Displaying reports 45721-45740 of 84819.Go to page Start 2283 2284 2285 2286 2287 2288 2289 2290 2291 End
Reports until 20:28, Monday 22 January 2018
H1 ISC
thomas.vo@LIGO.ORG - posted 20:28, Monday 22 January 2018 (40225)
Continuing to align DRMI

Keita, Cheryl, Jenne, TVo

- After getting the beam onto HAM6, Keita suggested optimizing the beam position on SR2 and SR3.  The difficulty with trying to use the cameras to align the beam to the center of SR2 is the key hole scraper baffle makes it difficult to figure out which beam (input or reflection) you're actually seeing scatter off the edges.  Not only that, the bright spots that we do see scatter don't seem to move linearly with SR3 pitch/yaw, this is very odd.

- Cheryl found a good pointing of BS and PR3 to center on SR3, but that changes the input beam into the Michelson. Also, by changing the SR2 alignment, she was able to sweep the SRM reflection across SR2.

- I found a better alignment through the Faraday that gives us approximately 10 mW single bounce onto AS_C (somewhat calibrated?), which approximately matches our back of the envelope power budget with input power of 5.9 Watts from the PSL, by sweeping SRM around, I was able to get a small SRCX and SRCY flash.

 

Rough plan for tomorrow:

Somehow we have to make the three points above converge to a decently aligned DRMI.

Since we've already done a lot of work aligning PRC and Mich in the past week or so, it might be worth it to preserve the PRC alignment by walking the beam around SR3 to find its center point.  This could possibly be done by changing the beamsplitter and ITM alignments to sweep the face of SR3, while maintain the LSC_POP relatively steady in value.  Mich will be flashing so it might be a little tedious to tell if you're improving but it's doable.  

At the same time, since we've got a AS_C signal, we can try to maintain a signal by changing SR3+SR2 alignment, so we don't have to try to find the beam when going into HAM6.

Then, per Keita's suggestion, we can enter HAM6 sweep around the combination of SR3 and SR2 pointing so that we find the edges of the baffles+Faraday and find the middle of the clipping, this might be as good as we can get with SR2 centering.

H1 SYS (SEI, SQZ, SUS, SYS, VE)
jeffrey.kissel@LIGO.ORG - posted 17:39, Monday 22 January 2018 - last comment - 15:03, Tuesday 23 January 2018(40224)
H1 HAM5 D3 Conflat Arrangement
J. Kissel, M. Pirello

After SUS'ing out the OMs and the OFI, and while still trouble shooting ZM2, I wanted to post redlines to D1002876-v4 which hasn't been updated to include new squeezer suspensions. Granted, we still haven't confirmed ZM2's functionality (see LHO aLOG 40207).
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 15:03, Tuesday 23 January 2018 (40236)SEI, SQZ, SUS, SYS, VE
Betsy reminds me that systems is more likely to update the in-vacuum cable harness routing documents than the flange layout documents. For HAM5, that's D1101917, v4 of which is indeed up-to-date and includes ZM2 (marked as SQZ-TIP/TILT) and the OFI.

Thanks for the reminder, Dubs!
H1 CDS (SUS, TCS)
filiberto.clara@LIGO.ORG - posted 16:25, Monday 22 January 2018 (40221)
TCS and SUS cabling

Continued with field cabling in the LVEA.

1. Illuminator cables for HAM4/HAM5/HAM6 were terminated and connected to chassis power. This completes illuminator cabling for the corner station. New modules need to be added/scanned to beckhoff to control on/off functionality.
2. Ran cables for VOPO and ZM1 from field rack to top of HAM 6.
3. Ran cables for TCS SR3 Heater (CER to HAM5).

