Displaying reports 69461-69480 of 85078.Go to page Start 3470 3471 3472 3473 3474 3475 3476 3477 3478 End
Reports until 15:48, Tuesday 13 January 2015
H1 SEI
hugh.radkins@LIGO.ORG - posted 15:48, Tuesday 13 January 2015 - last comment - 16:22, Tuesday 13 January 2015(16049)
Corner Station HEPI Pumps now running on Actual Differential Pressure

Spent the morning getting all the cable runs sorted and the pressure sensors zero'd.  Switched databases so the servo would run on the differential pressure collected at BSC2 in the LVEA.  This will address a long standing Integration issue and work permit.  Still need to do similar at EndX before these items are fully resolved.  The EndY has been running on the differential for several weeks.

Couple issues here at the corner station: 1) As I was doing some final cable coiling etc this afternoon, I lost the controller signal to the South Pump Station.  I valved the PS out to stop the back spinning.  I'll restart this next Tuesday; I think I can restart it without harm but didn't want to risk it after being off all morning and commissioning now ongoing.

2) Pressure sensor 3 on Pump Station 3 (3rd from South) has an issue so the signal is actually coming from sensor #2.  The apparent 25psi differential pressure across the 3u filter is not true.

3) The medm still shows the Differential Pressure coming from the Main Supply Line Sensor, again it is really coming from BSC2.

Again, I'll deal with issue 1) on Tuesday.  For issues 2) & 3) I'll rework the medm to correctly reflect reality.

Attached is the current medm.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 16:22, Tuesday 13 January 2015 (16051)

Okay, adjusted the medm.  So the servo pressure appears to be coming from BSC2 which it is.  Also annotated the PS3 sensor issue.  I've also adjusted the database calc so the red Pressure NOT OK will go green, the next time I restart the process, next Tuesday.  Corrected medm attached.

Images attached to this comment
H1 SUS
jeffrey.bartlett@LIGO.ORG - posted 15:42, Tuesday 13 January 2015 (16048)
3IFO Storage Container #2
Jeff B & Andres R

   This morning we loaded the 4 3IFO Quad Upper Structures (Quad-6, Quad-7, Quad-8, & Quad-9) onto the HAM ISI storage container #2. No issues or problems were encountered during the load. We will load the 2 TMS telescopes and Elliptical Baffles into this container during the week as opportunity allows.  
H1 SYS
daniel.sigg@LIGO.ORG - posted 15:39, Tuesday 13 January 2015 (16047)
Timing comaparator/frequency counters

Version 3 (svn tag 97) FPGA code was loaded into all timing comparator/frequency counters. This addresses:

There can still be a problem with crosstalk between channels, especially at frequencies above 200 MHz and signals stronger than 0 dBm. This has only been seen in open channels with no input. Channels with an RF input signal don't seem to suffer from it.

The CER and EX units were swapped with units which had a proper heatsink installed for the 5 V regulator. The following units were modified:

Serial Location Heatsink Code
S1107952 CER installed 3
S1201886 EX installed 3
S1201222 EY installed 3
S1201227 shop (MSR)   3
S1201224 shop (spare)   3
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
H1 CDS
james.batch@LIGO.ORG - posted 15:12, Tuesday 13 January 2015 (16046)
Install updated version of GDS tools
WP 4997

The gds tools have been updated to branch/gds-2.16.12.4.  This includes two bug fixes:

Bugzilla 288 - add ramp down of excitation to swept sine response measurement. (diaggui)

Bugzilla 778 - Make filter module lists iterable in Python (foton)

This affects only Ubuntu workstations.

The update of nds2-client software mentioned in the work permit will not take place until a bug is fixed affecting collection of trend data from NDS1 servers.
H1 SEI
fabrice.matichard@LIGO.ORG - posted 13:14, Tuesday 13 January 2015 (16044)
HAM Sensor Correction

We are not yet satisfied with the HAMs sensor correction performance.  The first plot attached is the detchar plot form Jan 6. Ignoring HAM3 (see all logs related to HAM3), only HAM6 shows the blend notches at 1Hz and 1.5Hz. Also the ISI units seem to be only slightly lower than the ground at low frequency.

The second plot attached shows HAM 4,5 and 6 with the sensor correction off and in high blend. The ground and the ISI should have similar amplitude. The third plot show the data that I grabbed from Jan 9th 2am to 3am, and recalibrated. I do find that ground and ISI have very similar amplitude, so we need to double check the automated plots.

Then, the fourth plot shows the transfer function between the ground instrument and the ISI. I averaged the transfer functions between 0.1Hz and 0.4Hz and got the following numbers. That doesn't match with the numbers that Sebastien posted. So I must be forgetting a number in one of the input filter banks, or there is an error in the script used to match the gains.

