Displaying reports 43921-43940 of 84071.Go to page Start 2193 2194 2195 2196 2197 2198 2199 2200 2201 End
Reports until 09:19, Thursday 05 April 2018
H1 PSL (IOO, ISC, OpsInfo, PSL, SYS)
jeffrey.kissel@LIGO.ORG - posted 09:19, Thursday 05 April 2018 (41304)
PSL Power Reduced to 100 mW, PSL Rotation Stage Locked Out
S. Dwyer, P. King, J. Kissel

Shiela reduced the 1064 nm laser power coming from the PSL going into the vacuum system via the PSL's rotation stage down to 108 mW (measured down stream of the PSL rotation stage, H1:IMC-PWR_IN_OUT16) to 108 mW, then Peter and I locked out the rotation stage controller. We've confirmed that requesting adjusting rotation stage angle does not change the power after locking out the controller.

It's currently laser SAFE (the PSL light pipe has been shuttered as normal), but in case we need the PSL light for alignment later, I figured we'd get the procedural stuff done before we need it. Due to IMC particulate concerns, we wish not to have higher than ~100 mW in-chamber while in air, so as to not burn stuff into a flashing IMC (see M1300464).
H1 FMP
jeffrey.kissel@LIGO.ORG - posted 08:43, Thursday 05 April 2018 (41303)
Dust Counts Before HAM5 Door Removal
J. Kissel

I gathered a dust count reading before doors were removed this morning. Counts are zero and zero!

Images attached to this report
H1 SEI (OpsInfo)
jeffrey.kissel@LIGO.ORG - posted 08:33, Thursday 05 April 2018 (41302)
HAM5 HEPI Locked
J. Kissel, J. Warner

In prep for today's vent, Jim and I locked HAM5 HEPI. 

Displacements between locked and unlocked are on the order of ~20-30 um, and 5-10 urad from nominal floating position with IPS-only, "position" loops closed. See attached screenshots, but I recap pertinent info below.

    dX    -2.3 um
    dY   +17.6 um 
    dZ   +23.7 um
    dRX   +1.2 urad
    dRY   +4.1 urad
    dRZ   -8.7 urad

I also attach pictures of the locking bolts / set screws. To lock HEPI (while attempting to preserve alignment):
    - Procure a CDS laptop, and open MEDM to get the DC BIAS screen of the given HEPI you want to lock
    - Take a screen cap of the screen before you get started.
    - Run all set screws and bolts into such that they're barely contacting the floating cube in each / every corner.
    - Using the appropriate allen wrenches (you'll need two sizes, 3/16" and 1/4"), and while watching the attached displacement screen, gently nudge the bolts further into contact until tool tight, rotating between bolts / set screws so as to not crank on any one bolt more than the others for a given tightening iteration. It's fine to do this sequentially around the corners. 
    - Displacements from nominal on the order of a few 10s of um / urad are the precision you'll be able to lock the position.
    - Take another screenshot of the position and displacement once done and record.

This process takes about 20-30 minutes.

    
Images attached to this report
LHO VE
patrick.thomas@LIGO.ORG - posted 19:09, Wednesday 04 April 2018 (41300)
PT246B 12 hour trend
Minute trend plot of PT246B for the last 12 hours attached per Gerardo's request.
Non-image files attached to this report
LHO VE
chandra.romel@LIGO.ORG - posted 17:06, Wednesday 04 April 2018 - last comment - 19:12, Thursday 05 April 2018(41296)
Vacuum summary for the day

Gerardo, Mark D. Tyler, Chandra

Corner

EY

We will start roughing down EY tomorrow.

Comments related to this report
chandra.romel@LIGO.ORG - 17:22, Wednesday 04 April 2018 (41297)

Checked on CP4 at MY.

gerardo.moreno@LIGO.ORG - 17:49, Wednesday 04 April 2018 (41299)VE

We have an aux cart running at Y-End right next to the BRS, it will be there until pressure at the BSC10 annulus system is kept at nominal by its ion pump.

Images attached to this comment
jeffrey.kissel@LIGO.ORG - 08:00, Thursday 05 April 2018 (41301)CDS, ISC, SYS
Prior to corner station vent, high voltage has been turned off (as per items mentioned in M1300464).
    - ESD driver
    - Fast shutter de-energized
    - OMC's PZT actuator drive
    - Picomotors
ITM Ring heater's measured power is zero (power is off at chassis), and I've changed the requested power to zero via MEDM.
kyle.ryan@LIGO.ORG - 19:12, Thursday 05 April 2018 (41318)
The net pump speed of this diaphragm backing pump is "much" less than what we are used to. I used this portable pump station for the first time the other day to evacuate 4 lengths of 1.5" flex line + the volume between IP6's closed GV and the zero-length reducer and it took "minutes" not seconds.
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 16:41, Wednesday 04 April 2018 (41295)
H1SUSTMSY Closeout TFs Look Great
J. Kissel

I've taken standard close-out transfer functions for H1 SUS TMSY. It's free and clear of rubbing, and results looking strikingly similar to before. OK for pump down!

