Displaying reports 35841-35860 of 89220.Go to page Start 1789 1790 1791 1792 1793 1794 1795 1796 1797 End
Reports until 00:00, Sunday 09 February 2020
H1 General
jim.warner@LIGO.ORG - posted 00:00, Sunday 09 February 2020 (54986)
Shift Summary

TITLE: 02/09 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 119Mpc
INCOMING OPERATOR: Camilla
SHIFT SUMMARY:
LOG:
0:18 Out of observe for Robert at EX

0:34 Back to Observe

6:44 Switch SEI_CONF to Earthquake for Papua New Guinea 6.0 earthquake

7:14 SEI_CONF back to Windy

 

 

H1 General
edmond.merilh@LIGO.ORG - posted 15:57, Saturday 08 February 2020 (54985)
Shift Summary - Day

TITLE: 02/08 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Observing at 117Mpc
INCOMING OPERATOR: Jim
SHIFT SUMMARY:

LOG:

H1 SUS
rahul.kumar@LIGO.ORG - posted 12:31, Saturday 08 February 2020 (54984)
switching off violin damping for few modes

Switching off the gains for the following SUS, to see if we are over damping them. The current monitor levels are below 0.5, if it rises above this value then I will turn them back ON.

 

1. ITMY - MODE 3, 14

2. ITMX - MODE 11

3. ETMY - MODE 15

4. ETMX - MODE 17

H1 General
edmond.merilh@LIGO.ORG - posted 10:00, Saturday 08 February 2020 (54983)
H1 back to Observing 17:42UTC
H1 General
camilla.compton@LIGO.ORG - posted 08:01, Saturday 08 February 2020 - last comment - 02:53, Sunday 09 February 2020(54981)
Shift Summary - Owl

TITLE: 02/08 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
INCOMING OPERATOR: Ed
SHIFT SUMMARY: Locked until 10 minutes before Ed takes over! Microseism and wind and some ground motion maybe were too much for H1. Handing off with green arms in INCREASE_FLASHES.
LOG:

Comments related to this report
camilla.compton@LIGO.ORG - 02:53, Sunday 09 February 2020 (54988)

The lockloss was very fast with no obvious channel saturations, so maybe it was just a coincidence that it happened around the time of the (small and definitely survivable) EQ.

H1 General
edmond.merilh@LIGO.ORG - posted 07:59, Saturday 08 February 2020 (54982)
Shift Transition - Day

TITLE: 02/08 Day Shift: 16:00-00:00 UTC (08:00-16:00 PST), all times posted in UTC
STATE of H1: Lock Acquisition
OUTGOING OPERATOR: Camilla
CURRENT ENVIRONMENT:
    SEI_CONF state: EARTH_QUAKE
    Wind: 13mph Gusts, 8mph 5min avg
    Primary useism: 0.23 μm/s
    Secondary useism: 0.65 μm/s
QUICK SUMMARY:

H1 TCS
camilla.compton@LIGO.ORG - posted 05:53, Saturday 08 February 2020 - last comment - 14:40, Friday 03 December 2021(54980)
TCSy CO2 Laser has only Kicked us out of Observing Twice since Chiller Swap
Following on from FRS 13095.  Before October we were pushed out of Observing a few times by the TCSy CO2 laser loosing lock. TCSY chiller was swapped 2019-09-18 alog 51996. Flow meter was swapped 2019-10-10 alog 52406.
 
By comparing H1:GRD-TCS_ITMY_CO2_STATE_N with our observation bit and checking logs, I have found only 2 cases since the swap (5months ago) where the TCSy CO2 laser has pushed us out of observing by loosing lock (2019-09-29 23:57 UTC and 2019-12-05 05:41 UTC). The first time being before the flow meter was swapped.
There were 15 times it pushed us out of observing from July 1st to the chiller swap (all between 2019-07-10 and 2019-08-31). Unless something else changed at the end of August I think we can confirm that the original chiller or new flow meter solved our problem.
Attached is the H1:GRD-TCS_ITMY_CO2_STATE_N from May 2019 to now (t1 line = chiller swap. t2 line = flow meter swap). The C02 laser now looses lock to search for a new lock point less regularly and seems to be able to wait until H1 is unlocked. 
Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 22:14, Monday 16 March 2020 (55638)

Happened a third time: 2020-03-17 05:04:09 UTC. Still much reduced since the chiller swap.

camilla.compton@LIGO.ORG - 11:28, Tuesday 02 November 2021 (60493)CDS

Looked back at this after TJ suggested we should check that both chillers are keeping constant temperatures and flow rates. Temperatures in ITMX and ITMY cCO2 chillers seems to be stable. See plot over last 2 years here. As the laser hasn't ben on recently we cannot check how stable it is.