 

  HAM4 HAM5 HAM6
X 0.945 1.001 1.035
Y 0.929 0.991 1.027
Z 0.918 1.039 1.103
Images attached to this report
H1 CDS
cyrus.reed@LIGO.ORG - posted 11:33, Tuesday 13 January 2015 (16043)
CDS Workstation Patches
I've run the latest patch sets against all of the workstations.  They should be rebooted when convenient to load the new kernel.

I have also patched and rebooted the vacuum boot server, vxboot, and the nameservers, ns0 and ns1.  vxboot did not have NTP installed (an oversight), so I did that as well.
H1 CDS
patrick.thomas@LIGO.ORG - posted 10:19, Tuesday 13 January 2015 (16041)
Conlog crashed
Conlog has gone down with the following error:

Jan 13 10:05:14 h1conlog2 conlog: ../conlog.cpp: 301: process_cac_messages: MySQL Exception: Error: Incorrect string value: 'xE0x0F=xE0xFF' for column 'value' at row 1: Error code: 1366: SQLState: HY000: Exiting.
Jan 13 10:05:15 h1conlog2 conlog: ../conlog.cpp: 331: process_cas: Exception: boost: mutex lock failed in pthread_mutex_lock: Invalid argument Exiting.
Jan 13 10:05:15 h1conlog2 conlog: ../conlog.cpp: 230: main: ca_poll returned 48. Exiting.
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 09:44, Tuesday 13 January 2015 (16040)
H1 upgrade to RCG2.9

Dave, Jim:

we are starting the upgrade of all H1 front end computers to RCG2.9. All systems will be put into their safe state and restarted. We are coordinating the restart order with commissioning staff.

H1 PSL (DetChar)
edmond.merilh@LIGO.ORG - posted 09:32, Tuesday 13 January 2015 (16039)
PSL Weekly Report

PSL Weeklies. Also Chiller water level is GOOD.

Images attached to this report
H1 DAQ (CDS)
james.batch@LIGO.ORG - posted 08:40, Tuesday 13 January 2015 (16038)
Dataviewer updated to 2.9.1
As part of the transition to RCG-2.9, dataviewer has been updated to 2.9.1. The new dataviewer reads the revised nds1 protocol and fixed bugzilla 728 to allow proper display of unsigned integer trend data.
H1 DAQ (CDS)
james.batch@LIGO.ORG - posted 08:28, Tuesday 13 January 2015 (16037)
Install new DAQ software, restart DAQ
The DAQ software has been updated to 2.9 on h1dc0, h1fw0, h1fw1, h1nds0, h1nds1, and h1broadcast0.  The DAQ was restarted to get the new software running on the named computers.  
LHO FMCS
bubba.gateley@LIGO.ORG - posted 06:54, Tuesday 13 January 2015 (16035)
Mid Station Chillers
Stopped the chillers I started yesterday and started the 2nd chillers at each mid station. They will run most of the day for periodic running and maintenance checks.
H1 ISC
daniel.hoak@LIGO.ORG - posted 21:31, Monday 12 January 2015 (16034)
OMC noise measurements with PDH locking

Dan, Koji

We succeeded in locking the OMC using AS45 and the OMC REFL beam, and took a number of noise measurements and transfer functions of the cavity length.  Data and plots are forthcoming.

On ISCT6, we took a pickoff of OMC REFL and steered this beam onto the ASAIR_A RFPD.  A lens was added to focus the spot onto the diode.  (Note that in order to recover the OMC REFL beam, we undid Keita's precautionary misalignment of the OMC REFL picomotors.  We'll need to steer this beam away from the OMC REFL QDPs again before we start locking.)  We used the OMC QPD alignment servo to keep the beam aligned to the cavity.  The dither alignment loops are still unstable and need to be fixed.

We used a pair of SR560s to take the ASAIR_A_45 I-phase signal and feed this back into the PZT driver.  We found that the aux input path for the PZT driver was working (yay!), and even better found that very little loop shaping was necessary to get a stable lock.  We were quite surprised that the flat-response PZT was giving us a nice 1/f loop; It looks like the capacitance of the PZT and the output impedance of the PZT driver are just right to provide a pole at around 2Hz, and the dewhitening filter on the board acts as a low-frequency boost.

We measured the cavity length noise from ~10mHz to 100kHz.  The resonances of the PZT mirror tombstone at ~8kHz and the PZT itself at ~80kHz were clearly visible.  There was a forest of lines around 1kHz that was *very* easy to excite by tapping on the HEPI crossbars.  The sensitivity of the OMC length to light taps on a structure outside the vacuum was rather alarming and needs to be investigated more closely -- does the noise couple into the ISI, the OMC suspension, the tip-tilts?  One good piece of news is the transfer function of PZT voltage --> cavity length is smooth around 20kHz, so there is a good place for an analog dither signal.

