Displaying reports 48521-48540 of 87894.Go to page Start 2423 2424 2425 2426 2427 2428 2429 2430 2431 End
Reports until 18:29, Monday 12 February 2018
H1 CAL (CAL, ISC, SUS)
evan.goetz@LIGO.ORG - posted 18:29, Monday 12 February 2018 - last comment - 16:34, Wednesday 28 March 2018(40508)
Compensation zero moved from ESD output filter bank
Evan G., Jeff K.

We moved a compensation zero out of the ESD output filter bank for each quadrant that had generated an uncompensated 5.2 kHz pole in the DARM loop (see LHO aLOG 33927). This resulted in an effective delay of ~20 usec. There is adequate roll off already from a low pass filter in the ESD driver, so moving this out of the DARM loop will be minimally impactful. Instead, the compensation zero will be a compensation pole in the CAL-CS path and doesn't result in an additional 5.2 kHz zero being added to the Foton filter.

We leave the filter in place and turned on, but the design string is now simply zpk([], [], 1, "n")

The new filter is installed in CS_DARM_ANALOG_ETMY_L3, FM5: zpk([], [3245.33075], 1, "n") (this comes from the mean of the summing node poles, see 27619)

Removing this from the DARM path means that we need to include these as an uncompensated poles in the DARM model and reduce the unknown actuation delay by 20 usec. This will bring the unknown actuation delay down to ~40 usec.
Comments related to this report
jeffrey.kissel@LIGO.ORG - 16:34, Wednesday 28 March 2018 (41189)
Associated with FRS Ticket 7351.
LHO VE
kyle.ryan@LIGO.ORG - posted 16:45, Monday 12 February 2018 - last comment - 20:08, Monday 12 February 2018(40506)
CP4 decommissioning status
see WP #7343 

1630 hrs. local -> Lowered CP4's level via CDS PI control set point to 70% down from 75%.  I expect this new pump level value should be reached prior to my leaving tonight.

Will start tomorrow morning with step 2 of WP #7343 (as step 1 was done this weekend).  Delay is the result of competing employee requirement/task in addition to my desire to complete construction of a relay box that will act as a second interlock and isolate the scroll pump as a function of foreline pressure.  As is, the foreline isolates only at the absence of 120VAC as seen by the scroll pump motor windings (i.e. one layer of protection - prefer two layers).  
Comments related to this report
kyle.ryan@LIGO.ORG - 18:41, Monday 12 February 2018 (40510)
1830 hrs. local -> Lowered CP4 level target down to 65% from 70%
kyle.ryan@LIGO.ORG - 20:08, Monday 12 February 2018 (40511)
2010 hrs. local -> looks stable.  Going home now.
H1 AOS (CDS, DetChar)
joshua.smith@LIGO.ORG - posted 16:25, Monday 12 February 2018 (40505)
First impressions of units in NDS2

Cross-posting from LLO alog here: https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=37737 

H1 SUS
betsy.weaver@LIGO.ORG - posted 16:03, Monday 12 February 2018 (40504)
ETMX AERM07 Prism #1 glued

Today, I knocked out the jig calculations for the AERM07 prism placements and updated the spreadsheet for all 4 new AERMs (05, 06, and 08 have been finished, spreadsheet E1000828).  Gerardo did a quick spotcheck of my work, then I went to the lab and glued the first prism on (specifically "180 ARM").  The EP30-2 epoxy is a newly procured vial and passed the usual pre-bake test, as usual.

LHO General
thomas.shaffer@LIGO.ORG - posted 16:00, Monday 12 February 2018 (40492)
Ops Day Shift Summary

TITLE: 02/12 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY: PSL was shut down and 70W amplifier work began. More work continuing down at MY for CP4. Team SUS working on ETMY. And SQZ crew is prepping for next week's install.
LOG:

H1 IOO (IOO, PSL)
cheryl.vorvick@LIGO.ORG - posted 12:59, Monday 12 February 2018 (40501)
PSL ISS Second Loop (in HAM2) QPD segment offsets set

Given that we have no laser light, confirmed by images of the PSL and cameras looking into HAM2, I set the PSL ISS Second Loop Array QPD dark offsets.  I accepted the values into SDF, and also had to accept the offset switch being on for all 4 segments, and I've confirmed that these offsets were zero in Feb 2017, during O2.

