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Reports until 12:25, Tuesday 14 November 2017
H1 AOS
koji.arai@LIGO.ORG - posted 12:25, Tuesday 14 November 2017 - last comment - 18:41, Tuesday 14 November 2017(39418)
OFI pre-/post-adjustment performance test

[Gerardo, Koji]

As reported before [LHO ALOG 39359], we confirmed the disqualification of the installed OFI in terms of the optical isolation. The OFI was pulled out and place in the optics lab. [LHO ALOG 39366].

Yesterday, the optical performance of the OFI was tested without any adjustment and then after the performance optimization. The reasonable performance was recovered. It's hard to believe that we can keep this 43dB isolation forever under environmental fluctuations.

Next steps: Today, some of the measurement will be repeated for confirmation of the stability. In addition, a dry run of the in-situ isolation measurement will be done in the optics lab to pin down the reference numbers and accuracy/precision.

Here the detailed testing procedure can be found in E1700350.

  LHO OFI 2017/11/13
Before the adjustment
LHO OFI 2017/11/13
After the adjustment
Transmission
From the input port to the output port
0.973 +/- 0.002
(2.7% loss)
0.967 +/- 0.002
(3.3% loss)
Back-scatter isolation S-pol
From the input port to the squeezer port
1960 +/- 20 ppm 1300 +/- 10 ppm
TFP AR reflection
From the input port to the squeezer port
N/A 890 +/- 10 ppm
Isolation
From the output port to the input port
1800 +/- 200 ppm
( = 27.4 +/- 0.5 dB isolation)
52 +/- 13 ppm
( = 43 +/- 1 dB isolation)
Back-scattering
From the input port to the input port
2.3 +/- 0.4 ppm   3.0 +/- 0.5 ppm
Squeezer transmission
From the squeezer port to the input port
0.974 +/- 0.002
(2.6% loss)
0.978 +/- 0.002
(2.2% loss)

The transmission was checked with a Thorlabs power meter with an integrated sphere. The numbers were 0.972+/-0.004 and 0.971+/-0.006. But the systematics is large (+/-1%) everytime the number is measured.

Other OFI Performance to compare:
LLO OFI Performance summary [LLO ALOG 25788]
Previous LHO OFI measurement in the opt lab [LHO ALOG 39276]


What has been done:

- A noticeable thing was that the half-wave plate (HWP) was not tightly fastened in the holder. It is a notorious holder (Attached Pic) that the HWP can still jiggle in the holder even the screw is fastened with a normal torque. This was the issue the initial OFI of the LLO (actually... this unit). This time, the screw was fastened much tighter with an Allen key.

- Other alignment was basically fine. The angle of the thin film polarizer (TFP) was a bit tweaked to minimize the backscatter iso, but it seems that this is the minimum. This may mean that the isolation was optimized by sacrificing the polarization purity of the transmitted beam through the faraday rotator and half wave plate.

Images attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 12:48, Tuesday 14 November 2017 (39421)

Can you please note the temperature in the optics lab? Temperature changes of a few degrees will limit us to <40dB of isolation.

koji.arai@LIGO.ORG - 13:31, Tuesday 14 November 2017 (39424)

I don't have a thermometer right now. We will measure it.

koji.arai@LIGO.ORG - 18:41, Tuesday 14 November 2017 (39425)

Degradation of the isolation due to the temperature dependence of Verdet effect for TGG

When the isolation was optimized (< -40 dB), the backscatter isolation (S-pol of the transmission from FR+HWP) was 1300 ppm. Assume this was caused by the deviation of the rotation angle at the faraday rotator  from the nominal 45deg.

Backward beam
Faraday: phi_0 = 45 + delta [deg]
HWP: phi_H = 45 - delta [deg]
Total: phi_0 + phi_H = 90 [deg]

Forward beam
Total: phi_0 - phi_H = 2 delta

==> S-pol power: sin[2 delta/180*pi]^2 == 1300ppm
==> delta ~ 1deg

Temp dependence of the faraday rotation
FR had the rotation of 45deg + delta at T=298. According to JOSA B 9 (1992) 1912, the Verdet effect of TGG crystal has the temperature dependence of the follwoing form: phi = a (6751/T - 6.968) [deg]. a is a constant. T is the temperature in K. In our case, phi = phi_0 at T=298. This gives us a=2.935. ==> dphi/dT @T=298 = -0.223 [deg/K]
This will cause additional dphi = dphi/dT x dT rotation on the backward beam

Temp dependence of the isolation
So, the isolation is given by the following expression:
sin[dphi/180*pi]^2 = sin[-0.223 dT/180*pi]^2
This will hit 40dB (1e-4) at dT = 2.6 K and 30dB (1e-3) at dT= 8.1 K.