H1 AOS (ISC)
eleanor.king@LIGO.ORG - posted 20:42, Monday 12 January 2015 (16033)
PLL for schnupp asymetry measurement

Evan, Elli

The auxiliary laser can now lock to the carrier (IM4 transmitted beam) on IOT2R using a NewFocus LB1005 servo controller.  LB1005 settings are gain=5, PI corner=3kHz, LF gain limit=60dB.

A 1.8GHZ network analyzer is used as the local oscillator to set the frequency offset.  We can sweep the frequency offset over 3.5MHz.

We measured the open loop transfer function (see attached plot).  The UGF is at 15kHz with 70 degrees of phase margin.

Images attached to this report
Non-image files attached to this report
H1 SEI (SEI, SUS)
sebastien.biscans@LIGO.ORG - posted 17:57, Monday 12 January 2015 (16032)
IPC error on ITMX

Jeff, Sebastien

It seems that we had an IPC error on ITMX today (around 18:30:00 UTC). The ISI-ITMX watchdogs reported a 'payload trip', but the SUS watchdogs were fine: the WDMON_RFM_EPICS_ERROR channel shows an error at that time. See plot attached for more details.

Images attached to this report
H1 SEI (DetChar, SUS, SYS)
jeffrey.kissel@LIGO.ORG - posted 17:39, Monday 12 January 2015 - last comment - 10:34, Tuesday 13 January 2015(16028)
H1 SUS ETMX Rings Up, Triggers Software Watchdog, Trips SEI System
J. Kissel, S. Biscans, D. Barker, J. Batch

*Sigh* there's always a fire. Today's fire was that just before Dave and Jim went at EX to swap ADC cards (see LHO aLOG 16023), they'd asked Seb to turn off SEI ETMX. Once they looked, they found that the IOP Software Watchdog had tripped on the SEI system. 

In summary, there is a nasty but slow instability between the ST2 Y isolation loop and the QUAD T, RX, and RZ motion. We've never seen it before because we rarely, if ever, run the QUAD without damping and the ISI in fully isolated for more than an hour or so to take transfer functions. However, the independent software watchdog did exactly what it what it was supposed to do, and prevented extended shaking of the suspension caused by ISI instabilities. As Vern suggests, perhaps I awoke a daemon by jokingly invoking quotes from the Poltergeist last night, but it looks like we're well protected against daemon attacks.

Here's the story.

05:25 UTC           - Jeff requests SEI_ETMX Manager guardian to go to Fully Isolated (Remember this configuration includes *no ST1 RZ isolation*, and *no ST2 Z, RX, RY, or RZ* see SEI aLOG 658)
05:28 UTC-5:35 UTC  - Jeff takes transfer functions of SUS ETMX (see LHO aLOG 16012), and *leaves* M0 damping loops OFF.

Over the next two+ hours, the maximum ISI ST2 Y RX RZ displacement begins to ring up, most prominently at exactly 0.46 [Hz], the first Transverse Mode of the QUAD's main chain. (Note that the first L Mode at 0.43 [Hz], the first R mode at 0.92 [Hz] are also rung up as well, but not at the same amplitude). There is some, very slow, parasitic, positive feedback cross coupling between the free ST1 ISI RZ, or ST2 Z, RX, RY, and/or RZ and the QUAD's first T / R mode that leaks into the ST2 ISI's Y DOF loop that *is* closed, and slowly but surely rings up the ST1/ST2 Y/RX/RZ motion, and eventually rings up the whole system into instability.
The QUAD's watchdogs DO NOT trip, because the M0 and L2 watchdog has been spuriously set to 80 000 [ct]. Even if they did, the SUS all actuation on the SUS is already OFF, so it would have made no difference. Only if ALL FOUR SUS USER watchdogs tripped (M0, R0, L1, and L2), would it have triggered the SUS USER DACKILL, and sent a "PAYLOAD BAD" flag to the ISI, tripping its USER watchdog.
However, the SUS Independent Software Watchdog (IOP watchdog or SWWD), which also watches the RMS of the Main Chain begins sees this increase in RMS.

