Displaying reports 44341-44360 of 88488.Go to page Start 2214 2215 2216 2217 2218 2219 2220 2221 2222 End
Reports until 21:44, Friday 23 November 2018
H1 ISC (GRD, IOO, ISC, SQZ)
georgia.mansell@LIGO.ORG - posted 21:44, Friday 23 November 2018 - last comment - 23:25, Saturday 24 November 2018(45474)
Vent recovery/commissioning today

Daniel Brown, Cheryl Vorvick, Haocun Yu, Terry McRae, Georgia Mansell

Summary: Today we started recovering the corner IFO after the vent. We worked on IMC/IO revival, alignment, and squeezer alignment. The IMC recovered well and we have reasonable transmission and reflection levels.

We are currently having a guardian/front end problem when locking PRMI - The ISC_DRMI guardian tries to turn on H1:LSC-MICH1_FM2 when it reaches the PRMI_LOCKED state. This filter module has a yellow "LC" flag above it on the MEDM screen (does this mean it is under local control?), and toggling the button or trying to set it in a guardian shell does not work. We're not sure how to get around this. First attachment is the guardian log when trying to toggle FM2.

While PRMI acquires easily we're having trouble locking DRMI (a familiar situation with short locks but nothing that holds well).

General vent recovery

- I transitioned the LVEA to laser hazard

- Turned on the HAM6 PZT HV and fast shutter HV

- Turned on the fast shutter chassis (in the rack next to isct6), and enabled its high voltage

- note HAM6 HEPI is locked, so we left its guardian paused, in the READY state, and the SEI_HAM6 guardian in ISI_DAMPED_HEPI_OFFLINE

- We've set the gate_valve_flag parameter in lscparams to True, so we can do DRMI without arms

IMC revival

- We locked the IMC at 2 W, it was clearly misaligned in yaw to start off with. We adjusted MC2 so we could lock on the 00 mode nad used the WFS to fix the alignment

     - Note to self, to get the WFS going from a pretty rubbish first alignment we had to lower the trigger threshold (from 40 to 21), then increase the IMC WFS gain by hand from 0.04 to 0.4. We waited for the WFS to converge then offloaded them with the IMC_LOCK guardian.

- The reflected power of the IMC is at 8.3 mW [edit: this was a typo, it's at 0.083 mW with ~1.9W input power], reduced again after two-tuesdays-ago's mystery excursion.

- Cheryl ran the IMC-spot-position measuring script. She tried to restore the IMC mirrors to their positions back in August, using the witness sensors, but found this was not a good alignment. She later found a good alignment.

Corner station alignment

 - We mostly got through initial alignment with the ALIGN_IFO guardian without too many problems, we couldn't do input align without the arms locked though

- We first did MICH_DARK and MICH_BRIGHT to check the contrast defect with the new TCS settings. Initially we measured ~1% contrast defect, however after we tweaked up the input alignment this was reduced to ~0.65%.

- To adjust the input alignment we went to the PRC_ALIGN state of ALIGN_IFO and adjusted IM4 and PR2 by hand to increase LSC_POP_A_LF. The input alignment might not be optimal yet.

Squeezer work

We repeated the squeezer single-bounce tests reported in alog 45375, with more seed power. We have ~20 counts on AS_A and AS_B when bouncing the seed beam off the SRM, compared with 8 counts 1 week ago. We still didn't have enough power to see the squeezer beam reflected off ITMX when SRM is misaligned. The second attachment shows the squeezer seed beam, as reflected off SRM, visible on the AS_AIR camera on ISCT6. Qualitatively, it does not look obviously astigmatic.

Images attached to this report
Comments related to this report
georgia.mansell@LIGO.ORG - 23:11, Saturday 24 November 2018 (45478)

Daniel Brown, Thomas Vo, Georgia Mansell

  • Today we locked DRMI-no-arms with a couple of different IFO alignments. The buildups we saw on POPAIR_B seemed quite reasonable. In PRMI_LOCKED we saw ~34 on RF18 and ~47 on RF90.* In DRMI_LOCKED we saw ~30-40 on RF18 and ~12 on RF90.
  • We saw lower counts on RF18 with what looked like a more stable DRMI lock, and with a nicer beam on ASAIR. So we went to ISCT1 to check the alignment onto POPAIR_B. The alignment seemed fine. We note that the beam on AS AIR with DRMI locked looks pretty good which suggests our 50W TCS settings haven't messed things up too bad.

