Displaying reports 67701-67720 of 77143.Go to page Start 3382 3383 3384 3385 3386 3387 3388 3389 3390 End
Reports until 00:09, Saturday 01 February 2014
H1 AOS
stefan.ballmer@LIGO.ORG - posted 00:09, Saturday 01 February 2014 (9735)
yarm IAL: pit and yaw was flipped
We found that the pitch and yaw outputs for the y-arm initial alignment were flipped. Fixed the model and recompiled.

h1asc.mdl: SVN revision 7011.


H1 SUS
arnaud.pele@LIGO.ORG - posted 21:07, Friday 31 January 2014 (9733)
SUS Guardian updates

Following updates of guardian at LLO from the past few weeks, I started updating some sus guardian

New feature for saving alignment :

It is now possible to save the aligned as well as the misaligned position of the suspensions for every optic. This can be done through the IFO_ALIGN medm screen via the Save Alignment menu (cf IFO_ALIGN.png) or with the pyhton script align_save_burt -a -m living in /opt/rtcds/userapps/release/sus/common/scripts/

For more details see llo alog 10436 and 10466

Restoring the saved alignments :

This is done through Guardian by switching between different states of the suspension. Guardian medm screens can be accessed via the ! G buttons in the IFO_ALIGN medm screen (cf IFO_ALIGN.png).

For now, only PRM PR3 and MC2 are running under the guardian and can be restored this way. For the other suspensions, it will need to be done manually (until a guardian process is created).

When the guardian medm screen is open, it is straightforward to switch between aligned misaligned damped or safe via the "REQUEST" menu (cf GUARD_PRM.png)


IFO_ALIGN.adl was updated from livingston but I had to make some modifications to get the links functioning. The new adl file was commited under the svn

1) As Kiwamu pointed out to me, the arguments under the Save Alignment link were in the wrong order (e.g. "align_save_burt MC1 -m" instead of "align_save_burt  -m MC1"), so I modified it for MC1/MC2/MC3/PRM/PR2/PR3/SRM/SR2/SR3/BS/ETMX/ETMY/ITMX/ITMY/TMSX/TMSY

2) Also, the command to create a guardian medm screen (guardmedm) had the full llo path defined (/ligo/apps/ubuntu12/guardian/bin/guardmedm) which doesn't exist here so I changed it to guardmedm without the path. That should also work at llo.

Images attached to this report
H1 SUS (ISC, SEI)
jeffrey.kissel@LIGO.ORG - posted 19:21, Friday 31 January 2014 (9734)
H1 SUS ETMX Trial L&P Damping Filters
J. Kissel

Though we're confident that the only way to improve the X-arm Test Mass angular performance is to improve the BSC-ISI performance between 0.3 and 0.7 [Hz], I tried tweaking the Level 2.1 Damping Loop design to see if I could do any better, by increasing the Q of the boost filters on the L and P degrees of freedom. Further, I moved the frequency of the P boost down from 0.56 [Hz] to 0.51 [Hz] to account for the difference between the modelled and measured frequency of this mode. Regrettably, I could not improve the strength (at the resonances) of the boosts much more than 5 to 10 [dB] without destroying the the stability of the L & P loops -- I'd already pushed the phase and gain margins of the *lower* unity gain frequency pretty far. As such, the improvement was only in the sharp frequency regions over which I'd focused the boost, but little-to-no change in the RMS. 

We'll continue to work on improving the performance of the ISIs. 

For posterity, I post all of the design information and performance comparisons. The good news is, that my MIMO model of the QUADs can now accurately predict the optic angular motion -- especially Pitch -- at all frequencies where not limited by its sensor noise. Check out the pg 2 of the third attachment for proof!

