Displaying reports 67201-67220 of 77164.Go to page Start 3357 3358 3359 3360 3361 3362 3363 3364 3365 End
Reports until 19:00, Friday 21 February 2014
H1 SYS
jameson.rollins@LIGO.ORG - posted 19:00, Friday 21 February 2014 (10268)
new guardian overview screen added to sitemap

I added a new GUARD_OVERVIEW screen to the sitemap, accessible from the blue GRD button on the sitemap.

Each block represents a guardian node.  There are place holders for nodes that I expect will show up eventually.  I also expect that more nodes will eventually be added that I haven't accounted for yet.

Each block has a button at the left that will open up the guardian control panel for the node.  The overall background color of the block represents the MODE of the node:

There are three indicator lights, which, from left to right indicate:

Blocks that are white indicate nodes that are current not running.

Images attached to this report
H1 AOS (AOS)
thomas.vo@LIGO.ORG - posted 18:53, Friday 21 February 2014 - last comment - 19:06, Friday 21 February 2014(10267)
ITMX and ETMX OpLevs
Keita K. informed me that whitening for OLs were off for both ITMX and ETMX and after looking at the spectra, I also agreed. So I went out to the field racks to check that the settings were correct.  

The OpLev whitening boards use a binary I/O daughter board to enable the gain stages.  They looked like they were on the correct settings for two levels of whitening, which matched the de-whitening filters set in software so I unplugged and plugged the board back in and this seemed to solve the problem.  I'm happy that this solved the problem, but I'm perplexed on how it happened.  The daughter boards just plug into the front of the chassis with no screws so it may have been bumped loose, not good.

I'm still investigating when this might have happened but it has some pretty big implications for the relatively new damping scripts that Stefan made, I've sent him an email.
Comments related to this report
keita.kawabe@LIGO.ORG - 19:06, Friday 21 February 2014 (10269)

The hardware whitening, which is supposed to be 2 stages of 1:10, was off while the software awhiteners were on for ITM. After Thomas plugged the daughter board off and on, both of the whitening came back.

This was first found while measuring the WFS sensing matrix, as there was a 90 degrees phase difference between WFS and oplev when we were wiggling ITM at 1Hz.

This means that ITM OPLEV was underestimating the angle for ITMX. This is nothing at 0.1Hz, a factor of 1.25 at 0.5Hz, and a factor of 2 at 1Hz.

I don't know if the situation was the same for ETMX, though I know that the ETMX OPLEV whitening changed after Thomas did his trick of plugging out and in. I just don't know if it was no whitening or just one stage whitening or what. That is to be confirmed by Thomas later.

 

 

H1 IOO (IOO, ISC, SYS)
jameson.rollins@LIGO.ORG - posted 18:52, Friday 21 February 2014 (10266)
upgrade of IMC guardian code complete

As reported earlier, the IMC guardian code was upgraded.  This upgrade is now fully complete and committed.

The new IMC guardian module is located at:

USERAPPS/ioo/h1/guardian/IMC.py

This new guardian follows a newer paradigm, whereby we follow a slightly less scrict heirarchy:

Rather than three nodes controlling the IMC locking (ISC_IMC, SUS_MC2, IFO_IMC (manager)), we now have just one: IMC.   The SUS_MC2 module is now identical to all other suspensions, without additional controls states for IMC locking.  The IMC guardian module instructs all IMC suspension nodes (SUS_MC{1,2,3}) to go to their ALIGNED states, and monitors those states.  It then controls all of the "LOCKING" filters in the SUS MC2 controller directly.  The result is much simpler code and simpler control.  I expect that we'll use this paradigm for the rest of the ISC control as well.

The trade off is that we need to be much more carefull about defining which channels are under SUS control and which are under ISC control.  Two different guardians should still never touch the same channels.