 

  • TVo fixed our trigger mask problem which was preventing us from engaging the integrator (MICH1 FM3) with PRMI locked, as mention in the above alog. The DRMI_MICH_FMs threshold was too high for PRMI with no arms. We made a new lower set of thresholds in lscparams for DRMI with no arms.

 

  • Dan and I plugged in and realigned the OSA on the AS port (on a pick off from the AS AIR camera path) to use as a diagnostic while tuning common/differential CO2 power. Dan will post an image of the scan currently.

 

  • At the end of the evening we lost the PSL with what looks like another crystal chiller trip.

 

*actual channels I'm quoting are POPAIR_B_RF[18/90]_I_NORM_MON

daniel.brown@LIGO.ORG - 23:25, Saturday 24 November 2018 (45479)

Images of AS AIR on DRMI lock today with the current 50W pretunings.

We also began tuning CO2 differentially to see how the sideband build up on the OSA changes. The OSA scan attached is after the first step of 100mW change. Another 100mW change was applied but we lost DRMI and then the PSL went down.

Images attached to this comment
H1 AOS (PSL)
peter.king@LIGO.ORG - posted 16:34, Friday 23 November 2018 - last comment - 16:40, Friday 23 November 2018(45471)
PSL chiller flow rates
Attached is the trend data plot for the flow rates in the power meter circuit, the front end laser, and the 70 W amplifier.
Lots of glitches, not sure of the reason why.  Especially when compared to the 70 W amplifier cooling circuit.

    The diode chiller is indicating an error message of "F3-error", which is something related to the hot gas valve.  That
might be an indication that the diode chiller needs servicing, I don't know.  The diode chiller temperature over the same
period of time looks pretty constant at 20 +/- 0.2 degC.  The diode chiller flow looks pretty constant over the same time
interval as well.

    The flow rate from the crystal chiller is noticeably lower upon restart.  14 lpm cf. 15.7 lpm.

    After restarting the laser, the power meter flow somewhat regularly flashes red indicating that the flow rate has
dropped to 0.5 lpm or lower.
Images attached to this report
Comments related to this report
peter.king@LIGO.ORG - 16:40, Friday 23 November 2018 (45473)
Attached is the data dump from TwinCAT.  In some stretches one can see some ripples before the flow rate
drops to zero.  These small fluctuations might be air bubbles making their way through the system.  The
drop outs occur with enough regularity that we ought to be able to test whether it's the EL3054 analogue
input terminal being intermittent or if it really is a flow rate problem.

    The alternate is that perhaps the connections in the junction box might be loose, although unlikely
I would think.
Images attached to this comment
H1 SQZ (SQZ)
haocun.yu@LIGO.ORG - posted 16:32, Friday 23 November 2018 (45472)
Squeezer Recovery

Squeezer recovery work after pumping down:

A quick cavity scan with green beam, as attached below.

Calculation:

This is pretty much better than before, and consistent with the scan in-air.

 

Images attached to this report
H1 CAL (DetChar)
aaron.viets@LIGO.ORG - posted 15:33, Friday 23 November 2018 (45470)
New GDS filters for LHO with better high-pass filters

I've produced new filters for use in the GDS calibration pipeline with improvements to the high-pass filters. These filters are otherwise the same as those mentioned in LHO aLOG 45428.  The new filters can be found in the calibration SVN at:

aligocalibration/trunk/Runs/PreER13/GDSFilters/H1GDS_1227048227.npz

They were produced from SVN revision 6059 with these parameters files:

The changes made in the high-pass filters were:

The first three of the attached plots show comparisons of the time-domain filters to the frequency-domain models.  The 4th plot shows ASDs produced by GDS using this filter and by CALCS.  The last plot is a transfer function beteen CALCS and GDS.

The primary and redundant GDS calibration pipelines were restated around GPS 1227050381 to pick up these new filters.

