Displaying reports 52961-52980 of 88171.Go to page Start 2645 2646 2647 2648 2649 2650 2651 2652 2653 End
Reports until 11:14, Wednesday 17 May 2017
LHO VE
chandra.romel@LIGO.ORG - posted 11:14, Wednesday 17 May 2017 (36236)
vertex pump down progress

Here's the latest pump down curve - log/log scale. Ideally we want to wait till 1.0e-7 Torr to open up to beam tube, but we can compromise with 2.0e-7 Torr. In that case, looks like we will be opening GV5,7 late next week.

We can open up GV 1,2 earlier if folks need oplev assistance for alignment.

Images attached to this report
LHO VE
chandra.romel@LIGO.ORG - posted 09:16, Wednesday 17 May 2017 (36234)
Turbos valved back into X&Y beam manifolds

I valved the turbos back into X&Y beam manifolds, valved out the IPs, and now X turbo is being backed by scroll (not turbo-leak checker), so both volumes are essentially identical. Trending pressure curve today. We have three full bottles of He on standby. ;)

H1 SEI (SEI)
cheryl.vorvick@LIGO.ORG - posted 09:06, Wednesday 17 May 2017 - last comment - 11:19, Wednesday 17 May 2017(36233)
HEPI Pump Trends - Monthly Plot

Attached is a trend plot of 45 days for the HEPI pumps.  I included the pressure channels from the vertex, where we are currently pumping down after venting to view/clean ITMX.  Changes in EY and EX Vout signals coincide with the vent, so possibly due to intentional changes.

Images attached to this report
Comments related to this report
hugh.radkins@LIGO.ORG - 11:19, Wednesday 17 May 2017 (36237)

Not sure if there were any intentional changes at the end station related to the vent that I'd think would impact these channels.  The changes appeared related to post shutdown of the pumps to do the Accumulator charge check and I would be suspicious of the motor restart after the check.  However, the pump speed is very dependent on the fluid temperature so looking at the VEA temps reveal a direct correlation with the pump speed, see related FMC log.  I'll give facilities a couple more days to smooth things out before more action.

H1 General
cheryl.vorvick@LIGO.ORG - posted 08:39, Wednesday 17 May 2017 (36232)
Ops Morning Update:
H1 AOS (IOO, ISC, SUS)
vaishali.adya@LIGO.ORG - posted 19:02, Tuesday 16 May 2017 - last comment - 17:48, Thursday 18 May 2017(36231)
ModeCleaner locking

[Jenne, Kiwamu, Vaishali with help from JimW and JeffK]

Continuing the locking effort from yesterday (36197), we managed to get the mode cleaner to lock. Here's a roll down of the events from today:

1. We (Jenne and I) first aligned the MC2 REFL camera because we were almost on the edge of the PD.

2. As this didn't fix the not locking problem, we asked Kiwamu for help and then we looked at a bunch of parameters like filters, gain thresholds, ramp times.  We also looked to check if the suspensions were behaving correctly and then found the mirror which had been turned off. This button (MC2 M2) was not in use at all. Maybe we should have double checked the sdf differences but we know better now.

While we were aligning the MC2 REFL we noticed that MC2 Trans wasn't looking like what it used to. We tried to trace the beam and found that the camera was being illuminated by a ghost beam and not the actual transmission beam of the MC. We found a bright spot by looking into the light pipe and then found that the beam wasn't coming onto the telescope at all. As we couldn't see anything on the viewer card, we turned up the laser power to 10 W and found the beam again in the light pipe only with the IR viewer.

Jenne then tried to gently tap the light pipe (this is the same pipe that had problems yesterday and was fixed) with me looking at the bright spot and it didn't move at all which leads to us believe that the beam might be hitting the edge of the table somewhere.

After hypothesising out loud that this might have been because the tables hadn't returned to the correct positions, we were corrected by JimW who told us that the ISIs return back to their positions on their own.

