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Reports until 12:17, Wednesday 05 February 2014
H1 SUS
arnaud.pele@LIGO.ORG - posted 12:17, Wednesday 05 February 2014 (9842)
ETMY TF still looking good

Results of last set of ETMY transfer function after finishing the alignment (see this alog for alignment numbers) are attached below, and look similar to what was taken monday night. TMS team can start (and probably already did) work on the installation. SUS will go in the next days check for lower masses flag/osem centering as well as top mass verticals. 

Attached files :

H1 ETMY fiber after finishing alignment (in black) compared to first alignment (in orange) compared to LLO ETMX fiber in chamber. Main chain (1st pdf) and reaction chain (2nd pdf)

To notice :

- First pitch mode of the main chain fiber quads are shifted down (0.52Hz) compared to the model (0.562Hz). Cf p5 of first attachment.

Non-image files attached to this report
H1 SEI (SUS)
sheila.dwyer@LIGO.ORG - posted 11:06, Wednesday 05 February 2014 (9839)
the right sign helps

Jim Rich and Hugh have been working on the ITMX ISI, and found a sign flip. Here are plots of the sus witness sensors (L2WIT) and OpLevs:

Modified instructions for turning on ITMX ISI after a trip:

Of course this mght change, especially the stage 2 blends might work with a different set of blends.

Images attached to this report
H1 AOS
filiberto.clara@LIGO.ORG - posted 10:31, Wednesday 05 February 2014 (9838)
ETMY Arm Cavity Baffle -photo diode test
Looked at photo diode forward voltage for ETMY ACB per LIGO-T1100637.
PD forward voltage(≈ 0.5V)

Pin 13 & 12 
PD forward voltage: 0.428V

Pin 10 & 9 
PD forward voltage: 0.421V

Pin 7 & 6
PD forward voltage: 0.428V

Pin 4 & 3
PD forward voltage: 0.421V


Filiberto Clara & Mitchell
H1 SUS
thomas.vo@LIGO.ORG - posted 09:17, Wednesday 05 February 2014 - last comment - 11:10, Wednesday 05 February 2014(9836)
SUS at HAM4 @ 9:17 AM PT
Andres and Jeff working on SR2
Comments related to this report
thomas.vo@LIGO.ORG - 11:10, Wednesday 05 February 2014 (9841)
Finsihed at 11:10 AM PT
H1 AOS
thomas.vo@LIGO.ORG - posted 09:09, Wednesday 05 February 2014 - last comment - 13:08, Wednesday 05 February 2014(9834)
Mitch at West Bay @ 9:08 AM PT
Working on ACB with Apollo.
Comments related to this report
thomas.vo@LIGO.ORG - 11:44, Wednesday 05 February 2014 (9843)
Out for lunch at 11:44 AM PT
thomas.vo@LIGO.ORG - 13:08, Wednesday 05 February 2014 (9844)
Back at the West bay @ 1:08 PM PT
H1 AOS
jason.oberling@LIGO.ORG - posted 09:08, Wednesday 05 February 2014 - last comment - 10:21, Wednesday 05 February 2014(9833)
ETMy Cartridge Alignment
IAS: J. Oberling
SUS: B. Weaver, T. Sadecki
 
Finished the ETMy cartridge alignment yesterday.  The position & angular errors are as follows (all yaw reported as viewing the relevant optic from the top down):

Also measured & aligned the ERMy (Note: the ERMy is aligned parallel to the AR surface of the ETMy) and measured the gap between the ETMy and ERMy.

Comments related to this report
betsy.weaver@LIGO.ORG - 10:21, Wednesday 05 February 2014 (9837)

Note - we discovered yesterday that the Kentek gap detector was highly dependent on how level it's mounting was.  So, the measurement is only good to about +/-0.25mm.

H1 AOS
mitchell.robinson@LIGO.ORG - posted 08:02, Wednesday 05 February 2014 (9831)
ETM-Y ACB
Mitchell, Scott (Apollo)

The assembly of the Arm Cavity Baffle was completed yesterday. Final weights need to be taken then, it will be suspended from the solid stack to begin balancing.
H1 CDS
sheila.dwyer@LIGO.ORG - posted 06:51, Wednesday 05 February 2014 (9830)
h1ecat x1 restarted
It had the usual problem of asking me to choose a run time system in the active and run step, and not being able to log in.  
I also did an svn update, and got a message about the redoubt certificate. 
H1 ISC
stefan.ballmer@LIGO.ORG - posted 00:10, Wednesday 05 February 2014 - last comment - 00:12, Wednesday 05 February 2014(9827)
PRMI locked - ring heater set to 4W
Lisa, Stefan

To get the PRMI locking we had to turn off all 2-stage ISIs.