Temp dependence of the backscatter-isolation (and transmission)
This 2.6K deviation cause the backscatter isolation changing {+830ppm,-630ppm}.
For the 8.1K deviation, it changes {+3300ppm, -1300ppm}. The sign depends on the sign of delta.

To be checked:
- Temp dependence of the retardation of the half wave plate
- Temp dependence of the other optical parameters

gerardo.moreno@LIGO.ORG - 17:25, Tuesday 14 November 2017 (39433)PEM

Attached are the temperature trends from inside the optics lab (lab1 channel) and the vacuum prep lab (lab2 channel), data taken from the dust monitors.

Images attached to this comment
H1 SUS
betsy.weaver@LIGO.ORG - posted 11:13, Tuesday 14 November 2017 - last comment - 16:22, Tuesday 14 November 2017(39416)
PR3 and PR2 SUS fully suspended

This morning I relieved the PR3 of the mechanical rubbing Kissel pointed out in 39384.  The Front HR Upper Right stop was grounded on the face of the optic.   I also freed up the locked down PR2.  We'll run some TFs at lunch when IO is finished with the MC bypass install, but before alignment through the PR chain.

Comments related to this report
betsy.weaver@LIGO.ORG - 16:22, Tuesday 14 November 2017 (39432)

At lunch I took the needed TFs.  Both suspensions look healthy now according to the 6 DOF TFs (each) which can be found in the usual spot at:

/ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/PR2/SAGM1/Data/2017-11-14*.xml

and

/ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/PR3/SAGM1/Data/2017-11-14*.xml

H1 SEI
hugh.radkins@LIGO.ORG - posted 10:48, Tuesday 14 November 2017 (39414)
WHAM3 ISI Pretty well Balanced and relocked

We'd like to go back at this after IO completes today to consolidate and put viton under another table mass.  Otherwise we are pretty well balanced and have repeating locking.  The delta tilts on the table are +44.6urad in RX and +23.7urad in RY.  This delta is the difference from when we first locked the ISI after venting but before work commenced to the current repeatable locked position.  To compare, on HAM4 the deltas were -46 and +11urads.

H1 PSL
jason.oberling@LIGO.ORG - posted 10:45, Tuesday 14 November 2017 - last comment - 10:56, Tuesday 14 November 2017(39412)
PSL Weekly FAMIS Tasks (FAMIS 3676 & 8448)

This morning I completed the weekly PSL FAMIS tasks.

HPO Pump Diode Current Adjustment (FAMIS 8448)

I immediately noticed that something was off; the power reading for DB1 was around 83%, when it was > 86% when I finished last week.  That is a large decline over 7 days, so I trended the individual laser diodes of the diode box (1st attachment).  Something happened with Diode 3 of DB1 on November 10th.  The laser diode power was last adjusted on Nov. 7, and the increase can be seen in the attached trend.  After this though, the power for laser diode 3 began increasing, finally hitting some tipping point on Nov. 10th at ~17:41 UTC; at this point the diode laser dropped over the course of ~7 hours and stabilized.  The effect this had on the overall diode box power can be seen in the final plot of the attachment (H1:PSL-OSC_DB1_PWR).  It is unclear at this time what caused this behavior; investigation continues.

Continuing with the FAMIS task, I turned the ISS OFF and adjusted the operating current of the HPO DBs.  The results are summarized in the below table and a screenshot of the PSL Beckhoff main screen is attached for future reference.

  Operating Current (A)
Old New
DB1 51.6 51.9
DB2 54.0 54.1
DB3 54.0 54.1
DB4 54.0 54.1

I should note that in the last 2 weeks, I have had to increase the operating current of DB1 by 0.6 A (0.3 A per week).  This is a change from the usual 0.1-0.2 A weekly increase.  It should also be noted that all of the DBs were increase by 0.3 A last week.  The increase should remain roughly linear, and a departure from linearity can be an early indication of a failing DB.  I will continue to monitor this.

