Displaying reports 77841-77860 of 86384.Go to page Start 3889 3890 3891 3892 3893 3894 3895 3896 3897 End
Reports until 20:39, Wednesday 04 December 2013
H1 SUS (INS)
jeffrey.kissel@LIGO.ORG - posted 20:39, Wednesday 04 December 2013 (8822)
H1 SUS ETMX Chamber Closeout TFs -- Looks Good!
J. Kissel

After chamber closeout, and subsequent close up, I've gathered a set of TFs for H1 SUS ETMX. I attach the results, all looks quite well, and ready for pump-down! I've left the ISI ETMX undamped with the MASTERSWITCH ON, and H1 SUS ETMX and H1 SUS TMSX are damped.

Of interesting note -- checkout the P to P transfer function comparison between the main chains for H1 ETMX, H1/H2 ETMY, and L1 ETMX, on pg 5 of allquads_2013-12-04_Phase3a_H1SUSETMX_ChamberCloseout_ALL_ZOOMED_TFs.pdf. It appears the 2nd Pitch mode (modeled to be at 1.31 [Hz]), whose motion is the top-three masses pitching in concert, differentially with the test mass, is different from the model, and different between these three examples. The one just measured here, H1 ETMX, seems to have the lowest frequency mode of the three, but all are within 6% of the model (-5.34%, 1.37%, 2.90%, respectively). Definitely not a show stopper, but something to consider when designing high-performance damping filters for this DOF -- the gain bump for this mode will have to be reasonably wide if we wanna use the same filter for every ETM.

------------------------
Details:

Data was taken with DTT, using the following templates,
${SusSVN}/sus/trunk/QUAD/H1/ETMX/SAGM0/Data/
2013-12-04_0146_H1SUSETMX_M0_Mono_WhiteNoise_L_0p01to50Hz.xml
2013-12-04_0146_H1SUSETMX_M0_Mono_WhiteNoise_P_0p01to50Hz.xml
2013-12-04_0146_H1SUSETMX_M0_Mono_WhiteNoise_R_0p01to50Hz.xml
2013-12-04_0146_H1SUSETMX_M0_Mono_WhiteNoise_T_0p01to50Hz.xml
2013-12-04_0146_H1SUSETMX_M0_Mono_WhiteNoise_V_0p01to50Hz.xml
2013-12-04_0146_H1SUSETMX_M0_Mono_WhiteNoise_Y_0p01to50Hz.xml

${SusSVN}/sus/trunk/QUAD/H1/ETMX/SAGR0/Data/
2013-12-05_0152_H1SUSETMX_R0_WhiteNoise_L_0p01to50Hz.xml
2013-12-05_0152_H1SUSETMX_R0_WhiteNoise_P_0p01to50Hz.xml
2013-12-05_0152_H1SUSETMX_R0_WhiteNoise_R_0p01to50Hz.xml
2013-12-05_0152_H1SUSETMX_R0_WhiteNoise_T_0p01to50Hz.xml
2013-12-05_0152_H1SUSETMX_R0_WhiteNoise_V_0p01to50Hz.xml
2013-12-05_0152_H1SUSETMX_R0_WhiteNoise_Y_0p01to50Hz.xml

Data was exported, processed, saved, using the usual tools,
${SusSVN}/sus/trunk/QUAD/Common/MatlabTools/
plotquad_dtttfs.m
plotallquad_tfs.m
the latter of which has had its measurement list updated, and is now committed to the repo as with all the above mentioned data and plots.
Non-image files attached to this report
H1 SEI (SEI)
hugo.paris@LIGO.ORG - posted 18:29, Wednesday 04 December 2013 (8820)
BSC-ETMX - Overnight TF

Post closeout transfer functions will be running on BSC-ETMX, once SUS is done, starting from 9.30 PCT tonight.

