Displaying reports 64921-64940 of 77211.Go to page Start 3243 3244 3245 3246 3247 3248 3249 3250 3251 End
Reports until 15:59, Tuesday 08 July 2014
LHO VE
kyle.ryan@LIGO.ORG - posted 15:59, Tuesday 08 July 2014 (12652)
Pumping GV7 annulus, vented GV5 annulus (prep for adapter spool removal)


			
			
H1 CDS (PEM)
david.barker@LIGO.ORG - posted 13:50, Tuesday 08 July 2014 (12649)
PEM models and DAQ restarted

WP4715: 

I made two changes to the H1 PEM models:

1. Fixed EX microphone channel names

2. Created quadrature sums on all MAG and ACC (x,y,z) triples if missing.

All PEM models were rebuilt against RCG2.8.4 and restarted. A corresponding DAQ restart was made.

H1 ISC
kiwamu.izumi@LIGO.ORG - posted 13:32, Tuesday 08 July 2014 - last comment - 18:17, Tuesday 08 July 2014(12648)
h1asc model updated: 8 RFM senders added

[Stefan, Kiwamu]

As part of the CDS activity today, we placed new eight RFM senders in h1asc.mdl. It complied fine and I restarted the model. The ASC frontend was then manually burtrestored to 8:00AM this morning. The SVN revision is now at 8346.

This update had been already applied to the Livingston model (i.e. l1asc.mdl) but we had not until today for some reason. Anyway this update was needed not only for the ASC model but also for making the h1iscex(y) model(s) identical to that of Livingston as the iscex(y) were supposed to acquire these RFM channels. After the restart, we checked a couple of the new channels to see if they successfully send signals to the end station. We checked QPD1_PIT and QPD1_YAW of iscex and seemed fine. We didn't check iscey. We didn't edit the ASC master model at all.

 

The name of the RFM blocks:

Comments related to this report
kiwamu.izumi@LIGO.ORG - 14:37, Tuesday 08 July 2014 (12650)

We then checked all the eight new RFM channels and confirmed that they all transmitted signals fine.

Dave noticed that there was a bogus blank channel in the ASC_IPC_STATUS screen and the red indicators for the channels associated with iscex and iscey. We then compiled and restarted iscex, iscey and asc models, resulting back in the all-green-good-status and successful removal of the bogus channel. Good.

stefan.ballmer@LIGO.ORG - 15:06, Tuesday 08 July 2014 (12651)ISC

(Kiwamu, Stefan)

We implemented the changes needed for driving the ALS_WFS_AUTOCENTERING servo from the iscex/ey models. In detail:

- updated ALS_END.mdl model to import LLO changes (include direct dither drive to END PZT's and additional link to QPD error points, see Kiwamu's log entry for ASC changes).
- adapted h1iscex for these changes, including links from ASC (SVN revision 8345)
- adapted h1iscey for these changes, including links from ASC (SVN revision 8347)
- updated ALS_CORNER_ASC.mdl from SVN (adds TRX_A_LF_OUT TRY_A_LF_OUT to science frame)
- Added ALS WFS AUTOCENTERING filter modules to ALS_END (SVN revision 8348), h1iscex and hy1iscey (SVN revision 8349)

- recompiled h1asc, h1iscex and h1iscey

- burt restored to 7am ASC


TBD: medm screens for:
 - screen for ALS WFS Autocentering
 - update ALS_CUST_ENDSTATION.adl screen for IAL to iscex/y PZT/QPD link
 

kiwamu.izumi@LIGO.ORG - 18:17, Tuesday 08 July 2014 (12667)

In respose to Stefan's previous log, I completed the remaining missions that are:

 - screen for ALS WFS Autocentering
 - update ALS_CUST_ENDSTATION.adl screen for IAL to iscex/y PZT/QPD link

The new auto-centering screen is called ALS_CUST_WFS_AUTOC.adl and it resides in als/common/medm. It is checked into the svn.

H1 SEI
hugh.radkins@LIGO.ORG - posted 12:17, Tuesday 08 July 2014 (12647)
WBSC9 ETMX HEPI Parker Valve Leak & Motor Noise

The minor leak at Pier2(SW) on BSC9 has filled its catch and has dripped out; it has taken months to fill the catch so it isn't going to make a mess in the next few weeks though.  I guess I failed to mind/clean this up frequently enough to prevent the overflow.  I could not access it this time though as the ameristating of the west side prevents getting to this and I didn't want to tear this down.  In case it isn't clear, the drip is outside the ameristat away from the west door.

