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Reports until 15:44, Tuesday 12 September 2017
H1 ISC (IOO, ISC)
corey.gray@LIGO.ORG - posted 15:44, Tuesday 12 September 2017 (38615)
IOT2L + ISCT6 Moved to Squeezer Bay; IOT2R Moved Out Of Way

(Apollo [Mark, Tyler], Corey, Daniel, Fil, Keita, Patrick)

This morning IOT2R (small table), IOT2L, & ISCT6 were prepped for being moved.  Prep work included:

Notes For IOT2L:

Notes For IOT2R: (smaller table)

Notes For ISCT6:

Images attached to this report
H1 IOO (IOO)
cheryl.vorvick@LIGO.ORG - posted 13:31, Tuesday 12 September 2017 (38612)
IMC beam position measurement on MC3

I measured the beam spot on MC3 yesterday, September 11, 2017, and found that it's +2.11mm in pitch, and -5.82mm in yaw.

Measurements from July 17, 2017, show similar results:  +2.26mm in pitch, and -5.84mm in yaw.

Above measurements are after the Montana 5.8M earthquake, and the measurement below is before.

Measurements from March 17, 2017, show: +2.16mm in pitch, and -5.70mm in yaw.

H1 ISC (ISC)
keita.kawabe@LIGO.ORG - posted 13:26, Tuesday 12 September 2017 (38614)
Loose things on ISCT6

OSA controller and red MHV to BNC cable -> ISC locker outside of the sqz bay.

OSA itself is on the table.

Thorlabs PD power supply, oscilloscope -> commissioning wire rack

ISCT6 LED power supply -> SQZ bay table

 

 

H1 PEM
jeffrey.bartlett@LIGO.ORG - posted 10:22, Tuesday 12 September 2017 (38613)
Install New DUst Monitors in LVEA

Installed 5 new dust monitors in the LVEA to support chamber openings. The LVEA dust monitors are located and named:

LVEA Dust Monitor Locations
Chamber Loc MEDM Loc #
HAM2 002
HAM3 003
HAM4 004
HAM5 005
HAM6 006
BSC1 010
BSC3 009

 

 

 

 

 

 

 

 

 

  

 

  

LHO VE
chandra.romel@LIGO.ORG - posted 09:02, Tuesday 12 September 2017 - last comment - 16:57, Tuesday 12 September 2017(38611)
corner station RGA filament on

9am local 

Turned on RGA filament at corner station. Will scan later. Beam tube GVs may be closed.

Comments related to this report
chandra.romel@LIGO.ORG - 16:57, Tuesday 12 September 2017 (38620)

Attached is scan and RGA settings.

Images attached to this comment
Non-image files attached to this comment
H1 AOS
peter.king@LIGO.ORG - posted 07:37, Tuesday 12 September 2017 (38610)
LVEA is LASER SAFE
The PSL and ALS shutters have been closed and locked out.

TCSX and TCSY lasers have been disabled.
H1 PEM
robert.schofield@LIGO.ORG - posted 02:50, Tuesday 12 September 2017 (38609)
Follow-up PEM injections

More follow-up studies, interferometer worked well, reports later. More to do but I think Ill let the last hours of the O2 IFO pass quietly. 

H1 ISC
sheila.dwyer@LIGO.ORG - posted 00:16, Tuesday 12 September 2017 - last comment - 14:49, Wednesday 20 September 2017(38608)
a couple more ESD measurements

I did a couple more measurements of the ESD actuation tonight.

1)I re-ran the script that allows us to measure 4 coefficicents for each test mass, (described in 38387).  Plots coming soon...

2) I measured Veff by driving the signal electrodes in length while we were locked and adjusting the bias voltage to minimize the coupling to DARM.  This can be checked against the results from the first measurement.  Veff = (beta-beta2)/2(gamma-alpha)

3) For some optics I also measured a different effective bias, by driving the bias path at 12 Hz and changing the offset in the bias path to minimize the coupling to DARM.  Veff 2= (beta+beta2)/2(alpha+gamma)

  Veff Veff 2 (driving bias)
ETMX -10.8  
ETMY 24.13 38
ITMX 122.4 -53.6
ITMY 95 54.8

Here I have written these as positive if the voltage requested out of the DAC is positive, although in reality there is a sign flip in some of the drivers (I will edit this entry in the morning with the correct sign).

Comments related to this report
sheila.dwyer@LIGO.ORG - 14:49, Wednesday 20 September 2017 (38723)

The signs are wrong for the ITMs in this table.  Multiply all ITM results by -1.

H1 SUS (CAL, DetChar, ISC, SUS, SYS, VE)
jeffrey.kissel@LIGO.ORG - posted 16:44, Monday 11 September 2017 (38604)
Charge Measurement Update; Confirmed results from Last week -- ETMY only half discharged; ETMX discharge, but as expected slowly recharging
J. Kissel

Charge measurements have been completed for today. ETMX remains at a low effective bias voltage, though the expected slow-and-steady charge accumulation has begun. ETMY, after last week's single-cycle TMDS discharge use (see LHO aLOG 38524), show consistent *reduced* effective bias voltage, but not nearly as well mitigated as on ETMX with a three cycle discharge. 

