TITLE: 05/19 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Planned Engineering
INCOMING OPERATOR: None
SHIFT SUMMARY:
Doors are on HAM1 and things are being wrapped up in order to start pumping down!
LOG:
| Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
|---|---|---|---|---|---|---|
| 14:15 | FAC | Kim, Nellie | LVEA | n | Tech clean | 14:58 |
| 15:20 | VAC | Jordan | LVEA | n | Turning down purge air on HAM1 | 15:27 |
| 15:51 | Oli | LVEA | YES | Transitioning LVEA to laser hazard | 16:06 | |
| 15:59 | - | Corey | EX | n | Wallet hunt | 16:19 |
| 16:00 | FAC | Kim, Nellie | EX | n | Tech clean | 17:08 |
| 16:11 | OPS | RyanC | LVEA | Y | Restart DM5 | 16:11 |
| 16:00 | Camilla | LVEA | YES | Turning down power | 16:37 | |
| 16:00 | SUS | Jeff, Rahul | LVEA | YES | Checking RM pointing (Jeff out 16:40) | 16:43 |
| 16:00 | EE | Fil | CER | YES | Checking if PM1 is jumpered | 16:14 |
| 16:39 | EE | Fil | LVEA | n | Running cables | 18:21 |
| 16:40 | EX | Eric | EX | n | Looking for hot breakers | 17:59 |
| 16:40 | Camilla | LVEA | YES | Transitioning us back to laser safe | 16:48 | |
| 16:44 | ISC | Betsy | LVEA | n | Last minute checks on HAM1 table | 17:40 |
| 16:57 | SUS | Jeff | CER | n | Checking SUS coil drivers | 17:00 |
| 17:04 | VAC | Travis | LVEA | n | Prepping for doors | 18:34 |
| 17:09 | FAC | Kim, Nellie | EY | n | Tech clean | 17:50 |
| 17:09 | PCAL | Tony | PCAL Lab | y(local) | Packing up standards | 18:28 |
| 17:24 | VAC | Jordan, Janos | LVEA | n | HAM1 doors | 18:41 |
| 17:26 | VAC | Gerardo | LVEA | n | HAM1 Doors | 18:41 |
| 17:44 | FAC | Chris | MY | n | Checking noisy bearing | 18:24 |
| 17:45 | EE | Jackie | LVEA | n | Helping Fil with cables | 18:21 |
| 17:53 | SUS | RyanC | CR | n | OpLev charge meas for ends | 19:21 |
| 18:16 | Elenna | LVEA | n | Watching doors get put on | 18:21 | |
| 18:22 | EE | Fil, Jackie | CER | n | ISC cabling for HAM1 | 19:36 |
| 18:34 | ISC | Camilla, Betsy | LVEA | YES | Transitioning to Laser Hazard and checking beams at ports | 19:07 |
| 18:57 | FAC | Nellie | LVEA CERish | YES | Restocking garb | 19:26 |
| 19:24 | VAC | Jordan | LVEA | N | Door work | 21:51 |
| 19:33 | VAC | Janos, Gerardo, Travis, Randy | LVEA | n | Putting on second door (Janos, Travis, Randy out 21:30) | 21:51 |
| 19:44 | FAC | Eric | EY | n | Checking breaker panel temps | 21:16 |
| 20:15 | CDS | Jonathan, Dave | MSR | n | Swapping frame writer power supply | 20:47 |
| 20:46 | Jeff | LVEA | n | Returning laptop | 20:48 | |
| 20:47 | TCS | Camilla | LVEA | n | Checking CO2X table parts (laser is off) | 21:13 |
| 20:48 | CDS | Dave | EY | n | Checking cameras | 21:56 |
| 21:13 | PCAL | Tony | PCAL Lab | y(local) | Starting measurement | 22:46 |
| 21:40 | FAC | Randy | LVEA | n | Helping with doors | 21:51 |
| 21:46 | EE | Fil | LVEA | n | Finishing up HAM1 cables | 23:34 |
| 21:46 | Richard | LVEA | n | Trying to not help out | 21:55 | |
| 21:56 | CDS | Dave | EX | n | Checking other cameras | 22:58 |
| 22:26 | SEI | Jim, Mitchell | LVEA | n | Moving Class A stuff out of HAM3 cleanroom | 22:43 |
| 22:41 | VAC | Jordan, Gerardo | LVEA | n | Prepping HAM1 for pumpdown | 23:34 |
| 23:17 | TCS | Camilla | LVEA | n | Measuring a distance and looking in the TCS cabinets | 23:34 |
FAMIS 31406
The sock filters had slight discolorization, but there were floating string-like particulate in both reservoirs (pic1 & pic2). This isn't a new finding, but I was hoping after the last flush in October that it would have reduced the amount of floaters over time as they were filtered out, but this doesn't seem to be the case.
