A reviewed version of the handbook for the 200 W laser, which is going to be installed in October, can now be found at the DCC: LIGO-T0900641-v4 (https://dcc.ligo.org/DocDB/0008/T0900641/004/Operating%20Manual%20AdL%20HPO.pdf) You are welcome to send me your comments, if you have some...
Michael Rodruck, Jose Puente
Finished installing the acoustic panels in the PSL acoustic enclosure. Very quiet in there now.
The dust monitor at location 3 has a sensor fail and may need to be replaced.
Recovery from power outage on Sunday Scheduled: Work platform for cartridge install, fit check assembly around BSC 4 Cleaning of the LVEA ISI test stand area Grouting for optical lever test
Both the crossbeams for HAM 9 have been installed despite the fights for crane time. With the aid of Ed and Scott we were able to pass the crossbeam under the beam tube first by picking with a cradle lift from the center of the tube, then setting the crossbeam down on stands and re-picking with the spreader bar. For some reason the HEPI foot took even more adjustment to bring into alignment than usual. The North end frames are a little south of an optimal Position (a few 32nds of an inch).
Remaining is to install the clamps on the frame and torque the south end to spec. Afterwards the clamps will be torqued around the support tube and hopefully the support tubes can be shot and brought into nominal position.
Cleared error on Corner Station purge air compressor - OK now.
LHO had a power outage (not sure at the moment if it was just the corner station or site wide). Outage was 20 seconds long, from 08:10:52 to 08:11:12. All front end systems (H1 and H2) are down. H1 and H2 DAQs are down down, H1 PSL screens are white. old ilog, web login services are down. Rebooting and restoring systems now.
We really need more section headings. "IFO and SubSystems" is everything. We could start with one heading for each major IFO subsystem, as well as a few for common activities (calibration, glitch investigation, data analysis, SciMon, automatic or robo entries, ...). These should all have different heading colors to aid the eye when scanning for interesting entries.
Matt, Lisa
We spent the afternoon assembling the green QPD sled in the new EY lab. Our reference design comes from G1100129.
The first picture is of the EY clean lab, in its current disorganized state. For the record, the particle counter reads 0 except when we are near it, in which case it may reach ~50 particles/CF.
The second picture shows the input green laser (~2mW of green, collimated at w ~ 2mm), arranged to send a beam across the class A sled to the beam scan. The 2" converging lens (L1, ROC = 154.5mm), the 50/50 beam-splitter, and the first 1" diverging lens (L2, ROC = -25mm) are in place, but the first HR mirror is absent to allow the beam to exit onto the beam scan.
The third picture is of the same setup. Yes, the laser is on. Yes, it is visible light. No, you can't see it on any of the clean optics, or in the air. Only the dirty fiber collimator shows some light.
While in this configuration, we adjusted the position of L2 until we got something we liked (based on quick beam scanning), and then we took some beam scan data. In the last 2 columns, I've divided the 36.8% data by sqrt(2) to convert it to beam waist radius, and then taken the mean of these data with the 60.7% data.
distance from L2 | 60.7% V | 60.7% H | 36.8% V | 36.8% H | w_V | w_H |
---|---|---|---|---|---|---|
10" | 281um | 266 | 476 | 379 | 309 | 267 |
12" | 264 | 215 | 402 | 355 | 274 | 233 |
14" | 243 | 210 | 393 | 337 | 260 | 224 |
16" | 249 | 231 | 390 | 341 | 262 | 236 |
18" | 270 | 258 | 410 | 373 | 280 | 261 |
20" | 300 | 306 | 440 | 440 | 306 | 309 |
The last picture is of the final assembly, with all mirrors, lenses and QPDs in place. The black glass beam dumps are AWAL.
