Displaying reports 44501-44520 of 88464.Go to page Start 2222 2223 2224 2225 2226 2227 2228 2229 2230 End
Reports until 17:24, Wednesday 14 November 2018
LHO VE
chandra.romel@LIGO.ORG - posted 17:24, Wednesday 14 November 2018 - last comment - 16:06, Monday 19 November 2018(45285)
NexTorr HV1600-10 data

We finally got a chance to test a new "high vacuum" style 1600 l/s NEG pump, installed at only EY, on BSC6, at relatively high pressures after the BSC10 vent. At around 3e-5 Torr, I valved in the HV1600 (turned its built-in 10 l/s IP off first), shortly after having spun up the main 2000 l/s turbo pump. After three hours of pumping, I cycled valves in time series below, all while running the RGA in faraday mode. Times are local.

(turbo pump valved in at start)

  1. 2:45p:  pressure = 3.4e-6 Torr; valved out NEG
  2. 3:00p:  pressure = 3.6e-6 Torr; valved in NEG
  3. 3:05p:  pressure = 3.4e-6 Torr; valved out turbo
  4. 3:11p:  pressure = 6.9e-6 Torr; valved out NEG (both NEG & turbo valved out here)
  5. 3:18p:  pressure = 1.0e-5 Torr; valved in NEG
  6. 3:48p:  pressure = 1.2e-5 Torr: valved in turbo

Annotated pressure plots attached.

*these hot cathode wide-range gauges have a large offset and don't follow pressure readings from cold cathode gauges until it changes emission current at 5.6e-6 Torr

By itself, this NEG pump is not able to maintain the gas load, but does contribute to pumping in high vacuum region.

I haven't had a chance to look at partial pressures yet, but RGA scan is attached.

 

 

Images attached to this report
Non-image files attached to this report
Comments related to this report
chandra.romel@LIGO.ORG - 16:06, Monday 19 November 2018 (45408)

RGA data collected this afternoon in SEM mode. Main turbo and HV1600-10 both valved in. Total pressure measures 1.4e-7 Torr.

Non-image files attached to this comment
LHO VE
kyle.ryan@LIGO.ORG - posted 16:46, Wednesday 14 November 2018 - last comment - 17:44, Thursday 15 November 2018(45284)
Switched Y-end Turbo backing pumps from QDP80 to local scroll pump

Jeff B. phoned me while I was doing this as he had noticed a very large spike in particulate in the Y-end VEA which exactly correlated with my having done this.  Investigation revealed that the Y-end Turbo's local scroll pump never got a particulate filter installed at its exhaust - Ooops!  -> I located this unit and will install it. 

Also, the chilled water booster pump used with the QDP80 is now leaking at the pump end -> will put this on the list. 

Comments related to this report
chandra.romel@LIGO.ORG - 17:29, Wednesday 14 November 2018 (45287)

FRS ticket 11827

kyle.ryan@LIGO.ORG - 17:44, Thursday 15 November 2018 (45321)

11/15/2018

I installed the particulate filter on the exhaust of the Y-end local scroll pump.

LHO VE
kyle.ryan@LIGO.ORG - posted 16:40, Wednesday 14 November 2018 (45283)
Torqued 2.75

I was asked to final-torque the 2.75" CFF which is part of the recently replaced squeezer fiber cable assembly at HAM6.  Fabrice had installed this assembly previously but was concerned about using a wrench to complete the task as multiple mechanically vulnerable components reside close by. 

For future reference, I have attached a photo showing the routing of this fiber (within orange loom) - Don't mechanically manipulate this run of fiber. 

Images attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 16:28, Wednesday 14 November 2018 (45282)
HAM1 West and East doors removed

Bubba G., Chris S., Gerardo M., Kyle R.

Removed HAM1's West then East doors (Chandra R. & Corey G. had prepped yesterday). 

