Displaying reports 45541-45560 of 84822.Go to page Start 2274 2275 2276 2277 2278 2279 2280 2281 2282 End
Reports until 11:11, Monday 05 February 2018
H1 SEI (SEI)
corey.gray@LIGO.ORG - posted 11:11, Monday 05 February 2018 (40412)
SEI Seismometer Mass Check (FAMIS#6095)

1) All STSs prrof masses that within healthy range (< 2.0 [V]). Great!

2) There are 8 T240 proof masses out of range ( > 0.3 [V] )!

LHO VE
chandra.romel@LIGO.ORG - posted 10:26, Monday 05 February 2018 - last comment - 08:46, Tuesday 06 February 2018(40410)
valved in corner IPs & RGA; valved out MTPs

Valved in vertex RGA and all six main ion pumps and valved out all three main turbo pumps (all pumps reading ~1 mA). Tomorrow will open GV 5,7 for x-arm commissioning (8am-8pm local).

Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 10:51, Monday 05 February 2018 (40411)

RGA scan with IPs valved in and MTPs valved out. Also attached scan pre-vent for comparison.

Non-image files attached to this comment
kyle.ryan@LIGO.ORG - 17:25, Monday 05 February 2018 (40424)
How long had the filament been energized before taking today's scan? 
chandra.romel@LIGO.ORG - 18:13, Monday 05 February 2018 (40426)

< 90 min. Jeff K. turned filament on for me via phone instructions. Will scan again tomorrow morning before opening up to beam tube.

chandra.romel@LIGO.ORG - 08:46, Tuesday 06 February 2018 (40431)

Here is a scan after the IPs were pumping over night and turbos valved out, and RGA filament turned on for > 12 hrs.

Images attached to this comment
H1 PSL (PSL)
corey.gray@LIGO.ORG - posted 10:25, Monday 05 February 2018 (40409)
PSL Weekly Report (FAMIS #7476)

NOTE:  PSL in middle of being downgraded to frontend 35W operations for this week....next week PSL upgrade work begins.
Laser Status:
SysStat is good
Front End Power is 34.93W (should be around 30 W)
HPO Output Power is 4.592W
Front End Watch is RED
HPO Watch is RED

PMC:
It has been locked 0 days, 0 hr 0 minutes (should be days/weeks)
Reflected power = 24.46Watts
Transmitted power = 0.2101Watts
PowerSum = 24.67Watts.

FSS:
It has been locked for 0 days 0 hr and 0 min (should be days/weeks)
TPD[V] = 0.08654V (min 0.9V)

ISS:
The diffracted power is around 2.4% (should be 3-5%)
Last saturation event was 0 days 0 hours and 24 minutes ago (should be days/weeks)

Possible Issues:
PMC reflected power is high
FSS TPD is low

LHO General
corey.gray@LIGO.ORG - posted 10:02, Monday 05 February 2018 (40407)
Monday 9:00am Vent Meeting Notes

Peek Down X-arm TOMORROW!  Here are notes regarding it:

Other Items:

H1 PEM
jeffrey.bartlett@LIGO.ORG - posted 09:54, Monday 05 February 2018 (40408)
Monthly PSL Chiller Filter Check (FAMIS #8305)
   Checked PSL filters. No debris noted in either filter. The crystal chiller filter is starting to yellow. The diode chiller filter has darkening somewhat, but not as much as the crystal chiller. I plan to swap both sets of filters (2 filters in the chiller room and 2 in the PSL enclosure) when the PSL goes down for the 70 watt amp change. I have all 4 filters on hand. 

   Peter King - added 300ml water to crystal chiller this morning. 

   Closing FAMIS task #8305   
H1 PSL
edmond.merilh@LIGO.ORG - posted 08:32, Monday 05 February 2018 (40404)
PSL Weekly Report - 10 Day Trends FAMIS #6186

The ongoing "trippy" saga of "As the Diodes Weaken" is reflected in all aspects of the trends as LASER outages and incursions have been more frequent. Peter and Jeff are currently in the enclosure and the Pre-Mode cleaner appears to be off its alignment.