Flow rate reported by ITMX chiller seems to regularly drop from the nominal 3.8 to 2 GPM to up to 10 times an hour. However these drops only last one data point which doesn't effect the laser controller safety controls. See zoomed plot here. The chiller has been like for the past 3.5 years (as far back as I can easily see in EPICS).

2021/09/21 Tuesday 17:30UTC Both ITMX and ITMY chiller temperatures decreased from 22 degC to 19.5 degC. The set point is still at 22degC but the channel H1:TCS-{ITMY/ITMX}_CO2_CHILLER_OUT_GAIN_OUT16 dropped to zero Simulink for h1tcscs . Ndscope trace here. This apears to be the day the h1tcscs model was installed on h1oaf0 - see alog 60002. Tagging cds.

Images attached to this comment
aidan.brooks@LIGO.ORG - 10:46, Wednesday 03 November 2021 (60511)

ECR for upgrading the CO2 controller is here: https://dcc.ligo.org/E1600312

Latest concept for redesigning CO2 controller is attached. Project is stalled right now due to lack of manpower.

 

Non-image files attached to this comment
camilla.compton@LIGO.ORG - 12:59, Tuesday 16 November 2021 (60663)

Daniel fixed this setpoint problem by finding the filters had been removed (see alog 60660).

Once the filters were added back in ~19.15UTC 11/16/2021, the filters seems to be maxed out. Daniel turned off the laser power servo loop (sitemap > TCS > CO2{X/Y} > LASER > ON/OFF for PZT_SERVO_GAIN) and they behaved as expected. These values are not recorded in SDF. It doesn't make sence for the chillers to be tied to the laser when the laser is off so will investigate if the matrix changed. 

 

camilla.compton@LIGO.ORG - 10:07, Friday 03 December 2021 (60842)

The PZT_SERVO_GAIN OUTPUT we turned OFF 2021/11/16 20UTC must have not being svn saved and turned back on on 2021/11/17 22UTC. See attached trend.

The design is to stabilize the laser PZT error signal by controlling the chiller temperature (E1300233p20). When the laser is off this seems to break down and change the have the setpoint given to the chiller (CHILLER_SETPT1) far from the ~20deg setpoint offset H1:TCS-ITM{}_CO2_CHILLER_SET_POINT_OFFSET (seen in TCS CO2 LASER screen). See table below.

TJ and I are looking into these settings. Maybe the matrix gain values or PZT gains are incorrect or the loop should be switched off when the laser is off.

Current values CHILLER_SET_POINT_OFFSET PZT_SERVO_GAIN CHILLER_SETPT1 (setpoint sent to chiller) 
CO2X 20.6 -111 16.6*
CO2Y 20.5 55 22.4

*Documentation states it's important not to let the chillers be +/- 5deg from 20deg otherwise there may be condensation formed in the laser. The chillers have limits to shut off if they get outside this range but only compared to the CHILLER_SETPT1 value. 

Images attached to this comment
camilla.compton@LIGO.ORG - 14:40, Friday 03 December 2021 (60850)

The PZT_SERVO_GAIN OUTPUT is turned off in the CO2 Guardian's DOWN state (well done guardian), running DOWN fixed the problem.

Now the lasers think the set point given to the chillers is 20deg but the chillers are receiving set point request of 22degC. So another issue to solve. 

H1 SUS
cheryl.vorvick@LIGO.ORG - posted 04:39, Saturday 08 February 2020 (54978)
relocking driving some violins, damping with lower gains
  1. TJ asked me to look into PI modes causing the fast lockloss, and I've been watching the violins ring up as H1 tries to relock, and tonight ETMY mode 1 was clearly being driven, as seen in the increase of  the drive.  The first attachment shows 3 unsuccessfil relock and then a 4th lock aquisition,.  The first 3 end in locloss, not necessarily due to violins, but looking at the increase of the amplitude of the drive on this mode, it's being driven with greater amplitude for each relock.  Other modes have the same feature.  The last attachment shows the peak growing.

