Displaying reports 2341-2360 of 83068.Go to page Start 114 115 116 117 118 119 120 121 122 End
Reports until 16:29, Saturday 01 March 2025
LHO General
corey.gray@LIGO.ORG - posted 16:29, Saturday 01 March 2025 (83119)
Sat DAY Ops Summary

TITLE: 03/01 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Aligning
INCOMING OPERATOR: Tony
SHIFT SUMMARY:

It's a been a rough day on the locking front.

Microseism is high (the 2hrs when H1 was OBSERVING, you could definitely see alot of 0.12 - 0.15 Hz oscillations in many LSC, ASC, & SUS signals ndscopes).  

DRMI has not looked great (even after fresh alignments).  Not seeing many triggers for it and the flashes are as high as they have been.  Hoping this is also microseism-related.

Also had a return of the SRC noise during OFFLOAD DRMI ASC earlier in the day, but then it went away.
LOG:

LHO General
corey.gray@LIGO.ORG - posted 12:42, Saturday 01 March 2025 (83122)
Mid-Shift Status: Rough Waters Continue

Managed to get 1.75hrs of OBSERVING this morning, but then had a lockloss.  Acquisition is no easy either. DRMI & PRMI have not looked great after Initial Alignments (like they usually had been).  BUT, there is high secondary AND primary microseism for H1.  Will keep battling.  Did not get to run the Saturday Calibration, because H1 was not thermalized this morning (in the last 13hrs we have not had a thermalized H1).

Have had some PRMI offloading which has taken as long as 4-5min (don't recall it taking that long...with that said, this current lock offloaded PRMI in under 2min).

H1 ISC (OpsInfo)
corey.gray@LIGO.ORG - posted 10:56, Saturday 01 March 2025 (83121)
H1 Status: Struggles Continue And SRC Noise During OFFLOAD_DRMI_ASC Returns

H1 struggled last night/this morning--H1 was down close to 6hrs (NOTE:  µseism is elevated). 

Since there hadn't been an alignment, thought this would do the trick since one hadn't been run a few hours into relocking.  Unfortunately, DRMI & PRMI didn't look great post-IA.  CHECK MICH FRINGES helped.  Then continued with locking with various locklosses.  During locking I happened to notice a RETURN of the SRC noise during OFFLOAD_DRMI_ASC (noted: alog83080, alog82997).  This is post-SRC2_Pitch gain reduction a couple days ago (alog83092, alog83078).

This noise issue definitely looks ugly and continues to exhibit SRM/SR2 Saturations heard via Verbal and for the one for this current lock it eventually calmed down on its own after a few minutes (this was around 1732utc).  While waiting for H1 to get to OBSERVING, looked to see if we if there were other instances of this noise returning (atleast for the last 1.5 days).  Here were the times when it occurred with the lower SRC2_P gain of 40 for ISC_LOCK state -111 (w/ notes for each one; also see attachments):

Perhaps it's getting worse?  Also only had the one lockloss from looking at these for the last 1.5 days.

Images attached to this report
LHO VE
david.barker@LIGO.ORG - posted 10:22, Saturday 01 March 2025 (83120)
Sat CP1 Fill

Sat Mar 01 10:12:29 2025 INFO: Fill completed in 12min 26secs

Delta time channels now continue post-fill showing the max-delta values attained, which for today is about 85C with the trip set to 50C. The Delta values are absolute, so the rise in TC temps appears as a second hump in the 30S lookback channels.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 07:54, Saturday 01 March 2025 (83118)
Sat DAY Ops Transition

TITLE: 03/01 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 5mph Gusts, 3mph 3min avg
    Primary useism: 0.11 μm/s
    Secondary useism: 0.81 μm/s
QUICK SUMMARY:

Walked in to see H1 down, after figuring out what was going on (ISC_LOCK was stalled due to H1 Manager), and seeing that H1 hasn't had an alignment for a few hours, started an alignment a few minuts ago (feels like H1 has been requiring an alignment after locklosses the last few weeks).  Alignment is almost done.

Primary microseism took a small quick stepup betwen 21-1utc, and secondary microseism returned to being above the 95th percentile since about 7utc.  Winds are calm.

H1 General
thomas.shaffer@LIGO.ORG - posted 06:37, Saturday 01 March 2025 (83117)
Ops Owl Update

H1 is trying to lock but things seem shaky. The primary useism has grown quite a bit in the last 12 hours and the secondary is peaking above1um/s. We've had a few higher state lock losses, not in the same place, and we've made it to NLN recently, so I think I'll just let it keep trying for now.