The simulink library part for the QUADs (used to produce the guts of every QUAD model) was generated from a version of my original model, before I knew that the LED light level voltages were *not* being stored in the DAQ, so today I went in and removed them from the guts of QUAD_MASTER model. Because I had them come in at the top level (as though from an ADC), I needed to then also modify the connections at the top most level of each of the suspension's models that have been built. Further, I had used the LED light level as a term that was watched by the watchdog, so removing them from that meant not only a reworking of the MASTER simulink model, but the generic MEDM screens, *and* the QUAD.c auxiliary watchdog front end code. All effected files have had there functionality re-confirmed, and have subsequently been committed to the cds_users_apps repository in the ${userappshome}/cds_user_apps/trunk/sus/ section (where ${userappshome} for H2 is /opt/rtcds/lho/h2/) During the process, I had Dave create the same soft-linked "release" folder in the /opt/rtcds/lho/h2/core/ directory, which links to whichever RCG release one is *supposed* to be using (which for the time being is the 2.3 branch, not a tag). That way, when we upgrade to any future generations of the RCG, the sysadmin merely updates the softlink, but to the average user, the build directory remains the same. Further, though ITMX doesn't exist yet, when I recompiled and installed the ITMX model that Rolf and Dave had built on the h2susb478 machine, I generated the OVERVIEW screen for it as well, as linked from the sitemap (which is delightfully easy once you've built a generic screen). Also, while messing with the models, I tried exploring how to use the cdsFiltCtrl CDS simulink part, run into a bunch of trouble with internal links and library parts, and also learned how generic MEDM screens are in use. Sadly very little science was done, and I'm still confused the blocks are supposed to be used, but at least there's now one more person on the planet that has any clue as to how we're doing things with the newest suite of CDS software (library simulink parts, generic medm screens, RCG 2.3, etc).
9:00- 10:00 moving of squeezer table. Clean room by hams 2 & 3 was moved a few feet from its original position. 9:40 – Michael R. and student working on the H2 PSL to install the acoustic panels. 10:30 - Rick and Gregorio at Mid-X 12-12:30 tour into the control room. throughout the day: quad test stand work in the LVEA HAM 5 door removal ongoing
R. Lane, R. McCarthy, B. Bland, T. Sadecki We attached the BOSEMS for the ITMY to the vacuum feed-through simulator. It took a bit more setup to get the signals on the right channels in the hardware. When we finally saw them we were confused by the fact that we are used to seeing them in the range of 0 to -32000 counts, but we were seeing them railed at +32000. After some debugging by Richard we determined that the hardware seemed to be working. We tried blocking the light in the OSEM, and the signal went to zero. Our conclusion is that the hardware is working in general, and we are getting real signals, although quite large. On the next working day we have plans to compare the control signals in the X1 test stand versus the H2. Richard has a theory that the LED is being driven harder in the H2 hardware (~30mA vs 10mA).
The other idea is that there's an unaccounted for minus sign (or lack there of) in the electronics hardware somewhere. Or at least one that's different from what has been seen in all of the past (on test stands, iLIGO, etc). *Ah-CHOOOOO*! Sorry... I'm allergic to minus signs.
We have a short cut for front end code developers. On the h2build machine as user controls, if you type "core" it will send you to the /opt/rtcds/lho/h2/core/release directory. This directory is a symbolic link to the RCG version we are running H2 at, currently branch-2.3.
Here is a glimpse of the testing done on the ISI BSC8: Electronic, we changed: - 1 coil driver - 1 anti-image chassis - 1 sensor electronic board (and the sensor that goes with it) Instruments: - We replaced on coarse CPS sensor (and the electronic board). We stole two sets from unit2. Spares will be shipped from M.I.T in the coming days. - We had to open a GS13 can to adjust the 3 main springs holding the moving mass. This mass was resting at the bottom. We should receive replacement GS13 from LLO in about 2 weeks - There is a gain of 2 between the front panel and the back panel of the CPS satellite box. Software: - We had a couple of issues with watchdogs tripping when threshold were set up higher than the 2^15 bit (40K for instance). This problem might be coming from the decimation filters from the IOP to the model (64K to 4K). We will investigate later. - The Matlab transfer functions measurement program uses the decimate function (8 order Chebychev low pass filters at 0.8 x Nyquist frequency) to downsample the excitation signal. The decimation filters used to record signals on the