Images attached to this report
H1 PSL (PSL)
cheryl.vorvick@LIGO.ORG - posted 15:09, Friday 23 November 2018 (45468)
PSL chiller pictures

Pictures from the PSL chillers: first two are the top chiller "Wallace," last two are from the lower chiller.  Jason was called, Danny and Georgia are here waiting for PeterK, who is on his way in.

Images attached to this report
H1 PSL (PSL)
daniel.brown@LIGO.ORG - posted 15:04, Friday 23 November 2018 - last comment - 15:15, Friday 23 November 2018(45466)
Crystal chiller restart

Jason (remote), Peter (remote), Cheryl, Georgia, Daniel

The PSL switched itself off today around 22:00 UTC. The crystal chiller had run out of water. We topped this back up and got the chiller restarted. However the various flow meters are all reading slightly low now. The power meter flow sensor seems to be glitching a lot. Peter is on his way in to check things out.

Image attached of the status screen when we got in to the diode room.

Images attached to this report
Comments related to this report
georgia.mansell@LIGO.ORG - 15:15, Friday 23 November 2018 (45469)

Attaching a screenshot of the flow meters for the power meter, amplifier, and 70 W amplifier. They're showing similar behaviour to what Jason reported in alog 45334.

There were occasional glitches in the flow meters, a drop when the chillers tripped, when we topped up the chiller and brought it back online around t-1250, the flow levels are lower than they were, and the power meter flow rate is very glitchy.

Images attached to this comment
LHO VE
kyle.ryan@LIGO.ORG - posted 06:51, Friday 23 November 2018 - last comment - 09:43, Saturday 24 November 2018(45464)
Kyle on site making routine checks on equipment

Y-end VEA and CS LVEA

I expect to be here for < 1 hr. and will make a comment to this entry when I leave.

Comments related to this report
kyle.ryan@LIGO.ORG - 07:24, Friday 23 November 2018 (45465)

At some point (later today? tomorrow?) PT110 will change voltage ranges and will then be showing comparatively lower pressure values.  After this occurs it will be helpful to revisit the state of the alarm texting system such that the Vacuum group receive alarm texts should PT100 or PT110 indicated pressures exceed X torr -> where "X" is the preset, traditional threshold pressure value (5 x 10-6 torr?). 

0725 hrs. local -> Leaving site now

david.barker@LIGO.ORG - 09:43, Saturday 24 November 2018 (45475)

The nominal high alarm levels for PT100 (HAM1) and PT110 (HAM6) are 5.0e-05 Torr. Both of these gauges are currently in the 2.0e-06 Torr range. We can either wait until they drop below 5.0e-05 Torr or raise the alarm level to re-engage the cell phone alarms.

LHO VE
chandra.romel@LIGO.ORG - posted 10:49, Thursday 22 November 2018 (45463)
Pressures safe for HV in HAM 1,6

Pressures are below 1x10-5 Torr in both HAM 1 & 6 and safe to turn on high voltage supplies.

H1 SQZ (SQZ)
haocun.yu@LIGO.ORG - posted 21:48, Wednesday 21 November 2018 (45462)
Summary of SQZ Distances and Mode

Made a drawing summary on SQZ distances measured. Will try to make a e-version later.

Can also be found at https://git.ligo.org/haocun.yu/lho_squeezing/wikis/VOPO

Images attached to this report
LHO VE
chandra.romel@LIGO.ORG - posted 18:47, Wednesday 21 November 2018 - last comment - 13:38, Friday 11 January 2019(45460)
HAM 1,6 on turbos and IP2+baffle installed

[Kyle, Gerardo, Chandra]

The day started with pumping HAM6, followed by HAM1 (after some cart controls troubleshooting by Kyle), along with pumping HAM 1,2,5,6 annulus volumes, and the team also managed to remove and replace ion pump #2, and install its chevron baffle.

We pumped on IP2, but its helium background is high, so we left leak detector valved in and plan to leak check on Monday. We also still need to leak check HAMs 1&6 new feedthroughs.

One of us will make a log entry when it is safe to turn high volts ON in HAM6 (and HAM1) for crews coming in over the weekend. PT-110 (on HAM6) and PT-100B (on HAM1) must read below 1x10-5 Torr.

All cleanrooms are OFF and VE decoupled from BSC10 annulus at EY.

