis MY n Checking equipment 20:41
20:00   Betsy LVEA YES Transitioning to LASER SAFE 20:13
20:06 SUS Ibrahim LVEA n DinoLighting the BBSS 22:06
20:13 SUS Betsy LVEA n Looking at the BS 22:06
20:16 FAC Jordan, Gerardo, Jake, Owen LVEA n HAM2 doors 23:16
20:18 SAF LVEA IS LASER SAFE (BIFURCATED) LVEA NO LVEA IS LASER SAFE (BIFURCATED) 12:18
20:18 EE Marc, Fil LVEA n Pulling cables 22:18
20:47 SQZ Camilla, RyanS, Madi LVEA YES HAM7 work (Camilla out 23:30) 23:34
21:09 VAC Travis LVEA n Watching HAM2 doors 21:59
22:14 IAS Jason LVEA N Setting up Faro 22:22
H1 SPI
jennifer.wright@LIGO.ORG - posted 16:14, Tuesday 16 June 2026 (90631)
Driving HAM2 Picomotor for centering SPI QPD B

Jennie W, Jeff K, Josh F

 

On Monday Betsy, Jeff and Josh got the light aligned from the ISIK breadboarrd in HAM3 to the ISIJ receiver in HAM2 manually while the HAM2/3 ISIs were locked (alog #90621). Then the ISI in HAM2 was unlocked (alog #90620).

 

This morning pitch was off on QPD A.

This morning Jeff recentred onto optical lever QPD A in HAM2 using M_M1 picomotor mirror. See pic. The SUM_OUT of the QPD was around 23.9V at 16:45 UTC.

 

Then we attempted to do the same for the optical lever QPD B in HAM3 using the ISIJ picomotor. See pic.

Jeff and Fil relocated the IOT2L picomotor driver in order to drive the ISIJ picomotor in this alog.

We were not finding a good point where we could center the beam solely with the picomotors so Jeff went in chamber and we were near the edge of the M_M5 pericope mirror.

 

I used the ISIJ picomotor to center on the first periscope mirror M_M5, but the alignment downstream from the periscope is still ongoing.

We could not center the beam on the QPD B so that it was equally on all four quadrants and we saw clipping on the beamsplitter in front of the QPD B, M_B4.

Picomotor is  now functional but now we need to do the correct thing; center the beam on M_M5, then use M_M5 to center on QPD B.

Centering on M_M5 with the picomotor was simple. Some notes for next time: moving left on the ISIJ picomotor moves the beam in +Y on the QPD and moving down on the picomotor moves up (or +Z) . Use the speed 'jog' on the picomotor and steps of 100 counts to see motion, finer steps of 10 are needed to do fine adjustment.

Eventually Jeff realised we needed to roll the periscope mount in RZ to change the pitch alignment in the QPD B local coordinates which is hard to get fine adjustment on as the whole mount must be moved and then the set screw re-tightened which can then again move the alignment. Yaw adjustment is done with the alignment screws on the mount so once we get pitch adjusted we can improve yaw.

Conclusions:

Images attached to this report
H1 SPI
jeffrey.kissel@LIGO.ORG - posted 15:55, Tuesday 16 June 2026 (90640)
Temporarily Relocated Picomotor Controller 5 for SPI ISIJ HAM2 Driving
J. Kissel, F. Clara

In order to get SPI ISIJ HAM2 picomotors for M_C1 functional, Fil and I pulled the production Picomotor Controller 5 from on top of IOT2L (which is away, parked over by HAM3 while the HAM2 doors are off), and move it back to near HAM2, next to SUS-R1, resting on the cable tray. We plugged in its production cabling as designed.

It worked! 

The M_C1 horizontal and vertical picomotors are channel 7 on PICO B, or Controller 5, driven by ECAT chassis Corner 2.
[1] D2400111 SPI Wiring Diagram
[2] D1900511 ISC Wiring Diagram
[3] D1100683 EtherCAT (Beckhoff) System Diagram
Images attached to this report
LHO VE (VE)
travis.sadecki@LIGO.ORG - posted 15:52, Tuesday 16 June 2026 (90641)
LLCV cut out of CP4 dewar system

See WP 13325.  The Liquid Level Control Valve was cut out of the decomissioned CP4 N2 dewar system.  The ends of the remaining piping were plugged with rubber stoppers and then covered with rubber caps held in place by pipe clamps.  We are looking into a more permanent solution for capping the pipes off, but LLO needs the valve ASAP so this temporary solution will do for now.  The valve is in shipping and receiving and will ship out tomorrow morning.

