Displaying reports 65961-65980 of 77207.Go to page Start 3295 3296 3297 3298 3299 3300 3301 3302 3303 End
Reports until 09:04, Monday 28 April 2014
H1 CDS
cyrus.reed@LIGO.ORG - posted 09:04, Monday 28 April 2014 - last comment - 10:10, Monday 28 April 2014(11588)
Rebooted cdsfs0

The workstations had lost their NFS mounts, which makes them unhappy.  While it was possible to log in directly on cdsfs0, there was a kernel stack trace in dmesg, so I rebooted it.  It hung on shutdown (not terribly surprising), but power-cycling brought it back with no apparent issues.

Non-image files attached to this report
Comments related to this report
cyrus.reed@LIGO.ORG - 09:17, Monday 28 April 2014 (11592)

Also, cdsfs0 was still trying to NFS mount h2boot which no longer exists, so I corrected this.  'df' shows that the filesystem usage on /ligo dropped from 66% to 64% after reboot, will have to look into that; not that I entirely trust the output from before the reboot based on the presence of a kernel stack trace.

cyrus.reed@LIGO.ORG - 10:10, Monday 28 April 2014 (11594)

The timestamp in the syslog for the start of the stack trace is Apr 27 05:08:27 (local).  This is absent in the cut and paste from the dmesg (which is timeticks only) in the file attached.

H1 AOS
sebastien.biscans@LIGO.ORG - posted 08:36, Monday 28 April 2014 (11587)
ISI Watchdogs trips summary (04/21 - 04/28)

Find attached the watchdogs trips summary of last week/beginning of this week. We'll discuss about it during the SEI portion of the testing meeting tomorrow.

Non-image files attached to this report
H1 CDS (DAQ)
jeffrey.kissel@LIGO.ORG - posted 14:40, Sunday 27 April 2014 (11586)
All Workstations Frozen and/or Failing Authentication
J. Kissel

Came in to complete the work of adding dither paths to the BSFM and QUADs, but found all -- yes all -- workstations frozen. I hard-rebooted (power cycled using the button on the back) opsws6 and opsws5 successfully only to be thwarted by a log-in screen that wouldn't let me log in (it goes black for a second like the log-in process was successful, and then ding-a-lings back to the log-in screen). A few other computers, opsws1 and opws10, just froze on the first re-attempt to log in. The rest I've left as I found them, either frozen in the power-saver screen saver (i.e. blacked out with a small clock on top), or frozen on whatever the last person was doing.

Apparently, the workstations are just as excited to take this sunny day off as I am!

See you tomorrow, CDS. 
#archnemesis
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 09:05, Sunday 27 April 2014 (11585)
CDS model and DAQ restart report, Saturday 26th April 2014

no restarts reported.

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:17, Saturday 26 April 2014 (11584)
CDS model and DAQ restart report, Friday 25th April 2014

model restarts logged for Fri 25/Apr/2014
2014_04_25 16:35 h1lsc

no unexpected restarts.

H1 ISC
keita.kawabe@LIGO.ORG - posted 18:39, Friday 25 April 2014 (11582)
ALS-C_TRY_A_LF ADC is acting up?

EY tripped, recovered, I started realigning Y arm, and at some stage when the arm transmission started to become decent the transmission number started jumping back and forth.

At first I was tempted to think of this as a HOM-related fluke, but when I looked at the time series, it looks as if some incorrect bits are flipped at certain number (though the data is already decimated to 2kHz and the decimation filter should make things somewhat fuzzy).

I'll connect a function generator or something to this channel and see what's going on on Monday.

Images attached to this report
H1 SUS (ISC)
kiwamu.izumi@LIGO.ORG - posted 18:23, Friday 25 April 2014 - last comment - 09:42, Tuesday 13 May 2014(11581)
QUAD angle transfer functions: a factor of 2-ish off

After Richard fixed the issue with the ETMX ESD (see alog 11573) this morning, I briefly took an angular transfer function of pitch and yaw using the oplev. They don't look crazy -- 1/f^2 shape and non-measurable crosscoupling between pitch and yaw. However there was a descrepancy from the model predictions by a factor of 2-ish. I am not sure what makes the descrepancy for the moment. The transfer functions are shown below with the models for comparison.

