Displaying reports 45641-45660 of 84821.Go to page Start 2279 2280 2281 2282 2283 2284 2285 2286 2287 End
Reports until 10:19, Monday 29 January 2018
H1 PSL
edmond.merilh@LIGO.ORG - posted 10:19, Monday 29 January 2018 (40308)
PSL Weekly Report - 10 Day Trends FAMIS #6185

Besides the ongoing tripping, everything else looks normal.

Images attached to this report
H1 PSL (PSL)
yannick.lecoeuche@LIGO.ORG - posted 08:44, Monday 29 January 2018 (40306)
PSL Weekly FAMIS 7475
Laser Status:
SysStat is good
Front End Power is 35.24W (should be around 30 W)
HPO Output Power is 140.2W
Front End Watch is GREEN
HPO Watch is GREEN

PMC:
It has been locked 0 days, 3 hr 16 minutes (should be days/weeks)
Reflected power = 23.22Watts
Transmitted power = 41.32Watts
PowerSum = 64.54Watts.

FSS:
It has been locked for 0 days 3 hr and 16 min (should be days/weeks)
TPD[V] = 1.968V (min 0.9V)

ISS:
The diffracted power is around 3.9% (should be 3-5%)
Last saturation event was 0 days 3 hours and 12 minutes ago (should be days/weeks)

Possible Issues:
PMC reflected power is high
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 05:18, Monday 29 January 2018 - last comment - 10:19, Monday 29 January 2018(40305)
Laser trip
Came in this morning to find the oscillator off.  The front end was still running.  Looks like the watchdog kicked in
some ime around 5:30 pm Saturday.

    The power decay from head 1 is the reason for the decay in laser output power.  I upped the current of the 3 other
diode boxes by 0.5 A.

    Laser restarted without any major hiccups.  Other stuff came on-line pretty quickly.  Witnessed a couple of
occasions where the injection locking was lost.
Images attached to this report
Comments related to this report
jason.oberling@LIGO.ORG - 10:19, Monday 29 January 2018 (40309)

In an attempt to stabilize HPO DB1, I adjusted the operating temperatures of the 7 individual pump diodes in DB1.  The changes are summarized below:

  Operating Temperature (°C)
Old New
D1 24.0 24.5
D2 24.0 24.5
D3 22.5 21.5
D4 24.0 23.5
D5 24.0 23.0
D6 24.0 24.5
D7 24.0 24.5

This took the output power of the HPO from 138.9 W to 140.4 W, an increase of 1.5 W simply from temperature tweaks.  We will continue to monitor.

LHO VE
kyle.ryan@LIGO.ORG - posted 16:41, Sunday 28 January 2018 - last comment - 17:23, Sunday 28 January 2018(40302)
Kyle on site checking equipment
VPW, LVEA, Mechanical Room.  I expect to be here less than one hour and will make comment to this entry when leaving. 
Comments related to this report
kyle.ryan@LIGO.ORG - 17:03, Sunday 28 January 2018 (40303)
1705 heading to Y-end to check on purge air
kyle.ryan@LIGO.ORG - 17:23, Sunday 28 January 2018 (40304)
1725 hrs. local - Leaving site now
H1 SQZ (SQZ)
nutsinee.kijbunchoo@LIGO.ORG - posted 22:20, Friday 26 January 2018 (40298)
SQZ SHG guardian improved

After a negative rail was added to the PZT driver and a new Beckhoff scanning tool became available (thanks Daniel!), I was able to simplify the SHG auto locker and modified it such that the positive and negative rails are taken into account. SHG guardian no longer toggles the offset slide bar to look for resonance but instead sends in a scan to look for resonance. Once the resonance is found, the PZT is offset by that X amount of voltage and the loop is engaged. The code currently looks at Trans PD output power. At some point I'd like to make it look at the reflected green power and make it dependent of the input power (which can be done with the LASER IR PD). If SHG is locked with too much or negative voltage being sent to the PZT, it will drop lock to find another sweet spot. The low limit is currently set to 0V, and high limit is set to 85V.

 

More warning messages and fault conditions will be added in the future. For now it is relatively robust (I think).

H1 ISC (SQZ)
sheila.dwyer@LIGO.ORG - posted 17:20, Friday 26 January 2018 - last comment - 23:59, Friday 26 January 2018(40297)
OPO aligned for 532

Terry, Nutsinee, Sheila

After looking at the fiber collimators we decided to try swapping them so that the one that has a greenish tint in the lens is used for 1064 and the one that looks very clear is used for 532, based on advice from Lisa, Lee and Maggie. After doing this we were able to align the cavity and saw that our mode matching isn't too bad although we haven't tried to optimize it by moving any lenses yet. 