~1/2 of the West Door's outer O-ring came out of its groove and contacted the C3 material placed on the floor for just such an event.  During the handling to re-seat the O-ring, we noticed excessive debris on it including a sliver of what looked to be remnant adhesive - from tape?  This was easily and completely removed.  However, considering the fact that this door had been leak tested under much scrutiny following the last door cycle, combined with the excessive particulate observed today, Chandra R. has elected to replace this O-ring when the door goes back on and not gamble on the sealing integrity.  The dirty O-ring can be reprocessed for future use.  A possible explanation as to the excessive debris could be the result of having removed all-but-four door bolts prior to the final wipe-down of the chamber.  A gap between the door and chamber flanges, large enough to allow debris to enter via wiping the flange perimeter, results when the door is prepped for removal.  We ended up being out of "sync" with this door removal exercise when compared to our normal sequence and didn't recognize this contamination potential. 

H1 General
jeffrey.bartlett@LIGO.ORG - posted 16:00, Wednesday 14 November 2018 (45280)
Ops Day Shift Summary
Ops Shift Log: 11/14/2018, Day Shift 15:00 – 23:00 (08:00 - 16:00) Time - UTC (PT)
State of H1: Unlocked for vent
Intent Bit: Maintenance
Support: N/A
Incoming Operator: N/A
Shift Summary: Vent and vent close out activities dominated the day’s work efforts.   

 

Activity Log: Time - UTC (PT)
14:25 (06:25) Peter – In the PSL enclosure
15:11 (07:11) Vanessa – Into the LVEA
15:13 (07:13) Karen – Into the LVEA
15:18 (07:18) Chris – Tumbleweed bailing on X-Arm
16:00 (08:00) Start of Shift
16:12 (08:12) Karen & Vanessa– Finished in LVEA
16:20 (08:20) Gerardo – Going to HAM1 to work on doors
16:22 (08:22) Karen – Going to End-Y
16:31 (08:31) Sheila – Transition LVEA to Laser Safe (WP #7943)
16:35 (08:35) Chris – Finished with tumbleweed bailing
16:48 (08:48) Ed – Going to Squeezer Bay to look for cables
16:50 (08:50) Hugh & Corey – Going to HAM1
16:54 (08:54) Charles – Going to HAM1 to observe door removal
17:00 (09:00) Jeff J. – Going to HAM1 to observe door removal
17:03 (09:03) Richard & Ed – Going to LVEA to PSL racks
17:12 (09:12) Niko – Going to HAM1 for cabling & L4C work
17:15 (09:15) Richard & Ed – Out of the LVEA
17:18 (09:18) Marc – Going to End-X to pull a couple of chassis for repair
17:19 (09:19) Karen – Finished cleaning at End-Y
17:22 (09:22) Ed – Going to End-X and End-Y to drop off electrical equipment
17:25 (09:25) Jason – Going to PSL enclosure
17:52 (09:52) Hugh & Sheila – Going to HAM1
17:53 (09:53) Charles & Jeff J. – Out of the LVEA
17:59 (09:59) Hugh – Out of the LVEA
18:00 (10:00) Finished pulling HAM1 doors
18:05 (10:05) Filiberto – Pulling cable at PSL racks
18:14 (10:14) Shelia & Hugh – Out of the LVEA
18:19 (10:19) Ed – Transitioned End-X to Laser Hazard because one table door is unlocked.
                              Could not find Key at End station
18:25 (10:25) TvO and Dan – Going to TCS tables
18:30 (10:30) Sheila – Transitioned LVEA to Laser Hazard (WP #7944)
18:32 (10:32) Terry – Going to HAM6
18:35 (10:35) Sheila – Going to HAM6
18:38 (10:38) Chandra – Going to End-Y to start turbo
18:45 (10:45) Karen – Cleaning in LVEA around HAM1& Optics Lab
19:11 (11:11) Robert – Into the Diode Room and PSL enclosure to look for noise in PSL cooling system
19:40 (11:40) Chandra – Going to End-Y to work on RGA
19:41 (11:41) Cheryl – Going into the PSL enclosure
19:42 (11:42) Betsy – Going out the HMA1
19:43 (11:43) TvO and Niko – Out of the LVEA
19:47 (11:47) Hugh & contractor – Going to End-X to look at wind fence
19:52 (11:52) Karen –Out of LVEA and Optics Lab
20:02 (12:02) Chris – Back
20:05 (12:05) Betsy – Into the LVEA to check on HAM1 progress
20:10 (12:10) Jason – Out of the PSL enclosure
20:20 (12:20) Betsy – Out of the LVEA
20:30 (12:30) Corey & Niko – Out of the LVEA
20:33 (12:33) Robert – Out of the PSL enclosure
20:35 (12:35) Cheryl – Out of the PSL enclosure
20:58 (12:58) Georgia & Keita – Going to HAM1
21:00 (13:00) Ed – Going to HAM1 to pull cable
21:15 (13:15) Richard – Going to HAM1
21:20 (13:20) Peter – In the PSL enclosure
21:30 (13:30) Terry & Sheila – Out of the LVEA
21:36 (13:36) Robert – Out of the PSL enclosure and LVEA
21:48 (13:48) Hugh, Corey, Niko – Going to HAM1
21:54 (13:54) Chris – Going into the LVEA to look for keys
21:59 (13:59) Chris – Out of the LVEA
22:00 (14:00) Jason – Going into the PSL enclosure
22:04 (14:04) Filiberto – Going to HAM1 for cabling work
22:08 (14:08) Marc – Going to End-X to replace chassis removed this morning
22:14 (14:14) Richard – Going to HAM1
22:16 (14:16) Chandra – Going to End-Y to work on NEG pump
22:38 (14:38) Terry & Sheila – Going to Squeezer table
23:01 (15:01) Ed – Delivering cable to Peter in PSL enclosure
23:12 (15:12) Georgia – Out of the LVEA
23:13 (15:13) Ed – Out of the LVEA
23:36 (15:36) Dave – Going to End-X
23:43 (15:43) Rick – Taking lens to PSL enclosure
23:43 (15:43) Ed – Going to End-X to lock table
24:00 (16:00) End of Shift
H1 AOS (ISC)
georgia.mansell@LIGO.ORG - posted 16:00, Wednesday 14 November 2018 - last comment - 08:21, Thursday 15 November 2018(45279)
ISC HAM1 work today - POP beam diverter replaced, inital tests of LSC-REFL_B completed

