Displaying reports 941-960 of 82959.Go to page Start 44 45 46 47 48 49 50 51 52 End
Reports until 09:26, Monday 19 May 2025
LHO VE
jordan.vanosky@LIGO.ORG - posted 09:26, Monday 19 May 2025 (84452)
Morning Purge Air Checks 5-19-25

Dry air skid checks, water pump, kobelco, drying towers all nominal.

Dew point measurement at HAM1 -43.9 °C.

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:38, Monday 19 May 2025 (84449)
Ops Day Shift Start

TITLE: 05/19 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: LIGHT_MAINTENANCE_WINDY
    Wind: 17mph Gusts, 10mph 3min avg
    Primary useism: 0.02 μm/s
    Secondary useism: 0.11 μm/s
QUICK SUMMARY:

HAM1 doors should be going on today!

LVEA is currently LASER SAFE (84443)

LHO VE
david.barker@LIGO.ORG - posted 10:14, Sunday 18 May 2025 (84448)
Sun CP1 Fill

Sun May 18 10:06:37 2025 INFO: Fill completed in 6min 33secs

 

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:17, Saturday 17 May 2025 (84447)
Sat CP1 Fill

Sat May 17 10:06:18 2025 INFO: Fill completed in 6min 14secs

 

Images attached to this report
H1 PSL
sheila.dwyer@LIGO.ORG - posted 20:02, Friday 16 May 2025 - last comment - 11:33, Monday 19 May 2025(84446)
PMC left unlocked

I left 10W out of the rotation stage, with the stage de-engergized this evening and the light pipe closed.  I've just now unlocked the PMC (LOCK off, RAMP off) so that we won't have 10W on the light pipe shutter all weekend. 

 

Comments related to this report
jason.oberling@LIGO.ORG - 11:33, Monday 19 May 2025 (84461)ISC, OpsInfo

This is a reminder that whenever the PMC is unlocked, especially for an extended period of time, the FSS and ISS should also be disengaged; otherwise, the respective autolockers will continue to try to engage these systems despite not having the means to do so (because they have no light, since the PMC is unlocked).  If there are ever any questions as to how to properly and safely disengage the PSL stabilization systems, CONTACT ME.  It does not matter if I'm offsite for any reason (RDO, vacation, sick, etc.).

From the 10-day trends Ryan posted this morning, neither the ISS nor the FSS were properly disengaged, so were left trying to lock all weekend.  For the FSS see the plot H1:PSL-FSS_NPRO_XTALTEMP in this set of plots.  It's clear from this plot that the FSS autolocker was doing a temperature search while trying to lock the RefCav, which means the NPRO PZT was also ramping.  Since there was no light in the FSS path the RefCav could not lock, so the search continued all weekend.

For the ISS, see the plot H1:PSL-ISS_DIFFRACTION_AVG in this set of plots.  The ISS diffraction should be completely flat if it is off, but the series of downward spikes indicate the ISS was trying to lock and failing to do so, since there was no light on the ISS PDs (my guess is it kept lowering the diffraction percentage to try to increase light on the ISS PDs, and unlocking when the diffraction hit 0% to start the process again).  This can also be seen in the behavior of the PMC reflected power (1st attached picture), which was moving around substantially all weekend as the ISS was trying and failing to lock; can also see the ISS diffracted power moving between 0% and 40%.  A zoomed in portion is also attached, in which it's seen that the ISS diffraction was moving from zero to ~20% (but as high as 50%) in a roughly 15 second period; note the changes in PMC Refl during this time (the small spikes in PMC Trans are not the PMC trying to lock, it's small flashes of resonance as the temperature of the PMC changes combined with the FSS actuating on the laser frequency).

While not strictly necessary, it's good practice to also close the PSL external shutter if the stabilization systems are going to be disabled for an extended period.

I don't think that this will compromise the performance of the ISS or FSS, but this does represent unnecessary wear on the mechanical components that are the actuators for both of these stabilization subsystems.  I should have caught that the PSL was left in this state, but did not pay attention to the alog during my RDO weekend and therefore did not catch this.  For this I apologize.

Images attached to this comment
H1 ISC
elenna.capote@LIGO.ORG - posted 17:26, Friday 16 May 2025 (84445)
Final ISC checks in HAM1 complete

Sheila and I went into HAM1 today to do a few last things:

From ISC perspective, we are good to go for doors and pumpdown.

H1 General (Laser Safety, Laser Transition)
anthony.sanchez@LIGO.ORG - posted 17:06, Friday 16 May 2025 (84443)
LVEA is now LASER SAFE.

Sheila, has Transitioned the LVEA back to LASER SAFE.

H1 General (SUS)
oli.patane@LIGO.ORG - posted 16:30, Friday 16 May 2025 - last comment - 17:06, Friday 16 May 2025(84440)
Ops Day Shift End

TITLE: 05/16 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:

Work is ongoing in HAM1 to finish up all the checks we need done before doors go on next week.