Comments related to this report
nutsinee.kijbunchoo@LIGO.ORG - 23:59, Friday 26 January 2018 (40299)

Terry, Nutsinee

Here I attached the waist measurement and fit of 532nm coming out of the correct green coupler. The Thorlabs beam profiler we use is not great with beam diameter < 1000um for 532 so we took that into account this time. The waist size we got was 183um (radius) located 270mm away from the coupler.

 

I also attached a photo of the couplers we have. Couldn't capture the reddish color very well but the left coupler was for 532 and the right coupler was for 1064.

Images attached to this comment
Non-image files attached to this comment
LHO VE
chandra.romel@LIGO.ORG - posted 17:05, Friday 26 January 2018 (40296)
IP4 tested and vented

Kyle, Chandra

IP4 is back from rebuild and shipped under vacuum (measured mid e-5 Torr range). We pumped down with an aux cart, isolated the turbo, and then turned on high volts and measured 1.8-2 micro-amps at 7 kV on each channel. The pump is now vented with dry N2. Monday we will vent the blank on IP4's new gate valve, verify there is no leak into main volume, and then install IP4.

LHO VE
chandra.romel@LIGO.ORG - posted 17:00, Friday 26 January 2018 - last comment - 11:02, Saturday 27 January 2018(40295)
Mid-Y work

Kyle, Chandra

We tested the leaks in GV12's gate o-rings by flooding the gate annulus with dry N2 (with active turbo connected and ready to be valved in to evacuate) and discovered the adjacent volumes' pressures rise too high too quickly. The Y2 beam tube rose to 7e-8 Torr and CP4 side rose to 1.4e-6 Torr in less than one minute. We may try to jog the gate on Monday to see if we can get a better seal, at least on inner o-ring. Will also re-evaluate the bake enclosure dimensions so see if gate annulus tubing can stay (GV11's definitely gets in the way and had to go).

We realized that we did not get any email or text alarms when we should have - pressure was well past the 5 minute and 15 minute set point thresholds on PT-245B and PT-256B. Will contact Dave B. about this.

Comments related to this report
chandra.romel@LIGO.ORG - 11:02, Saturday 27 January 2018 (40301)

Dave Barker rebooted alarm system this morning after a crash yesterday morning.

H1 General
edmond.merilh@LIGO.ORG - posted 16:01, Friday 26 January 2018 - last comment - 16:14, Friday 26 January 2018(40288)
Shift Summary - Day

TITLE: 01/27 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:

14:13 Terry out to Squeezer bay

16:00 Karen ad Vanessa out to EY

17:00 Karen and Vanessa back

17:04 Karen ad Vanessa back to EY - with stock

17:05 Marc out to LVEA-returning chassis to SUS rack near HAM

17:12 Dust Monitor at EY not responding

17:21 Betsy out to EY

17:32 Betsy power cycled dust monitor 2 at EY

17:40 Patrick reset the HV at EX

17:43 Travis, Danny, and Angus to EY

17:47 Patrick back

17:57 Richard out to LVEA - camera check PSL

18:01 Richard back

18:06 Terry back

18:20 Betsy back

18:23 Greg out to LVEA - resetting  TCSY LASER

18:28 N out to optics lab

18:30 Greg back

18:37 Kyle and Chandra moving new ION pump from large high bay to S side floor near HAM4

18:40 Betsy out to EY

19:19 Terry and N back

19:19 Greg out to LVEA - movin curtains from TCSY to TCSX

19:20 Angus, Travis and Danny back

19:40 Dany out to LVEA - pics

20:00 Danny back

20:00 Betsy back

20:05 Jeff back

21:14 Tvo and Sheila out for lunch

21:45 Kyle out to MY

22:02 Peter and Jeff B out to LVEA- ITMX camera

22:10 N, Sheila and Terry into optics lab

22:16 Kyle back

22:30 N back

22:54 Kyle and Chandra to MY

 

 

 

 

Comments related to this report
peter.king@LIGO.ORG - 16:14, Friday 26 January 2018 (40294)
00:10 Jeff and Peter finished with the ITMX and ITMY cameras.
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 12:32, Friday 26 January 2018 - last comment - 08:39, Saturday 27 January 2018(40292)
ETMY Welding Pics
J. Kissel, for A. Bell, T. Sadecki, and D. Sellers

While on my way to and from B&K hammering the EY PCAL periscope, I snapped a few publicity photos of Angus, Travis, and Danny who were fine-tuning the alignment and measuring violin modes of the brand new fibers of newly suspended H1 SUS ETMY.