Keita, Richard, Corey, Craig, Georgia

Images attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 16:06, Wednesday 14 November 2018 (45281)

For now,

  • REFL B is only held at an approximate place using just one screw.
  • 50:50 BS for REFL_A REFL_B splitting is yet to be installed.
  • Black glass beam dump for REFL_B is yet to be installed.
  • 5-way coax continuity check was done for the feedthrough but we don't know if the RF connection at the diode is good.

These are finalized/installed/checked on Saturday after the PSL beam becomes available and IMC locked in vacuum.

 

alena.ananyeva@LIGO.ORG - 08:21, Thursday 15 November 2018 (45298)
Here is some experience on cleaning the foggy patterns on black glass:
https://nodus.ligo.caltech.edu:8081/OMC_Lab/283
https://nodus.ligo.caltech.edu:8081/OMC_Lab/283
H1 SUS
betsy.weaver@LIGO.ORG - posted 13:27, Wednesday 14 November 2018 - last comment - 10:32, Monday 19 November 2018(45278)
ETMY and TMS Transfer Functions good

After quick peeks at the TFs at closeout yesterday showed healthy suspensions, the door to the chamber was closed and pump downs started.  Today, Travis and I ran the full set of Transfer functions for ETMY MAIN, REACTION, and TMSY suspensions (18 measurements).  All plots look good and can be found at 2018-11-14* Files in the appropriate directories.  Between Travis and I, we're a few hours into this today (running, exporting, troubleshooting matlab, etc) and I need to move on to other things, so pretty plots aren't going to be posted today, especially without the auto-renumbering scrip at my fingertips for the master plotting script.  See the files if you want to look at them yourself although I still need to commit them to the svn.

Comments related to this report
betsy.weaver@LIGO.ORG - 08:56, Monday 19 November 2018 (45381)

Note, the alignment offsets were ON for these measurements.

Directory of measurements:

ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ETMY/SAMG0/Data/2018-11-14-1658_H1SUSETMY_*

or R0 and Results directory for processed matlab files.

betsy.weaver@LIGO.ORG - 10:32, Monday 19 November 2018 (45389)

Can't commit data to svn because it throws an error about upgrading svn.  I was working on the "controls login.  Maybe someone can fix this.

