J. Kissel, B. Weaver Betsy and I took standard top-to-top mass transfer functions of H1 SUS SRM and H1 SUS SR3 to ensure after the heat of first contact removal and door re-application they're still free. They are. Great! Results attached. (Suspensions are undamped, with alignment offsets ON) Data and updated processing scripts have been committed to the repo. /ligo/svncommon/SusSVN/sus/trunk/HSTS/H1/SRM/SAGM1/Data/ 2017-12-14_1729_H1SUSSRM_M1_WhiteNoise_L_0p01to50Hz.xml 2017-12-14_1729_H1SUSSRM_M1_WhiteNoise_P_0p01to50Hz.xml 2017-12-14_1729_H1SUSSRM_M1_WhiteNoise_R_0p01to50Hz.xml 2017-12-14_1729_H1SUSSRM_M1_WhiteNoise_T_0p01to50Hz.xml 2017-12-14_1729_H1SUSSRM_M1_WhiteNoise_V_0p01to50Hz.xml 2017-12-14_1729_H1SUSSRM_M1_WhiteNoise_Y_0p01to50Hz.xml /ligo/svncommon/SusSVN/sus/trunk/HLTS/H1/SR3/SAGM1/Data 2017-12-14_1743_H1SUSSR3_M1_WhiteNoise_L_0p01to50Hz.xml 2017-12-14_1743_H1SUSSR3_M1_WhiteNoise_P_0p01to50Hz.xml 2017-12-14_1743_H1SUSSR3_M1_WhiteNoise_R_0p01to50Hz.xml 2017-12-14_1743_H1SUSSR3_M1_WhiteNoise_T_0p01to50Hz.xml 2017-12-14_1743_H1SUSSR3_M1_WhiteNoise_V_0p01to50Hz.xml 2017-12-14_1743_H1SUSSR3_M1_WhiteNoise_Y_0p01to50Hz.xml
Attached are a few pictures of the newly added baffles around the West (+Y) side of the HAM5 table, shielding the table, and SRM and SR3 optics.
Here are a few pix of the new OFI baffle and AWC mirrors on HAM5, installed over the last couple of weeks.
Although Kissel has been posting mass records of B&K results on lots of in-vacuum items, I'll show the full whiteboard list of what he has measured and been analyzing in the attached photo. All B&K measurements for this vent have been complete! Well done!
I'm posting the BnK measurements of the HAM2 & HAM5 table baffles. I've split the plots up into similar structures (Plus/Minus X/Y beard baffles, Middle beard Baffles, HAM2 table top baffles, HAM5 table top baffles) and equivalent excitations/accelerometer orientation relative to "beamline" (X for HAM2, Y for HAM5). I'm using Jeff's names for the baffles, so Table baffles are the beard baffles. Table Top baffles are the table baffles that typically lie flat on the ISI optics table in front of the suspensions. It looks like I grabbed the wrong data for the MC1 Table Top baffle, so I need to look into that some more.
Most of the well resolved stuff seems to be well damped, I don't think I saw any of the low frequency (50-60 hz stuff) on the first plot in the HAM5 or HAM2 ISI tfs. The sharp 120 hz feature on the HAM5 MinusX table baffle is worrying, but there was probably a lot of loose mass on the table at the time. The HAM5 measurements are from Dec 6, before Hugh and Brijesh balanced that table.
I've put the txt BnK exports in the Seismic SVN at:
/ligo/svncommon/SeiSVN/seismic/HAM-ISI/H1/Common/Data/HAMBnK_measurements/HAM2/
/ligo/svncommon/SeiSVN/seismic/HAM-ISI/H1/Common/Data/HAMBnK_measurements/HAM2/
The script I made the plots with is at:
/ligo/svncommon/SeiSVN/seismic/HAM-ISI/H1/Common/Data/HAMBnK_measurements/HAM2_table_baffles.m
As far as the HAM5 table goes--I cleaned up the table and bolted down and viton'd the table top masses on Dec1. However, on Dec7, GM found the new ZM2 mirror and the Septum Beam dump needing torquing.
HAM2: align intensity stabilization photodiode align beam coming off HAM2 table Betsy, Travis done with BSCs, leaving first contact on due to delay in HAM2 work IP4 is removed, next step is to install NEG pumps, first is ready to go on Chandra out next week, Kyle in charge of pump down Gerardo testing HAM5 viewport TMDS installed Cryopump decomissioning at mid Y scheduled for mid January Hugh: feedthrus ready to go on HAM6 Jason asked to start bringing optical levers back online over next couple of days TJ and Sheila starting to populate table Volunteers sought for onsite inspections during holidays Kyle and Chandra may run leak checks over holidays
The LVEA has transitioned to LASER HAZARD
We have been observing was seems to be flow restrictions in purge air so today as means of trouble shooting we replaced filters at the skid. Three of the four filters were replaced (could not replace the third one because its threads seem to be galled, but it visually looks ok and has been replaced in the past). The first filter had burn marks. The second filter was heavily loaded with rust dust. The fourth filter looked ok.
We disconnected all seven purge air points of use in LVEA to flush system with new filters. After several minutes we measured zero particle counts and -28degC dew point.
Closed WP 7247.
I'm running TF's oin SRM and SR3 SUSes.
At around 5:30 am several text alarms for CP7 rolled in all at once. MEDM screen looks normal. Will be in soon for visual inspection. Alarms are LN2 level error and discharge pressure error. Also got alarms for EY Y2 pressure and RO water system.
CP7 and PT-424 signals have all flat lined. In fact all signals at EY have flat lined. Going back out to check Beckhoff rack.
