I have enabled multicast routing in the core switch to allow multicast streams to be routed to the ops network from the auxilliary network (between VLAN 20 and 106) - this is to support the upcoming digital video system. The Loopback0 interface has been created in the switch to act as the PIM RP[1] for the CDS network, with address 172.17.2.1/32. Interfaces Vlan20 and Vlan106 are configured to use 'ip pim sparse-dense-mode'. No other VLANS are currently configured to route multicast traffic. [1] Protocol Independent Multicast Rendezvous Point
The feedforward control is used as a complement of the feedback control mainly to reduce the motion around 10Hz (created by the HEPI piers). The L4Cs installed in the HEPI boots are used to feed the stage 1 actuators.
In https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=6768, the feedforward filters were set-up using transfer functions measured while the ISI was damped. I evaluated how the ideal feedforward filters would change if the ISI was “feedback controlled”. I compared the ideal feedforward filters obtained in the two configurations: Damped vs feedback controlled (attachment shows the feedforward filter for the X direction).
Above 1Hz (super sensor dominated by the inertial sensor), the two filters are almost identical. The ground path and the force path are modified in the same manner by the feedback control.
Regarding these results, it doesn’t seem essential to measure transfer functions with the ISI “feedback controlled” to set the feedforward controllers.
Apollo removing door bolts on HAM5/6 Greg and Apollo craning optics tables into East Bay enclosure Michael & Pablo in H2-PSL enclosure Kyle replacing annulus ion pump on GV1 Betsy working around ITM-X Test Stand
Two large clean rooms were turned off at the request of the HIFO crew.
HAM1,2 cleanroom and HAM3 cleanroom.
Time of occurrence ~ 14:06 local time.
The two small clean rooms in the same area are on temporary power and may be turned off for short periods ~1 or 2 hours. They are currently ON.
[Stefan, Chris, Kiwamu]
We spent some time today at ISCT1 to locate the forest-type noise at around 1 kHz which we saw in the ALS CARM signal (see alog 6900) and also did some hardware works.
We did find a couple of suspicious optics on the table although we are still studying how they pollute the ALS CARM signal. We have stick foam in the mount of every reflective optic on the table to help their mechanical damping ability. The work continues.
Noise hunting at ISCT1
To do noise hunting on ISCT1 we did a speaker technique --- we hooked up a small speaker at the output of the common mode servo while keeping the green beatnote within the PLL's readout range by ezcaservo acting on the ALS_COMM VCO. The ALS CARM noise sounded mostly high frequency-ish although we didn't confirm how exactly high the frequency was. Then we bought the speaker close to every optic to see if they resonate due to the acoustic (positive) feedback at exactly the same frequency as that of the ALS CARM noise. We found a couple of optics which do resonate with the CARM sound. They are :
We are suspicious about these optics. They may be the ones introducing the forest noise at around 1 kHz. We have stick foam in the mount of every reflective optic to damp unwanted mechanical vibration. We will take another noise spectrum tomorrow to see how this improves it.
SHG mystery
There has been a mystery that somehow the SHG efficiency dropped by a factor of 4 or so at some point (approximately from 0.5 mW to 0.1 mW level) and it didn't come back to the high value. As a part of the ISCT1 works we inspected the doubling oven to see if there is an obvious clipping or something stupid. However we didn't find a thing. We did the following things:
After all these works we measured the SHG power again and it was measured to be 0.140 uW which is still low compared with the past. It is still unclear what happened and we are not quite sure how this can be related to the ALS CARM noise.
REFL alignment
To evaluate the residual noise in the PSL frequency we needed a length sensor of the Y arm, namely the interferometer reflection (REFL) RFPD. We started rearranging the optics to guide the REFL beam to the RFPD. The work is ongoing. Currently the REFL beam is dumped. To prevent a damage on the RFPD due to an accidental power increment we need the trigger function of the mechanical shutter working.
As for the SHG power measurement,the SHG power is consistent with the monitor PD signal. I think the low power at 0.1 mW level is real. On the other hand I was unable to measure the incident 1064 nm power on the doubling crystal --- the Ophir power meter didn't give us a reasonable number when the filter was put on the head. I tried to measure the power without the filer but this simply saturates the signal, indicating the power is more than 100 mW. I will try measuring this power with another power meter.
