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Reports until 18:20, Tuesday 04 June 2019
H1 ISC
sheila.dwyer@LIGO.ORG - posted 18:20, Tuesday 04 June 2019 (49662)
DRMI ASC work

Sheila, Jenne, Georgia

We took some time coming back from Tuesday maintence to work on our DRMI ASC, continuing the work we started on Friday 49586  We have been able to run all the DRMI ASC loops and offload them before doing the CARM offset reduction. 

LHO VE
kyle.ryan@LIGO.ORG - posted 18:10, Tuesday 04 June 2019 (49661)
Cored holes in VEA floor at Y-mid

Chris S., Gerardo M., Kyle R.

We used the HILTI core drill to core (4) ea. 1 1/8" x 6" holes in the LVEA floor at the Y-mid.  I then installed 2 of 4 threaded inserts but had a problem with the installation tool.  I'll fix the tool and finish installing the threaded inserts next Tuesday. 

These new threaded inserts are for anchoring the new turbo station which is scheduled for installation on 6/25. 

H1 CAL (CDS, DAQ, DetChar, ISC, OpsInfo)
jeffrey.kissel@LIGO.ORG - posted 16:29, Tuesday 04 June 2019 - last comment - 11:53, Thursday 20 June 2019(49658)
PCALX OFS Railed from Morning Beckhoff Restarts, Fixed Before Observation
J. Kissel

After restarting the front wall Main DELTAL EXTERNAL ASD figure of merit, I saw that PCALX did not show the expected high-frequency roaming line. A quick look at the PCALX overview, and it was easy to see that the optical follower servo (OFS, the intensity stabilization and linearization servo for PCAL) was railed. The main time-series trend on the overview, of the OFS PD -- H1:CAL-PCALX_OFS_PD_OUTMON -- was steady at -7.7 V, with no sign of the expected ~kHz oscillation. 

I trended back to find out when the OFS had railed, and it appears coincident with the Beckhoff restarts this morning at 15:06:46 UTC (08:06:46 PDT). The OFS PD went to zero then, and then a few minutes later (at 15:13:44 UTC, 08:13:44 PDT), after bouncing around between OFF and RAILED, it settled on RAILED.

I fixed this by turning OFF, then turning ON the OFS loop, i.e. toggling the orange H1:CAL-PCALX_OPTICALFOLLOWERSERVOENABLE "loop enable" switch next to the diagram of the loop -- also on the PCALX overview. I did so at 23:11:55 UTC (16:11:55 UTC), before we resumed any observation ready segments, so this has no permanent impact on that quality of data.

We should consider adding "check on the PCALs!!" to the recovery checklist after any maintenance day in which a Beckhoff restart has taken place.
We should also add "Restart the wall FOMs!" to the recovery checklist after any maintenance day in which a DAQ restart has taken place.
Such activities should be considered akin to a physical VEA sweep done at the close maintenance.
Comments related to this report
jason.oberling@LIGO.ORG - 11:53, Thursday 20 June 2019 (50092)

Now associated with FRS ticket 13113.  I also see there was a FRS ticket entered for a similar issue on PcalY back in 2017 (FRS ticket 8274).  Similar cause?

H1 General
edmond.merilh@LIGO.ORG - posted 16:04, Tuesday 04 June 2019 (49640)
Shift Summary - Day

TITLE: 06/04 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Commissioning
INCOMING OPERATOR: Cheryl
SHIFT SUMMARY:

Maintenance day went well. The remainder of the day was used by commissioners to work on adding and optimizing DRMI ASC loops.
LOG:

1515:01 GRBV alert

15:04 Lockloss - Sheila induced

15:16 Sheila out to optics lab or squeezer bay to look for beam profiler

15:17 Sensor correction turned off at end stations.

15:18 Chris taking pest control into LVEA

15:21 Kyile out to MY - WP 8226

15:24 Fil out to pull cable from HAM5/6 to CER - climbing on chambers

15:25 Niko and Driptha out to EY for PCal work

15:26 Fire System maintenance on site

15:34 Dave B turning off Fire Pump Cell Phone notices until noon

15:36 EY to LASER HAZARD

15:46 Chris and pest guys back

15:47 Richard out to LVEA HAM5/6 area

15:52 IMC_LOCK guardian is now OFFLINE and unmanaged at Dr Kissel's request.

