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Reports until 17:15, Wednesday 02 April 2014
H1 SUS (SUS)
giles.hammond@LIGO.ORG - posted 17:15, Wednesday 02 April 2014 (11138)
ITMY monolithic welding
We started welding in fused silica fibres this morning and now have 3/4 fibres installed. We plan to weld the final fibre tomorrow morning, followed by de-stress and hanging.

Travis, Gary, Giles
H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 16:52, Wednesday 02 April 2014 (11137)
TCSX and TCSY install - with an army.

Aidan, Alastair, Dave H, Dave R, Albert L, Eric G, Thomas V.

Tidied up the plumbing on TCSX. Installed plumbing on TCSY. All three picomotor mirrors installed and confirmed to be working on TCSX.

Hooking up proximity sensors for flipper mirrors. Installed shutter on TCSX laser.

Images attached to this report
LHO General
justin.bergman@LIGO.ORG - posted 15:57, Wednesday 02 April 2014 (11133)
ops afternoon

Morning shift covered by Corey

130 - TCS crew energizing laser on optical table at BSC3. Beginning to populate table at BSC1. Did I see Dave Reitze working on this?

various ISI/SUS trips throughout the afternoon as a result of commissioning.

 

 

H1 SUS
arnaud.pele@LIGO.ORG - posted 15:04, Wednesday 02 April 2014 (11136)
QUAD oplev

New screens showing oplev path on the QUADS after updating what Stuart did at LLO. I made a small correction and commited SUS_CUST_QUAD_OVERVIEW to the svn. cf attached screenshot

Images attached to this report
H1 SUS
margot.phelps@LIGO.ORG - posted 14:57, Wednesday 02 April 2014 (11135)
ITMX stored in box
Betsy and I stowed ITMx (see attached picture). Plan for this guy is to get the sealed door on the box later today or tomorrow, then leave it in the cleanroom until its ready to move over to the beer garden.  
Margot 
Images attached to this report
H1 SEI
arnaud.pele@LIGO.ORG - posted 14:42, Wednesday 02 April 2014 (11134)
ETMY GS13 V2

[Rich M. Arnaud]

ETMY GS13 V2 input signal was sitting at around 6000cts whereas the others at ~100 cts. Turning off/on the digital Gain + DWH switches brought it back to ~1000cts. Better. Though, it seems like there is still an offset that adds up to the signal.

H1 AOS (AOS, SUS)
thomas.vo@LIGO.ORG - posted 14:04, Wednesday 02 April 2014 (11131)
H1 ETMY Optical Lever
Arnaud, Eric G, Apollo, Thomas

We've installed the optical lever with two levels of 1:10 whitening in hardware and complimentary de-whitening in software.
 
They are calibrated to micro-radians and I've attached a plot showing the linear response.  The difference in their gains is most likely due to their difference in beam width.
Pit_Gaussian_width = 2.02 mm
Yaw_Gaussian_width = 1.41 mm

H1:SUS-ETMY_L3_OPLEV_PIT_GAIN = 95.50
H1:SUS-ETMY_L3_OPLEV_YAW_GAIN = 69.33

H1:SUS-ETMY_L3_OPLEV_SUM_OUT = 20,000 counts.

Images attached to this report
H1 ISC
alexan.staley@LIGO.ORG - posted 14:00, Wednesday 02 April 2014 (11132)
IMC Noise Measurements

(Daniel, Alexa)

We measured the dark noise and shot noise of the LSC RF PD in the refl path of the IMC.

  1. Dark noise: We blocked the PD and confirmed this by looking at the H1:IMC_REFL_DC_OUT which went down to about 0.02 counts. The noise was measured to be approx 80nVrms/sqrtHz from the SR785.  For greater accuracy, we took the power spectrum of H1:IMC-I_OUT using DTT. The result is deipcted in (REF2) -- this measurement is in counts and must be calibrated using 20/2^16 V/cnts conversion with a factor of 100 to take into account the whitening filter.
  2. Shot noise: We placed a light bulb in front of the PD and read back 8705 counts at DC (again, using H1:IMC-REFL_DC_OUT). The noise was measured to be approx 280nVrms/sqrtHz from the SR785. We also took a power spectrum of H1:IMC-I_OUT (the same calibration above must be applied). 

From this measurement we calculated the AC transimpedance of the PD to be 2.1kOhm (with a 100 Ohm DC transimpedance). 

