Displaying reports 45821-45840 of 83686.Go to page Start 2288 2289 2290 2291 2292 2293 2294 2295 2296 End
Reports until 12:06, Tuesday 10 October 2017
H1 SUS
angus.bell@LIGO.ORG - posted 12:06, Tuesday 10 October 2017 (38965)
Monolithic ITMx assembly welding
Travis, Jason & Angus.	Oct 5th, 6th & 9th

The new ITMx has been welded and the violin modes of the fibres measured in air with the PUM clamped. The welding went quite smoothly apart from a couple of points. 
1)	The epoxy around the sapphire prism on one side of the PUM (+Y side) has charred due to heat from the welding of that fibre.
2)	The lengths of the horns on the PUM after fibre removal were not all exactly 6.0 mm above the ear, and this was not compensated for exactly with each fibre. The consequence is that the break-off values for one of the fibres (+X-Y) will be higher at the PUM and a bit lower at the ITM
The following fibres were used and the violin harmonics recorded

Posn	S/N		fund	2nd	3rd	4th	5th	(predicted in-vac)
+X+Y	S1400158 	502.45	994.8	1463.8	(1930)	[2390]	503.0
-X+Y	S1400137	503.96	997.85	1468.3	1931.6	(2391)	504.0
-X-Y    S1400164	504.71	1001.6	1472.4	1940.3	2408.3	504.6
+X-Y	S1400154	504.45	1002.6	1466.6	1936.4	2390.0	505.4

Accuracy is about +/- 0.05 for the fundamental, +/- 0.2 for the 2nd harmonic and the higher harmonics are generally +/- 0.5 or better, except for the ones in brackets which are worse. The round brackets are +/-1 and the square is +/-10 Hz (yes ten!).
It can be seen that the harmonics “cross” and that without this measurement it would be harder to determine which harmonic belongs to which fibre.
The pitch prediction from the fibre profiles was 0.1 mrad up (wrt PUM), the actual pitch is 0.3 mrad up. The roll and separation are as good as, or better than, the previous ITMx assembly. The yaw and pendulum frequencies were measured with +/- 0.005 Hz accuracy to 0.650 and 1.095 Hz respectively.
Attached are typical (linear) plots of the modes and a zip file of the original data files and excel files. Plus pics of the welds.
Fibre guards are on.
Images attached to this report
Non-image files attached to this report
H1 ISC
betsy.weaver@LIGO.ORG - posted 10:56, Tuesday 10 October 2017 (38968)
HAM5 OFI Actuation - cables and AOSEMs

In anticipation of attaching AOSEMs to the OFI for HAM5, I laid out a string of the appropriate cables and AOSEMs next to the chamber on a staging table.  I've fastened to the table the clean-to-dirty ribbon-feedthru-simulator-cable to the table and Fil has run a grey temp out of vac cable from it to the sat amp located on the other side of the chamber.  So, the OFI guys can test fit and test the new AOSEMs and their brackets when ever they are ready.

 

The cables and AOSEMs are:

D1000234-88"  S/N 932

D1000225-230"  S/N S1104240

D0901065  S/N  525, 559, 511

H1 PSL
edmond.merilh@LIGO.ORG - posted 10:35, Tuesday 10 October 2017 - last comment - 10:39, Tuesday 10 October 2017(38966)
PSL Noise Eater not Resetting

The Noise eater has tripped and is currently NOT resettable. Jason and Peter are aware of this and are investigating it. An FRS ticket has been filed.

Comments related to this report
edmond.merilh@LIGO.ORG - 10:39, Tuesday 10 October 2017 (38967)

Link to FRS ticket.

H1 PSL
jason.oberling@LIGO.ORG - posted 09:35, Tuesday 10 October 2017 (38963)
PSL Weekly FAMIS Tasks (FAMIS 3671 & 8443)

This morning I completed the weekly PSL FAMIS tasks.

HPO Pump Diode Current Adjust (FAMIS 8443)

With the ISS OFF, I adjusted the operating currents of the HPO DBs, changes summarized in the below table.  A screenshot of the PSL Beckhoff main screen is attached for future reference.