Images attached to this report
H1 SPI (SEI, SPI)
jeffrey.kissel@LIGO.ORG - posted 15:24, Tuesday 16 June 2026 - last comment - 15:38, Tuesday 16 June 2026(90633)
SPI Pathfinder MEDM and EPICs Infrastructure Tune-up with Real Signals
J. Kissel, J. Wright, J. Freed

Now that we've got the SPI in chamber and moving things along with beams (LHO:90621), it was time to make another run through the MEDM screens and infrastructure (last touched during the initial release of the screens LHO:90006) to make sure the signals flow as intented and the UIUX has everything it needs.

This morning we:
    - Added linked to the picomotor control to the overview
    - turned on inputs, outputs, and set gains to 1.0 to make sure IFO PDs were demodulated and producing a legit live contrast estimate with the amplitude and mean of the PD signals
    - turned on inputs, outputs, and set gains to 1.0 in any bank necessary to make sure optical lever QPDs SUM, PIT, YAW signals made it to the {PIT,YAW}_OUT_DQ channels 
    - added a first-guess low pass -- 4th order butterworth filter with 10 Hz corner frequency -- to the MEAN banks that filter the raw IFO PD signals (with the 4096 Hz beat note on it) to get the mean of the signal.

This needed several mods to MEDM screens that had some missing filter banks:
    in /opt/rtcds/userapps/release/spi/common/medm/
    - Addition of links to picomotor control screens 
         SPI_CUST_OVERVIEW.adl            committed to   rev 35342
    - Added missing HETPHA and HETAMP filter banks at the output of I/Q to AMP/PHASE conversion
         SPI_CUST_IFO_DEMOD.adl           committed to   rev 35337
    - Added missing CONTRAST Filter Banks, and changed the precision of the OUT16 displayed on the screen from truncated (for signals above 1) to decimal.
         SPI_CUST_IFO_MON.adl             committed to   rev 35338.
    - Quick resolution of long-standing bug with labels of banks in 
         SPI_CUST_OL_ISIOUTF.adl          committed to   rev 35336

All of the above settings have been committed to the h1spih23's safe.snap
    /opt/rtcds/userapps/release/spi/h1/burtfiles
         h1spih23_safe.snap               committed to   rev 35340
Comments related to this report
jeffrey.kissel@LIGO.ORG - 15:27, Tuesday 16 June 2026 (90634)
SPI Overview Screen Update

BEFORE vs. AFTER screenshot.
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 15:29, Tuesday 16 June 2026 (90635)
SPI CUST IFO DEMOD Update

BEFORE vs. AFTER screenshots.
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 15:32, Tuesday 16 June 2026 (90636)
IFO MON Contrast Screen Update

BEFORE vs AFTER screenshot.
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 15:34, Tuesday 16 June 2026 (90637)
OL ISIOUTF Banks

BEFORE vs. AFTER.
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 15:38, Tuesday 16 June 2026 (90638)
Details of IFO_MEAN Filters

The 10 Hz low pass fitler for the mean bank are 
    Channel                                 Module    Design String
    H1:SPI-H23_IFO_{REF,MEAS}_{A,B}_MEAN    FM1       butter("LowPass",4,10)

Screenshot of location in MEDM.
Bode Plot of filter frequency response.
Images attached to this comment
H1 COC (COC)
ibrahim.abouelfettouh@LIGO.ORG - posted 16:36, Thursday 11 June 2026 - last comment - 17:35, Tuesday 16 June 2026(90600)
Mystery Spots/Streaks on BBS01 AR Side

Ibrahim, Betsy, Anamaria

Upon first in-chamber BBS01 inspection, we found 3 large clumps of spots approximately 100mm from the edge. We're consulting GariLynn at CIT for steps on how to clean.

Acetone swab: We tried to go over the spots with a cotton swab with acetone, but the spots remained.

First contact: We then tried to first contact a small portion with one thin layer, but the spots remained.

While there's no evidence that the beamsplitter was contacted, dinked, touched or scratched in anyway, this might be a cause for the damage. There is texture to the spots upon brushing them with a swab and while it seems more likely that these are above the surface, we are not totally sure.

Hypotheses (and their problems)

1. Peek In-Vac cable scratch: maybe an in-vac cable fell on that area but they would have had to imprint multiple times with some force to show something like this. 

2. Falling foil: maybe a piece of foil fell onto the surface and scratched it that way? No foil was used or wrapped at height during BBS and again, the foil would have had to fall with some heft.

3. There-the-whole-time: Maybe the spots were there the whole time and are invisible to non-chamber conditions. Because this is on the AR side, there is no good scatter plot of the surface. Since we did not see this in normal light conditions, but immediately saw this in chamber (dark) conditions, this may have been there all along. The spots are quite large (as attachments show), so this makes that less likely.