Thanks and keep up the good work, gents!
Images attached to this report
Comments related to this report
angus.bell@LIGO.ORG - 08:39, Saturday 27 January 2018 (40300)
The violin modes were remeasured (with 0.25 Hz accuracy)
position  (Hz)    fibre S/N
+X/+Y	504.5	S1400157
-X/+Y	503.0	S1400159
+X/-Y	513.25	S1800486
-X/-Y	510.5	S1800491

as these will shift after in-chamber alignment, we didn't go for higher accuracy. The  laser we used was quite noisy and should be replaced before using the kit again.
H1 SUS (SYS)
betsy.weaver@LIGO.ORG - posted 12:24, Friday 26 January 2018 - last comment - 16:01, Wednesday 07 February 2018(40291)
ETMY PenRe reworked

In order to compensate for the missing mass of the new holey AERM optic being installed in the ETMY suspension, I had to rework the PenRe mass to be heavier.  SYS had designed a heavier new set of parts to swap, and I'll report that the rebuild went smoothly - the weigh compensation was pretty spot on and the install of the parts which we have had fit troubles with in the past, went in easy (thanks to Eddie's tweak on the design based on my feedback).

For the record, the weights of these masses are as follows.  Note, the idea is to make the old PenRe mass plus the old ERM mass weight equal the total of the new sets, such that the suspension hangs in the same vertical position as before.

OLD ETM01 mass 25,993g NEW AERM07 14,873g
OLD PenRe mass 53,236g NEW PenRe mass 64,356g
Total 79,229g   79,229g

Assembly weighs of the new PenRe:

  OLD PenRe New PenRe
Keeping Same Main Body 29,857g 29,857g
Keeping Same batch of small parts 3,002g 3,002g
Keeping Same wire clamp assys 168g 168g
Cans and Plates (new and old species) 19,087g 30,284g
Addable mass assys, to make total weight 1,122g 1,045g
Total from above 53,236g 64,356g

 

Comments related to this report
betsy.weaver@LIGO.ORG - 16:01, Wednesday 07 February 2018 (40460)

Doh - Typo, the ETMY AERM is AERM06, not 07.

The difference in weight between these 2 is a negligable 8g however.

H1 CDS
patrick.thomas@LIGO.ORG - posted 12:09, Friday 26 January 2018 (40290)
Added illuminators to sitemap
I created a medm screen to control all of the illuminators and added it to the sitemap under SYS. The controls for the illuminators in the corner station are not connected to the hardware yet.
I also removed the link to the older analog video camera medm screen.
H1 SUS (CDS, SQZ, SUS)
jeffrey.kissel@LIGO.ORG - posted 11:42, Wednesday 24 January 2018 - last comment - 12:46, Friday 26 January 2018(40254)
ZM2 Fully Functional, Doesn't Care Whether Sat Amp Jumpered to AOSEM or BOSEM Configuration
J. Kissel, R. McCarthy, M. Pirello
FRS Ticket 9771

After solving all of ZM2's signal chain problems (all of which were mis-jumpered boards inside its new HAM-A coil driver and US Sat Amp, see LHO aLOG series starting with 40237), I'd accidentally told Marc to jumper the SatAmp to the AOSEM setting (ZM2, an HTTS, uses BOSEMs). He's jumpered it to the BOSEM setting this morning, so I've taken another diagnostic suite. 

Turns out, though the OSEM sensor response dropped by an inconsequential ~13%, ZM2's BOSEMs don't care whether they're read out with a Sat Amp jumpered in the AOSEM or BOSEM configuration. 

Richard and I recall that perhaps all US sat-amps are jumpered to the same configuration, because (as Richard specifies) one species of OSEM doesn't use the feature implied in that configuration, it just needs to be jumpered to either/or. So we recall having set all US sat-amps one way (or the other). We'll figure out which (by checking the OMs and RMs), and set all the new US Sat Amps (for OFI, ZMs, and VOPO) the same way.

For all intents and purposes, ZM2 is now fully functional.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 12:46, Friday 26 January 2018 (40293)
J. Kissel, M. Pirello, R. McCarthy

Marc has verified that all US Sat Amps are jumpered to the BOSEM position. As such, we need not make any change to the current configuration of the Sat Amp, and we should consider the electronics and suspension in its final functional state.

Thanks for all your help Marc!
Displaying reports 45641-45660 of 84821.Go to page Start 2279 2280 2281 2282 2283 2284 2285 2286 2287 End