15:55 Richard back

15:57 Dick out to LVEA and CER for measurements

15:58 Karen leaving EY

15:58 Vanessa out to LVEA

16:03 Karen out to MY

16:09 Amber called about tour coming to CR around 10:00ish

16:10 Christina out to LVEA

16:23 Hugh heading out to EY to tend wind Fence

16:30 Karen leaving MY

16:30 Coffey Refigeration coming through gate - Jeff Bartlett

16:31 Norco on site - dewar 71

16:40 Rick and Laurence out to EY

16:50 Betsy and Sheila out to LVEA

17:09 Norco on site(second load) _ dewar 77

17:12 Vanessa back and heading out to EX

17:32 Marc out

17:35 Richard out to roof

17:36 Pest control done

17:39 Gerardo out to LVEA

18:00 Tour into control room

18:10 Initial Alignment re-locking ALS

18:10 Kyle back from MY

18:13 Sensor correction re-engaged

18:17 Niko out to optics lab

18:22 Input Align - following ALS attention

18:51 Begin locking

18:55 Daniel and Patrick out to LVEA

20:17 Pep out to CER to move a magnetometer

20:22 Pep back

 

 

H1 CDS
david.barker@LIGO.ORG - posted 15:56, Tuesday 04 June 2019 - last comment - 22:34, Tuesday 04 June 2019(49657)
Integrated slow controls status and SDF on CDS Overview Screen

I'm not sure if this looks any better, but all the slow controls displays are now in one block, including buttons to open the SDF screens. Also the SDF diffs are now marked with a RED circle since guardian DIAG_SDF is monitoring these systems. Snippet is attached.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 22:34, Tuesday 04 June 2019 (49667)

Confirming that all SDF systems (fast and slow) are now using their OBSERVE.snap reference file.

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 15:54, Tuesday 04 June 2019 (49656)
HEPI Pump Controller SDF is now monitoring the complete set of EX set points

Dave, Hugh:

The h1hpipumpctrlsdf_monitor.req file I put together this morning was not complete. Hugh and I have extended it to include all the detailed PID settings. I then restarted h1hpipumpctrlsdf and ACCEPT+MONITOR'ed all the new channels into h1hpipumpctrlsdf_OBSERVE.snap.

Attached screen shows the complete set of channels.

Images attached to this report
H1 CDS (CDS, PEM)
patrick.thomas@LIGO.ORG - posted 15:40, Tuesday 04 June 2019 - last comment - 16:48, Tuesday 04 June 2019(49653)
Corner station weather station moved to Vantage Pro 2
WP 8227

Daniel, Filiberto, Patrick, Richard

The code in PLC1 on h1ecatc1 was changed to use the Vantage Pro 2 library that I created prior. The weather station console was connected to port 2 (RS232 for channel 1) of an EP6002-0002 serial interface module. This module was named Corner MSR Weather and added to the end of the MSR Auxiliary device chain. A screenshot of the COM settings is attached.
Images attached to this report
Comments related to this report
patrick.thomas@LIGO.ORG - 16:48, Tuesday 04 June 2019 (49659)
Filiberto has added the wiring pin layout to the DCC as document D1900187.
H1 CDS (PEM)
filiberto.clara@LIGO.ORG - posted 15:38, Tuesday 04 June 2019 (49655)
CS Weather Station

FRS 9765

New Davis weather station installed in CS. Unit running on Beckhoff code. Old unit was removed.

F. Clara, R. McCarthy, P. Thomas

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 15:34, Tuesday 04 June 2019 (49654)
CDS Maintenance Summary, Tuesday 4th June 2019

WP8231 Remove h1calcs from OBSERVE SDF snap exception

Jeff, TJ, Ed, Dave

Actually the scope of this WP was extended to removing all SDF safe->OBSERVE transitions exceptions. The current exceptions were for h1calcs (it is unknown why this was) and most, but not all, slow controls systems (again, it is not known why).

h1calcs: Jeff has made both safe and OBSERVE symlinks to the h1calcs_safe.snap file. I removed this model from the exception list.

slow controls: I created a checker script (check_beckhoff_sdf) which 1) informs of any systems with different safe and observe references and 2) systems which do not start up in safe.

