Jason and Travis set the IAS PLX in the HAM3 South spool.  After coarsely adjusting yaw and pitch of the reflected beam back into the PLX, we are now fine tuning those DOFs via the pushers and the pitch masses.

Today, with the approval of the resident IO rep Chris, I swapped in the MC3 top mass blade tip EQ stops (a necessary retrofit with an ECR (has a number, yada yada).  To date, the MC1 and MC2 still need them.  Other HSTSes have the correct screw.  These are on the to-do list for next week.

Kiwamu had a DC Power Supply box (D1002932) he wanted installed inside the IOT2L.  After ordering a few parts, I went about installing the box; this required installing support brackets.  These support brackets required moving the entire internal cable tray a few inches toward the doors (which isn't trivial with all the cables cable-tied down).  After a bit of grief and sweat, the box is installed and ready to go. 

Pictures for IOT2L are in ResourceSpace here.

15:08 DAQ restart to add back the EX DUST monitor channels.

All front-end computers were restarted at the end Y after someone tripped over the power cord for the I/O chassis power supply, AGAIN.

crashed last night

Ryan Fisher, Jeff Kissel, Stefan Ballmer

We started added the epics bit label strings to the ODC medm screen. Ultimately these strings are intended to be initialized my the front end model to keep track of long-term ODC bit assignment changes. For now we populated them by hand (see Ryan's elog).

So far we modified the medm screens for the BSCISI (BSCISI/ISI_CUST_CHAMBER_ODC.adl) and added the SUS quads (SUS_CUST_QUAD_ODC.adl). For the quads we modified the OVERVIEW screen to include a button to the ODC screen, and reduced the number of ODC bit indicators to the bits 0 to 12 that are currently used.

Many more screens need to be done: SUS triples and auxiliaries, HAMISI and HEPI.

Ryan Fisher, Stefan Ballmer

We have set the EPICS records for the labels that describe the ODC bits for the SUS and ISI models currently running in H1.*  The labels provide a short description of what every bit in each ODC channel represents, for each ODC channel.  The higher order bits in the ODC channels that do not have labels are currently unused, but may be used in the future.

These records were set using scripts located in /ligo/home/ryan.fisher, and attached to this entry.  

* Excluding H1:SUS-TMSY_ODC_BIT* for now.

Attached are plots of dust counts > .3 microns and > .5 microns in particles per cubic foot requested from March 13 00:00 UTC to March 14 00:00 UTC. Also attached are plots of the modes to show when they were running/acquiring data.

Data was taken from h1nds1.
T0=13-03-13-00-00-00; Length=86400 (s)
1440.0 minutes of trend displayed

'No data output' error on > .3 micron plots.

I forgot that the dust monitor at end X had been removed from the edcu, so the data has not been saved since I turned it back on this morning.

[Deepak K., Rodica M., Chris M.]

Tasks Accomplished:
* Realigned MC Refl beam through the periscopes.  It was off center on some of the baffles by 1/2 a beam diameter.
* Tweaked the alignment of the beam through the Faraday. It was reasonably well aligned already, but we made a small adjustment to IM1.
* Implemented Rodica's brilliant idea to reroute the MC Refl beam to overlap with the main beam.  We did so by using two eLIGO steering mirrors and injecting at MC3 (see pictures).  This gives us the full ~180 mW of power downstream of the IMC to align auxiliary beams.
* Installed the HWP in the rerouted MC Refl beam to correct the funky polarization.

Notes:
* The first hard aperture(HA1) needs to be recentered after the clamp issue is fixed.  (It has a large dog clamp).
* The AOEs are missing their second SiC baffles still.  Recheck the centering after the baffle is installed.  
* We removed MC3 AR Baffle and placed it in front of MC3.
* We borrowed the HWP from the main beam line to correct the polarization of the rerouted MC Refl beam.

Mick (Apollo), Thomas V

We've completed building the boxes per E1200667-V4.  No mishaps, picture attached.

• Longitudinal Error: +0.3 mm (North)
  • Tolerance: ±3 mm
• Lateral Error: -0.1 mm (East)
  • Tolerance: ±1 mm
• Vertical Error: -0.02 mm (low)
  • Tolerance: ±1 mm
• Pitch Error: 45 µrad up
  • Tolerance: ±100 µrad
  • Target: 0.0 µrad
  • Actual Pitch: 45 µrad up
• Yaw Error: 48 µrad CW
  • Tolerance: ±100 µrad
  • Target: +8.092 mrad (CW w.r.t. x-axis)
  • Actual Yaw: +8.14 mrad (CW w.r.t. x-axis)

• Longitudinal Error: +2.8 mm (North)
  • Tolerance: ±3 mm
• Lateral Error: -0.5 mm (East)
  • Tolerance: ±3mm
• Vertical Error: +2.4 mm (high)
  • Tolerance: ±3 mm

• Longitudinal Error: -4.9 mm (South)
  • Tolerance: ±3 mm
• Lateral Error: -1.56 mm (East)
  • Tolerance: ±2 mm

Tomorrow we will measure the PRM vertical position error, make any shifts of the PRM that are required, and then move on to PR3 pitch/yaw alignment.

