Today, on BSC-ISIs:
- Calibration filters were reinstalled (the minus gain of the HEPI L4C is introduced in the calibration filter)
- The feedforward controllers were retuned/reinstalled on the 3 BSC-ISIs (The gain is 1 when engaged)
- The sensor correction filters were retuned/reinstalled on the 3 BSC-ISIs

At 18h50 PT:
- HEPI BSC6 and BSC2 are controlled in position
- ISI BSC6 and ISI BSC1 are controlled with
    - Feedforward ST0->ST1
    - Damping
    - Feedback Level 3
    - Sensor correction Stage 1 X,Y,Z
    - Sensor correction Stage 2 Y

ISI-BSC2 controlled with
    - Feedforward ST0->ST1
    - Damping

The DAQ went 10 years into the future for about 10 minutes this morning due to an IRIG-B error. Unfortunately this bogus time was then written into the raw minute trends. You will find if you ask for minute trend data which spans this time (approx 9:22 - 9:50 local time this morning) you will only get data up to 09:22. To get the rest of the data you will have to ask a second time for data from 09:50 onwards.

We stopped writing raw minute trends for a short while this afternoon and switched them to a new disk location. This will allow us to fix the now static broken files, most probably tomorrow.

Mark Barton, Gerardo Moreno, Arnaud Pele, Scott Shankle, Mike Vargas, Thomas Vo

Magnets were added to the plates.
B&K Testing performed; results are being reviewed.
Purchased ~20 18-8 SSTL 1/3-13 x 1.25" and 1.5" Flat Head Cap Screws (Made in USA) locally. Additional were Made in INDIA, but will not be used. Screws will be cut to size and Class A cleaned tomorrow.

Alignment Tooling and Baffle/Ring Spacer Bar have been Class B cleaned.
Forceps need to be shaved and re-cleaned.

We will begin working Arm Cavity Baffle for BSC9 and return to Manifold Cryopump baffle for ETMx on Tuesday (7/23)

Kyle
HAM1 currently vented but not nominally being purged (HIFO-Y noise), HAM2 under vacuum -> Closed HAM1 ion pump gate valve -> Opened HAM1 purge valve and exhaust of HAM1 turbo resulting in flow from bottom to top of HAM1 -> Returned to as found state after 90 minutes (purge valve closed, turbo exhaust capped) -> We are trying to systematically eliminate all adjacent external-to-vacuum potential helium reservoirs.  

Also, verified YBM leak detector calibration using external calibrated leak -> 5 x 10-8 torr*L/sec leak registered as 7 x 10-8 torr*L/sec value on detector -> Not a significant discrepancy for our current purposes -> left stored calibration factor alone

DAQ Re-start this morning at 9:22am(Dave & Jim)

Kyle working on HAM1 purge air flow, he finished before lunch

HAM6 cable running (Filiberto & Interns)

Running cable & bending conduit around HAM1 started this morning (Mark/Ed)

EY Field Rack Transfer Functions (Alexa/Daniel)

Prepping for Oplev work (Thomas)

Alarms in Labs--probably should raise alarm levels to 500 counts?

Stefan working on MC Electronics

Vincent restarted the DAQ for his work in the afternoon.

Dave and Jim

Second try to fix the dataValid=1 flag in the frame.

This morning we tried a version of the DAQ code which was tested successfully on the DTS yesterday afternoon. Unfortunately on the H1 DAQ the IRIG-B date was incorrectly read, putting the data concentrator 10 years and 5 days into the future. This then marked all the FE's as having bad timing.

We immediately reverted back to the original code. The whole excercise took about 15 minutes.

We are checking the configuration differences between L1, H1 and X1 to see why this would happen. Early result, the IRIG-B drivers between all three are definitely different.

(Corey, Keita)

Telescope Assembly

Now that we had a new set of machined Side Clamps (machined by Tyler and Class-A-ed over the weekend), we installed these parts on the Telescope Assy, and then installed the Primary Mirror.

Telescope Rough Alignment

With all Mirrors installed on the Telescope (the F1 [6"] Mirror is an IAS Alignment Mirror we are "iffy" on, we're waiting for some recently-ordered 6" Mirrors to see if they have a better coating), we started rough alignment of the Telescope.  This was done with autocollimators at the input and output of the Telescope and per Keita's alignment document (T1100603).  Next we were going to move to a more fine alignment with the IR Laser, but we discovered the 8" Alignment Mirror we were going to use had a frosted back surface, and this would not be useable for shooting the Autocollimator through it.  So, this is where we stopped for the afternoon.  Today (Wed), Keita found a gold-coated mirror to use for this alignment and will proceed from here.

SUS Cables Run

I grabbed two cables which run from the "roof feedthru" to the Test Stand at EY, and installed them at EX.

[Stefan, Alexa, Kiwamu]

 The IMC wasn't locking today. We found that this was because the demodulation phase changed.

