Displaying reports 67481-67500 of 83122.Go to page Start 3371 3372 3373 3374 3375 3376 3377 3378 3379 End
Reports until 15:08, Wednesday 14 January 2015
H1 SUS (ISC, SYS)
jeffrey.kissel@LIGO.ORG - posted 15:08, Wednesday 14 January 2015 (16072)
H1 SUS ETM QUAD 'resg1' and '+12dB' damping filters now ON for both ETMs
J. Kissel, K. Izumi

Kiwamu is making sure the online calibration filtering (currently in the "OAF" model, will eventually be in the "CAL" model) is reasonably up-to-date. In doing so, we discovered that the two ETMs have different damping loop filters installed and ON. Most filter modules are as expected, according to the original, low noise, Level 2.1 quad design (see LGO aLOG 6760). However, in FM3 of the L and Y banks of both ETMX and ETMY, there are filters called "resg1" and "+12dB" respectively. They are ON only in ETMX.

After a little digging down memory lane, we recalled that in attempts to get ALS DIFF up and running last time (see e.g. LHO aLOG 15025), before we lost the arms, we had copied over LLO's damping filters' differences at the time -- described in detail in LHO aLOG 14959. However, as indicated in LHO aLOG 15037, having the filters constantly ON never got captured in any sort of configuration control, because ALS and LSC control was bouncing between using ETMX and ETMY depending on the functional-state and state-of-confusion for each test mass.

We have now turned both FM3's of L and Y filter banks ON, and changed the DAMP_STATE_?_GOOD state to match the current state with those ON. We have not yet captured a new safe.snap in this configuration, but we'll do so ASAP.

A note -- the ITMs do NOT have these "bonus" LLO filters installed, so FM3 is therefore OFF.
H1 General
jim.warner@LIGO.ORG - posted 14:10, Wednesday 14 January 2015 (16071)
Morning meeting minutes
Z/RZ seb ongoing
Changing CD at HAM3
Sus 3IFO storage
Recovery from RCG update ongoing
Schnupp measurements
Possible loose mirrors in REFL path in vaccuum
Opening X-arm gate valves, annulus ion pump needs to be repaired
Safety meeting this afternoon
Z/RZ on filtering on BSC-ISI testing ongoing
Changing coil drivers at HAM3 ISI
Sus 3IFO storage activities in the VLEA
Recovery from RCG update ongoing
Schnupp measurements ongoing
Possible loose mirrors in REFL path in vaccuum on HAM2
Opening X-arm gate valves, annulus ion pump on BSC3 needs to be repaired
Safety meeting this afternoon
 
H1 CDS
james.batch@LIGO.ORG - posted 13:24, Wednesday 14 January 2015 (16070)
Replaced projector lamp on left side projector
Replaced bad projector lamp on left side projector in control room.  

NOTE: The lamp socket internal to the projector has badly overheated and the plastic mount that holds the socket pins has lost it's integrity. If you smell smoke in the control room, this projector should be powered off.  This seems to be a common problem with these projectors.
H1 ISC
evan.hall@LIGO.ORG - posted 12:20, Wednesday 14 January 2015 (16068)
ISC rack patch panel

For the Schnupp asymmetry measurement, one of the patch panel connectors on ISC R1 (by the PSL) is now wired to another patch panel connector on ISC R3 (by HAM6). The wiring is as follows:

Initially, all these ports were labeled as "spare" and most of them were terminated.

The connector on ISC R1 will be driven by an rf signal from an IOT2R PD. The connector on ISC R3 will go into a spectrum analyzer.

H1 DAQ (CDS, ISC)
david.barker@LIGO.ORG - posted 12:09, Wednesday 14 January 2015 - last comment - 13:08, Wednesday 14 January 2015(16066)
DAQ restart of h1iscey model change

DAQ was restarted to sync up with temporary h1iscey model change which was applied in the last hour.

Comments related to this report
david.barker@LIGO.ORG - 13:08, Wednesday 14 January 2015 (16069)

restarted h1iscey model, looks like it wasn't started completely due to obsolete wiki restart instructions.