OFFSETS: Seg1 = 0.180, Seg2 = 0.180, Seg3 = 1.540, Seg4 = 2.370, and the SUM, which had been at +4.2, is now oscillating around zero.

I put an offset of -2.0 on the SUM to prevent it from going negative.  I tried using -1.0, but the pitch and yaw signals were still occasionally railing +/-32K.  The SUM during Feb 2017 reached 60K counts, so an offset of -2.0 is small.

Changes are recorded in the attached screenshot:  Left side shows current settings, rich side shows a snapshot of the QPD segment settings as found (zeros).

Images attached to this report
LHO General
thomas.shaffer@LIGO.ORG - posted 10:06, Monday 12 February 2018 (40497)
LVEA is Laser SAFE

Peter has transitioned the LVEA to Laser SAFE

Images attached to this report
H1 PSL
edmond.merilh@LIGO.ORG - posted 09:44, Monday 12 February 2018 - last comment - 09:47, Monday 12 February 2018(40495)
PSL Weekly Report - 10 Day Trends FAMIS #6186

PSL tripped this past Saturday. HPO has been bypassed and powered down for water removal and dry-out in preparation for the 70W amp install.

Images attached to this report
Comments related to this report
edmond.merilh@LIGO.ORG - 09:47, Monday 12 February 2018 (40496)

Correction. This is FAMIS task#6187

LHO General
thomas.shaffer@LIGO.ORG - posted 09:23, Monday 12 February 2018 (40494)
Morning Meeting Minutes

PSL

    Starting 70W amp work after meeting.

Commissioning

    HAM6 looks good, DRMI was locked. Looking at HAM6 South door removal this week, as well as placing ISCT6 being placed just outside the cleanroom. Will capture SDF.

Vac

    MY CP4 work continues; craning, electrical, and piping work.

    More discussion on the HAM6 septum view port cover.

EX

    Activity will be ramping up at this end station, including: prepping cleanrooms, prepping weld room, PCAL alignment, ALS power supply, staging equipment, VE interlock.

Film crew will be on site Thursday Friday.

Will be going laser SAFE until we need lasers for commissioning. Work Safe!

H1 PSL
thomas.shaffer@LIGO.ORG - posted 08:21, Monday 12 February 2018 (40493)
PSL Weekly Report


Laser Status:
SysStat is good
Front End Power is 34.81W (should be around 30 W)
HPO Output Power is 29.17W
Front End Watch is GREEN
HPO Watch is RED

PMC:
It has been locked 1 days, 15 hr 1 minutes (should be days/weeks)
Reflected power = 3.255Watts
Transmitted power = 22.57Watts
PowerSum = 25.82Watts.

FSS:
It has been locked for 0 days 2 hr and 9 min (should be days/weeks)
TPD[V] = 0.7296V (min 0.9V)

ISS:
The diffracted power is around 2.7% (should be 3-5%)
Last saturation event was 1 days 15 hours and 2 minutes ago (should be days/weeks)

Possible Issues:
FSS TPD is low

LHO General
kyle.ryan@LIGO.ORG - posted 16:02, Sunday 11 February 2018 - last comment - 20:29, Sunday 11 February 2018(40487)
Changed CP4's level PID setpoint to 75% full (down from nominal 92%)
I'll put in a Work Permit tomorrow that details the process of letting CP4 go "dry".  Starting from 75% full will give a little head start to the lengthly process.  Chandra R. has lots of activities related to CP4's decommissioning scheduled for this week so we don't have a lot of "wiggle room".  


This step may well result in CP4 level alarms tonight.  This is expected and is being monitored remotely. 
Comments related to this report
david.barker@LIGO.ORG - 20:29, Sunday 11 February 2018 (40489)

affirmative. The LN2 alarm level is 80%, CP4 just went below that. We'll reconfigure CP4's alarms tomorrow.

