Displaying reports 74541-74560 of 85472.Go to page Start 3724 3725 3726 3727 3728 3729 3730 3731 3732 End
Reports until 11:05, Thursday 10 April 2014
H1 ISC
sheila.dwyer@LIGO.ORG - posted 11:05, Thursday 10 April 2014 - last comment - 12:07, Thursday 10 April 2014(11263)
ITMX also tripped earlier

ITMX has tripped twice this morning, no known cause for the first trip, the second one we caused.

Comments related to this report
sheila.dwyer@LIGO.ORG - 11:29, Thursday 10 April 2014 (11266)

ITMX and ITMY both tripped in the last few minutes.  Jim is recovereing.  Phil and Aaron are pulling cables, these might be a good example of times when overly sensitive watchdogs make it difficult to commision while there is normal install activity in the LVEA. 

sheila.dwyer@LIGO.ORG - 12:07, Thursday 10 April 2014 (11267)

Jim, Rich, Sheila,

several more trips, BS, both ITMs. 

Rich and I tried to put ITMX into a safe state:

GS13 and L4Cs in low gain mode, all blends on Start, raise T240 watchdog threshold, Sensor correction off.

After we heard that Fil and Aaron are out of the LVEA I tried switching back to the good performance state, it trippped again while I was switching blends.

Why do these trip while switching blends?  According to Rich that shouldn't happen, but it does.  The second attached plot below is the actuator trip that happened while I was switching blends. 

Images attached to this comment
H1 TCS
david.hosken@LIGO.ORG - posted 10:26, Thursday 10 April 2014 - last comment - 17:29, Thursday 10 April 2014(11262)
TCS status
Dave H, Alastair, Thomas, Greg

Quick summary of progress:

TCSX:
Laser was operated for a few hours on Monday with an output power of ~58.5W. Optics have been mounted and placed in position on the table. This table is now ready for alignment.

TCSY:
Optics/mounts have been staged, and are ready for table installation. Cabling is almost complete. Attempts were made on Wednesday to operate the laser/test the output power, however this was unable to be performed due to a fault with the paddlewheel flow meter (amongst other interlock/laser controller issues that are still to be tracked down). Some additional cabling is still to be installed. 

TCSX/Y periscopes have been partially assembled, still to track down one last component. Socket head cap screws with lower profile heads have been ordered, as it was observed that the cap screws for the periscope base sit proud. 
Comments related to this report
david.hosken@LIGO.ORG - 11:17, Thursday 10 April 2014 (11264)
TCSY paddle wheel flow sensor power checked and settings confirmed. Still unable to display water flow value. Will need to remove from system and check operation on the bench and/or replace.
david.hosken@LIGO.ORG - 17:29, Thursday 10 April 2014 (11277)
DavidH/Greg : Paddle wheel flow sensor removed, tested and was found to be working as expected. Reinstalled/reseated and now appears to be working correctly. As per installation instructions, for this install no teflon tape was used... previously used tape was removed.
H1 PSL
sheila.dwyer@LIGO.ORG - posted 10:17, Thursday 10 April 2014 (11261)
PSL restarted

Power watchdog trip, Gerardo is making plots to investigate.

H1 SEI
sheila.dwyer@LIGO.ORG - posted 10:01, Thursday 10 April 2014 (11260)
HAM 3 HEPI L4C trip

Threshold raised

Images attached to this report
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:20, Thursday 10 April 2014 (11258)
CDS model and DAQ restart report, Wednesday 9th April 2014

model restarts logged for Wed 09/Apr/2014
2014_04_09 07:27 h1fw1
2014_04_09 12:17 h1hpiham4
2014_04_09 12:17 h1hpiham5
2014_04_09 12:17 h1iopseih45
2014_04_09 12:17 h1isiham4
2014_04_09 12:17 h1isiham5

h1fw1 unexpected, all others due to power down of h1seih45.

H1 SEI (INS)
jim.warner@LIGO.ORG - posted 17:03, Wednesday 09 April 2014 (11257)
ITMY ISI tf running on OPSWS0

No touching, please.

H1 SEI (SEI)
richard.mittleman@LIGO.ORG - posted 16:50, Wednesday 09 April 2014 (11256)
BSC-ISI Diagram

This is to remind me (and anyone else who is involved) that we need to modify the BSC-ISI control diagram to allow all 6 degrees of freedom of stage 1 to stage 2 sensor correction

H2 SEI (SEI)
mitchell.robinson@LIGO.ORG - posted 16:33, Wednesday 09 April 2014 (11255)
Staging building, 3IFO (unit 3) progress
Yesterday,
Scotty and I were able to populate the 400+ 1/4-20 hardware into the stage 2 closeout plate cover, as well as attach the back and side ribs. 