H1 PSL
edmond.merilh@LIGO.ORG - posted 11:16, Wednesday 14 January 2015 (16064)
PSL Diagnostic Breadboard Reports w/ISS RPN
Non-image files attached to this report
H1 SEI
keita.kawabe@LIGO.ORG - posted 10:00, Wednesday 14 January 2015 - last comment - 11:22, Wednesday 14 January 2015(16063)
Restoring HAM2 and HAM3 HEPI angle

We only restored PIT of HEPI2 (H1:HPI-HAM2_IPS_RY_SETPOINT_NOW) yesterday, but there was a change in ROLL (RX) on the order of 10 urad that was not restored, which might affect the input pointing.

Also, there was a jump in ROLL in HEPI3, again on the order of 10 urad, which would affect POP and ALS beam position on ISCT1 as well as POP sled in HAM3.

These DOFs were brought back to pre-maintenance levels.

I don't know/remember why, but it seems that a new set of angle setpoints is made for HEPI such that the system starts new with free-hanging position after each restart. Seems like this free hanging position changes over time.

Since any change in HEPI angle (RX, RY and RZ) on HAM2 and HAM3 would affect many things related to the alignment, most notably pointing references like IM4 transmission QPD and POP sled, it's a good idea to keep the set points unchanged over multiple restarts.

Comments related to this report
hugh.radkins@LIGO.ORG - 11:22, Wednesday 14 January 2015 (16065)

I've done a survey a of all the SEI Guardians with regard to the position dofs that are restored (maintained everytime.)

HAM_ISIs maintain every dof but the HAM_HEPIs only maintain the RZ dof.  I'd say this is backwards given the range and more importantly hysteresis of HEPI.

While at it, for the BSCs: their HEPIs all maintain the RZ dof, the ETMs maintain their pitch and the ITMY maintains pitch roll and X dof to deal with ACB install and Initial Alignment.  The BSC ISIs maintain NO dof.

It certainly makes sense to me that at least the HAM2 & HAM3 RX & RY dofs are also restored along with the RZ.  Don't know why we wouldn't do this with HAMs 4, 5 & 6 too.  The X Y & Z dofs are probably okay to let wander but commissioners can comment.

H1 CDS
cyrus.reed@LIGO.ORG - posted 09:41, Wednesday 14 January 2015 (16062)
Autoburt Maintenance
I noticed the autoburt VM was behind in patches, so I updated it and rebooted in between snapshot runs.  There should be no gaps in the autoburt coverage, though the next run may take longer as the embedded gateway re-caches the PV names.
H1 SEI
filiberto.clara@LIGO.ORG - posted 09:25, Wednesday 14 January 2015 (16061)
HAM3 - ISI Coil Drivers Replaced
Replaced the ISI Coil Drivers D0902744 for HAM3. This is a temporary swap to help with troubleshooting the 0.6Hz seen in HAM3.

Electronics removed:
S1103321 U24-U25
S1103358 U23-U22

Electronics Installed:
S1103316 U24-U25
S1103301 U23-U22
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:14, Wednesday 14 January 2015 (16060)
CDS model and DAQ restart report, Monday, Tuesday 12th,13th January 2015

model restarts logged for Mon 12/Jan/2015
2015_01_12 08:59 h1nds0
2015_01_12 10:49 h1hpietmx
2015_01_12 10:49 h1iopseiex
2015_01_12 10:49 h1isietmx

2015_01_12 13:41 h1fw0

two unexpected restarts. ADC replacement of h1seiex in preparation for RCG2.9 upgrade.

model restart for Tue 13/Jan/2015

in attached file. RCG2.9 upgrade required all systems to be restarted. Several later unexpected DAQ restarts of frame writers.

Non-image files attached to this report
H1 SUS
brett.shapiro@LIGO.ORG - posted 18:44, Tuesday 13 January 2015 - last comment - 20:29, Tuesday 13 January 2015(16057)
ETMX charge trend over 3.5 hours

Now that ETMX is back to vacuum, I measured a trend of the effective test mass charge voltage over 3.5 hours. The sensor was the oplev, since there is no cavity. I was told by Jeff K, who was told by Richard (or was it Kyle?) that the ion pump is valved out. The pressure was about 1.5e-6 torr, pumping with the turbo for about 2 days since the last vent.