Raw data is committed here:
    /ligo/svncommon/SusSVN/sus/trunk/TMTS/H1/TMSY/SAGM1/Data
        2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_L_0p01to50Hz.xml
        2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_P_0p01to50Hz.xml
        2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_R_0p01to50Hz.xml
        2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_T_0p01to50Hz.xml
        2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_V_0p01to50Hz.xml
        2018-04-04_2209_H1SUSTMSY_M1_WhiteNoise_Y_0p01to50Hz.xml
Non-image files attached to this report
H1 DCS (CDS, DCS)
gregory.mendell@LIGO.ORG - posted 16:31, Wednesday 04 April 2018 (41294)
DMT test box patched and rebooted

The DMT test box, h1dmt3, was patched and rebooted today at about 2 pm PDT. This should have no impact on the control room.

H1 General
yannick.lecoeuche@LIGO.ORG - posted 16:03, Wednesday 04 April 2018 (41293)
Shift Summary - Day

TITLE: 04/04 Day Shift: 15:00-23:00 UTC (08:00-16:00 PST), all times posted in UTC

STATE of H1: Planned Engineering

INCOMING OPERATOR: None

 

LOG:

14:39 (7:39) Tyler, Mark to EY

15:00 (8:00) Start of shift

15:15 (8:15) Bartlett to EX -- reset dust monitor #2

15:39 (8:39) Bartlett leaving EX

15:59 (8:59) Chris to EY -- delivering bolt

16:05 (9:05) Tyler, Mark back from EY

16:14 (9:14) Peter and Fil transitioning to laser safe

16:31 (9:31) Gerardo to EY -- vacuum work

18:14 (11:14) TVo, Sebastien, Dan, Alexei to LVEA

18:39 (11:39) Gerardo back from EY

19:02 (12:02) Gerardo to LVEA

19:29 (12:29) Fil to ISCT6 -- collect GIGE cameras

19:57 (12:57) TVo, Sebastien, Dan, Alexei out of LVEA

20:19 (13:19) TJ to HAM5 -- cleaning up

20:39 (13:39) Chandra, Tyler to LVEA -- craning work

20:43 (13:43) Gerardo to IP5

20:46 (13:46) Betsy to LVEA -- find something for Livingston

20:48 (13:48) Elizabeth to LVEA

21:02 (14:02) Jason to PSL enclosure -- grab materials

21:03 (14:03) Betsy out of LVEA

21:20 (14:20) TJ out from HAM5

21:29 (14:29) Jason out of PSL enclosure

21:37 (14:37) Elizabeth out of LVEA

22:01 (15:01) Betsy to LVEA -- investigate HAM5 HEPI

22:26 (15:26) Tyler out of LVEA

22:38 (15:38) Mark out of LVEA -- finished moving forklift

23:00 (16:00) End of shift

H1 SUS
betsy.weaver@LIGO.ORG - posted 15:34, Wednesday 04 April 2018 (41292)
H1 ETMY closeout TF's, door on WBSC10

I spend most of the day taking transfer functions of the ETMY main and reaction chains intermittant with my other crazy business.  Kissel took over after I exported all of the data but got a flag during the matlab processing of it and had wandered off with my patience.

Things look good with the plots now (as hinted via the quick looks at closeout yesterday), see attached.

Kissel has committed the new data to the SVN repository.  Data can be found at the usual Data or Results directories at

/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMY/SAG*/

Non-image files attached to this report
H1 General
yannick.lecoeuche@LIGO.ORG - posted 13:33, Wednesday 04 April 2018 (41290)
Weekly PSL Chiller Reservoir Top-Off

FAMIS 6569

Added 70 mL to crystal chiller.

H1 General
yannick.lecoeuche@LIGO.ORG - posted 13:12, Wednesday 04 April 2018 (41288)
H1 ISI CPS Sensor Noise Spectra Check - Weekly

FAMIS 6944

Reported ETMX frequency noise as being high.

Images attached to this report
LHO VE
chandra.romel@LIGO.ORG - posted 11:29, Wednesday 04 April 2018 - last comment - 17:23, Wednesday 04 April 2018(41285)
Venting vertex and turbos spinning on beam manifolds

Started venting vertex this morning and spun up turbos on XBM and YBM. Looks like IP1 isn't going to make it - its isolation GV is probably leaking. The new GV on IP4 is sealing great!

Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 12:50, Wednesday 04 April 2018 (41287)

Turned IP1 off.

michael.zucker@LIGO.ORG - 13:14, Wednesday 04 April 2018 (41289)

another one bites the dust. i hear there's room in the dumpster... 

chandra.romel@LIGO.ORG - 17:23, Wednesday 04 April 2018 (41298)

There are very few more satisfying feelings.

H1 ISC
keita.kawabe@LIGO.ORG - posted 17:08, Tuesday 03 April 2018 - last comment - 12:57, Wednesday 04 April 2018(41274)
replacing 1" pico mirror with fixed one in OMCR path, removing OMCR components downstream of SiC dump (Sheila, Keita)

We're replaced a 1" pico high reflector and a black glass behind with non-pico version in OMCR path. PSL beam was not available so no alignment.

We removed the following components from HAM6 (refer to D1000342):

We found that the black glass dump had some fogging on one of the two panels. Photos to follow.

Comments related to this report
sheila.dwyer@LIGO.ORG - 08:55, Wednesday 04 April 2018 (41278)

Yesterday Terry, Nutsinee and I also prepared for tomorow's in chamber work by settings the apertures in their original places on the squeezer path, and aligning the beam produced by scanning the OPO through the apertures.  We then moved the apertures out of the way.  

keita.kawabe@LIGO.ORG - 12:57, Wednesday 04 April 2018 (41286)

1st attachment shows before the change. Green is uninstalled, red is replaced.

2nd is after.

3rd, 4th. Fogging apparent for left panel of the black glass V dump. The difference between these two is that I'm illuminating different part of the panel using a green flashlight.

5th. Right panel under the similar lighting. The fogging is much less severe.

6th, 7th. Outer side of the left panel also has fogging.

Note that I was able to wipe this off easily using a dry Vectra Alpha wipe, it didn't need any force, just wipe and it's off. I only wiped off the left 1/4 of the inside of the left panel that looks foggy in picture 4.

The dump is on the flow bench in the cleaning area next to optics lab in OSB, if somebody wants to inspect.

Images attached to this comment
H1 SUS
betsy.weaver@LIGO.ORG - posted 15:59, Thursday 30 June 2016 - last comment - 14:46, Wednesday 04 April 2018(28090)
ETM15 Ears bonded

Between yesterday and today, Gerardo and I successfully bonded the ears to core optic mass ETM15, destined for LLO for post-O1 eventual replacement. 

Ear s/n 195 bonded to S3 flat of mass June 29, 2016

Ear s/n 196 bonded to S4 flat of mass June 30, 2016

The first ear (s/n 195) has a series of bubbles along it's edge, but the surface area of these do not add up to more than the allowed amount as per E1000277, so it passes, see pix attached.

The second ear (s/n 196) has no bubbles and is nice full bond. 

Images attached to this report
Comments related to this report
betsy.weaver@LIGO.ORG - 11:54, Friday 01 July 2016 (28118)

Inspection of the bonds this morning showed no change to the nice S4/Ear surface bond.

The small edge bubbles along the S3 Ear have migrated a bit (not worse, just moved a bit).  Therefore, we decided to rewet the edge with solution to see if it would wick in and close some of the bubbles.  This worked to close one of the larger bubbles, but one bubble continued to morph so we'll reinspect Monday.  Note, none of the sizes of the bubbles got bigger, so the surface area of the bubble total remains the same and below spec.

Images attached to this comment
betsy.weaver@LIGO.ORG - 10:02, Tuesday 05 July 2016 (28148)

Attached is a picture of what the bubbles in the ETM15 S3 Ear bond look like today (recall, it was bonded last Wed so it has now been over 5 days since initial bond).  Apparently over the weekend, the bubbles ran inbound a bit further.  I estimate the surface are of the bubbles to be near 20mm sq., still under the 50mm sq. spec. E1000278, although it isn't pretty.  I measured the longest streaks to be almost 3mm long, with a width of 0.4mm.  There are no bubbles inward from the edge near the center - anything shown in the picture is a camera reflection.

 

The S4 Ear bond looks unchanged from inspection last week, very good bond, very little bubbles.

Images attached to this comment
betsy.weaver@LIGO.ORG - 14:46, Wednesday 04 April 2018 (41291)

Pictures of this ear bond taken by Danny at LLO just before use at LLO, indicate that the bubbles have not changed shape or size since the picture attached July 2016.  Phew, said both Gerardo and I.

Images attached to this comment
Displaying reports 43921-43940 of 84071.Go to page Start 2193 2194 2195 2196 2197 2198 2199 2200 2201 End