The battery that stores solar energy for Y2-8 gauge at IP isn't charged up enough and caused the gauge to turn off which caused a communications fault at EY. Richard and Patrick are on it.
I misread one of the texts. It was actually EY Y2 CC error (CC=communications). Not PT-424, which just so happens to be labeled "EY_Y2_PT-424"
Richard, Patrick The same thing happened at end X later this morning. The equivalent of the following was done: end Y: Disabled Pressure Gauge Y2-8 (BPG 402) File -> Save All TwinCAT -> Activate Configuration Popup: Restart in Run Mode?: Yes PLC -> Login Check that the values of the GVL variables are changing Close and restart the EPICS IOC end X: Disabled Pressure Gauge X2-8 (BPG 402) File -> Save All TwinCAT -> Activate Configuration Popup: Restart in Run Mode?: Yes PLC -> Login Check that the values of the GVL variables are changing Close and restart the EPICS IOC Burtrestore: On vacuum1: cd /ligo/cds/lho/h0/burt/2017/12/13/06:00 burtwb -f h0vacex.snap burtwb -f h0vacey.snap
The LVEA has been transitioned to LASER SAFE.
(Kyle R, Gerardo M)
Right before lunch both feedthroughs were removed and replaced while all door covers were on. We removed the old style feedthroughs and installed the new type (Accuglass PN100520) on BSC1 and BSC3 (flange F2, subflange 3 for both BSCs). Both need to be leak checked.
WP7245
To complete the transition of the ISI Cartesian bias setting scripts from Perl to Python, today I edited all the MEDM files which call these scripts. In all cases the scripts are called indirectly via an xterm running a wrapper bash script. I changed the dimensions, font and colors of the xterm to make it more readable. Again I used ISI ITMY ST1 as my test system, returning the settings after I had finished.
J. Kissel I've process several sets of data to show results of B&K measurements which characterize the new scraper baffles in HAM3 / HAM4, the MC2 scraper baffle (), the PR2 scraper baffle (), and the SR2 scrapper baffle (), all of which are assembled with viton built into the structure, so we expect very little high-Q features. Attached are results from all three LHO baffles, in addition to comparing the same DOFs measured at LLO (though, LLO used a laser vibrometer, and only measured the response to 2D excitation in one direction). It's difficult to make any broad sweeping statements about any of these baffles. I would have naively expected that the PR2 and SR2 baffles from both sites would have similar resonant features in the comparable excitation + response directions, but they're all different. Similarly, the MC2 scraper baffle shows a different response. I could easily imagine the response being different because of the differing hit locations -- from the looks of pictures, Arnaud / Stuart hit the centers of big surfaces on each baffle (think excitation of drumhead modes of those panels), where Siddhesh and I were hitting the top corners of structures (think excitation of flag-pole modes of the entire structure). Also, the response sites were different between observatories: the laser vibrometer can directly measure (at least one) surface of each baffle, where as the accelerometer bolted to the table picks up ISI table resonances (i.e. the high Q features around 10-15 Hz which are the locked / HEPI cross-beam resonances). If we're really looking to confirm that these are built identically, and have confirm that *all* resonances are damped to a sufficiently low Q, then we're going to need to standardize our measurements. For now, all we can do is acknowledge what frequencies we see where, and hope the don't show up in the IFO's sensitivity! For those who need more detailed information, I attach the data (zipped up in an archive that you'll need to decompress), and the script to process the data to make these plots. Details of the measurements can be found in the following aLOGs: H1 MC2 / PR2 LHO aLOG 39590 H1 SR2 LHO aLOG 39288 L1 MC2 / PR2 LLO aLOG 36908 L1 SR2 LLO aLOG 37020
After another marathon day in chambers, Fil, Richard, Travis, and I finally finished connecting the newly fabricated ITM ESD feedthru connections in-chamber and their subsequent testing (FRS Ticket 5033). The testing, of course, was not straight forward and we walked around troubleshoot a few things here and there. We struggled with the ITMX BIAS intermittently failing the HIPOT testing and continuity checks (see issues with this reported last year 27562). We tracked down the issue to the pin at the other end of the cable we reterminated (and have not touched during this vent) which led to me disassembling the connector a bit and looking for shorting mechanisms. I didn't find any, but upon reassembling the connector, things seemed to test fine. Sigh.
Fil will likely post the full numbers above or below this alog for both ITMX and ITMY testing (which included HIPOT).
Meanwhile, the ground checks of the SUS cables that were checked on ITMX, ITMY, and the BS which failed a few days ago were fixed via a variety of reseating the connection fasteners at the feedthru end of the cable, remedying pinch points of cables in-vacuum, or resolving to have EE fix it somewhere on the outside. Most of the cables had not been touched during this vent, with the exception of the ITMX PUM one which had migrated out of it's viton pad seat during the ITMX rebuild last month.
So, really, really we could do the BSC 1, 2, 3 closeout tomorrow.
Sorry, forgot the shout out to Gerardo and Kyle who swapped the actual feedthru at the chamber port.
After new feedthru was installed:
1. In-vacuum cable was connected
2. New 5-way connector pigtail was connected to feedthru (air-side).
3. All pins were tested with HI-POT tester to 1KV, except ITMX bias which was only tested to 500V. This included new pigtail air-side cable.
4. After HI-POT testing, grounding shorts were addressed for cables SUS-42 and SUS-57. See alog 39744. Found one of the cables had its air-side backshell shorted to cable shield. This was fixed. Other issue was fixed in chamber, see above entry from Betsy.