Details:
---------
allquads_2014-01-31_AllGoodFibers_P.pdf 
     -- Shows a collection of transfer functions of all monolithic suspensions. It shows that compared against the modeled first, top mass, P2P mode at 0.56 [Hz], all the measurements show that this mode is at 0.51 pm 0.01 [Hz]. This is what motivated me to focus the sharp P boost at a lower frequency.
2014-01-31_H1SUSETMX_M0_DAMP_Filters.pdf
     -- Bode plots comparing the 2013-06-14, Level 2.1 Filters against the new 2014-01-31 Sharp Boost filters. 
dampingfilters_QUAD_2013-06-14_Level2p1_2014-01-30_H1ISIETMX_Seismic_SelectPlots.pdf
     -- Using current seismic data input, this is a few select plots from the loop design script for the 2013-06-14 Level 2.1 filters. As mentioned above, it predicts the measured P motion extremely well below ~1.5 [Hz]. Interestingly, the Y prediction is not perfect, but I suspect that below 0.5 [Hz] the signal is dominated by L and P motion of test mass, confused as Y. Especially because the two extra modes that appear at ... you guessed it 0.44 and 0.56 [Hz].
dampingfilters_QUAD_2014-01-30_Level2p1_RealSeismic_SelectPlots.pdf
     -- Selected performance plots with the new sharper boost. Bare in mind that I've used the *model* for the predicted transfer functions, which don't get the first P mode at the right frequency. That's why things appear like they will be unstable, and all sort of gain peaky near the lower unity gain frequency. 
dampingfilters_comparison_2013-06-14vs2014-01-31.pdf
     -- A comparison between the two designs. 
2014-01-31_H1SUSETMX_Level2p1vsSharpBoost_Performance_ASDs.pdf
     -- A comparison of the optical lever performance between the two configurations. Of course, the spectra were taken at different times of day, so above ~0.6 [Hz] the input motion is a little different, but below 0.6 [Hz] the motion is the *same*,  and one can see the expected change in shape of the hump, but no change in RMS. Oh well.


Design Scripts:
SusSVN/sus/trunk/QUAD/Common/FilterDesign/Scripts/
compare_quad_dampfilter_design_20140131_NormalvsSharp.m
design_damping_QUAD_20130614.m
design_damping_QUAD_20140123.m
plotquaddampingcontroldesign.m

Filters and Model saved to:
SusSVN/sus/trunk/QUAD/Common/FilterDesign/MatFiles/
dampingfilters_QUAD_2013-06-14.mat
dampingfilters_QUAD_2014-01-30.mat
dampingfilters_QUAD_2013-06-14_Level2p1_2014-01-30_H1ISIETMX_Seismic_model.mat
dampingfilters_QUAD_2013-06-14_Level2p1_RealSeismic_model.mat
dampingfilters_QUAD_2014-01-30_Level2p1_RealSeismic_model.mat
Non-image files attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 17:39, Friday 31 January 2014 (9732)
MSR doors left open for the weekend, fan not on
Due to the non-zero chance of a second cooling unit failing, we are leaving the doors between the MSR and the hallway open for the weekend. We should keep the control room doors closed to reduce the noise.
H1 IOO
paul.fulda@LIGO.ORG - posted 16:40, Friday 31 January 2014 - last comment - 17:34, Monday 03 February 2014(9716)
MC2trans and IM4trans calibration

I made a calibration of the IM4trans and MC2trans SUM channels into uW.

The conversion from W incident on the PDs to counts registered on IMC-IM4_TRANS_SUM_OUTMON is as follows:

[counts/W] = responsivity [0.16 A/W] x transimpedance gain [1000V/A] x differential to single input gain [2V/V] x whitening gain [36dB=63.1 V/V] x ADC gain [1.6384x10^3 cts/V].

