Displaying reports 45361-45380 of 88367.Go to page Start 2265 2266 2267 2268 2269 2270 2271 2272 2273 End
Reports until 12:13, Tuesday 02 October 2018
H1 ISC
richard.mccarthy@LIGO.ORG - posted 12:13, Tuesday 02 October 2018 - last comment - 16:41, Tuesday 02 October 2018(44297)
Cleaning of ALS fiber ends from Corner to End

With the noise and problems we have been having with ALS X I attempted to Clean the fiber ends at all junctions between the LVEA and the End station.  I used a FiberScope to look at the end before and after cleaning.  The attached pdf shows one of the worse.  This was the fiber that runs from EX patch panel to the Table.  This is the patch panel end.  All fibers showed visual improvement after cleaning.

I did not take apart the patch panel main runs.  This would be the next step if we find this helps.

 

Non-image files attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 16:41, Tuesday 02 October 2018 (44309)

X end got better, now it's similar to Y. See the first plot (top) showing the past 18 hours or so, zero-power period corresponds to the maintenance. You need to look at peak to peak, ignoring the spikes.

Don't worry about spikes as far as fiber is concerned, that's the result of failed locking attempts after the maintenance (IMC loses lock, FSS is kicked). See 2nd attachment.

Images attached to this comment
H1 AOS
yannick.lecoeuche@LIGO.ORG - posted 12:06, Tuesday 02 October 2018 (44296)
LVEA transitioning to LASER HAZARD (WP #7855)

TJ is transitioning to LVEA to LASER HAZARD

H1 AOS
betsy.weaver@LIGO.ORG - posted 10:44, Tuesday 02 October 2018 - last comment - 11:06, Tuesday 02 October 2018(44290)
Late entry on yesterday's TCSX table water leak

Since it wasn't posted yesterday:

FRS Ticket 11569

[reply[−]Descriptionbetsy.weaver@LIGO.ORG 2018-10-01 15:30:08 CDT

This morning, TJ went to check the TCS chiller fill levels and discovered that the X one was showing nearly empty.  He filled it up, and went to inspect the table and lines.  Indeed, he found a 1 sec drip which had developed on one of the t-joints just inside the table enclosure where the lines enter the table and split into 2 directions. The leak caused a puddle on the table in the corner of the leak.  He and TVo cleaned up the leak.  We then added a trough to catch the water for now while we gear up for a fix tomorrow during the Tuesday Maint window.

We'll continue to monitor the trough fill level this afternoon.

We may need to turn the chiller off after commissioning completes tonight to avoid the case where the trough fills overnight.

 

Comments related to this report
jason.oberling@LIGO.ORG - 11:03, Tuesday 02 October 2018 (44292)

J. Bartlett, T. Shaffer, J. Oberling

The new fitting has been installed and the leak is tentatively fixed.  One of us will check on it near the end of the maintenance window to make sure there are still no drips.  We will also monitor the new fitting over the next couple days before declaring final victory, but so far we are leak-free.

thomas.shaffer@LIGO.ORG - 11:06, Tuesday 02 October 2018 (44293)

With the new fitting in place, the leak seems to be fixed. We will monitor during today and the next few days to make sure before closing the FRS out.

I've attached some pictures of the table after I found the leak.

Images attached to this comment
betsy.weaver@LIGO.ORG - 10:47, Tuesday 02 October 2018 (44291)

Jeff Bartlett is on the case this morning, hunting down the last remaining black plastic t-fitting which looks to be a replacement for what is currently leaking on the TCSX table.  

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 10:27, Tuesday 02 October 2018 - last comment - 14:31, Tuesday 02 October 2018(44289)
Corner station models crash at 05:03PDT this morning

Most models which are Dolphin'ed computers in the corner station crashed at 05:03:44 PDT (12:03:44 UTC) Oct 02 2018.

For most computers, all the user models stopped with ADC timeout errors. For some, not all models crashed.

Comments related to this report
david.barker@LIGO.ORG - 11:15, Tuesday 02 October 2018 (44294)

here is the CDS overview before we started the recovery process.

Images attached to this comment
jonathan.hanks@LIGO.ORG - 14:24, Tuesday 02 October 2018 (44299)
Rolf asked for some information on the cpu cycle count through the glitch.  I've two plots of the cpu meter from h1iopsusb123, h1iopsush2a, h1ioplsc0, h1iopasc0.  The first plot is in dataviewer and gives the mean round the glitch, the second is from ndscope is is raw data (cpu_meter + cpu_meter_max).

A summary from nds_query giving raw numbers:

Data for 5 seconds starting at GPS: 1222517040
Channel                                  type      nWords   units
H1:FEC-28_CPU_METER                      int_4         80 
Channel: H1:FEC-28_CPU_METER  type: int_4  nWords: 80
    0        5        5        5        5        5        5        5        5
    8        5        5        5        5        5        5        5        5
   16        5        5        5        5        5        5        5        5
   24        5        5        5        5        5        5        5        5
   32        5        5        5        5        5        5        5        5
   40        5        5        5        5        5        5        5        5
   48        5    20228    20228    20228    20228    20228    20228    20228
   56    20228    20228    20228    20228    20228    20228    20228    20228
   64    20228        6        6        6        6        6        6        6
   72        6        6        6        6        6        6        6        6
Images attached to this comment
david.barker@LIGO.ORG - 14:28, Tuesday 02 October 2018 (44300)

Jonathan, Dave:

Recovery process:

Took h1psl0 out of the Dolphin fabric before restarting the models. Disabled its IXS600 switch port and pulled the IX cable at the rear of the computer. This should insulate the PSL from any further corner station Dolphin issues.  We will re-attach when the system is more stable.