Images attached to this report
LHO General
corey.gray@LIGO.ORG - posted 08:32, Monday 05 February 2018 (40403)
Morning Report

TITLE: 02/05 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Planned Engineering
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    Wind: 9mph Gusts, 8mph 5min avg
    Primary useism: 0.03 μm/s
    Secondary useism: 0.16 μm/s
QUICK SUMMARY:

H1 General
peter.king@LIGO.ORG - posted 05:13, Monday 05 February 2018 (40402)
LVEA transitioned to LASER SAFE
The LVEA has transitioned to LASER SAFE.
LHO VE
kyle.ryan@LIGO.ORG - posted 19:08, Friday 02 February 2018 (40400)
Installed Turbo and RGA assembly at CP4
I misplaced a small adapter needed to connect the leak detector but will pump down and leak check this new setup early next week.
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 18:20, Friday 02 February 2018 (40398)
HPO status
A couple of status screens at the time of shutdown.  Both the diode and crystal chillers are off.  Internal and external shutters
are closed.  The PSL Beckhoff computer will remain on.  The diode currents for all heads have been set to zero.

head 1 diode current: 65.0A
head 2 diode current: 59.8A
head 3 diode current: 59.8A
head 4 diode current: 59.8A

    Autolockers for the pre-modecleaner, intensity stabilisation and frequency stabilisation are off.  I took the input modecleaner
off line.


"It is a far, far better thing that I do, than I have ever done; it is a far, far better rest that I go to than I have ever known."
Sydney Carton
Images attached to this report
H1 AOS
thomas.vo@LIGO.ORG - posted 18:04, Friday 02 February 2018 - last comment - 18:19, Friday 02 February 2018(40397)
MICH Fringes Seen, but confusion on AS Sensors

Jenne, TVo

We set out today trying to lock MICH with the newly aligned AS_A and AS_B senors from aLOG-40338, however, we had problems trying to get the light back on the diodes which is confusing because there weren't large alignment changes between now and this past Tuesday.  

In the end of a lot of alignment tweaks, we were able flash MICH fringes and get light onto the AS_A, AS_B, and AS_C individually, but not at the same time as we would expect.  Attached is the screenshot of our current alignment.

Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 18:19, Friday 02 February 2018 (40399)

We did have some successes today in commissioning the new configuration of AS_A WFS. 

Since our ASC_IMC model runs at 16k, we don't need our AS WFS to be up in the IOP model.  Daniel and DaveB made the changes, however upon restarting the model today TVo found that the ADC connection in the model wasn't right, which is why we weren't getting any signals in.  Once Dave fixed that and restarted the model again, we see sensible signals in the AS_A WFS.

We copied over the antiwhitening filters, as well as all of the EPICS settings from the old AS_A locations (since it's now on a new model).  We also installed AA filters on the pitch and yaw filter banks just before the signals get sent from the 16k ASCIMC model down to the 2k ASC model. 

We checked that the same signal in, for example, AS_A_Pit_I goes through the ASC input matrix to the inputs of the various degrees of freedom, as you would expect.

We also checked that the AS Sum signal goes through the LSC input matrix as you would expect. 

So, the digital signals for the new AS A WFS configuration seem all okay now.  *Then* we wanted to try to lock MICH, but as TVo said, couldn't get to a point where we had light on all the AS and OMC diodes that we were expecting, all at the same time.  We'll relook at this on Monday after the PSL is back up, or perhaps wait until ~Wednesday after we've set the input alignment to match the Xarm.

H1 SEI (DetChar, SEI)
krishna.venkateswara@LIGO.ORG - posted 17:26, Friday 02 February 2018 (40396)
BRS-X shows unusual noise

Krishna

The new BRS DetChar Summary pages alerted me to a strange noise visible on Jan 19th and Jan 20th.

I looked at the rY_in DQ channel and the noise looks like short duration spikes in the angle channel. See first attached plot. The low-frequency oscillation of BRS-X is visible and the spikes start in the 17th minute of the plot. Zooming in (next plot), these spikes last for 8-10 second and the data resumes it's previous trend, with no apparent offset. I looked at most of the error bits listed in the BRS troubleshooting guide and saw no indication of any kind of hardware issue. I have also attached the DRIFTMON data showing a similar spike but appropriately smaller, indicating that it is a real deviation as seen by the C# code. I looked through two months of recent data and don't see any other similar noise.

I have two theories to explain this:

1. We have a literal bug in the autocollimator - most likely near the CCD. The CCD isn't fully enclosed and there is room for bugs/critters to get in there especially since they are attracted by the heat of the CCD. We had a similar issue some time ago in the lab. Whether or not this is what happened, Michael and I agree we should try to more fully seal the autocollimator so that this never happens.