  Operating Current (A)
Old New
DB1 50.5 50.7
DB2 53.0 53.1
DB3 53.0 53.1
DB4 53.0 53.1

I did not adjust the DB operating temperatures.  The HPO is now outputting 154.4 W and the ISS is back ON.  This completes FAMIS 8443.

PSL Power Watchdog Reset (FAMIS 3671)

I reset both PSL power watchdogs at 16:19 UTC (9:19 PDT).  This completes FAMIS 3671.

Images attached to this report
H1 CDS (ISC, SEI, SQZ)
filiberto.clara@LIGO.ORG - posted 09:28, Tuesday 10 October 2017 (38964)
DC Power Distribution for SQZ Install

Yesterday we tied in ±18V to SUS-R3 and SUS-R4. We now have our standard 8 awg shielded cable running from the CER mezzanine down to the LVEA racks. The following electronics were moved to the new ±18V line: Op Lever whitening chassis, CPS Timing Fanout, and the SAT Amp units. Some of the "temporary" cabling used to previously power these electronics will be removed.

Both TCS LVEA racks are sharing their own dedicated power supplies for ±18V and ±24V. One thing to note is that the CPS Timing Fanout in TCS-R2 (next to BSC1) is being powered by TCS rack power.

The new SQZ-R1 rack is now powered by its own dedicated ±18V power supplies. We used the the existing ±24V from ISC-R3/R5 since the current draw is minimal.

LHO VE
kyle.ryan@LIGO.ORG - posted 17:59, Monday 09 October 2017 (38959)
Vacuum Bake Oven C (a.k.a. "VBOC") is out of service until further notice
The hex nut integral to the actuation lead screw on the 1.5" isolation valve separating VBOC's RGA from the oven chamber physically broke off! -> Venting the RGA was required to replace this valve.  As such, VBOC will be out-of-service for a week or more while the RGA volume bakes-out at high temperature etc...  
Non-image files attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 17:52, Monday 09 October 2017 - last comment - 08:32, Tuesday 10 October 2017(38958)
Attempted to adjust "ATM" calibration on newly installed PT120A
Kyle R., Arnab D., Rakesh K. 

Today we adjusted the "ATM" potentiometer on the new parani gauge (local electronics unit) but could only achieve a minimum value of 906 torr indication on CDS.  This is too high.  The actual pressure under these conditions is closer to 760 - 790 torr -> The measured voltage supplied to the gauge electronics is 24.5 VDC and the output signal from the sensor electronics, 5.6 VDC, which is consistent with the CDS-converted value of 906 torr.  Any voltage drops across signal wiring connections between the gauge and the CDS rack should result in a CDS value which would be biased to less than the actual value, not more than the actual value.  

We will continue troubleshooting at the next opportunity.  

Comments related to this report
john.worden@LIGO.ORG - 08:32, Tuesday 10 October 2017 (38961)

I assume you checked - Orientation of the gauge is important since it depends on convection at these pressures. 

H1 TCS
thomas.shaffer@LIGO.ORG - posted 17:12, Monday 09 October 2017 - last comment - 17:23, Tuesday 17 October 2017(38956)
Installed SR3 RoC Heater

Betsy, Hugh, TJ

Last week Betsy put the heater on the table and today Hugh checked it's vertical center with an auto-level. Some washers were added to get it as close to center as possible, which ended up around 0.4mm high. Betsy and I then had to wiggle the assembly into place, and rotate the entire gold ceramic holder to allow the screws on the outside to clear the OSEM brackets. The heater is currently sitting ~6mm away from the back of the SR3 optic and it is plugged into the feed through.

Picture attached.

Images attached to this report
Comments related to this report
betsy.weaver@LIGO.ORG - 17:24, Monday 09 October 2017 (38957)

Here are a few more pics.  As TJ notes, the ROC front face is 5-6mm from the SR3 AR surface.  It is locked down in this location. 

 

Note, we followed a few hints from LLO's install:

https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=25831

 

Continuity checks at the feedthru still need to be made.  Will solicit EE for their help.

Images attached to this comment
filiberto.clara@LIGO.ORG - 12:42, Tuesday 10 October 2017 (38969)

Initial continuity test failed. Found issues with in-vacuum cable, power pins not pushed in completely. Pins were pushed in until a locking click was heard.

