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Reports until 23:59, Friday 17 March 2017
LHO General
patrick.thomas@LIGO.ORG - posted 23:59, Friday 17 March 2017 (34902)
Ops Eve Shift Summary
TITLE: 03/17 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 69Mpc
INCOMING OPERATOR: Ed
SHIFT SUMMARY: In observing the entire shift. No issues or changes in status to report. Note Cheryl's alog about SDF changes for bounce mode damping if we lose lock.
LOG:

~03:39 UTC Unidentified noise in control room. Sounded vibrational. Lasted for about a minute. HVAC?
LHO General
patrick.thomas@LIGO.ORG - posted 20:07, Friday 17 March 2017 (34901)
Ops Eve Mid Shift Summary
No change in status or issues to report.
H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 17:25, Friday 17 March 2017 - last comment - 12:55, Friday 24 March 2017(34900)
Second measurement of ITMX

I analyzed the HWS data for the lock-acquisition that occurs around 1173641000. The "point source" lens appears very quickly (within the first 60s) and then we see a larger thermal blooming over the next few hundred seconds. I've plotted the data below (both gradient field and wavefront OPD). There are a few obviously errant spots in the HWS gradient field data. Since I'm still getting used to Python, I've not managed to successfully strip these off yet. However, it is safe to ignore them.

Check out the video too. Next step is to match a COMSOL model of thermal lensing with a point absorber to the data to get a best estimate of the size of absorber and the power absorbed (preliminary estimates are of the order of 10mW).

FYI: this measurement compares the system before, during and after a lock-acquisition (ignore the title that says "lock-loss"). The previous measurement, 34853, looked at lens decay before, during and after a lock-loss.

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 18:11, Monday 20 March 2017 (34958)

For your amusement I've attached a GIF file of the same data. My start time is 79 seconds prior to Aidan's "current time".

Images attached to this comment
aidan.brooks@LIGO.ORG - 12:09, Thursday 23 March 2017 (35043)

The integrated gradient field data for H1ITMX is contained in the attached MAT file. It shows the accumulated optical path distortion (OPD) after 2.75 hours following the lock acquisition around 1173640800. This is the total accumulated OPD for a round trip through the CP+ITMX substrates, reflection off ITMX_HR and back through ITMX+CP substrates.

  • H1HWSX_wf_data.x = hswf.grid_x;      % x coordinates of every point in WFcropped
  • H1HWSX_wf_data.xUnits = 'm';           
  • H1HWSX_wf_data.y = hswf.grid_y;      % y coordinates of every point in WFcropped
  • H1HWSX_wf_data.yUnits = 'm';
  • H1HWSX_wf_data.WFcropped = hswf.wf_numerical;        % optical path distortion of every point in WFcropped
  • H1HWSX_wf_data.WFcroppedUnits = 'm';
  • H1HWSX_wf_data.t0 = 1173640800;
  • H1HWSX_wf_data.t1 = 1173649900;
  • H1HWSX_wf_data.deltat = 1173649900-1173640800;
  • H1HWSX_wf_data.comments = 'Integrated HWS data. H1ITMX. Start (reference) and finish times are t0 and t1. x and y arrays contain coordinates. Cropped wavefront is central region where genuine data is believed to be. Outside the 85 mm radius is not real data'

Note: this image is inverted. In this coordinate system, the top of the ITM is at the bottom of the image.

Here is the wavefront data with the superimposed gradient field. The little feature around [+30mm, +20mm] does not appear in the animation of the wavefront or gradient field over much of the preceeding 2.75 hours. My suspicion is that this is a data point with a larger variance that the other HWS data points, rather than a true represtation of wavefront distortion.

 

 

Images attached to this comment
Non-image files attached to this comment
aidan.brooks@LIGO.ORG - 11:58, Friday 24 March 2017 (35069)TCS

I fitted, by eye, a COMSOL model of an absorber (14mm diameter Gaussian, ~25mW absorbed) to the measured HWS data. I then removed this modeled optical path distortion to get the following residual (lower left plot). I then fitted a COMOSL model of 30mW uniform absorption to this model and subtracted it to get the residual in the lower right plot.