Anyway, the ESD is functional and ready to go.

 

Note that I included Jeff K's arc-integral-factor which gave an extra factor of 2/pi for the torque in the model. For those who are interested in the details of the calculation, please find it in the attachment (ESD_pitandyaw.m). The raw data are attached as well.

Images attached to this report
Non-image files attached to this report
Comments related to this report
peter.fritschel@LIGO.ORG - 07:40, Saturday 26 April 2014 (11583)

The L1 ESD actuation measurements, applying 2 Hz pitch and yaw signals and looking at the optical lever signals, also show the reponse being a factor of 2 smaller than expected. There seems to be something systematic here that we are missing.

jeffrey.kissel@LIGO.ORG - 09:42, Tuesday 13 May 2014 (11846)
The original templates for this measurement can be found here:
/ligo/home/kiwamu.izumi/Desktop/binary/20140424_ESD_ETMX/dtt/
swept_sine_long.xml (for L2L)
swept_sine_pit_yaw.xml (for P2P and Y2Y)


In addition, they've been copied and committed to the SUS repository here:
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMX/SAGL3/Data/
2014-04-28_H1SUSETMX_L3_L2LPY_SweptSine_1to20Hz.xml
2014-04-24_H1SUSETMX_L3_P2PandY2Y_SweptSine_1to20Hz.xml
H1 CDS
cyrus.reed@LIGO.ORG - posted 17:07, Friday 25 April 2014 (11580)
Workstations

I believe I have ameliorated the wireless problems with the workstations at EX.  Let me know if they continue to misbehave.

Also, I rebooted the dedicated vacuum workstation in the control room since it was running terribly.  It's also had the latest updates applied.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:57, Friday 25 April 2014 - last comment - 11:38, Monday 28 April 2014(11579)
ALS DIFF noise

Sheila, Alexa, Stefan, Daniel

Attached is a spectrum, in Hz/rt Hz, of the PLL control singals for ALS diff and COMM.  This looks simliar to what was measured at Livingston last week.

We made changes to the LSC model to route these control signals into the input matrix to allow us to lock ALS DIFF. 

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 11:38, Monday 28 April 2014 (11600)

These are calibrated in Hz, the spectra plotted above.  The first column is frequency, the second is COMM ASD in HZ/rt Hz,the third DIFF ASD in Hz/rt Hz. 

Non-image files attached to this comment
H1 ISC (SEI)
sheila.dwyer@LIGO.ORG - posted 16:52, Friday 25 April 2014 (11578)
LSC model restart tripped HAM2+3

HAM2+3  HEPI and ISIs have tripped along with MC2+PR2.  We have seen similar behavoir before after a beckhoff restart, but this time it was the LSC model. 

The LSC model restart would have killed the guardian, and unlocked the modecleaner, meaning that the integrator at the top stage of MC2 would get saturated, so it makes sense that MC2 tripped.  The ISIs and HEPIs weren't payload trips, so something else is going wrong. 

This probably could have been prevented if I unlocked the mode cleaner and puased the guardian first.

 

Here is an error message from the plotting script failing:

  File "/opt/rtcds/userapps/release//isi/common/scripts/wd_plots/main.py", line 170, in _BufferDict
    abs_threshold_mask=abs_threshold_mask, host=host, port=port)
  File "/opt/rtcds/userapps/trunk/isi/common/scripts/wd_plots/pydv/bufferdict.py", line 243, in __init__
    self.add_channels(channel_names, wd_state_mask=wd_state_mask, abs_threshold_mask=abs_threshold_mask)
  File "/opt/rtcds/userapps/trunk/isi/common/scripts/wd_plots/pydv/bufferdict.py", line 382, in add_channels
    abs_threshold_mask=abs_threshold_mask)
  File "/opt/rtcds/userapps/trunk/isi/common/scripts/wd_plots/pydv/bufferdict.py", line 344, in __fetch_data
    self.conn.clear_cache()  # clear any saved information from a previous connection
RuntimeError: Input/output error
 

