Displaying reports 74061-74080 of 76956.Go to page Start 3700 3701 3702 3703 3704 3705 3706 3707 3708 End
Reports until 12:10, Wednesday 30 May 2012
H2 CDS
david.barker@LIGO.ORG - posted 12:10, Wednesday 30 May 2012 (2979)
h2 FMY front end glitch and crash, IPC took ITMY down
The H2 FMY front end computer (h2susb78) sent IPC Dolphin error glitches which IOP tripped the SEI for BSC8 in several separate occasions between 9am and 09:30 this morning local time. At 10:10 the front end locked out, no ping, no ssh, console stuck at last log message. All lights looked good on the front end, but the only recovery was to power cycle the computer. This in turn crashed h2susb478 (ITMY front end) because of the Dolphin drop out. We took the opportunity to recompile the SUS ITMY model since it had not been built since Apr 11th and was missing the DACKILL part (RCG branch 2.5 build).

I took the opportunity to rebuild the temporary optlev model to make it generic. A H2 DAQ restart was also performed, the master file was changed and the OVERVIEW medm regenerated.

The cause of h2susb78 problems is not known, but there is some work progressing around BSC8 at the times in question.
H1 AOS
jason.oberling@LIGO.ORG - posted 11:58, Wednesday 30 May 2012 (2978)
BSC06 ETMy Pitch Alignment
IAS: J. Oberling
SUS: B. Bland, T. Sadecki
 
We adjusted pitch this morning with no First Contact on the ETMy to correct for the pitch error induced by the First Contact.  The pitch was adjusted to 623 µrad down which is 16 µrad away from our target (639 µrad down) and well within the ±160 µrad spec.
H2 SEI
vincent.lhuillier@LIGO.ORG - posted 18:14, Tuesday 29 May 2012 (2976)
BSC8 - ISI and HEPI

HEPI:
Last week, the L4C gain of the pier modules were increased from 22 to 333. The transfer functions measured over the week end showed that this new gain is appropriate. No saturations on the L4Cs during the measurements.
I will start to work on controllers for the HEPI pretty soon.

ISI:
This morning, I fixed the isi2stagemaster.mdl and recompiled ISI-BSC6 and ISI-BSC8 due to an error mentioned in a previous aLOG.
I installed the new aLIGO BSC-ISI matrices freshly computed. I posted them in the SVN at /BSC-ISI/Common/Basis_Change_BSC_ISI/aLIGO/Matrices/Y/aLIGO_BSC_ISI_Matrices_Direction_Y.mat
I installed using one measurement:
- Symmetrization filters (actuators, geophones)
- Damping filters (stage 1 and 2)
- Blend filters (basic filters with a blend at 750mHz).
- Isolation filters. I haven't spent time on tuning. The goal is just to make sure the scripts and the model are ready. (UUG=15Hz, comfortable gain and phase margin).

I have attached spectra of the ISI undamped and controlled:

LHO General
david.barker@LIGO.ORG - posted 18:02, Tuesday 29 May 2012 (2975)
DAQ configurations available on web page
Every hour on the hour a copy of the INI PAR and FILTER files are copied to the LHO CDS web server. The URLs are:

https://lhocds.ligo-wa.caltech.edu/exports/running_config/h1/daqfiles/

https://lhocds.ligo-wa.caltech.edu/exports/running_config/h1/filterfiles/

https://lhocds.ligo-wa.caltech.edu/exports/running_config/h2/daqfiles/

https://lhocds.ligo-wa.caltech.edu/exports/running_config/h2/filterfiles/
LHO General
patrick.thomas@LIGO.ORG - posted 17:50, Tuesday 29 May 2012 (2974)
plots of dust counts
Attached are plots of dust counts > .5 microns.
Non-image files attached to this report
H2 AOS
douglas.cook@LIGO.ORG - posted 17:02, Tuesday 29 May 2012 (2973)
First Contact effects on optic pitch
Jason, Travis and Doug,
Jason measured the ETMy pitch just prior to the First Contact removal from the H2 ETMy optic.
the pitch was 629urads down (req is 639 urads down)

After the first Contact was removed it change to 379 urads down (a change of 250urads)

This is near what was predicted for a 1.74g weight First Contact coating.