This is actually the same for both MC2trans QPD and IM4trans QPDs: 2.087x10^9 [counts/W]

I used this calibration factor to calculate the power on IM4trans and MC2trans currently:

IM4trans counts ~= 57890 counts, which converts to 1.75mW. Comparing this with the expected power on IM4trans:

8.73W into IMC * 0.85 IO throughput * 2400ppm IM4 transmission * 0.1 transmission of BS between IM4 and IM4trans QPD = 1.78mW

MC2trans counts ~= 2.17x10^4 counts, which converts to 655uW. Comparing this with the expected power on MC2trans:

8.73W into IMC * (IMC gain = IMC Finesse/pi = 166 ) * 5.1x10^-6 MC2 transmission * 0.1 transmission of BS between MC2 and MC2trans QPD = 740uW.

Both these estimates for the power incident on each PD agree pretty well yes so I'll go ahead and add a new filter called "cts2uW" in the SUM_OUTMON paths to give the outputs in uW incident on the PDs.

Comments related to this report
paul.fulda@LIGO.ORG - 14:30, Friday 31 January 2014 (9725)

The fact that the SUM output is used to normalize PITCH and YAW signals meant that adding the filter in front of just the SUM channel increased the gains on PITCH and YAW significantly, affecting the IMC ASC loops. I have now put the cts2uW filters in the input filter banks for each segment of both QPDs. It works fine now, so the MC2trans SUM and IM4trans SUM are calibrated in uW. If anyone changes the whitening gains on these PDs, please be sure to adjust the calibration factor accordingly. I may look into automatically factoring the whitening gain into the calibration to avoid this issue in future.

paul.fulda@LIGO.ORG - 17:34, Monday 03 February 2014 (9772)

Just to be clear, the calibration from counts to uW for both IM4trans and MC2trans was 0.032 uW per count. The number 2.087x10^9 [counts/W] was in error: this number should have been 3.3080x10^7 [counts/W]. Although the number in the alog post was in error, the correct number was used in the filters which were applied.

H1 ISC
sheila.dwyer@LIGO.ORG - posted 16:05, Friday 31 January 2014 (9731)
X arm IR transmission

Aaron, Luis, Fil, Sheila

There is now a camera installed on the IR trans path at the x end.  The image is of the IR path incident on a baffle (a scratched up, old piece of aluminum painted black, to be more acurate.)  There is about 30uW of green power coming out of the chamber into the IR path, you can see a square of 4 green ghost beams on the camera image, and ocassional flashes of the IR beam.  Adding a dichroic to the path might make it a little more clear what is going on here.  

We sent the signal to the red cable behind the monitors in the front row of the control room.  I unplugged the image of the BS from the top monitor, and replaced it with this camera.  IF anyone want to see the BS camera, plug the blue cable back in.

H1 General
andres.ramirez@LIGO.ORG - posted 16:00, Friday 31 January 2014 (9730)
Ops Shift Summary
8:53-9:43 Checking SUS cables on HAM 4 (LVEA) - Filiberto
9:07-10:10 Moving, cleaning, and organizing elements for SR2 installation (HAM4 LVEA) Jeff.B/Jodi
9:40-10:40 Going into LVEA to check a dust monitor which has lost     communication Patrick
9:47-11:20 Heading to LVEA West Bay (cleaning/organizing ACB components) – Mitchell
10:15-12:15 Stiffener rings and o ring protectors installation on HAM4 – Apollo
10:33-11:53 Going to HAM 4 to install SR2 Pre-installation Plate(Cookie cutter) – Jeff B.
12:40-12:46 DAQ restart and new h1asc model – Dave
12:54-13:17 Going to BSC2 to work on HEPI – Hugh
13:30-15:11 Heading to LVEA West Bay (cleaning/organizing ACB components) – Mitchell
13:44-15:12 Going to HAM 4 to install SR2 Pre-installation Plate(Cookie cutter) – Jeff B.
14:22-15:05 Heading into the LVEA to search for cables - Corey
H1 SEI (CDS, FMP, PEM, SEI)
jeffrey.kissel@LIGO.ORG - posted 15:32, Friday 31 January 2014 (9727)
H1 STS2 Assessment -- Vault STS-2 Needs Repair
J. Kissel, R. Mittleman, R. McCarthy

Looking for functional STS-2s to use for BSC-ISI sensor correction at ETMX, one suggestion that came up was the Vault STS-2. However, Rich immediately reminded us that it's over 10 years old and hasn't received any TLC in a while, so it's most likely functioning poorly at low-frequency and will need to be shipped back to Quanterra for maintenance. To confirm, I've measured its low-frequency coherence with the functional corner station STS-2s. Ideally, we'd go grab the VAULT STS2, and huddle test it against one of the LVEA STSs, but ... it's cold, and for the frequencies we're concerned about it shouldn't matter.