 

Date UTC Time RMSLP_LOG10 Drive Output
    seconds top of first bounce +/- envelope
         
7 Feb 2020 22:35 UTC T = 0 2 0.009
7 Feb 2020 23:17 UTC T = 2561 4.32 3.4
7 Feb 2020 23:47 UTC T = 4336 4.92 9.8
7 Feb 2020 00:51 UTC T = 8197 5.02 13.4
8 Feb 2020 01:13 UTC T = 9500 5.21 21

 

  1. I looked at the drives for the high gain modes from multiple attempts at relock
    1. IX mode 11, gain = 600
    2. IY mode 14, gain = 500
    3. EY mode 17, gain = 200
    4. EX mode 15, gain = 1500
  2. reduced gains
  3. as soon as I started reducing the high gains, other modes damped with their current gains
  4. damped the high gain modes damped with  values below, others gains reduced if possible
    1. IX mode 11, gain = 10
    2. IY mode 14, gain = 5
    3. EY mode 17, gain = 50 (could likely go lower)
    4. EX mode 15, gain = 10
  5. Then I restored all the nominal damping
Images attached to this report
H1 General
camilla.compton@LIGO.ORG - posted 04:23, Saturday 08 February 2020 (54979)
Mid Shift Summary
Locked 6hours45m. Quiet shift so far.
Still have some 10-20mph winds and high microseism (Secondary useism: 0.51 μm/s). Not too many glitches so staying in WINDY SEI_CONF
H1 General
jim.warner@LIGO.ORG - posted 00:07, Saturday 08 February 2020 (54976)
Shift Summary

TITLE: 02/08 Eve Shift: 00:00-08:00 UTC (16:00-00:00 PST), all times posted in UTC
STATE of H1: Observing at 118Mpc
INCOMING OPERATOR: Camilla
SHIFT SUMMARY: winds were bad
LOG:
0:00 Niko started initial alignment as I came in, winds also started to pick up, got to NLN around 1:00 utc, but winds promptly hit 60 mph and broke the lock, next couple hours were high winds

5:37 back to NLN and observing

H1 General
camilla.compton@LIGO.ORG - posted 00:05, Saturday 08 February 2020 (54977)
Shift transition to Owl

TITLE: 02/08 Owl Shift: 08:00-16:00 UTC (00:00-08:00 PST), all times posted in UTC
STATE of H1: Observing at 118Mpc
OUTGOING OPERATOR: Jim
CURRENT ENVIRONMENT:
    SEI_CONF state: WINDY
    Wind: 19mph Gusts, 13mph 5min avg
    Primary useism: 0.08 μm/s
    Secondary useism: 0.43 μm/s
QUICK SUMMARY: Locked 2h30m. Microseism is on the rise but the winds have died down considerably since Jim was locking.

H1 ISC
jenne.driggers@LIGO.ORG - posted 16:30, Friday 07 February 2020 (54974)
Turning off ASC-AS36Q offset brings buildups down

[Sheila, Jenne]

Sheila remembered that there are some ASC offsets that change in ASC engagement, and pointed out that those could be affecting our ability to lock.  In the attachment we see that the POP18 drops and POP90 comes up a bit when the AS36Q filter banks change their SWSTAT (which is them turning off the offsets).

We put in offsets in the MICH ASC sensor AS36Q when we have DRMI locked before the CARM offset reduction, in preparation for switching from AS45Q to AS36Q.  But, once we're engaging the full IFO ASC, we want to get rid of those offsets.  Sheila had moved the offset turn-off from PREP_ASC_FOR_FULL_IFO to the end of ENGAGE_ASC_FOR_FULL_IFO in September of last year, but maybe we should move it even further down the sequence, to after the arm soft loops have converged. 

However, I'm not sure that this is the thing that is killing the lock, since it happens ~80 seconds before lockloss. 

For now, we've followed the hands-off procedure and since we've had several locklosses in a row, Jim has just completed initial alignment, and we'll see how this acquisition goes.