1) only h1hpipumpctrl had different safe and observe snaps, and its safe snap was incorrect. I made the two point to h1hpipumpctrlsdf_OBSERVE.snap and updated this file with the new Beckhoff setpoint channels for the EX system (CS and EY are still using Ben's Purple Box).

I restarted all the slow controls SDF systems on h1ecatmon0 to resync to the new start state and the changes Daniel made this morning.

The changes were made to the file /opt/rtcds/userapps/release/isc/h1/guardian/switch_SDF_source_files.py

Ed reloaded ISC_LOCK to get the new code.

WP8232 Guardian SQZ node channels in DAQ-DMT broadcaster

Dave:

I removed the not-needed GRD-SQZ channels and add the one which was needed to the broadcaster list:

-[H1:GRD-SQZ_BEATNOTE_OK]
-[H1:GRD-SQZ_SHG_OK]
+[H1:GRD-SQZ_MANAGER_OK]

This change went in when the DAQ was restarted.

Beckhoff Slow Controls Work

Daniel, Patrick, Dave:

New Beckhoff code resulted in six new INI files (C1PLC[1,4], X1PLC[1,2], Y1PLC[1,2]), the same list of autoburt.req and three new SDF monitor lists (C1PLC4, X1PLC2 and Y1PLC2).

The DAQ restart and SDF monitor restarts installed these.

DAQ Restart

Dave:

The DAQ was restarted for the above changes. To prevent out-of-band data showing up in EDC channels, I used my new DAQ restart procedure:

1 - generate the new H1EDC.ini file

2 - check the DAQ has no duplicate channels

3a - restart the DAQ at the appropriate time

3b - a few seconds later, after h1dc0 daqd has stopped, restart h1edc on h1susauxh34

This appears to have succeeded.

H1 SYS
jeffrey.bartlett@LIGO.ORG - posted 13:48, Tuesday 04 June 2019 (49650)
TCS Chiller Water Level Top-Off (FAMIS #11494)
   Both TCS chiller water levels are at the full mark. I did not add any water to either.  
H1 SUS (DetChar, ISC, OpsInfo)
jeffrey.kissel@LIGO.ORG - posted 13:14, Tuesday 04 June 2019 (49649)
Updates to Corner Station SUS Highest Bounce and Roll (V3 and R3) Filters: Only PRM, SR3, and BS Changed
J. Kissel, P. Covas

Part of the focus of Pep's current LSC fellowship was to continue work mitigating sharp features in DARM to help out the CW group's search sensitivity. Recently, he's suspected that features in the ~15-50 Hz region of DARM (and confirmed in PRCL and SRCL as well -- see LHO aLOG 48947) are corner station triple suspensions, predicted to have their highest frequency vertical (a.k.a "bounce") and roll modes (V3 and R3) in this region. As such, we've remeasured all of these suspensions' V3 and R3 mode frequencies, using this morning's maintenance period to complete the inventory -- see LHO aLOG 49643.

Armed with this inventory, we then perused all triple suspension notches for these mode frequencies. Below are the list of changes we've made based on our findings, and the expected features that the changes are expected to improve -- ranked by the hopeful amount of improvement.

SR3
    - [Attachment 1]Changed/fixed the frequencies of FM9 "SB27.7" and FM10 "SB45.3" elliptic bandstop filters in the M1 DAMP banks for every top mass DOF (L, T, V, R, P, Y).
     >> We expect this will reduce the 27.71 Hz feature in DARM.

PRM
    - Turned ON FM8 "SB27.5" and FM9 "SB40.9" elliptic band stop filters that were already there in the M1 DAMP banks for every top mass DOF (L, T, V, R, P, Y).
     >> We expect this will reduce 27.59 Hz and 40.87 Hz features in DARM.