In summary -- yes: the VAULT STS-2 is poorly coherent with any of the corner. If functional, we'd expect to see coherence down to 50-60 mHz in the Z directions. Richard suggest we'll grab in the Spring.

Details:
--------
Serial Number Layout:
HAM2 -- SN 89922
HAM5 -- SN 100145F
ITMY -- SN 89941
VAULT -- (Known, but not yet by me)
(ETMY -- SN 89938)

Calibration Details:
HAM2, HAM5, and ITMY -- 1e-9 [(m/s) / (nm/s)]. These aLIGO GND STS2s, with channels H1:ISI-GND_STS_${CHAMBER}_${DOF}_DQ, are already calibrated in the front end to (nm/s), so all I have to do was convert to (m/s).
VAULT -- 3.052e-7 [(m/s) / ct]. Although pem.ligo.org suggests that the calibration should be 0.0076e-6 [(m/s) / ct], it did not match any of the corner station STS-2s at the microseism, where the motion should be identical. So, I just scaled the VAULT to match. Further, the channels are different from pem.ligo.org, they're now H1:PEM-VAULT_SEIS_1030X195Y_STS2_${DOF}_DQ
Non-image files attached to this report
H1 SUS
betsy.weaver@LIGO.ORG - posted 15:22, Friday 31 January 2014 (9728)
ETMy suspension alignment continues

At COB yesterday we had roughed in the longitudinal, lateral, pitch and yaw positions of the ETMy test mass within the suspension structure.  We had to push the structure ~3mm to achieve this.  Today, while bringing the height into alignment, we threw the yaw out of tolerance (because the height mechanics are grossely coupled to yaw).  After finally getting the height into tolerance (iterate: go up, whoops too far, go down, no up, now down!) we re-tuned yaw to within ~300uRad.  We still need to work on yaw more but our backs were literally breaking getting to these adjustments (see pic) so we opted to stop there and start fresh on Monday.  We now have the long, lat, and height within spec with the pitch and yaw almost in spec for the main chain.  We also adjusted some bad roll on the reaction ERM which for some reason induced pitch.  We'll attack that chain Monday.  IAS plans to bring the gap measuring aparatus out on Monday which we'll need to use soon.

Images attached to this report
H1 CDS
patrick.thomas@LIGO.ORG - posted 14:34, Friday 31 January 2014 - last comment - 14:37, Friday 31 January 2014(9724)
updated conlog channel list
It is now using the file /ligo/lho/data/conlog/h1/pvlist_1391196748 (attached). There are 99,264 channels in this list. 5,755 are currently unmonitored.
Non-image files attached to this report
Comments related to this report
patrick.thomas@LIGO.ORG - 14:37, Friday 31 January 2014 (9726)
There are 62,966,023 rows in the database.
H1 SUS
andres.ramirez@LIGO.ORG - posted 13:46, Friday 31 January 2014 - last comment - 15:22, Friday 31 January 2014(9722)
Going to HAM 4 to install SR2 Pre-installation Plate(Cookie cutter) – Jeff B.