We then tried to change the axis of the modecleaner in order to redirect the beam in the light pipe but we weren't too successful.

Not having solved this mystery of what happened to MC Trans, we concluded the work for today with a modecleaner that locks at 2 W and 10 W.

Jenne will correct me if I have missed something or used wrong names of mirrors in comments !

Comments related to this report
jenne.driggers@LIGO.ORG - 11:10, Wednesday 17 May 2017 (36235)

I'm hoping that we can talk to someone today with some memory of how IOT2L used to look, because it seems pretty bad right now.  The beam that we suspect is the real IMC trans beam (which comes from the transmission through IM1) seems like it's hitting inside the light pipe, or the wall of the enclosure, but it's nowhere near the top periscope mirror. 

There is only one mirror on HAM2 to steer the beam transmitted through MC3 and IM1 out of vacuum, and it's on a standard fixed mount, so it doesn't seem like it should have the slip problems that we suspect exist with the IMC REFL path.  Since the HAM ISI tables restore their DC positions, the beam really ought to be coming out of the vacuum in nearly the same way it went in. 

We tried putting offsets in the IMC WFS loops (both DOF4, the uncontrolled degree of freedom and DOF1) to move the Trans beam around a bit, but to make any significant change to the ghost beam's position (and therefore, presumably, the actual beam's position) we were clearly misaligning the IMC. 

Anyhow, right now the IMC locks just fine.  We cranked the digital gain of the trans PD so that it looks like the ghost beam's power is similar to the actual beam, so that some of the filter module triggering works, but otherwise we don't really need IMC trans, so maybe we should move forward with the IFO rather than spending too much time with this.

jenne.driggers@LIGO.ORG - 17:48, Thursday 18 May 2017 (36274)

After talking with Cheryl this afternoon, she points out that the path the beam must take through the light pipe / ducting between HAM2 and IOT2L is extremely tight, much tighter than I had realized.  That ducting was dislodged on accident earlier this week when it was bumped, and when it was reattached it likely didn't get put back in exactly-exactly the right way.  So, probably the solution will be to scootch the middle part of the flexible ducting so that it's farther away from where the IMC Trans beam path needs to be.

H1 SUS
jeffrey.kissel@LIGO.ORG - posted 17:51, Tuesday 16 May 2017 (36230)
H1 SUS ITMX Clear of Rubbing (with no Alignment Offsets)
J. Kissel

Checking the bill of health of H1 SUS ITMX's suspension with standard driven transfer functions, I can say that both the main and reaction chains appear clear of rubbing without any normal offsets used in the Nominal Low Noise. Recall the ITMX reaction has had rather large offsets on for most of O2 to alleviate suspected rubbing (see e.g. LHO aLOG 33395). I'll do some more study tomorrow with various combinations of alignment and rubbing alleviating offsets in place to make sure that this statement holds in all locations we use.

For now, today's data lives here:
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMX/SAGM0/Data
    2017-05-16_2250_H1SUSITMX_M0_WhiteNoise_L_0p01to50Hz.xml
    2017-05-16_2250_H1SUSITMX_M0_WhiteNoise_P_0p01to50Hz.xml
    2017-05-16_2250_H1SUSITMX_M0_WhiteNoise_R_0p01to50Hz.xml
    2017-05-16_2250_H1SUSITMX_M0_WhiteNoise_T_0p01to50Hz.xml
    2017-05-16_2250_H1SUSITMX_M0_WhiteNoise_V_0p01to50Hz.xml
    2017-05-16_2250_H1SUSITMX_M0_WhiteNoise_Y_0p01to50Hz.xml
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMX/SAGR0/Data
    2017-05-16_2345_H1SUSITMX_R0_WhiteNoise_L_0p01to50Hz.xml
    2017-05-16_2345_H1SUSITMX_R0_WhiteNoise_P_0p01to50Hz.xml
    2017-05-16_2345_H1SUSITMX_R0_WhiteNoise_R_0p01to50Hz.xml
    2017-05-16_2345_H1SUSITMX_R0_WhiteNoise_T_0p01to50Hz.xml
    2017-05-16_2345_H1SUSITMX_R0_WhiteNoise_V_0p01to50Hz.xml
    2017-05-16_2345_H1SUSITMX_R0_WhiteNoise_Y_0p01to50Hz.xml