Reading are:
Larger Outer Pins, Heater: 66.9Ω
Inner pair (left most looking at connector from air side), thermacouple: 105Ω

hugh.radkins@LIGO.ORG - 15:24, Tuesday 10 October 2017 (38974)

Found center of SR3(-X Scribe) to be 230.2mm above optical table.  By siting the top and bottom of RoC Heater, found center to be at 231.4mm. Removed available shim to put center of RoC Heater at 229.6 for 230.2-229.6=0.6mm below perfect.

thomas.shaffer@LIGO.ORG - 08:27, Wednesday 11 October 2017 (38981)

Hugh's comment reminded me that to get the heater to fit, Betsy and I added a 1mm washer to raise the height of the assembly. In total we have 4mm of washers (2x1.5mm & 1x1mm).

stephen.appert@LIGO.ORG - 17:23, Tuesday 17 October 2017 (39058)TCS
I conducted measurement of quantity 6 of [D1600104 SR3 ROC Actuator, Ceramic Heater Assy] at CIT on 4 March 2016. Dirty state before baking.
The serial number of the heater assy installed in LHO HAM5 is S1600180 - see https://ics-redux.ligo-la.caltech.edu/JIRA/browse/ASSY-D1500258-002
S1600180 Resistance = 66.8 Ohms on 4 March 2016.
There is good agreement between the as-installed and pre-bake measurements.
H1 SYS
thomas.shaffer@LIGO.ORG - posted 16:55, Monday 09 October 2017 (38955)
HAM5 Below Table Baffles Rotated

With new redlines on the HAM5/2 baffles I rotated our below table baffles (beard baffles) that Jim and I had already installed. LLO did this to help cover up more of the exposed metal on the table (see <a href="https://alog.ligo-la.caltech.edu/aLOG/index.php?callRep=36113">LLOalog36113</a>), so while I was already in HAM5 I did some 180's.

No picture yet, I'm hoping to get some when we can look from HAM4.

H1 General
thomas.shaffer@LIGO.ORG - posted 16:45, Monday 09 October 2017 (38954)
Attached HAM Install Arm on HAM5

This morning Mark, Tyler, Bubba, and I attached the install arm on to the West side of the North door on HAM5. We couldn't find the tub of bolts dedicated to this assembly, but found some others nearby (which included some of the door bolts, that we will need to remember to put back when we are finished). The arm is currently only held on with 3 of the 4 bolts that were previously used with this arm. HEPI blocked access from the front to the lower right thru hole, and there was not enough clearance in the back. Perhaps this arm hasn't been used wiht the new style HEPI's yet? Bubba doesn't think the missing bolt will cause any problems and a possible fix with a shorter piece of all-thread is in the works.

Picture attached of the arm installed but all covered up. (Forgot to take pictures until we were walking away.)

Images attached to this report
H1 IOO
edmond.merilh@LIGO.ORG - posted 16:11, Monday 09 October 2017 (38953)
I/O work in HAM2

Cheryl V., Ed M.

This afternoon we installed an access platform into HAM2 on the SW corner of the ISI table for accessing IM3.

Images attached to this report
H1 General
corey.gray@LIGO.ORG - posted 16:00, Monday 09 October 2017 (38930)
Operator DAY Shift Summary

Day's Log Of Activities

H1 CDS
david.barker@LIGO.ORG - posted 15:30, Monday 09 October 2017 - last comment - 15:31, Monday 09 October 2017(38950)
SITEMAP changes

Jeff, Sheila, Dave:

to show off my recently acquired skills in drawing ellipses using gimp, the attached plot shows the three main changes made to the LHO SITEMAP as part of SQZ install.

1. PEM has been reduced from two to one button. To permit this, I have replaced the links to building detail screens with a launcher screen.

2. OPS and O1 (sic) screens have been merged to the OPS button

3. new SQZ button added.