LHO VE
chandra.romel@LIGO.ORG - posted 11:39, Wednesday 14 November 2018 - last comment - 12:07, Wednesday 14 November 2018(45275)
EY turbo spun up and NexTorr valved in

Spun up main turbo pump and also valved in a new NEG pump that we're testing at EY that is designed to pump relatively high pressures (e-4/e-5 Torr range). I turned its little ion pump off before valving in.

Purge air valve is closed.

The chilled water booster pump is leaking water in mechanical room. Kyle is investigating.

Next I'll valve in RGA and warm up filament to collect some data on NEG.

Comments related to this report
chandra.romel@LIGO.ORG - 12:07, Wednesday 14 November 2018 (45277)

Turned EY RGA filament on at 12:07 pm local.

H1 CDS (ISC)
filiberto.clara@LIGO.ORG - posted 10:30, Wednesday 14 November 2018 (45274)
Field Cabling for HAM1 REFL PD

Installed new DB25F to DB9M cable from ISC-R1 to HAM1. Part of installation of new REFL Photodiode.

Pin Layout:

DB25 Pin 1 to DB9 Pin 1
DB25 Pin 14 to DB9 Pin 6
DB25 Pin 2 to DB9 Pin 2
DB25 Pin 15 to DB9 Pin 7
DB25 Pin 3 to DB9 Pin 3
DB25 Pin 16 to DB9 Pin 8
DB25 Pin 4 to DB9 Pin 4
DB25 Pin 17 to DB9 Pin 9

Pin 5 on DB9 not connected.

H1 General
jeffrey.bartlett@LIGO.ORG - posted 08:02, Wednesday 14 November 2018 (45272)
OpsDay Shift Transition
Ops Shift Transition: 11/14/2018, Day Shift 15:00 – 23:00 (08:00 -16:00) - UTC (PT)
State of H1: Unlocked for vent  
Intent Bit: Maintenance
Weather: Fog turning to overcast, Highs forecast to be in the upper 40s   
Primary 0.03 – 0.1Hz: 0.02µm/s
Secondary 0.1 – 0.3Hz: 0.3µm/s
Outgoing Operator: N/A
Quick Summary: Work at End-Y, HAM6, HAM1 and in the PSL
LHO VE
kyle.ryan@LIGO.ORG - posted 07:12, Wednesday 14 November 2018 (45270)
~0650 hrs. local -> Resumed attended pumping of Y-end

I valved-in the BSC10 AIP that had been isolated whilst the remaining portion of the annulus piping had been vented for the door removal.  Upon doing so, the turbos spun down as the AIP isolation valve must have leaked -> a lot!

LHO VE
chandra.romel@LIGO.ORG - posted 22:36, Tuesday 13 November 2018 (45268)
EY rough pumping (valved out for night)

We started pumping on EY volume around 4pm local and continued for 6 hours before valving out for the evening. Pressure is currently at 1.6 Torr (same reading at local gauges on turbo station). Will valve back in tomorrow morning and spin up the turbo at ~100 mTorr.

I first closed the header o-ring valve, then the 10" gate valve, and finally the safety valve. This gate valve is the only CETEC turbo valve left in operation (aside from midstations and H2). When I closed it the wheel rotated CCW (open) slightly with spring back. I didn't want to over extend and break something (known to happen with these valves) so I turned it in CW direction a few times until the spring back dissipated. I closed the safety valve as well since there is a leak in foreline behind it.

Leaving site now.

 

Images attached to this report
H1 AOS (DetChar)
robert.schofield@LIGO.ORG - posted 19:13, Tuesday 13 November 2018 (45241)
DARM coherence with EX ESD power supplies, mains monitors, and chamber-to-rack voltages around 60 Hz and other frequencies

I looked at the coherence between DARM and the ESD power supply voltage monitors (the power supply voltages are run into temporary PEM channels through high-pass filters - soon to be permanent). There was quite a bit of coherence around 60 Hz, explaining some, but not all of the features around the 60 Hz peak in DARM (see Figure 1). Some of the other 60 Hz sidebands in DARM are associated with suspension resonances at about 0.4 Hz (Figure 2). There is also a roughly 1 Hz comb of side bands that is visible in the temporary channel that monitors the voltage between rack ground and the chamber (Figure 1) as well as in the mains monitors at all stations (Figure 3). Finally, at certain other frequencies, such as around 280 Hz, there is also strong coherence between DARM and power supply or rack-to-chamber voltage monitors (Figure 4).