Comments related to this report
chandra.romel@LIGO.ORG - 18:47, Wednesday 21 November 2018 (45461)

Excellent work, vacuum team! laugh

stephen.appert@LIGO.ORG - 15:35, Thursday 10 January 2019 (46345)

Did anyone track nipple and baffle serial number information?

gerardo.moreno@LIGO.ORG - 13:38, Friday 11 January 2019 (46371)VE
H1 CDS
patrick.thomas@LIGO.ORG - posted 17:17, Wednesday 21 November 2018 (45459)
Powercycled h1digivideo3 and h1digivideo1


			
			
H1 SUS
thomas.shaffer@LIGO.ORG - posted 16:07, Wednesday 21 November 2018 (45456)
HAM6 SUS Chamber Closeout TFs

I finally got around to processing the data from the TFs that Jeff and I took on Monday (alog45418). OPOS, OMC, OMs, and ZM1 all still look good.

Non-image files attached to this report
H1 AOS
jeffrey.bartlett@LIGO.ORG - posted 16:04, Wednesday 21 November 2018 (45457)
Ops Day Shift Summary
Ops Shift Log: 11/21/2018, Day Shift 16:00 – 00:00 (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:   Happy Thanksgiving
 
Activity Log: Time - UTC (PT)
14:20 (06:20) Peter – Into the PSL enclosure
15:45 (07:45) Karen & Vanessa – Into the LVEA for cleaning
16:00 (08:00) Start of Shift
16:10 (08:10) Ed – Going to HAM1 for electrical work
16:13 (08:13) Hugh – Going to HAM1 for HEPI work
16:39 (08:39) Hugh – Out of the LVEA – HAM1 HEPI is unlocked
16:45 (80:45) Peter – Out of the PSL enclosure
16:57 (08:57) Chandra & Kyle – Leak checking at HAM1
17:01 (09:01) Karen – Finished in the LVEA
17:02 (09:02) Vanessa – Going to End-X for cleaning
17:11 (09:11) Betsy & Daniel – Going into the LVEA
17:25 (09:25) Corey – Connecting HAM1 IO table light pipes
17:26 (09:26) TVo – Going into LVEA to recover CO2 lasers
17:33 (09:33) TVo – Out of the LVEA
17:50 (09:50) Richard – Going to HAM1 for electrical connections
17:56 (09:56) Chris – Taking parts to Kyle for leak checking
17:59 (09:59) TVo & TJ – Going into the LVEA to turn on CO2 lasers
18:00 (10:00) Daniel – Out of the LVEA
18:04 (10:04) Chris – Going to Mid-Y to look for equipment
18:14 (10:14) Corey – Out of the LVEA
18:18 (10:18) Chris – Back from Mid-Y
18:19 (10:19) Gerardo – Going to End-Y to recover vacuum equipment
18:53 (10:53) Gerardo – Back from End-Y
20:28 (12:28) Peter, Ed, & Richard – Going to the LVEA to check status of IFO for laser transition
21:00 (13:00) Peter, Ed, & Richard – Out of the LVEA
23:03 (15:03) Chandra & Kyle – Into the LVEA of IP2 work
00:00 (16:00) End of Shift

 

H1 CDS (VE)
david.barker@LIGO.ORG - posted 15:15, Wednesday 21 November 2018 (45455)
Vacuum Alarms to Cell Phones for HAM1,6 Bypassed Until Monday

Chandra has requested that HAM1 and HAM6 cell phone alarms be bypassed until Monday (email alarms are unaffected).

Bypass will expire:
Mon Nov 26 15:13:11 PST 2018
For channel(s):
    H0:VAC-LX_Y0_PT110_MOD1_PRESS_TORR
    H0:VAC-LY_X0_PT100B_PRESS_TORR

 

H1 IOO (IOO)
cheryl.vorvick@LIGO.ORG - posted 11:17, Wednesday 21 November 2018 - last comment - 14:22, Wednesday 21 November 2018(45440)
IO on PSL for Nov.20

Cheryl, Jason

Images attached to this report
Comments related to this report
cheryl.vorvick@LIGO.ORG - 13:16, Wednesday 21 November 2018 (45451)

plots of data for PMC, ideal, and measured, and beam scan data collected yesterday, as well as distances used for the plots in a matlab .m file, and a huge image (7.5MB).

