TITLE: 03/19 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Observing at 143Mpc
INCOMING OPERATOR: Oli
SHIFT SUMMARY:The low range coherence check yielded, CHARD_Y and PRCL at low frequency. The range has been in the mid 140s, we've been locked for 5.5 hours.
02:06 low frequency glitch, EX and DCPD saturation
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:34 | Electrical | Ken | LVEA | No | Finding lift for work Above HAM1 | 18:59 |
14:56 | Vent Prep | TJ | near HAM1 | N | Taking down laser Curtains. | 15:28 |
15:09 | VAC | Rogers | Mech room | N | Working on kobelco units | 20:39 |
15:11 | PCAL | Rick, Francisco | EX, EY | Yes | Beam Spot movment on EX. | 16:44 |
15:23 | VAC | Gerardo | West bay LVEA | No | Vac work, ION pumps into FCT | 18:03 |
15:25 | FAC | Kim & Nelly | EY, HAM SHAQ, EX | N | Technical cleaning. | 18:05 |
15:27 | VAC? | Travis | EX, EY | Yes | Taking Measurements | 20:54 |
15:27 | EE | Fil | LVEA, CER | N | Pulling cables. | 19:48 |
15:29 | IAS | Jason | Input - West LVEA | N | Doing some FARO work. | 21:05 |
15:47 | EE | Marc | LVEA | N | helping Fil | 19:48 |
15:48 | Site Safety | McCarthy | LVEA | N | Checking roll up door. | 16:01 |
15:49 | VAC | Norco | Y arm | N | Filling N2 tanks. | 18:44 |
16:07 | PEM | Robert | LVEA | N | Accel, cable clean up | 16:13 |
16:20 | FAC | Chris | Out Side West bay | N | Moving Big Green Harvester | 19:41 |
16:48 | Faro | Jim | HAM1, HAM SHAQ | N | Helping Jason | 18:36 |
17:07 | PCAL | Francisco | PCAL Lab | Yes | Putting away tools | 18:59 |
17:14 | FAC | Christina | Receiving | N | Picking up batteries , driving truck | 17:59 |
17:28 | SUS | Rahul | Remote/ EY & EX | N | SUS measurements on EY | 19:14 |
17:49 | TCS | Camilla & TJ | EX | Yes | opening laser table and adjusting TCS system | 17:49 |
18:03 | IAS | Ryan C | LVEA input- west | N | FARO-ing with Jason | 21:05 |
18:06 | FAC | Kim, Nelly | LVEA | n | Tech clean | 19:30 |
18:23 | SEI | Jim | LVEA, HAM ShAQ | N | Looking for Install hardware | 19:01 |
18:49 | Exercise | Mayank & Shiva | Overpass | N | Enjoying the noon view | 19:19 |
19:25 | TCS | Camilla | ITMY | n | Checking CO2 laser | 19:32 |
19:42 | LASER Transition | Oli | LVEA | YES | LASER Transition & LVEA Sweep. | 19:56 |
19:53 | CPy | Sheila, Robert , Betsy | ITMY | Yes | Centering CPy using Oplevs | 21:21 |
19:57 | LASER HAZ | LASER HAZARD | LVEA (\u2310\u25a0_\u25a0) | YES | LVEA IS LASER HAZARD (\u2310\u25a0_\u25a0) | 06:36 |
21:07 | ISC | Rahul & Camilla, Shiva , Mayank | Optics Lab | Local | Working on ISS, Rahul Out early | 23:37 |
21:55 | ISS | Camilla | HAM6 | Yes | Getting parts | 21:58 |
22:32 | walk | Ryan C | Y-arm | N | Jogging the Y-arm | 23:02 |
23:40 | ISC | Camilla | OSB Receiving | N | Drove to OSB rec | 23:50 |
01:35 | FIT | Matt, Francisco, Mayank | Yarm | N | Going for a run | 02:09 |
FranciscoL, RickS
On Tuesday, March 18, we moved the PCALX lower beam by r = 2.5mm, \theta = +237 deg from its nominal center. We expect to see a change of 20 HOPs in \chi_XY -- returning to the value it was a week ago.
Placed target in the same alignemnt as in the previous actuation (TARGET_ON). Both individual beam voltage values, as found, were very similar to the values recorded at the end of the move done last week. We actuated by turning counterclockwise on the pitch adjuster of the outer beam folding mirror, with minor adjustments in yaw. The voltage of the lower beam after the move was higher than last week, it could be from AoI of the optics, but documenting here for future reference.