4. Dry first contact: Maybe it's dry first contact? We went over some of the spot with acetone but it stayed. We also first contacted a thin layer on one part but it stayed. The nature of the spots do look like they're small first contact bubbles. We found the first contact sheet that we used on that side and indeed, there are some similar streaks in size but nothing conclusive. We're looking at matching the spot with the first contact to see if there is a streak in this region. Problem is - first contact wouldve come off quick with the acetone treatment. So this is also not likely it.

What to do next:

- Analyze with Dino-Lite: We're going to zoom in on the spots with our DinoLite mount to get a better look. This could tell us if they are truly scratches or stuck particulate.

- Match first contact sheet with spots: Seeing if these spots were visible during FC (done on May 6) - alog 90149. Nothing visible. 

- Anamaria suggested at any rate shining a gaussian beam at it to analyze the damage in a short experiment to characterize. 

Images attached to this report
Comments related to this report
ibrahim.abouelfettouh@LIGO.ORG - 17:35, Tuesday 16 June 2026 (90639)

Ibrahim, Betsy

First, we imaged the spot, which yeilded these attached pictures of what look like... specks. No idea what these may be.

We then went over the spot with some thicker first contact, which did not remove any of the specks.

We recieved the procedure for spot-water cleaning which is the only last thing that we're thinking of trying.

In the attachment, the thinner lines are dry acetone and can be removed. Focus on the brighter dots instead.

Also adding a "map" of our AR side features thus far. I will digitize it and add this as an alog/DCC of its own once we're done with optic inspection.

Images attached to this comment
H1 CDS (SPI)
filiberto.clara@LIGO.ORG - posted 17:19, Wednesday 10 June 2026 - last comment - 21:28, Tuesday 16 June 2026(90585)
SPI Fiber Cover Installed

A plexi security cover was installed over the SPI Laser Chassis. Cover will be locked under normal operating conditions.

Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 21:28, Tuesday 16 June 2026 (90646)
More pictures of the plexi-glass hatch. It secures to the chassis via screws and stand-offs, and has side openings. The box is merely trying to satisfy the "requires a tool to detach the fibers" criteria to make the system laser safe. The key will live in the control room lock box with all the other laser safety keys.
Images attached to this comment
H1 TCS
ibrahim.abouelfettouh@LIGO.ORG - posted 16:04, Thursday 16 April 2026 - last comment - 08:38, Wednesday 17 June 2026(89926)
TCS Chiller Water Level Top-Off - BiWeekly FAMIS 28639

Closes FAMIS 28639

Last checked in alog 89720

TCSX read 30.8 - nothing added

TCSY read 10.6 - nothing added\

No water in small cup under the slow leak

TCSX is reading HIGH PRESSURE FAULT. See attached picture. 

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 17:25, Thursday 16 April 2026 (89931)

Betsy and I locked and tagged out the CO2X chiller, it will remain off until all needed repairs and safety documents have been completed next week. 

At 15:44UTC the chiller tripped off with a HIGH PRESSURE fault, as found by Ibrahim.  The CR verbal machine also alerted Ryan with a "low flow" warning.

I went out to the LVEA inspecting the pipes and found that the outgoing CO2X line was disconnected at the quick-connect, image. There was no water on the floor, so the quick-connect did it's job. Maybe this was already loose and we need to add the the pipe inspection FAMIS to inspect these connections, but. there was also lot of work in that area today. I inspected and reconnected the quick-connect, it did not seem damaged.

At out weak point in the chiller lines at the flexible baffle in the pipe bridge, the plastic sheeting that had been attached to catch any spilled water had a small amount of water in it photo, but none leaking out. Expect this water would have been pushed out a small break in the rubber while the chiller was trying to push water around the incomplete lines before the high pressure sensor in the chiller tripped it off. We will inspect and probably repair this part next week. In the meantime with water dripping out of the pipe bridge connection, we are fine to leave the chiller locked out with water in the lines. 

Images attached to this comment
camilla.compton@LIGO.ORG - 11:07, Monday 20 April 2026 (89949)

TJ, Camilla. Trending the pressure values doesn't tell us much. The chiller appears to go to the high pressure fault and trip off before the  pressure channels register a high pressure, see attached. ANALOG1 PSI starts at 65 PSI and ANOLOG2 started at 26 PSI, after the chiller trips off, these increase to 6500 PSI (unphysicial) and 44 PSI. The chiller must have an additional pressure sensor it uses to trip off. Current settings are to trip off at 80 PSI, see FRS 30283.

Images attached to this comment
camilla.compton@LIGO.ORG - 08:38, Wednesday 17 June 2026 (90650)

Randy built a unistrut protective barrier around both CO2X and CO2Y water pipes to protect them from this happening in the future. Photos attached. 

Images attached to this comment
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