The new IMC guardian also adds more sophisticated fault checking (for PSL, ISI, and SUS fault conditions), falling into a FAULT state if there is a problem.  This state then uses the new notification feature of guardian to notify the operator of what the problem is.  Once the fault has been cleared, it proceeds back to the state that was previously requested.

Images attached to this report
H1 AOS
thomas.vo@LIGO.ORG - posted 17:33, Friday 21 February 2014 (10263)
02/21/2014 Ops Summary
Relieving Corey G for a few hours.

- Fil and Luis moving cabling from test stand to BSC10 1:35 PM PT

- Karen cleaning at EY 1:15 PM PT

- Kiwamu doing a DAQ restart 3:01 PM PT
H1 ISC
kiwamu.izumi@LIGO.ORG - posted 17:17, Friday 21 February 2014 (10262)
Red lock from this morning

Evan, Yuta, Kiwamu,

Commissioning of the dithering system is underway.


A summary of the red commissioning from this morning:

H1 SUS (IOO, ISC)
alexan.staley@LIGO.ORG - posted 17:13, Friday 21 February 2014 (10261)
IMC-X Calibration Filters

(Alexa, Jeff)

The IMC-X_M1 and IMC-X_M2 wresg calibration filters are off by a minus sign. I have attached the plots depicted in foton and those produced by Jeff's model. The phase is 180 deg in foton, but should be 0 at DC. I have not updated foton, but an email has been sent out to the relevant parties.

Images attached to this report
Non-image files attached to this report
H1 SEI (ISC, SEI)
hugo.paris@LIGO.ORG - posted 16:52, Friday 21 February 2014 (10258)
BSC-ISI - WD Plotting Fixed

The BSC-ISI watchdog plotting software was reported disfunctional by Hugh earlier this week.

I looked into the scripts and they were fine. What I had missed is that Charles had updated the BSC-ISI WD screens, wich thus needed to receive an svn up at the site to match the latest wd_plotting software update, performed when updating the HAM-ISI models last week.

I run the the svn up on: /opt/rtcs/userapps/release/isi/common/medm/ISI_CUST_CHAMBER_WATCHDOg.adl remotely.

The WD plotting software now works on all the SEI platforms of H1.

Images attached to this report
H1 SUS
arnaud.pele@LIGO.ORG - posted 16:12, Friday 21 February 2014 - last comment - 12:49, Sunday 23 February 2014(10257)
HAM2 HAM3 trip

HAM2 and HAM3 as well as the HEPIs tripped at the exact same time (actuator trip for all of them) @ gps 1077061619 (15:46 PT)

Comments related to this report
arnaud.pele@LIGO.ORG - 20:34, Friday 21 February 2014 (10270)

It happened again this evening when Sheila restarted the Beckhoff at 1077078129. HAM2 and HAM3 ISI actuactors tripped because of a spike in the act signal, as well as the HEPI. cf attached plots

Images attached to this comment
sheila.dwyer@LIGO.ORG - 12:49, Sunday 23 February 2014 (10272)

Jamie and I tried this a few more times..

Stoping and restarting the EPICs database doesn't unlock the IMC.

Stoping PLC2 does unlok the IMC (and FSS) , although in the three times I tried it it didn't trip any HAMs today. Restarting the other PLCs doesn't cause any problems, and it doesn't matter wether or not the Guardian is running. 

H1 DAQ (CDS, ISC)
david.barker@LIGO.ORG - posted 15:53, Friday 21 February 2014 - last comment - 17:02, Friday 21 February 2014(10256)
DAQ Restart, new h1lsc model

15:47 DAQ Restart. Support of h1lsc model change.

