Displaying reports 12801-12820 of 86444.Go to page Start 637 638 639 640 641 642 643 644 645 End
Reports until 09:25, Wednesday 14 February 2024
H1 CDS (CDS)
erik.vonreis@LIGO.ORG - posted 09:25, Wednesday 14 February 2024 (75852)
Conda environment updated

The CDS conda environment has been updated.

If you run in to trouble with the new environment, you can switch back to the production environment with 'conda activate cds-py310-2023120401'

This environment includes two new programs from Gabriele: 'interactivefitting' and 'loopdesigner'.

It also includes a new release of diaggui and foton, version 4.0.3.  This version has minor improvements and bug fixes.

foton now can suppress warnings for zeros in the right-hand plane.  Pass -Z f as a command line argument or set the environment variable FOTON_WARN_RHP_ZEROS=false.  The environment variable will also work with python-foton.

Difference cursors now work in diaggui plots.

For a full list of changes see https://git.ligo.org/cds/software/dtt/-/wikis/ChangeHistory

H1 General
anthony.sanchez@LIGO.ORG - posted 08:12, Wednesday 14 February 2024 (75851)
Wed Feb 14th Ops Day shift.

TITLE: 02/14 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 11mph Gusts, 9mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.34 μm/s
QUICK SUMMARY:
Fire Dept has 2 pickups and 2 Engines down X arm for Burning tumbleweed with Tyler.
Eric and Randy are already heading down to EY for Wind fence work.
HAM7 Door has been closed. and Vacuum team will likely be trying to start the prepareing for pump down today.

 

 

LHO VE
janos.csizmazia@LIGO.ORG - posted 19:49, Tuesday 13 February 2024 (75850)
2-13 vent vacuum diary
Today's activities:
- HAM7 X+ X- doors have been closed. With the new X+ septum door, we had a hard time, as the O-ring didn't stay easily
- The O-ring blanks have been installed back on the septum door
- The Annulus volume of HAM7 - after closing the doors - is being pumped
- Corner pumpdown status: we are at ~30 Torr
- The Annulus Ion Pump of GV5 has been switched back on
- EX pumpdown status: 4.33E-8 Torr
H1 CDS (CDS, VE)
patrick.thomas@LIGO.ORG - posted 13:04, Tuesday 13 February 2024 - last comment - 13:10, Tuesday 13 February 2024(75846)
Updated MEDM screens on Beckhoff vacuum machines
Closes WP 11686.

I tried to use WinSCP to copy the Git for Windows installation file across from opslogin0, but it would not connect (something about the encryption protocol I think). I tried to update WinSCP, but the browser would not connect to the site (outdated Internet Explorer maybe?). I then recalled the Samba share I had set up, and copied the Git installer over from there. (For future reference, open the Windows file explorer and put \\10.20.0.118 in the location and use the username and password from the shared secrets page.) I first tried to install the 64 bit version, but was told by the installer that it was a 32 bit machine, so downloaded the 32 bit installer (Git-2.43.0-32-bit.exe) onto opslogin0 and copied it to the Samba share and then copied it from there onto the Windows machine. I received a warning when installing it that "Git for Windows (32-bit) is nearing its end of support. More information at https://gitforwindows.org/32-bit.html". I then cloned https://git.ligo.org/cds/ifo/vacuum/h0/medm.git onto the Desktop and ran the "/Source/create_medms.py" script in it. I changed the path in the sitemap.xlaunch shortcut to point to the cloned repo. The medm screens should now be up to date on all of the vacuum Beckhoff machines.
Images attached to this report
Comments related to this report
patrick.thomas@LIGO.ORG - 13:10, Tuesday 13 February 2024 (75847)
This reads like I just did this on one machine, but it was done for all except for h0vacly and h0vacmr, which already had Git installed from alog 65799. For those I just had to clone the new repo for the medm screens and update the sitemap.xlaunch.
H1 General
ibrahim.abouelfettouh@LIGO.ORG - posted 12:07, Tuesday 13 February 2024 (75845)
OPS Day Midshift Update

LVEA is laser SAFE

Current ongoing activities

H1 CDS
david.barker@LIGO.ORG - posted 10:15, Tuesday 13 February 2024 (75843)
DTS ENV services started following x1dtslogin reboot

Jonathan, Dave:

Following Jonathan's maintenance reboot of x1dtslogin, I restarted the dts_tunnel and dts_env services on cdsioc0 to reconnect with the DTS Gneiss environmental monitor.

