Attached are plots of dust counts > .3 microns and > .5 microns in particles per cubic foot requested from 5 PM Jan. 30 to 5 PM Jan 31. Also attached are plots of the modes to show when they were running/acquiring data. Dust monitor 10 in the H1 PSL enclosure is still indicating a calibration failure.

Data taken from h1nds0.
T0=13-01-31-01-00-00; Length=86400 (s)
9780 seconds worth of data was unavailable on this server
1419.0 minutes of trend displayed

Attached are plots of dust counts > .3 microns and > .5 microns in particles per cubic foot requested from 5 PM Jan. 31 to 5 PM Feb. 1. Also attached are plots of the modes to show when they were running/acquiring data. Dust monitor 10 in the H1 PSL enclosure is still indicating a calibration failure.

Data taken from h1nds0.
T0=13-02-01-01-00-00; Length=86400 (s)
7740 seconds worth of data was unavailable on this server
1427.0 minutes of trend displayed

Design of isolation loops for HAM-ISIs go in 3 steps:
1) - Isolation loops level 1 :UGF=10Hz
2) - Isolation loops level 2: UGF=25Hz
3) - Isolation loops level 3: UGF=35Hz
The higher the step, the more sophisticated the control loops are.

Level 3 Isolation loops were designed, and installed, on HAM3-ISI a couple weeks ago. They were not used then.

The design of Level 3 isolation loops for HAM2-ISI was completed today. These control loops were installed and tested in cunjuction with their counterparts, running on HAM3-ISI:
- The IMC was locked right away (Gain=10dB, boost filter engaged) ~ 1.45pm PCT
- Spectra of the IMC length controls were taken, and compared with results obtained with the level 2 isolation loops (same blen filters used)

Improvements:
- Better performance in the 5Hz-10Hz range
- Better performance in low frequencies, below 200mHz

Notes:
- The IMC is still locked (5.41pm) and I am about to lower its loop gain to 0dB, just to make sure the servo does not damage anything if the IMC loses lock (requested by Giacomo & Cheryl)
- Ground motion is a bit favorable now, but not in the range of improvements, along the X-axis.
- Level 3 isolation loops will be left engaged over the weekend (see attached screenshots for Watchdog Values).

Giacamo/Cheryl worked out at IOT2R for the first part of the day with Laser Hazard (then after their work, we transitioned to Laser Safe).  This cleared up Hugo to do work on HAMISI & Barton to run measurements.

The Y Beam Manifold Spool was installed this morning.

Betsy worked on ITMy & Travis worked at Test Stand

EY BSC10 door was removed

Toppenish Middle School had an 8th Grade tour of the site (~100students)

This morning, I pulled the First Contact from ITMy-HR.  I then swapped in fresh witness plates for the ones I placed under the ITMy yesterday since I already saw particulate on them.  I did a final check over of the chamber and moved out all of my equipment.  The chamber is ready to close.

For the record, here are the weights of the glass optic, compared to the weight of the dummy we used to tune the suspension:

BS optic = 14,251g

Dummy mass = 14,180g

So, the optic hangs a bit lower in the structure than the metal dummy mass - Travis confirms this with the position error of the top BOSEMs.  We will correct this if IAS measures that we need to.

Also, FYI - a BS shipping cake tin weighs = 22,538g

Fogot to post this Wednesday.  These are the pitch/yaw numbers after Travis locked the quad pitch adjustor set screws Wednesday morning.

• Pitch: 5.0 µrad up
  • Target: 12.5 µrad up
  • Error: 7.5 µrad down
  • Tolerance: ±160.0 µrad
• Yaw: 72 µrad CCW
  • Target: 0.0 µrad
  • Error: 72 µrad CCW
  • Tolerance: ±160 µrad

All BSC8 HEPI actuators have been removed.  These may be used for BSC3 after replacing the left(NW,SE) return vertical flexible pressure lines from 30" to 41".

Attempting undamped TFs on IM1 using new script. Commissioning switch should go on and off automatically.

- Giacomo, Cheryl

Alignment of the IMC, and IM3 and IM4, increased IFO REFL from 106mW earlier this week to 147mW today, giving 90% power coupled into the IMC.  In our first measurement, the IMC alignment had drifted away from optimum, and the the IFO REFL beam was clipped on the baffle in front of IM4.