The HEPI pump station motor/pump noise has changed and there is an obvious wobble in the pump side coupler.  John has recommended a few tests and I'll try to implement these soon.

LHO General
corey.gray@LIGO.ORG - posted 11:10, Tuesday 08 July 2014 (12643)
Morning Installation Meeting Minutes

(Took these notes for Gerardo)

H1 CDS
james.batch@LIGO.ORG - posted 10:42, Tuesday 08 July 2014 (12646)
Updated Dataviewer installed for Ubuntu and OS X
WP 4719

Installed updated dataviewer to fix a bug that incorrectly displayed trend mean data as 0 when max and min values are integers.
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:02, Tuesday 08 July 2014 (12642)
CDS model and DAQ restart report, Monday 7th July 2014

model restarts logged for Mon 07/Jul/2014
2014_07_07 00:40 h1fw0
2014_07_07 01:38 h1fw0
2014_07_07 02:46 h1fw0
2014_07_07 03:45 h1fw0
2014_07_07 04:39 h1fw0
2014_07_07 05:27 h1fw0
2014_07_07 05:43 h1fw0
2014_07_07 06:39 h1fw0
2014_07_07 07:33 h1fw0
2014_07_07 07:41 h1fw0
2014_07_07 08:40 h1fw0
2014_07_07 09:39 h1fw0
2014_07_07 11:24 h1fw0
2014_07_07 11:53 h1fw0
2014_07_07 13:02 h1fw0
2014_07_07 13:25 h1fw0
2014_07_07 14:43 h1fw0

h1fw0's problem (purple) resolved when solaris QFS box rebooted. No unexpected restarts.

H1 IOO (SUS)
jeffrey.kissel@LIGO.ORG - posted 23:06, Monday 07 July 2014 - last comment - 10:02, Tuesday 08 July 2014(12625)
H1 HAUX Alignment Biases -- Won't Risk Physically Offloading
J. Kissel

Executive Summary: 
(1) I believe we DO NOT need to manually alleviate the alignment on the IMs, but it's close.
(2) Assuming a worst-case scenario, IM2 would use up ~80% of it range to maintain alignment.
(3) The alignment slider calibration I recommend we use is:
P: 0.21 +/- 0.015 [urad/ct]
Y: 0.39 +/- 0.009 [urad/ct]
(4) Calculating the calibration from from a model of the signal chain fails; there's still unknowns in the signal chain that add up to discrepancies of 2 and 4 for P & Y.
(5) Given the EUL2OSEM gain, and the usage of the same actuators for P & Y, the actuators can drive 2.96 [mrad] in P and 1.62 [mrad] in Y if alignment offset is needed in both DOFs. 
(6) We would need to relieve 1 [mrad] of pitch, which is about at the limit of the mechanical alignment precision.

I have *not* installed the calibration gain. I'll do it tomorrow.

----------
During the last integrated testing stint, good alignment of IM2 and IM4 was believed to be at the limit of the DAC range of their OSEMs, given their actuation strength has now been decreased by ~10 (see LHO aLOGs 8767, 8759). 

However, due the confusion of uncalibrated alignment sliders, artificial limitation of the slider range on the MEDM screen, 16-bit vs 18-bit DAC range, coil driver strength changes, computer reboots, electronics being swapped in and out, and a few vent cycles ... I think the saturation had been misreported. 

Currently, the worst offending with the largest alignment bias request is IM2 with + ~81000 [ct] out of +/- 2^17 = 131072 [ct], or 61% of its range. I've confirmed with the OSEMs that the range of drive is still roughly +/- 6 [mrad] in P and Y, and the calibration of the slider counts into [urad] is
P: 0.21 +/- 0.015
Y: 0.39 +/- 0.009
where the uncertainty is the standard deviation across the four IMs. Unfortunately (and the reason why I just measured it), a component by component model of the calibration doesn't make any sense, even after using measured compliance values. More on that later.

