Displaying reports 77661-77680 of 83147.Go to page Start 3880 3881 3882 3883 3884 3885 3886 3887 3888 End
Reports until 12:02, Tuesday 05 March 2013
H1 SUS
arnaud.pele@LIGO.ORG - posted 12:02, Tuesday 05 March 2013 (5661)
PR3 Phase 3a power spectra (bis)

Following my previous log on PR3 power spectra, showing suspicious resonnances at 2.7 Hz for several degrees of freedom, Travis went in chamber and found a blade tip EQ stop touching.
A new set has been ran, and look very good, as what we expect.
To sum up phase 3a power spectra, the attached pdf shows comparison between LLO phase 3b (Sept 2012), LHO Phase 2b (Feb 2013), LHO phase 3a (before moving the EQS March 2013) and LHO Phase 3a (after moving the EQS March 2013)

data and plotallhlts_spectra have been commited on the svn

Non-image files attached to this report
H1 IOO
guido.mueller@LIGO.ORG - posted 11:04, Tuesday 05 March 2013 (5660)
IMC 1 misalignment
Cheryl V., Deepak K., Joe G., Betsy B., Jeff K., Guido M.

We discovered yesterday that the flag of the side OSEM on the first stage of the IMC triple suspension was hitting the top of the OSEM hole. Betsy moved the OSEM and it should now be free.
However, this should mainly affect the roll motion of the mirror. It did not fix the problem with the IMC1 alignment. 

The alignment problem turned out to be just a confusion between calibrated and non-calibrated data (thanks Jeff). The IMC mirrors were never misaligned. 

However, that puts the blame for the misalignment into the IMC squarely on the beam coming from the PSL table. This is something we need to keep monitoring and fix today.

GM
H1 SUS
arnaud.pele@LIGO.ORG - posted 10:42, Tuesday 05 March 2013 (5652)
HAM2 HAUX B&K hammer measurements (chamber-side)

Jeff K. Arnaud P.

In order to confirm that the SUS-style dog clamps securing the HAUXs on HAM2 ISI table at LHO don't adversely lower their cage resonant frequencies, we took B&K measurements on IM1/IM2/IM3/IM4. We followed a similar measurement prescription as in LLO aLOG 3692.
The measurement was performed in chamber with the tri-axial accelerometer (as opposed to the laser vibrometer), mounted on the structure as described on the aatached picture ( X=Front and Y=side). The ISI table was locked, each had their IM scrapper baffles installed (secured to the front of the structure, as best they could be, see LHO aLOG 5633), the optic was freely suspended and the damping was turned off.


The pdf attached (2012-03-04_XYexc_H1_HAUX.pdf), shows that there is no resonances below the required 150 Hz (indicated by the vertical dashed line).


This should be sufficient proof that the SUS dog clamps are perfectly acceptable at securing the HAUX. Comparisons with LLO's data is to come.

 

The attached data lives in the SUS SVN under:

${SusSVN}/sus/trunk/HAUX/H1/IM?/BandK/

and has been committed as of this entry. This data was painfully exported following the procedure outlined here.

The data analysis was performed using

${SusSVN}/sus/trunk/Common/MatlabTools/BandK_plot.m

Images attached to this report
Non-image files attached to this report
H1 SEI
jim.warner@LIGO.ORG - posted 08:11, Tuesday 05 March 2013 (5659)
BSC2 mostly ready for flight

HughR, MitchR, JimW

Yesterday morning, TeamSEI finished most of the prep work for the BSC2 cartridge install. Lifting pads were added, cables were disconnected and tucked away, the ISI was checked for leftover tools, CPS racks were removed, and the walking plates cleared. A check on the underside is still needed, for more loose tools and to make sure we are not still bolted to the stand, but otherwise ready to go, IAS work still pending.