I'll export and compare with old reference data in due time.
LHO VE
chandra.romel@LIGO.ORG - posted 17:44, Tuesday 16 May 2017 - last comment - 18:21, Sunday 21 May 2017(36227)
X&Y beam manifold pressures

Interesting pressure trends on X & Y beam manifolds. See my previous aLOG about rate of rise test followed by pumping on just turbos (IPs valved out). PT180 (y-arm) trend has shifted and headed up! Does this mean the fault is in IP6 and not a leak?

Images attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 17:44, Tuesday 16 May 2017 (36228)

Valving in IPs and valving out turbos for the night.

kyle.ryan@LIGO.ORG - 18:08, Sunday 21 May 2017 (36304)
Also interesting is how PT170 steps "up" its reading when reacting to the, as yet unkown internal, gauge "step" change (voltage change?) while PT180 steps "down" when this unknown internal gauge change happens.  I wonder if the electronics use varying voltages for various pressure ranges etc?  
chandra.romel@LIGO.ORG - 18:21, Sunday 21 May 2017 (36305)

Those steps that I think you are referring to are me hard closing GV 5,7.

H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 17:04, Tuesday 16 May 2017 - last comment - 17:47, Tuesday 16 May 2017(36225)
Ring heater drivers back on temporarily

After speaking with Chandra, I've turned the RH drivers back on to do a test on the HWSY alignment right now.

I'm going to turn them off again in about 40 minutes.

 

Comments related to this report
aidan.brooks@LIGO.ORG - 17:41, Tuesday 16 May 2017 (36226)

The ring heater drivers are now switched off.

 

chandra.romel@LIGO.ORG - 17:47, Tuesday 16 May 2017 (36229)

Until we open gate valves 1 & 2, we don't have HV interlock protection on the vertex, so we shouldn't leave HVs on when not needed. Thanks!

H1 SEI
jim.warner@LIGO.ORG - posted 16:57, Tuesday 16 May 2017 (36224)
ITMX & HAM4 HEPI unlock, LHO Seismic back to running configuration

Because commissioning work is starting in earnest now, all of the seismic systems have been restored to their nominal configurations. This means ITMX & HAM4 HEPI's were unlocked yesterday after the cleanroom was moved out of the way, all HEPI's and ISIs are back up and running and all sensor corrections (including BRSs) are running on all chambers.

The only difficulty we found was the GS13 gain switching on HAM2 is no longer stable (ie we can't switch GS13 gains while the ISI is isolated). Hugh and I are working with Fil to try to figure that out, but this is a new "feature", we will probably be opening an FRS on it soon.

H1 PSL
jeffrey.bartlett@LIGO.ORG - posted 16:47, Tuesday 16 May 2017 (36223)
Install PSL Chiller Air Trap/Bleed
   Peter K. & Jeff B.  ECR E1700096

   Installed the PSL Air Trap/Bleed in the Crystal Chiller return line. The installation went well. Encountered one small issue. The pipe being cut was installed about 6 years ago. It did not cut as cleanly as the new pipe. On a couple of cuts the last third of the pipe broke before it was sheared through. Will need to be cognizant of this when installing the next three assemblies. 

   When the chiller was restarted the water compressed several inches of air in the standpipe. The ball valve at the top of the standpipe was used to bleed off excess air. I left about 4 inches of air trapped in the standpipe to act as a water flow damper. 