Images attached to this report
H1 General
andres.ramirez@LIGO.ORG - posted 15:59, Friday 25 April 2014 (11577)
Ops Shift Summary
9:00- 10:45 Getting ready to remove payload on HAM5 – Hugh and crew
9:05- 10:00 Performing PET swipe at HAM 5 – Jeff  B.
9:25- Doing inventory by the squeezer bay area – Corey
9:43- Moderate dust  alarms  at both end station 
10:00-11:55 Working at End X-Richard
10:06 PSL check (Done)
10:07: 11:30 Heading to End Y to work on dust monitors – Jeff B. 
10:40 Moving laser barriers around the HAM4 TCS table area – Justin/Cris
11:02-12:45 Heading into H2 Laser enclosure to set up the OFI - Gerardo 
12:37 Heading to End X (cleaning) – Chris
12:49-14:16 Heading to Mid Y (cleaning) – Karen
13:27 Running hose from near HAM4 to inside Diode Room – Jeff B.
13:36-14:48 Back to H2 Laser enclosure to set up the OFI - Gerardo
13:44-14:48 Joining Gerardo in H2 Laser enclosure (LVEA) – Mark B.
13:45-14:41 Setting signs around TCS area in LVEA – Justin
14:47 Beckoff power recycling – Matt/Greg
15:25 Heading to End X to fix CDS workstations - Cyrus
LHO VE
kyle.ryan@LIGO.ORG - posted 15:58, Friday 25 April 2014 (11576)
Dumped unpumped volume seen by PT246B into adjacent pumped RGA volume
This exercise will need to be done occasionally until the Y2-1 port is restored to its nominal configuration (i.e., following the removal of the RGA test setup)
H1 SUS (INS, SUS)
richard.mccarthy@LIGO.ORG - posted 13:20, Friday 25 April 2014 (11573)
ETM-X ESD Power up
Finally installed all of the cabling and interlock boxes for the ESD drive.  There is a short cable at the feed through that goes to a current limiting resistor box.  From that box a 5 conduct cable with SHV connectors goes to the ESD amplifier.   The ESD amplifier has +-430V dc and +-18v dc supplied to it.  The HV supply is interlocked to a Vacuum gauge on the chamber.  

One item of note for the installation is the SHV coax cable label 1 goes to ESD amp port 3 and Coax cable 3 goes to ESD amp port 1.  I have used sharpie to mark this.

If the vacuum gauge trips the HV supply or if we have a power outage the HV supplies need to be switched on by hand.  The +430 Volt supply was found in Sink mode.  I am not sure how it arrived in this state because you would have to program the unit to do this and when the unit was turned on this was not done.  WE WILL have to track this to see if it is a problem. 

Before connecting the unit to Vacuum I checked the output values.

With See Table on attached pdf


								

Non-image files attached to this report
H1 SEI (INS)
hugh.radkins@LIGO.ORG - posted 12:08, Friday 25 April 2014 (11572)
WHAM5 SEI Activity/Status--Locked; ISI Off, HEPI Sensors On
HEPI was locked(put on stops) a couple days ago but its sensors remain on.  At the same time, the ISI interface electronics were powered down to allow decabling the air side.
This morning the ISI was locked (with lockers) and then the 800lbs of dummy payload was removed to make room for Suspension installs.
Thanks to Apollo Scott, Mark & Bubba.
H1 SEI
sheila.dwyer@LIGO.ORG - posted 12:04, Friday 25 April 2014 (11571)
still logging trips

ITMX tripped, this might have been a result of Jim's measurement, but I am not sure. 

 

The gps time was 1082487591

H1 ISC
daniel.sigg@LIGO.ORG - posted 10:14, Friday 25 April 2014 (11570)
RF amp added to COMM PLL BBPD

A ZFL-500LNB+ Mini-Circuits amplifier was added to the output of the COMM PLL BBPD. It is mounted directly to the output connector of BBPD using a SMA barrel. This amplifier was measured to have 29dB-30dB of gain in the 80MHz frequency range. Currently, there is a power supply on top of the enclosure. Longer term, we want to splice this into the +/-15V supply running to the BBPD. All other amplifiers were removed from the path.