Comments related to this report
kiwamu.izumi@LIGO.ORG - 17:02, Friday 21 February 2014 (10260)ISC

As requested by the green team, I edited the LSC model which now allows one to route the LSC sensor signals to the DAC through ALS_C_REFL_DC_BIAS.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 15:35, Friday 21 February 2014 (10255)
Swap Dust Monitor at End-Y
   Tested the dust monitors at End-Y. Found dust monitor #2 (in the test stand cleanroom) was not working. I moved dust monitor #1 (from the spool area cleanroom) to under the test stand, and verify its operation. Dust monitor #2 has been returned to Richard. 
H1 ISC
keita.kawabe@LIGO.ORG - posted 15:12, Friday 21 February 2014 (10254)
Green WFS setting was lost and restored

Seems like it was yesterday's burt-restoring to a bad time for ALS WFS. Manually restored them.

H1 PEM
james.batch@LIGO.ORG - posted 15:01, Friday 21 February 2014 (10253)
Signal injection on seismic channels at mid X
At 14:25:00 and 14:26:00 a signal was injected into the seismometer channels for H1:PEM-MX to test a suspected delay in signals showing up in dataviewer displays in the control room.  There was no delay. Signal was injected by striking the floor of the VEA with a heavy plastic mallet.  There is a time conversion issue on playback in dataviewer in which the UTC time entered is not the time that gets played back, but if GPS time is used, it is correct.  This will be investigated and corrected.
H1 INS (ISC, SEI, SUS)
hugh.radkins@LIGO.ORG - posted 14:35, Friday 21 February 2014 (10252)
EndY ISI/Cartridge ready for Install in chamber

Except for Corey doing some last moment inventorying, the Cartridge is ready for install.  The Test Stand is stripped of all field cables, in-vac cables are all tucked away, accessible areas of the ISI were wiped down (not too much collected it seemed,) and covers are on ready to drop around Stage0 when the assembly lifts from the Stand.  No incumberances seen at this time.

Thanks to Betsy & Mitchell.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 14:26, Friday 21 February 2014 (10251)
TMS alingment today

Keita is getting started with green WFS, so we are doing the strait shot alignment first.

Baffle PD 1: PIT 221.0 YAW  -228.1, saved using the new guardian state

Baffle PD4 PIT 290.6 YAW -289.8 saved as well

Alinged: 255.8PIT  -259 YAW saved as Alinged

I didn't move PR3 since the spot already looks centered on the camera: -244 PIT -254 YAW

H1 PEM (PEM)
richard.mccarthy@LIGO.ORG - posted 14:03, Friday 21 February 2014 (10250)
Dust Monitor 12
Installed DustMonitor 12 in clean room over Ham5.  Alarm levels are set high at the moment as the chambers are closed.
H1 AOS (AOS)
richard.mccarthy@LIGO.ORG - posted 14:00, Friday 21 February 2014 (10249)
ITMx Spool camera
Cleaned the lens and repositioned the camera.  Zoomed in and focused on the ITM.  We can see PRMI spot on optic.  Someone may want to make more adjustments.  The camera view is probably upside down.
LHO VE
kyle.ryan@LIGO.ORG - posted 13:45, Friday 21 February 2014 (10248)
~1130 hrs. local -> Stopped pumping CP8 dewar's vacuum jacket
This completes dewar vacuum jacket pumping exercise.  Summary below: 

8514374 As found = 780 microns -> As left on 12/20/2013 TC = 4 microns, Pirani = 1.5 x 10-3 torr, 
8514372 As found = 28 microns -> As left on 1/23/2014 TC = 4 microns, Pirani = 1.4 x 10-3 torr, 
8514371 As found = 61 microns -> As left on 1/27/2014 TC = 7 microns, Pirani = 1.6 x 10-3 torr, 
8514375 As found = 45 microns -> As left on 1/31/2014 TC = 6 microns, Pirani = ? torr, 
8514376 As found = 49 microns -> As left on 2/4/2014 TC = 6 microns, Pirani = 1.7 x 10-3 torr, 
8514377 As found = 42 microns -> As left on 2/7/2014 TC = 6 microns, Pirani = 1.8 x 10-3 torr, 
8514379 As found = 81 microns -> As left on 2/13/2014 TC = 6 microns, Pirani = 2.0 x 10-3 torr, 
8514380 As found = 58 microns -> As left on 2/21/2014 TC = 7 microns, Pirani = 1.8 x 10-3 torr.
H1 ISC
jaclyn.sanders@LIGO.ORG - posted 10:14, Friday 21 February 2014 - last comment - 17:39, Friday 21 February 2014(10216)
WFS sensing matrix