frame builder have a corner frequency at ~0.7 x Nyquist frequency (with an order lower than 8). The Transfer functions are strongly affected over 700Hz for the geophones and 300Hz for the CPS. It will be fixed in the coming days. - In attachment, you will find a list the (101) channels recorded on the DAQ with their datarate. This list is the minimum required for testing and commissioning. The Overall datarate is 1.4MB/s. The allowed datarate is 2MB/s. Main results: - Stage1 is closed to a final balance - First resonance is at 215Hz on stage 1 (blades resonance? Need to be investigated) - First resonance is over 150 Hz on stage 2 (poor quality measurements at high frequency) I have attached few figures - The ISI with the cabling - Powerspectra of the sensors - Linearity test - Transfer functions (L2L main coupling)
B. Bland, J. Kissel, N. Roberston, T. Sadecki As discussed yesterday, today in one last bit of effort to understand which the lowest pitch mode frequency is lower than expected, we flipped the M3 dummy mass upside-down, in efforts to change the height of the suspension point between M2 and M3 at that mass ("d4"). The solid works model predicted that this flip would increase d4 from 1 mm above the COM to 2 mm above the center of mass. However, recall from yesterday that a model that best fit the measured data showed that d4 was in fact ~0 +/- 0.1 mm, i.e. dead even with the center of mass. The attached plot shows the results of the flipped M3. The result is that the pitch frequency did increase, but only by 0.01 Hz up to 0.47 Hz, as opposed to the expected 0.50 Hz. Hence, as with adjusting the M1 blade tip heights, the lowest pitch frequency moved quite a good deal less than expected. Further, a model matching the data shows that d4 had actually increased only from -0.1 mm (GREEN/PURPLE) to 0.4 mm (CYAN/GOLD), a 0.5 mm change, where a 1 mm change (from 1 mm (BLUE) to 2 mm (RED)) was expected. This concludes our foray into investigating this particular mode, as achieving a 0.48 Hz lowest pitch mode (where the lowest longitudinal mode remains at 0.41 Hz) was a goal, not a requirement. Hence, we will settle for the first pitch mode being at 0.46 Hz, in which the M3 mass is returned right-side up, and the M1 blade tip heights are set to 23.6 mm from the M1 base plate, making that the new baseline. Because we're going with a M1 lower blade tip height, we must now recalculate the appropriate wire lengths for the stages below M1, to restore the nominal heights of M2 and M2. We will do so, and remeasure the pitch frequency response to ensure that the lowest mode frequency remains *at least* above 0.46 Hz.
(Corey G, Jeff G, Jim W, Mike V)
Yesterday, we focused on subassemblies and getting them installed on the system.
Horizontal Small Actuators
All three of these were installed. A couple of notes:
1) The bolt on the "Base" (i.e. Magnet Mount) which is closest to the center of the ISI is really in a tough location to get a wrech at. Yoga poses are needed to tighten this bolt down (a torque wrench will not work back there).
2) The Actuator is pre-assembled with a Tooling Bracket which holes the coil & magnet in an ideal position. The magnet & coil sides are then carefully bolted down to Stage2 & Stage1 respectively. Coil/Magnet gaps are measured and then the Tooling is removed. Repeatedly, when the Tooling is removed, it was observed that the coil would drop on the order of 0.010-0.015"! Not sure what the trick is here to prevent this. For two of the Actuators this shift kept the gaps under the NO-GO value (we didn't want to have gaps over 0.115"). But on one, we had a gap of 0.118". This one had to be removed, Tooling re-attached, and then it was re-installed. With re-installation, this one fit in like a charm. It's gaps were balanced and no major shift was observed. It should be noted on this last Actuator that it's Pin Carrier Tooling were left in the Assembly during installation. perhaps this helped keeping things together.
3) It should also be noted that even with the Tooling, the Actuator gaps weren't always balanced (saw this with the Large Actuators). I thought this was the point of the Tooling! Is there a trick to putting these guys together. Perhaps keeping the Pin Carriers in place during the whole installation process is important.
Here are notes on biggest gap observed after Tooling removed (and also "before" gap measurements):
CORNER 1 Biggest gap (on top) = 0.111 (originally 0.098)
CORNER 2 Biggest gap (on top) = 0.118 (originally 0.109)
-----Reinstalled tooling and was balanced around 0.091"
CORNER 3 Biggest gap (on top) = 0.114 (originally 0.099)
Vertical Small Actuators
Just started installing one of these toward the end of the day. The Actuator Magnet Mounts (D0902191) were installed early, and it was noticed some of the bolts had somewhat tight fits into their helicoils. Perhaps these are electro-polished bolt candidates. Able to get the standard bolts to drop in by jiggling them a bit as you screwed them in.