Sheila and I used the thorlabs power meters to do a quick power budget along the POP and REFL paths. Just as a note, this alog from Craig and others in 2022 still holds and is probably the best authority for the REFL path.
Attached is a handy cartoon with the naming convention for HAM1, see D1000313.
POP path measurements:
POP path measurements were taken in "single bounce" 10 W input. So PRM misaligned, ITMX aligned. 9.4 W was incident on IM4 trans.
Expected power to HAM1 = 9.4 W * 0.977 (IFI transmission) * 0.031 (PRM transmission) * 0.5 * 0.5 (two passes of the BS) * 229e-6 (PR2 transmission) = 16.3 uW (this assumes the reflection off the ITM is 1)
The POP beam then sees a 90/10 split at M12 (air/vac) and a 50/50 split at M15 (LSC/ASC).
| Location | Measured | Expected (how calculated) | Ratio Measured/Expected |
| After periscope | 15 uW | 16.3 uW (9.4 * 0.977 * 0.031 * 0.5 * 0.5 * 229e-6) | 0.92 |
| reflection of M12 (90/10 splitter for air/vac) | 14 uW | 14.7 uW (9.4 * 0.977 *0.031 * 0.5 * 0.5 * 229e-6 * 0.9) | 0.95 |
| transmission of M15 (just before POP ASC diode) | 0.65 uW | 0.81 uW (9.4 * 0.977 * 0.031 * 0.5 * 0.5 * 229e-6 * 0.1 * 0.5) | 0.8 |
The beam is hard to see until after the lens so these were the only measurements possible.
REFL path measurements:
These measurements were taken in two sets, with the first set at 10 W input with PRM misaligned and the second set at 2 W input with PRM aligned and ITMX misaligned.
Set 1 is single bounce with PRM misaligned and 9.4 W on IM4 trans.
Expected power to HAM1 = 9.4 W * 0.977 * 0.031 * 0.5 *0.5 * 0.031 * 0.977 (double pass of beam splitter, PRM and IFI) = 2.15 mW (this assumes that the backward throughput of the IFI is the same as the forward throughput)
| Location | Measured | Expected (how calculated) | Ratio Measured/Expected |
| Before M14 (beam just coming to HAM1) | 2.05 mW | 2.15 mW (9.4 * 0.977 *0.031 *0.5 * 0.5 * 0.031 * 0.977) | 0.95 |
| reflection of M14 (90/10 splitter) | 1.9 mW | 1.94 mW (9.4 * 0.977 * 0.031 *0.5 * 0.5 * 0.031 * 0.977 * 0.9) | 0.98 |
| transmission of M17 (first 50/50) | 0.1 mW | 0.11 mW (9.4 * 0.977 * 0.031 *0.5 * 0.5 * 0.031 * 0.977 * 0.1 * 0.5) | 0.91 |
| transmission of M1 (second 50/50) | 40 uW |
53.9 uW (9.4 * 0.977 * 0.031 *0.5 * 0.5 * 0.031 * 0.977 * 0.1 * 0.5 * 0.5) |
0.74 |
Set 2 is single bounce with PRM aligned and 2 W input, so 1.9 W on IM4 trans.
Expected power to HAM1 = 1.9 W * 0.977 (IFI throughput) * 0.97 (PRM reflection) * 0.977 (IFI throughput)= 1.76 mW
| Location | Measured | Expected (how calculated) | Ratio Measured/Expected |
| before M2 (third 50/50 splitter) | 64 mW** | 44 mW (1.9 W * 0.977 * 0.97 * 0.977 * 0.1 * 0.5 * 0.5) | 1.45 |
| before M6 (LSC/ASC splitter) | 14 mW | 22 mW (1.9 W * 0.977 * 0.97 * 0.977 * 0.1 * 0.5 * 0.5 * 0.5) | 0.64 |
| transmission M6 (50/50 LSC/ASC splitter) | 7 mW | 11 mW (1.9 W * 0.977 * 0.97 * 0.977 * 0.1 * 0.5 * 0.5 * 0.5 * 0.5) | 0.64 |
| reflection of M18 (50/50 LSC A/B splitter) | 3.5 mW | 5.5 mW (1.9 W * 0.977 * 0.97 * 0.977 * 0.1 * 0.5 * 0.5 * 0.5 * 0.5 * 0.5) | 0.64 |
| transmission of M18 (50/50 LSC A/B splitter) | 3.5 mW | 5.5 mW (1.9 W * 0.977 * 0.97 * 0.977 * 0.1 * 0.5 * 0.5 * 0.5 * 0.5 * 0.5) | 0.64 |
** we made this first measurement as a quick check to see what power was going to the other side of the table, but clearly something is wrong with it! Maybe I transposed a number?