LHO General
bubba.gateley@LIGO.ORG - posted 18:10, Wednesday 04 December 2013 (8819)
Apollo crew
Clean room was moved from BSC 6 to BSC 10, work platform disassembled at BSC 6 and reassembled around BSC 10.
Clean room then moved back over BSC 10.
E module relocated to east side of test stand clean room (only 3 bolts per leg) and in position. TIGHT FIT
West door installed on BSC 9 and bolts torqued. Only 4 bolts in dome and east door, remainder to be installed and torqued tomorrow.
H1 SUS (SEI)
betsy.weaver@LIGO.ORG - posted 17:19, Wednesday 04 December 2013 (8818)
BSC 9 H1-ETMx Chamber closeout

After the ACB crew finished this morning, Travis, Jim and I finished the rest of the closeout work:

- Reapplied FC to ETMx-HR thin alignment windows

- Set and secured all 72 ETMx SUS EQ stops

- Set 4 top stage BOSEMs to counter upcoming buoyancy shift under vac (Left, Right BOSEMs on M0 and R0)

- Removed the ACB locking bracket and 4 screws

- Performed chamber inspection for tools, FC on viewports, tokk a few pix, etc.

- Wiped and wiped and wiped some SUS, ACB, TMS surfaces and the floor many times ("good" IPA + alpha 10 wipes)

- Added a witness plate to the vertical holder mounted off the bottom of the front of the QUAD lower structure (LS)

- Added a 1" witness optic + PEEK holder to side of the QUAD LS

- Pulled the FC from the ETMx-HR and blew with ~10psi Top Gun N2 and inspected

- Blew the TMS telescope mirrors - didn't look great, but lots of stuff lifted with the blowing

- Unlocked the ISI

- Damped ETMx to make sure it seemed healthy

- Placed 2 witness plates (not in holders since I didn't have any with me), one directly under the QUAD, one under the front of ACB towards the tube (these should be pulled asap at next vent!)

- Left Apollo to toss the door on

H1 TCS (TCS)
thomas.vo@LIGO.ORG - posted 16:40, Wednesday 04 December 2013 - last comment - 09:38, Friday 06 December 2013(8816)
TCS ITMY Ring Heater
Steps taken to commission the ITMY ring heater pair:
- Updated to the recently committed Beckhoff code that Joe B and Adam M worked on yesterday.
- Added the calibration values that Aidan B had recommended for running the ring heaters.
- Opened up a strip tool to monitor the vacuum pressure with the closest gauge (HVE-LY:Y1_120BTORR)
- Turned the ring heaters on to low power (~.01 Watts) to make sure that the channels were working properly
- Increased the power to 1 Watt for a 4 hour period starting at 12:00PM Pacific Time, keeping an eye on the pressure gauge previously mentioned.


Upper:
Requested Power = 1.00 Watts
Measured Voltage = 5.94 Volts
Measured Current = 0.17 Amps 
Calculated Power = .99 Watts
Calculated Resistance = 34.94 Ohms

Lower:
Requested Power = 1.00 Watts
Measured Voltage = 5.92 Volts
Measured Current = 0.16 Amps 
Calculated Power = .98 Watts
Calculated Resistance = 37.0 Ohms

A four hour trend of the pressure gauge and ring heater settings is attached.

A quick, back-of-the-envelope calculations shows that the ring heaters are working properly. The next step for measuring the thermal lensing would be to measure the beam diameter of a single reflection off of the back of ITMX independently and then changing the radius of curvature of ITMY using the ring heater to match. This requires looking at the REFL beam either in the HAM1 chamber or on the ISCT1 table, depending on how much power we are able to get out of REFL.  The Thorlabs beam profile we have on site requires a minimum of ~1e-5 Watts of incident beam power to function.
Images attached to this report
Comments related to this report
mindy.jacobson@LIGO.ORG - 09:38, Friday 06 December 2013 (8859)AOS, TCS
NOTE:
This pair of upper and lower ring heater segments is due to be replaced, per "Bug255"
https://services.ligo-wa.caltech.edu/integrationissues/show_bug.cgi?id=255

See, also, T1300463
LHO General
corey.gray@LIGO.ORG - posted 16:07, Wednesday 04 December 2013 (8810)
Ops DAY Summary

Day's Activities:

Swapping out PSL Chasis (Filiberto)

Greg craning dewar over Beam Tube in LVEA

Move ITMy Lower Structure to LVEA (Jeff/Andres)

Tumbleweed baling on X-arm

Lots of Apollo activity at EY (moving cleanrooms, platforms, E-module; installing BSC6 door, installing hard covers on Spool)

PSL work by Kiwamu (investigating mysterious RF jump by unplugging EOM cable); external shutter was also closed.  EOM was fixed in situ

PSL Shutter was replaced (Gerardo, Joe D.)