2. The CCD is failing. I think this is less likely since it seems to be functioning perfectly now, even though the code hasn't been restarted since Jan 4. The previous time the CCD malfunctioned (Jan 31), the symptoms were very different (see 4th plot). However, we can't rule this out completely. We need to see if this happens again (after sealing up the CCD), and if needed the CCD can be replaced. It is an off-the-shelf item - Basler Racer raL4096-24gm.

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 17:08, Friday 02 February 2018 (40395)
ALS medm's were temporarily unavailable

Due to the large size of the isc userapps repository (4.1GB), while I was checking out the ISC from scratch some ALS MEDM macro-substitutions did not work. For other large systems I will do the checkout into a temp directory and then do the 1.6 to 1.8 upgrade in one atomic operation.

This also caused bogus filter-file-changed warning with no actual content changed.

H1 ISC
daniel.sigg@LIGO.ORG - posted 15:54, Friday 02 February 2018 - last comment - 11:01, Saturday 03 February 2018(40394)
ALS laser End X

We shifted the ALS laser in the X end stations by ~18.6GHz (-6.2V on the crystal temperature control voltage) to bring it close to the PSL. This offset was then relieved using the front panel potentiometer. The ALS autolocker is working again.

The same shift will have to be applied to the Y end laser.

Some other strangeness:

Comments related to this report
keita.kawabe@LIGO.ORG - 11:01, Saturday 03 February 2018 (40401)

The beat note had 8MHz sidebands (attached). Shouldn't be a big problem but I don't remember seeing this before.

 

Images attached to this comment
H1 General
jim.warner@LIGO.ORG - posted 15:49, Friday 02 February 2018 (40382)
Shift Summary

16:30 JeffB to LVEA

16:30 Bubba to EX, back 17:45

16:50 Hugh to HAM6

17:35 Nico to LVEA, back 18:10

17:45 JeffB to LVEA

18:15 TJ to optics lab

18:15 Jason to EY

18:25 Kyle to MY

18:30 - 18:56 UTC Corey and Richard to end X, looking at solar panels, batteries for
vacuum gauge
18:37 - 19:32 UTC Karen and Vanessa cleaning at mid Y
19:00 - 19:16 UTC Bubba taking measurements in LVEA
19:00 - ~20:00 UTC Marc WP 7327
19:00 - 19:23 UTC Filiberto WP 7309
19:07 - 19:34 UTC Amber and two visitors from OSA in LVEA
19:23 - 19:58 UTC Jeff B. to LVEA, ITM camera work
19:37 UTC Sheila back from optics lab (in about an hour ago)
19:44 UTC Chris opening OSB outer rollup door
19:45 UTC Dave restarting models, IMC down
19:48 UTC Jason back from end Y

21:15 TJ Nico to LVEA

21:15 TVo checking to see if light pipe was closed

21:15 Keita, Georgia, DaveO, Daniel to LVEA then EX

22:45 Sheila to optics lab

 

 

 

H1 ISC (ISC)
marc.pirello@LIGO.ORG - posted 13:25, Friday 02 February 2018 - last comment - 11:24, Monday 05 February 2018(40389)
Corner 4 & Corner 6 Channels Repaired

Elizabeth C., Marc P.

Taking advantage of a one hour window in operation we repaired the Corner 4 and Corner 6 squeezer readbacks per WP7309

In Corner 4 we replaced module 19 on the left rail with a new EL3104 (4 channel differential ADC)

In Corner 6 we replaced module 5 on the right rail with a new EL1124 (4 channel digital input)

Both of the replaced modules appear to be working.

Comments related to this report
daniel.sigg@LIGO.ORG - 15:44, Friday 02 February 2018 (40393)

ASC-AS_B_RF42_DEMOD_LOMONCHANNLE_3/4 is fixed.

H1:ISC-RF_C_AMP42M4_POWEROK still reads zero. Maybe a cabling problem?

marc.pirello@LIGO.ORG - 11:24, Monday 05 February 2018 (40413)

Fil C., Marc P.

It was a indeed an internal wiring problem.  We moved the wires to the correct positions on the beckhoff terminal and verified OK1 through OK12 are working as intended.

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
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