Note: This was not accounted for on the H2 ITMy or measured.

We should possibly measure this for each optic or compensate for it in the calculations as we will also be adding additional weight with the new plan for using First Contact which will remain in place until just before we close up.
H2 AOS
hugo.paris@LIGO.ORG - posted 16:58, Tuesday 29 May 2012 - last comment - 22:00, Tuesday 29 May 2012(2972)
HAM-ISI Unit #4 (HAM2)- Chamber Side Testing - CPS Investigation

Vern, Hugo,

 

During the chamber side testing HAM-ISIs are locked. Part of the testing consists in measuring the DC voltages outputted by the CPSs to make sure that the probes and the electronics are still functional. This measurement is taken at the BNC output of the ADE boxes. 

 

We recently observed that the voltages we measured depended on the number of probes that were connected to the ADE Boxes. We also noticed that the voltages measured with only one probe connected to the ADE boxes were high in comparison to what we expect on a locked ISI.

 

Vern and I investigated it this afternoon: 

The voltage measured at the BNC output of the ADE boxes would then match our expectations (0V +/- 4V), without varying with the number of probes that were connected.

 

We tried disconnecting the grounding cable between the test stand and the ADE boxes. The DC voltage read on the ADE boxes increased and became dependent on the number of probes that were connected, again. This latest observation confirms that the issues we experienced on the CPSs were related to the grounding of the ADE boxes.

 

conclusion:

 

Voltages and noise spectra were re-measured for each CPS and HAM-ISI Unit #4 (HAM2) chamber side testing report is being updated.

 

Pictures are attached

Non-image files attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 22:00, Tuesday 29 May 2012 (2977)

Hugo and his baby.

Images attached to this comment
LHO VE
kyle.ryan@LIGO.ORG - posted 16:29, Tuesday 29 May 2012 (2971)
Leak testing of H1 input MC done for the time being -> Vented H1 input MC

Kyle, Gerardo 

Summary ->  
Looking for large leaks -> We found a total of (7) leaking conflat flanges that will need to be addressed (>10-6 torr*L/sec typical).  In all cases, these were the large 10" and 12" joints and not the smaller feed-through joints.  We wrapped the leaking joints in RED UltraTape for indentification.  Also, both O-rings of the septum between HAM3 and BSC2 are leaking (inner high 10-4 torr*L/sec, outer mid 10-5 torr*L/sec), these are the O-rings on the BSC2 side which are integral to the septum plate.  


Kyle 

Vented H1 input MC
H1 CDS
david.barker@LIGO.ORG - posted 14:23, Tuesday 29 May 2012 (2970)
CDS maintenance h1boot machine cloned for DTS test stand
We took down h1boot for about 3 hours from 10am to 12:20 during this morning's maintenance in order to clone its boot drive. Michael unlocked the H1 PSL prior to the shutdown, and relocked it after h1boot was restored.

The cloned drive will be used to create x1boot as an identical copy of the production H1 and H2 systems.

A new backup VLAN network cable was installed to h1boot, and the switch reconfigurations were submitted to SVN.
LHO General
patrick.thomas@LIGO.ORG - posted 12:49, Tuesday 29 May 2012 (2969)
CDS FMCS code change
The code which reads the data from the FMCS web server and writes it to EPICS has been moved over to new code. I had tried this earlier, but it appeared to have some bugs, which these changes address. The same things noted here apply.
H1 FMP
jodi.fauver@LIGO.ORG - posted 12:37, Tuesday 29 May 2012 (2968)
BSC2-HAM4 ICC
First vacuum and wipe down of BSC2 were completed on Friday, 25 May. The dome was also documented and cleaned. Second vacuum of BSC2 was started on Friday and completed this morning. Final inspection was finished before lunch. FTIR samples were taken right after lunch and then dust barriers were removed. One dust barrier was wiped down and moved to the transition area between BSC2 and HAM4. The dome was replaced on BSC2 and torqued down. 
H2 SUS
jeffrey.kissel@LIGO.ORG - posted 14:14, Monday 28 May 2012 - last comment - 14:23, Monday 28 May 2012(2965)
H2 SUS ETMY, 2012-05-25 Measurements
J. Garcia, J. Kissel