The RM/PM damping issues that we've been seeing (84427) are most likely due to the higher purge air in HAM1 since they had been working fine two days ago when the purge air had been turned way down, and yesterday and today when the purge air had been turned up, were not working. We'll be able to better confirm this on Monday during a time when we can have the purge air very low and there isn't any activity happening in HAM1. RM1, RM2, and PM1 have been put into SAFE for the weekend.

The LVEA is currently LASER HAZARD.

Sensor correction is on in the LVEA (SEI_ENV: LIGHT_MAINTENANCE_WINDY and SEI_CONF: NOBRSXY_WINDY).
LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:52 FAC Kim LVEA YES Tech clean 15:40
15:28 ISC Sheila LVEA YES Transitioning to laser hazard 15:42
15:28 VAC Jordan LVEA YES Purge air checks 15:44
16:01 ISC Sheila LVEA YES Turning off a sideband 16:08
16:36 ISC Marc, Sheila LVEA YES Turning on HV for HAM6 16:41
16:37 VAC Janos LVEA YES Checking things 16:45
17:10 ISC Sheila LVEA YES Turning sidebands back on 17:26
17:53 ISC Sheila, Elenna LVEA YES Final beam checks in HAM1 20:13
20:04 SEI Michael, Shoshana EY n Minor wiring on BRS 20:47
20:14 VAC Jordan MX n Vacuum measurements 21:46
20:47 PEM Robert LVEA YES Looking for scattered light in HAM1 21:57
21:46 VAC Jordan LVEA YES Vacuum measurements 21:57
21:55 TCS Tony & Mitchel Mech room N Chiller water checks. 22:06
22:07 CDS Oli, Marc CER YES Checking out PM1 coil drivers 22:14
22:16 ASC Sheila & Elenna LVEA HAM1 Yes Final Beam Checks. ongoing
22:43 VAC Jordan LVEA YES Turning HAM1 purge air down 22:46
23:13 VAC Jordan LVEA YES Turning purge air back up 23:14
Comments related to this report
elenna.capote@LIGO.ORG - 17:06, Friday 16 May 2025 (84444)

Just adding a note:

As of the end of the day, Sheila and I have left the sidebands OFF, and the HAM6 high voltage ON (per WP #12545).

H1 General
anthony.sanchez@LIGO.ORG - posted 16:01, Friday 16 May 2025 (84439)
TCS Chiller Water Level Top-Off Weekly

Famis 27815 TCS Weekly Chiller Water Level Top-Off

DCC T2200289

 

H1 SEI
jim.warner@LIGO.ORG - posted 13:51, Friday 16 May 2025 (84436)
EX Wind Fence is about 1/3 done

We wrapped a little early today because of 20mph gusts, but we got most of the second set of scrim attached this morning. Still have to finish the top level wrap with the 3/16" wire and do the vertical  wrap on both ends. We'll pick it up next week, probably after doors go back on HAM1.

Images attached to this report
H1 ISC
daniel.sigg@LIGO.ORG - posted 13:31, Friday 16 May 2025 (84435)
Excess Noise in ISC Whitening Chassis

This alog summarizes the measurements done with an ISC whitening chassis that implements ISC whitening boards D1001530-v7 using a 9V battery at the input.

Several issues were found:

  1. Due to a BOM error resistors R15 and R21 were stuffed with 3kΩ thick film resistors instead of metal film. Plot 1 shows the output referred noise measure at test point TP1. The blue curve was measured with a grounded input, whereas the red curve was measured with a 9V battery at the input. The later clearly shows the flicker noise of a carbon film resistor at roughly 600nV/√ f.
  2. The power supply input of the whitening board eomploys 10µH series inductors. Together with the bypass capacitors this forms a resonant circuit near 10kHz which shows up as a noise peak in the plots. Plot 2 shows the output noise with no whitening engaged for the original board (blue curve), the board with fixed 3kΩ resistors (green), and with the power supply indcutors shorted out (red).
  3. The gain stages will generate excess noise when over driven. The whitening board employs 4 switchable gain stages with 24, 12, 6, and 3dB of gain, respectively. With 9V input both the 24 and 12dB stage are over driven with their ouput voltage limited by the power supply rails. This will in turn lead to a large differential input voltage at the inputs of the OpAmp which then triggers the protection diodes. The current is limited by the 300Ω resistors (R11) in series with the + input. Even so, it is safe to operate like this, it can generate execss noise as seen in Plot 3. The blue curve shows the output noise with the input grounded, whereas the red curve uses a 9V battery at the input. The green curve shows the noise of the SR785 and the battery alone.