LHO VE
david.barker@LIGO.ORG - posted 10:12, Tuesday 13 February 2024 (75842)
Tue CP1 Fill

Tue Feb 13 10:09:20 2024 INFO: Fill completed in 9min 16secs

Gerardo confirmed a good fill curbside.

Images attached to this report
H1 General
ibrahim.abouelfettouh@LIGO.ORG - posted 09:25, Tuesday 13 February 2024 (75841)
OPS Day Shift Start

TITLE: 02/13 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 3mph Gusts, 1mph 5min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.25 μm/s
QUICK SUMMARY:

 

H1 CDS (CDS)
erik.vonreis@LIGO.ORG - posted 06:46, Tuesday 13 February 2024 (75834)
Workstations updated

Workstations updated and rebooted.  This was an OS package update.  Conda packages were not updated.

LHO VE
janos.csizmazia@LIGO.ORG - posted 19:47, Monday 12 February 2024 (75832)
2-12 vent vacuum diary
Today's activities:
- The Corner pumpdown has been started. After 5h50min pumping, we are at 250 Torr
- HAM6 / HAM5 common Annulus volume is now pumped also with the Ion pumps, they are at the mid-E-6 Torr range
- EX pumping status: 4.65E-8 Torr
- EX RGA bakeout has been ramped down; it is now ready for a post-vent RGA scan
- HAM8 RGA is being pumped. The HAM8 turbo pump has also been started up, they are now ready to be valved in and for a pre-vent RGA scan, although there are issues, see here: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=75814
H1 CDS (ISC, SQZ)
filiberto.clara@LIGO.ORG - posted 16:26, Monday 12 February 2024 (75831)
Field Cabling for SQZT8 Disconnected

WP 11689

The field cabling to the SQZT8 enclosure are now disconnected. Part of the safety interlock system was moved away from the table (Beckhoff 1908 field box). This required the door & panel status cable to be disconnected. Safety MEDM is showing SQZT8 in a fault (panels and doors open). FCES E-stop button is still active.

H1 General
rahul.kumar@LIGO.ORG - posted 11:50, Monday 12 February 2024 - last comment - 08:17, Tuesday 13 February 2024(75825)
HAM7 close-out exit check list

Given below are the list of things I did in HAM7 to prepare for the close out of the chamber.

- Took particle counts outside and inside the chamber and they were zero (inside chamber) and few tens (outside chamber).

- Removed the two irises from the chamber and handed it over to Camilla (wrapped and bagged).

- ZM4 & ZM5: checked their pitch adjuster is locked, checked their dog clamps, checked all the EQ stops, centered the BOSEMs and took transfer function measurements - they look good.

- Confirmed that all wiring appears properly secured and is free of the beam path.

- Placed a silicon wafer inside the chamber on the ISI table.

- Removed all tools from the chamber (checked it twice).

- Took pictures - attached below.

Currently Fil is performing ground loop checks and Jim is un-locking the ISI.

We will be ready to put the doors once SEI and SUS transfer function measurements comes out healthy.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 08:17, Tuesday 13 February 2024 (75835)EPO

Tagging EPO for these HAM7 closeout photos.

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 16:26, Friday 09 February 2024 - last comment - 08:22, Tuesday 13 February 2024(75810)
HAM6 Doors Installation

(Randy P., Jordan V., Janos C., Gerardo M.)

We installed two doors on HAM6.  +X door went on very smoothly, no problems. -X door we had a small issue with the inner o-ring, did not wanted to stay put, it took some convincing, no new issues to report.

We are currently pumping down the annulus system with two aux carts, thus far the vacuum pressure at the aux carts pumping the AIPs appears nominal.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 08:22, Tuesday 13 February 2024 (75836)EPO

Tagging EPO for Door install pics.

H1 SEI
shoshana.apple@LIGO.ORG - posted 10:02, Thursday 08 February 2024 - last comment - 08:31, Tuesday 13 February 2024(75785)
BRS Remote Mass Adjuster Install
[Michael, Jim, Tony, Shoshana, Neil]

We've spent the week working on installing a remote mass adjusting/balancing system for the End-X BRS. Upon opening the End-X BRS we discovered that it is slightly different than the other BRSs (most likely because it was the first one built, photo 1 below) so we had to get a couple extra parts machined for the parts we brought from UW to fit properly. The hardware has finished being installed (photo 2), and we've run a quick test of the picomotor (Newport  8341-UHV) to make sure it has full range of motion. We've finished closing the BRS up and are now waiting for it to pump down before doing some additional in-vacuum tests. 

