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Reports until 23:51, Thursday 08 June 2017
H1 General
edmond.merilh@LIGO.ORG - posted 23:51, Thursday 08 June 2017 (36748)
Shift Summary - Eve

TITLE: 06/09 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 65Mpc
INCOMING OPERATOR:Patrick
SHIFT SUMMARY:

Quiet shift. There were a couple of small quakes that were of no consequence to H1. A2L was run towards the end of the shift as Livingston dropped their lock. Handing of locked/Observing H1 to Patrick. There was 1 RO alarm.
LOG:

23:10 Chandra to MY

23:23 Kyle called to inform me that he had driven past the barricade to the bunker with the pickup truck for gas cylinders.

23:25 Little Quake from around the Mariana Islands ~.05um

23:53 Chandra back

00:17 Wind is picking up in excess of 30mph over the last hour.

H1 General
edmond.merilh@LIGO.ORG - posted 23:22, Thursday 08 June 2017 (36747)
Running a2l - Livingstgon down

Attached are the before and after screen caps.

H1 back to Undisturbed @ 6:17UTC

Images attached to this report
H1 PSL (ISC)
koji.arai@LIGO.ORG - posted 18:29, Thursday 08 June 2017 - last comment - 15:11, Saturday 10 June 2017(36746)
ISS Out-of-loop stability comparison before/after the vent

Jenne and I reviewed the ISS status this morning. Jenne noticed that the RIN of the 2nd loop out-of-loop PD array shows increased coherence between 7~30Hz. I continued to investigate the comparison of the ISS state between now (6/8 19:00 UTC) and May 1st (5/1 1:00 UTC).

The 2nd loop out-of-loop floor level shows the stability of 1e-8 [1/rtHz] for both cases. However, the stability below 30Hz is worse than the one on May 1st. (Attachment 1. The blue curves are the current, and the red curves are the ones on May 1st.)

Attachment 2 shows the ISS QPD pointing. The yaw shows the shift from 0 to +0.3 while the pitch stayed ~-0.7. (Is that Okay?)

The 2nd loop PDs (inner/outer) exhibited 5~7% decrease, while the input power was also decreased 5%. So there looks some real decrease of the incident power on the PD exist. (Note tthat the QPD sum decreased -6.5%).

Can we change the features in the power spectrum by realigning the ISS PDs?

Images attached to this report
Comments related to this report
koji.arai@LIGO.ORG - 15:11, Saturday 10 June 2017 (36778)

Rick sent me a couple of reference alogs regarding the ISS QPD centering:
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=30915
https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=29583

It seems that the last ISS QPD centering was done on Oct 27, 2016. (Attachment 1)
I've checked the ISS QPD pointing since this last centering (Attachment 2). The pointing gradually drifted out from the center in the pitch diection during the first two months. There was no yaw drift. After the vent, there was no big change in pitch, but was in yaw.

I took the in-loop/out-of-loop spectra of the invac ISS array outputs right after the last centering (Attachment 3). The spectra were basically the same as the ones seen before the vent, and thus were better than the current level.

Because there was no intentional offset on the QPD pointing, we should try to center the beam on the ISS QPD (in the next possible occasion) to see if this helps to reduce the residual intensity noise at the low freq band.
 

Images attached to this comment
H1 SEI
edmond.merilh@LIGO.ORG - posted 16:50, Thursday 08 June 2017 (36743)
H1 ISI CPS Sensor Noise Spectra Check - Weekly FAMIS# 6901

Based on what I know about this spectra, I don't see any outliers worth mentioning. Everything looks nominally ok.

Images attached to this report
H1 PEM
robert.schofield@LIGO.ORG - posted 16:41, Thursday 08 June 2017 (36742)
No change in jitter features June 8 vs. May 1, coupling likely similar

The first figure shows the jitter peaks in DARM from last night and their coherence with PSL table accelerometers, along with the same plot from May 1. Little has changed.

The second figure is a reminder that the jitter is mainly driven by the chilled water flow to the HPO. The vibration from this flow didn’t change much between May 1 and June 8. However, it is greater than it was during O1. We might get significant improvement in DARM by turning down the flow to the specified minimum flow.

Because of the similarity in the jitter noise, Im guessing that only minimal PEM injections will be needed to characterize coupling in last night’s state before we continue commissioning and try to reduce jitter coupling.

Non-image files attached to this report
LHO General
corey.gray@LIGO.ORG - posted 16:16, Thursday 08 June 2017 (36724)
DAY Operator Summary

TITLE: 06/08 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: Ed
SHIFT SUMMARY:

Main push in the morning was to get our Nominal Low Noise H1 back into OBSERVING.  H1 is now back in O2.  Had one lockloss toward the end of the shift which was recovered fairly quickly.  Had a bit of wind earlier in the day (& we rode through that).
LOG:

H1 General
edmond.merilh@LIGO.ORG - posted 16:15, Thursday 08 June 2017 (36741)
Shift Transition - Eve

TITLE: 06/08 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing! at 66Mpc
OUTGOING OPERATOR: Corey
CURRENT ENVIRONMENT:
    Wind: 21mph Gusts, 15mph 5min avg
    Primary useism: 0.07 μm/s
    Secondary useism: 0.13 μm/s
QUICK SUMMARY:

 

H1 SEI
hugh.radkins@LIGO.ORG - posted 15:48, Thursday 08 June 2017 - last comment - 15:57, Thursday 08 June 2017(36739)
LHO LVEA Tilt Studies at Roam5--With wind from SW

Decent blast of wind today gave opportunity to assess the Roam5 position--I only moved there on Tuesday.