With the 1-day old heating of ITMY at 1.5W, and an alignment tweak, we got 6000cts of POP18. Unfortunately I am not 100% sure how much of that is alignment, and how much is heating.

At UTC 08:4:33 we turned the ring heater to 4Watt total (2Watt each).
Comments related to this report
lisa.barsotti@LIGO.ORG - 00:12, Wednesday 05 February 2014 (9828)ISC, SUS
This is a comparison ISI ON/OFF as seen by the ITMX optical lever.
References are with ISI on (blue and red), compared to ISI off (cyan and magenta).
Non-image files attached to this comment
H1 SUS (ISC, SUS)
lisa.barsotti@LIGO.ORG - posted 23:10, Tuesday 04 February 2014 - last comment - 09:15, Wednesday 05 February 2014(9826)
ITMX Optical Lever Signals
I believe the ITMX optical lever signals are calibrated in urad. If that's the case, the ITMX PIT motion right now is 0.3 urad RMS  (this is with the ISI in the configuration Rich left it in).

All the RMS comes from 0.1 - 0.7 Hz and I see 1 urad / sqrt(Hz) @ 0.5 Hz. 

This is significantly worse than ETMY/ITMY motion during the one arm test (0.2 urad/ sqrt(Hz) and 0.3 urad / sqrt(Hz) @ 0.5 Hz T1200450), and normal operations at LLO (0.4 urad RMS, and 0.05 urad/ sqrt(Hz) at 0.5 Hz - LLO log 8637).

Need to double check that I am comparing apples to apples.


Non-image files attached to this report
Comments related to this report
peter.fritschel@LIGO.ORG - 06:04, Wednesday 05 February 2014 (9829)

Don't you mean an RMS of 0.3 rad for pitch? At least, if the vertical axis is in microradians.

lisa.barsotti@LIGO.ORG - 09:15, Wednesday 05 February 2014 (9835)
Yes, bad typo, I fixed the entry.
H1 SEI
hugh.radkins@LIGO.ORG - posted 19:44, Tuesday 04 February 2014 (9825)
WBSC 1 & 2 ITMY/BS ISIs Running

Have(had) both ISIs running, RichM took over on the BS.  Have both running at lvl3 with blends of T100mHz.44NO on X & Y and T250 elsewhere on stage1. 250mHz on Stage2.  Decided to try the T40mHz.44NOs on ITMy and they work.  They aren't available on the BS now but with them on on the ITMY there is more lower band green on the BLRMS.  Toggled the Stage2 blend to a fro 750 vs 250 mHz and at the cost of some higher frequencies, the lower bands on the stage2 are greener with higher blend.  Maybe due to the blending bump?

H1 PSL
sheila.dwyer@LIGO.ORG - posted 19:18, Tuesday 04 February 2014 (9824)
PSL restarted, ref cav alinged
Sheila, Paul

We restarted the PSL after the power watchdog tripped.  (to do this we transitioned the enclosure to science mode).  After the laser had been on for about 15 minutes I thought it would be OK to try to align the ref cav (the trans power had dropped to 0.75 V in the last few days).  
Before the AOM we had 31mW,( measured with the filter in) 30.5 after the first pass, and 18.6 after the second pass.  (60% double pass diffraction efficiency).  I tried to improve this my adjusting the alignment of the retroreflecting mirror, but wasn't able to get any better, and the final alignment had about 17.6 mW after the second pass (57% double pass eifficency).  Tuning up the alignment into the cavity we got the trans PD up to 0.94V, but after I transitioned back to science mode the trans power dropped to 0.86V.  

H1 PSL
david.barker@LIGO.ORG - posted 16:47, Tuesday 04 February 2014 - last comment - 09:00, Wednesday 05 February 2014(9818)
H1 PSL down, recovery ongoing
Rick, Sheila,

at 00:16 the PSL turned off. Rick and Sheila think the power watchdog may have tripped. Sheila has started the recovery procedure.
Comments related to this report
david.barker@LIGO.ORG - 09:00, Wednesday 05 February 2014 (9832)
I forgot to specify 00:16UTC, 16:16PST.
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