While there is clearly a discrepancy between what light we measure vs expect at M6, all the splitting ratios after seems to make sense. Craig calculated what the true splitting ratios for M14, M17 and M1 in alog 63510. None of these optics have changed. The splitting ratios are as follows:
M14 trans = 0.0756
M17 trans = 0.5072
M1 trans = 0.5295
If I update the calculations of the REFL path using those numbers, I get the following, with bolded values noting which ones have changed:
| Location | Measured | Expected (how calculated) | Ratio Measured/Expected |
| Before M14 (beam just coming to HAM1) | 2.05 mW | 2.15 mW (9.4 * 0.977 * 0.031 *0.5 * 0.5 * 0.031 * 0.977) | 0.95 |
| reflection of M14 (90/10 splitter) | 1.9 mW | 1.99 mW (9.4 * 0.977* 0.031 *0.5 * 0.5 * 0.031 * 0.977 * (1-0.0756)) | 0.95 |
| transmission of M17 (first 50/50) | 0.1 mW | 0.083 mW (9.4 * 0.977 * 0.031 *0.5 * 0.5 * 0.031 * 0.977 * 0.0756 * 0.5072) | 1.2 |
| transmission of M1 (second 50/50) | 40 uW |
43.8 uW (9.4 * 0.977 * 0.031 *0.5 * 0.5 * 0.031 * 0.977 * 0.0756 * 0.5072 * 0.5295) |
0.91 |
| Location | Measured | Expected (how calculated) | Ratio Measured/Expected |
| before M2 (third 50/50 splitter) | 64 mW** | 35.7 mW (1.9 * 0.977 * 0.97 *0.977 * (0.0756) * 0.5072 * 0.5295) | 1.8 |
| before M6 (LSC/ASC splitter) | 14 mW | 17.8 mW (1.9 * 0.977 * 0.97 *0.977 * (0.0756) * 0.5072 * 0.5295 * 0.5) | 0.79 |
| transmission M6 (50/50 LSC/ASC splitter) | 7 mW | 8.9 mW (1.9 * 0.977 * 0.97 *0.977 * (0.0756) * 0.5072 * 0.5295 * 0.5 * 0.5) | 0.79 |
| reflection of M18 (50/50 LSC A/B splitter) | 3.5 mW | 4.46 mW (1.9 * 0.977 * 0.97 *0.977 * (0.0756) * 0.5072 * 0.5295 * 0.5 * 0.5 * 0.5) | 0.78 |
| transmission of M18 (50/50 LSC A/B splitter) | 3.5 mW | 4.46 mW (1.9 * 0.977 * 0.97 *0.977 * (0.0756) * 0.5072 * 0.5295 * 0.5 * 0.5 * 0.5) | 0.78 |
Following up to add that Sheila and I recently checked the POP calibration in 82656, and it appeared we were missing about 15% of the power we expected on POP. Based on the measurements above, I can convince myself that it is possible we could have had that discrepancy, due to extra loss in the path into/on HAM1. However, these measurements do not exactly recreate that scenario because before we had a 95/5 at M12 and an HR at M15.
Jeff, Oli
Following up on one of Jeff's followup tasks about the signs of RM1 and RM2 (84462):
"(II) Measure the amplitude spectral density of each individual OSEMs well above the data rate we typically store them; look to see if there's no giant noise features. If there is -- debug that (usually a reboot of the satamp is the first step.)"
