The RAID card has been replaced in cdsfs0.  The new controller is now in the process of verifying the blocks on disk, which is a lengthy process and will take in the neighborhood of ~20 hours.  I will be back on site tomorrow early afternoon to run some additional checks on the filesystem before booting the CDS workstations and starting the RAID cache battery test.  There should be no issues with any of the CDS web pages at this point, it looks like everything is running normally there.  The external login server will be turned back on at the same time the workstations are ready.

RichM, HughR
Check for valid HEPI signals at BSC3 showed problems.  Found Cable going from HEPI AA chassis going to incorrect card on I/O comp.  HEPI I/O adc had an ISI cable attached.  We made BSC3 look like BSC 1/2 to correct; this matched the drawings.  The cable running from HEPI AA chassis was unlabeled.  The labeled cable was unattached at both ends.  I suspect the EEguys know something about this--maybe the labeled cable was deemed bad.  It should be removed is so and the cabling being used should be labeled.

The main fileserver for CDS workstations will be going down for maintenance today at 5PM local time, as specified in WP4188. ALL CDS workstations and remote logins will be unavailable during this work, which is anticipated to finish at 5PM PDT Saturday. Some web services will have interruptions in service during this period as well, such as the MEDM screenshots.  The front end systems and DAQ will continue to operate normally.  A follow up logbook entry will be posted when the work is completed.

Please save your work and log off soon if you are logged in remotely, or are using a local CDS workstation.

LVEA Laser safe
Alarms: Dust in Vac Prep Lab, Diode Room, and CDS frontends

Apollo – Installing walking plates at BSC3
Doug – Shooting alignment of the Elliptical Baffle in BSC2
Richard – Pulling cables at End-Y

09:20 Gerardo working on BOSEMs and Cable Brackets in SUS Cleanroom in LVEA
09:30 Rick & Peter working in the H2-PSL enclosure
10:37 Alexa – To End-X working in VEA
13:10 Patrick working on Dust Monitor #15 calibration failures 
    
  Getting continual low level (100 to 150 counts) dust alarms during the day from the Diode Room. Rick S. and I looked in the chiller anti-room, the diode room, and the A/C system, but could not find an apparent source for the alarms. Further investigation is needed to find the source of these alarms. 

As for the HSTSs, I took a spectra of PR3 from Monday. The isolation and damping loops of the ISI were closed (isolation level 3), as well as the damping loops of the suspension. The chamber was still under vacuum. Status of HEPI needs to be double checked.

The attached plot compares the spectra of LHO and LLO PR3, in a similar configuration (ISI isolated, SUS damped), for the 3 levels (M1 M2 and M3) and every degree of freedom.

Looking at the plots, we can see that LLO get more isolation at each level, even though we are using the same damping filters. That said, Jeff discovered that the suspension medm gains are set to different values, (higher values at LLO) which would explain why the resonnances of the suspension are more damped there. Other than this, spectra is very close to sensor noise. The larger signal between 0.1Hz and 1Hz is highly due to ground motion (I quickly took a spectra of the streckeisen sitting next to HAM2 chamber,  which shows the same shape around 0.1Hz) More details to come next week.

We installed C P Stat on the X arm tube opening where the spool was removed yesterday. We also lowered the clean room over BSC 3 to prepare for cartdrige install early Monday. I did a recheck of the upper limit on the main crane and found that the block was traveling up just a little to close to the drum so I adjusted the anti two block limit and it is ready to go.

As I mentioned in my last aLOG entry [8087], when performing the IMC sideband sweep measurements, the broad peaks when the sideband frequency is around an integer multiple of the IMC FSR are only expected to appear in the presence of a length/frequency lock offset. As such, we can try to compensate any offset in the length error signal by applying a digital offset in the IMC-L feedback path until these peaks are minimized*.

I recorded sweeps across the 45.5MHz FSR peak while adjusting the offset in the IMC-L path. The results are shown in the attached plot. As the offset is increased towards 20k counts, the peak reduces in magnitude.