Replaced h1asc0's Dolphin cable (this machine reported a Dolphin Gen1 issue). Powered h1asc0 down, replaced 2m cable with new 1m cable temporarily ran directly from IX600 switch C0 port 8 to cpu.

Systematically restarted all  models on all computers with errors.

When h1iopseib1 was starting, the computer froze. SSH session was unresponsive, local console was dark. Disabled IXS600 switch port and power cycled computer.

There were DAC errors on h1seib2 and h1seih16, so these IOP models were also restarted.

By the end of the day, h1seib3 was the only Dolphin'ed corner machine which did not get anything restarted on it.

I've started a wiki page to overview these recent front end issues: https://cdswiki.ligo-wa.caltech.edu/wiki/FrontEndCrash

 

david.barker@LIGO.ORG - 14:31, Tuesday 02 October 2018 (44301)

Note that there are expected IPC errors on h1psliss and h1lsc following the disconnection of h1psl0 from the Dolphin network.

h1psliss receives two IPC channels from h1lsc (TRX and TRY normalised photodiode signals). Used for ISS third loop, not needed in the short term.

h1lsc receives one IPC channel from h1psldbb (FF_JITTER). Used to add to OMC-DARM signal. Has not had a useful signal for some time.

H1 AOS
yannick.lecoeuche@LIGO.ORG - posted 09:19, Tuesday 02 October 2018 (44285)
EX transitioned to LASER HAZARD

Rick is transitioning EX to LASER HAZARD

H1 CDS
patrick.thomas@LIGO.ORG - posted 09:14, Tuesday 02 October 2018 (44284)
Beckhoff updates
WP 7842

Updated system managers and PLC code on h1ecatc1, h1ecatx1, and h1ecaty1 to changes made in preparation to migration to TwinCAT3. These include:

- Created TwinCAT libraries for the wind fence speed and direction sensors. There are now channels for 8 wind speed sensors and 8 wind direction sensors. Only the first four wind speed sensors and the first wind direction sensor are connected to hardware.

- Replaced the input and output structures for the weather, fiber polarization correction, TCS chiller readback, and video control libraries with EL6inData22B and EL6outData22B structures.

- Removed AlsCExtra1, AlsCExtra2, LscCAsSpare_E, and LscCAsSpare_F channels from h1ecatc1 PLC2.

- Changed IscExtraEnd to IscEndExtra in the end station PLC2 code.

A DAQ restart still needs to be done.
H1 ISC (ISC)
jeffrey.kissel@LIGO.ORG - posted 08:38, Tuesday 02 October 2018 - last comment - 10:07, Tuesday 02 October 2018(44281)
ALS End Station WFS -- Unmonitoring Guardian Controlled Channels, Letting other DIFFs Perish
J. Kissel

Not clear if the end stations need to be rebooted this morning after the corner station front-ends seems to have crashed, but I'm reconciling the ALS EX and ALS EY front-end models with their settings definition files. 

It is dreadfully obvious from the time stamp that a few filters in ALS WFS control (DOFs 1 and 2) are turned on and off by guardian during the lock acquisition sequence, namely FM9, a -14 dB gain filter. As such, I'm unmonitoring FM9 in the ALS-[X/Y]_WFS_DOF_[1/2]_[P/Y] filter banks. Note that these are filter banks, so I can individual monitor / unmonitor this filter module only, so I have. I've also consistently unmonitored the inputs to these filter banks, which are also guardian controlled, and weren't consistently unmonitored in any of the 6 filter banks.

There remains several diffs that are either 
- related to the fact that we're currently ignoring ALS WFS on the X arm because they're broken LHO aLOG 44206, which appears to be coded into the guardian, or
- because (surprisingly) some of the elements of the ALS Y WFS sensing matrices have changed.

I attach the remaining diffs that I'm leaving present.
Images attached to this report
Comments related to this report
gabriele.vajente@LIGO.ORG - 10:07, Tuesday 02 October 2018 (44286)

Both X and Y end ALS WFS sensing matrices were changed on September 26th, as reported in 44178

The new values should be accepted.

H1 ISC (AOS, CAL, CDS)
jeffrey.kissel@LIGO.ORG - posted 07:50, Tuesday 02 October 2018 - last comment - 10:11, Tuesday 02 October 2018(44275)
SDF Differences for Models getting Booted Today
The following models / PLCs are planned to be booted today and have differences against their settings definitions file (SDF).
    OAF
    ASC
    CS ECAT PLC2
    CS ECAT PLC3
    CS ECAT PLC4
    EY ECAT PLC2
    EX ECAT PLC2
I've screen captured those differences below. For those whom are doing the booting (Jenne, Jeff, Dave, Patrick) try to make sure you've reconciled these changes BEFORE you get started with boots. For the record, the IFO ws in the DOWN state when these SDFs were captured. It also appears as though the entire front-end world has crashed last night, but that does not seem to be affecting the reporting of differences in settings.