ACB work at EX (Gerardo/Mitch)

SUS work at EX (Betsy/Travis)

Had a couple of IOP SUS Watchdog INVALID alarms during shift; not really sure of the cause (also popped up window stating:  "Channel Access Exception...")

PSL Checks:

LHO VE
kyle.ryan@LIGO.ORG - posted 15:59, Wednesday 04 December 2013 (8817)
Removed aux. pump cart from BSC3, began pumping GV20 annulus


			
			
H1 AOS
mitchell.robinson@LIGO.ORG - posted 12:17, Wednesday 04 December 2013 (8815)
ETM-x ACB
Gerardo M, Mitchell R

The ETM-x Arm Cavity Baffle has been dog clamped. All class B tools and hardware has been removed from chamber. The ACB is still locked.
H1 INS
jim.warner@LIGO.ORG - posted 11:24, Wednesday 04 December 2013 (8812)
BSC6 Cartridge De-install Complete

Bubba, Randy, Scott, Tyler, Ed, Mark, Corey, Jim

Yesterday, we completed the removal of the BSC6 cartridge. The assembly is now resting comfortably on the test-stand, 180 degrees to it's final in-chamber position (necessary for cleanroom clearances). Both suspensions are covered, and the ISI has 3 separate covers. No unusual difficulties beyond some misplaced hardware, but Apollo took an early lunch so I could scramble and find it.

H1 IOO
stefan.ballmer@LIGO.ORG - posted 11:05, Wednesday 04 December 2013 - last comment - 11:44, Wednesday 04 December 2013(8811)
EOM RF return loss measurement after the latest phase jump
Kiwamu, Stefan

Attached is a new RF return loss measurement for the EOM cable taken at the PSL rack end. This was taken after the latest RF phase jump.
As before, the marker labeled 24.08MHz is at the actual IMC modulation frequency of 24.078360MHz.

Compare this to alog 7959 (before RF jump).
Images attached to this report
Comments related to this report
stefan.ballmer@LIGO.ORG - 11:25, Wednesday 04 December 2013 (8813)
Kiwamu repeated the measurement directly at the EOM, and he was able to jump between the two setting by pushing at the EOM's Sam connector.

Conclusion: a bad connector at the EOM is responsible for our phase jumps.

rich.abbott@LIGO.ORG - 11:44, Wednesday 04 December 2013 (8814)
The resonant frequency of the notch appears to have changed such that one could reasonably account for the phase shift.  The million dollar question is how?  Either the tuning has bistable states (such that a mechanical tuning screw clicks between two states) or the external loading changes due to a bad connection to the EOM.  It seems the latter has just been identified by Stefan...
H1 IOO
kiwamu.izumi@LIGO.ORG - posted 06:07, Wednesday 04 December 2013 (8807)
further alignment of IMC

Sheila and Kiwamu

We improved the clipping of the IM1 trans beam by moving the uncontrolled degree of freedom in the IMC alignment control.

As a result, the amount of the light detected at the trans PD went up from about 240 counts to more than 800 counts. Also the beam shape on the camera became more round-looking.

 

The clipping was mainly in yaw. The shift we introduced was visible in the IM4 trans QPD. The spot moved in yaw from -0.3 to 0.

The screen shots below are the current alignment settings that gives a less clipping on the IM1 trans beam. Note that we didn't touch IM1-4 suspensions.

Images attached to this report
H1 IOO
kiwamu.izumi@LIGO.ORG - posted 17:39, Tuesday 03 December 2013 - last comment - 23:13, Wednesday 04 December 2013(8805)
IMC alignment much better, WFS loops engaged, but IM1 trans light seems clipped in chamber

Stefan and Kiwamu

We continued working on the alignment of IMC today. We managed to get the alignment back i.e. the beam hits the center of the IM4_TRANS QPD with all WFSs in action. It is now happiy locking.

However, we found that the IM1 trans path, which is used for a camera and trigger PD, seemed clipped. By moving the mirrors on IOT2L, we concluded that the clipping happened in chamber, namely in HAM2. This is not a critical issue as this light is used only for triggering purpose and it still gives a reasonable amount of the light. We will keep studying what is happening in the chamber. Perhaps this could be due to the uncontrolled degrees of freedom in the IMC alignment control.