A video to show how we did the ISCT1 noise hunting:
Bram clarified that 'pendulum length' in P1100090 was exclusive of dpitch, whereas yesterday's version assumed it was equivalent to tl0 which includes dpitch.
Preferred version is now Mathematica 20130628TipTilt or Matlab httpopt_test.m r5013 of 6/28/13. Wiki page is
https://awiki.ligo-wa.caltech.edu/aLIGO/Suspensions/OpsManual/HTTS/Models/20130628TipTilt
Attached are plots of dust counts requested from 5 PM June 26 to 5 PM June 27.
Attached are plots of dust counts requested from 5 PM June 25 to 5 PM June 26.
Attached are plots of dust counts requested from 5 PM June 24 to 5 PM June 25.
Attached are plots of dust counts requested from 5 PM June 23 to 5 PM June 24.
There is a camera on the IR transmission on ISCETY, and the PD is aligned. I turned the periscope by 90 degrees, and removed two unlabeled TCS optics that were on the periscope. (part of the Hartman reference path). There are still the other optics from that path that need to be removed, and a better beam dump is needed. I took the power for the camera from the Green refl camera (the second connector on that cable is a different connector) Filiberto connected the signal to the blue cable on CB7-050-0005, which is now connected to channel B on the lower of the monitors in the front of the control room. It would be good to add a longer focal length lens and an ND filter. The reason for adding the camera was that this morning we were locking on a first order mode, but could not tell from the control room.
8:50 Pablo and Colin to H2 PSL laser enclosure Corey informed me that he, Virginio and Keita would be working on and off in the end X transmon lab 10:00 Michael R. to H2 PSL laser enclosure 10:54 electric man-lift pickup well sampling CP6 filled Dave rebooted the DAQ for Vincent 1:29 Pablo, Colin, Michael R. and Rick going into H2 PSL laser enclosure Cyrus took down a network switch, which took down the H1 PSL Beckhoff, H1 PSL video cameras and communication to the dust monitor in the diode room. Switch was rebooted and restored. all left the H2 PSL laser enclosure
I believe there was also talk of tightening bolts on a spool piece and installing HEPI electronics at end X in the morning meeting.
Cyrus, Dave, Jim Attached a new SSD RAID to h1fw0. This RAID is to be used for storage of raw minute data that was formerly written to the SATAboy hard drive array in LDAS. Reconfigured the h1fw0 daqd to write raw minute data to /trend/minute_raw instead of /frames/trend/minute_raw. Reconfigured h1nds0 to read raw minute data from both /frames/trend/minute_raw and /trend/minute_raw. The raw minute data in /frames/trend/minute_raw is now in two subdirectories of /frames/trend/minute_raw, and is considered archive data while still being available for viewing via h1nds0. Note that frame files written to /frames/full, /frames/trend/minute, and /frames/trend/second are not affected by this change. The benefit of this change is a remarkable decrease in the amount of time required to write raw minute data, allowing it to be written much more often. Hopefully this will help make h1fw0 more stable, as the daqd process was having difficulty writing files in the time allocated for the task. The downside is the raw minute data will have to be copied to the archive as the SSD RAID fills up, which is a maintenance task to be performed a few times per year.
Valved-out YBM turbo @ 1600 hrs. -> 4.0 x 10-7 torr*l/sec indicated
(Betsy W, Gerardo M, Gerardo A. M)
Prism was removed today, finally. It took about 7 days of the common process of soaking the prism joint in acetone, then working on the joint by hand with a razor blade along with some acetone as a lubricant.
2 photos attached, one is where the prism used to be, second photo is the removed specimen.
The prism will be reglued (into a new position that corrects for the ear placement error) during the early part of the week of July 8th. The PUM will then be packed up and sent to LLO for use in their ETMx monolithic suspension.
This timing for regluing depends on our having resolved the likely cause of the PUM crack and how to avoid it happening again during future welds.