BS
    - [Attachment 3] Added previously non-existent FM8 "SB17.79" and FM9 "SB26.06" elliptic band-stop filters in the M1 DAMP banks for every top mass DOF (L, T, V, R, P, Y).
    - [Attachment 2] Updated the frequencies of the FM5 "NotBR_BS" elliptic band-stop filter collection in the optical lever OLDAMP banks for P and Y.
     >> We expect these actions will help reduce the 17.79 and 26.06 Hz features in DARM.
    - [Attachment 4] Turned OFF FM2 "not19.1" and FM3 "not23.1" elliptic bandstop filters in the M3 ISCINF P and Y banks. These, we believe, are unneccessary -- intended to be temporary -- notch filters single-line oscillator excitations for exploratory ASC loop tuning. These were accpeted inthe SDF by Jeff Kissel back in Oct 2018 (see LHO aLOG 44277) during the height of commissioning, and were likely just accidentally left ON after a night of loop tuning.
    >> We expect this will claw back a bit of phase for the MICH ASC loops, but otherwise have little to no effect (other than cleaning up an unneeded mess.)
    - Changed the names of FM5 "NotBR_BS" and FM7 "NotBR_Quad" from their original ambiguous names "BounceRoll" and "EvanBR"
    >> We expect no change  in DARM from this change, just cleaning up the filter banks.

PR3
    - Moved FM2 "SB46.09" elliptic band stop filter in to FM10 (overwriting the unused, incorrect frequency filter that was there before) in M1 DAMP bank, in order to 
     >> We expect no change in DARM from this change, just making PR3's filter location consistent with every other SUS.

For all of the above changes, the new settings have been saved into both the safe.snap and OBSERVE.snap such that they stick.

MC2
    - [Attachment 5] We *looked* at the various implementations of notch filters for the highest bounce and roll modes (V3 and R3) for MC2 (and comparing against MC1 and MC3), but decided that the notches were well centered enough, and because we don't see any of MC2's resonances in DARM, we elected not to make any changes.

All other corner station suspensions have been confirmed to have correct notches for their newly re-measured highest bounce and roll (V3 and R3) modes. 
Images attached to this report
H1 ISC (SQZ)
filiberto.clara@LIGO.ORG - posted 12:44, Tuesday 04 June 2019 - last comment - 14:47, Tuesday 04 June 2019(49648)
SQZ Controls Chassis 3 Modified

WP 8229
ECR E1900035
E1600386

Following Beckhoff terminals were added to SQZ Controls Chassis 3:

1. EL9410 QTY 2
2. EL3104
3. EL4132
4. EL1124
5. EL2124

New DB25 cable was pulled from SQZ-C1 rack in the CER to SQZ-R1 rack in the LVEA. Part of the AM modulated AOM amplifier installation, alog 48353.

F. Clara, R. McCarthy, M. Pirello, D. Sigg

Comments related to this report
daniel.sigg@LIGO.ORG - 14:47, Tuesday 04 June 2019 (49652)

The new interface is mostly working:

  • The power readback is 10dB too low right now (requires software restart)
  • The modulation bias input has a gain of 1/20 rather than 1 (requires hardware swap)
  • Errors are not pushed upwards (requires software restart)

This will be fixed during next maintenance.

Here is the new medm screen for the AM-modulated AOM driver.

Images attached to this comment
H1 AOS
sheila.dwyer@LIGO.ORG - posted 11:18, Tuesday 04 June 2019 - last comment - 11:42, Thursday 20 June 2019(49645)
polarization controller hystoresis

Operators have been saying that they have difficulty adjusting the ALS polarizations lately.  I tried to adjust the Y fiber polarizaton today and saw the stange behavoir in the attached screenshot.  There are certain steps that are not like the others, and seem to make a large jump in the polarization. 

Images attached to this report
Comments related to this report
rahul.kumar@LIGO.ORG - 11:42, Thursday 20 June 2019 (50089)

FRS ticket 13111

https://services.ligo-la.caltech.edu/FRS/show_bug.cgi?id=13111

H1 SUS
pep.covas@LIGO.ORG - posted 10:37, Tuesday 04 June 2019 - last comment - 14:30, Tuesday 04 June 2019(49643)
Measurements of HSTS, HLTS and BSFM bounce/roll modes (expanded)

Pep Covas, Jeff Kissel

This is an update on past's week alog regarding bounce/roll measurements:

 

Optic Bounce mode [Hz] Roll mode [Hz]
SRM 27.45 40.88
SR2 27.50 40.91
SR3 27.71 45.32
PRM 27.59 40.87
PR2 27.41 40.94
PR3 28.21 46.09
MC1 27.39 40.81
MC2 27.74 40.91
MC3 27.42 --
BS 17.79 26.06