- 12:00 water sampling

- no safety meeting

- Patrick turn on DUST EX monitor

- PSL ENV alarms were on, and still on, for several days

- EY laser hazard

- Rick gave T.K. Machine's crew a tour
    13:30 LSB
    15:00 - 15:20 LVEA
    15:25 roof

- Dave and me with Ski consent, changed the MAX value of the channels
    H0:FMC-MX_AH_COOLTEMP_1_DEGF
    H0:FMC-MX_AH_COOLTEMP_2_DEGF
from 75F to 80F

- 16:30 LVEA transition to laser hazard

Today I vented X-end -> An Apollo crew (Mark L., Chris, Scott) removed BSC5's dome and found an insect on the underside of the outer O-ring at the exact point that I had marked as the leak location -> They lifted up this portion of the outer O-ring +/- 1' in either direction, removed the offending insect and wiped down the O-ring with an alcohol wipe -> During an overall visual inspection they also noticed a cut "sliver" of O-ring at a non-leaking location but this cut was not on the portion of the O-ring that comes in contact with the sealing surface and they left it be -> I pumped down the annulus volume following the dome's re-installation and helium leak tested only the area addressed -> No response (1 x 10-8 torr*l/sec baseline) -> This is encouraging but inconclusive as new leaks may have resulted from the dome's removal/installation -> I'll know more tomorrow.

J. Kissel

With the TMS in it's current rubbing state, it's difficult to properly model any damping loop design based on the measured transfer functions -- and as you know, we don't yet have a dynamical model that we trust to design on instead. But, I did so anyways, and discovered that the loops really just needed their gains adjusted. Some degrees of freedom had no open loop gain above unity, others had way way way to much open loop gain, and were just down-right unstable.

Here're the changes to the damping loops:
(1) Included a "from_um" or "from_urad," which takes out the "to_um" calibration of the sensors, so we can stick with the otherwise-normalized filter design. These are in FM5, like every other type of the suspension (which is usually poorly named "norm").
(2) Turned the ELF10 elliptic filter back on, as was the original design intent. 
(3) Changed the gains from [L,T,V,R,P,Y] = [-20.0; -7.0; -10.0; -20.0; -5.0; -5.0] to [-20.0; -10.0; -20.0; -0.05; -0.5; -0.1]. (These new gains are also now roughly consistent with the ratios between DC magnitude (i.e. the stiffness) what's seen in the transfer functions).

I attach the modeled open loop gain and suppression for each degree of freedom with the new gains I've installed. Note, I intentionally removed the phase subplot because the data is so noisy / incoherent, I couldn't trust anything regarding phase margins, and flew by the seat of the modeled closed loop gain and suppression magnitude to help me determine where the stability regions lie.

If you're interested in using the scripts to make these plots in the future, they live in
${SusSVN}/sus/trunk/TMTS/Common/FilterDesign/
design_damping_L_TMTS_20130313.m
design_damping_P_TMTS_20130313.m
design_damping_R_TMTS_20130313.m
design_damping_T_TMTS_20130313.m
design_damping_V_TMTS_20130313.m
design_damping_Y_TMTS_20130313.m

[Paul, Kiwamu, Keita, Dick, Rodica]

Today we measured the mode cleaner cavity length by modulating the EOM at 45 MHz and doing a sweep around this frequency. We measured the spectrum using an HP 43968 Spectrum Analyzer. The maximum source power was 19 dBm from a Mini-Circuits RF amplifyier with gain 19 dB. The bandwidth for the highest zoom on the peak was 300 Hz.

The frequency of the dip in the middle should correspond to the 5th FSR away from the carrier resonance. The calculated length is 9.09918 MHz +/-  100 Hz, only 291 Hz away from the design value of 9,099,471 Hz. This is equivalent to 1.05 mm difference from the design length.

We tried a full sweep over one FSR but we realized that the modulation away from resonance would be too small to give us any useful results, so we focused on the 45 MHz resonant peak. Attached is a plot of the data over a full FSR, that also shows a peak corresponding to the non-resonant polarization, and few other peaks possibly due to higer order modes.

Similar measurements at LLO are described in alog 4702.