Non-image files attached to this report
LHO General
corey.gray@LIGO.ORG - posted 13:31, Wednesday 02 April 2014 (11125)
Ops DAY Summary

Started off morning with many RED systems.  Jeff B walked me through getting everyone (SUS, HEPI, ISI) in BSC2 back & then went from there.

Days Activities:

-Had to leave shift at 1:30 and was spelled by Justin B.

LHO VE
john.worden@LIGO.ORG - posted 13:14, Wednesday 02 April 2014 (11129)
YEND Pumpdown

Log-Log plot attached with T0 set to start of rough pumping (~700 torr).

Images attached to this report
Non-image files attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 11:26, Wednesday 02 April 2014 (11127)
~1100 hrs local -> Valved-out MTP at Y-end briefly while switching between QDP80 and scroll backing pumps
Demonstrated MTP safety valve closes and turbo spins down with the removal of AC to the scroll pump -> This mimics the functionality of a loss of "Motor Run" signal from the nominal backing pump -> Shut down QDP80 and purge air supply
H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 08:39, Wednesday 02 April 2014 (11124)
CDS model and DAQ restart report, Tuesday 1st April 2014

model restarts logged for Tue 01/Apr/2014
2014_04_01 12:39 h1susetmy
2014_04_01 12:39 h1susitmy
2014_04_01 12:42 h1broadcast0
2014_04_01 12:42 h1dc0
2014_04_01 12:42 h1fw0
2014_04_01 12:42 h1fw1
2014_04_01 12:42 h1nds0
2014_04_01 12:42 h1nds1
2014_04_01 12:51 h1susitmx
2014_04_01 12:52 h1susetmx

All restarts expected and part of Tuesday maintenance.

H1 General (VE)
rainer.weiss@LIGO.ORG - posted 20:46, Tuesday 01 April 2014 (11123)
Time for Yend pumpdown
The attached log/log plot gives the estimate that it will take a little over three weeks
for the pressure to get to 3 x 10^-7 torr which will reduce to 1 x 10^-8 torr when the chamber
is open to the cryo pump.
Non-image files attached to this report
H1 SEI
sheila.dwyer@LIGO.ORG - posted 17:44, Tuesday 01 April 2014 - last comment - 11:43, Thursday 03 April 2014(11120)
ISIs tripped

There was a magnitude 8 earthquake in Chile, all BSC ISIs tripped. 

Images attached to this report
Comments related to this report
jameson.rollins@LIGO.ORG - 18:01, Tuesday 01 April 2014 (11122)

How did the new BSC SEI guardians do in recovering everything?  Where there any problems or hiccups?  Did it go smoothly?

brian.lantz@LIGO.ORG - 13:41, Wednesday 02 April 2014 (11130)ISC, SUS, SYS
Thanks for posting the data, Sheila. 
We (by which I mean Hugo) will look at this a bit more. A quick look makes it seems that all three vertical drives on 3 of 4 platforms were pushed to the max within 1 second of each other. Many people (W. Hua, Rana, Dan Clark, me, Peter F, et. al.)  have suggested that using that using the sensor correction to only isolate against differential motion, rather than trying to get rid of the absolute motion as the whole site heaves up-and-down would be a smart thing to do. I think this will be a good example to look at. 
-Brian
hugo.paris@LIGO.ORG - 11:43, Thursday 03 April 2014 (11153)

TIme series were collected on both BS (ground STS, high gain) and ETMX (ground T240, low gain) at LHO. 

They can be found on the svn at:
ligo/svncommon/SeiSVN/seismic/Common/Data/2014_04_01__Chile_Earthquake_Data/

For reference, LHO ground sensor time series were also colected for previous earthquake data, recorded on March 3rd of 2014. ligo/svncommon/SeiSVN/seismic/Common/Data/2014_03_10__Earthquake_Data/

Images attached to this comment
LHO VE
kyle.ryan@LIGO.ORG - posted 16:06, Tuesday 01 April 2014 (11119)
Installed 1.5" O-ring valve in foreline plumbing of Y-end Main Turbo pump
Y-end pumping interrupted for ~15 mins during valve install -> Flex line from MTP to Turbo Header can now be isolated at the MTP plumbing -> Flex line from MTP to locally mounted scroll pump can now be isolated at the MTP plumbing -> Currently both QDP80 and scroll pump are running, QDP80 backing MTP and scroll running but isolated from MTP -> ~500 watt scroll pump is currently being powered via an extension cord plugged into local vacuum 120VAC receptacle -> Would like to add a dedicated 120VAC receptacle local to the MTP control panel and eliminate the "scurge" of the extension cord
H1 SUS
arnaud.pele@LIGO.ORG - posted 16:04, Tuesday 01 April 2014 (11104)
quad oplev damping - model changes -

Since oplev damping might be used for Y arm commssioning as it is currently for X arm, I modified the QUAD_MASTER simulink model to have oplevs feedback on all the quads. 