Images attached to this report
H1 General
yannick.lecoeuche@LIGO.ORG - posted 16:04, Friday 07 February 2020 (54973)
Shift Summary - Day

TITLE: 02/07 Day Shift 16:00 – 00:00 (08:00-16:00), all times posted in UTC

STATE of H1: Locking

INCOMING OPERATOR: Jim

SHIFT SUMMARY: Did some SQZ troubleshooting, followed by commissioning. Lost lock at 22:40, been struggling to relock since then

LOG: 

16:32 (08:32) Chandra to MX/MY -- do an inspection

17:15 (09:15) Leaving Observing to investigate SQZ oscillations

17:29 (09:29) Sheila to LVEA -- continue SQZ investigation

17:37 (09:37) Chandra back from MX/MY

17:55 (09:55) Sheila out of LVEA

18:00 (10:00) Starting scheduled commissioning break

19:27 (11:27) Done with commissioning, going into Observing

22:12 (14:12) Gerardo to MX/MY -- pick up equipment, inspect gauges

22:40 (14:40) Fast lockloss

22:45 (14:45) Gerardo back from MX/MY

22:47 (14:47) Chandra to LVEA

23:00 (15:00) Chandra out of LVEA

23:09 (15:09) Travis to Optics Lab

23:12 (15:12) Travis out of Optics Lab

H1 SQZ
sheila.dwyer@LIGO.ORG - posted 15:36, Friday 07 February 2020 - last comment - 15:22, Monday 24 February 2020(54967)
squeezer green ISS lines at 15kHz and 30kHz seem to degrade range

Keita, Sheila

We had another example of the squeezer oscillations that were seen last weekend:  54864  The first screenshot shows the signals related to gree power in the OPO getting very noisy over ~ 6 hours this morning.  We went out of observing earlier than our planned commisioning time to try to address this.  We turned off the green ISS, which brough all the signals back to normal.  Turning that loop back on brought the noise back.  We also tried reducing the gain in that loop, which did reduce the peak to peak noise seen in the ndscope.  Based on loop measurements taken on Tuesday, 54888, the shape of this loop at its nominal 31dB gain setting should be fine. 

Next I went to the floor, while Keita took spectra and changed the gain from the control room.  On the floor I measured a spectrum of IN1 (the error point) on the green ISS, and I saw large lines at 15kHz and 30kHz.  Keita saw that there is an aliased line at 1249Hz in the spectra in the control room, which would correspond to a line at 15135 Hz.  The height of the 15kHz and 30kHz lines didn't change with gain changes, although the overall noise floor did change.  Ketia disabled the loop, and I could no longer see the lines on the error point, and the low frequency intensity noise increased (as you would expect).  

We then unlocked the squeezer by requesting no squeezing, and relocked it.  We saw no evidence of the 15kHz and 30kHz lines on the analyzer, although the red trace in the second attachment shows that the 1kHz line is still present.  We reset the ISS gain to 31Hz, which is nomal, and everything seems fine for the time being. 

Photos attached (after screenshots):

For operators: 

The first attached screenshot is from the ndscope that is accessible from the upper right corner of the SQZ_OVERVIEW screen, called locking signals.  If you see the range dropping, open this ndscope and see if there is trend similar to what is shown in the attached screenshot that lines up in time with the range drop.  In the left column of the screenshot you can see that the OPO REFL power is changing and the max-min difference gets larger, the max-min difference of OPO_IR_RESONANCE trigger gets larger, and the SQZ_SHG_LAUNCH power max-min difference also gets larger.  If this is happening and corresponds to a range drop, please unlock the squeezer by requesting "NO_SQUEEZING" from SQZ_MANAGER, then once it arrives, request SQZ_READY_IFO.  Once it arrives there hopefully the signals in the ndscope will have returned to normal, if so you can request "SQUEEZING" again.  If not you can try again or call for help. 

Images attached to this report
Comments related to this report
thomas.shaffer@LIGO.ORG - 12:28, Friday 07 February 2020 (54970)OpsInfo

Tagging OpsInfo to propagate the message

sheila.dwyer@LIGO.ORG - 15:22, Monday 24 February 2020 (55261)

During today's calibration time, this oscillation happened again, and Patrick called me so I could make a few more observations.  