H1 General
anthony.sanchez@LIGO.ORG - posted 22:06, Friday 28 February 2025 (83116)
Friday Eve Shift Report.

TITLE: 03/01 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 151Mpc
INCOMING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 9mph Gusts, 5mph 3min avg
    Primary useism: 0.12 μm/s
    Secondary useism: 0.52 μm/s
SHIFT SUMMARY:
H1 has been locked for 8 hours and 14 minutes and Observing all shift.  I expect the Owl shift should be peaceful.
Everything seems to be running smoothly.

LOG:
                                                                                                                                                                                                                                    

Start Time System Name Location Lazer_Haz Task Time End
22:14 isc keita.siva optics.lab - iss pd array 01:03
22:24 ISC Matt, Mayank OpticsLab n ISS array 01:03

 

LHO General
corey.gray@LIGO.ORG - posted 16:34, Friday 28 February 2025 (83105)
Fri Ops DAY Shift Summary

TITLE: 02/28 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 143Mpc
INCOMING OPERATOR: Tony
SHIFT SUMMARY:

Decent shift with only one lockloss (whose recovery was straightforward but an initial alignment was needed due to usual ALSy shenanigans).  Also had a tour from a group from the VIT plant.
LOG:

H1 CDS
david.barker@LIGO.ORG - posted 16:33, Friday 28 February 2025 (83113)
Added critical camera marker on DIGIVIDEO Overview, expanded INFO to include switch port information

The digital camera MEDM main window now indicates which cameras are copied by the CDS_CA_COPY Guardian node and written to front end models. These are denoted by a blue tick at the left edge.

The camera.yaml file has been expanded to add how the camera is powered and which network-switch and switch-port the camera is connected to.

Images attached to this report
H1 General
anthony.sanchez@LIGO.ORG - posted 16:31, Friday 28 February 2025 (83114)
Friday Eve Shift Start

TITLE: 03/01 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 150Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
    SEI_ENV state: CALM
    Wind: 7mph Gusts, 3mph 3min avg
    Primary useism: 0.08 μm/s
    Secondary useism: 0.37 μm/s
QUICK SUMMARY:

LHO H1 has been locked for 2.5 hours.
The IFO seems to be running smoothly, with decent range.
The plan is to continue to Observe for the rest of the Evening & night,

 

H1 CDS
david.barker@LIGO.ORG - posted 12:33, Friday 28 February 2025 (83112)
VACSTAT detected BSC3 sensor glitch, restarted VACSTAT to clear

At 12:17:36 PST we had a sensor glitch on the BSC3 gauge, causing a VACSTAT alarm. This was another of the periodic glitches, the pressure stepped up from 3.2e-08 to 4.9e-08 for 4 seconds and then immediately stepped back.

vacstat_ioc.service was restarted at 12:26.

LHO FMCS
eric.otterman@LIGO.ORG - posted 10:46, Friday 28 February 2025 (83110)
End X chiller pump repair
I replaced the bad pump seal on the one of the chiller pumps at the End X chiller yard on 2/27. 
LHO VE
david.barker@LIGO.ORG - posted 10:46, Friday 28 February 2025 (83108)
Fri CP1 Fill

Fri Feb 28 10:06:02 2025 INFO: Fill completed in 5min 59secs

New code did not post-fill the ROC channels, I tracked this to a "calculated ROCs but didn't write to PVs" bug. Will test again tomorrow.

Images attached to this report
H1 PSL (PSL)
corey.gray@LIGO.ORG - posted 08:06, Friday 28 February 2025 (83106)
PSL Status Report (FAMIS #26366)

This is for FAMIS #26366.