F. Clara, E. Merilh

H1 General
jim.warner@LIGO.ORG - posted 15:54, Monday 22 January 2018 (40216)
Shift Summary

TITLE: 01/22 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:
LOG:
 

17:45 Sheila to  optics lab

18:15 Ed to output arm, terminating cables

18:15 Kyle to MY

18:30 Peter & Gerardo to optics lab

18:30 Travis & Danny to EY, back 20:30

18:45 Jason to EY

19:00 TJ to optics lab

19:30 Marc to LVEA

19:30 Cheryl to IOT2

19:30 JeffB to ITMX camera, back 20:30

21:30 Welding crew to EY

21:30 Marc to HAM5 done 22:15

22:00 JeffK to HAM5 done 22:15

22:00 Kyle to LVEA

22:00 JeffB to ITMX camera

22:15 Corey to optics lab

22:15 Nutsinee to sqz

22:45 Tvo to HAM4

LHO VE
chandra.romel@LIGO.ORG - posted 15:48, Monday 22 January 2018 - last comment - 17:20, Monday 22 January 2018(40220)
GV-11 mid-y work

[Kyle, Chandra]

Note:  this activity caused expected Y-arm pressure alarms.

Verified we have an outer o-ring leak on GV-11 gate that needs to be addressed before CP4 bake. We back filled the gate annulus with dry N2 and allowed pressure to rise for 7 minutes to see if it would flatten out (it did not as it approached 1e-7 Torr). Once we're back on its AIP, we will re-seat the gate and retest. If that doesn't fix the o-ring we will install a valve at the 1-1/3" gate port so we have the ability to pump on it during bake. If need be, we can soft close GV-10 (which will isolate mid-Y's large ion pump from Y1 arm) and valve in the small ion pump attached to CP1.

Then we repeat for GV-12.

Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 17:16, Monday 22 January 2018 (40222)

We re-seated GV-11 gate which made the outer o-ring leak worse. Shoot.

Side note:  when we stroked GV-11 to a yellow state, GV-12 open/closed status turned yellow too.

Images attached to this comment
chandra.romel@LIGO.ORG - 17:20, Monday 22 January 2018 (40223)

Also note that hard closing GV-11 was quiet second time around.

H1 ISC (IOO)
jenne.driggers@LIGO.ORG - posted 14:01, Monday 22 January 2018 - last comment - 14:35, Monday 22 January 2018(40217)
PRM parking spot set

[Keita, Gerardo, Jenne, Cheryl]

With the new input alignment from after the vent, we checked the PRM's parking spot and have found the misaligned location that puts the beam on the steering mirror above the viewport above HAM2.  Keita made some small adjustments on that steering mirror to center the beam on the beam dump.

This was WP 7305.  It turns out there is no insert for a lexan cover, but Gerardo had (from a previous time doing this) a thick piece of plexiglass that was cut to size to fit over the viewport while these checks and adjustments were made.  The plexiglass was removed, and the cover reinstalled.

Comments related to this report
gerardo.moreno@LIGO.ORG - 14:35, Monday 22 January 2018 (40219)

Photo of beam on beam dump.

Images attached to this comment
H1 PSL
jim.warner@LIGO.ORG - posted 09:48, Monday 22 January 2018 (40215)
PSL Weekly FAMIS 7474

Laser Status:
SysStat is good
Front End Power is 35.34W (should be around 30 W)
HPO Output Power is 140.9W
Front End Watch is GRE
HPO Watch is GREEN

PMC:
It has been locked 3 days, 23 h/weeks)
Reflected power = 28.09Watts
Transmitted power = 38.88Watts
PowerSum = 66.97Watts.

FSS:
It has been locked for 3 days 21 TPD[V] = 1.627V (min 0.9V)

ISS:
The diffracted power is around 2.8% (s
Last saturation event was 3 days 21o (should be days/weeks)

Possible Issues:
PMC reflected power is high

H1 PSL
edmond.merilh@LIGO.ORG - posted 08:57, Monday 22 January 2018 (40214)
PSL Weekly Report - 10 Day Trends FAMIS #6184

Plots show the last two trips. All  other plots look normal.

Images attached to this report
H1 SQZ (SQZ)
sheila.dwyer@LIGO.ORG - posted 20:49, Sunday 21 January 2018 (40213)
VIP update

Last week we added the OPO and some of the optics to the VIP.  

H1 ISC
jenne.driggers@LIGO.ORG - posted 18:27, Saturday 20 January 2018 (40212)
Beam to AS_C

[Sheila, Terry, TVo, Jenne]

Beam go through hole, all the way to HAM6!

Attached are 3 screenshots, with titles indicating what they mean.  The important one is the last, BeamOn_AS_C.png, which is the slider locations where we see some beam on AS_C.  That means that we're making it through the output Faraday!