I ran ASD measurements for RM1 and RM2 at OSEMINF_OUT for each OSEM (with the comb60 filter turned off), and we verified they all look good(attachment1). To further check and compare them, we reran the same template (and filter) setup but for OM1 and OM2(attachment2). Since doors are currently being put on and the HAM1 ISI isn't isolated yet, we can see that the RM OSEM spectrum are very noisy below 30 Hz due to seismic noise, and other noises caused by the immediate environment are causing peaks at several different frequencies for thre RMs as compared to the OMs, but overall all four suspensions' OSEMs asymptote the same way and there aren't any noise features that seem to be of concern.
As per WP 12455 Dave and Jonathan replaced the power supply on h1daqframes-1. Due to the available space in the rack we decided to power off the system so that we could move it safely and replace the power supply.
We did some double checking to verify which machines where hooked together. We followed the physical connections and cross checked them with the names and numbers for interfaces on each machine. This was good as the labels on the front of the system where wrong. This is the frame disk associated with h1daqfw1.
We powered down h1daqfw1, verified that the link to h1daqframes-1 had gone dark. After that we powered off h1daqframes-1 pushed it forwared enought to replace the power supply, pushed it back in th place and restarted it.
After the disk server was back we restarted h1daqfw1 as well.
Dave will fix the labeling.
Labels are now good. MSR-RACK09 U02-U03 (bottom unit) is h1daqframes-1. MSR-RACK09 U04-U05 (next to bottom unit) is h1daqframes-0.
Closed FRS27399
R. Kumar, C. Compton, J. Kissel (Using Cartoon from other files of D1000313-v19) (Following sign conventions from T1200015) Given the sign confusion of the RMs (LHO:84289), I wanted a physical, with-our-eyeballs, confirmation of how the RMs deflect the beam under different alignment offsets given the current state of the system while we still had doors off HAM1. Using the REFL beam as our optical lever, we drove +/-20000 [ct] alignment offsets into each suspensions H1:SUS-RM[1,2]_M1_OPTICALIGN_[P,Y]_OFFSET, and watched the displaced beam downstream of the optic. Rahul was in chamber with the card and his eyeballs, Camilla was chamberside in view of the card as a second set of eyeballs to confirm, and I was driving with a CDS laptop and taking notes. Detailed blow-by-blow and raw convention-free data can be found in the attached text file. Conclusions (all statements made with "Today," preceding the statement): (0) We checked that On the actuation side, (a) H1:SUS-RM[1,2]_M1_OPTICALIGN_[P,Y]_GAINs are all positive, at +1.0; (b) The sign of the pitch and yaw elements of the EUL2OSEM matrices for both RM1 and RM2 match convention; (c) There's no sneaky sign flop in the *filters* of the COILOUTF banks, i.e, in none of the "LPM1" or "AntiLPM1" filter modules (see (1) below for statement on sign of gains) On the sensor side (d) The raw ADC counts for both RM1 and RM2 are positive, as expected after the cable swap, and per a normal OSEM sensor; (e) The sign of the OSEMINF bank gains are all positive values close to +1.0, as expected for a standard OSEM sensor chain; (f) There's no sneaky sign flip in the *filters* of the OSEMINF banks, i.e. in none of the "10:0.4", "to_um," or "comb60" filter modules (g) The sign of pitch and yaw elements of the OSEM2EUL matrices are the correct transpose (in the mathematical sense) of the EUL2OSEM matrices, so they match convention (1) the COILOUTF gains are set as they were reverted to their "been like this forever value" on May 6th LHO:84289, with (a) RM1 obeying convention (UL, LL, UR, LR = +, -, -, +) and (b) RM2 disobeying convention (UL, LL, UR, LR = +, -, -, +). (2) RM1 displaces the beam per convention, with a (a) positive pitch offset displacing the downstream beam down and (b) positive yaw offset displacing the beam in +Y (IFO Cartesian coordinates) i.e. rotating RM1 in +RZ, or +yaw, at RM2, (3) RM2 displaces the beam against convention, (a) positive pitch offset displacing the downstream beam up and (b) positive yaw offset displacing the beam also +Y (IFO Cartesian coordinates) i.e. rotating RM2 in -RZ, or -yaw, at M5, (4) Under these displacements, (a) the RM1 OSEM sensor sign agrees with the physical displacement: (i) positive requested pitch shows up as more positive pitch OSEM sensor value, (ii) positive requested yaw shows up as more positive yaw OSEM sensor