Images attached to this report
Comments related to this report
david.barker@LIGO.ORG - 15:31, Monday 09 October 2017 (38951)

here is a wiki page to show how ellipses and circles can be drawn:

https://cdswiki.ligo-wa.caltech.edu/wiki/GIMPDrawOvalsAndCircles

H1 PEM
jeffrey.bartlett@LIGO.ORG - posted 15:28, Monday 09 October 2017 (38949)
Dust Monitor Quarterly Testing (FAMIS #7316)
  Checked all monitors except PSL (will do on Wed when in for other work), and #2 and #10 in the LVEA. These are in running cleanrooms with vent work underway. Will check these early in the morning before the work day starts. 

   The rest of the monitors are working within specifications.   
H1 SUS
travis.sadecki@LIGO.ORG - posted 17:42, Friday 06 October 2017 - last comment - 16:05, Monday 09 October 2017(38924)
ITMx fiber welding complete

A. Bell, J. Oberling, T. Sadecki

ITMx has been successfully hung as a newly welded monolithic.  I'll leave it to Jason to post the actual numbers, but the PUM to TM differential pitch better than the old version of ITMx.  Now to put it back together in chamber next week.

Comments related to this report
jason.oberling@LIGO.ORG - 16:05, Monday 09 October 2017 (38952)

Final alignment numbers for the new monolithic are below.  All measurements were done with the ITMx suspended, PUM and UIM locked.  All directions assume the reader is looking in the +X direction (i.e. at the ITMx AR surface); it should be noted for future reference (if comparing to the numbers in the alignment notebook) that this is opposite the convention used in the alignment notebook, which is set relative to the IAS equipment used in the alignment and looks in the -X direction (at the ITMx HR surface).

  • Roll
    • PUM: 0.15 mm CCW
    • ITMx: 0.20 mm CCW
  • Pitch
    • PUM: 1.51 mrad down
    • ITMx: 1.20 mrad down
    • Differential: 310 µrad up
  • Fiber Stretch
    • Left: 5.7 mm
    • Right: 5.8 mm
  • PUM/ITMx Center of Mass Separation
    • Left: 601.5 mm
    • Right: 601.4 mm

The serial numbers of the fibers used and their locations in the monolithic are as follows:

  • +X/+Y
    • SN S1400158
  • -X/+Y
    • SN S1400137
  • -X/-Y
    • SN S1400164
  • +X/-Y
    • SN S1400154
H1 SUS (SUS)
borja.sorazu@LIGO.ORG - posted 12:49, Tuesday 22 August 2017 - last comment - 07:00, Tuesday 10 October 2017(38309)
Violin mode frequency changes from in-air measurements to in-vacuum complete results for LHO and LLO

I have compiled the results of in-air measurements during installation and in-vacuum measurements from the alogs; 14231 LLO (including corrections mentioned in alogs 21652 and 27901) and 17610 at LHO (including corrections mentioned on the comments).

In the case when a frequency split is shown on in-vacuum measurements we have taken the average of both frequencies. I have grouped these numbers per front and back fibres, then per test mass and then per detector, finally I obtained the difference as (in-vacuum – in-air) including the sign:

We notice that in most cases the frequency difference is always positive, so frequency increases when moving the suspension to in-vacuum.

The increase in frequency is always a few hundred mHz (mean of 0.3Hz and median of 0.4Hz), with a clear outlier on LLO_ITMY_FL (which as explained here seems to be involved with uncertainty in the identification).

There is not clear difference in frequency variation between front and back fibres (especially no sign difference) which would indicate pitch effect.

However, notice that as per the Technical document T1700399 the expected increase in frequency due to buoyancy is of 0.14Hz, and the variation in frequency due to pitch angles of 2mHz is of 0.33Hz (although that would be an opposite sign change between front and back fibres). Therefore while the observed changes cannot be explained through pitch and buoyancy alone, they are of the same order.

Images attached to this report
Non-image files attached to this report
Comments related to this report
borja.sorazu@LIGO.ORG - 05:41, Wednesday 23 August 2017 (38323)

Further discussions on the results presented here has led to realize that the in-air measurements of the violin modes fundamental frequencies have a potential error of about 0.25Hz (as an example here are measurement results for LHO ITMX suspension). In base of this and to better understand the actual differences between in-air and in-vacuum measurements, now that we have very accurate measurements in-vacuum, it would be informative to measure in-air values once the suspensions are taken out. 