LHO VE
kyle.ryan@LIGO.ORG - posted 12:24, Sunday 11 February 2018 - last comment - 16:03, Sunday 11 February 2018(40485)
On site working solo.
I'll be at Y-mid VEA making temperature measurements and/or adjustments or in the VPW tinkering with VBOC.  I expect to only be here 90 minutes or so.  Gerardo M. is my "phone buddy" and I'll make a comment to this entry when I am leaving the site. 
Comments related to this report
kyle.ryan@LIGO.ORG - 16:03, Sunday 11 February 2018 (40488)
1603 hrs. local - Kyle leaving site now.
H1 PSL
sheila.dwyer@LIGO.ORG - posted 12:53, Saturday 10 February 2018 - last comment - 15:52, Monday 12 February 2018(40480)
PSL is off

I came in to do some last DRMI/PRMI tests, and found the laser is off.  This happened about 4:15 am pacific time.  THe epics channels don't show any problems with the chillers, and it looks like the power watch dog tripped after the laser went off. (screenshot attached)

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 15:56, Saturday 10 February 2018 (40481)

It looks like this possibly was the power watchdog. The NPRO power and currents have been stable since the HPO has been off, but the PSL-AMP_PWR channels show that the power had been dropping before the laser shut off.  The Beckhoff status screen shows that everything is normal except the power watchdog. 

Images attached to this comment
sheila.dwyer@LIGO.ORG - 18:04, Saturday 10 February 2018 (40483)

Jason logged in remotely and restarted the PSL.

peter.king@LIGO.ORG - 05:32, Monday 12 February 2018 (40490)
Various data trends are attached.  At the time the power watchdog was engaged the output power was ~34.8 W.
There is no indication that the power decreased by 15% since the watchdog was enabled.  Trend data also
suggests that the amplifier dropped out before the NPRO.
Images attached to this comment
peter.king@LIGO.ORG - 15:52, Monday 12 February 2018 (40503)
Indeed the front end laser was tripped off by the power watchdog.  The trigger signal for the watchdog is the output of the third
amplifier stage and not the output of the front end - something that is rectified with the upcoming front end laser modifications.
When the watchdog was last engaged the power was ~106.  The watchdog tripped in at ~90, ie at the 15% drop level.  So the watchdog
worked as it should.

    Oh and the drop in power is most likely due to the large drop in relative humidity.  We know the e-beam sputtered coatings
for the pick-offs have issues with relative humidity.
Images attached to this comment
H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 10:30, Saturday 10 February 2018 - last comment - 10:45, Monday 12 February 2018(40478)
ISCT6 green path faraday isolator measurement

Terry, Nutsinee

Got some measurement of the EOT faraday isolator on the green path:

Over all transmission ~ 91% (S and P pol)

Isolation ~ -26dB

Couldn't find a non-polarizing beam splitter for 532 so I used a dichroic beam splitter set at weird angle (~30 degree or so) to partially let light though. I used one of the precision photonics mirror found in the SQZ bay drawer to reflect transmitted light straight back into the faraday and measure the light that bounced back from the beam splitter. I couldn't measure the part of back reflected light that went though the beam splitter so I guesstimated the transmission knowing what came in and what gets transmitted on its way into the faraday. Terry thinks this number is disappointingly low, given the dodgy set up I'd take this number as an upper limit (in a sense that it can't get any worse). But again, given the nearly 10% loss maybe we just have a not-so-great isolator. 

Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 10:45, Monday 12 February 2018 (40499)

Correction: according to the manual here the measurement is still within the spec. The isolation is a bit low but that could be due to our dodgy set up.

Images attached to this comment
H1 ISC
sheila.dwyer@LIGO.ORG - posted 18:40, Friday 09 February 2018 - last comment - 14:15, Monday 12 February 2018(40477)
measuring spot positions in PRC

This afternoon Georgia and I locked PRMI and ran a2l for PRM, PR2, and PR3.  

  PRM PR2 PR3
P2L 1.099 0.173 2.614
Y2L 0.046 -8.34 -0.050

There is a file called by the a2l scripts (for the matrices) that is no longer in the place it used to be.  We added the ads matrix to the list of matrices used in ISC_library, so that these scripts now import and use that.  

Comments related to this report
georgia.mansell@LIGO.ORG - 14:15, Monday 12 February 2018 (40502)

I have converted these P2L and A2L values to spot position using Alexa and Kiwamu's numbers for the HSTS (PRM & PR2) and HLTS (PR3), shown in alog-14788, and the same maths as in alog-40422.