The following table shows the voltage values as read by the Keithley voltmeter we use during the procedure
Step | Comment | Readout [V] |
---|---|---|
1 | Both beams - target off | 3.377 |
2 | Both beams - target on (as found) (BEFORE_MOVE) | 2.896 |
3 | Lower beam after actuation | 1.43 |
4 | Both beams - target on (AFTER_MVOE) | 2.940 |
5 | Both beams - target off | 3.383 |
We have one more actuationg left in which we move the beam back to nominal center. For the upcoming move, we expect \chi_XY to stay the same.
FranciscoL, RickS, SivanandaR
In summary:
On Tuesday, March 11, we moved PCALX lower (outer) beam by r = + 2.5 mm, \theta = - 33 deg (from horizontal) on the ETM. We expect to see a large (~20 HOPs) change in \chi_XY.
From our investigations -- an independent method to estimate IFO beam offset using the Pcal -- we believe that the IFO beam offset, when facing the ETM, is (+ 14.3 mm, -- 09.3 mm) in cartesian coordinates. These coordinates yield an angle of arctan(-- 9.3/14.3) ~ -- 33 deg from the horizontal axis of the ETM center.
The first pdf file (polar_out.pdf) plots the IFO beam offset. The black points represent the measurements of a2l (located at '/opt/rtcds/userapps/trunk/isc/common/scripts/decoup/BeamPosition/a2l_lookup.m'). The green points are what is inferred by Pcal measurements. For the Pcal to estimate the IFO beam offset, we use the scalar product of \vec(c) -- the displacement vector of the Pcal center of force for a given actuation, and \vec(b) -- the IFO center of force, as it is derived in T2400032 equation 11. From the plot, there is a clear disagreement on the horizontal component of the IFO beam from both methods. Following equation 11, a measurement in which an actuation from the Pcal beams results in a parallel displecement of the pcal center of force to the real IFO beam center of force should maximize the change \chi_XY. Conversely, an actuation that is perpendicular would not be seen by \chy_XY (no change). The actuation for today was parallel to what the Pcal estimates is the IFO beam position. We plan to make a second actuation, in which we move perpendicular to our estimate of the IFO beam. Ideally, these measurements would increase our confidence of the IFO offset.
We aligned the target by setting an angle gauge at the calculated 33 deg as seen in the first image (TARGET_ON).
We aligned the Pcal beams to the corresponding apertures by (1) blocking one beam and (2) aligned beam of interest by maximizing the Rx sensor voltage readout from a Keithley digital multimeter (KVM). Since the upper beam has shown inconsistencies in the horizontal displacement (83051), we are actuating on the lower beam. The second image (BOTH_BEAMS) shows both beams after moving the lower beam.
The following table lists the voltage value at each relevant step of the process:
Step | Comment | Rx Readout [V] |
---|---|---|
1 | Both beams, as found | 2.840 |
2 | Upper beam, as found | 1.440 |
3 | Upper beam, centered | 1.50 |
4 | Lower beam, as found | 1.396 |
5 | Lower beam, centered | 1.40 |
6 | Lower beam, moved | 1.390 |
Some observations from today's visit to ENDX:
This is the first of three actuations. Additionally, the data processing still needs about a week of data to diagnose results. We will have nominal results in ~3 weeks.
J. Freed
Today I collected 2 phase noises, first phase noise is of the 80 MHz OCXO after it has gone through an RF distributer. The reference was the SRS SG382 at 80MHz
The second is of the Double Mixer again but with an extra focus on the 8192Hz sideband.The reference was agian the SRS SG382 at 80MHz-4096Hz
These tests was done with the direct plug in method without using a PLL. This requires both the device under test and the reference device to be at quadrature. Normally a PLL is required to keep them there, however since both devices are connected to the LIGO timing system in some way, a PLL is unnecessary to keep them locked in quadrature. To put them in quadrature I just lined them up on an oscilloscope best I could then added 90 deg by adjusting the phase on the SRS. I bypassed the internal amp of the BluePhase1000 for all tests.
DM_vs_RF.pdf Is a plot of the two phase noises, as seen, the low frequency noise (<2Hz) has these humps. I now attribute these to the RF distributer causeing a shape change in the pure sin wave signal.
RF_Distributer_Signal.jpg Shows how the RF distributer has a not exact sin wave (Yellow) compared to the SRS Pure tone (Blue)
DM8kSideband.pdf Shows a close up on the 8k sideband that will also couple into our SPI output
The measured curve looks very similar to the SRS SG382 spec at 100MHz. There is no reason to believe the SG382 is better than the OCXO.