  • There are two PZT positions in which the OPO can lock, when the PZT voltages is towards the high end of the range the reflected power is higher because of a misalignment in the OPO (and the trans power is servo'd).  Looking at the trend over the last couple of weeks, the oscillation has only happened when the PZT is in this position and the reflected power is high. The two cursors show examples of this in the attachment, but there are several more examples without cursors. This suggests that we could avoid this problem with a guardian or setting modification that only allows us to use the lower PZT position.  
  • The state of the CLF loop and CLF ISS seem to have no impact on the oscillation.
  • The oscillation stops and starts depending on the OPO green power level, not the AOM drive level:
    • I could stop the oscillation and see it repeatably return if I turned the green ISS set point down (more positive set point meaning less green light in OPO trans).  In the second attachment, the OUTPUTRAMP channel is 0 when the servo is on and 1 when the servo is off.  You can see that at three different times, I increased the ISS_SETPOINT while the servo was on and each time that the setpoint reached -2.582 the oscillation stopped, as you can see by the OPO_TRANS peak to peak dropping.  The OPO trans is also noisy when the servo is off, which might be confusing when looking at this plot. 
    • I tried moving the green power control half waveplate in small steps (which didn't unlock the OPO), to change the operating point of the AOM.  The oscillation happens repeatably at the same OPO trans power, even when the AOM set point has changed. In the second attachment you can see that when I repeated the set point stepping with the picomotor moved, the ISS CONTROLMON signal is at a sligthly different value each time we get to the ISS setpoint of -2.852, but this is still the point where the oscillation stops. 

 

Images attached to this comment
H1 CDS
david.barker@LIGO.ORG - posted 14:12, Friday 07 February 2020 (54971)
ETMX Hardware Watchdog started having periods of noise starting Nov 2019

Richard, Fil, Rahul, Dave:

The EX hardware watchdog (HWWD) starting having periods of low led-monitor signal warning (STAT=8) starting 12th Nov 2019. The transitions between periods of low signal and normal signal occur mostly on Tuesdays. Attached plot shows a 6 month trend of the EX-HWWD STAT channel. Prior to 12th Nov there was little noise, on that date the signal went noisy. The transition back to no noise was Tue 19th Dec 2019, then noisy Tue 07 Jan 2020, then to a short period of low noise Tue 04 Feb 2020. For these transitions there is evidence that the monthly charge measurement may be the trigger. The only transition which does not fit this theory is on Wed 05Feb when it went noisy again at noon local, at this time H1 was in observe.

We will work with Rahul on the next charge measurement in March to see if the LED-mon voltage is indeed varying.

This is not a problem per-se (for example EY HWWD is much more noisy). However it would be nice to know why the HWWD changed its behaviour around 12th November 2020. A look at the alog says that NCAL and PEM PWR work was ongoing in EX at that time.

Images attached to this report
H1 ISC
jenne.driggers@LIGO.ORG - posted 11:42, Friday 07 February 2020 - last comment - 16:16, Friday 07 February 2020(54969)
Checking different DARM offsets

[Sheila, Jenne]

We did a few tests of changing the DARM offset, to see if there are any notable differences in the noise.  In particular, we're looking to see if there are noise terms like RIN from 9MHz that scale with the DARM offset.  Because of this test, the front end calibration is not correct during this time, and so the range reported in the control room is not correct.  The offline calibrated data takes into account the calibration lines, and will correct for these changes, so range on the summary pages should be fine to trust.

Attached is a screenshot of an ndscope showing the DARM offset changes, and the resulting online (incorrectly calibrated) range calculation. 

Analysis of the data is forthcoming, I just wanted to let people who wander into the control room (or our screenshots) what is going on.

Images attached to this report
Comments related to this report
jenne.driggers@LIGO.ORG - 16:16, Friday 07 February 2020 (54972)

We may need to repeat this measurement with the squeezer off, since changing the DARM offset seems to affect the squeezing that we see.

In the attached screenshot, the top plot is whitened DARM, with the time dependent correction applied, and the bottom is SRCL coherence with DARM.  Green is when we had a smaller-than-usual DARM offset, and red is when we had a larger-than-usual DARM offset.  I checked that the CFTD time dependence correction is working by checking that the calibration lines are at the same height in both DARM traces (they aren't the same height if you look at the pre-correction CAL-DELTAL that we plot on the front wall).  So, the differences in the 2 DARM traces are real. 

The high frequency classical noise shouldn't have been affected by changing the DARM offset.  Probably the squeezing angle shouldn't have been either, if there were no weird effects.  But, perhaps changing the DARM offset is changing the SRCL detuning, which would then change the optimal injected squeezing phase angle. 