H1 INS
jodi.fauver@LIGO.ORG - posted 08:08, Tuesday 05 March 2013 (5658)
BSC6 Entry
First cleaning completed  and door bolts (except four) removed yesterday. Second cleaning early this morning.
H1 INS
jodi.fauver@LIGO.ORG - posted 08:06, Tuesday 05 March 2013 (5657)
BSC10 Feedthrough/Blank Install
Install continues. We should be finished today. (1 16" with 7 small adapters, 1 12", 1 10" remain.)
H1 CDS
james.batch@LIGO.ORG - posted 06:21, Tuesday 05 March 2013 (5656)
Changed gds tools to version gds-2.16.3.2
WP 3740

Changed gds link to gds-2.16.3.2 to allow more than 64 models to be detected by gds tools.
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 21:22, Monday 04 March 2013 (5655)
H1 SUS MC1 and H1 SUS MC3 Transfer Functions Show Clean Bill of Health
J. Kissel

After noticing that H1SUSMC1 and H1SUSMC3 have deviated from their previous alignment (see LHO aLOG 5642), one speculation was that the SUS is somehow hanging improperly or perhaps rubbing. However, a set of transfer functions on both suspensions show that their dynamics are the same as what was in Dec 2012. A clean bill of health from transfer functions would/does not (of course) reveal the state of DC alignment (or cause of misalignment), but it at least rules out worst-case-scenarios like a wire break, invisible [EQ stop / flag / magnet] interference, or that somehow the optic's wires had been knocked out of their prism grooves. *phew*

-------------
The data was taken with the following DTT templates:
${SusSVN}/sus/trunk/HSTS/H1/MC?/SAGM1/Data/2013-03-04_*_H1SUSMC?_M1_WhiteNoise_?_0p01to50Hz.xml,
exported to ascii files with the same name (with the usual _tf.txt extension),
individually processed by 
${SusSVN}/sus/trunk/HSTS/Common/MatlabTools/plotHSTS_dttfs.m
and collectively compared using
${SusSVN}/sus/trunk/HSTS/Common/MatlabTools/plotallhsts_tfs.m
Non-image files attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 19:29, Monday 04 March 2013 (5654)
plots of dust counts
Attached are plots of dust counts > .3 microns and > .5 microns in particles per cubic foot requested from 5 PM February 28 to 5 PM March 1. Also attached are plots of the modes to show when they were running/acquiring data.

Data was taken from h1nds1.
3600 seconds worth of data was unavailable on this server
1438.0 minutes of trend displayed
Non-image files attached to this report
LHO General
patrick.thomas@LIGO.ORG - posted 19:07, Monday 04 March 2013 (5653)
plots of dust counts
Attached are plots of dust counts > .3 microns and > .5 microns in particles per cubic foot requested from 5 PM March 3 to 5 PM March 4. Also attached are plots of the modes to show when they were running/acquiring data.

Data was taken from h1nds1.
1440.0 minutes of trend displayed
Non-image files attached to this report
LHO General
justin.bergman@LIGO.ORG - posted 15:53, Monday 04 March 2013 (5650)
Ops Summary
LVEA laser safe all day.

-Technical cleaning crew working on BSC2 and BSC6
-Apollo installing feedt-throughs on BSC10
-Michael R restarted PSL
-Hugh wandering LVEA making HEPI inspections
-Platt Electric delivery for Richard M
-Travis working in HAM2 (1030)
-Maya Angelou Elementary tour of the site; interesting questions asked and answered
-Thomas V in LVEA doing SLC inventory (1330)
-Jim B to LVEA to check cabling  on H1PEM
-Corey G installing power supply on IOT2L
H1 INS
jodi.fauver@LIGO.ORG - posted 13:32, Monday 04 March 2013 (5646)
BSC2 Install Prep Checklist
Lower level garbing/staging cleanroom moved into place and central curtain installed
Dome bolts removed
2nd cleaning at BSC2
Dome bolts removed (Additional cleaning complete.)
Leg jacks tested
Work on crane rails complete
Baffle assembly (work tables craned over beam tube, cleaned, moved into cleanroom)

Still need to:
Remove dome
Check chamber cleanroom function
Stage garbing/staging cleanrooms
H1 PSL
michael.rodruck@LIGO.ORG - posted 13:21, Monday 04 March 2013 - last comment - 17:29, Monday 04 March 2013(5641)
PSL shutdown/restart

The laser shut off over the weekend due to the power watchdog tripping. It looks like I had set the watchdog on the laser when the humidity was relatively high, and once the weather changed the humidity dropped back down and tripped the laser. We really need to look into this since the majority of shutdowns have been due to this humidity issue.