We hope that at least some of the noise from the power supply will be reduced once the ESDs have dedicated power supplies (I think the plan is to replace them this week), but the 1 Hz comb on the mains, at least, will still likely couple and needs to be tracked down. I have doubts that the broad features around 280 will go away either, since they are in the rack-to-chamber voltage monitors as well as the power supply monitor.

Non-image files attached to this report
H1 IOO (IOO, PSL)
cheryl.vorvick@LIGO.ORG - posted 19:11, Tuesday 13 November 2018 (45265)
IO optic inspection identifies L1 as having areas of contamination or damage to the coating

I inspected the optics in the IO path on the PSL, and discovered that L1, the first lens after the EOM, has one easily identifiable area on the surface near the EOM, and two easily identifiable areas on the surface away from the EOM, that are contamination/damage to the coating.  Two areas are at or close to the center of the optic, the other area is about 1/8th of the optic that is covered in what looks like a thick film.

The first three images attached are of L1:

  1. L1, looking toward the EOM, this is the "filmed" area, it's on the surface that's closer to the camera, with a reflection from the other side of the lens.  There are circular marks through the film and this looks like someone used a wipe to clean the optic, possibly for dust, and happened to clean off a bit of film.  The film was only visible to me with the flashlight.
  2. L1, looking toward the EOM, and the "filmed" area is on the left side, there's a large bright white spot and reflections that are from the flashlight above the filmed area, and to the right there is a small area of contamination/damage that looks somewhat like a ring.  This is on the surface that's closer to the camera, and it's close to the center of the lens.
  3. L1, looking toward the EOM, showing the contamination/damage that's on the surface that's closer to the EOM, on the EOM side of the lens.  This is feature has very clear edges, and is close to the center of the optic.

With L1 being very close to the EOM output, I was not able to see the output face of the EOM crystal, so this still needs ot be inspected, and the best opportunity to do this is when L1 is replaced.  The EOM crystal surface sits within a few mm of housing aperture, so it can be seen through the EOM housing.

The last two images attached are of the EOM output aperture and crystal:

  1. the EOM output aperture from the -Y side of the PSL table, where the output aperture faces in the +X direction.  This image shows the crystal without IR light, so the crystal is seen through the EOM housing and is dark, and at this viewing angle, the right front edge of the crystal face is visible.
  2. the EOM output aperture from the -Y side of the PSL table, where the output aperture faces in the +X direction.  This image is from a similar viewing angle with IR light, taken with an IR sensitive camera, and there's a back reflection from L1 that is clipping on the EOM housing, and through the aperture, the right front edge of the EOM crystal is seen as a vertical line, which matches it's location in the first image.

I talked to Daniel, and he saw the images, and we talked about replacing this lens after recovering the IMC, so next week or later, and before O3.

Images attached to this report
H1 PSL
jason.oberling@LIGO.ORG - posted 17:55, Tuesday 13 November 2018 - last comment - 06:13, Wednesday 14 November 2018(45262)
Summary of PSL Work Today

J. Oberling, P. King, J. Bartlett, R. Savage

Following on from yesterday's plumbing work, today we concentrated on recovering the 35W FE, the 70W amplifier, and completing the remaining items from FRS 10753.

This morning, Peter recovered the 35W FE without much fuss and also installed the new solid block base for the 70W amplifier.  He and I recovered the 70W amplifier, also without much trouble; we tweaked beam alignment for a compromise of power and beam quality and were able to return the beam very close to what it was before the new base installation.  We then proceeded to take a beam propagation measurement to use in PMC mode matching.  This was necessary as the installation of the new amplifier base resulted in the 70W amp moving closer to the PMC by ~1/2", which in turn will have an effect on PMC mode matching.  At this point we broke for lunch.

The final part we needed to complete the chiller work (an adapter for installation of a throttling valve on the supply line out of the chiller) arrived today, so this afternoon Jeff and I installed the valve.  After leak checking and leak fixing, we fired the chillers up and all was well.