Beyond 20k counts, the IMC would not stay locked long enough to make the measurement. I suspect this is caused by one of the outputs railing due to the additional offset, but I wanted to move on to higher-order mode peak measurements so I didn't investigate further. Maybe there is a better location to add the offset, for example on the analog common mode servo board itself. Apart from the lock losses above 20k counts, I didn't notice any drop in the IMC transmitted power with added offsets. This eliminates the possibility that the offset was driving the cavity further from carrier resonance and thus causing a large drop in the carrier light power, in turn causing the peak to drop in magnitude.

On a side note, since a bigger locking offset makes the FSR peaks easier to observe, it might be worth deliberately making this offset worse (i.e. adding -20k counts) for future measurements of the IMC FSR/length. This could help improve the SNR around e.g. the 18.2MHz, 27.7MHz and 54.5MHz peaks to make those measurements useful.

*At low frequencies the IMC-L path dominates over the IMC-F path, so applying an offset in the IMC-L path should suffice and eliminate the need to directly cancel any offset at the analog servo board input.

  Ops has been getting continual low level (100 to 150 counts) dust alarms all day from the Diode Room. Rick S. and I looked in the chiller anti-room and the diode room, but could not find an apparent source of the particles. Further investigation is needed to understand the source of these alarms.  

[Kiwamu, Stefan, Joe, Paul]

Last Thursday, measurements of several IMC FSR resonances were taken using the sideband sweep method [see e.g. LLO alog entry 4849].

In short, this method involves phase modulating the light into the IMC with a swept sine signal from a network analyzer and observing the signal in transmission of the IMC with an RF photodiode to observe various optical resonances within the cavity.

In this case, the RF photodiode was the broadband REFL AIR photodiode on ISCT1. The network analyzer output was split with a power splitter, with one output going to the REF input, and the other fed to a mini-circuits RF amp with a gain of 18.8dB. The network analyzer source Voltage was tuned to give around 10Vpkpk output from the RF amplifier. The RF amplifier output was then passed to the 45.5MHz input of the EOM on the PSL table. The RF output of the REFL AIR photodiode was connected to the A input of the network analyzer.

When the sideband frequency gets close a multiple of the FSR, a broad peak in the the N.A -->REFL AIR PD transfer function is observed, as reported in [1] and subsequent errata [2]. According to these references as well as Araya et al. [3] this broad peak is only present if there is an offset in the length/frequency lock of the cavity (more on that in a forthcoming post). There is a narrow dip in this peak however, when the sideband frequency approaches the exact FSR multiple frequency. The frequency at which this dip hits a minimum is an integer multiple of the cavity FSR.

The first attached plot shows 5 FSR peaks measured in this way. Since we apply the signal to the 45.5MHz input of the EOM, the modulation depth, and thus the SNR of the measurement, is low at frequencies far from 45.5MHz (e.g. the 18.2MHz FSR, the 27.3MHz FSR and the 54.5MHz FSR). The 36.4MHz peak and the 45.5MHz peak measurements came out the best, so I fitted the central dip using a simple Lorentzian function to estimate the frequency of the minima (see second attached plot).

The results from these two fits are summarised and compared to the design values in the following table:

The calculated lengths from each peak fit agree to within 100um, and are within 0.5mm of the design length.

If higher precision on this measurement is required later on, we could try syncing the network analyzer with a rubidium standard, and also try implementing the measurement technique described in [3]. Also, separately using the 9.1MHz input of the EOM to measure a greater sample of FSRs could be helpful.

[1] K. Skeldon and K. Strain, Applied Optics Vol 36, Number 27 (1997): http://www.opticsinfobase.org/ao/abstract.cfm?uri=ao-36-27-6802

[2] K. Skeldon and K. Strain, Applied Optics Vol 37, Number 21 (1998): http://www.opticsinfobase.org/ao/abstract.cfm?uri=ao-37-21-4936

[3] A. Araya et al, Applied Optics Vol 38, Number 13 (1999): http://www.opticsinfobase.org/ao/abstract.cfm?uri=ao-38-13-2848

An NPRO was setup for aligning and testing the outer loop power stabilisation photodetector array in the H2 PSL Laser Area Enclosure.  The power incident on the array was measured to be 250-260 mW, the beam diameter close to the location of the 8 individual photodiodes was about 800 microns.

Attached are plots of dust counts requested from 4 PM October 9 to 4 PM October 10.