H1 General
andres.ramirez@LIGO.ORG - posted 09:15, Friday 25 April 2014 (11569)
Installation Meeting Minutes
8:15-8:35

Mike, Terry, Pablo, Daniel, Steban, Vern, Justin, Richard, Bubba, Kiwamu, Jim, Hugh, Mark, Jason, Aaron, Mitchell, Mark B., Keita, Jeff K.

LVEA is Laser HAZARD

HAM4- Cleaning crew in action – Karen and Chris
Craning activity by APOLLO
HAM5 ISI:  Removing payload –Hugh/Apollo 
TCS tables work continues. David/Aidan
TCS racks work at end stations (Richard & crew)
3ifo BSC ISI assembly  work continues in Staging Building – Mitchell
Dust monitors work at end stations. Switching the dust monitor unit in diode room. Jeff B.
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:28, Friday 25 April 2014 (11568)
CDS model and DAQ restart report, Thursday 24th April 2014

no restarts reported.

H1 SUS (AOS)
mark.barton@LIGO.ORG - posted 11:37, Wednesday 23 April 2014 - last comment - 13:18, Wednesday 02 July 2014(11530)
OFIS vertical Q adjustment

Mark B. and Gerardo

Yesterday (4/22/14) Gerardo and I measured the vertical mode Q of the OFIS for three different positions of the ECD block to try to get the Q in the specified range of 25-30.

The OFIS was set up on the optical bench in the H2 laser enclosure. The ECD block sits on a tray below the payload which is supported by four groups of vertically pointing screws at accessible positions around the edge of the structure. Gerardo had earlier attempted to set the ECD block at the nominal height using the spacer tool provided but found that this was too high and caused interference. He therefore lowered the block until it was just barely clear plus approximately an extra two turns of the 1/4-20 screws. This was our starting point for further adjustments.

To measure the vertical Q, we used the laser pointer and QPD from the monolithic violin mode setup and used a convenient screw on the top of the payload to partially block the beam. We displayed the "pitch" output of the QPD box on a digital oscilloscope with a 1 sec/div timebase and photographed the screen to capture the data. I read off the peak positions with GraphClick, and worked out the logarithmic decrement and Q with Mathematica.

For the initial position, the Q was 10.7. We lowered the ECD by one turn on all the screws and got Q = 18.9. We lowered the ECD another half turn and got Q = 23.3. Finally, today (4/23/14) we lowered the ECD another 3/4 turn and got 27.8, which is in spec.

Attached is a JPG of the setup, a PDF of all the screenshots, and for the fourth and final run, the Mathematica notebook, PDF thereof and the raw data.

Images attached to this report
Non-image files attached to this report
Comments related to this report
mark.barton@LIGO.ORG - 15:06, Friday 25 April 2014 (11575)AOS

We went back on Friday 4/25 and used the same method to measure the longitudinal (parallel to the OFI beam axis) and transverse mode Qs. For the longitudinal measurement we were able to keep the laser in almost the same position, just clipping a different edge, but for the transverse we had to send the beam on an odd diagonal path clipping one corner and then passing through the hole in the beam dump at the end (see photo). The results were

L: 21.3

T: 15.3

V: 27.8 (from 4/23, above)

The spec is <30 per T1000308-v1, p36, so these Qs look good and we propose to leave it like this.

Images attached to this comment
gerardo.moreno@LIGO.ORG - 10:37, Wednesday 30 April 2014 (11646)

I measured the gap between the copper plate and the magnets, 4 mm and all 4 corners.

mark.barton@LIGO.ORG - 13:18, Wednesday 02 July 2014 (12588)

Per request of Jeff Kissel, I extracted the frequencies from the data of 4/23 and 4/25 for the final configuration of the dampers:

L: f = 0.6211 Hz, Q = 21.3
 
T: f = 0.6248 Hz, Q = 15.3
 
V: f = 1.509 Hz, Q = 27.8
 
As before, L/longitudinal was taken to be along the OFI beam axis (the long axis of the bench).
 
T: 15.3
 
V: 27.8 (from 4/23, above)
 
L: 21.3
 
T: 15.3
 
V: 27.8 (from 4/23, above)
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