We are writing up some installation and balancing instructions as well as leaving another set of parts, so a remote balancing system can be installed on the other BRS. We assume the End-Y BRS should fit the drawings on the dcc (D1800045), so no additional parts should need to be machined. We are also leaving 16 flexures here with Jim.


The pico motor controller chassis was not working, so we are leaving our UW picomotor driver (Newport 8742) here so that the End-X BRS can be adjusted until the chassis is fixed. Once it is fixed the in-air wiring will need to be re-connected to get the motor to the chassis. For now adjusting will have to be done with a laptop at the End-X station, but once hooked up to the chassis, adjustments can be made from the control room.
Images attached to this report
Comments related to this report
brian.lantz@LIGO.ORG - 08:35, Friday 09 February 2024 (75799)

Yeah! Jim's back will be grateful.

Notes about the design and additional details on the installation are in SEI log 1886 and attachments.

corey.gray@LIGO.ORG - 08:31, Tuesday 13 February 2024 (75837)EPO

Tagging EPO for these new BRS innards photos.

H1 PEM (OpsInfo)
ryan.crouch@LIGO.ORG - posted 10:51, Thursday 01 February 2024 - last comment - 11:31, Tuesday 13 February 2024(75671)
Dust monitor levels

The dust monitor IOC was restarted this morning by Dave which can reset the alarm levels. Following document E1600132, I confirmed that the alarms levels are still set properly, The CS dm alarms, 5, 6 & 10 are set to the "Class-100" (major alarm at 100 counts for both 0.3u and 0.5u as opposed to their normal 10000 for 0.5u and 7000 for 0.3u) as defined in the document since these monitors are by vented open chambers. Once the chambers are closed back up I'll put the CS dm alarm thresholds back.

Comments related to this report
ryan.short@LIGO.ORG - 15:32, Monday 05 February 2024 (75734)OpsInfo

I've set the alarm levels for dust monitors 6 and 10 back to their nominal levels of 7000 counts minor and 10000 counts major for both 0.3u and 0.5u since HAM3 is closed and the cleanroom is off. Dust monitor 5 (HAM6) remains at the lower alarm level of 70 counts minor and 100 counts major.

ryan.crouch@LIGO.ORG - 11:31, Tuesday 13 February 2024 (75844)

DM5 is actually the DM by HAM3 and DM6 is by HAM5/6/7. So I set DM5 back to its higher levels since the doors back on and I lowered DM6s to CLASS 100 levels till the doors go back on later this week. 

H1 ISC (ISC, SUS)
keita.kawabe@LIGO.ORG - posted 21:34, Monday 29 January 2024 - last comment - 09:10, Tuesday 13 February 2024(75601)
HAM6 work Jan/29/2024: Alignment of the laser into the new OMC, day 4 (Camilla, Vicky, Julian, Rahul, Sheila, Betsy, Keita)

day 1 (alog 75548), day 2 (alog 75557), day 3 (alog 75575)

HAM7 irises were good

Sheila/Camilla checked the iris position on HAM7 and it was good.

ASC-AS_C whitening gain was increased by 18dB, dark offset was reset

I didn't like that the ASC-AS_C input was so small. Increased the whitening gain by 18dB (from nominal 18dB to 36dB) and reset the dark offset.

Recentered the beam on ASC-AS_C. One thing that was strange was that the ASC-AS_C_NSUM would become MUCH bigger (like a factor of 10) when SRM is misaligned. I was worried that I was looking at a ghost beam. Camilla measured the  beam power to be ~1mW out of HAM7 and ~0.7mW into HAM6. When ASC-AS_C was centered, ASC-AS_C_NSUM_OUT became ~0.008 give or take some. Taking the 16dB extra whitening (i.e. a factor of 8) into account, ASC-AS_C_NSUM~0.008 means about 1mW into HAM6, which was in a ballpark, so I convinced myself that the beam on AS_C was good.

HAM6 irises and beam height on OM, the beam was still very low on OM2

At this point OMC QPDs are reasonably centered, so Sheila and Camilla checked the beam position on irises in HAM6.

The beam was OK on the first iris but was a bit low (~2mm) on the iris closer to the OM1.

The beam position on OMs at this point as well as the slider values and max DAC output are listed below (see Camilla's pictures, too). Note that the YAW position in the table is the position of the incoming beam on the mirror measured at some (unknown) distance, it's not on the mirror.  

  OM1 OM2 OM3
Beam height (nominal 4") 1/8" too high 1/4" too low 1/16" too low
YAW position 1/8" to +X 1/32" to -X Cannot measure
PIT slider 430 20 610
YAW slider 600 1300 -231
Max DAC output 11k 7k 9k

The beam was clearing the input and output hole on the shroud, was cleanly hitting the small OMCR steering mirror by the cage, and was already going to the OMCR diode.