Power budget: 

• 2:58am:  6.0mag earthquake near Alaska.
• 9:09am:  Arnaud starting ITMy (BSC1) SUS Transfer Functions (at 9:09am till 11?)
• Rodruck/Apollo craning/fit checking Photon Calibrator periscopes (10-12)
• 10:30am:  Filiberto running cable around HAM3 around 10:30
• Hugh checking out issues with BSC1 HEPI Sensors
• SUS gave ok, so tomorrow (Fri), Spool & BSC1 door can be installed
• FMCS alarms:  EY Temperature (temperature heading over 75deg [from 69deg]) & MX Air Handler

The sensors used by HEPI-ITMY look functional. The attached plot shows the spectra of the L4Cs and the STS-2 (ground instrument).
STS-2 signals from HEPI-BSCs are broad-casted to the other chambers via a STS-2 distribution chassis (D0900351).
STS-2 signals seen by HEPI-HAM2 et HEPI-ITMY are identical (cf spectra).

Please see LLO aLOG 6041 for details.

Took a (last) set of TF on the ITMY. DTT xml files can be found here :

/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGM0/Data/2013-01-31_1000_H1SUSITMY_M0_*_WhiteNoise.xml
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H1/ITMY/SAGR0/Data/2013-01-31_1000_H1SUSITMY_R0_*_WhiteNoise.xml

The plots are consistents with models and last measurements, cf pdf enclosed

[Robert, Giacomo]

In the past few week we have alwayis notice a ~1 h period variation in the IMC-REFL power during IMC locks. We suspected that it has something to do with the temperature, but only this morning Robert forced me to take 5 minutes and look into it. There is a clear correlation between PSL room temperature and IMC-REFL power (i.e. alignment into the IMC) at and below about 1 mHz (no surprise).

Attached are data taken during an IMC lock at UTC 2013-01-25 04:30:00 (GPS = 1043123416)

- time series of the IMC REFL power (H1:IMC-REFL_DC_OUT_DQ) and the four temperature sensors in the PSL room (H1:PSL-ENV_LASERRM_[ACN/ACS/TBLN/TBLS]_TEMP_DEGC)

- transfer function and correlation between each of the temperature channels and IMC-REFL

TBLS (not surprising as the periscope is right there) and ACN (not sure where this sensor is...) show the biggest corelation with the IMC_REFL power.

GPS = 1043654615

Common gain = 20 db, 1st boost on.

Betsy W. and Arnaud P.

We took B&K hammer measurements on the QUAD installed on BSC1. The configuration during the measurement was BSC1 locked  QUAD unlocked and Vibration Absorbers ON.
The position of the accelerometer and the direction of axis were chosen from LLO measurements, cf picture attached to post 6022.
As for LLO, the hammer trigger threshold was set to 10N.

Two configurations of measurement have been recorded. For each of them, the 3 directions (X Y and Z) were saved from the accelerometer :
-excitation (hammer hit) along the X axis
-excitation (hammer hit) along the Y axis

The TF plots generated by Pulse Labshop have been directly exported to excel then pdf (enclosed). Each figure is showing phase (plot above) and magnitude (plot below) 

Comparing the results to the ones from LLO  (cf post 6022), the only particular thing to mention is the anti-resonnance at 25Hz for the two measurements. 
Otherwise, for the X impact-X response (first pdf, blue curve, 2nd plot), as for LLO we find peaks at 75Hz, 125Hz and 150Hz.
For the Y impact-X response (second pdf, blue curve,2nd plot), as for LLO we find a peak at 75Hz and an anti-resonnance at around 125Hz.

A bit of investigation will be needed before validating that step. 




 
 

The CBC data quality group have been looking at the noise coming out of the PSL to practice detector characterization for aLIGO. We noticed that there is a significant change in the nature of the PSL spectrum between Jan 29 and Jan 30, 2013, possibly correlated to the PSL reboot. I have attached plots of spectrum of H1:PSL-ISS_PDA_OUT_DQ to show this.

The first plot (viewer-0.png) shows the PSL spectrum from a good time on Jan 29. I have also attached the status of the PSL online detchar channel (ODC) for the same time period (viewer-1.png). The ODC state is all green, indicating that the PSL is functioning correctly and both the ISS and FSS are locked. This spectrum looks good.

However, the PSL spectrum from this morning (Jan 30) appears to have a strong line at 60 Hz with a harmonic at 120 Hz, a new line at 300 Hz, a forest of lines above 500 Hz, and a large bump at 650 Hz (viewer-2.png). I looked at the ODC data to pick 60 seconds where the PSL is locked to make the spectrum (viewer-3.png). The PSL appears to be going in and out of lock much more today. 

I tried picking a time this morning when the PSL was in a good state for a longer period of time. I have attached the PSL ODC plot for 40 mins from 0800 PST (viewer-5.png) which shows that there appears to be a good stretch of data at 0828 PST. The PSD for this time (viewer-4.png) does not have the large bump at 650 Hz, but the other lines are still there.

Is this a known issue with the PSL?