 

Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:30, Tuesday 04 June 2019 (49651)ISC, OpsInfo
Measurement technique:
- Using DTT, grab amplitude spectral densities of individual OSEMs on M2 and M3 stages (or only M2, or including Optical Levers, depending on which sensors the suspension has), e.g. 
     H1:SUS-${OPTIC}_${M2/M3}_OSEMINF_${OSEMDOF}_OUT_DQ
     H1:SUS-${OPTIC}_M3_OPLEV_${PIT/YAW}_OUT_DQ
- It is good practice and helpful to also grab an ASD of the excitation channel used below, treat it as an "A" channel, and plot the coherence as well.
While exploring for the given mode, use 5 exponential (aka "running") averages, with a 0.05 Hz frequency resolution. Once you've found the mode, increase the resolution to 0.01 or 0.005 Hz resolution, and measure for 5+ averages, depending on your patience and/or the amount of time you have.

- Using the COIL DRIVER Binary IO, switch the coil driver state to the highest possible range (State 2 -- ACQ ON, LP OFF for all of the above mentioned suspensions, and if need be, use the "secret" functionality to request State -2, and switch off all COILOUTF compensation filters).

- Using AWGGUI, excite an individual OSEM coil on the M2 stage, using a band-limited uniform noise excitation, where the frequency limits of the bands are ~1-2 Hz wide, centered around the expected frequency. We used a 4th order elliptic band-pass, with 1 dB ripple. One can typically drive amplitudes of 5e6 counts without saturating the DAC. Channels are of the form
    H1:SUS-${OPTIC}_M2_COILOUTF_${OSEMDOF}_EXC.

- Use the cursor in the DTT ASD template to find the resonant feature that results from your excitation. 

The above data was gathered at a 0.01 or 0.005 frequency resolution, so one should tried the numbers as though they have an uncertainty of f_res +/- 0.01Hz.

An example template is shown in the attachment (i.e. during the measurement of PR3's V3 mode), but all templates have been saved to:
    /ligo/svncommon/SusSVN/sus/trunk/${SUSTYPE}/H1/${OPTIC}/SAGM2/Data/YYYY-MM-DD_H1SUS${OPTIC}_M2*Search.xml


Note -- the only suspension mode for which we don't have an answer is H1 SUS MC3's Highest Roll Mode (R3). We tried several different excitations in order to find it, but turned up unsuccessful everytime:
    - Driving an M2 coil as described above (we tried UR), with band-limited uniform noise,
    - Driving all M2 coils in PITCH (via the M2_DRIVEALIGN_P2P_EXC channel), with band-limited uniform noise,
    - Driving all M2 coils in PITCH, with a swept sine excitation, and dense frequency vector between 39 and 42 Hz.
We tried the above both in the standard State 2 acquire filtering and also in the secret State -2 and the compensation filters off.
Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 08:38, Tuesday 04 June 2019 - last comment - 12:39, Tuesday 04 June 2019(49642)
bypassing fire pump cell phone alarms for this morning.

Due to maintenance work requiring the fire pumps to be operated, I've bypassed these cell phone alarms.

Bypass will expire:

Tue Jun  4 12:36:36 PDT 2019

For channel(s):

    H0:FMC-CS_FIRE_PUMP_1

    H0:FMC-CS_FIRE_PUMP_2

 

Comments related to this report
david.barker@LIGO.ORG - 12:39, Tuesday 04 June 2019 (49647)

Bypassed has expired, all cell phone alarms are now active.

H1 General
cheryl.vorvick@LIGO.ORG - posted 00:30, Tuesday 04 June 2019 - last comment - 18:02, Tuesday 04 June 2019(49633)
Range BLRMS results

I looked at 30 days of H1 range and the BLRMS channels, and found a clear increase in the frequency range 100-450Hz (H1:OAF-RANGE_BAND_5), and 400-420Hz (H1:OAF-RANGE_BAND_10).   I found 6 channels that have a clear decrease, and two channels that are either flat or jump around, making their contribution unclear with this first look.