 

Images attached to this comment
aidan.brooks@LIGO.ORG - 12:55, Friday 24 March 2017 (35071)

Here's the total fitted distortion from the sum of two COMSOL models (point absorber + uniform absorption):

 

Images attached to this comment
H1 AOS (AOS, SEI, SUS)
cheryl.vorvick@LIGO.ORG - posted 17:00, Friday 17 March 2017 (34899)
Optical Lever 7 Day Trends
Images attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 16:56, Friday 17 March 2017 (34898)
Ops Eve Shift Transition
TITLE: 03/17 Eve Shift: 23:00-07:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 69Mpc
OUTGOING OPERATOR: Cheryl
CURRENT ENVIRONMENT:
    Wind: 6mph Gusts, 4mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.18 μm/s 
QUICK SUMMARY:

No issues to report.
H1 SUS
cheryl.vorvick@LIGO.ORG - posted 16:48, Friday 17 March 2017 (34897)
Bounce Mode Damping
ETMX 9.776 Hz
ITMY 9.831 Hz
Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 16:31, Friday 17 March 2017 (34896)
Ops Day Summary:

TITLE: 03/17 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 66Mpc
INCOMING OPERATOR: Patrick
SHIFT SUMMARY:

 

H1 ISC
kiwamu.izumi@LIGO.ORG - posted 16:12, Friday 17 March 2017 (34892)
Size of spot position move on ITMX during the jitter coupling test

This is a follow up of the jitter coupling measurements (34502, 34389).

I estimated the size of the beam spot shift on the PRC mirrors (PRM, PR2, PR3 and ITMX) which we had moved during this measurement.

Here is the result for ITMX which is of our main interest (34853).

Note: if we assume a 10% calibration accuracy on the suspensions' bias sliders, the size of uncertainty is 3-5 mm.


[The script moves not only the PR3 spot but also all the spots in PRC]

As it turned out, the script that we used was actually moving not only the PR3 spot but also all other PRC mirrors despite the name of the script, pr3spotmove. Historically this script was developed in order to move the degree of freedom that is sensed by POP A QPD (28764). Indeed this script touches IM4, for example, which no doubt moves the spot on PR2.

[The move]

The way this script works is such that as we manually move PRM in angle, the script subsequently moves other optics in a deterministic manner in such way that it results in a change in POP A QPD without disturbing any of the angular control loops. Therefore, for estimating the spot positions, the quantity we need to know is the size of alignment shifts that we introduced on PRM only. This will automatically give us the alignment shifts for the other optics.

Looking at the measurement from the 1st of this month (34502), I found that we have moved PRM by -51 urad in pitch and by -36 urad in yaw. The below is a summary table of the move.

 

 size of the move
PRM PIT   -51 urad
        YAW   -36 urad
PR2 PIT  0
        YAW  0
PR3 PIT  0.27 urad
        YAW  -0.09 urad
ITMX PIT  -1.74 urad
         YAW -1.04 urad

As shown above, the script didn't touch PR2 at all. In addition to the optics listed above, the script also moved IM4, ITMY, ETMX, ETMY, SR2 and SRM at the same time. While some of them can give the same information about the ITMX spot position shift in a redundant way, I have just used the optics shown in the table to simplify the estimation of the spot positions.

[Estimation of the spot positions]

I have made an ABCDEF matrix model (e.g. LLO 9278) for the power recycling cavity with the BS and ITMY omitted. I have used the parameters that Stefan posted at 28747. By plugging the alignment vectors shown in the table, I get the following results.

[v_p, v_2, v_3, v_i] = [-0.27 mm, 016 mm, 1.7 mm, 1.7 mm]

[h_p, h_2, h_3, h_i] = [-0.43 mm, 1.7 mm, -15 mm, -15 mm]

where v and h are vertical and horizontal positions as illustrated in the cartoon below.

Also, since I wasn't sure if the calibration of suspensions' bias sliders are accurate, I assumed a 10% error in each optic and propagated them through the same ABCDEF model to estimate the uncertainties. The uncertainties are estimated to be

[delta v_p, delta v_2, delta v_3, delta v_i ] = [0.22 mm, 0.62 mm, 5.4 mm, 5.3 mm ]

[delta h_p, delta h_2, delta h_3, delta h_i] = [0.14 mm, 0.41 mm, 3.6 mm, 3.5 mm]

Images attached to this report
H1 CDS (SYS)
david.barker@LIGO.ORG - posted 14:30, Friday 17 March 2017 (34895)
Lockloss Matlab Application Roll Out

To run the new matlab lockloss application please do the following:

From the SITEMAP MEDM, Select the 'SYS' pull down, select the last item  'Lock Loss'. This opens the LOCKLOSS_MEDM.adl screen.

Press the 'Run the LockLoss Analysis program' button to start the application. An xterm should open, followed by the matlab2016b splash screen. The UI Figure graphical user interface window will then appear, and you should see no errors in the xterm window (see figure).

We have several minor issues we are working on:

To exit the program, it is best to press the 'X' close button on the top bar of both the UI and the xterm. When the UI window is closed, the matlab session won't return a command line prompt in the xterm without a ctrl-c.