value, (b) the RM2 OSEM sensor signs disagrees with the physical displacement: (i) positive requested pitch displaces the beam up (negative pitch), so the optic has physically tilted up in negative pitch, but the OSEM reads this as positive pitch (ii) positive request yaw displaces the beam in -RZ (negative yaw), so the optic has physically rotated in negative yaw, but the OSEM reads this as positive yaw. In each of the attach trends of the test -- RM1 PIT, RM1 YAW, RM2 PIT, and RM2 YAW -- that show - The digitally requested alignment offset - The OSEMINF raw ADC channels (just to show that these are all positive now, after the cable work discussed in LHO:84027; you can't actually see the displacement) - The projected Euler basis OSEM sensors - The REFL WFS DC QPD signals (these didn't turn out to be that useful because we didn't take care to let the beam settle at each alignment, and predicting what the sign of the measured beam spot downstream of the WFS lens is not straight-forward) All of the above conclude that There are no sign issues in the sensor or actuator chains for RM1 Given the combination of (1)(b) and (3)(a) + (3)(b), we conclude that There is *no* magnet polarity problems, and we *could* make RM2 actuators obey actuation convention without any hardware change. Instead, from (4)(b) There remains a sign issue with the OSEM *sensor* chain for RM2. And yet, even in the face of the *difference* in RM sensor sign, (3)(a) vs. (3)(b), With what *very* low level "does it work or not" MEDM screen viewing that we've done, *both* RMs "need" the same *positive*, +1, damping loop gain which disobeys convention. So -- - Why do the RM2 sensors readout opposite from physical displacement? and - Why don't RM1's damping loops work with a -1.0 damping gain? From here we need to: (I) Compare the *phase* of now vs. old "damping loop OFF" "health check" transfer functions. If these show a sign change after the cable swap changed the OSEM sensor sign, good. (II) Measure the amplitude spectral density of each individual OSEMs well above the data rate we typically store them; look to see if there's no giant noise features. If there is -- debug that (usually a reboot of the satamp is the first step.) (III) If/once there's no gross electronics noise, after the dust settles in the chamber, with doors on, turn on the damping loops with +1 gain. (IV) Measure the open loop gain transfer functions (drive M1_DAMP_EXC, measure TF of IN1/IN2), and confirm stability and appropriate amount of gain; they should look like they did when I improved the damping loop filters back in 2022. LHO:63656. Debug further if they don't.
Looked into (II) here: 84468
* Not a great measurement, low coherence and large error bars*
I took the OPLEV charge measurements for ETMX and ETMY this afternoon. There were more overflows than typical on both ETMs during the measurements, ground motion was also elevated due to highish (~20mph) winds.
ETMX's charge is close to +/- 50 [V] on all DOF, ETMY's charge is under +/-50[V] on most DOFs except for UL_Y, and maybe LL_P.
For chamber closeout finalization, this morning I * placed a 3" contam control wafer on the center of the HAM1 table today * took a few last pics, removed the stowed 3x septum covers (missed removing the 4th one from the septum, thanks vac good eye, pic 4) * looked around for left behind tools * retraced the beam path to look for errand in-the-way cables (none observed) * inspected under and around lower area of table for left goods (none found) * cleaned up last tool pans to get ready for doors * particle counts were <50 all sizes, zero most often * purposefully coiled the to-be-used in post O4 next vent cable with the peek connector not grounding to anything - it sits in the PSL side door well below the table * all subsytems have signed for doors, so we are putting doors on.
Tagging for epo
Betsy, Sheila, Camilla. WP 12551
When we first put together everything for PM1, we just copied all the filters over from RM1(84457). It turns out that the coil drivers for RM1 and RM2 both have had ECRs completed (ECR:E2200307, IIET:24501) that changed the frequency response for the coil drivers, a change which the PM1 coil drivers do not have.
After some troubleshooting (84454), we figured this all out, and so I just went in and updated the COILOUTF filters for PM1 to be what they are supposed to be, which is identical to the filters used in the other HAMA driver top masses that haven't had the ECRs done to them, like the ZMs. Filters have been loaded in.