The in-air measurements have so far been done by acoustically driving the violin mode resonances. During this measurements the frequency of the driving acoustic signal is changed as a sweep sine. Because the in-air Q of the violin modes is considerably less than the in-vacuum values of 1 billion, if the sweep sine drive is not done with suitable slow pace then the observed a violin mode excitation at a frequency on the sweep sine which actually correspond to a previous frequency of the sweep but took some time to  ring up. Under this assumption, if the sweep sines were driven down (from high frequencies to lower frequencies) then there would be a consistent error on the measured in-air frequencies with values being lower than in-vacuum ones.

A way to improve the acoustic excitation could be by building a tower of speakers so that they could inject more energy into the violin modes of the fibres. Also be sure to drive the sweep sine at enough low pace or inject random noise excitation instead. Finally a lot of information could be gained by in-air measurements of higher order harmonics, this would help on characterization and understanding of higher order inharmonicity as well as higher order mode identification. 

 

borja.sorazu@LIGO.ORG - 10:46, Tuesday 29 August 2017 (38415)

In order to proceed with the in-air measurements of the violin mode and its harmonics during the installation of the suspensions in the near future (as well as measuring the already install suspensions once removed), we have built in Glasgow a line array of 24 speakers of 60 cm length to match the length of the fused silica fibres. Its lightweight and compact design make it suitable to locate it parallel and in close proximity to the fibre that wants to be excited.

This line array produces considerable sound from 300Hz and well above several kHz making it suitable to excite the fundamental mode and up to the 6th harmonic and beyond.

A more complete description can be found on the technical document T1700414T1700414.

Images attached to this comment
borja.sorazu@LIGO.ORG - 11:20, Tuesday 29 August 2017 (38416)

It is relevant to this alog to remember that while preliminary FEA modelling of the actual fibre profiles measured during installation of the LHO ITMX suspension (end of March 2014), has been used to predict in general terms the observed departure of the frequencies of the violin mode harmonics from whole multiples of the fundamental (“inharmonicity”):

 

However this preliminary results show that this prediction is not yet accurate to the few Hz level required for identification:

 

Images attached to this comment
borja.sorazu@LIGO.ORG - 07:00, Tuesday 10 October 2017 (38960)

In order to complete the list of possible causes for the different inair and invacuum measured violin mode frequencies, I add next the contributions suggested recently by Norna, Dennis and Jon Feicht:

Violin modes frequency variations due to air damping

Air damping lowers the in-air measured violin mode frequency by a value inverse proportional to the violin mode’s Q-factor. Such that the maximum frequency for a damped oscillator (fm) is related to the undamped maximum frequency (f0) by:

fm f0 ∙ sqrt[1-1/(2∙Q2)]

A quick look at recent in-air measurement on the LHO alog 38743 suggest a Q of at least 100 in-air at the ~ 500 Hz fundamental mode. This would give a in-air measured frequency value of the fundamental of 0.012Hz lower than in-vacuum.

Violin modes frequency variations due to mass/length of the fibre decreasing as the water desorbs from the silica fibre in vacuum

The mass loading on the fibre, due to water adsorption in-air, should in principle cause the in-air measurement of the violin mode fundamental frequency to be lower than in-vacuum, as once much of the water is pumped off the fibre in vacuum the frequency should increase. Dennis Coyne calculated that about ~3500 monolayers of water (each 2.5 angstroms thick) would be necessary to cause a 1 Hz shift at 500 Hz, due to mass loading alone. It is commonly asserted in vacuum literature that stainless-steel surfaces of a vacuum system exposed to air can start with "hundreds of monolayers of water".

However fused silica is hydrophilic and the interaction of silica surfaces and water is complex; Surfaces of silica under water can swell and form layers of silica gel1. The modification of the fused silica surface by the chemisorption and physisorption of water may even lead to a reduction in the elastic modulus of the fused silica in the outer layers.

References

[1] V.V. Yaminsky, et. al., "Interaction between Surfaces of Fused Silica in Water", Langmuir 1998, 14, 3223-3235.

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