			
			
Comments related to this report
andres.ramirez@LIGO.ORG - 15:22, Friday 31 January 2014 (9729)
Suspension has been stopped and Pre-installation plate installed. Work completed!
H1 SEI
andres.ramirez@LIGO.ORG - posted 12:57, Friday 31 January 2014 (9720)
Going to BSC2 to work on HEPI (LVEA) - Hugh
Work completed
H1 DAQ (CDS, ISC)
david.barker@LIGO.ORG - posted 12:46, Friday 31 January 2014 (9718)
DAQ restart and new h1asc model
We fixed Daniel's channel naming problem with the ALS addition to the ASC, actually the problem went away. So I restarted the new h1asc model at 12:41 and restarted the DAQ at 12:44 to install the new model and DAQ channels associated with it.
H1 SEI
hugh.radkins@LIGO.ORG - posted 11:28, Friday 31 January 2014 - last comment - 13:37, Friday 31 January 2014(9714)
WBSC2 HEPI V2 Leak at Parker Valve

Noticed some fluid in the bottom of the SW SEI Pier at the BS.  Cleaned up the mess in the Pier yesterday and this morning found fresh fluid.  Climbed up to Housing and found the Vertical Actuator Fluid Catch overflowing.  I can see drips coming off the Parker Valve.  Can't tell if it is coming out of the Valve itself or just the Valve/Manifold seal.  It looks like it could be the former.  I'd like to clean up the catch and tighten the valve to manifold screws and see what it looks like in a couple days.

This may require a valve change which would briefly glitch the fluid pressures twice and in between have the BS HEPI uncontrolled for a few hours as we bleed after the valve change.

Comments related to this report
hugh.radkins@LIGO.ORG - 13:37, Friday 31 January 2014 (9721)

I cleaned up the Catch Pan and checked the Valve to Manifold screws.  They were plenty tight.  When I look again (Monday, tomorrow?) I'll be pretty confident about from whence the leak comes but I fairly sure now that is is from the Valve itself.

H1 General
andres.ramirez@LIGO.ORG - posted 10:16, Friday 31 January 2014 - last comment - 12:17, Friday 31 January 2014(9709)
Stiffener rings and o ring protectors
Starting Stiffener rings and o ring protectors installation on HAM4 - Apollo

Comments related to this report
andres.ramirez@LIGO.ORG - 12:17, Friday 31 January 2014 (9717)
Work completed!
H1 ISC
kiwamu.izumi@LIGO.ORG - posted 15:09, Thursday 30 January 2014 - last comment - 00:30, Friday 15 January 2016(9630)
REFLAIR and POPAIR PD chain check

I have been silently checking the signal chain of the REFLAIR and POPAIR RFPDs using the AM laser (a.k.a. PD calibrator) to make sure that they are functional expectedly.

Summary

The RF frequency of the AM modulation was adjusted in each measurement such that the demodulated IF signal was below 50 Hz.


Calibration of the amplitude modulation depth

We recalibrated the AM laser.

The current setting of the laser was changed recently because we opened up the current driver when we thought the laser diode had been dead in the early December. Then the laser head and its current driver were sent to Rich at Caltech for his extensive testing although the laser magically fixed itself and he didn't find anything wrong. So this was the first time for us to use the AM laser which had been fixed. Because of that mysterious event, I wanted to recalibrate the laser. First of all, Yuta and I measured the power to be 2 mW with an Ophir Vega without the attenuation filter. Then we measured the modulation depth for the amplitude modulation by using a Newfocus 1611 as a reference.

The new calibration for the amplitude modulation is:

P_am =  5.13 mW x (P_dc / 1 mW) * (1 V / V_drive)

where P_dc is the laser power at DC and V_drive is the drive voltage when it is driven by a 50 Ohm source. For example, if one puts this laser to a PD which then shows a DC laser power of say 2 mW, the AM coefficient is now 5.13 mW x ( 2 mW / 1 mW) /V_drive = 10.26 mW/V_drive.


REFLAIR_A_RF9 (S1203919)

Remarks:

The signal chain is OK. The PD response is smaller by 15% for some reason.

It seems as if the transimpedance is smaller by 15% than what had been measured at Caltech (LIGO-S1203919). The cable loss from the RFPD to the rack was measured to be 0.47 dB. Be aware that the demod gain is half of the quad I/Q demodulator because this is a dual channel demod (see E1100044). The demod conversion gain is assumed to be 10.9 according to LIGO-F1100004-v4.