I took the opportunity to increase the current on the pump diodes to get us back to nominal power. The changes made are as follows:

I found that I could increase the power from the diodes by decreasing the temperature, but there was a point where increasing the diode power actually decreased the output of the laser. Instead of trying to maximize power from the diodes I watched the output of the laser and brought it up to 33 W. This is where we were back when the laser was installed.
Images attached to this report
Comments related to this report
michael.rodruck@LIGO.ORG - 17:29, Monday 04 March 2013 (5651)

I lowered the current on diodes 3/4 to 53 A after I got a bit more power out of diode 3, by decreasing its temperature to 20 C.

Also decreased the AC units to 20 C (unrelated) to try and stabilize room temperature for IO.

H1 SEI
jim.warner@LIGO.ORG - posted 13:13, Monday 04 March 2013 - last comment - 13:28, Monday 04 March 2013(5644)
SEI vacuuming at BSC2 ISI

This is from Friday morning.

With Jodi's help, I vacuumed the upper surfaces of the ISI. I found a fair amount of particulate, most of which appeared to be metallic flakes, though there was the occasional black fleck.I didn't think to get samples, but there are probably still specks to be collected, there's a lot of ground to cover. Most of what I found was collected in up-facing recesses in the plates, especially around the vertical L4C's. I also wiped down the keel and the larger exposed upper surfaces of the stages. Additionally, I found a bug that had crawled into the vent for a dowel pin and died, which I extracted by flushing with a large quantity of isopropyl.

Comments related to this report
jodi.fauver@LIGO.ORG - 13:28, Monday 04 March 2013 (5645)
Wow! Did you save the carcass so that we can ID the bug?
H1 SUS
mark.barton@LIGO.ORG - posted 12:02, Monday 04 March 2013 - last comment - 14:22, Monday 04 March 2013(5642)
MC1 and MC3 pitched
Cheryl reported that MC1 and MC3 were badly pitched relative to the last time she worked with them. Trending the M3 level signals shows that it went bad at about 20:30 UTC (12:30 PST) on Tue 2/19, possibly in connection with the removal of dummy masses in preparation for installation of PR3 and PRM (alog 5527).

Travis looked and didn't find anything obviously touching, so Cheryl is going to check the table levelness. Then we'll do another round of TFs to confirm that it's fixed or provide further clues.
Images attached to this report
Comments related to this report
cheryl.vorvick@LIGO.ORG - 13:12, Monday 04 March 2013 (5643)
I looked into the HAM ISI sensors and found that they also show changes from before the temporary weights were removed to after both PR3 and PRM were installed, which does indicate that changes to MC1 and MC3 could be caused by ISI changes.

The plot shows the March 18, 6AM to March 22, 6PM, so covers all the HAM2 weight changes during the week.
Images attached to this comment
hugh.radkins@LIGO.ORG - 14:01, Monday 04 March 2013 (5647)

Attached are HEPI trends showing maximum excusion during the unweighting/reweighting period.  None exceed 200 counts (.0003").  After reloading the table with the suspensions, the largest change is ,0.0001"

Images attached to this comment
jim.warner@LIGO.ORG - 14:22, Monday 04 March 2013 (5648)

Just for future reference, the conversion for the HAM cps's is about 800cts/.001", according to the HAM Integration Testing Procedure. The biggest shift is ~1000cts, so about 1.25 milli-inches, which is basically the slop in the lockers.

Displaying reports 77661-77680 of 83147.Go to page Start 3880 3881 3882 3883 3884 3885 3886 3887 3888 End