It's still most interesting that while ETMX's discharge has drastically reduced the (non-limiting) unexpected ISI ST2 to DARM coupling (see LHO aLOG 38507), ETMY's discharge appears to have reduced *the* mystery noise (LHO aLOG 38540), via unidentified coupling.

Just for ease of "one number reporting" I again take the mean of all pitch and yaw data points, and compute their standard deviation to form a ball-park uncertainty:
         2017-08-31     2017-09-08     2017-09-11    
ETMY      51+/-34        -21+/-12       -22+/-12 
ETMX      -4+/-3          -4+/-3         -4+/-2

Since we're replacing both ETMs in due time, I think we just don't care what the charge is beyond tomorrow, for the forseeable future.
   (a) We know that we can use the TMDS system to discharge an optic at vacuum in ~2 days
   (b) We know we can use the Bias voltage over a long time period to control / minimize the effective bias voltage
   (c) We now will be using conductive gloves in chamber, as well as plenty of dry-N2 gunning.
So may we just take this off our list of things to care about once Post O2 commissioning ceases until a pre-O3 detector begins to appear.

Thanks to T. Vo, T. Shaffer, and J. Warner for running measurements while I was out, see LHO aLOGs 38593 and 38576 for ETMX and ETMY respectively.
Images attached to this report
H1 IOO
keita.kawabe@LIGO.ORG - posted 16:18, Monday 11 September 2017 (38606)
Loose things removed from IOT2R

In preparation for IOT2R transport, I removed loose things from IOT2R.

Loose beam dumps were moved to the optics lab.

NPRO controller (S/N 406), an adjustable Faraday isolator from Drever lab, one wave plate (no ID), one 45 deg 99% splitter, one mirror (HR?, no ID), one cube (no ID), and two lenses (one is BICX-25.0-76.6-C, the other is without ID) were all moved to ISC cabinet in the sqz bay.

Two lexan viewport protection plates were moved from inside to the top of the table enclosure.

Everything else is still inside the table. Most notably, NPRO head and the cables.

H1 General
jim.warner@LIGO.ORG - posted 16:01, Monday 11 September 2017 (38605)
Shift Summary

TITLE: 09/11 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: Jim
SHIFT SUMMARY:
LOG:

15:30 Fil, Richard to LVEA for HAM4
15:30 Peter closing PSL shutter
16:15 TCS lasers turned off in software for HWS table move
16:30 HWS table is moved
18:00 Dave to EX replacing workstations, done 20:00
22:15 Kyle to EY

23:00 Peter unshutters PSL, locking starting

 

LHO VE
kyle.ryan@LIGO.ORG - posted 14:37, Monday 11 September 2017 (38602)
Isolated IP7 and IP8 from 2k Diagonal vacuum volume
Kyle, Gerardo 

We are going to remove IP7 and IP8 this week and send them off to be rebuilt.  We had planned on venting both ion pumps today and removing most of their flange bolts in preparation for removal tomorrow.  After we observed a sizeable leak accross IP7's isolation gate valve (see attached), we decided to leave it evacuated until we are set up to actually remove the pump.  We then can, and in a short period, install a zero-length reducer w/pump port valve in place of the ion pump which will then allow us to pump out to vented volume between the gate and zero-length reduecer and minimize the amount of "wet" air the Diagonal is exposed to.  

Note that the orientation of IP7's isolation gate valve is such that venting the pump side of the valve puts 15psi across the 10" diameter gate trying to force "open" the gate.  
Non-image files attached to this report
H1 SEI (CDS)
filiberto.clara@LIGO.ORG - posted 12:01, Monday 11 September 2017 - last comment - 14:32, Monday 11 September 2017(38601)
Newtonian Noise Sensors cabling

Most of the cabling for the Newtonian Noise array in the LVEA floor have been picked up. It is worth noting that the tape used left parts of the floors sticky. Cleaning crew has been made aware.

Comments related to this report
david.barker@LIGO.ORG - 14:32, Monday 11 September 2017 (38603)

I'm planning on leaving the h1ngn model in the DAQ for trending purposes until its second trends have expired. At that point we could harvest the model's dcu-id and core, and ngn data would be then available from NDS2 only.

H1 TCS (CDS)
filiberto.clara@LIGO.ORG - posted 10:59, Monday 11 September 2017 (38599)
HWS Table Enclosure Cabling Disconnected

The field cables to the HWS (TCSHT4R) enclosure have been disconnected. The TCS Sled Driver Chassis was powered off. See attached for cabling documentation.