REFLAIR_A_RF45 (S1203919)

Remarks:

The signal chain is healthy.

Found cable loss of about 1.5 dB. The measurements excellently agree with the loss-included expectation.


POPAIR_A_RF9 (S1300521)

Remarks:

The signal chain is healthy.

The measurement suggests that there is loss of 1 dB somewhere. I didn't measure the cable loss this time.


POPAIR_A_RF45 (S1300521)

Remarks:

The signal chain is OK. Though loss sounds a bit too high.

The measurement suggests a possible loss of 2.6 dB somewhere. I didn't measure the cable loss.


REFLAIR_B_RF27 (S1200234)

Remarks:

The signal gain is bigger than the expectation by a factor of 2.3.


REFLAIR_B_RF135 (S1200234)

Remarks:

The signal gain is bigger than the expectation by a factor of 1.5


POPAIR_B_RF18 (S1200236)

Remarks:

The signal gain is bigger than the expectation by a factor of 2.3


POPAIR_B_RF90 (S1200236)

Remarks:

The signal gain matches with the expected value, but I don't believe this.

Comments related to this report
kiwamu.izumi@LIGO.ORG - 17:16, Thursday 30 January 2014 (9678)

There was a typo:

P_am =  5.13 mW x (P_dc / 1 mW) * (1 V / V_drive)

P_am = 5.13 mW x (P_dc / 1 mW) x (V_drive / 1 V)

koji.arai@LIGO.ORG - 18:38, Thursday 30 January 2014 (9686)

For 27MHz and 136.5MHz, the RF gains are +19.8dB and +50.7dB, respectively. S1400079

 

daniel.sigg@LIGO.ORG - 22:46, Thursday 30 January 2014 (9696)

The response of the BBPD isn't really flat over all frequencies. See D1002969.

koji.arai@LIGO.ORG - 12:59, Friday 31 January 2014 (9719)

The description in D1002969 is for the initial version. (The schematics seems up-to-date.)

The latest version has the rf performance as attached.

Non-image files attached to this comment
kiwamu.izumi@LIGO.ORG - 13:11, Wednesday 05 February 2014 (9845)

This is a follow up of the calibration measurements for REFLAIR_B and POPAIR_B.

I have updated the expected signal gain for these photo detector chains using more realistic gains which Koji gave (see his comments above). Now all the values make sense. Note I did not perform any new measurements.

In the following calculations, the quantity in red represent the updated parameters.

 


REFLAIR_B_RF27(S1200234)

Remarks:

The signal chain is healthy. There is loss of 0.92 dB somewhere.

  • Expected AM at 27 MHz = 5.13 mW x (1.045 mW / 1 mW) x 0.05 V_drivepp x 0.4 A/W x 2.1 kOhm = 225 mVpp
  • Expected ADC counts = 19.8dB (S1400079-v1) x 225 mVpp x 10.9 x 2^16/40 counts/V = 39294 counts pp
  • Measured ADC counts = 35431 counts pp
    • The signal is smaller by 0.92 dB than the expected.

REFLAIR_B_RF135(S1200234)

Remarks:

The signal chain is OK. There is loss of 3.9 dB somewhere.

  • Expected AM at 135 MHz = 5.13 mW x (1.045 mW / 1 mW) x 0.0014 V_drivepp x 0.4 A/W x 1 kOhm = 3 mVpp
  • Expected ADC counts = 50.7 dB (S1400079-v1) x 3 mVpp x 10.9 x 2^16/40 counts/V = 18377 counts pp
  • Measured ADC counts = 11689 counts pp
    • The signal is smaller by 3.9 dB than the expected.

POPAIR_B_RF18 (S1200236)

Remarks:

The signal chain is healthy. The signal was bigger by 9% than the expected.