TITLE: 03/18 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
INCOMING OPERATOR: Ryan C
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 10mph Gusts, 6mph 3min avg
Primary useism: 0.03 μm/s
Secondary useism: 0.22 μm/s
SHIFT SUMMARY:
H1 has almost recovered from Maintenance day changes, We are currently in Nominal_Low_Noise but not Observing as the Cameras need to be reverted back to the old server.
NLN reached at 23:27 UTC.
Sheilas CPy measurements were completed.
LOG:
Start Time | System | Name | Location | Lazer_Haz | Task | Time End |
---|---|---|---|---|---|---|
14:34 | Electrical | Ken | LVEA | No | Finding lift for work Above HAM1 | 18:59 |
14:56 | Vent Prep | TJ | near HAM1 | N | Taking down laser Curtains. | 15:28 |
15:09 | VAC | Rogers | Mech room | N | Working on kobelco units | 20:39 |
15:11 | PCAL | Rick, Francisco | EX, EY | Yes | Beam Spot movment on EX. | 16:44 |
15:23 | VAC | Gerardo | West bay LVEA | No | Vac work, ION pumps into FCT | 18:03 |
15:25 | FAC | Kim & Nelly | EY, HAM SHAQ, EX | N | Technical cleaning. | 18:05 |
15:27 | VAC? | Travis | EX, EY | Yes | Taking Measurements | 20:54 |
15:27 | EE | Fil | LVEA, CER | N | Pulling cables. | 19:48 |
15:29 | IAS | Jason | Input - West LVEA | N | Doing some FARO work. | 21:05 |
15:47 | EE | Marc | LVEA | N | helping Fil | 19:48 |
15:48 | Site Safety | McCarthy | LVEA | N | Checking roll up door. | 16:01 |
15:49 | VAC | Norco | Y arm | N | Filling N2 tanks. | 18:44 |
16:07 | PEM | Robert | LVEA | N | Accel, cable clean up | 16:13 |
16:20 | FAC | Chris | Out Side West bay | N | Moving Big Green Harvester | 19:41 |
16:48 | Faro | Jim | HAM1, HAM SHAQ | N | Helping Jason | 18:36 |
17:07 | PCAL | Francisco | PCAL Lab | Yes | Putting away tools | 18:59 |
17:14 | FAC | Christina | Receiving | N | Picking up batteries , driving truck | 17:59 |
17:28 | SUS | Rahul | Remote/ EY & EX | N | SUS measurements on EY | 19:14 |
17:49 | TCS | Camilla & TJ | EX | Yes | opening laser table and adjusting TCS system | 17:49 |
18:03 | IAS | Ryan C | LVEA input- west | N | FARO-ing with Jason | 21:05 |
18:06 | FAC | Kim, Nelly | LVEA | n | Tech clean | 19:30 |
18:23 | SEI | Jim | LVEA, HAM ShAQ | N | Looking for Install hardware | 19:01 |
18:49 | Exercise | Mayank & Shiva | Overpass | N | Enjoying the noon view | 19:19 |
19:25 | TCS | Camilla | ITMY | n | Checking CO2 laser | 19:32 |
19:42 | LASER Transition | Oli | LVEA | YES | LASER Transition & LVEA Sweep. | 19:56 |
19:53 | CPy | Sheila, Robert , Betsy | ITMY | Yes | Centering CPy using Oplevs | 21:21 |
19:57 | LASER HAZ | LASER HAZARD | LVEA (\u2310\u25a0_\u25a0) | YES | LVEA IS LASER HAZARD (\u2310\u25a0_\u25a0) | 06:36 |
21:07 | ISC | Rahul & Camilla, Shiva , Mayank | Optics Lab | Local | Working on ISS, Rahul Out early | 23:49 |
21:55 | ISS | Camilla | HAM6 | Yes | Getting parts | 21:58 |
22:32 | walk | Ryan C | Y-arm | N | Jogging the Y-arm | 23:02 |
TITLE: 03/18 Eve Shift: 2330-0500 UTC (1630-2200 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
OUTGOING OPERATOR: Tony
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 7mph Gusts, 4mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.22 μm/s
QUICK SUMMARY:
00:03 UTC Observing
FYI - I've added a new block to the SUS SVN at SUS/common/models/
Adding SIXOSEM_T_ESTIM_STAGE_MASTER.mdl - this is simulink R2019a
Adding SIXOSEM_T_ESTIM_STAGE_MASTER_tmp.mdl - this was my working file in R2023b
Committed revision 31074.