So the questions are:
- Is +/- 6 [mrad] enough to cover the alignment change from in-air to in-vacuum? Yes. Data from prior to the vent and before installation attacked shows that the optics move by at *most* 1 [mrad], where the majority moved of order 100 [urad]. So, assuming IM2 moves the worst amount of distance (which this past vent shows it moved 148 and 174 [urad] in P & Y respectively) that's only an additional ~17% on top of 61%, or 78% (and the damping control signal variation on this is a negligible ~0.1%).
- Is it worth trying to mechanically alleviate the alignment for 78% and 2 [mrad]? We have no experience HAUX aligners on site for this remaining week in which we indeed to keep HAM2 open. The precision to which one can mechanically align the SUS is roughly 1 [mrad] (see section 2.1.1 of T1200469). Given Murphy's law, the lack of alignment references, the amount of stuff we've already changed in HAM2 with the IMC bypass, and the uncertainty which still swirls around the exact numbers and direction, I say it's a gamble not worth taking.

Below is a collection of information needed to assess how much the optics need moving.

I've surveyed the (1) alignment sliders, (2) OSEM sensor values, and (3) DAC output values over the past 30 days, to get a feel for how much we need to move. However, three events have occured that complicate the story:
(a) On 2014-June-04 16:21 UTC to 2014-June-04 23:13 UTC, Filiberto and Aaron swapped out / investigated AA and AI chassis of H1sush2b, so OSEM sensor signals went dead (no aLOGs, but Fil confirms that's when his work-permit for this swap was open via email).
(b) On 2014-Jun-12 17:21 UTC, a power glitch necessitated a restart of the h1sush2b computer (among many others). This reboot reloaded a save.snap value that must have been out of date, because IM4 P & Y alignment value changed by a few hundred counts (see below).
(c) On 2014-Jun-24 ~23:00 UTC (+/- 15 [minutes]), the alignment was modified in order to accommodate the IMC bypass.
"IM2_P_35DayTimeline.pdf" shows this timeline on IM2 P only for clarity, but "OSEMPosition_2014-06-01_to_2014-07-04.png" shows that all 8 DOFs show similar features over the 35 day period.


(1) OSEM sensor values, before the vent (Jun 1), after the vent, once the alignment had asymptotically stabilized just before the (a) AA/AI chassis shutdown on the Jun 4, and after the alignment had been left alone from the IMC bypass during the 4th of July weekend:

% Pre-vent            P          Y
osems(1).disp =  [  225.0     1709.5;... % [urad] IM1
                   1380.6      -45.5;... % [urad] IM2
                    447.6      620.0;... % [urad] IM3
                  -3034.0    -2174.8];   % [urad] IM4
% Post-vent           P          Y
osems(2).disp =  [  195.7     1772.9;... % [urad] IM1
                   1528.8     -220.2;... % [urad] IM2
                    511.8      599.3;... % [urad] IM3
                  -3167.0    -2302.0];   % [urad] IM4
% Post-IMC Bypass     P          Y
osems(3).disp =  [  335.0     1851.0;... % IM1
                   2179.0      165.0;... % IM2
                   1522.0      816.0;... % IM3
                  -3201.0    -2212.0];   % IM4
       %   P          Y
diff =  -29.3         63.4  % [urad] IM1
        148.2       -174.7  % [urad] IM2
         64.2        -20.7  % [urad] IM3
         -133       -127.2  % [urad] IM4


(2) Alignment slider values, before vent and after their change from (c) above. These slider values *have* not been calibrated into physical units, as the alignment bias gain is 1. The only P&Y gain between the sliders and the DAC are the EUL2OSEM matrices compensating for the lever arm, which have a gain of +/- 8.594. 