The new lockloss3 python script opens an xterm which shows an error "execvp guardlog: No such file or directory" and does not show the guardlog, but the data plot is generated correctly. Also the xterm requires two 'X' close button presses to dismiss it.

Please email me if there are any other issues with this install. Thanks, Dave

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 13:57, Friday 17 March 2017 - last comment - 13:59, Friday 17 March 2017(34893)
brief power glitch at 20:09 UTS

we had a very brief power glitch at 20:09 UTC (13:09 PDT). It is visible on MAINS_MON trends of all 3 phases in the corner station, and also seen at the end stations (plots attached). Both GC and CDS UPS system reported the event, and the CUR fire panel beeped for about 10 seconds. Many people saw their room lights flicker.

We cannot see any issues with CDS computing, looks like we rode through OK. Jim and I checked the TCS chillers on the MR-mezanine, no problems.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 13:59, Friday 17 March 2017 (34894)

H1 was locked and in observation mode the whole time.

H1 SEI (ISC, PEM, SEI)
jeffrey.kissel@LIGO.ORG - posted 12:31, Friday 17 March 2017 (34889)
ISI Blade Spring Damper Tuning Kit Packed Up, Moved to Optics Lab
J. Kissel

The setup used to tune the frequency of the HAM ISI Tuned Mass Dampers (D0900703) during the most recent HAM6 vent (see LHO aLOG 26488) has been packed up to make room for other up-coming post-O2 installation prep work in the OSB Optics Lab. 

We will need this set up again as we continue to populate the rest of the HAM's ISIs with blade spring dampers (), which necessitate retuning of the already-installed TMDs.

The setup has been put into a bin, and is now stored in the blue set of cabinets in the back "IOO" room of the OSB optics lab, on the right half of shelf 2 of Cabinet 21.

I attach a set of pictures that show the setup as it was found, and then several follow up pictures to show how it was packed and where it lives as of this aLOG.
Images attached to this report
Non-image files attached to this report
LHO VE
logbook/robot/script0.cds.ligo-wa.caltech.edu@LIGO.ORG - posted 12:10, Friday 17 March 2017 - last comment - 13:16, Friday 17 March 2017(34888)
CP3, CP4 Autofill 2017_03_17
Starting CP3 fill. LLCV enabled. LLCV set to manual control. LLCV set to 50% open. Fill completed in 1259 seconds. LLCV set back to 15.0% open.
Starting CP4 fill. LLCV enabled. LLCV set to manual control. LLCV set to 70% open. Fill completed in 130 seconds. TC A did not register fill. LLCV set back to 43.0% open.
Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 13:16, Friday 17 March 2017 (34891)

Raised CP3 by 1% to 16% open

H1 General
cheryl.vorvick@LIGO.ORG - posted 09:06, Friday 17 March 2017 (34887)
Ops Day Transition

TITLE: 03/17 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 66Mpc
OUTGOING OPERATOR: Ed
CURRENT ENVIRONMENT:
    Wind: 11mph Gusts, 9mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.20 μm/s
QUICK SUMMARY:  in Observe, 13+ hour lock, about 5 small earthquakes in the last hour, and at least one earthquake large enough to be seen on 0.03-0.1Hz seismic plot

H1 General
edmond.merilh@LIGO.ORG - posted 08:18, Friday 17 March 2017 (34886)
Shift Summary - Owl

TITLE: 03/17 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 66Mpc
INCOMING OPERATOR: Cheryl
SHIFT SUMMARY:

Quiet night
LOG:
 

H1 General (DetChar)
edmond.merilh@LIGO.ORG - posted 07:52, Friday 17 March 2017 (34884)
Bubba and Apollo to MY Mechanical room

14:45 UTC

H1 General
edmond.merilh@LIGO.ORG - posted 02:54, Friday 17 March 2017 - last comment - 07:53, Friday 17 March 2017(34883)
Shift Summary - Owl

9:50 GRB alert. Livingston contacted for confirmation of alert. Both IFOs observing.

Comments related to this report
edmond.merilh@LIGO.ORG - 07:53, Friday 17 March 2017 (34885)

Not acutally 'Shift Summary'

H1 PSL
edmond.merilh@LIGO.ORG - posted 01:23, Friday 17 March 2017 (34882)
PSL Weekly 10 Day Trends - FAMIS #6139

Box Humidity is elevated since the incursion/flow meter changes done on Tuesday's maintenance. This also shows correlation with Laser Room and Ante Room RH levels (slightly lower) . Inversely, the PMC temp output has marginally decreased. Headflows 1&4 look to be lower and approx equal while #2 is marginally lower. Inversely #3 is showing somewhat of a slight increase. Osc Power Meter flow  shows a downward trend from prior to the maintenance incursion.

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