I also adjusted the operating temperatures of the HPO DBs, changes summarized in the below table.

  Operating Temperature (°C)
DB1 DB2 DB3 DB4
Old New Old New Old New Old New
D1 27.5 26.5 19.5 19.5 21.0 20.5 22.0 22.0
D2 27.5 26.5 19.0 19.0 25.0 24.5 19.5 19.5
D3 27.5 26.5 20.0 20.0 25.0 24.5 21.0 21.0
D4 27.5 26.5 18.0 18.0 22.0 21.5 19.5 19.5
D5 27.5 26.5 18.0 18.0 26.0 25.5 21.5 21.5
D6 27.5 26.5 18.5 18.5 20.5 20.0 21.5 21.5
D7 27.5 26.5 19.0 19.0 21.5 21.0 21.5 21.5

Despite this, the HPO is still only outputting 154.1 W, down from the 155.0 W I left it at after last week's adjustment.  I will continue to keep an eye on DB1, and investigation into the DB1 diode #3 glitch discussed above will continue.  This completes FAMIS 8448.  The ISS is back ON.

PSL Power Watchdog Reset (FAMIS 3676)

I reset both PSL power watchdogs at 18:03 UTC (10:03 PST).  This completes FAMIS 3676.

Images attached to this report
Comments related to this report
jason.oberling@LIGO.ORG - 10:56, Tuesday 14 November 2017 (39415)

Attached are plots of the TEC voltage and operating temps for the individual diodes of DB1.  The short spikes early in the graphs are from my adjustments from last week (testing new operating temps to see if laser output power improved).  Interestingly enough, at the time of the power runaway for diode 3, the TEC voltage for that diode was also changing; this is not seen on any of the other 6 laser diodes in the DB.  At this same time, however, the operating temperature of the diode did not register a change.  Investigation continues.

Images attached to this comment
H1 PEM
jeffrey.bartlett@LIGO.ORG - posted 10:37, Tuesday 14 November 2017 (39413)
Monthly Dust Monitor Vacuum Pump Check (FAMIS #7518)
Check of dust monitor vacuum pumps on 11/13/17 showed: 

End-X - Opened up air bypass to adjust pressure to 15 in/Hg.

End-Y - No changes all within spec.

CS - Opened up bypass just a little to fine tune pressure to 15 in/Hg. Pump is getting a bit noisy and there is carbon dust buildup on the filter. These are signs of wear on the vanes, and a pending rebuild. Have the rebuild kit in stock. 
H1 SEI
arnaud.pele@LIGO.ORG - posted 21:50, Monday 13 November 2017 - last comment - 10:05, Tuesday 14 November 2017(39410)
earthquake and watchdogs

Following on the LHO recent watchdog upgrades (39392,39298) I was interested in seeing how the platforms and suspensions behaved during yesterday's earthquake (alog 36683).

At LHO, most platforms were already tripped when the earthquake happened (because of the vent, I suppose), except for the end stations, which did not fully trip during the earthquake, and were switched to the damping state instead (End-Y after the first wave peaked, and end-X after the second one). See figure 1.

At LLO, all platforms tripped, BSCs first, then HAMs when the large wave hit us, see figure 2.

It would be interesting to know how Sheila's sus guardian change helped keep the suspension damped at LHO (from the operators screen, all sus were green at the time of the eq, see screenshot from alog 36683).

Otherwise this is a positive first demonstration of the new sei watchdog scheme.

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 10:05, Tuesday 14 November 2017 (39411)

Thanks Arnaud.  

It looks like none of the suspensions tripped, so we didn't get a test of the SUS guardian change.  But it is nice to see that they did not trip, maybe the ISI watchdog changes helped.  

 

LHO VE
kyle.ryan@LIGO.ORG - posted 18:17, Monday 13 November 2017 (39409)
LVEA purge-air supply halted for maintenance
The purge-air supply for the LVEA was shut down between 0900 - 1400 hrs. today for short notice maintenance.  As such, in-chamber activity was prevented for much of the day.  
LHO VE
kyle.ryan@LIGO.ORG - posted 18:07, Monday 13 November 2017 (39407)
Replaced 12"CFF-ISO adapter on CP1's 10" gate valve
Chandra R., Kyle R., Rakesh K.  