Laser Status:
    NPRO output power is 1.85W
    AMP1 output power is 70.39W
    AMP2 output power is 140.0W
    NPRO watchdog is GREEN
    AMP1 watchdog is GREEN
    AMP2 watchdog is GREEN
    PDWD watchdog is GREEN

PMC:
    It has been locked 23 days, 19 hr 46 minutes
    Reflected power = 22.42W
    Transmitted power = 106.6W
    PowerSum = 129.0W

FSS:
    It has been locked for 0 days 1 hr and 21 min
    TPD[V] = 0.8066V

ISS:
    The diffracted power is around 3.4%
    Last saturation event was 0 days 3 hours and 1 minutes ago


Possible Issues: None reported

LHO General
corey.gray@LIGO.ORG - posted 07:46, Friday 28 February 2025 (83104)
Fri Ops Day Transition

TITLE: 02/28 Day Shift: 1530-0030 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Observing at 144Mpc
OUTGOING OPERATOR: TJ
CURRENT ENVIRONMENT:
    SEI_ENV state: USEISM
    Wind: 6mph Gusts, 4mph 3min avg
    Primary useism: 0.04 μm/s
    Secondary useism: 0.47 μm/s
QUICK SUMMARY:

H1 just recovered from a lockloss and has been in OBSERVING 10min.  Secondary microseism continues to come down, the last 24hrs, from peaking above the 95th percentile & winds are calm.

At 1533utc there was a Verbal for Wifi on in the LVEA, but see that it has been OFF the last hour.

ALSO:  Continue to have a note about limiting activity in the Optics Lab near the Fume Hood which had a termite nest--this is a message from the exterminator.

H1 General
ryan.crouch@LIGO.ORG - posted 22:00, Thursday 27 February 2025 (83101)
OPS Thursday EVE shift summary

TITLE: 02/28 Eve Shift: 0030-0600 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 149Mpc
INCOMING OPERATOR: TJ
SHIFT SUMMARY: 1 lockloss with an automated recovery with an IA. We've been locked for 2.5 hours.
LOG: No log

The SQZ PMC PZT voltage is reporting as low and has been dropping over the past 8 hours

 

Images attached to this report
H1 General (Lockloss)
ryan.crouch@LIGO.ORG - posted 17:55, Thursday 27 February 2025 - last comment - 21:08, Thursday 27 February 2025(83102)
01:53 UTC lockloss

01:53 UTC lockloss

Comments related to this report
ryan.crouch@LIGO.ORG - 21:08, Thursday 27 February 2025 (83103)

03:36 UTC observing

H1 ISC
keita.kawabe@LIGO.ORG - posted 18:07, Friday 10 June 2022 - last comment - 10:44, Friday 28 February 2025(63544)
HAM1 work on Friday (Ryan1, Craig, Georgia, Keita)

For mirror identification, see attached.

ASC-REFL_A replacement.

The new one is D1102004-V6 S/N 005 S1301248 (ICS ASSY-D1102002-001), the old one is S/N 012, S1301242.

With the old one, one of the differential output for DC4 segment failed and we've been using H1:ASC-REFL_A_DC_SEG4_GAIN=2 to compensate. With the new one, this didn't seem to be the case and we changed the digital gain to 1.

Daniel used the external RF injection ports to confirm that RF circuits are connected.

DC centering loops worked.

Beam dump relocation.

POP_air BDV reflection was hitting the corner of the V of the V-shaped beam dump.

ASC_REFL_A and ASC_REFL_B reflection were hitting the corner of the V of the V-shaped beam dump.

We moved these beam dumps so the beam hits one of the panels, not the corner.

We weren't able to see the LSC POP_A reflection. We might want to increase the power to 10W or so after everything is done so we can at least see the flashes.

We forgot to check the LSC REFL_A and REFL_B beam dumps.
Swapping the optic in M2.

This is one of the corner mirrors in the REFL in-vac path, and we swapped the HR with the 50:50. We made sure that the wedge orientation is correct (thinner edge is close to [+X, +Y]) For the 50:50 using the laser pointer. Since HR doesn't have any wedge, we had to manually adjust M2 to restore the REFL path.

The AOI of that optic is not accurately known but I eyeballed it to be 50 degrees, and based on that I measured the reflectivity of the 50:50 in the lab before installation (alog 63404). It was about 43% reflection at 50degrees, 35.6% at 55 degrees.

In situ, we got 41.1%, so AOI is probably a bit larger than 50 degrees.

We put a beam dump to catch the ghost beam of the new optic.

Power measurements, continued.

We're done. If we can carrier-lock PRMI we could do more, but we couldn't.

Looking at the direct reflection of PRM when IMC_PWR_IN=1.001W, the power between M5 (2" HR at [-X,-Y] corner downstream of RM2) and M6 (REFL LSC-ASC splitter) is 5.96mW after we swapped the optic.

At See Craig/Ryan's comments.

Clipping check in REFL path.