 

What we did:

Comments related to this report
sheila.dwyer@LIGO.ORG - 23:41, Tuesday 03 December 2013 (8808)
This evening Kiwamu and I tried to mitigate the clipping of the im4 Trans beam by putting some angle offsets on mc2 and mc3 while the wfs loops were locked. The hope was that this would change the uncontrolled dofs, while the loops keep the others under control. We used the pico motors to keep the spots centered on the wfs, and had to take small steps. We had to go out to the table and realign the whole path after a few iterations because the power on the lsc pd was dropping. This is a slow process, and didn't fix the problem, the shape of the beam on the imc trans camera did improve. Before and after pics attached
Images attached to this comment
stefan.ballmer@LIGO.ORG - 08:38, Wednesday 04 December 2013 (8809)
Comments on the 5th or 6th phase rotation of the IMC:

We are now using the I demod output for IMC locking. The delay line settings are:
1/16:Up 1/8:Dn 1/4:Up 1/2:Up 1:Up 2:Up 4:Up 8:Dn 16:Dn

The WFS phase settings are:

H1:IMC-WFS_A_SEG1_PHASE_R = -90
H1:IMC-WFS_A_SEG2_PHASE_R = -17
H1:IMC-WFS_A_SEG3_PHASE_R = -27
H1:IMC-WFS_A_SEG4_PHASE_R = -22
H1:IMC-WFS_B_SEG1_PHASE_R = +15
H1:IMC-WFS_B_SEG2_PHASE_R = -34
H1:IMC-WFS_B_SEG3_PHASE_R = +28.5
H1:IMC-WFS_B_SEG4_PHASE_R = -81

For previous rotations, see Oct 1st alog 7941.


kiwamu.izumi@LIGO.ORG - 23:13, Wednesday 04 December 2013 (8827)

There is a similar report from the last May (alog 6265). I wonder if an optic is loose somewhere in this path.

H1 CDS (DAQ)
david.barker@LIGO.ORG - posted 16:56, Tuesday 03 December 2013 (8806)
CDS Maintenance Summary

Sysadmin tasks: Patched internal machines accessible from outside of CDS. Performed nmap network scans on 10.20.0.0/24 and 10.101.0.0/24 subnets. Updated network drawings

h1asc0: Replaced the h1asctt model with the new h1sushtts model.

updated the H1EDCU_DAQ.ini file to trend status of all models. Updated autoBurt.req for DAQ frame writers to archive all EPICS channels associated with these systems.

Updated overvew MEDMs (for ASC TT change)

Multiple DAQ restarts were required to support these changes.

LHO General
gerardo.moreno@LIGO.ORG - posted 16:12, Tuesday 03 December 2013 (8804)
Ops Summary

- FM-200 Systems (OSB and LSB), annual inspection took place today.
- Apollo at Y-End, working on extraction of cartridge out of BSC06.
- Baling crew @ Y-arm, baling tumbleweeds, now at X-Arm, opening a path.
- Kiwamu and Stefan, working on IMC recovery.
- Dave, some DAQ reboots.
- Thomas, to LVEA, connected TCS ring heater for ITMY.

LHO VE
kyle.ryan@LIGO.ORG - posted 15:59, Tuesday 03 December 2013 (8803)
LVEA purge-air fixes complete but particulate levels not measured
Kyle, Gerardo 

Repair of the drying towers is done but the purge-air supply isn't available to the LVEA yet -> We still need to devise a method to demonstrate the effectiveness of the removal of the alumina dust before routing the dry air through the final filtration stages and on to the LVEA
H1 SEI (SEI)
hugo.paris@LIGO.ORG - posted 15:34, Tuesday 03 December 2013 (8802)
IMC HAM-HEPI Controlled

HEPI common parts were updated yesterday per WP #4315

HEPI-HAM2 and HEPI-HAM3 were turned ON using the new Command scrips (Command2 Button from the overview screen).

They are running on their respective position loops, with the generic position blend filters (L4C=0, IPS=1).

Both HEPIs are aligned to the initial alignment position (aLog 7180)

 

HAM2 alignment TARGET (nm or nrad):

X -34219.8
Y -28697.6
Z -49473.8
RX 8810.3
RY -67894.6
RZ -20905.3
HP 30465.4
VP 16344.5

 

HAM3 alignment TARGET (nm or nrad):

X -3129.6
Y 106783
Z -104514
RX -23729.6
RY -25190.7
RZ 123598
HP 87442.4
VP 200991
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