Jason and I set 2new monuments and a new elevation target in preparations for tomorrow baffle alignment. I will setup the total station in the AM and be ready in the first hr.

Thanks to the matlab script Stuart A. wrote, I processed the DTT transfer functions of PR3 M2-M2 undamped TF and compared them with the ones from Livingston.

The TF were taken with a white noise excitation, while PR3 was under vacuum in July 2013, with the ISI damped.

The results of the three degrees of freedom are presented in the attached pdf

(1) First attachement compares the measured LHO PR3 M2-M2 transfer function against the model.

(2) Second attachement compares LHO PR3 M2-M2 against last measured PR3 M2-M2 TF from LLO (today) which was under vacuum.

Data are noisy at DC and above 5Hz but the measurements are matching very well the model and LLO's transfer functions.

09:19 Hugh to BSC3, electronics checkout
10:10 Betsy going to end X
10:32 Dale taking camera into LVEA
10:34 Filiberto working on cabling at end Y
10:45 Delivery for Richard
11:06 Justin turning off optical lever lasers in LVEA
11:30 Arnaud bypassing BS SUS IOP watchdog
12:32 Ops computer froze, restarted
13:51 Thomas heading into BSC2
14:30 I restarted h1conlog
15:50 Jonathan going into LVEA to test GC wireless network

MCL C02219: EX Table PZT 2, NB85-AR10 (to be replaced)

MCL C02218: EX Table PZT1, ND2-AR10-ISS

MCL C02718: EY Table PZT 2

MACL C02722: EY Table PZT 1 (test previously and seen similar results to MCL C02718)

The three PZT's (two on EY, one on EX) have a range from 0 to 10V. Another 0 to 10 V will be placed on EX. Important note: the controller must be hooked up to it's respective PZT in order to be properly tested.

It's been a few days since either activity has been mentioned, therefore:

ITMx cartridge cleanroom has been cleared for access and the suspension is clamped, shielded, and bagged in prep for the flight likely to happen ~Monday.  We still wait for elliptical baffle work to conclude before parking the ITMx cartridge in the baffle's alignment line-of-sight.

ETMx in-chamber alignment is still on hold after a stack up of longitudinal errors was found late last week.  Two possible paths forward of where to take up the residual error (14mm) are under consideration.

In preperation for trying out some HEPI to ISI tilt decoupling I've modified Hugo's controller in the X direction to be more like what we have decided will be the "standard" HEPI-PS controller

It now has a close to 5Hz UUG and some what less gain peaking

Black and Pink are the old Open loop and Suppression

Red and Blue are the current Open Loop and Suppression

  Hopefully the rest of the DOFs will get upgraded soon.

Looking at the counts since the dust monitor software change (alog 8055), I noticed that some of these channels have started picking up 'noise'.

It appears on the .3 micron counts in the first attached plot for the following channels:

Ch 1: H0:PEM-CS_DUST_DR1_300NM_PCF
Ch 3: H0:PEM-CS_DUST_LAB2_300NM_PCF
Ch 5: H0:PEM-CS_DUST_LVEA4_300NM_PCF
Ch 8: H0:PEM-CS_DUST_LVEA16_300NM_PCF
Ch 9: H0:PEM-EX_DUST_VEA1_300NM_PCF

It appears on both the .3 micron and .5 micron counts in the other three attached plots.

While the install work is taking place along the X-manifold I have de-energized the optical lever power supplies for HAM2, HAM3, Beamsplitter and ITMY (okayed by Thomas Vo).

(Daniel, Alexa)

We have installed all the RF cables on the field and remote racks at EX for ISC. We still need to intall the RF cables that go from the field rack onto the table. There are also some short cables missing:

1 x DB37 - 6 ft (for RF Amp concentrator)

2 x BD25 - 5 ft (for RF Amp concentrator to RF oscillators)

1 x DB15 - 3 ft (to phase frequency discrimantor from port 1 of demod concentrator)

1 x DB14 - 5 ft (to demod from port 2 of demod concentrator)

1 x DB37 - 3 ft (for timing concentrator; to replace a 5ft cable)

There is also a long cable missing from the RF Pre Amplifier (D1201294) to the concentrator.

We also noticed that the 71 MHz RF Oscillator did not seem to be properly tuned.