Large & Small Lockers
The Small Lockers were installed with no issues. The Large Lockers were installed and then it was noticed that we blocked out access for the Spring Barrel Nuts(!). So, we had to remove all (3) Large Lockers, slip all Barrel Nuts into their holes, and then re-install the Lockers.
Locker Drawing Bolt NOTE:
So on the Assembly Drawings for both the Large (D1000854) & Small Lockers D(1000855), there are some items which aren't pointed out & are also just wrong. The issue we had were with bolts---the ones which bolt the Housing Locker Sleeve to the Stage/Plate above it (for both Lockers) and for the Large Lockers, the bolts which clamp Pin Caps down.
On the Large Actuators it is not pointed out which bolt should be used for the Pin Caps. By elimination, one would think it was the 3/8-16 x 1.5" bolts, BUT holes aren't tapped deep enough to take these bolts. So on BSC ISI#1, 1-3/8" bolts were used here. Unfortunately, the bolts used for Housing Locker Sleeves are also not pointed out in the drawing. By the process of elimination, we assume the 1-3/8" bolts were used here! (for both Large & Small Lockers).
So on BSC ISI#1, the 1-3/8" bolts were used for the Large/Small Sleeves & also on the Large Pin Caps. Unfortunately, we had a limited amount of these bolts and this left us short for BSC ISI#2! This is what we did for #2:
We saw for the Large/Small Housing Sleeves, that the 1-3/8" bolt provide LOTS of thread. We also saw that the 1-1/4" long bolt also provided plenty of thread as well. So, 1-1/4" bolts were used here for both Large/Small Lockers on BSCISI#2. Since the 1.5" bolt didn't work on the Large Locker Pin Cap, we put the 1-3/8" bolt here (as we did on #1).
Drawings changed to note this issue.
Temperatures in the LVEA have fallen dramatically overnight - average temps are ~60F. This is due to a broken wall temperature sensor which was sending back a reading of 256F - as a result the control system has been doing it's best to reduce that one zone temperature. I have disabled this sensor until it is repaired. Temps should begin to return to normal.
(G. Tellez, E. James, E. Black) Installation of the X-Y stage for the RX is complete. Both piers are in their final positions, leveled, and ready to be grouted. The laser (red, class II) was tested and the beam diameter will be measured to confirm the expected 2mm spot size. Telescope will not be used for test; opted to use commercial beam expander. A breakout box was built for preliminary tests of the QPD readout.
R. Lane, A. Ramirez Testing ITMY (QUAD 2) Took the Top Mass OSEM Coil Resistances, Photo Diode Voltages, and LED Voltages today. Took measurements at the connection between the octopus cables (D1000234) and the top mass extension cable. The OSEMS meet the requirements.* Coil Resistances: 39±1Ω PD Voltages: 1.01±0.05V LED Voltages: 0.53±0.05V Main Chain OSEM S/N Cable Coil(Ω) LED(V) PD(V) Face 1 481 695 36.3 1.017 0.554 Face 2 638 695 36.0 1.018 0.551 Face 3 501 695 36.4 1.018 0.558 Left 496 695 36.0 1.017 0.551 Right 499 698 36.5 1.018 0.558 Side 445 698 36.7 1.017 0.558 Reaction Chain OSEM S/N Cable Coil(Ω) LED(V) PD(V) Face 1 471 698 35.9 1.018 0.553 Face 2 484 698 36.4 1.018 0.554 Face 3 472 707 36.9 1.016 0.554 Left 630 707 36.8 1.017 0.562 Right 466 707 36.7 1.019 0.558 Side 415 707 36.0 1.018 0.559 *The requirement for the coil resistance to be 39±1Ω was defined at LLO using "extra long" non final cables. This requirement is not sufficient to determine if the resistance is within standard. I will inquire with the correct authorities to determine what the new value should be for the in-vacuum final cables. However, they do meet the tolerance of ±1Ω. We took the measurement at the octopus cable, not at the vacuum feed through simulator as specified. We did not have the cables available. Although this should not add more than a few tenths of an ohm to the final resistance and would not make up the difference.
The "M0 F2" OSEM now has a S/N 261. This is the current list on the H2 ITMY QUAD in the LVEA.