Plot 4 shows the 9V input noise using the optional whitening stages. A whitening stage consist of a 1Hz zero and a 10Hz pole.
Plot 5 shows the same plot but with the 300Ω resistors removed, the 3kΩ resistors replaced with metal films, and the inductors at the power supply shorted out.
Plot 6 is an overlay of Plots 4 and 5.

Non-image files attached to this report
H1 ISC
jennifer.wright@LIGO.ORG - posted 10:33, Friday 16 May 2025 - last comment - 11:40, Tuesday 03 June 2025(84432)
OMC scans with SR3 heater on

Jennie W, Sheila, Elenna

 

In order to get data for mode-matching and for Elenna to get data to calibrate sideband heights we ran some mode scans after the SR3 heater was turned on last night.

16:55:24 UTC Carried out single bounce OMC scan at 10W PSL input with sensor correction on HAM6 on, high voltage on for PZT driver in HAM6, sidebands off , SRM mis-aligned, ITMY mis-aligned, DC 3 and 4 on, OMC ASC on.

Excitation freq changed to 0.005 Hz as the top peak of the TM00 mode looked squint so could have been saturating. Lowering this frequency prevented this.

Ref 15-17 corresponds to dcpd data, pzt exc signal, pzt2 dc monitor.

 

Then mis-aligned ITMX and aligned ITMY (Sheila had to re-align SR2 to centre on ASC-AS_C).

Measurement starts at 17:08:18 UTC.

Ref 18-20 corresponds to dcpd data, pzt exc signal, pzt2 dc monitor.

 

Traces saved in 20250516_OMC_scan.xml. The top left plot is the first scan bouncing beam off ITMX, the second scan is the bottom right bouncing off ITMY.

The top right is the two plots of the PZT2 DC voltage monitor. That is, the current voltage applied to the PZT. The bottom left is the plot of the voltage ramp applied to the PZT2 on the OMC for this measurement.

 

The ndscope attached shows the power in mA transmitted through the OMC on the top, then the PZT used for the scan DC voltage underneath, then the input PZT voltage underneath that, then the reflected power from the OMC in mW, then at the bottom the SR3 heater element temperature in degrees.

 

Elenna did two more scans in single bounce with sidebands back on and different modulations depths in each.

Images attached to this report
Comments related to this report
jennifer.wright@LIGO.ORG - 10:38, Friday 16 May 2025 (84433)

See Elenna's comment on her previous measurement where this saturation happened.

Turn off the sidebands - instructions in this alog.

elenna.capote@LIGO.ORG - 16:51, Friday 16 May 2025 (84441)

Sheila and I ran one more OMC scan with sidebands off after OM2 heated up. Attached is the screenshot with scans off both ITMX and ITMY, data is saved in [userapp]/omc/h1/templates/OMC_scan_single_bounce_sidebands_off.xml

 

Images attached to this comment
elenna.capote@LIGO.ORG - 17:02, Friday 16 May 2025 (84442)

I also ran two OMC scans, single bounce off ITMY, 10 W input, with the sidebands ON. One measurement I ran with the sidebands set to 23 dBm and 27 dBm (9 and 45 MHz) and another set to 20 dBm and 21 dBm (9 and 45 MHz). I will use these measurements to calibrate the modulation depth. Data saved in /opt/rtcds/userapps/release/omc/h1/templates/OMC_scan_single_bounce_RF_cal.xml

SR3 heater was on for this measurement but it should have little effect on my results.

camilla.compton@LIGO.ORG - 11:40, Tuesday 03 June 2025 (84749)

Looked closer at these HWS signals during SR3 heater heat up and cool down. In all these plots, the two t-cursors are used as the reference and shown HWS live image.

  • Heat up plot attached
  • Cool down plot attached (ITMX was misaligned so there's no HWS data)

Some strange things:

  • ITMX heat up ndscope spherical power looks the opposite direction of ITMY, this isn't physical. Looking at the HWS Live plot, this isn't really want's happening, it appears that the SR3 signal just appears if the edge of ITMX is heating up so the center that the calculations are made from isn't correct, making the calculated spherical power wrong.
  • In both the heat up and cool down of the ITMY signal, there appears to be two steps with a flat region in the middle. Looking at the the flat region only, attached, it appears that the spherical power is continuing to change in the expected direction, unsure why this change isn't shown in the calculated spherical power.
Images attached to this comment
LHO VE
david.barker@LIGO.ORG - posted 10:11, Friday 16 May 2025 (84431)
Fri CP1 Fill

Fri May 16 10:06:36 2025 INFO: Fill completed in 6min 33secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 SEI (SEI)
shoshana.apple@LIGO.ORG - posted 15:54, Monday 12 May 2025 - last comment - 15:04, Friday 16 May 2025(84366)
BRS ETMY Mass Adjuster Install
[Shoshana, Michael]