 

The first pdf shows the charge seen the pitch and yaw oplev signals from excitation in each ESD quadrant. The second pdf shows the deviation from the average of each quadrant - oplev siignal pair, e.g. pitch from UL exc, etc. The largest deviation is -12 V. Most of the data is within +-10 V.

 

The charge measuring script is

/ligo/svncommon/SusSVN/sus/trunk/QUAD/Common/Scripts/ESD_UL_LL_UR_LR_charge_07-H1.py

The charge analysis script is

/ligo/svncommon/SusSVN/sus/trunk/QUAD/Common/Scripts/ESD_UL_LL_UR_LR_analysis07_H1.m

The charge trend script is

/ligo/svncommon/SusSVN/sus/trunk/QUAD/Common/Scripts/Long_Trend_H1.m

Non-image files attached to this report
Comments related to this report
john.worden@LIGO.ORG - 20:29, Tuesday 13 January 2015 (16059)

Yes, the ION pump is valved out. You can see on the EX Vacuum MEDM screen that IP12 is registering 4 decades better pressure than PT510. Therefore it is isolated from the BSC volume.

https://lhocds.ligo-wa.caltech.edu/screens/png/H0VE_EX-current.png

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 17:33, Tuesday 13 January 2015 - last comment - 12:17, Wednesday 14 January 2015(16056)
H1 upgraded to RCG2.9

Jim, Dave: WP5003

This morning we upgraded H1 FE and DAQ to RCG2.9. First the DAQ was upgraded and restarted. Then FE startup scripts were changed, model startup scripts changed.

Then a "make installWorld" was ran to install the models which were compiled yesterday. The H1.ipc file generated yesterday was re-installed.

We tested a reboot-restart first on a non dolphin FE (h1susauxh2) and then on a Dolphin FE (h1seib1).

We then restarted all frontends in the MSR by power cycling the computers, and end station frontends by rebooting the computers. We ended up having to powercycle h1iscex because it got stuck in reboot. In the MSR when we were restart testing, h1susb123 got stuck on reboot and needed a power cycle which Dolphin crashed the other MSR machines.

We got to a stable system with DAQ and FE reboots proceding correctly. We had 6 front end IOP models with large IRIG-B excursions into the 1000-2000 counts. The h1oaf0 IOP took 4 hours to return to normal IRIG-B range. One IOP went below zero (999998) which caused IPC errors on models receiving its channels. This fixed itself in about 10 minutes.

We noticed a single ADC error on the h1ioplsc0, which was cleared with a DIAG_RESET.

We noticed the DAQ frame size is smaller now. For science frames 670MB to 610MB (10% reduction) and commissioning frames 1.2GB to 1.0GB (20% reduction). We suspect new common models are the reason for this.

I linked Jamie's SDF_OVERVIEW MEDM screen to the SITEMAP under the GRD section. We are configuring the IOP, PEM and PSL systems.

This closes WP5003

Comments related to this report
david.barker@LIGO.ORG - 12:17, Wednesday 14 January 2015 (16067)

Frame size reduction was bogus. I checked too soon after the reboots when systems were not fully engaged and the frame was compressing zeros. After a few hours of ifo operation the frame sizes came up to nominal. Attached plot show commissioning and science frame sizes for the past two days.

Images attached to this comment
H1 CDS
patrick.thomas@LIGO.ORG - posted 17:29, Tuesday 13 January 2015 - last comment - 17:31, Tuesday 13 January 2015(16054)
Conlog running again, had to remove ODC channels
Some of the ODC channels now appear to have string values with unrecognized characters. For example:

caget H1:PSL-ODC_FSS_BIT21
H1:PSL-ODC_FSS_BIT21           FSS Not Resonant (Loop 300370216d377177

I regenerated the channel list, searched it for channels with ODC in the name, added these to the exclude list, and regenerated the channel list again.
Comments related to this report
patrick.thomas@LIGO.ORG - 17:31, Tuesday 13 January 2015 (16055)
The alog didn't like the backlashes. Here it is with forward slashes in place of backslashes:

caget H1:PSL-ODC_FSS_BIT21
H1:PSL-ODC_FSS_BIT21           FSS Not Resonant (Loop /300/370/216d/377/177
H1 SEI (SEI)
sebastien.biscans@LIGO.ORG - posted 17:28, Tuesday 13 January 2015 (16053)
ETMY Z-RZ substraction: very encouraging preliminary results

(To know the whole story about the Z-RZ coupling, see DCC document #E1400432.)