They confirmed that the OMC trans video beam was visible on the viewer card when OMC flashes and it was hitting the steering mirror (but we need a viewport simulator to see if the beam will clear the viewport aperture).

Bringing the beam up higher on OM2

Unfortunately the beam was still very low (~1/4"), however I was able to use OM1 alignment slider to bring the beam up on OM2 and use OM2/3 alignment sliders to still center the OMC QPDs. After this was done, OM2 PIT offset became large but OM1/OM3 offsets became low-ish. This was a very good sign as it's infinitely easier to mechanically tilt OM2 than OM1/OM3 due to superior mechanical design.

Anyway, by doing this, the beam height on OM2 went up by about 1/8" (see Rahul's pictures). It's still too low by 1/8", but bringing the beam up more would mean that OM3 DAC output will become large w/o mechanically relieving, which I didn't want to do, so I decided to stay here.

  OM1 OM2 OM3
Beam height 1/8" too high (didn't measure, no reason to suspect that it changed) 1/8" too low 1/16" too low
PIT slider 20 2710 -590
YAW slider 650 660 60
Max DAC output 7.2k 21k 7.1k

Mechanically relieving the OM2 PIT offset

Julian set the OM2 PIT slider gain to 0.75 (from 1), Rahul turned the balance mass screw on the upper mass of OM2 to compensate. We repeated the same thing four times (slider gain 0.75->0.5->0.25->0, each step followed by Rahul's mechanical adjustment). We had to adjust OM2 Y slider in the process to bring the beam back to the center of the OMC QPDs, but overall, this was a really easy process (did I mention that tip-tilt adjustment is not an easy thing to do?).

We ended up with this (we haven't measured the beam height again as OM2 was the only thing that moved, so the height numbers are from the previous table just for convenience).

  OM1 OM2 OM3

Beam height (didn't measure, no reason to suspect that they changed)

1/8" high 1/8" low 1/16" low
PIT slider 20 0 -590
YAW slider 650 760 60
MAX DAC output 7.2k 5k 7.1k

I declared that this is a good place to stay. Rahul fixed the balance mass on OM2 upper mass.

Rahul also fixed the balance mass on OMCS.

Fast shutter path, WFS path, ASAIR path, OMCR path

We closed the fast shutter and the reflected beam goes to the high power beam dump.

We opened the fast shutter and checked the WFS path. The beam was already hitting one quadrant of WFSB but was entirely missing the WSFA. The beam was a bit low on the lens on the WFS sled, so I used two fixed 1" steering mirrors upstream of the WFS sled to move the beam up on the lens and keep the path reasonably level. See Rahul's pictures for the beam height. After this, both WFSs saw the light, and at this point we used pico to center both. We weren't able to see the beam reflected by the WFS but assume that it still hit the black glass.

We tried to see the ASAIR beam but couldn't. Since the beam is hitting the center of ASC-AS_C, we assume that the ASAIR beam will still hit the black glass.

OMCR beam was already hitting the OMCR photodiode, but the beam was REALLY close to the beam dump that's supposed to catch ghost beam. We temporarily moved the dump so the beam is about 5mm from the edge of the glass, but this might be too far. I'll find how close it's supposed to be from the past alog.

Couldn't check if PZT1 is working.

We tried to see if OMC length error signal makes sense when scanning the OMC length, but whenever the OMC is close to resonance there was a huge transient in the DCPD SUM as well as the length signal, probably the intensity noise (due to acoustics or jitter or something) is too much. We'll measure the capacitance of the PZT from outside.

Current status of LVEA

Laser hazard, HAM5 GV is closed, HAM6 and HAM7 curtains are closed.

Remaining tasks

Comments related to this report
camilla.compton@LIGO.ORG - 08:43, Tuesday 30 January 2024 (75614)

Photos attached before the beam height on OM2 was adjusted. In Keita's stage "HAM6 irises and beam height on OM, the beam was still very low on OM2".

Photos of OM1 Pit and OM1 YawOM2 Pit and OM2 Yaw, no photo of OM3. Position of beam on Iris 1, Iris 2 (and the backside of Iris 2). And photos of HAM7 with curtains split for SQZ beam. HAM6 with iris 1.

Images attached to this comment
rahul.kumar@LIGO.ORG - 10:08, Tuesday 30 January 2024 (75615)

Attached below are the pictures showing the beam height on OM2 (pitch and yaw position) and WFS in HAM6 chamber after we made the adjustments.