(Jax, Keita)

Yesterday morning we measured the sensing matrix for the ALS WFS. We did this by Injecting 30000cts at 5Hz into H1:SUS-L2_(I/E)TMX_L2_TEST_(P/Y)_EXC, then measuring the transfer function between H1:ALS-X_WFS_(A/B)_I_(PIT/YAW)_OUT and H1:SUS-(I/E)TMX_L3_OPLEV_(PIT/YAW)_OUT. 

In cavity basis:

Pitch Sensing Matrix: (WFS ct/uRad)

  Hard Soft
A -24871 -44392
B -10475 52694

Pitch Input Matrix: (uRad/WFS ct)

  Hard Soft
A -2.967e-5 -2.5e-5
B -5.899e-6 -1.401e-5

Pitch Output Matrix:

0.707 0.707
-0.707 0.707

Yaw Sensing Matrix: (WFS ct/uRad)

  Hard Soft
A 38421 67629
B -18263 -25945

Yaw Input Matrix: (uRad/WFS ct)

  Hard Soft
A -1.088e-4 -2.838e-4
B 7.665e-5 1.612e-4

Yaw Output Matrix:

0.707 0.707
0.707 -0.707

Raw data: 

Useful information for determining sign conventions from raw data:

1. ETM/ITM Yaw is defined with positive as a counter-clockwise rotation of the optic around the z-axis. 

2. ETM/ITM pitch is defined as positive pitch "down", but ITM oplev is set such that an increase in pitch gives a decrease in oplev measurement.

ETM Yaw:

WFS dB Magnitude Phase
A 86.3 126
B 74.7 -46.1

ETM Pitch:

WFS dB Magnitude Phase
A 93.79 123.2
B 89.5 -57.8

ITM Yaw:

WFS dB Magnitude Phase
A 97.5 -62.58
B 89.9 122.24

ITM Pitch:

WFS dB Magnitude Phase
A 82.8 115.7
B 93.0 -60.7
Comments related to this report
jaclyn.sanders@LIGO.ORG - 11:38, Friday 21 February 2014 (10244)

Edited the main alog to make some of the definitions more clear and add the calculated output matrices.

The input/output matrices have been added to the computer system:

H1:ALS-X_WFS_INPIT_MTRX_...

channel value
1_1 -0.00003
1_2 -0.00003
2_1 -0.00001
2_2 -0.00001

H1:ALS-X_WFS_INYAW_MTRX_...

channel value
1_1 -0.00011
1_2 -0.00028
2_1 0.00008
2_2 0.00016

H1:ASC-OUTMATRIX_P_...

channel value
5_17 0.70711
5_18 0.70711
7_17 -0.70711
7_18 0.70711

H1:ASC-OUTMATRIX_Y_...

channel value
5_17 0.70711
5_18 0.70711
7_17 0.70711
7_18 -0.70711
kiwamu.izumi@LIGO.ORG - 17:39, Friday 21 February 2014 (10264)

Written by Yuta

From the measured WFS sensing matrix, the estimated Gouy phase difference between WFSA and WFSB is 66 +/- 4 deg for pitch and 24 +/- 5 deg for yaw.
I think this is a reasonable measurement. See also alog #10056.

[Method]
Theoretical WFS sensing matrix can be written as;
    DIFF        COMM
WFSA    P*(a*sin(etaA)-b*cos(etaA))    P*(c*sin(etaA)-d*cos(etaA))
WFSB    P*(a*sin(etaB)-b*cos(etaB))    P*(c*sin(etaB)-d*cos(etaB))

a,b,c,d can be calculated by the cavity geometrical parameters(length, RoCs). So, from the sensing matrix measurement, P, etaA, etaB can be estimated by the fitting.
Here, I used the least squares method (scipy.optimize.leastsq) to estimate etaA and etaB, and the measurement error is assumed to be 10% for all the sensing matrix element.