  • Expected AM at 18 MHz = 5.13 mW x (0.93 mW / 1 mW) x 0.1 V_drivepp x 0.4 A/W x 2.1 kOhm = 401 mVpp
  • Expected ADC counts = 401 mVpp x 10.9 x 2^16/40 counts /V = 7157 counts pp
  • Measured ADC counts = 7803 counts pp
    • The signal is greater by 9 % than the expected.

POPAIR_B_RF90 (S1200236)

Remarks:

The signal chain is healthy. There is loss of 1.2 dB somewhere.

  • Expected AM at 90 MHz = 5.13 mW x (0.93 mW / 1 mW) x 0.1 V_drivepp x 0.4 A/W x 1.2 kOhm = 229 mVpp
  • Expected ADC counts = 229 mVpp x 10.9 x 2^16/40 counts/V = 4090 counts pp
  • Measured ADC counts = 3549 counts pp
    • This is smaller than the expected by 1.2 dB
evan.hall@LIGO.ORG - 14:08, Wednesday 06 January 2016 (24728)

From these measurements, we can use POPAIR to infer the calibration for POP.

I looked at a recent lock acquisition while the interferometer was trying to engage the outer ISS loop. The LSC is relatively stable during this time, and the POP beam diverter is still open.

After undoing whitening gain and digital gain (2 ct/ct for POPAIR9/45, and 32 ct/ct for POP9/45), we find the following TFs:

  • POP9I/POPAIR9I = 0.19 ct/ct
  • POP45Q/POPAIR45Q = 0.21 ct/ct

This implies calibrations of 1.7×106 ct/W for POP9 and 1.8×106 ct/W for POP45.

Images attached to this comment
evan.hall@LIGO.ORG - 00:30, Friday 15 January 2016 (24959)

There's a factor of 4 difference in power between POP and POPAIR (17 mW versus 68 mW with a PSL power of 23 W), so the values I gave above are off by a factor of 4. The demod gains should be 6.4×106 ct/W for POP9 and 7.2×106 ct/W for POP45.

H1 SUS
betsy.weaver@LIGO.ORG - posted 12:01, Thursday 30 January 2014 - last comment - 14:07, Friday 31 January 2014(9658)
Ring Heater in line of fire during welding

We've observed some burn marks on the shielding of the ETMy ring heater cables which occured sometime during the 3 prior weld sessions (May 2012, Dec 2013, Jan 2014).  The burns are on the lowest ring heater cable that laces around the test mass and makes a connection between the test mass and the PUM.  There is a burn on the right segment and the left segment.  I dug up a picture that shows that the burn on the "right" segment (as viewed from the back of the suspension) was there just after the May 2012 weld session, so that one is not new.  However the "left" cable burn is new from the Dec or Jan welding.  We did not see when this actually occured.

Filiberto tested the ring heater cable and found that all pins are operating as per spec, although he thinks pin 1 is shorting.  We are tracking down what this means (did we test it correctly, when was it last tested, is it possible that the burn is contributing to the short, even though it does not look like it is, etc.).

Comments related to this report
betsy.weaver@LIGO.ORG - 12:03, Thursday 30 January 2014 (9659)

This is the picture of the RH "right" cable taken in May 2012.

Images attached to this comment
betsy.weaver@LIGO.ORG - 12:11, Thursday 30 January 2014 (9660)

And here is the "left" RH segment burn which happened in the Dec or Jan weld.

Images attached to this comment
filiberto.clara@LIGO.ORG - 14:07, Friday 31 January 2014 (9723)
For the ring heater cable, the following pins were tested.

Pins 2,3,4, and 5 are tied together.
Pins 14,15,16, and 17 are tied together.
The resistance between these two sets is 47.5 ohms.

Pins 8,9,10, and 11 are tied together.
Pins 20, 21, 22, and 23 are tied together.
The resistance between these two sets is 45.9 ohms.

Pin 1 is tied to shield and shorted to ground.

Filiberto Clara 
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