Today we replaced the 12"CFF-ISO adapter mounted to CP1's 10" gate valve (in closed position since 1998) with a 12"CFF x 8"CFF x 4.5"CFF x 2.75"CFF reducing cross.  

Last week, during our initial preparation for leak testing the vacuum volume bound between GV5 and GV6, i.e. CP1 plus misc. flanges, we had tightened the 10" gate valve (1/2 turn) and noticed a pressure response on PT114B. This observation, combined with the fact that this volume had been helium leak tested in the past without finding any external air leaks, caused us to suspect that the blanked-off adapter volume could be at a relatively high pressure and may have been acting as a "virtual leak" across the inadequately closed gate valve for the past 20 years.  To test this theory, we "cracked" open the ISO blank so as to allow some room air into the adapter volume.  In doing so, we did not perceive that any air back-filled into the adapter.  Rather, it seemed as if the adapter was already at atmosphere.  However, there may have been a slight pressure increase in PT114B when we did this (see attached graph).  

The pressure response of PT114B seems counter-intuitive but is not unprecedented.  The as found adapter volume may have been less than an atmosphere and back-filled in a small amount of room air (noisy work area, may not have heard this) and thus increased the leak rate(?).  This would explain the small "bump" in pressure.  Following this by then pumping the newly installed reducing cross would have significantly reduced the closing force experienced by the gate which could then have resulted in more gas making it across the closed gate(?) 

We will continue tomorrow.  For tonight, we are leaving the 10" valve closed and the reducer cross under vacuum. 
Non-image files attached to this report
H1 PSL (IOO, PSL)
cheryl.vorvick@LIGO.ORG - posted 17:37, Monday 13 November 2017 (39408)
PSL set to Science Mode

More info / changes needed to find an AC-ON-all-the-time stable temperature for the PSL.

Temperature range of the table sensors change with changes to the makeup air.

commissioning, 100% makeup air N: 72.6F to 73.9F S: 67.7F to 69.5F delta N: 1.3F delta S: 1.8F
commissioning, 40% makeup air N: 71.5F to 75.1F S: 69.4F to 72.3F delta N: 3.6F delta S: 2.9F

There's a way to see/set the temperatures that controls the AC unit coming on and turning off, and with the table temperature range changing with makeup air, I suspect these AC on/off temperatures are either not set or set to a wide range, and this could be a place where a change may allow for more PSL cooling options.

H1 SEI
hugh.radkins@LIGO.ORG - posted 16:42, Monday 13 November 2017 (39406)
WHAM 3 ISI is unlocked and unbalanced

We have used all the available balancing mass and need more.  We will bring more from the staging building and continue balancing in the morning.  Meanwhile, the ISI is unlocked and very unbalanced.  We will continue in the morning in an effort to at least get it reasonably lockable before we relinquish if not completely balanced before leaving it.

When we got started there was Baffle hardware to install and lots of cleanup.  As well, we marked the PR2 iris with an upside down dog-clamp and removed both irises.

LHO General
thomas.shaffer@LIGO.ORG - posted 16:10, Monday 13 November 2017 (39399)
Ops Day Shift Summary

TITLE: 11/13 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: Purge air work took up the morning, and then a few crews went in. MC2 and PR2 WD have tripped, but I will wait for the SEI crew to finish the balancing before someone (not me) untrips it. Film crew is out in the LVEA with Keita.
LOG:

H1 PSL
thomas.shaffer@LIGO.ORG - posted 09:25, Monday 13 November 2017 - last comment - 09:27, Monday 13 November 2017(39403)
PSL Weekly Report

Laser Status:
SysStat is good
Front End Power is 35.82W (should be around 30 W)
HPO Output Power is 153.0W
Front End Watch is GREEN
HPO Watch is GREEN

PMC:
It has been locked 0 days, 0 hr 2 minutes (should be days/weeks)
Reflected power = 22.43Watts
Transmitted power = 45.97Watts
PowerSum = 68.4Watts.