| Filter | Before (matching RMs) | After (matching ZMs) |
| LPM1 (not used) | zpk([52.32;50.77],[0.5;3174],1,"n") | zpk([9.99999;20.9999],[0.9;211.883],1,"n") |
| AntiLPM1 | zpk([0.5;3174],[52.32;50.77],1,"n") | zpk([0.9;211.883],[9.99999;20.9999],1,"n") |
J. Kissel, R. Kumar, O. Patane, F. Clara We're debugging why high-frequency asymptote/slope/frequency response of PM1's transfer functions do not match RM1's -- see RED (PM1) and BLACK (RM1) from the attachments of LHO:84397. I immediately suspected coil driver compensation filters in COILOUTF banks did not match the analog HAM-A driver's low pass filter *state.* In the modern era all HAM-A driver's low pass filters are to be jumpered ON since we don't have binary input/ouput remote control of them. And when instantiating a new HTTS suspension, because there's no MEDM interface to set it, and you have to "caput" the channel (H1:SUS-RM1_BIO_M1_STATEREQ) to 2.0 via the command line. When we forget to do this, we errantly see the analog response of the driver in the health check transfer functions rather than the expected "falls as 1/f^2 above the resonances." We confirmed (via trend) that I *did* set this correctly when I original brought the infrastructure online see LHO:84457 comment to LHO:83293 on Mar 20 2025. We also confirmed that it's still the case today -- see attached screenshot, with magneta box around the CD state. We also confirmed that the LED status lights of the LP filter are green / ON, which report that, internally, indeed the HAM-A driver's LP filter switch is in the "Run" state, which is LP ON, see attached photo of SUS-C4, U-heights 3 (for PM1),4 (for RM2), 5 (for RM1) (per page 14 of D0902810-v11). HOWEVER (1) In taking that picture, I noticed that all the HAM-A drivers in that rack had a sticker mentioning ECR E2100430 *except* for PM1's driver in U3. In that ECR -- which is for modifying the OMs -- is better described in T2100410, the low pass filter response was changed from a z:p = [10,20]:[1,200] to z:p = [0.5,3174]:[52.32, 50.77]. There are later ECRs E2200307 and E2400048 that demand the *rest* of the HAM-A drivers should be modified with these same changes. Tickets IIET:20650 (for OMs) IIET:24501 (for IMs, RMs, and OFI), confirm that these modifications have been done at LHO for those suspensions. (2) IIET:30349 (for the A+ SUS), suggests that no such modifications have been done at LHO (and partially implemented at LLO). Rahul confirms with a pictures from SUS-M1 that the ZM1 ZM2 ZM3 and the OPO, and SUS-C8 for ZM4 ZM5 ZM6 that there are no stickers referencing any ECR E2100430, E2200307, and what it *should* reference, E2400048. From this we conclude that E2400048 has NOT been implemented here at LHO. (3) Finally - even though ECRs demand that essentially ALL HAM-A drivers should now have this LP filter change -- there exists NO version of D1100117 that has the the change in components or callout of new frequency response. This is likely why this change got overlooked when setting up PM1's HAMA driver. So, from the lack of sticker, lack of updated circuit drawing, and odd health check transfer function response -- we conclude frequency response PM1's HAM-A driver has frequency response is still the z:p = [10,20]:[1,200] response. When I set up PM1, I copied RM1's COILOUTF frequency response. RM1's COILOUTF is *correctly* was compensating the z:p = [0.5,3174]:[52.32, 50.77] analog response. However, that will NOT correctly compensate the unmondified PM1 driver's z:p = [10,20]:[1,200] response. *sigh* For now, we'll update the COILOUTF filters, and then discuss later when / if we want to modify the driver.
I am attaching two pictures as a reference to Jeff's comments above ("there are no stickers referencing any ECR E2100430, E2200307, and what it *should* reference, E2400048"), please see them below,
1. Picture01- SUS-M1 for ZM1 ZM2 ZM3 taken at the MER
2. Picture02 - SUS-M1 for ZM4-5-6 taken at the CER (see slot U11 and U12).
Yikes! E2200307 also mentions to eliminate the binary switching for the IMs and use jumpers like all the others. Since the binary IO chassis for the IMs are still in the rack, I suspect this hasn't been completed. We should go ahead and install the jumpers for the IMs and remove the binary IO chassis.
The COILOUTF filters have been updated to compensate the current, z:p = [10,20]:[1,200], frequency response -- see LHO:84455.
I left 10W out of the rotation stage, with the stage de-engergized this evening and the light pipe closed. I've just now unlocked the PMC (LOCK off, RAMP off) so that we won't have 10W on the light pipe shutter all weekend.