Rick and I then balanced the flows and pressures out of the crystal chiller.  To do this we completely opened the new external bypass Jeff installed a couple months ago and completely closed the chiller's internal bypass; this internal bypass being open was what was causing the very high operating pressure (70 psi!) for the system.  In this configuration the chiller had a flow of 38 lpm.  We then used the throttling valve to reduce the overall chiller flow to 18.7 lpm (keep in mind that the external bypass was still completely open, so almost all of that water was flowing through the bypass, not the PSL manifold).  We then slowly closed down the external bypass to provide a pressure drop for the PSL manifold, therefore letting water flow through the various cooling circuits.  As it stands right now, the flows and pressures of the PSL cooling system are:

Please keep in mind that most of that chiller flow is still going through the external bypass.  This is an absolutely huge improvement as prior to this work we were running with a manifold inlet pressure of 70 psi (!!!).  At this point I returned to the enclosure to return it to "Science Mode" so Robert can assess if all of this plumbing work made a difference in PSL table vibration.  Tomorrow we will begin mode matching the PMC, with our goal being >50W transmitted power with the ISS ON.

Comments related to this report
richard.savage@LIGO.ORG - 20:54, Tuesday 13 November 2018 (45267)PSL

One small, but important, clarification.  

The high supply- and return-side pressures observed earlier were not due to the internal bypass being open.  They were due to the 50 psi pressure drop across the heat exchanger due to the high total flow (internally bypassed, externally bypassed, and through the laser circuits) going through the heat exchanger (on order 30 lpm) inside the chiller on the return path to the open reservoir.

Similar pressures were observed with the internal bypass closed but the external bypass open, also giving about 30 lpm through the heat exchanger.

Closing the internal bypass valve, reducing the pump output flow by about a factor of two using the throttling valve,  and adjusting the flow through the laser circuits using the external bypass valve allowed us to set the desired flows through the laser circuits while reducing the overall system pressure.

This scheme was developed in consultation with J. Riebock, an engineer at TechnoTrans, US rep for the chiller manufacturer.

peter.king@LIGO.ORG - 06:13, Wednesday 14 November 2018 (45269)
Front end and neoVAN flow rates for the past day.  Clear reduction of flow rates observed
after the plumbing work.  Still settling out I would think.  The 4 excursions in the front
end flow rate are probably bubbles making their way through the system.
Images attached to this comment
H1 SQZ (SQZ)
haocun.yu@LIGO.ORG - posted 17:32, Tuesday 13 November 2018 - last comment - 09:21, Thursday 15 November 2018(45261)
VOPO Alignment and Mode Matching

[Sheila, Fabrice, Nutsinee, Terry, Haocun]

Summary:

We have OPO coupling 89% 00 mode, alignment >~95%, mode matching >~95% and polarization mode ~2%.

I will add more details with numbers later.

Comments related to this report
haocun.yu@LIGO.ORG - 11:51, Wednesday 14 November 2018 (45276)

Detailed measurements:

These numbers are the best ones we tried to take because the signal was noisy in air.

  • 00 mode peak: 387.5mV (max: 441; min: 344)
  • Polarization mode: 87mV
  • 10 mode (misalignment): 92~93.6mV
  • 20 mode (mis-mode matching): 92mV
  • Dark noise: 78mV

 

Calculation:

  • 00 mode: 89%
  • Polarization mode: 2.6%
  • Misalignment: 4.5%
  • Mis-mode matching: 4% (Mode matching efficiency = 96%)

 

nutsinee.kijbunchoo@LIGO.ORG - 09:21, Thursday 15 November 2018 (45303)

Here's a picture of the scan. Will go back and save the data properly later.

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 11:32, Tuesday 13 November 2018 - last comment - 10:07, Wednesday 14 November 2018(45252)
EY models crashed at 11:04

At 11:04 most models stopped running at EY. We are currently unsure if this is a Dolphin crash or caused by electrical work at EY.

Interestingly in addition to the expected corner station IPC errors, all SEI frontends have an ADC error on their IOPs.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 16:33, Tuesday 13 November 2018 (45260)

And to answer the question of what is special about the seismic IOP models: they all have Dolphin receivers.

david.barker@LIGO.ORG - 10:07, Wednesday 14 November 2018 (45273)

However, h1susitmpi is a 64kHz user model with Dolphin receivers.

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