First plot shows the speed & direction for the CS and w/ Robert have learned the wind sensor has shifted out of position.  Don't know when but need to add about 90 degrees to reading.  Will fix Tuesday--FRS 8292.

The second plot shows the usual ASD and coherences between the ITMY and HAM5 (roamer) STS2s.  Roam5 position is getting pretty close to ITMY so no surprise that it is looking very similar.  While close, as previous positions have shown, no need to relocate the ITMY yet.  The quiet time in this measurement is 1000 utc 8 June; the windy period analyzed begins at 1700 utc 8 June.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 15:57, Thursday 08 June 2017 (36740)

Here is my roaming locations map.  The green bordered red disks with numbers are the locations.

Non-image files attached to this comment
LHO VE
chandra.romel@LIGO.ORG - posted 15:41, Thursday 08 June 2017 (36738)
Replaced IP9 power supply

One channel of IP9 power supply went bad on Wed. Swapped with same model - Varian dual vac - a used unit from IP6 (uses same CDS signal cables).

Closed WP 7024

Closed FRS 8289

H1 General
corey.gray@LIGO.ORG - posted 13:47, Thursday 08 June 2017 (36735)
SDF Diffs & ASC Excitation Needed To Be Cleared To Hit OBSERVE

Earlier this morning after the VEAs were swept, we had to go through a couple of other items before we could get back to OBSERVING:

1) DIAG_EXC

We had a stuck ASC Excitation channel (H1:ASC-INP1_P_EXC).  Dave confirmed this excitation was run briefly (seconds/minutes?) on Maintenance Day and has remained OFF ever since.  So Dave cleared this excitation test point and h1asc is no longer red on the CDS Overview.

2) DIAG_SDF (see attached screenshot of all diffs found this morning before they were addressed.)

We had handful of SDF Diffs in a few systems, but surprisingly not a whole lof of diffs.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 13:39, Thursday 08 June 2017 (36737)
Thurs 1pm Meeting Notes

Went over Past Tues Maintenance Open items

New Items for June 13th Maintenance (there was mention of possibly going over 4hrs)

  1. Power cables at end stations for beckhoff (Fil)
  2. Running pump CP3 MY dewar (kyle)
  3. Crane (no gate valve closing needed) lifting platform for diode box back to H2 PSL where it is stored (Peter)
  4. Move roaming seismometer (hugh)
  5. HAM6 ISI model change/update for connecting OMC SUS to HAM6ISI. No DAQ restart (hugh)
  6. PEM injections (Robert)

Closed meeting by going over work permits on the TV.

 

LHO VE
chandra.romel@LIGO.ORG - posted 13:39, Thursday 08 June 2017 (36736)
HAM 11 AIP

Vacuum staff is aware that annulus IP on HAM 11 is out of range again. Next Tuesday we will check it out. It failed recently but Kyle revived it with a tap. We may have a leak in the o-rings.

LHO VE
logbook/robot/script0.cds.ligo-wa.caltech.edu@LIGO.ORG - posted 12:10, Thursday 08 June 2017 (36734)
CP4 Autofill 2017_06_08
CP4 log file DOES NOT exist!
Images attached to this report
H1 General (OpsInfo)
corey.gray@LIGO.ORG - posted 11:45, Thursday 08 June 2017 (36733)
H1 Returning to O2 & Back to OBSERVING!

After getting Official OK from the LHO Run Coordinator (Keita Kawabe), and help with others to address a few tasks Keita wanted addressed, as of June 8th 18:40:06 UTC, H1 is now back to OBSERVING (H1 had been out of OBSERVING for a month & have now rejoined L1 in O2!).

LHO Operator Team:  Ops Observatory Mode Returns

This had been in PLANNED ENGINEERING for most of the last month.  Let's return to the habit of marking H1's Observatory Mode.

H1 General
keita.kawabe@LIGO.ORG - posted 11:43, Thursday 08 June 2017 (36732)
SDF before going into observing

ACCEPTed changes:

H1:SUS-ITMY_R0_OPTICALIGN_P_OFFSET (from -150 to -400), this is for HWS and ghost beam (alog 36264).

H1:LSC-PD_DOF_MTRX_SETTING_4_1 and 4_7 (from [0.0091, -849] to [0.035, 0]). These are for PRC input matrix (alog 36473).

H1:ALS-C_COMM_A_DEMOD_LONOM (from  19 to 12). Don't know why it was 19dBm, 12dBm sounds good to me.