PLOT 1: Increasing BLRMS:

PLOT 2: decreasing BLRMS:

PLOT 3: flat/variable BLRMS:

Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 11:51, Tuesday 04 June 2019 (49646)

Another thing that I thought of was PR3 potential drift, since the COMM beatnote looks like it's been getting a little lower over time.

In the attached plot I have the range as well as the COMM beatnote on the top row, and then the PR3 oplev and PR3 osems on the lower two rows.  The beatnote trace in orange is nearly impossible to interpret since the beatnote changes with alignment, and I haven't taken the time to plot only times when we're actually aligned, so nevermind.  But, the oplev and osems don't seem to show any dramatic drift (good, and expected that PR3 shouldn't really move a lot), and certainly they don't seem to correlate with the overall shape of the range.

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 18:02, Tuesday 04 June 2019 (49660)DetChar
@DetChar: Isn't this the kind of study for which LASSO was designed? My impression is that LASSO would do this more rigorously, providing mathematically confirmed correlation (as opposed to "by eye"). I understand that there's a LASSO summary page (e.g. LASSO:20190603), but as is often the case, we're interested in trends over much longer time-scales than a single day...
H1 ISC (ISC)
marc.pirello@LIGO.ORG - posted 14:15, Tuesday 02 April 2019 - last comment - 13:49, Tuesday 02 July 2019(48165)
Installed new v3 Baluns in CER

M. Pirello, D. Gustafson

We installed new v3 Baluns on the following signals in the CER:

ISC-C3(37-1) 40Mhz TCS AOM Return exchanged v1-117 with v3-S002

ISC-C3(33-4) 158.8Mhz Fiber Beat Note Return exchanged v1-193 with v3-S003

ISC-C3(33-5) 79.4Mhz SQZ VCO Return exchanged v1-151 with v3-S004

ISC-C3(33-6) 203.125MHz SQZ VCXO Return exchanged v1-052 with v3-S005

ISC-C4(39-3) 79.4MHz PSL VCO Return exchanged v1-093 with v3-S010

These are all return signals, the impact should be minimal.  Work was completed per WP8150

Balun status can be seen here E1900100.

Comments related to this report
marc.pirello@LIGO.ORG - 11:55, Tuesday 30 April 2019 (48873)

Continuing the Balun exchange program:

We installed new v3 Baluns on the following signals in the CER:

ISC-C4(39-1) 79.4MHz "ALS DIFF VCO Return" exchanged v1-102 with v3-S006

ISC-C4(39-2) 79.4MHz "ALS COMM VCO Return" exchanged v1-094 with v3-S068

ISC-C4(26-2) 45.5MHz "PEM Readback for Antenna Demod"  exchanged v1-055 with v3-S009

ISC-C4(19-8) 9.1MHz "PEM Readback for Antenna Demod" exchanged v1-147 with v3-S116

Work was completed per WP8190.  WP was modified to reduce impact to the IFO during this weeks maintenance, we did not touch squeezer.

Balun status can be seen here E1900100.

marc.pirello@LIGO.ORG - 15:26, Tuesday 07 May 2019 (49074)

Continuing the Balun exchange Program:

We installed new V3 baluns on the following 45MHz signals in the LVEA:

ISC-R1 (41-6) 45MHz Auxiliary Modulation (EOM Driver) exchanged v2-DG146 with v3-S152

ISC-R2 (41-2) 45MHz Distribution exchanged v2-DG083 with v3-S094

ISC-R3 (41-3) 45MHz Distribution exchanged v1-145 with v3-S117

Work was completed per WP8200, balun status can be seen here E1900100.

I have attached Insertion Loss and Leakage scans from the old baluns as well as the new ones.

Images attached to this comment
marc.pirello@LIGO.ORG - 12:10, Tuesday 21 May 2019 (49379)ISC

M. Pirello, D. Gustafson

Continuing the Balun exchange Program:

We installed new v3 baluns on the following signals at the PSL racks and at HAM6:

PSL-R2 (18-2) ISS AOM 80MHz exchanged DG-104 with v3-S069

ISC-R3 (41-2) Distribution 4th Harmonic exchanged v1-053 with v3-S160

ISC-R3 (41-4) Distribution 8th Harmonic exchanged v1-091 with v3-S040

ISC-R3 (39-4) Distribution 42.2MHz exchanged v1-125 with v3-S060

Work was completed per WP8215, balun status is in the same place it was last week, E1900100.