(The 2nd screenshot is where we think we're roughly centered through the OFI).

Images attached to this report
H1 SUS
betsy.weaver@LIGO.ORG - posted 13:13, Saturday 20 January 2018 (40210)
Fri ETMY SUS stat

In Friday, Travis finished cleaning up the ETMY PUM horns by filing them to the proper length and then cleaning up the debris in the flats. I then thoroughly cleaned the lower main structure using a tiger vacuum and wipes. Gerardo aided us in weighing the new ETM test mass (ETM16) and installing it in the structure using the ergo arm.

Jason also worked on setting up IAS equipment to look at the suspension in the afternoon. His equipment is parked in the far side of the weld cleanroom away from the man-door entrance into the VEA and he has caution tape around some of it. Please limit activities around this equipment and watch your step near it if you need to get to the other side. We anticipate the equipment to be removed after next week.

We are in good shape to start the fiber welding process on this suspension next week.

H1 ISC
thomas.vo@LIGO.ORG - posted 12:01, Saturday 20 January 2018 - last comment - 16:51, Saturday 20 January 2018(40209)
Still working on SRC Alignment

Jenne, Sheila, TVo

We spent most of Friday using cameras to get the pointing of SR3 onto SR2 and back down to SRM correctly but it was much more difficult without a sensor to tell if you're actually getting the center of the baffle aperture.  We think we were able to eventually get the right beam down to the SRM but it's not obvious how well centered you are on any of the optics (except SR3 since we have the input chain well aligned).   We were hoping to get the optics close enough so that an excitation on all three optics would show up all the way back at LSC-POP but unfortunately this didn't work.

The next hopeful resolution is to get into HAM6 and try to align through the Faraday with an IR card.

Comments related to this report
jenne.driggers@LIGO.ORG - 16:51, Saturday 20 January 2018 (40211)

Re-finding that place where we are hitting SRM and getting some beam back toward SR2, I realized that we hadn't put in any screenshots of the alignment for a while.  So, here's an alignment that gets us back toward SR2, although I can adjust the SR mirrors quite a bit and still get this. 

In the photo, the beam returning from SRM is at the bottom of the top TV.  It's hitting something much lower than the baffle aperture (bottom of cage, or side of ISI or something?). On the lower TV, the smaller circle on the left is where we think the SRM is, and the larger circle on the right is the SR3 baffle aperture. The vertical lines are where we think the cages are for the suspensions, and the dotted line at the bottom is the eye-baffle between HAMs 4 and 5.  The top TV has markings for the SR2 baffle, but it's hard to capture.  The SRM return beam is directly below the center of the circle part of the SR2 baffle aperture.

Images attached to this comment
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 17:35, Friday 19 January 2018 - last comment - 14:24, Monday 22 January 2018(40207)
H1SUSZM2 Electronics Still Not Perfectly Functional
J. Kissel, M. Pirello

After finishing out the OFI, I moved on to H1SUSZM2. It doesn't yet work.

Symptoms:
- The OSEM sensor readbacks (the ADC inputs on the MEDM screen) are showing little-to-no signal (only ~1000 cts), however transfer functions still have plenty of coherence.
- Although ZM2 is driven with an ISC configuration HAM-A driver, which supposedly has all binary control jumpered such that the low-pass filter is engaged, the pitch and yaw transfer functions show excess response at high frequency, which can be "calibrated out" by using exactly the same poles and zeros as the low pass filter (zpk(zeros,poles,gain,normalization) = zpk([0.9;211.883],[10;21],1,"n")). So it's as though the filter *has not* been jumpered. However, because there's plenty of coherence with the TFs, the Test/Coil enable jumper must be good.
- In a quiescent state (damping loops OFF, but no excitation), the BOSEMs ASD shows noise elevated way above the noise floor.
- Earlier in the day, when the external OFI's signal chain was unknowingly hooked up to the ZM2 in-vacuum chain, we saw lots of signal (i.e. the typical ~15000 cts), and transfer functions showed a normal frequency response (except for the poor basis conversion; see MAGENTA comments below).