We also plan to boot these processes, but they don't have any differences with there current reference file (safe)
    CAL EY
    CAL CS

I, finally, attach a screen cap of the SDF overview.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 08:47, Tuesday 02 October 2018 (44283)
ECAT settings don't come back up exactly the same after PLC restart.

See attached screenshots of ECAT CS PLC2 and PLC4 after Patrick finished his prep work for TwinCAT 3 this morning in which he had to restart all IFO-related PLCs. Compare these agains the above screenshots taken before the boot.
Images attached to this comment
daniel.sigg@LIGO.ORG - 10:11, Tuesday 02 October 2018 (44288)

The TwinCAT system saves its values once minute. After a reboot it will restore to the last set point automatically—in most cases. If the code was changed significantly, it may choose to ignore the old settings and start fresh with all zeroes. The above screens indicate the former, where the settings were restored to the last settings, but probably the sdf was and is outdated. TwinCAT will never use an EPICS/SDF saverestore, this has to be done by a user.

H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 13:58, Monday 01 October 2018 - last comment - 11:42, Tuesday 02 October 2018(44257)
SQZ model changed

Sheila, Haocun, Terry, Nutsinee

We moved the PSL feed forward summing point so that it happens before the OPO frequency servo filter bank.

WP#7845

Comments related to this report
terry.mcrae@LIGO.ORG - 11:42, Tuesday 02 October 2018 (44295)

Model attached.

Non-image files attached to this comment
H1 TCS (AWC, TCS)
daniel.vander-hyde@LIGO.ORG - posted 02:15, Sunday 30 September 2018 - last comment - 10:10, Tuesday 02 October 2018(44243)
Testing the inverted ring heater step response

Stefan, TVo, TJ, Danny

      Stefan has the idea of significantly reducing the amount of time it takes a test mass to reach a final lens by utilizing the ring heater step response and carefully designing an inverse filter to realize the inverse response.  We tested the idea in a previous post using Comsol data and were able to get a time series of the ring heater settings necessary to achieve a "step lens". To test this with measured data I took a time series  from H1:TCS-ITMY_HWS_PROBE_SPHERICAL_POWER after the ring heater settings had been changed by a reasonably large amount and attempted to perform the same procedure. The matlab zpk model of the system filter and inverse filter are attached figures. There are also comparison figures of the ring heater inputs and another figure their respective responses. 

Testing the new ring heater time series: 

With an initial lens around 3 microdiopters, the following figure shows convergence to a final lens of approximately -16 +/- 3 microdiopters within the first three hours but is about 1/2 the predicted lens. I might need to take another look at my model to see why this might be. 

I cut the script the short because there will probably be commissioners coming in tomorrow so I am using this method (on workstation ZOTWS2) in attempts to restore the original ITMY lens by tomorrow morning (but will run till 9/31 00:00 PST to maintain the lens). 

 

 

Images attached to this report
Comments related to this report
daniel.sigg@LIGO.ORG - 01:32, Sunday 30 September 2018 (44245)

Could the same missing 50% explain why the preloading was off?

daniel.vander-hyde@LIGO.ORG - 09:58, Tuesday 02 October 2018 (44271)AWC, TCS

Sorry Daniel. This 50% was due to a couple of ridiculous mistakes on my part. The first mistake was that I assumed that the initial step response was caused by a ring heater step of 1 watt when in reality it was caused by a step of 3.13 watts (please see attached image for updated plant zpk model with new gain).  The second, and most glaring mistake, was not thinking about the additive power from both of the upper and lower portions of the ring heaters so this left a factor of two missing in my model. I've attached time series of the measured data of the ring heater power compared to the time series from the updated model. I've attached a spherical power time series comparison as well. The final differential lens that the model suggests is 18.98 microdiopters.

In regards to pre-loading, I can update you on how these time series compare to the TCS simulation time series whose input parameters are used in the pre-loading estimates. 

Images attached to this comment
thomas.vo@LIGO.ORG - 08:47, Tuesday 02 October 2018 (44282)

The model of the pre-loading estimates use the calibration in diopters/watt on the TCS simulation page.

Spherical power (udiopters) = [ 2*(-9E-6) + 0.9E-6]  * P_RH = -17 udiopters for 1 Watt

The first coefficent in the equation is the substrate lens (the factor of 2 for double passing) and the second coefficient is the radius of curvature change.

daniel.vander-hyde@LIGO.ORG - 10:10, Tuesday 02 October 2018 (44287)AWC, TCS

Here is a comparison plot with the added TCS simulation time series. The simulation appears to be converging to a differential lens of 18 +/- 1 microdiopters.  

Images attached to this comment
Displaying reports 45361-45380 of 88367.Go to page Start 2265 2266 2267 2268 2269 2270 2271 2272 2273 End