F Clara, P. King, R. McCarthy

Non-image files attached to this report
H1 TCS (TCS)
peter.king@LIGO.ORG - posted 10:40, Monday 11 September 2017 (38598)
TCSX & TCSY controllers
Earlier it was suspected that the flow rate trip point for the TCSX laser was different from the TCSY laser
because of component value differences for the comparator setpoint voltage.  Both controllers have R115 = 4.87k,
R12 = 10.0k and R11 not stuffed.

    So the trip setpoints are the same and is not the reason for the difference.
H1 PSL
edmond.merilh@LIGO.ORG - posted 09:23, Monday 11 September 2017 (38597)
PSL Weekly Report - 10 Day Trends FAMIS #6165

Powers and ensuing temps reflect the weekly current increase. The PMC "creep" downward in trans is evident as is it's, inverse,  refl counterpart. I'm not sure what's going on with the chiller data having not spoken to those directly involved. I am confident due to the scheduled manifold work that these chiller conditions are being closely monitored by those directly involved.

Images attached to this report
H1 AOS
robert.schofield@LIGO.ORG - posted 08:33, Monday 11 September 2017 (38596)
PEM follow up injections

Got several hours of PEM follow-up injections last night. This is follow-up on findings in the first round https://dcc.ligo.org/DocDB/0144/G1701613/002/GenevaTalkSm.pdf. Work on identifying the high magnetic coupling in the output arm, the scattering in the input and output arms identified during PEM injections, whether there is significant scattering from the P-cal TX and RX ports and the source the high vibration coupling in the 600 Hz region of the BS. Partial progress, little time.

H1 SUS (ISC, SUS)
thomas.vo@LIGO.ORG - posted 19:47, Saturday 09 September 2017 - last comment - 11:17, Monday 11 September 2017(38591)
ITMY VIolin Mode Rang Up

Hang, TVo

We were locked for about 3 hours before the ITMY Vioilin Mode 5 rang up.  The mode rang up pretty steadily but we were only alerted to it about 30 seconds before it broke lock so we didn't have enough time to change the damping loop.

Upon re-locking, we stopped at ENGAGE_SRC_ASC to look at the status of the violin modes and it seems that the phase has shifted from what is set by the guardian and what is reported in the Violin Mode Wiki.  There were no earthquakes at the time so we couldn't find any obvious environmental reason for this shift.

Here is the summary of the change we made to the ITMY Violin Mode 5 Damping:

Before After
[FM1, FM3, FM4] = ON, GAIN = +200 [FM1, FM4] = ON, GAIN = -200    

Effectively, this shifts the phase by -120 degrees.  I'm not exactly sure if these settings are the nominal ones but it gets the job done.  When the mode was damped sufficiently at nominal low noise, I tried to go back to the "Before" configuration and could see it ringing up so I'm updating the guardian gen state to reflec the "After" configuration.

Comments related to this report
thomas.vo@LIGO.ORG - 11:17, Monday 11 September 2017 (38600)

Changed the violin mode wiki and committed the ISC_GEN_STATES to SVN.

H1 ISC (ISC)
thomas.vo@LIGO.ORG - posted 19:04, Wednesday 06 September 2017 - last comment - 17:11, Monday 11 September 2017(38540)
Back to NLN after ETMY Discharge

Patrick, Daniel, Hang, Sheila, TVo

We are back at NLN with a range of about 55 MPC.

Good news, it seems like the ETMY TMDS slightly lowered the noise floor in the 15-55 Hz band!

Attached is a spectra comparing a few different times, the first 3 are just to get a rough reference about what the noise floor was before the discharge measurement but after the Montana EQ.

It seems like ETMX discharge also helped a bit but it wasn't obvious unless you take on the order of hundreds of averages, this still doesn't reconcile all of the mystery noise but there is some progress.

Images attached to this report
Non-image files attached to this report
Comments related to this report
hang.yu@LIGO.ORG - 21:16, Wednesday 06 September 2017 (38541)

We also looked at the spectra before/after discharging with jitter noise removed. Instead of running Jenne's code with time-domain causal filters, we just did a rough freq domain subtraction. The results are attached.  

Images attached to this comment
sheila.dwyer@LIGO.ORG - 22:20, Wednesday 06 September 2017 (38544)

We'll try to check the calibration in the morning.

jeffrey.kissel@LIGO.ORG - 17:11, Monday 11 September 2017 (38607)
J. Kissel, S. Dwyer, T. Vo,

Just in case any one is mistrusting that the changes in actuation strength of the ETMY from discharging were not covered by the time-dependent correction factors (i.e. kappa_TST), we show a zoom of the ~35 Hz PCAL calibration line. The largest discrepancy between line heights is 5%, which is within the stated limit of uncertainty and systematic error for 68% confidence interval. So, no need to mistrust the calibration here. 

We've decided against making a full sweep given that we're so crunched for time on this last night with the O1-O2-like H1 interferometer. May we come back more sensitive than ever!
Images attached to this comment
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