[Result]
Attached. Curves show theoretical WFS signal dependence on the Gouy phase. DIFF and COMM is approximately HARD and SOFT mode of the caivty.

(Comment added: HARD/SOFT is opposite in the measurement?)

Images attached to this comment
H1 SEI
hugh.radkins@LIGO.ORG - posted 08:15, Thursday 20 February 2014 - last comment - 17:01, Friday 21 February 2014(10201)
Thursday AM SEI States--All good except BS ISI Trip

The BS IS tripped on GS-13 watchdog at 1328 utc this morning.  Traffic, wind, something--plotting scripts still not functioning...

Anyway, I brought it back to lvl2 with 750mHz blends on stage2 and T250s on all Stage1 blends except T100mHz_0.44 blends on X & Y dofs.

I reset the target positions, there was about 700nrads on RX and <4um on Z, all other shifts were less.   Please let us know if this impacts any alignments.  This allowed for a one button isolation.

Comments related to this report
hugo.paris@LIGO.ORG - 09:57, Thursday 20 February 2014 (10207)

I reported the WD plotting issue mentioned by hugh last week. Details can be found in LHO aLog #10057

I am not sure what is going on yet, scripting or server access issue, but I am looking into it.

hugo.paris@LIGO.ORG - 10:12, Thursday 20 February 2014 (10208)

The plotting scripts work for the HAM-ISI. WD plotting is still disfunctional on the BSC. I think it is a scripting issue in that case, and I am working towards fixing it:

   Called with arguments: subsystem='ISI_ST1', debug=False, lookback=20, chamber='BS', lookforward=15, device='CPS', rough_trip_time=<object object at 0x7f70dd9050f0>, ifo='H1'
2014-02-20 10:09:21,199 : WDTripPlotter :
    Quitting program
Traceback (most recent call last):
  File "/opt/rtcds/userapps/release//isi/common/scripts/wd_plots/main.py", line 321, in <module>
    main()
  File "/opt/rtcds/userapps/release//isi/common/scripts/wd_plots/main.py", line 241, in main
    rough_trip_time, wd_trip_time_channel_name = util.get_rough_wd_trip_time(ifo, subsystem, chamber)
  File "/opt/rtcds/userapps/trunk/isi/common/scripts/wd_plots/util.py", line 33, in get_rough_wd_trip_time
    channel_suffix = const.WDMON_GPS_TIME_CHANNEL_SUFFIX[_subsystem]
KeyError: 'ISI'   Called with arguments: subsystem='ISI_ST1', debug=False, lookback=20, chamber='BS', lookforward=15, device='CPS', rough_trip_time=<object object at 0x7f70dd9050f0>, ifo='H1'
2014-02-20 10:09:21,199 : WDTripPlotter :
    Quitting program
Traceback (most recent call last):
  File "/opt/rtcds/userapps/release//isi/common/scripts/wd_plots/main.py", line 321, in <module>
    main()
  File "/opt/rtcds/userapps/release//isi/common/scripts/wd_plots/main.py", line 241, in main
    rough_trip_time, wd_trip_time_channel_name = util.get_rough_wd_trip_time(ifo, subsystem, chamber)
  File "/opt/rtcds/userapps/trunk/isi/common/scripts/wd_plots/util.py", line 33, in get_rough_wd_trip_time
    channel_suffix = const.WDMON_GPS_TIME_CHANNEL_SUFFIX[_subsystem]
KeyError: 'ISI'
hugo.paris@LIGO.ORG - 17:01, Friday 21 February 2014 (10259)

The BSC-ISI WD plotting software was fixed, see LHO aLog #10258 for more details.

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