The guilty RF cable:

 We took a look at the demod phase of not only the length diode but also both WFSs and found that the amount of rotation they got were identical. So we started suspecting something common, for example the cable length of the modulator. Eventually Stefan found that wiggling the N-connector of an RF cable rotates the demod phases by tens of degrees. This is the 4th output of the 24 MHz RF amplifier in the R1 rack at the field. In fact this is the one supplying the EOM with the 24 MHz modulation. This rotation happens more or less in a random fashion but the amount of rotation was relatively repeatable --- we could reproduce a couple of certain conditions with a certain demod phase by wiggling around the connector.

 We tightened the N-connector and it seems that the problem was solved. Additionally we briefly tested it by wiggling the connector again but we didn't see any more rotations.

Demod phase need to be adjusted again :

 Then an issue we got after fixing the RF cable is that all the demod phases were consistently off. Probably this may indicate that the we had been in a particular, but a different condition for a long time due to the loose connection at the RF connector. In any case we need to adjust all the demod phases associated with the IMC i.e. length diode and two WFSs.

Demod phase of the Length diode readjusted:

 We readjusted the demod phase of the length diode as a first recovery step. The new optimum setting, where the I signal is maximized, is

• 28.625 nsec = 1/8 + 1/2 + 4 + 8 + 16 nsec
• (This is set by the hardware switches at the front panel of the delay line phase adjuster)

Comparing it with the past setting of 14.4375 nsec (see alog 6282) we found that the amount of rotation we newly introduced is 123 degrees with the modulation frequency at 24078360 Hz. This resulted in a sign flip in the error signal. So we had to flip the control sign to properly lock the IMC.

Next step : readjustment of WFS demod phases :

 Apparently we have to do the same correction for all segments of the WFSs. Unlike the length diode the demod phases can be adjusted in the digital land. Since we now know that we need to rotate everyone by 123 degrees from whatever previous phase, correcting the demod phases should be relatively straightforward --- we simply punch in some numbers in the digital system. Of course we have to pay attention to the sign flip.

Just before the laser went dark, we discovered that the demod phases of both IMC length and WFS diodes had moved significantly, with all the signal ending up in the Q phase.

We found a bad connector on spigot 4 of the RF distribution panel, going to the EOM. Wriggling te cable resulted in ~30deg of phase shift.

The connector should be replaced tomorrow.

We reinstalled the primary mirror with re-machined clamp parts, and the new clamp parts worked well.

We're still waiting for the procedure to set the spring tension of the clamps right, but in the mean time we decided that 1/4 revolutions of the clamp screws after finger-tight felt about right.

Anyway, from there on we quickly set two auto collimators up, and roughly aligned the path correctly as per the procedure. 

Next we'll tune the telescope using a laser beam and mode master. That'll be about a day of setup and three days of going back and forth.

The PSL got down at around 5:50 PM in PDT due to errors in the diode and crystal chillers according to the status medm screen.

Gerardo Moreno, Scott Shankle and Mike Vargas

Attached the Face Plates. One screw on the Right Face Plate could not be attached (pic 2); hole does not line up. One screw on the Left Face Plate could not be attached (pic 1); holes do not line up.
Attached the Balance Weights and the Tongue Depressors released very nicely (pics 3 and 4).
The baffle was balanced using a Plumb Bob (pic 5).

The height needs to be checked. The Assembly Fixture and Crane will be needed if height needs to be changed.

Observations - the Face Plates are very flimsy and rattle a lot. They are tied to the baffle on the outer circumference only.

SLC crew - EX working on Cryopump Baffle

CDS crew - Rebuild of data concentrator - did not work, re-stored to previous working version

Filaberto- Running PEM Cables

Pcal - Working in the H2 PSL Enclosure

Robert - Disconnect dust monitors at ISCT1

Prax Air - Refill CP2

Hugo and Jim W - Taking overnight transfer functions starting at 9 PM PT

Jonathan Hanks - Reconfigure router on GC

Filaberto and crew - Run HAM 5/6 cabling to feed through(s)

Apollo - Install feed through(s) on HAM5/6 and install 16" conflat with new gasket on HAM6

Launched a delayed overnight measurement on HAM3-ISI, with the help of JimW. 

Measurement should start around 9.50pm PCT. Horizontal isolation loops will be turned OFF then. Only vertical isolation loops will be left ON for the duration of the measurement.

Measurement will be finished by 8.30am PCT. Isolation loops will be turned back ON by then.

Installed new framecpp-1.19.24-p1 package, obtained from Livingston.

Built new daqd from advLigoRTS/trunk, installed on x1dc0, x1nds1, x1fw1.

Restarted daqd on the three systems, ran tests to verify that the dataValid flag works properly.  dataValid is definitely non-zero for bad channels, and 0 for good channels.  Note that the value of dataValid is the same as the DAQ status, which can be various values depending on the cause of the bad data.

Plot shows 80 days of pumping at the vertex.