Optic DOF      Pre-vent     After Glitch     After Realignment       Diff [ct]
   IM1 P         0.0           (same)             (same)               n/a
       Y      1469.0           (same)             (same)               n/a
   IM2 P      4600.0           (same)             7600.0              +3000
       Y      2000.0           (same)             (same)               n/a
   IM3 P     -1397.9           (same)             2980.0              +4377
       Y      1060.8           (same)             2120.0              +1060
   IM4 P     -2350.0           -2707.0            (same)              -357
       Y     -3607.0           -3390.0            (same)              217


(3) DAC Output values, before the vent

Optic     DOFs         DAC Output  
IM1      UL / UR     -12631 / -12631
         LL / LR     +12631 / +12631

IM2      UL / UR     +22344 / -56720
         LL / LR     +56720 / -22344

IM3      UL / UR     -21130 /  +2897
         LL / LR      -2897 / -21130

IM4      UL / UR     +10802 / +51194
         LL / LR     -51194 / -10802


------
What I think the alignment slider gain should be:
If I use the same method as used in other susTypes (see e.g. LHO aLOG 4730), where the EUL2OSEM matrix properly compensates for the lever arm an number of OSEMs, 

OPTICALIGN GAIN [cts/urad] = ( DAC [V/ct] * Coil Driver [A/V] * Coil/Magnet [N/A] * HAUX M1 to M1 [rad/N.m] * 1e6 [urad/rad] )^-1
                           = ( (20/2^18)  * 0.988e-3          * 0.0158            * 74.23 (for Pitch)       * 1e6            )^-1
                           = 11.311 [ct/urad] (for Pitch)
                          or 0.08841 [urad/ct]
OPTICALIGN GAIN [cts/urad] = ( DAC [V/ct] * Coil Driver [A/V] * Coil/Magnet [N/A] * HSTS M1 to M1 [rad/N.m] * 1e6 [urad/rad] )^-1
                           = ( (20/2^18)  * 0.988e-3          * 0.0158            * 73.87 (for Yaw)         * 1e6            )^-1
                           = 11.367 [ct/urad] (for Yaw)
                          or 0.087974 [urad/ct]

-- a factor of 2 and 4 off the measured values -- where the DAC gain is taken from T1200311, the coil driver transconductance from T1200264, and coil magnet strength from T1000164, and the compliance from the collection of H1 HAUX measurements in LHO aLOG 8344, since the transfer function model still does not well-match the transfer function data.

--------
The final attachment "2014-07-08_H1HAUX_AlignmentOffset_Calibration.pdf" shows the measurement results of simply taking the alignment sliders at several data points along its range, and pulling the OSEM value off of a data viewer trace. Because I left the opposing DOFs offsets ON during the range walk through, some of the SUS which already had appreciable offsets reached saturation more quickly (i.e. IM4P, IM2Y, and IM2Y). For those data sets, I removed the end points from the fitting routine (which was just a first order polyfit, nothing fancy).

Data was reduced and plots were created by
${SusSVN}/sus/trunk/HAUX/H1/Common/alignmentrelief_Summer2014.m
Images attached to this report
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 10:02, Tuesday 08 July 2014 (12645)
I've installed the above calibration gains, adjusted the alignment offsets to yield the same displacement, and captured a new safe.snap.

The new alignment offsets are

H1:SUS-IM1_M1_OPTICALIGN_P_OFFSET 0
H1:SUS-IM1_M1_OPTICALIGN_Y_OFFSET 3786.1
H1:SUS-IM2_M1_OPTICALIGN_P_OFFSET 35849.3
H1:SUS-IM2_M1_OPTICALIGN_Y_OFFSET 5154.7
H1:SUS-IM3_M1_OPTICALIGN_P_OFFSET 14057
H1:SUS-IM3_M1_OPTICALIGN_Y_OFFSET 5464
H1:SUS-IM4_M1_OPTICALIGN_P_OFFSET -12769.1
H1:SUS-IM4_M1_OPTICALIGN_Y_OFFSET -8737.1
Logbook Admin Feature Requests
jameson.rollins@LIGO.ORG - posted 18:49, Monday 07 July 2014 (12640)
Search results "Display reports" links should include "Next" and "Prev"

Currently, the bottom of a search results page includes the "Displaying reports X-Y of Z. Go to page Start 5 6 ... End" links.  Conspicuously absent from the links are links for the Next and Previous pages of results.  Navigating through the results therefore always requires more energy than should be needed, to identify the number of the current results page, and select the next number.  If a Next link was provided, it would be much easier to scroll through search results.

Better yet, the subsequent results should just automatically show up at the bottom of the page when scrolling down.  This can be achieved fairly simply with the jQuery jScroll plugin.