07:49 UTC           - The ETMX SWWD begins to register that the QUAD's "OSEM4," i.s. Main Chain LF, a Vertical Sensor, is surpassing the 110 [mV] RMS threshold, originally defined by Jeff during the Hardware Watchdog testing (see LHO aLOG 12496. As stated there, this is roughly 10 +/- 5 [um] or [urad] peak-to-peak thoughout the ISI/ QUAD system. Note that the LF sensor is seeing MUCH more RMS than any other sensor, but RT and SD are the next biggest contenders, implying some sort of Roll / Transverse / RX / Y - ey kind of motion.
08:00 UTC          - The SWWD's ETMX / QUAD watchdog is now constantly above threshold (State 3)
08:05 UTC          - The SWWD ETMX / QUAD watchdog sends a warning to the SEI ETMX watchdog indicating things are getting serious (SUS WD goes to State 4, SEI WD goes to State 3), and shuts down the SUS DACs, tripping the all SUS IOP's DACKILL (for TMSX, ETMX M0, and ETMX R0).
08:08 UTC          - The ISI's ST2 USER watchdog trips on the Actuators, but going only to State 3. This turns off ST2 X&Y, and the SWWD OSEM RMS begins to decline. << -- This points the finger at an ST2 X & Y instability (but ONLY when M0 is free).
08:09 UTC          - The SWWD's SEI watchdog get the final 1 minute warning that the SEI DACs are about to be shut down (SEI WD goes to State 4)
08:10 UTC          - The SWWD shuts down the SEI DACs, tripping the SEI IOP DACKILL (State 0). This sends both stages of the ISI to their USER WD State 4: full isolation shutdown.


I attach a whole bunch of plots I needed to back up this story. 

However, in addition to data mining, I *did* re-create the chamber configuration and take a standard SUS transverse transfer function, but gathered all of the ST1 T240s and ST2 GS13s as response channels, and plotted the transfer functions and coherence between M0 T and ISI Y RX and RZ -- 2015-01-12_2355_H1ETMX_WhiteNoise_tf.pdf
There's a lot of interesting information in there, but most importantly, there's a very coherent, transfer function at 0.46 [Hz] for all stages and all DOFs, with a magnitude of
       Y/T [m/m]      RX / T     RZ / T
ST1     2.3e-4        1.3e-4     0.014
ST2      0.16          0.018     0.033     


Images attached to this report
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 10:34, Tuesday 13 January 2015 (16042)DetChar
The SEI Team:

Action Items from this event:

- Hook the SUS IOP watchdog's warning flag up (when the SUS IOP watchdog switches to State 4) to the ISI USER watchdog, to smoothly ramp down the isolation loops *before* the SEI DACs are shut down. This will also enhance /increase the warning signs / notifications / alarms, by default. 
  (highest priority)
- Reduce the M0 threshold SUS USER WD 
  (would not have affected the outcome of this event, but it should be reduced just the same)
- Find out exact what the instability was 
  (this will be time consuming both for the IFO and man-power, so we will likely *not* do this.)
LHO General
patrick.thomas@LIGO.ORG - posted 17:02, Monday 12 January 2015 (16020)
Ops Summary
Karen & Cris in LVEA

08:04 Jim W. running excitations on HAM3
08:36 Corey boxing 3IFO ISC table components in squeezer bay and mechanical room
08:43 Jim B. taking down nds0 to compile daqd modules for RCG 2.9
09:11 Elli to IOT2R
09:18 Cris to end X
09:24 Bubba to end Y fan room to put heater unit in place
09:32 Jeremy and Mitchel to LVEA West Bay to work on elliptical baffle
09:35 Sudarshan and Rick to end Y for PCAL work
09:42 Hugh and Brian to LVEA
10:11 Hugh operating crane
10:16 Dave and Jim B. to end X
10:16 Karen to end Y to clean
10:26 Dave and Jim B. powering down h1seiex to replace ADC cards
10:57 Travis to LVEA West Bay to pick up and store equipment
10:57 Hugh operating crane
11:28 Hugh operating crane
11:45 Cris back from end X
11:47 Brian and Hugh out of LVEA
11:53 Corey out of LVEA
11:53 Mitchel and Jeremy done
11:57 Karen back from end Y
11:58 Bubba back from end Y
12:00 Betsy running transfer functions on ETMX
13:41 Corey back to squeezer bay
13:52 Cyrus to end X to reboot workstation
14:18 Cyrus back from end X
14:28 Delivery for Richard
14:52 Elli back to IOT2R
15:15 Aaron looking for chassis near BSC3
15:52 Jeff K. running transfer functions on ETMX
H1 PSL (PSL)
sudarshan.karki@LIGO.ORG - posted 16:47, Monday 12 January 2015 (16031)
ISS Second Loop Status

Sudarshan, Dan

The ISS second loop didnot close using the automated python script.  We also tried to close the loop manually with the steps described in alog 14291 but without any success. The loop rails each time we try to close it. From some prelimianry investigation, it looks like there is some problem with the electronics readout of the PDs. Attached is a plot showing all 8 PD signals of the ISS photodiode array.

Images attached to this report
Displaying reports 69461-69480 of 85078.Go to page Start 3470 3471 3472 3473 3474 3475 3476 3477 3478 End