At low frequency, the extra noise in the green trace is likely mostly due to the excess SRCL control noise in DARM, as seen by the increased coherence. since the SRCL FF is tuned only for our usual DARM offset. 

All that said, since squeezing shouldn't be affecting the noise between 10-30 Hz, it is still probably worth while to subtract away that SRCL noise to see if there is any evidence of 9 MHz noise change (or other noise change) when we changed the DARM offset.

Images attached to this comment
H1 PSL
yannick.lecoeuche@LIGO.ORG - posted 10:16, Friday 07 February 2020 (54968)
PSL Status Report-Weekly

 Laser Status:
    Front End Power is 32.4W (should be around 30 W)
    70W Output Power is 70W
    Front End Watch is GREEN
    70W Watch is GREEN

    PMC:
    It has been locked 9 days, 22 hr 37 minutes (should be days/weeks)
    Reflected power = 11.7Watts
    Transmitted power = 51.9Watts
    PowerSum = 63.6Watts.

    FSS:
    It has been locked for 0 days 16 hr and 3 min (should be days/weeks)
    TPD[V] = 5.367V (min 0.9V)

    ISS:
    The diffracted power is around 2.5%
    Last saturation event was 0 days 16 hours and 2 minutes ago (should be days/weeks)

    Possible Issues:

 

H1 ISC
jenne.driggers@LIGO.ORG - posted 16:45, Thursday 06 February 2020 - last comment - 08:20, Tuesday 11 February 2020(54949)
Commented out unneeded 2 min sleep in MOVE_SPOTS

While watching the lock acquisition, I was surprised at how long we were in the state MOVE_SPOTS before the A2L gains are actually changed.  Looking at the code, it is because there are some sleep statements in there for initializing the TMS centering servo that don't need to be in there. 

Recall that we use a servo (that Craig implemented over the October break) to move the TMSs such that we are centered on the IR trans QPDs, and maintain that centering as we engage ASC and change the IFO alignment.  The first time the servo is used in ENGAGE_SOFT_LOOPS, we are careful to zero the offsets of the TMS TEST filter banks carefully, if they were somehow left on (they get turned off in DOWN).  Then a cds.servo is used, and when we leave the state we leave the TMS in its new pointing. 

The servos are started up again when we go to MOVE_SPOTS.  But, we seem to be resetting the pointing of the TMS before starting the servos up.  The way the reset code was written, it waits 30 seconds to ramp off each TMS offset, but it does it in series, for a total of 2 minutes of sleeping.  We shouldn't be resetting the offsets here, because that erases the centering that was done earlier, so I commented out this whole section which also removed the sleeps. 

It's possible that the IFO liked this 2 min wait to get some time for convergence and thermalization after going up to 10W.  If there are problems at this state, please uncomment lines 3611-3621 in ISC_LOCK to put these sleeps back in (if this is needed, I'll fix them on ~Tuesday so that they are timers and not sleeps, since we're not checking for lockloss during each of these 30 sec sleeps).

 

Separately, we should probably be resetting the A2L gains to their centered locations in PREP_FOR_LOCKING, rather than waiting until PREP_ASC_FOR_FULL_IFO, since we engage DHARD before prep_asc_for_full_IFO.  Seems to not be a big deal, but we are jerking that around on poor DHARD when we set them to their centered values just before turning on the dither lines, so we're changing the amount of DHARD noise injected to DARM.

Comments related to this report
jenne.driggers@LIGO.ORG - 17:12, Thursday 06 February 2020 (54951)

The lines to uncomment are now 3616-3626 if needed, since I added a few lines in PREP_FOR_LOCKING to center the A2L gains (see alog 54950).

sheila.dwyer@LIGO.ORG - 17:27, Friday 07 February 2020 (54975)

We lost lock once in move spots today (after Jim did an initial alignment).  I serached on the lockloss page for locklosses at move spots (506).  We've had two lcoklosses here since this change was made, and we had 3 locklosses from move spots in January.  I rearranged the order of these guardian states on Jan1st, 54219, which is how some of these pauses got in here.  Since we've only had two locklosses, and we made it though for now, I'm not going to make a change, but if we keep having locklosses here it might be that we do need to wait for the TMS servo.

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