Today,
I made a cable kit for 3IFO BSC unit 2. Unit 3 will need 4 cables tested before it is a complete kit. All bolts connecting the closeout plate and closeout plate cover were torqued to spec. Locker sub-assemblies have begun. General cleanup and shelf organization is also ongoing.
H1 General
jim.warner@LIGO.ORG - posted 15:38, Wednesday 09 April 2014 (11254)
04092014 Ops Log

9am Justin HAM2 area working on laser barriers

9:15 DaveH & Alastair to LVEA for TCS work

9:30 Hugh HAM4 HEPI work

9:30 Fil & Aaron to EY for camera install

10:30 Bubba to EX

10:30 Ark Roofing on site

10:45 Corey to LVEA looking for cameras

12:00 Fil & JimB powering down HAM4/5 rack for fix BIO cabling

I didn't hear from anyone after lunch, so I'm assuming all work stopped about then.

H1 ISC
alexan.staley@LIGO.ORG - posted 15:36, Wednesday 09 April 2014 (11253)
Noise Hunting Cont

(Alexa, Pablo)

 

We examined the noise spectrum of REFL_DC_BIAS in several configurations. The first was in the nominal setting. We then placed an ND filter along the PSL reference path on ISCT1 after the shutter. Finally, we placed the ND filter along the x-arm green transmission path (before ALS-BS5). We saw that the beatnote signal appropraitely decreased by 3dBm (or Sqrt(2) in amplitude) with the ND filters placed. This signal was taken from the RF MON readback; I confirmed that this was consistent with an RF anaylyzer after the RF pre-amp.The 1/f noise changed by the same amount regardless of which path the ND filter was placed in. Surprisingly, the noise increased by a factor of 4. One would imagine only an increase by sqrt(2). This increase is also higher compared to what we saw when we did this measurement yesterday (alog 11221).

  REF # ALS-C_TRX Cnts Beatnote Signal
No ND Fiilter 4,5(RMS) 0.85-0.93 -14.6dBm
ND Filter in x-arm trans path 6,7(RMS) 0.35-0.48 -18dBm

NF Filter in PSL ref path

2,3(RMS) 0.80-0.94 -18dBm

While on the table, I noticed that there is clipping in the PSL reference path. The beam is clipped at the bottom of the PBS. I have not done anything to fix this clipping yet. This will affect our mode matching and our noise.

Images attached to this report
H1 SEI
hugh.radkins@LIGO.ORG - posted 15:35, Wednesday 09 April 2014 (11252)
WHAM4 HEPI Parker Valve

Just for the record, plots attached to show the problem we saw on the horizontal corner1 HEPI actuator.  The first and second plot shows the unmatched response slopes to the H1 drive.  The third plot shows an acceptable result although it might be nice to normalize/overlay the traces but we are also looking at the calculated slopes so we aren't just sticking a thumb up and seeing if it looks ok, but almost.  These acceptable slopes range from 1.75 to 2.00cts/ct.  The first plot H1 slope is low at 1.35 and the second is too high at 2.6cts/ct.  The PTB haven't given an explicit criteria, so, executive decision: if you have to look closely to see if the slopes are much different then they are ok.

Images attached to this report
H1 SEI (SEI)
hugo.paris@LIGO.ORG - posted 13:21, Wednesday 09 April 2014 - last comment - 14:50, Friday 11 April 2014(11240)
04/01/14 Chile Earthqake Seismic Study

A magnitude 8 earthquake coming from Chile tripped all the BSC-ISIs on 04/01/14. Sheila's wd plots show that the ISIs tripped on the actuator watchdogs. We suspected that the servo loops were trying to compensate for the common mode seen by the BSC-ISIs at both ends of the arms, thus saturating the actuators. We studied the ground motion recorded by the ground STS at the corner station (BS-STS) and the ground T240 installed at EX (EX-T240) at the GPS time provided by Sheila, in order to find out.

On the attached document:

 

We could considerably reduce the amount of signal sent to the BSC-ISI actuators during a major earthquake (factor as big as 6), and thus reduce the risk of saturating the actuators, by removing the common mode from the signal we feed to the servo loops of the BSC-ISIs.