   The remaining three air Trap/Bleeders will be installed during the next big vent.         
Images attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 16:28, Tuesday 16 May 2017 (36222)
Ops Day Shift Summary
From 1 PM to 4 PM local time.

Good catch report:
I told Corey it was alright for him to open the high bay rollup door into the LVEA to push a pallet into the LVEA. Later I remembered that the LVEA was in laser hazard and therefore he should not do this. I managed to run over and stop him before he opened the door.

20:22 UTC Corey taking forklift to highbay to drop off pallet.
20:30 UTC Filiberto to end stations to check documentation.
20:40 UTC Karen driving car to VPW
20:42 UTC Corey opening high bay outside rollup door, driving forklift into highbay, dropping off pallet
Aidan and TJ to HAM4, work on HWS table
~ 20:59 UTC Let a truck related to Norco through gate. Could not understand driver after three attempts.

Gerardo changing IP6 from dualvac to gamma controller
21:22 UTC Filiberto back from end stations
22:13 UTC Betsy to LVEA to store equipment
22:17 UTC Jenne, Vaishali and Jeff to LVEA to talk to Aidan
22:25 UTC Jenne and Vaishali working on MC table
22:25 UTC Jeff K. taking transfer functions of ITMX, turning on sensor correction for ITMX
Jenne and Vaishali out of LVEA
23:13 UTC Aidan and TJ done in LVEA, TJ returning to get something
23:19 UTC TJ back
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 15:11, Tuesday 16 May 2017 (36216)
cooling ircuit pressure regulator
Attached are pictures of the pressure regulator and barometer for the auxiliary water
cooling circuit.  This circuit serves the power meters and water-cooled beam dumps on
the table.  The pressure in the circuit was ~3.5 bar, which seems to coincide with when
the regulator is fully closed.  The pressure is ~2.2 bar with the regulator fully open.

Useful information to have when or if we decide to remove the regulator from the cooling
circuit in the quest to simplify things.
Images attached to this report
LHO VE
chandra.romel@LIGO.ORG - posted 14:36, Tuesday 16 May 2017 - last comment - 16:18, Tuesday 16 May 2017(36213)
Troubleshooting x-beam manifold pressure discrepancy

[John, Chandra]

More investigation on leak hunt of x-beam manifold. Here's what we're trying now:

Images attached to this report
Comments related to this report
patrick.thomas@LIGO.ORG - 16:11, Tuesday 16 May 2017 (36217)
In regard to GV5 not showing as hard closed on the medm screen.

I looked at the Beckhoff code. It appears that I am just not seeing a change in signal (from 0 to 1) for the closed limit switch. Both the code and documentation agree that this should be LY terminal 2 channel 4.

On April 8 2015 Kyle reported that GV5 hard closed (https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=17748). I see this in the minute trends (attached). This is the most recent time I can find GV5 being hard closed from the alogs.

On April 26 2016 LY was upgraded to Beckhoff (https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=26803).

I guess we should check the wiring into the Beckhoff chassis?
Non-image files attached to this comment
patrick.thomas@LIGO.ORG - 16:18, Tuesday 16 May 2017 (36219)
From minute trends, the last time that GV5 hard closed is on March 14 2016.

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=26065
Non-image files attached to this comment
H1 FMP (DetChar, FMP, ISC, OpsInfo, SUS)
jeffrey.kissel@LIGO.ORG - posted 12:49, Tuesday 16 May 2017 - last comment - 15:03, Tuesday 16 May 2017(36208)
HVAC Upgrade at EY means H1 SUS ETMY (and likely TMS) Has Drifted / Sagged
J. Kissel

Charge measurements prefer the test mass suspension's optical levers be very well centered on their QPDs before starting. As I was centering the optics manually this morning, I found the H1 SUS ETMY suspension suspiciously low (pointed down) in pitch. After some investigation, I've learned that we're taking the opportunity during the break to upgrade the EY VEA HVAC system. After trending the optical lever, the L2 OSEMs in Pitch, and M0 OSEM in Vertical, coupled with the (formerly correct?) channel for temperature, I can see some sort of obvious, large, drift in the suspension that would be easily explained by VEA temperature excursions.