  A2L L_{euler} a_{euler} alpha spot position* [mm]
PRM p 1.099 .25 5.2382

0.0524

-2.21
PRM y

.046

.25 5.2382 0.00220 0.0926
PR2 p .173 .25 5.2382 0.00826 -0.348
PR2 y -8.34 .25 5.2382 -0.398 -16.797
PR3 p 2.614 .25 2.4096 0.271 -14.2
PR3 y -0.05 .25 2.4096 -0.00518 -0.492

*spot position relative to center of mirror, face-on.

H1 ISC (ISC)
thomas.vo@LIGO.ORG - posted 20:31, Tuesday 06 February 2018 - last comment - 16:52, Monday 12 February 2018(40447)
Loss Measurement, Locked and Unlocked XARM

[For the commissioning team]

We did a quick measurement of the loss in the x-arm after improving the pointing into the cavity using IM4 and PR2.

It is important to note that there were no angular loops closed when doing this measurement, so the power build up wasn't optimized ( LSC-TR_X_QPD_B_SUM ~ 0.95).   We were running short on time and verified that the DC angular alignment was good enough so that the locked vs unlocked state gave us a big enough dip to estimate a visibility.  

Channel Locked Power(Cts) Unlocked Power(Cts) Visibility Loss PPM (calc'd)
AS_A_DC_NSUM 286 307 93% 302

Comparing the above numbers to alog-38493. They are close, but I can't say anything definitive about the change in loss between the two ITMXs (before and after swap), we can redo this measurement when we have more time to close angular loops (and maybe try a more sophisticated loss measurement).  Also important to note, mode-matching contributes to the loss as well and this is not taken into account with this measurement.

Images attached to this report
Comments related to this report
thomas.vo@LIGO.ORG - 16:52, Monday 12 February 2018 (40498)

Sheila commented that the visibility/loss is a bit concerning, so I trended some other channels to see if they gave any other estimates, unfortunately, the ones I could think of (REFL and AS) were not of much use because they didn't show an obvious dip (First and second attachment) .  It is important to also note that the dark offsets for ASC-AS_A_DC_NSUM were on and roughly correct.

That got us thinking, if there is alignment or modal mismatch, will we be over or under estimating the total loss with this measurement? And how much does the modulation depth from the sidebands cause a difference in the power ratio between unlocked and locked compared to the losses of the ITM?

Using Finesse and the as-built Nebula page, I modeled the  single x-arm with input power of 1 W.  The modulation depths for 9 and 45 MHz was measured by Kiwamu in aLOG-8867.  Also, setting the arm cavity eigenmodes as the basis, I estimated 15% mode-mismatch and 15% alignment mismatch by injecting 01 and 02 modes alongside the 00 into the cavity.  Another parameter is of course the loss at the input coupler which for display purposes I used 5ppm. (Third attachment)

Conclusion:

The loss of the input-coupler dominates over the modulation depth from the sidebands, and the mismatch either from modal or misalignment will cause us to underestimate the total losses.

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 10:48, Tuesday 06 February 2018 - last comment - 06:18, Monday 12 February 2018(40433)
xmgr plot skipping sections and displaying "max drawing path length" error

Some recent modest ASC full data trend plots have shown gaps in the data with an accompanying popup error:

[Error] Purging failed. Increase 'Max drawing path length' in prefs.

It is not immediately clear what "purging" and "max drawing path length" mean, but if you increase it from the default of 20k to 100k the gaps disappear.

Attached is the 'gappy' plot with the popup, and the preferences with the increased max drawing path length

Images attached to this report
Comments related to this report
keith.thorne@LIGO.ORG - 06:18, Monday 12 February 2018 (40491)CDS
Recently, Rolf and Jonathan alerted CDS to the existence on 'qtgrace', a currently-supported grace implementation that appears to solve several issues.  In the attached plot, you can see an extra sizing slider (currently at 1.3) and a "Fit" button that resizes a plot to fit the window. Currently packaged by Michael Thomas for SL7, we are working on a test rollout at LLO
Images attached to this comment
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