Attached is a comparision between the balun modified by hand (DG-104), and the new v3 balun which replaced it.

Images attached to this comment
marc.pirello@LIGO.ORG - 16:31, Tuesday 14 May 2019 (49243)

M. Pirello, P. King, D. Gustafson

Continuing the Balun exchange Program:

We installed new v3 baluns on the following signals at the PSL racks:

PSL-R2(17-1) FSS Modulation exchanged v1-043 with v3-S157

PSL-R2(17-2) FSS exchanged v1-014 with v3-S093

PSL-R2(17-4) PMC Modulation exchanged v1-021 with v3-S115

PSL-R2(17-5) PMC exchanged v1-050 with v3-S156

PSL-R2(17-6) Injection Locking exchanged v1-084 with v3-S095

ISC-R1(41-2) Distribution JAC Future exchanged v1-159 with v3-S092

** On the last one, the labels on the feed through may be more correct than the DCC.  I followed the cable path to the ALS VCO for the PSL.

If it is the ALS VCO, Peter told me that it is possibly 80MHz and in this case the difference between V1 and V3 is about 0.75dB more power, and no measurable difference in phase.  The PSL signals being under 45Mhz should be less than 1 degree difference in phase, and less than 0.25dB difference in power.

Work was completed per WP8208, balun status is in the same place it was last week, E1900100.

I have attached insertion loss and leakage scans of v1 vs v3 baluns.

Images attached to this comment
marc.pirello@LIGO.ORG - 13:54, Thursday 16 May 2019 (49283)

We checked the ISC-R1 (41-2) Balun and determined this signal is the REFL_B demod, 9MHz.  There should be very little phase & power difference between V1 and V3 baluns at this frequency.

marc.pirello@LIGO.ORG - 14:09, Tuesday 28 May 2019 (49507)

M. Pirello, D. Gustafson

Continuing the Balun exchange Program:

We installed new v3 baluns on the following signals at the end stations.

EX-ISC-C1 (41-5) Return PLL Beat Note 39.5MHz exchanged v1-176 with v3-S050

EX-ISC-C1 (41-6) Return ALS Laser VCO 79.4Mhz exchanged v1-049 with v3-S042

EX-ISC-R1 (41-1) ALS Laser VCO 71MHz exchanged v1-189 with v3-S114

EX-ISC-C1 (41-5) Return PLL Beat Note 39.5MHz exchanged v1-137 with v3-S041

EX-ISC-C1 (41-6) Return ALS Laser VCO 79.4Mhz exchanged v1-199 with v3-S155

EX-ISC-R1 (41-1) ALS Laser VCO 71MHz exchanged v1-039 with v3-S059

Work was completed per WP8222, balun status is in the same place it was last week, E1900100.

marc.pirello@LIGO.ORG - 11:14, Tuesday 04 June 2019 (49644)

M. Pirello, D. Gustafson

Continuing the Balun exchange Program:

We installed new v3 baluns on the following signals at the Squeezer

ISC-R3 (39-1) 80MHz SQZ EOM (OPO) exchanged v1-178 with v3-S082

ISC-R3 (39-2) 35.5MHz SQZ EOM (SHG) exchanged v1-060 with  v3-S089

ISC-R3 (39-3) 200MHz SQZ EOM (CLF) exchanged v1-166 with v3-S031

SQZ-R1 (41-1) 80MHz OPO Demodulation exchanged v-122 with v3-S084

SQZ-R1 (41-2) 35.5MHz SHG Demodulation exchanged v1-020 with v3-S033

SQZ-R1 (39-3) 71MHz SQZ VCO Laser Locking exchanged v1-190 with v3-S083

Work was completed per WP8230, balun status is in the same place it was last week, E1900100.