H1:ALS-X_LASER_HEAD_NOISEEATERTOLERANCE (from 0.5 to 0.6), H1:ALS-X_REFL_SERVO_COMOFS (from 0.375 to 0.25). These were all changed during the X end investigation.

H1:ALS-Y_REFL_A_DEMOD_LONOM (from 20 to -100) and B_DEMOD_LONOM (from -100 to -9), we used to use channel A but at some point A was broken and we switched to B. Since then the board was swapped and both work but we still use channel B.

H1:ALS-Y_VCO_REFERENCENOM (from 21 to 20).

H1:ALS-X_QPD_A_YAW_OFFSET, H1:ASC-X_TR_A_PIT_OFFSET, H1:ALS-Y_QPD_A_PIT_OFFSET, H1:ALS-Y_QPD_A_YAW_OFFSET, H1:ASC-Y_TR_B_PIT_OFFSET and H1:ASC-Y_TR_B_YAW_OFFSET,  no real change, just the numerical error on the order of 1E-17.

REVERTed changes:

H1:ASL-X_FIBR_LOCK_TEMPERATURECONTROLS_HIGH and LOW were temporarily set to  +-1300 during the X end investigation, doesn't look like we need to keep it, reverted them back to +-600.

H1:ALS-Y_REFL_SERVO_IN2GAIN was set to 1, don't know why but inconsequential, reverted to 0.

 

 

H1 ISC
peter.king@LIGO.ORG - posted 11:27, Thursday 08 June 2017 (36731)
ALS X laser tuning coefficient
Measured the tuning coefficient of the laser crystal temperature for Prometheus S/N 2011B
(the one that was removed from EndX a week or so ago).

    The tuning coefficient is ~2.72 GHz/V for the green light and is fairly constant for
laser crystal temperatures from 24 degC to 34 degC.

    Increasing the laser crystal temperature decreases the laser frequency.  Increasing the
diode current also decreases the laser frequency.
LHO General
corey.gray@LIGO.ORG - posted 10:50, Thursday 08 June 2017 (36729)
LVEA & EX/EY VEAs SWEPT

On the Ops white board, there is a note of the last time the VEAs being swept on May 2nd.  

Jeff mentioned needing to unplug unneeded items at the End Stations, and I unplugged unused extension cords & phones. For the H1 PSL, I went through the checklist to confirm the room is in "Science Mode".  I assume we do not do this for H2 PSL because it running at 100%.

LHO VE
john.worden@LIGO.ORG - posted 00:40, Thursday 08 June 2017 - last comment - 10:44, Thursday 08 June 2017(36715)
CP4 level control coming back on line.

Kyle, Gerardo, Chandra, John

CP4 liquid level control appears to be controlling normally now. The large dip in the red trace is likely due to warm gas in the liquid transfer line being pushed into the pump as the transfer line cools to liquid temperature. This means that the 20% setting was not enough to keep the transfer line cold. 

Blue is the control valve position.

The current setpoint is 96%.

 

It would be nice if DVWEB could provide up-to-the minute data.

Images attached to this report
Comments related to this report
john.worden@LIGO.ORG - 01:11, Thursday 08 June 2017 (36716)

Here is the MY chamber pressure for the last 28 hours as well as the liquid level for the same period. Pressure spike at 5 hours was due to the loss of the ion pump.

The large drops in liquid level are not real - they are due to human actions. The smaller drops to the 80 and 90% range are real and normal as the PID control takes over from manual settings.

Images attached to this comment
michael.zucker@LIGO.ORG - 04:03, Thursday 08 June 2017 (36718)

Amazing!

chandra.romel@LIGO.ORG - 07:04, Thursday 08 June 2017 (36720)

This is the result of applying GN2 pressure (40-100 psi) to the clogged sensing line for many days (vs hours that we had tried in the past). We think we melted the blockage with the relatively warm gas. Went through two bottles of GN2 with a few small leaks in fittings.

Happy to close out FRS 6875!

chandra.romel@LIGO.ORG - 10:44, Thursday 08 June 2017 (36728)

I lowered the %full set point to 92% and LLCV lower limit to 30% open since we think 20% warms the transfer line.

LHO FMCS
bubba.gateley@LIGO.ORG - posted 14:51, Friday 02 June 2017 - last comment - 17:01, Thursday 08 June 2017(36627)
REGULATOR REPAIRED
The faulty regulator which turned out to be only a bad o-ring in the regulator itself, has been repaired, reinstalled, and air is flowing again. I unlocked the valves with Chandra watching the vacuum screen in the control room.
While I was repairing the regulator, Kyle was ordering a couple of new regulators for spares. 

Chandra and I also replaced the check valves on the corner station instrument air compressor.
Comments related to this report
chandra.romel@LIGO.ORG - 17:01, Thursday 08 June 2017 (36745)

The regulator failed again the next day, so we replaced it with an odd ball spare. Awaiting order delivery of direct replacements.

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