Images attached to this comment
Non-image files attached to this comment
cheryl.vorvick@LIGO.ORG - 14:11, Wednesday 21 November 2018 (45452)

beam scan data from the bottom periscope is attached, distances are from the PZT, and the lens after the bottom periscope mirror is ~238.5mm from the PZT.  

Non-image files attached to this comment
cheryl.vorvick@LIGO.ORG - 14:22, Wednesday 21 November 2018 (45454)

DUE TO SPACE AND COOLING LINE ISSUES, the original power readings were done with a power meter head that is supposed to be water cooled, but currently isn't.   The readings from yesterday matched very closely the power out of the PMC that was measured with the water cooled beam dump, and were consistent when running the power to max and min at the bottom periscope.  The plan for today was to use the air-cooled power meter head that can go to 50W, that we borrowed from TCS (TVo),  to verify power at the bottom periscope mirror and the PMC.

H1 SUS
thomas.shaffer@LIGO.ORG - posted 18:22, Monday 19 November 2018 - last comment - 16:08, Wednesday 21 November 2018(45418)
HAM6 SUS TFs All Good

J. Kissel, T. Shaffer

All of the suspensions in HAM6 have been given the okay based on the ran transfer functions listed below. OM2 needed a cable to be repositioned by Hugh on the vacuum side of the feedthrough. These measurements still need to be processed in MatLab, but file names for the good measurements are listed below. These are located in the appropriate areas in the sus svn. They are the xml files for now (I incorrectly exported many of them so I will check on that tomorrow):

2018-11-19_2130_H1SUSOMC_M1_WhiteNoise_V_0p01to50Hz.xml
2018-11-19_2130_H1SUSOMC_M1_WhiteNoise_T_0p01to50Hz.xml
2018-11-19_2130_H1SUSOMC_M1_WhiteNoise_L_0p01to50Hz.xml
2018-11-19_2130_H1SUSOMC_M1_WhiteNoise_R_0p01to50Hz.xml
2018-11-19_2130_H1SUSOMC_M1_WhiteNoise_Y_0p01to50Hz.xml
2018-11-19_2130_H1SUSOMC_M1_WhiteNoise_P_0p01to50Hz.xml

2018-11-19_2130_H1SUSOPO_M1_WhiteNoise_Y_0p02to50Hz.xml
2018-11-19_2130_H1SUSOPO_M1_WhiteNoise_V_0p02to50Hz.xml
2018-11-19_2130_H1SUSOPO_M1_WhiteNoise_T_0p02to50Hz.xml
2018-11-19_2130_H1SUSOPO_M1_WhiteNoise_L_0p02to50Hz.xml
2018-11-19_2130_H1SUSOPO_M1_WhiteNoise_P_0p02to50Hz.xml
2018-11-19_2130_H1SUSOPO_M1_WhiteNoise_R_0p02to50Hz.xml

2018-11-19_2117_H1SUSOM1_M1_WhiteNoise_L_0p02to50Hz.xml
2018-11-19_2117_H1SUSOM1_M1_WhiteNoise_P_0p02to50Hz.xml
2018-11-19_2117_H1SUSOM1_M1_WhiteNoise_Y_0p02to50Hz.xml

2018-11-20_0025_H1SUSOM2_M1_WhiteNoise_L_0p02to50Hz.xml
2018-11-20_0025_H1SUSOM2_M1_WhiteNoise_P_0p02to50Hz.xml
2018-11-20_0025_H1SUSOM2_M1_WhiteNoise_Y_0p02to50Hz.xml

2018-11-19_2149_H1SUSOM3_M1_WhiteNoise_L_0p02to50Hz.xml
2018-11-19_2149_H1SUSOM3_M1_WhiteNoise_Y_0p02to50Hz.xml
2018-11-19_2149_H1SUSOM3_M1_WhiteNoise_P_0p02to50Hz.xml

2018-11-12_1849_H1SUSZM1_M1_WhiteNoise_L_0p02to50Hz.xml
2018-11-12_1849_H1SUSZM1_M1_WhiteNoise_Y_0p02to50Hz.xml

 

Comments related to this report
thomas.shaffer@LIGO.ORG - 16:08, Wednesday 21 November 2018 (45458)

See alog45456 for the processed results.

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