I turned ON the substraction on ETMY-ISI ST1 with good results. If you look at the first attachement:

- Red curve -> nominal configuration (RZ loop OFF)

- Blue curve -> RZ loop ON. As expected, we amplified the RZ motion around 0.1Hz by turning the loop ON. The loop provides some isolation above 0.5Hz. Z doesn't change.

- Brown curve -> RZ loop ON + Substraction ON. We can see an improvement by almost a factor of 10 in the RZ spectrum around 0.1Hz. The substraction seems to work just fine.

 

As Ryan suggested, we also wanted to see if we can obtain similar results without the substraction. We do have Z sensor correction on HEPI, so we might be able to relax the actuation on Z (meaning higher blend) and still have reasonable performance in vertical. By relaxing Z, the couping with RZ should be reduce. Unfortunately, the Z motion seems to big for our need if we swich to higher blend  (see second attachement).

 

Last attachement shows different substraction configurations:

- Red curve: Substraction ON with a 90mHz blend on Z and Z sensor correction on HEPI

- Blue curve: Substraction ON with a 45mHz blend on Z and Z sensor correction on HEPI

- Brown curve: Substraction ON with a 90mHz blend on Z and Z sensor correction on ISI

 

Viewing those results, it seems that switching to a lower blend on Z might be a good idea.
For further analysis, we need to look at more sensors and the optical lever. We might want to look at the other chambers as well.

Images attached to this report
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 15:18, Tuesday 13 January 2015 - last comment - 19:13, Tuesday 13 January 2015(16045)
IMC REFL Path Falls Again After RCG 2.9 Upgrade
J. Kissel, S. Dwyer, D. Sigg, E. Hall, N. Mavalvala

After performing all of the usual alignment position checks (SUS, SEI, MC TRANs QPD, IM4 TRANS QPD), after the RCG 2.9 upgrade (see LHO aLOG 16040) we've confirmed that the IMC REFL path has jumped down in pitch again as it has done several times in the past after major computer reboots or SEI/SUS events (see Integration Issue 854, LHO aLOGs 10335, 11481, and 15650). 

We didn't preserve camera views prior to the reboot, and I didn't get the chance to capture an UNLOCKED camera view in which the REFL path was similarly low, but I attach the misaligned views after the RCG, then SEI and SUS recovery before realigning the path, and the realigned views after Evan, Sheila, and Nergis have realigned the whole path. We've also confirmed that the MC WS are running happily now as well.

Note that the IMC REFL L RFPD and trigger PD are on different image planes and lens focal points than the MC WFSA and MC WFSB and MC REFL GIGE Camera (see D0902284), so it's to be expected that they're differently affected by a misalignment of the MC REFL path. In other words, the IMC LSC path is much less sensitive to misalignments than the IMC ASC path (which contains the MC REFL GIGE Camera View).

Finally, for future reference, I attach a screenshot of all of the relevant camera views and screens I can for the IMCASC and surrounding sensors, with 2015-01-13_H1IMC_Status_ScreensandCamera.png
Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 19:13, Tuesday 13 January 2015 (16058)

We added an iris to the IMC refl path on IOT2L, in front of the calcite polarizer, in the hopes that we can use this next time to recover the alignment.  

Keita, Brett and I also noticed that HAM2 HEPI moved between before and after the bootfest, as can be seen both on the oplevs and the IPSs. (RY, which is pitch, was different by about 15 urad before and after the bootfest) We have restored HAM2 RY, but I didn't finish checking this for the rest of the chambers since the schnupp crew want the michelson locked for now.  In the morning we will have to go through the rest of the chambers and redo the alignment procedure. 

This isn't a big enough shift to explain why we had to realign on IOT2L earlier, but restoring this did bring the IM4 trans QPD back to almost the same position it was at before the bootfest.  

Images attached to this comment
Displaying reports 67481-67500 of 83122.Go to page Start 3371 3372 3373 3374 3375 3376 3377 3378 3379 End