Also shown is the lens before the WFS, on this the yaw looks OK and is slightly low on pitch but Keita is happy with this.

On a different note:-

OM1, OM3, OMC BOSEM flag position looks fine, OM2 will need some adjustment (once we are laser safe).

The latest slider values for OM1-3 has been attached below.

Images attached to this comment
keita.kawabe@LIGO.ORG - 09:43, Tuesday 30 January 2024 (75616)

The last photo in alog 65101 from Sept. 2022 shows the distance between the OMCR beam dump and the main OMCR beam back then. We will get close to this photo.

https://alog.ligo-wa.caltech.edu/aLOG/uploads/65101_20220923181903_BD_clearance.jpg

julian.gurs@LIGO.ORG - 17:09, Wednesday 31 January 2024 (75653)
Possibly clipping at a beam dump.
In picture "beforemoving" it can be seen how the beam hits the outer left edge of the IR card and this side "touches" the beam dump.
We have moved the beam dump because the beam is centered on the lens.
Images attached to this comment
corey.gray@LIGO.ORG - 09:10, Tuesday 13 February 2024 (75840)EPO

Tagging EPO for alignment of HAM6 work

H1 General (SEI)
betsy.weaver@LIGO.ORG - posted 12:38, Wednesday 24 January 2024 - last comment - 09:07, Tuesday 13 February 2024(75543)
EY wind fence needs repair again

For the record, late alog - a couple weeks ago the EY wind fence was found to be damaged, again from early JAN severe winds (50+mph gusts for a few days).

Plans are in place to repair it with an improved round of reinforcement.  A second snorkel lift is being delivered to aid in the repair scheduled for ~next week.  FRS ticket filed.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 09:07, Tuesday 13 February 2024 (75839)EPO

tagging EPO for our EY wind fence

H1 SQZ
camilla.compton@LIGO.ORG - posted 08:53, Wednesday 17 January 2024 - last comment - 09:04, Tuesday 13 February 2024(75436)
Unplugged and replugged HAM7 FC 532nm Fiber from Feedthorugh

For the VAC team to bag and leak check the HAM7 leaky fiber feedthorugh FRS30141, yesterday afternoon I unplugged the  HAM7 FC 532nm Fiber from the Feedthrough, covered with a plastic endcap and then replugged in when the VAC team was finished. 

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 09:04, Tuesday 13 February 2024 (75838)EPO

Tagging EPO for fiber feedthru pics.

H1 ISC
evan.hall@LIGO.ORG - posted 21:06, Tuesday 25 April 2023 - last comment - 14:20, Wednesday 14 February 2024(69026)
Driving PR3 pitch and yaw at low frequency

Sina, Elenna, Kevin, Evan

Similar to Anamaria's measurements at Livingston last year (LLO:58623), we drove PR3 sinusoidally in pitch and yaw at low frequency to try to ascertain the amount of beam spot motion coupling into the arms. The following times are all 2023–04–12 UTC:

Comments related to this report
evan.hall@LIGO.ORG - 21:04, Monday 12 February 2024 (75833)

At 0.34 Hz, the transfer functions from oplev to oplev are

  • |IX/PR3| = 1.81
  • |EX/PR3| = 0.76
  • |IY/PR3| = 0.57
  • |EY/PR3| = 0.60

The absolute values are indicated because the measured phases are neither clearly around 0° nor 180°. The coherences are above 0.85. (At 0.11 Hz, the coherences are somewhat lower so I omitted those values.)

Livingston also saw order-unity transfer functions like this: LLO:59846.

A series of finesse simulations (G2400278G2400281) indicated that by itself, PR3 cannot drive arm cavity motion at this level since (in the absence of any angular feedback control) the arm cavity finesse suppresses PR3-induced spot motion by a factor of order 100. On the other hand, PR3 motion can appear in the reflection wavefront sensors with an optical strength similar to or even greater than cHard motion, meaning that if PR3 has not been carefully diagonalized out of the sensing matrix then its motion can easily be impressed onto the test masses with an order unity ratio.

evan.hall@LIGO.ORG - 14:20, Wednesday 14 February 2024 (75859)

The attachment shows coherences between PR3 oplev and test mass oplevs from the end of O4a. Ignoring the microseism region, there is coherence between PR3 pitch and EY pitch from 0.4 to 0.8 Hz. One might guess this coherence arises because of LVEA ground motion, but there is no coherence between the PR3 oplev and either the HAM1 Z L4C channel or the HAM2 Z ground motion.

Images attached to this comment
Non-image files attached to this comment
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