Nothing was clipping in the REFL path, but the beam was pretty high on M5 (that's the 2" HR at [-X, -Y] corner), M6 (ASC-LSC splitter), L1 (1" lens in front of LSC REFL sensors) and 2" lens on the WFS sled.

The beam height was ~105mm in front of M6 (see Georgia's picture), that's ~3.4mm higher than nominal, and the beam looks uncomfortably high on L1 because of the smaller aperture but it's not clipping.

We're leaving it as is because we don't want to touch the WFS sled and the only quick solution is to make the lens higher using a shim, then use M6 so steer the beam down on the LSC sensors.

Searching for the ghost beam of the main septum viewport.

The main PSL beam is reflected by the AR of the HAM1-HAM2 septum viewport and land inside the nozzle of the PSL-HAM1 viewport at around 4 or 5 o'clock position viewed from inside the chamber. See Georgia's pictures. We haven't done anything yet, we need help from people to assemble and install nozzle baffle.

Catching a snake.

That was big.

 

 

Images attached to this report
Comments related to this report
georgia.mansell@LIGO.ORG - 18:16, Friday 10 June 2022 (63545)

Some photos from today

1-3 Overhead shots on HAM1, including photo of slightly adjusted POPAIR beam diverter beam dump

4-6 The lens before the LSC_POP diode was dirty, before and after cleaning with a q-tip (for the large piece of dust) and puffer for the small dust.

7 IR viewer shot of the ghost beam from the AR surface of the newly installed M2, looks well dumped

8-9 Beam height and centering checks on the REFL path after swapping M2

10 The Snake!!! (Thanks to Gerardo for putting it out for us, and Keita for catching it so smoothly!!!)

11-12 The main beam and ghost beam on the HAM1 lightpipe viewport nozzle.

 

Images attached to this comment
keita.kawabe@LIGO.ORG - 09:42, Monday 13 June 2022 (63555)

It's hard to see from Georgia's picture 7 (shot through the IR viewer), but the beam dump to catch the ghost beam from 50:50 (M2) is to the -X direction of RM2, in front of one of the balance masses. See attached.

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 14:05, Tuesday 14 June 2022 (63583)EPO
Tagging EPO -- look at that SNAKE!!
corey.gray@LIGO.ORG - 10:44, Friday 28 February 2025 (83107)

For the new WFSA noted above (D1102004-V6 S/N 005 S1301248), I wanted to update the ICS  Assy Load to make more sense.  So the ICS Assembly Load link above no longer works, but the new one is now this: 

ASSY-D1102002-S1301248 

Just a note on these in-vac WFS:  The Body for these assemblies is D1102004 and it has its own s/n stamped on it from when it was machined.  However when a WFS Assy has its electronics installed, thus determining its operating frequency, and it is locked at this frequency because the WFS is then welded shut for in-vacuum install.  When this happens, the WFS (assembly really) is then assigned a new s/n (such as the DCC-generated serial number for the electrical innards of this WFS---S1301248 in this case).  I did not know this when I made this Assy Load, so I just picked a random s/n of 001---using the DCC s/n is a better and cleaner way to identify an installed-WFS assy.

H1 ISC (ISC)
keita.kawabe@LIGO.ORG - posted 15:57, Wednesday 01 June 2022 - last comment - 10:46, Friday 28 February 2025(63420)
In-lab test of spare 9-45MHz WFS (Jordan, Rich, Keita)

We tested a replacement in-vac WFS for 9MHz/45MHz (ICS ASSY load D1102002-001, S1301248) in preparation for the upcoming HAM1 vent (E2200228).

Rich will write about the details, but in short we have tested that the DC power supply current was good, DC responded as expected, and RF outputs made sense for 9MHz and 45MHz. We used screw-on type ISC AM laser head for this test.

Attached show the LOW (9MHz) and HIGH (45MHz) results measured using the network analyzer. In these pictures, reference trace (green) is Q3 and the live (yellow) is either Q2, Q1 or Q4. All in all these look good in that there's no reason to suspect that they aren't working as intended.

Minor detail is that there are differences not just in overall level because the beam is not centered on the diode and the beam is not circular either, but sometimes in the shape of the traces (for example look at the Q2 HIGH at around the shoulder of 45MHz peak). We've confirmed that both the level and the shape changed when Rich rotated the AM laser head. Don't know why the shape changes but Rich mentioned that the modulation might not uniform across the beam, or maybe we're somehow saturating something (but it didn't change much when we reduced the modulation current by 10dB w/o rotating the head).