H1 SUS
betsy.weaver@LIGO.ORG - posted 17:23, Monday 07 July 2014 (12639)
H1 ITMy SUS work re-resumed

This morning, I finished the cable routing through the reaction chain to the lower stage OSEMs.  Then, Travis and I worked on fully suspending both chains.  After adjusting out some course pitch observed at the test mass and CP, we noticed we have a large pitch at the top mass.  Both chains are also hanging about 1-2mm high (we have shims to remove which will correct this later when IAS sorts any SUS+HEPI height issues).  We'll continue the coarse pitch work tomorrow which is a bit of a head scratcher.  Both chains have been left ~fully suspended.

H1 SUS
jeffrey.kissel@LIGO.ORG - posted 17:13, Monday 07 July 2014 - last comment - 09:40, Tuesday 08 July 2014(12638)
New H1 SUS ITMY Open Light Current Values
J. Kissel, T. Sadecki, B. Weaver,

Because it was free, we took some new open light current values for H1 SUS ITMY, the have been installed. No values have changed more than 10-15%, but all have gone down since we last took these (see LHO aLOG 4549).


OSEM     Open        Normalizing    Compensating
        Light           Gain           Offset
       Current [ct]
M0F1     27894         1.075           -13947
M0F2     27280         1.100           -13640
M0F3     27059         1.109           -13530
M0LF     25600         1.172           -12800
M0RT     23555         1.274           -11778
M0SD     27538         1.089           -13769
R0F1     23855         1.258           -11927
R0F2     24148         1.242           -12074
R0F3     24696         1.215           -12348
R0LF     25745         1.165           -12872
R0RT     23838         1.258           -11919
R0SD     24543         1.222           -12271
L1UL     27800         1.079           -13900
L1LL     28750         1.043           -14375
L1UR     27706         1.083           -13853
L1LR     29654         1.012           -14827
L2UL     23978         1.251           -11989
L2LL     20272         1.480           -10136
L2UR     16251         1.846            -8125
L2LR     17254         1.739            -8627

Note that these values still need to be captured in a safe.snap, and the OSEM Chart needs updating.
Comments related to this report
jeffrey.kissel@LIGO.ORG - 09:40, Tuesday 08 July 2014 (12644)
I've captured a new safe.snap, and committed it to the svn repo.
LHO General
bubba.gateley@LIGO.ORG - posted 16:21, Monday 07 July 2014 (12636)
Apollo crew
The north door on ham 5 was removed this morning. 
We replaced the adapter spool at GV 7 and installed the annulus piping. The cleanroom was transported from the north bay to north / west bay main crane access area.
H1 CDS (DCS)
david.barker@LIGO.ORG - posted 16:05, Monday 07 July 2014 (12635)
h1fw0 down, QFS file system diagnostics ran.

Dan and Dave.

h1fw0 was down for about an hour today, Dan performed diagnostics on the /ldas-h1-frames file system. He first tried a samfsck on the file system, but the problem reappeared within 5 minutes. After many other investigations we ended up rebooting the h1ldasgw0 machine and h1fw0 has been stable for over an hour. 

H1 SEI (SEI, SYS)
justin.bergman@LIGO.ORG - posted 13:08, Monday 07 July 2014 - last comment - 07:39, Tuesday 08 July 2014(12631)
difficulty recovering ETMY ISI through Guardian

While trying to untrip the ETMY ISI through guardian the ISI stage 2 watchdogs tripped (again). JeffK suggested manually turning on the Gain filters for the GS-13 inputs (to reduce the analog gain by 10...or LOW GAIN mode), resetting the watchdogs again, then requesting Fully_Isolated from guardian.

if it is necessary to reduce the gain by hand, shouldn't guardian handle this?

 

Images attached to this report
Comments related to this report
jameson.rollins@LIGO.ORG - 16:21, Monday 07 July 2014 (12637)

> if it is necessary to reduce the gain by hand, shouldn't guardian handle this?

Yes it should, if it is determined that this is necessary to achieve full isolation.  However, this wasn't previously necessary, so something in the system has clearly changed.

But either way, more information is needed.  Did you try letting guardian handle the isolation with the default procedure more than once?  If so, did it trip the GS13 in the same way every time?  Presumably lowering the GS13 input gain did allow the isolation to succeed?  Was there other activity going on around ETMY at the time?  Have any other parameters of the system changed, such as cart bias offsets on any of the HPI or ISI dofs?

justin.bergman@LIGO.ORG - 07:39, Tuesday 08 July 2014 (12641)

All good questions. Mostly I just wanted to get a trip report logged as a data point to see if this is happening with some frequency and not getting reported.