Only FOUROSEM_STAGE_OPLEV.adl part was commited to the svn

Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 23:01, Monday 31 March 2014 - last comment - 13:02, Wednesday 02 April 2014(11106)
WFS bring COMM noise to 30Hz rms

Chris, Sheila

Our measurements of the COMM noise with the WFS locked have an rms of 20Hz, measured down to 0.1 Hz.  To make sure this was reasonable, we turned off the refl bias path so that the laser was locked only to the green beat note. The transmitted power fluctuations are noticably less than the HWHM of 40Hz, so this seems believable. (StripTool is the second screenshot attached). 

We wanted to try locking the arm half way down the fringe so we could make a measurement of the noise using the transmitted power.  Since the IR trans PD is normalized to 1 when the cavity transmission is maximized, the calibration of this signal is just a high frequency gain of 84 (FWHM of the arm cavity), and to correct for the refl bias loop gain we have a pole at zero and a zero at 3Hz.  The correct calibration has a more complicated frequency dependence, so we would have to do the real calibration to make a comparison above about 42 Hz.  Neither of these traces have the cavity pole at 42 Hz corrected for.  You can see that the side of fringe measurement agrees with the normalized refl PD signal well up to 100 Hz . (1st screen shot attached)

We repeated the measurement in the normal configuration, where we lock on resonance using the refl bias path, and the noise is the same (30Hz rms down to 0.02Hz). The RMS is dominated by the pitch mode, so we will work on increasing the WFS bandwidth tomorrow. Tonight we tried OpLev damping (this added noise around 1 Hz) and turning up the pitch OSEM damping gains (inconclusive so far). 

We redid the measurement with the WFS outputs held, and saw that the noise was high again (100Hz rms down to 0.1Hz), with the WFS on again we were back to the low noise state. So we can safely say the WFS are helping.

We also checked that the noise is the same from 3-100Hz with and without the refl bias path engaged. 

Images attached to this report
Comments related to this report
peter.fritschel@LIGO.ORG - 05:50, Tuesday 01 April 2014 (11108)

It's very nice to at last see a benefit from the WFS aignment control! good job.

sheila.dwyer@LIGO.ORG - 13:02, Wednesday 02 April 2014 (11128)

Here is the plot of the Noise with WFS on and with WFS off, for those who want to see it.

Images attached to this comment
H1 SUS
arnaud.pele@LIGO.ORG - posted 19:13, Wednesday 09 October 2013 - last comment - 17:49, Tuesday 01 April 2014(8069)
HSTSs Spectra

For future reference I took a spectrum of the 5 HSTS (MC1 MC2 MC3 PR2 PRM) from monday morning before the corner station was vented.

The isolation and damping on HAM2 and HAM3 ISIs were ON, and feedforward was OFF. The suspensions damping loops were closed. The chambers were under vacuum.

The attached pdf shows a comparison between the 5 HSTS, for every "mass" levels (M1 M2 and M3) and every degree of freedom.

Few things to notice on the plot :

- The performances are really consistent from one chamber to an other

- Signal is really close to sensor noise, especially at the bottom mass

- There is an interesting feature between ~0.1Hz and ~1Hz seen for longitudinal transverse and vertical dofs. This is something I would need to double check, but I'm pretty sure it is transmitted ground motion.

Non-image files attached to this report
Comments related to this report
arnaud.pele@LIGO.ORG - 17:49, Tuesday 01 April 2014 (11121)

For future reference and ACCEPTANCE REVIEW I attached the undamped/damped version of the spectra, adding the local osem basis to the plots for the 5 HSTS in HAM2-HAM3 chamber.


FIRST PDF = UNDAMPED
SECOND PDF = DAMPED

NOTE : 60Hz spike for some of the osems spectra, especially top mass osems of PRM.

Non-image files attached to this comment
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