We've started preparing to install the BRS mass adjuster to the End-Y BRS. The plan is to follow the same procedure/same parts as the End-X install outlined in LIGO-T2400043 and SEI log 1886 (https://alog.ligo-la.caltech.edu/SEI/index.php?callRep=1886).
 We've taken apart the BRS and discovered that doesn't match the designs on the DCC. How the parts are arranged blocks access to where the pico-motor mount should attach, but we think we have a work around that should work.
The electronics/wiring of the BRS is as expected and we've finished all the wiring for the pico-motor so that it should attach to the feed through.
Assuming all goes well we plan on installing the mass adjuster parts and begin testin.
Images attached to this report
Comments related to this report
shoshana.apple@LIGO.ORG - 16:51, Tuesday 13 May 2025 (84379)SEI
[Shoshana, Michael]

We've managed to get all of the hardware/parts installed in and we've closed up the BRS chamber. We had to add an inch of shims beneath to motor mount in order to get it to fit/align properly, but otherwise there were only minor complications during installation. We've tested the pico-motor and the mass adjuster using the pico-motor driver that we brought from UW and both seem to work fine. 
For in air balancing, we left the new mass adjuster centered to increase range for future adjustments for when the BRS is pumped down and running, and tried to just stick to moving masses that are inaccessible when the BRS chamber is pumped down. We unfortunately reached the maximum range with the internal masses and had to slightly move the manual mass adjustment system (what is currently used to adjust the center of mass) from center, but that might be returned to center after we re-balance it when it's pumped down. Right now the resonance frequency looks to be around ~7mHz (around 130 second period) which is about the same as it was before Mass Adjuster installation, but we'll check again after the chamber has been pumped down.
Tomorrow we'll finish all of the wiring and electronics to hook up the pico-motor to the LIGO system. The plan is to pump down the BRS chamber tomorrow and re-balance and test the pico-motor some more.

The reference pattern has a higher intensity than expected and we aren't sure why. Right now our best guess is that the light source drifted slightly, and we'll look into it more tomorrow.


Images attached to this comment
jennifer.wright@LIGO.ORG - 13:36, Wednesday 14 May 2025 (84391)EPO

EPO tag for BRS pics

shoshana.apple@LIGO.ORG - 16:05, Thursday 15 May 2025 (84411)SEI
[Shoshana, Michael]

Pumped down the BRS chamber overnight and started the ion pump this morning and got it down to 1.9e-6 Torr before we left end End-X. We also wired up the picomotor to the LIGO picomotor controller system. It is hooked up to the 7th channel X-direction and we tested it out and were able to hear it spinning for both directions. The BRS's thermal insulation was reapplied the box closed and the temperature sensors and heating plate were all re-attached and plugged back in. The reference beam's intensity has gone down to be closer to normal somehow, so it doesn't seem to be anything to worry about
We might go back to End-Y one more time tomorrow to clean up the wiring and do a final check of the vacuum pressure.
We waited for the temperature to equilibrate a bit before balancing  because we were hoping that as the temperature rises it would drift back to center, but we ended up using the mass adjuster to try and balance it.
It looks like the + - wires for the damping were switched, meaning when the damping was on it would ring up the BRS. Fixed by changing a line in the BRS code[IF H1_ISI_GND_BRS_ETMY_CAPDRIVE>=0] by switching the [>=0] to [<=0] and switching [H1_ISI_GND_BRS_ETMY_CAPOUTL] and [H1_ISI_GND_BRS_ETMY_CAPOUTR], and [H1_ISI_GND_BRS_ETMY_RELAYL] and [H1_ISI_GND_BRS_ETMY_RELAYR]


FROM THE END-X INSTALL:
Coupling/decoupling move: 1.25k steps
Maximum: +-140k steps
Be careful: +-100k steps

NOTE: MOVING PICOMOTOR +(POSITIVE) DIRECTION TRANSLATES TO MOVING THE BRS UP

TOTAL MOVEMENT TODAY:+21k steps
shoshana.apple@LIGO.ORG - 11:49, Friday 16 May 2025 (84434)
Centered both ETMY and ETMX BRSs.
For ETMX net movement was +2200 steps, for ETMY net movement was -3200 steps.
For ETMX we saw that the DRIFTMON was moved by about ~3.27 counts per step, and ~2.3 counts per step for ETMY
shoshana.apple@LIGO.ORG - 13:55, Friday 16 May 2025 (84437)
Cleaned everything up for the ETMY BRS and relabeled all the wires. The final reading that we saw for the ion pump was 9.9e-7 Torr (186uA, 6950V) which seems about right. We left some extra mass adjuster parts with Jim just in case. 
michael.ross@LIGO.ORG - 15:04, Friday 16 May 2025 (84438)

Shoshana, Michael

We took tilt subtraction spectra as a final life check of the BRSs. Both BRSs appear to be in good working order and doing their jobs well.

Non-image files attached to this comment
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