** The 200MHz SQZ EOM CLF signal may require a slight phase change, about 8 degrees difference and 2dB more power with the V3.

marc.pirello@LIGO.ORG - 14:09, Tuesday 11 June 2019 (49820)

M. Pirello, D. Gustafson

Continuing the Balun exchange Program:

We installed new v3 baluns on the following signals at the Squeezer and the PSL racks:

SQZ-R1 (41-3) 3.125MHz SQZ Angle Demodulation exchanged v1-171 with v3-S108

SQZ-R1 (41-4) 3.125MHz SQZ Angle Demodulation exchanged v1-145 with v3-S109

SQZ-R1 (41-5) 6.25MHz CLF Demodulation exchanged v1-183 with v3-S085

ISC-R1 (41-1) 71MHz Distribution exchanged DG-02 with v3-S086

ISC-R1 (41-3) 15th Harmonic Modulation exchanged DG-01 with v3-S058

TCS-MEZ (41-1) TCS exchanged v1-153 with v3-S079

Work was completed per WP8240, balun status is in the same place it was last week, E1900100.

 

marc.pirello@LIGO.ORG - 10:17, Tuesday 18 June 2019 (50025)

M. Pirello, D. Gustafson

Continuing the Balun exchange Program:

We installed new v3 baluns on the following signals at the field racks near the PSL:

ISC-R2 (41-1) 9MHz Distribution exchanged v1-047 with v3 S019

ISC-R2 (41-3) 2nd Harmnonic Distribution exchanged v1-098 with v3-S019

ISC-R2 (41-4) 3rd Harmonic Distribution exchanged v1-157 with v3-S015

ISC-R2 (41-5) 10th Harmonic Distribution exchanged v1-179 with v3-S016

ISC-R2 (41-6) 15th Harmonic Distribution exchanged v1-074 with v3-S132

ISC-R1 (41-4) 24MHz MC Distribution exchanged v1-040 with v3-S017

ISC-R1 (41-5) 9MHz Main Modulation exchanged v1-033 with v3-S018

Work was completed per WP8244, balun status located at this link: E1900100.  This concludes all "known" balun work at the corner station.  We are sprinting to next week where we intend to replace the remaining twelve v1 baluns at the end stations.

marc.pirello@LIGO.ORG - 16:15, Tuesday 25 June 2019 (50184)

M. Pirello, D. Gustafson

Continuing the Balun exchange Program, we installed new v3 baluns on the following signals at both end stations:

EX

ISC-R1 (41-2) 24.4MHz Modulation exchanged v1-022 with v3-S074

ISC-R1 (41-3) 24.4MHz Demodulation exchanged v1-184 with v3-S131

ISC-R1 (41-4) Not Connected exchanged v1-064 with v3-S078

ISC-R1 (39-1) 24.4 WFS A Demod exchanged v1-077 with v3-119

ISC-R1 (39-2) 24.4 WFS B Demode exchanged v1-026 with v3-S076

ISC-R1 (39-3) 71 CPS Timing Fanout exchanged v1-059 with v3-S020

EY

ISC-R1 (41-2) 24.4MHz Modulation exchanged v1-127 with v3-S073

ISC-R1 (41-3) 24.4MHz Demodulation exchanged v1-118 with v3-S011

ISC-R1 (41-4) Not Connected exchanged v1-013 with v3-S012

ISC-R1 (39-1) 24.4 WFS A Demod exchanged v1-126 with v3-S075

ISC-R1 (39-2) 24.4 WFS B Demod exchanged v1-161 with v3-S013

ISC-R1 (39-3) 71 CPS Timing Fanout exchanged v1-191 with v3-S135

Work was completed per WP8255, balun status located at this link: E1900100.  

** In the process of walking through the LVEA we found 4 more Baluns hidden among the TCS and SUS racks which need upgrading.  We were able to upgarde one of these with this Tuesday, and will finish the remainder next maintenance day.

SUS-R3 (40-1) CPS HAM 71MHz exchanged v1-011 with v3-S113

This additional work was started per WP8261

marc.pirello@LIGO.ORG - 13:49, Tuesday 02 July 2019 (50349)

M. Pirello, H. Radkins

The final three baluns were exchanged at the corner this morning for a total of 64 baluns replaced over 14 weeks.

TCS-R2 (41-1) 71Mhz CPS Timing exchanged v1-088 with v3-S144

TCS-R2 (41-2) N/A Empty signal with Balun exchanged v1-081 with v3-S001

TCS-R1 (41-6) TCS Signal from Mechanical Room exhcnaged v1-143 with v3-S045

All work finished per WP8261.  This completes work done per FRS9794 and ECR-E1700404 at LHO.

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