Jeff launched a set of TFs on ETMY before heading out on Friday, just after Team TMS finished up in chamber, and Travis  had set ETMY's EQ Stops to pump-down ready ~0.75 mm distance to confirm that the SUS was still free. Attached are the results. Everything looks just as it did before, matches up with other SUS's up its type, and agrees well with the model. Things are looking good, couldn't ask fo mo betta!
Non-image files attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:23, Monday 28 May 2012 (2966)
The data was taken by the template collection script

/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/collectTF_H2SUSETMY_M0R0_allDoFs.m


which saved the data to the following raw files

M0 Raw Data (and diary of workspace): 
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/SAGM0/Data/2012-05-25_H2SUSETMY_M0_0p01to50Hz_allDOFs_DAMPSOFF_tf.mat
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/SAGM0/Data/2012-05-25_H2SUSETMY_M0_0p01to50Hz_allDOFs_DAMPSOFF_tf_diary.txt
R0 Raw Data (and diary of workspace):
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/SAGR0/Data/2012-05-25_H2SUSETMY_R0_0p01to50Hz_allDOFs_DAMPSOFF_tf.mat
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/SAGR0/Data/2012-05-25_H2SUSETMY_R0_0p01to50Hz_allDOFs_DAMPSOFF_tf_diary.txt


These were processed and plotted using

/ligo/svncommon/SusSVN/sus/trunk/QUAD/Common/MatlabTools/plotquad_matlabtfs.m


which produced the 2nd and 3rd attached set of detail plots, as well as the usual generic data file:

/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/SAGM0/Results/2012-05-25_H2SUSETMY_M0_fiber_model_MATTF.mat
/ligo/svncommon/SusSVN/sus/trunk/QUAD/H2/ETMY/SAGR0/Results/2012-05-25_H2SUSETMY_R0_erm_model_MATTF.mat


This data set has been added to the list of measurements and plotted against other selected measured measurements in

/ligo/svncommon/SusSVN/sus/trunk/QUAD/Common/MatlabTools/plotallquad_dtttfs.m

which generates the first attachment's collection of plots.
LHO General
patrick.thomas@LIGO.ORG - posted 18:37, Friday 25 May 2012 (2964)
plots of dust counts
Attached are plots of dust counts > .5 microns.
Non-image files attached to this report
H2 ISC
daniel.hoak@LIGO.ORG - posted 17:16, Friday 25 May 2012 (2962)
Picomotor breakout boxes
For posterity, I wanted to show how the picomotor signal from the driver box is broken up into the individual DOF signals.  In the pictures attached, the signal from the driver box goes to the Picomotor Break-out Feedthrough Panel [image 1].  This box takes the DB25 cable and splits it into two DB9 cables [2,3].  These DB9 cables go to a Picomotor Breakout Box, which rests inside the table on the cable tray.  This box has a PCB which splits the signals on the DB9 cable into four 4-pin RJ45 connectors, which are the pitch and yaw signals for two different picomotor assemblies [4,5].
Images attached to this report
LHO General
gerardo.moreno@LIGO.ORG - posted 17:06, Friday 25 May 2012 (2961)
Ops Day Summary

- Travis visited the Y-End station, EQ stops and FC removal of ERM, see his entry for more.
- Jason at Y-End station, alignment check up of ETMY, see his entry for more.
- TMS team was at Y-End station, see Keita's entry for more.
- Filiberto visited Y-End station to check on reports of odd smell, no smell found in or out of the building.
- Kyle checking for leaks in the H1 input tube.