These are a long way from done. This will be the new piece for the OSEM Estimator part for the HLTS (PR3)
The ECR is https://services1.ligo-la.caltech.edu/FRS/show_bug.cgi?id=32526
Robert, Betsy, Sheila
We went to the ITMY optical lever piers to check the CPY alignment, similar to 77557. We tried to reset the optical lever back to where it was before we started, the optical lever is now slightly shifted though. The sum dropped from 9060 coutns to 8930 counts, PIT went from -12.7 urad to -19.7 urad and YAW went from 1.3 urad to -4.4 urad.
WP 12393
ECR E2200105
DCC D2200162
DCC D1002872
T2300221
Started installation of the SEI HAM1 ISI field cables. Cables are now pulled from the CER SEI-C1 rack to the LVEA near HAM2/SUS-R1. Final routing of cables will continue next week. Documents D2200162, D1002872, and T2300221 don’t have the same flange layout. Imagine they will get updated once plans are finalized. Cables will be routed to HAM1 flanges as listed below:
Corner 1: Flange D1
SEI_HAM_15
SEI_HAM_16
SEI_HAM_17
SEI_HAM_18
Corner 2: Flange D5
SEI_HAM_33
SEI_HAM_34
SEI_HAM_35
SEI_HAM_36
Corner 3: Flange D3
SEI_HAM_51
SEI_HAM_52
SEI_HAM_53
SEI_HAM_54
CPS 1&2: Flange D5
SEI_HAM_63
SEI_HAM_64
CPS 3: Flange D3
SEI_HAM_65
SEI_HAM_66
F. Clara, M. Pirello
I took two single bounce OMC scans today with the help of TJ and Tony. Here are some notes to future me and others to reference if we want to do single bounce scans:
Edit to add: unfortunately the scan results from today look pretty bad. In short, the peaks look "lopsided" somehow, and so I'm not sure the results are usable. Looking back at Jennie W's previous scans, it looks like she had to slow them down to 200 second scans. I only did a 100 second scan with amplitude 105 so maybe I scanned too fast. I'm not sure what the correct resolution of this is, because the scans I did in 2022 were 100 second scans and the results were fine. Adding this note here for reference in the future to think about the appropriate scan length and amplitude.
Jennie, Sheila, and I ran OMC scans this morning and realized that the proper way to slow down the scan to avoid weird saturation effects is to reduce the excitation frequency in the template. The nominal templates have excitation frequencies of 0.01 Hz, so sweeping over 200 seconds just sweeps at the same speed twice. To sweep once, slower, you have to increase the sweep time to 200 seconds AND reduce the sweep frequency to 0.005 Hz.
Sheila and I want to note some things that are "obvious" but easily forgotten:
TITLE: 03/18 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Preventive Maintenance
CURRENT ENVIRONMENT:
SEI_ENV state: CALM
Wind: 7mph Gusts, 4mph 3min avg
Primary useism: 0.02 μm/s
Secondary useism: 0.24 μm/s
QUICK SUMMARY:
Be careful using the Roll up down between the receiving area and LVEA. It seems to be in need of maintenance.
SNEWS Test T565015 16:00:15 UTC
HAM7 ISI WD Tripp17:09 UTC
HAM7 CPS Glitch 17:10 UTC
2 Norco trucks went in the Y armdirection from the parking lot.
Mechanical room has fumes in it , doors have been opened to allow ventilation while Roger Bros
HAM7 CPS glitches 18:03 UTC
Dust alarms have been telling us there is dust.
Expected work:
LVEA:
Ham1 Laser Barrier taken down?
Lighting Fixtures above HAM1
Fil HAM1 pulling cables.
Vac roughing pumps & compressor
OMC scans by Elenna
EX:
PCAL ES Beam Mv over by 9am
Laser hazard Camilila & TJ TMS & ALS Return beam
Rahuls OPLEV SUS Charge measurements
EY:
Rahuls OPLEV SUS Charge measurements
Vac EY comp still in progress
CDS:
Dan LDAS maint.
Eric BS camera server testing
Still on going:
ITMY CPy adjustments.
M. Todd, C. Compton, T.J. Shaffer
We went down to EX with the intention of getting the reflected ALS beam to be a little cleaner, as we've been plagued with this lobey beam seen in alog 82752. If we were to succeed in cleaning up the beam we would have taken beam profile measurements; however, we were unable to make the beam any clearner, and any profile measurements did not make sense.