Images attached to this report
Comments related to this report
rich.abbott@LIGO.ORG - 10:41, Thursday 02 June 2022 (63426)

Adding to what Keita and Jordan put in yesterday:

1.  We looked at the data from the S1301248 WFS that's going to be the replacement device to be installed into HAM1.  This was the original manufacturing data from when the head was built in 2014.

2.  We checked that the quiescent current draw was the same as that described in the data sheet for this part.  Saw 170mA and 240mA on positive and negative 18V rails respectively

3.  We verified that each DC path responded both to ambient light (in terms of magnitude and polarity), and the photocurrent produced by the laser calibrator head we use to check the response of ISC photodetectors.  The magnitude and polarity of the observed DC response was reasonable and confirms what Keita mentioned that the beam pattern coming out of the calibrator head is elliptic and offset slightly from the center of the four quadrants of the photodiode.  Rotating the calibrator head allows the user to verify all quadrants behave similarly.

4.  Using the calibrator head and a network analyzer, we were able to take the transfer function of each quadrant both 9.1 and 45.5MHz.  Each quadrant's response was reasonable when compared to identical functions of other quadrants.  We took the first quadrant we happened to measure and stored this to a reference trace on the network analyzer.  The remaining quadrants were then superimposed onto the reference trace to make a comparison.  While there are differences in the absolute amplitude of each trace (due to the elliptic nature of the calibrator head beam pattern), the overall shape of each trace was reasonable when compared to the other quadrants.

corey.gray@LIGO.ORG - 10:46, Friday 28 February 2025 (83109)

For the new WFSA noted above (D1102004-V6 S/N 005 S1301248), I wanted to update the ICS  Assy Load to make more sense.  So the ICS Assembly Load link above no longer works, but the new one is now this: 

ASSY-D1102002-S1301248 

Just a note on these in-vac WFS:  The Body for these assemblies is D1102004 and it has its own s/n stamped on it from when it was machined.  However when a WFS Assy has its electronics installed, thus determining its operating frequency, and it is locked at this frequency because the WFS is then welded shut for in-vacuum install.  When this happens, the WFS (assembly really) is then assigned a new s/n (such as the DCC-generated serial number for the electrical innards of this WFS---S1301248 in this case).  I did not know this when I made this Assy Load, so I just picked a random s/n of 001---using the DCC s/n is a better and cleaner way to identify an installed-WFS assy.

H1 ISC (ISC)
haocun.yu@LIGO.ORG - posted 15:02, Friday 22 July 2016 - last comment - 11:05, Friday 28 February 2025(28589)
Summary of WFS spec

I am working on the Noisebudget Model these days and made a summary of the WFS in use with calibrations:

WFS

Serial No.

RF Trans.

[Ω = V/A]

Responsivity

[A/W]

Demod. Gain

[dB]

Whit. Gain

[dB]

(40W)

ADC

[cts/V]

Digital Gain

Cal

[cts/W]

Freq.

Q1

Q2

Q3

Q4

AVE

REFL_A

S1301242

9 MHz

894

894

1069

974

958

0.85

21

21

1638

1

1.7E8

45 MHz

642

662

657

634

649

21

1

1.14E8

REFL_B

S1301243

9 MHz

822

873

742

861

824.5

0.85

21

21

1638

1

1.44E8

45 MHz

678

644

635

648

651

21

1

1.14E8

AS_A

S1300635

36 MHz

810

828

872

891

850

0.85

21

12

1638

1

5.3E7

45 MHz

707

718

732

766

731

3

1

1.6E7

AS_B

S1300634

36 MHz

846

904

826

832

852

0.85

21

15

1638

1

7.5E7

45 MHz

644

711

719

691

691

3

1

1.5E7

 

Calibration (from W to cts) = RF Trans. * ADC * Responsivity * Digital Gain * 10^(Demod. Gain + Whit. Gain)/20

Comments related to this report
corey.gray@LIGO.ORG - 11:05, Friday 28 February 2025 (83111)

Just a note for ASC WFS REFL_A:  S1301242 was swapped out in 2022 for S1301248.  See alog #63544.

Displaying reports 2341-2360 of 83068.Go to page Start 114 115 116 117 118 119 120 121 122 End