FSS:
It has been locked for 0 days 0 hr and 2 min (should be days/weeks)
TPD[V] = 1.931V (min 0.9V)

ISS:
The diffracted power is around 4.2% (should be 3-5%)
Last saturation event was 0 days 0 hours and 1 minutes ago (should be days/weeks)

Possible Issues:
PMC reflected power is high

Comments related to this report
thomas.shaffer@LIGO.ORG - 09:27, Monday 13 November 2017 (39404)

FAMIS7464 closed.

LHO General
thomas.shaffer@LIGO.ORG - posted 09:21, Monday 13 November 2017 (39402)
Monday 9am Vent Meeting Minutes

Notice: Purge air work this morning, no in chamber work till this has completed. Should be complete this afternoon.

BSC arm removal to happen this morning during the purge air work, cover will stay on.

Squeezer Bay will still be intermittent laser hazard.

IO - IMC bypass planned to go in this afternoon/tomorrow morning. MC2 & PR3 are rubbing and they will revisit, alignment looks good.

OFI still a wip in lab.

ITMX --> PR3 Aux beam still set up.

Hugh ready to balance HAM3 when time permits. Half a day, few hours is lucky.

TCS tables are still being worked on by Greg.

GV6 is still closed, leak checking has finished.

 

Tues. Maintenance:

Make sure to continue to do FAMIS tasks, and remember to close the task from the dropdown menu.

 

H1 PSL
edmond.merilh@LIGO.ORG - posted 08:43, Monday 13 November 2017 (39401)
PSL Weekly Report - 10 Day Trends FAMIS #6174

Trends all look normal for the most part. Temperature trends show an ongoing effort to stabilize for alignment work.

Images attached to this report
H1 PSL (IOO, PSL)
cheryl.vorvick@LIGO.ORG - posted 00:20, Monday 13 November 2017 - last comment - 09:46, Monday 13 November 2017(39396)
PSL TBLS and ACS look like they're switched

Looking into PSL temperatures, I started looking at the AC temperatures, and what I see is that the signals for TBLS and ACS appear to be switched.  Attachment shows from left to right:

Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 09:46, Monday 13 November 2017 (39405)CDS, DetChar, IOO, OpsInfo
Opened 
FRS Ticket 9425 to address temperature sensor channel swap problem.

FRS Ticket 9426 to address suspected problem with calibration of the north and south table temperature sensors (we can't believe a ~5 [deg F] between the two sensor exposed to the same air, ~15 ft apart.)
H1 CAL (CAL)
alexander.urban@LIGO.ORG - posted 14:15, Monday 18 September 2017 - last comment - 13:02, Tuesday 14 November 2017(38692)
Times switching from TX/RX PCAL channels for calibration

For the purpose of injecting PCAL lines, there are two channels that can be used: H1:CAL-PCALY_RX_PD_OUT_DQ (for reflected light) and H1:CAL-PCALY_TX_PD_OUT_DQ (for transmitted light). At various points during O2, we switched off between these two channels in C00 and C01 data at Livingston to account for things like PCAL clipping in the RX channel. The exact dates of each change are listed below, as documented on the filter configurations wiki page.

Version C00
Used RX from 116440990 (2016 Sep 14, 16:43:07 UTC) -- 1182618646 (2017 Jun 27, 17:10:28 UTC)
Used TX from 1182618646 (2017 Jun 27, 17:10:28 UTC) -- now

Version C01
Used RX from 1163173888 (2016 Nov 14, 15:51:11 UTC) -- 1181941760 (2017 Jun 19, 21:09:02 UTC)
Used TX from 1181941760 (2017 Jun 19, 21:09:02 UTC) -- now

The corresponding record over at Livingston is in aLOG 35948.

Comments related to this report
shivaraj.kandhasamy@LIGO.ORG - 13:02, Tuesday 14 November 2017 (39420)

Attached plot show the ratio of TX PD to RX PD during O2.  The size of deviations from one in that plot, when RX PD is used, indicates the systematic uncertainty introduced by the PCal clipping. The circled regions show the times when RX PD was used and the ratio was not close to one. The systematic uncertainties introduced by the clipping during those time is <3 %. This systematic would be reduced in the C02 frames. Each data point in that plot is running average of an hour of data. We plot data only during the observation times and with hoft ok state.

Images attached to this comment
Displaying reports 45421-45440 of 83725.Go to page Start 2268 2269 2270 2271 2272 2273 2274 2275 2276 End