There was no other work going on at EY at the time and the seismic background was not particularly choppy. I did not let guardian try a second time before changing the gain. As for changes to the DOFs or bias, I don't know. Guess we'll just see if it happens again. Thanks.

H1 SUS
jeffrey.kissel@LIGO.ORG - posted 17:28, Monday 30 June 2014 - last comment - 17:10, Monday 07 July 2014(12544)
H1 SUS ITMX Discrepant Drive Strength Fixed.
J. Kissel, A. Pele, T. Sadecki, B. Weaver,

After another day's worth of fumbling and hand-waving, we've finally traced the discrepant transfer function magnitude to a loose cable connection at the air-side of the feedthrough. In the course of attempted fixes, we measured a few more things, moved a few more things, replaced the R0 F2 and F3 OSEMs, but the only thing that fixed it was the cable connection. This flaw with the electronics chain should have been found earlier with our cable swap on Friday, with remeasuring the open light current, and with Arnaud's DC actuation test below, but frustratingly, it did not. But we found it. 

I'm in the process of getting formal transfer function measurements now, but I'm confident from what I'm seeing thus far that this SUS is read for close-out. Will post comparison TFs once they're finished.
We have exORSIIIIIIIZED the demons. This SUS is clee-uh.

Details (In rough chronological order)
-------
- Arnaud compared the ETMY and ITMX R0 F2 to F2 and F3 to F3 drive at DC using the alignment offsets (the only QUADs available, so take ERM and TCP chain comparison with a grain of salt), and concluded that the chains are driving with comparable and within a chain F2 and F3 are of comparable strength with such a quick study. 
- Betsy retook an L2L transfer function (just for sanity's), saw the same discrepant factor of two -- and some more Yaw resonant cross-coupling. Still F2 shows the majority of the badness.
- Decided just to swap the OSEMs, and hopefully move on. Below are the new serial numbers, open light current, and compensation gains and offsets. These *have* been installed. We'll take a new safe.snap this evening after all the commotion has died down.
- Betsy & Travis poked at this, looked at that, iterated with measurements several times on the floor.
- At last, Betsy went a long the signal chain, and made sure all connections were secure, and finally found this bad connection at the in-air connection at the feedthrough.
- Simultaneously, Travis loosened up the the cable loop from the optical table to the top mass. This may have alleviated the extra Yaw peaks that had shown up today. 

Open light current values and serial numbers for the new OSEMs.
      Raw    New     New        S/N
      ADC    Gain    Offset      
R0F2 25646   1.170   -12823     077
R0F3 26554   1.130   -13277     147

We'll also update the OSEM chart and grab a new safe.snap once transfer functions are finished.
 
Comments related to this report
jeffrey.kissel@LIGO.ORG - 21:57, Monday 30 June 2014 (12555)
TFs look great. For some reason the comparison script is failing on my laptop; will post comparisons tomorrow. But, for all intents and purposes, H1 SUS ITMX is ready for close-out. A victory for team SUS!
Non-image files attached to this comment
jeffrey.kissel@LIGO.ORG - 09:00, Tuesday 01 July 2014 (12560)
Comparison plots. All looks well, as expected. To demonstrate the problem, I also include the prior *bad* measurements of the reaction chain (2014-06-27_2117).
Non-image files attached to this comment
arnaud.pele@LIGO.ORG - 17:10, Monday 07 July 2014 (12634)

More transfer function measurements were taken on the lower stages of ITMX last tuesday.

Interesting things to notice :

1. The measurements with no top mass damping (1st and 3rd attachments) appear to show resonnances which are not predicted by the model. Those are most certainly resonnances of the reaction chain moving because of the reaction force (e.g. 3rd page of 1st attachment : resonnance at 0.66Hz is not predicted by the model, but matches with the frequency of the first yaw mode measured on the top mass reaction chain, cf this measurement from alog 12555).

2. There is a factor of 2ish discrepancy between the model and the measurement for both UIM and PUM

Non-image files attached to this comment
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