The various activities at Y-End generated some dust, counts up to 1500.
H2 AOS
keita.kawabe@LIGO.ORG - posted 16:47, Friday 25 May 2012 - last comment - 17:28, Friday 25 May 2012(2959)
TMS alignment done (again)

This was the first attempt after the viewport was rotated back, and our alignment was still at the same bad position and the beam was not hitting the ETM. So apparently something moved, but we couldn't figure out what.

Anyway, we steered the beam back by adjusting the ALS table periscope mirrors, using the green QPDs on the TMS ISC table. then steering the TMS itself so the beam retro reflects back to the ALS table through an aperture we set up on the ALS table. We didn't use the picomotors as we knew that the alignment was pretty good two weeks ago and we were sure that that the picomotors were not moved since then.

After some tweaking, the beam looked really good at the secondary, F2, and the primary (Cheryl took pictures). It was low on F1 (a bigger of the two folding mirrors on the TMS telescope), but in the end I think it's more important to have the secondary and the primary reasonably well centered than the folding mirrors, and the beam retro reflects, so I think we're in a good shape.

The new offsets: 16000 counts for PIT, -5100 counts for YAW.

Before we started, Cheryl noticed that the EQ restraint bar is not centered any more (it used to be reasonably centered). We readjusted the bar position.

We also relieved that crazy PZT offset. It was on YAW of the upstream PZT mirror. Since the PZT mirrors themselves don't have any fine manual adjustment, we used the closest steering mirror. The input to the MCL PZT controllers were terminated. This made a tiny change in the alignment (which we were able to measure by QPDs) but these were taken care of manually by the periscope mirrors later. 

The diff-single converter on the field rack as well as the anti-imaging chassis on the ISC rack was turned off.

Comments related to this report
cheryl.vorvick@LIGO.ORG - 17:02, Friday 25 May 2012 (2960)
Pictures from today's realignment:

1) beam position on first steering mirror

2) beam on secondary mirror - there are two ghost beams, one above and one below the real beam

3) beam on the primary mirror

4) viewport from inside - the small green dot below the input beam is the Hartmann beam

5) viewport form the outside - beam going through viewport - Dan's idea to see if we could show how the surfaces and substrate are scattering

6) viewport form the outside - input and retro-reflected beam are seen separately in this shot
Images attached to this comment
daniel.hoak@LIGO.ORG - 17:28, Friday 25 May 2012 (2963)
For future reference, the sums of the green TMS QPDs with ~20mW of light going into the chamber are:

~315 counts on QPDA
~325 counts on QPDB
X1 SEI
hugo.paris@LIGO.ORG - posted 15:49, Thursday 24 May 2012 - last comment - 10:56, Tuesday 29 May 2012(2944)
HAM-ISI Unit #5 - Assembly Validation Report Ready

The report for HAM-ISI Unit #5 - Assembly Validation is now posted under the DCC for validation.

This unit was tested at the begining of the month with testing horizontal GS13s (alog #2802). These testing pods were replaced with production pods. All tests involving GS13s were performed again this week. This report is now waiting for approval. This Unit will then be our second HAM-ISI coming out of the staging building with a full set of production GS13s (the first one was HAM-ISI Unit #4).

Reports regading the Assembly validation of previous units at LHO are also available on the DCC:

HAM-ISI Unit #1 - Assembly Validation
HAM-ISI Unit #2 - Assembly Validation
HAM-ISI Unit #3 - Assembly Validation
HAM-ISI Unit #4 - Assembly Validation

 
Reports regading the Chamber Side testing of other units at LHO are also available on the DCC:
HAM-ISI Unit #4 (HAM3, or HAM2 chamber)
Comments related to this report
hugo.paris@LIGO.ORG - 10:56, Tuesday 29 May 2012 (2967)

This testing report is now approved

Displaying reports 74061-74080 of 76956.Go to page Start 3700 3701 3702 3703 3704 3705 3706 3707 3708 End