This is a reminder that whenever the PMC is unlocked, especially for an extended period of time, the FSS and ISS should also be disengaged; otherwise, the respective autolockers will continue to try to engage these systems despite not having the means to do so (because they have no light, since the PMC is unlocked). If there are ever any questions as to how to properly and safely disengage the PSL stabilization systems, CONTACT ME. It does not matter if I'm offsite for any reason (RDO, vacation, sick, etc.).
From the 10-day trends Ryan posted this morning, neither the ISS nor the FSS were properly disengaged, so were left trying to lock all weekend. For the FSS see the plot H1:PSL-FSS_NPRO_XTALTEMP in this set of plots. It's clear from this plot that the FSS autolocker was doing a temperature search while trying to lock the RefCav, which means the NPRO PZT was also ramping. Since there was no light in the FSS path the RefCav could not lock, so the search continued all weekend.
For the ISS, see the plot H1:PSL-ISS_DIFFRACTION_AVG in this set of plots. The ISS diffraction should be completely flat if it is off, but the series of downward spikes indicate the ISS was trying to lock and failing to do so, since there was no light on the ISS PDs (my guess is it kept lowering the diffraction percentage to try to increase light on the ISS PDs, and unlocking when the diffraction hit 0% to start the process again). This can also be seen in the behavior of the PMC reflected power (1st attached picture), which was moving around substantially all weekend as the ISS was trying and failing to lock; can also see the ISS diffracted power moving between 0% and 40%. A zoomed in portion is also attached, in which it's seen that the ISS diffraction was moving from zero to ~20% (but as high as 50%) in a roughly 15 second period; note the changes in PMC Refl during this time (the small spikes in PMC Trans are not the PMC trying to lock, it's small flashes of resonance as the temperature of the PMC changes combined with the FSS actuating on the laser frequency).
While not strictly necessary, it's good practice to also close the PSL external shutter if the stabilization systems are going to be disabled for an extended period.
I don't think that this will compromise the performance of the ISS or FSS, but this does represent unnecessary wear on the mechanical components that are the actuators for both of these stabilization subsystems. I should have caught that the PSL was left in this state, but did not pay attention to the alog during my RDO weekend and therefore did not catch this. For this I apologize.
|
location number on drawing |
distance | horizontal 13.5% diameter [um] | vertical 13.5% diameter [um] | photo of profiler location | photo of profiles | photo of beam scan measurements |
| 1 | 52 mm from dichroic M10 | 6243 | 64040 | here and here | 9022 | 9023 |
| 2 | 147 mm from dichroic M10 | 6202 | 6365 | 9028 | 9026 | 9027 |
| 3 | 119 mm from HR of 50/50 BS M15, also 295mm from center of lens L2 | 870 | 874 | 9031 | 9030 | 9029 |
| 4 | 153 mm from HR of 50/50 BS, approximate location of LSC diode | 279 | 284 | 9035 | 9032 | 9033 |
| 5 | 128 mm from HR of 50/50 BS | 721 | 726 | 9036 | 9037 | 9038 |
| 6 | 139 mm from HR of 50/50 | 483 | 490 | 9041 | 9040 | 9039 |
| 7 | 353 mm from HR of 50/50 BS | 3280 | 3372 | 9042 | 9043 | 9044 |
Camilla made these measurements with 20W input power into the IMC, PRM and ITMY misaligned single bounce beam. We didn't place the 90/10 BS M12 in the pop path yet so that we would have about 35uW to measure beam profiles. There's a rough pen sketch of where these locations are in this photo.
Camilla also made ruler measurements of some distances:
I think these measurements look pretty good, and the result is not that much different than the model (at least in terms of where to put the diodes). The biggest surprise is that Keita and I were pretty sure the beam coming into HAM1 is just over 2 mm in radius, when in reality it is more like 3 mm in radius.
I have attached plots of both the horizontal and vertical propagations, but you can see that the results for each direction are very similar. The black points are the measurements Sheila and Camilla took today, and I fit them with a la mode and the 2 inch POP lens (f = 334 mm), using the distances from the dichroic mirror that Sheila and Camilla measured.
If we place the POP LSC diode about 140 mm from M15 and the POP WFS about 200 mm from M15, we should get the beam sizes we want on each. I think these positions are a little closer to M15 than they are in the drawing, but I don't think that's a problem.
I also attached my a la mode script.
Linking here that Keita added distances to the refl air and popair periscopes here: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=84345
Here is the layout to reference optic numbers listed above: D1000313-v20
And here are Corey's chamber close out photos: 84561