We started off a little cleaner than the previous log (82752) but we still had some weaker lobes that looked like ears (lending a sort-of Mickey Mouse shape).
Measuring the ALS return beam at ETMX, we misaligned ITMX and ITMY. Starting slider values were:
20250318 - 16:00:00 UTC | P | Y |
ETMX | -34.6 | -145.1 |
TMSX | -87.0 | -90.2 |
Moved to ETM Y: -2.4, TMSX: 634.8. (seems too big check this number on ndscope??), got worse, now has almost two lobes
Other way in Tat: ETM Y: -346.4, TMSX: -275.2. looks better, similar to original: Mickey Mouse.
Yaw back, not in Pitch: ETM P :204.4, TSMX P 139.0, now worse in Pit than yaw
LVEA has been swept
Plot attached, reset at 19:30UTC.
There has been activity near that TCS rack this AM, both cable pulling and wire racks moved nearby. We've seen this happen before, LLO is currently trying to investigate why.
Tue Mar 18 10:12:51 2025 INFO: Fill completed in 12min 47secs
h1caley's OBSERVE.snap is now a sym link to its safe file, bringing it in line with h1calex and the LLO models. h1caley_safe.snap was modified to monitor all of its channels.
lrwxrwxrwx 1 controls advligorts 62 Mar 18 11:01 h1caley/h1caleyepics/burt/OBSERVE.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1caley_safe.snap
lrwxrwxrwx 1 controls advligorts 62 Apr 21 2015 h1caley/h1caleyepics/burt/safe.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1caley_safe.snap
lrwxrwxrwx 1 controls advligorts 62 Apr 28 2017 h1calex/h1calexepics/burt/OBSERVE.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1calex_safe.snap
lrwxrwxrwx 1 controls advligorts 62 Apr 21 2015 h1calex/h1calexepics/burt/safe.snap -> /opt/rtcds/userapps/release/cal/h1/burtfiles/h1calex_safe.snap
We lost lock from the calibration, so we tried to lock ALS without the linearization (some background in this alog: 83278.) An active measurement of the transfer function from DRIVEALIGN_L to MASTER out was 1 without the linearization, and -0.757 with the linearization on. So I've changed the DRIVEALIGN gain to -1.3 in the ALS_DIFF guardian when the use_ESD_linearization is set to false.
We tried this once, and it stayed locked for a DARM gain of 400, but unlocked as the UIM boosts were turning on. We tried this again but it also didn't lock DIFF, so it is now out of the guardian again.
I looked at a few more of the past ALS DIFF locks, both sucsesful and unsucsesful attempts we are saturating the ESD (either the DAC or the limiter in the linearization) in the first steps of locking DIFF. We do these steps quite slowly, stepping the darm gain to 40 waiting for the DARM1 ramp time, stepping it to 400, then waiting twice the ramp time, then engaging the boosts for offloading to L1. I reduced the ramp time from 5 seconds to 2 seconds to make this go faster. This worked on the first locking attempt, but that could be a coincidence.
We will leave this in for a while, so that we can compare how frequently we loose lock at LOCKING_ALS. In the last 7 days we've had 48 LOCKING_ALS locklosses, and 19 locklosses from NLN, so roughly 2.5 ALS locklosses per lock stretch.
Since the time of this alog, around 19 UTC on March 13th, we've had 68 locking_ALS locklosses and 12 NLN locklosses, so about 6 locklosses per sucsesful lock. It seem though that the change to 2 seconds was never in place, and the guardian code still said 5 seconds. So this issue seems to be getting worse without any change.
Now I've loaded the change to 2 seconds, so this should be sped up after today's maintence window.
I've looked at a bunch more of these locklosses, and they mostly happen in the time when the DARM gain is ramping, less often as the boosts are coming on in L1, and 1 I saw happened while COMM was locking.
In all the cases the linearization seems to hit its limiter before anything else goes wrong.
We removed the BSC1 temperature sensor to run some testing in the lab. Will reinstall next week.
After testing in the lab, the sensors are working as designed, outputs are clean. We reinstalled the BSC1 temperature sensor but left it floating (not attached to BSC1). The BSC3 sensor we isolated from BSC3 with a thermal pad, and the power supply was isolated from the pier it is resting on. This is an effort to remove ground loops on these systems. Will revisit next week.
M. Pirello, F. Clara
After review of the data over the week, we saw a marked improvement in temprature information so we reapplied the BSC1 sensor to the chamber along with a thermal pad to maintain electrical ground isolation. We also isolated the power box for both supplies.
M. Pirello, F. Clara, D. Barker