Attached are 
- Transfer Functions. BLACK is an old OM1 result, RED is as it stands now, MAGENTA is driven and readout with the OFI chain. Regarding MAGENTA -- Unfortunately, when driving a 4-OSEM tip tilt through the 3 OSEM OFI chain with the wrong coordinate transformation matrices means that all three "long" "pitch" and "yaw" drives were some wonky combination of only UL, LL, and UR. That's why you see a poorly diagonalized result, and you see all three DOF's modes in each TF.
- Some MEDM screen shots relevant to the discussion
- The DTT and Foton comparison for the "calibration" of the Pitch and Yaw TFs. Note, the TFs are *not* shown with the calibration, but trust me, when it's applied it makes the high frequency response of the RED match BLACK
- The OSEMs ASD compared against the target / spec BOSEM noise.

Because of the incorrect frequency response, I suspect the coil driver either hasn't been jumpered or it's just a bad board. Note, also, as is standard on the HAM-A driver, US field sat-amp systems, the sensor signals are plugged directly from the sat-amp into the AA chassis towards the ADC / IO chassis. That means that the sensor signals, which are polluted with noise are *not* being polluted by the coil driver. So maybe both are problematic?
We know the in-vac suspension and electronics are OK, because they tested well with the OFI signal chain.

We'll investigate further on Monday.
Images attached to this report
Comments related to this report
marc.pirello@LIGO.ORG - 14:24, Monday 22 January 2018 (40218)

After discussing with Jeff, I pulled the ZM2 coil driver S1700079 and found that the jumpers were not installed correctly.  I installed jumpers on the W2 links and P3 (Run/Acquire Controls and Indicators) matching this unit to the ones we worked on prior.

LIGO-D1100117

It looks like the  ZM1, VOPO 1-4, VOPO 5-6 also need the same treatment as their indicator lights are not correct on the front of the chassis.

H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 17:20, Friday 19 January 2018 - last comment - 09:25, Monday 05 February 2018(40199)
SHG Conversion Efficiency

Sheila, Nutsinee

Here I attached the SHG conversion efficiency measurement as a function of 1064 input power (red dots) plotted against theoretical prediction (the equation came from Polzik and Kimble 1991 paper on frequency doubling) . ~75% conversion efficiency at 400mW input, 48% conversion efficiency at 100mW input. For the fit I tweaked a couple parameters, intracavity losses (L) and the single-pass nonlinear conversion efficiency (Enl).

 

Here's everything I wrote down.

P in (1064, mW) P out (532, mW) P trans (1064, mW) Common mode board gain (dB) responsivity (A/W)
100  48.6   24   
151 88 2.6 23  
102  49.5     0.313
206 135.5 3.1 22  
250 175 3.45 22  
300 220.2 3.8 21 0.297
350 267 4.1 21  
400 306.5   22  
401 315.5 4.5 22 0.293

 

The common mode board common path gain was adjusted to keep the UGF at 3kHz.

The responsivity was adjusted to match the photodiode readback to the power meter.

P in and P out was measured with a 1W Thorlabs power meter. P trans was read out of the photodiode.

The optimized crystal temperature for green output was the same for all input power, at 35.9 C

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 09:25, Monday 05 February 2018 (40406)

More SHG characterizations:

  • Low rail = -10V, high rail 100V, actual usage: 0-85 V. 
  • 35.9 C nominal temperature, optimized for green output 
  • Mode matching: 96%. Can be better. 
  • PZT calibration: 52V/um 
  • PDH Vpp = 623 mV @2mW trans DC output. 
  • Open loop gain Transfer function: UGF ~3kHz. Nominal common path common mode board gain: 12dB

 

 

Images attached to this comment
LHO VE
chandra.romel@LIGO.ORG - posted 17:12, Friday 19 January 2018 (40206)
all metal right angle valve leak test

[Kyle, Chandra]

We leak checked the gate of this valve after suspecting a leak. Kyle cycled it five times on leak detector and four out of the five times it leaked (e-6 mbar-L/s range leak). Then we sprayed the gate with IPA to clean it and re-tested with three cycles. No more leaks! It could be that particulate fell on the gate gasket during rough down when it was installed on OMC NEG housing. 

We have since received six more of this valve model and decided to leak check all at once right out of packaging. All six are leak tight to a level of 5e-8 mbar-L/s background. I cycled each valve once while on leak detector.

https://services.ligo-la.caltech.edu/FRS/show_bug.cgi?id=9593

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