I merely post this as a reminder that once we get the VEA temperature back under control -- and back to the VEA's former temperature set point, we'll need to re-assess ETMY and TMSY suspension alignments. 

For now, I've left ETMY with its alignment centered on the optical lever.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:24, Tuesday 16 May 2017 (36212)DetChar, FMP, ISC, OpsInfo, SUS
A little more poking around reveals that the Y-End Beam Rotation Sensor also sees an effect of the HVAC upgrade's resulting temperature changes in the Y VEA. Namely, it shows / confirms the ~3 hour, +/- (1 deg F / 0.5 deg C) oscillation in temperature reported by the FMCS channel and by the ETMY optical lever (presumably the vacuum system's effective low-pass filter is filtering out this "fast" oscillation). Note, that the variance in the VEW temperature previously was only about (+/- 0.25 deg F / 0.1 deg C). Since this is seen in both the optical lever and in the beam rotation sensor, I'm quite confident that this is a real temperature swing.

Further note -- the static temperature has also changed after the upgrade. We used to hold the VEA at 68.0 deg F / 20 deg C, but it appears as though the upgrade has left the VEA at 67.1 deg F / 19.5 deg C. This likely explains the long term sag / pitch of the ETM.

John will write a more detailed log later, but upon pointing this out to him, he adjusted the HEATING OFFSET and COOLING OFFSET in the new HVAC control system in hopes to reduce the ~3 hour temperature oscillation. He changed the values from 1 deg F to 0.25 deg F (though the system echoed back that these are now set to 0.0 deg F). He'll work with Bubba to change the static temperature.
Images attached to this comment
jeffrey.kissel@LIGO.ORG - 14:53, Tuesday 16 May 2017 (36214)CAL
J. Kissel

Also note that PCAL Y sees a substantial effect of the large temperature excursions seen in the VEA during the upgrade as well, indicating that there is still some temperature sensitivity left in the system, like what was seen back in January (see, e.g. LHO aLOG 34153). 

The gross clipping has gone away since the temperature has *mostly* recovered, but -- presumably because of the 0.5 deg C difference in static temperature, the RXPD is reporting 0.2% higher displacement than before the HVAC upgrade. Further, one can see the ~3 hour oscillation in the RX and TX PDs.
Images attached to this comment
john.worden@LIGO.ORG - 15:03, Tuesday 16 May 2017 (36215)

For the record I have changed two parameters in the ENDY VEA heat/cool control.

Both "Heating Offset" and "Cooling offset" were set to 1F. I reduced these both to 0.5 after discovering that the system would not accept 0.25. The setpoint is 68F (which it was before)

The control routines may need fine tuning to get back to the control level we had before this upgrade. We await the Apollo expert for this.

See the attached screen shot. An updated temperature trend is also attached and shows a response to our changes.

Images attached to this comment
H1 SUS (CDS)
filiberto.clara@LIGO.ORG - posted 16:56, Thursday 11 May 2017 - last comment - 16:21, Tuesday 16 May 2017(36143)
High Voltage Supplies for ESD Drivers

WP 6625
ECR E1600210

The Kepco HV power supplies for ITMX, ITMY, and ETMX were replaced with an equivalent linear supply made by Mid-Eastern Industries Inc. Power supplies for ETMY were replaced on Dec 5 2016. Alog 32186.

New units installed:
S1700114 & S1700115 ITMY/ITMX
S1700116 & S1700117 ETMX
S1610431 & S1610433 ETMY

Comments related to this report
filiberto.clara@LIGO.ORG - 16:21, Tuesday 16 May 2017 (36221)
Units at EY are S1610431 & S1610432. Previous entry with S1610433 is incorrect.
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