 

Data, plots and scripts are commited to the seismic SVN:
/ligo/svncommon/SeiSVN/seismic/Common/Data/2014_04_01__Chile_Earthquake_Data/

 

Note 1: X and Y had to be swapped on EX data, and a minus sign was also added to the new x-axis EX data. It is likely that EX T240 is mis-oriented.
Note 2: The calibration of EX-T240 was still the one that JeffK made, at the time we looked at. RichM updated it since.

Non-image files attached to this report
Comments related to this report
hugo.paris@LIGO.ORG - 14:50, Friday 11 April 2014 (11289)

Units were updated.

Plots and script were commited to the svn.

Non-image files attached to this comment
H1 SEI (SEI)
stefan.ballmer@LIGO.ORG - posted 13:02, Wednesday 09 April 2014 - last comment - 15:51, Thursday 10 April 2014(11244)
ETMX BSC ISI Performance
We Left ETMX running over night (it wasn't very windy so this should probably count as a quite time, I need to make a tool that will tell me that kind of thing).

Sensor correction was installed in three degrees of freedom last night and running. This is ground to stage 1, using Ryan's filter which is targeting the first suspension mode at 0.45Hz.

I've attached three sensor correction plots on/off, blue is sensor correction off the other colors are sensor correction on with various gains. The X direction gain ended up at 1 (which is what it was designed to be) Y and Z came out to be 0.6,
which is very weird.

  There are also three performance plots from last night, with the GS13 and T240 curves.  In general we are buried in the GS13 noise above 0.5Hz (red vs green) except at the BSC pier resonance, we do not have the HEPI L4C feed forward filters installed yet. GS13 rY and rX tilt coupling (yellow line) explains most of the low frequency gs13 signal.  There is clearly some room to relax rZ loop to reduce the gain peaking below 0.2Hz

and again none of this is Stephen's fault I can't figure out how to change the login to me

Rich 

Mabey I hope that I now have the correct plots
Images attached to this report
Comments related to this report
richard.mittleman@LIGO.ORG - 15:51, Thursday 10 April 2014 (11259)SEI

I added the projected motion at the suspension point (Longitudinal), where we aren't noise limited we are completely dominated by table X motion, which of course at low frequency is completely dominated by rotation motion (rY).

Yaw motion only couples to table rZ so I didn't plot that

 

added ETMX and ITMX optical lever signals

Images attached to this comment
LHO VE
john.worden@LIGO.ORG - posted 12:56, Wednesday 09 April 2014 (11251)
YEND Pumpdown

Latest curve. 11 days shown.

loglog plot also attached - note that the BSC6 annulus was probably vented until day 8. There may be a slope change after this date.

Images attached to this report
Non-image files attached to this report
H1 SEI (SEI)
richard.mittleman@LIGO.ORG - posted 12:45, Wednesday 09 April 2014 (11250)
SEI Ground Seismometers

 

   Here is a check list for setting up/working with the ground STS2s (or T240)

   Before touching a STS2 the THREE test masses should be locked using the special non-magnetic screw driver, the T240s do not have locks and are more rugged
 
   After you are done mucking with it

   Make sure that it is aligned using the swizzle stick

   Make sure that the instrument is levelled (bubble level on the sensor)

   Make sure that the feet are locked  (unlocked feet are not stable)

   For STS2s unlock the masses using the special screw driver

   Restore the thermal insulation (exactly what we need is not clear, but we know that at least an enclosure is important)

   Zero the mass positions (this happens at the electronics racks) and read mass positions to make sure that it was successful

 

  ------------------------------------'

 

  Eventually it is nice to take a transfer function from the ground instrument to a set of ISI platform instrument to check the alignment

H1 CDS
david.barker@LIGO.ORG - posted 12:29, Wednesday 09 April 2014 (11249)
h1seih45 binary output cabling fixed

Jim B, Filiburto, Jim W, Dave

we powered down h1seih45 computer and its IO Chassis. Filiburto installed a fourth binary cable to the output port of the second Contec card (HAM5's card). He disconnected HAM4's CN-B from the upper 32 channel input of the binary-output chassis and connected HAM5's CN-A to this port.

We powered up the system, verified that the new logging script worked.

Jim W verified binary output switching for both HAM5 and HAM4 is working correctly.

reboot log shows the startup as:

2014_04_09 12:17 h1hpiham4
2014_04_09 12:17 h1hpiham5
2014_04_09 12:17 h1iopseih45
2014_04_09 12:17 h1isiham4
2014_04_09 12:17 h1isiham5
2014_04_09 12:17 h1iopseih45
2014_04_09 12:17 h1isiham4
2014_04_09 12:17 h1isiham5
LHO VE
john.worden@LIGO.ORG - posted 11:43, Wednesday 09 April 2014 (11245)
BT insulation trial

We have insulated ~100 feet of beam tube as a trial. In the near future vibration measurements will be taken in order to understand the damping performance of this configuration.

Images attached to this report
H1 ISC
alexan.staley@LIGO.ORG - posted 16:03, Tuesday 08 April 2014 - last comment - 16:52, Friday 11 April 2014(11228)
HEPI and ISI ETMX Tripped

(Rich M, Sheila, Alexa)

 

HEPI and ISI ETMX tripped because we were playing with the suspension watchdogs.

Comments related to this report
sheila.dwyer@LIGO.ORG - 17:47, Tuesday 08 April 2014 (11233)

We had a hard time recovering from this trip which caused several more trips, the wd plotting script is not working this afternoon, possibly beause of our network problems so we don't have any plots.  Once HEPI was isolated, we tried letting guardian isolate the ISI. It tripped immediately on CPSs (stage1) after we cleared this and tried again it tripped on GS13 (stage2). 

We then paused the guardian, moved all the blends to start, and gave the gaurdian another try. (note, the ground motion is fairly quiet today).  This tripped again, GS13s. 

We then puased the guardian, and tried the command script, stage 1 level 3, tripped on the actuator limit.  I then stopped taking notes. 

The rough procedure that Rich used to bring it back was damping both stages, turning on 1 DOF at a time RX, RY, Z, RZ, X, Y (stage 1 first, then stage 2).  Then Alexa moved the blends over to Tbetter without anything tripping. 

We don't know why the things that used to work don't anymore, but now ETMX ISI is harder to untrip and neither the guardian nor the command script seem to be able to do it anymore. 

Rich may not have mentioned in the alog, but after our trip the other day while trying to switch blends, he changed the filters from zero crossing to ramp, which should make it easier to switch blends without tripping the ISIs. 

One thing about guardian, its not clear to me how we should unpause if we need to pause it for some reason.  TO pause it we paused all three, stage 1, stage2 and the manager.  Wen unpausing the subpodinates they don't come back in managed mode.  I was able to get them back to managed mode by going to init on all three, but in the meantime they were doing their own thing, but happily didn't trip the ISI.  What is the best way to do this?  Also, maybe the right way to pause and unpause a manager with subordinates is something that needs to be made more obvious to a user. 

Alexa also tried pausing, she only paused the manager, bringing that back was not a problem but it doesn't pause the subordinates.

jameson.rollins@LIGO.ORG - 11:41, Wednesday 09 April 2014 (11246)

quoth Sheila:

We don't know why the things that used to work don't anymore, but now ETMX ISI is harder to untrip and neither the guardian nor the command script seem to be able to do it anymore. 

But you did mention one likely important thing that changed: new blend filters (Tbetter?).  What happens if we go back to Tcrappy?  Do we have the same problems?

also quoth Sheila:

One thing about guardian, its not clear to me how we should unpause if we need to pause it for some reason.  TO pause it we paused all three, stage 1, stage2 and the manager.  Wen unpausing the subpodinates they don't come back in managed mode.  I was able to get them back to managed mode by going to init on all three, but in the meantime they were doing their own thing, but happily didn't trip the ISI.  What is the best way to do this?  Also, maybe the right way to pause and unpause a manager with subordinates is something that needs to be made more obvious to a user.

Alexa also tried pausing, she only paused the manager, bringing that back was not a problem but it doesn't pause the subordinates.

This is definitely sounds like something that could be improved.  It is true that all nodes, manager and subordinates, need to independenty be paused and unpaused.   I'll try to think about how to make that smoother.  In the mean time, here's the procedure that should be used:

  1. pause the manager
  2. pause each of the subordinates (ISI_ST1/2).  order does not matter
  3. ...do work...
  4. request the INIT state in the manager while it's still paused
  5. unpause the manager

The manager INIT state resets all the works, restarts them, and puts them into managed mode.  That should be the most straightforward way to do things for the moment.

sheila.dwyer@LIGO.ORG - 12:19, Wednesday 09 April 2014 (11248)

Thanks Jamie.  

We did try both the command script and guardian with all the blends on start, which used to work.  I don't think we tried turning sensor correction off, which is another change.  

stefan.ballmer@LIGO.ORG - 16:52, Friday 11 April 2014 (11301)SEI
I heard that rumors were spread that this alog was written during an earthquake that we hadn't noticed, so there is no reason to worry about our inability to use guardian or the command scripts to reisolate ETMX.  

That is false, there was no earthquake.  

PS, this is sheila, still loged in as Stefan. 
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