Displaying reports 221-240 of 77236.Go to page Start 8 9 10 11 12 13 14 15 16 End
Reports until 23:58, Thursday 25 July 2024
LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 23:58, Thursday 25 July 2024 - last comment - 00:01, Friday 26 July 2024(79320)
Corner Station Dew Point Measurement

Dew point measurement taken this morning read at -43.4 oC.  Measurement taken before removing HAM6 -X door.  Some demand from HAM5, and HAM6 with soft covers on.

Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 00:01, Friday 26 July 2024 (79321)VE

End of the day dew point measurement, -43.4 oC.  Minimal demand, purge air only open at the purge port at output mode cleaner tube near HAM4.

Images attached to this comment
H1 ISC (SUS, SYS)
jason.oberling@LIGO.ORG - posted 17:13, Thursday 25 July 2024 - last comment - 10:19, Thursday 01 August 2024(79319)
KTP Wedge Assembly Prepped for Swap and Realignment

C. Compton, S. Dwyer, J. Oberling

This afternoon we prepared the KTP wedge assembly for swap and realignment.  Camilla had already mostly prepped a beam path for this using the beam reflected from the PBS cube in front of the Prometheus laser, but there was some oddness with the beam so Sheila and I moved one of the mirrors so we could use the beam transmitted by the PBS cube.  There was still oddness with the beam when at low power (looked like it had a bit of a halo around it), but it went away at a slightly higher power (a couple mW vs just under 1 mW).  Moving on, we aligned the beam along a row of holes and then installed the KTP wedge assembly (after Sheila wiped the area down several times with IPA wipes).  We had removed the beam dump assembly before placing the KTP wedge in the beam path, and the bolts were very tight.  It looked like the black coating on the assembly was also in the threaded bolt holes; this coating had been rubbed off by the bolts during assembly, and it looked like this was the cause of the difficulty in removing the beam dump assembly (there was coating visiblt deep in the threads but none on the outside where the bolt fully contacts the threads).  A HWP was placed in the beam so we could adjust the power in the beams transmitted by the KTP wedge.

With the KTP wedge assembly in place we found the two transmitted beams and set irises in the near and far field, 2 irises for each beam.  We also found the beam reflected from the front surface of the KTP wedge and placed an iris in this beam as well.  I placed beam dumps to block the beams so there are not unblocked beams when the laser gets turned on.  To preserve the cleanliness of the KTP wedge assembly I placed several layers of dry wipes over the assembly and then covered it with foil; I then wiped the area down again with IPA wipes.  The KTP wedge assembly is now ready for the damaged KTP wedge to be swapped with a spare and realigned; Keita and Sheila plan on starting the swap and realignment tomorrow.

I've attached several pictures of the setup and they are, in order:

  1. The 2 near field irises behind the KTP wedge (with beam dump between KTP wedge and the irises)
  2. The near and far field irises
  3. The reflected beam iris and its beam dump
  4. Another picture of the KTP wedge assembly
  5. Foil covering over KTP wedge assembly (with several layers of dry wipes between the foil and the KTP wedge assembly)

NOTE: There is now a Class A assembly in the Optics Lab.  Please observe ALL posted contamination control signs when entering the Optics Lab, and DO NOT enter the far cleanroom (with the Prometheus laser on it) unless you are working on the KTP wedge assembly swap.  This assembly is going back into the vacuum envelope, so we have to do our absolute best to preserve its cleanliness.  Thank you.

Images attached to this report
Comments related to this report
corey.gray@LIGO.ORG - 10:19, Thursday 01 August 2024 (79404)EPO

Tagging for EPO.

LHO VE
janos.csizmazia@LIGO.ORG - posted 16:54, Thursday 25 July 2024 - last comment - 16:03, Friday 26 July 2024(79318)
7-25 vent vacuum diary
Today's activities:
- The purge air dew point was measured at the purge port: (9:15 am) -43.9 deg C, so it is consistently dropping in time. Some more specifics here: https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=79306
- HAM6 -X door has been removed. The O-rings seem to be intact
- The opportunity was taken for replacing the HAM6 RGA. It will be also re-wrapped with heat tapes, and after the chamber work ends, will be baked out.
- Pressures: the arms' pressures slowly dropping (probably because of the weather is getting colder). The Y-manifold pressure is stabilized around 2-3E-8 Torr.
Comments related to this report
jordan.vanosky@LIGO.ORG - 16:03, Friday 26 July 2024 (79329)

HAM6 RGA was swapped with a brand new Pfieffer PrismaPro RGA. We had not been able to connect to the old RGA since ~March 24, through the network nor locally using a laptop. The new unit has been installed and is currently prepped for bakeout once chamber work has finished.

Images attached to this comment
H1 General
oli.patane@LIGO.ORG - posted 16:32, Thursday 25 July 2024 (79317)
Ops Day Shift End

TITLE: 07/25 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: None
SHIFT SUMMARY: KTP has been removed from the OFI and is in the Optics Lab(79315), where it will be removed and replaced.
LOG:

Start Time System Name Location Lazer_Haz Task Time End
14:00 FAC Chris, Eric LVEA n Starting door removal 14:44
14:52 FAC Karen LVEA n Tech clean 15:32
14:56 FAC Kim LVEA n Tech clean 15:22
15:16 OFI Camilla LVEA n Move AUX laser out of the way 16:28
15:18 FAC Gerardo, Jordan, Tyler, Chris, Eric, Janos LVEA n Taking HAM6 door off (Eric, Chris, Tyler out 16:10)(Janos out 16:16) 16:28
15:25 FAC Richard LVEA n Watching door removal 15:33
15:28 EE Fil MY n Picking up parts 15:52
16:03 FAC Kim H2 n Tech clean 16:17
16:27 OFI Camilla, Jason LVEA n OFI work 18:51
16:49 OFI Tony LVEA n Taking tiny magnet in big bag out to OFI team 17:03
17:05 FAC Eric, Chris EX n Fan swap 18:56
17:08 FAC Richard LVEA n Watching OFI work and trying not to laugh 18:35
17:29 OFI Keita OpticsLab y(local) Prep for KTP 20:02
17:32 OFI Sheila LVEA n Helping with OFI and looking for cube 18:56
17:33 PEM Robert, Carlos, Millie along YARM n PEM work for CE 19:29
17:35 VAC Gerardo, Jordan LVEA n Checking RGA for leaks 18:19
18:49 FAC Richard LVEA n Checkingn out work 19:32
20:24 VAC Janos, Jordan LVEA n Looking for parts 21:54
21:15 OFI Sheila OpticsLab y(local) Working on KTP optic 22:54
21:25 OFI Camilla OpticsLab y(local) Working on KTP optic 22:47
21:29 OFI Jason OpticsLab y(local) Working on KTP swap ongoing?
H1 ISC (SUS, SYS)
jason.oberling@LIGO.ORG - posted 14:14, Thursday 25 July 2024 - last comment - 10:19, Thursday 01 August 2024(79315)
KTP Wedge Assembly Removed from OFI

C. Compton, S. Dwyer, J. Oberling

This morning we removed the KTP wedge assembly (D2000038) from the OFI and moved it into the OSB Optics Lab.

We began by trying the "transport shims" that are supposed to help secure the OFI.  Unfortunately, these did not work.  The slot in the shims was not wide enough to fit around the OFI Earthquake Stop Posts we were supposed to fit them around, and the shims were too skinny (the posts bottomed out before contacting the shims).  So we had to pivot to Plan B, which was to use dog clamps instead.  This mostly worked, but the OFI still moved around enough that we decided one of us would try to support the OFI while the other turned bolts.  Camilla has some pictures of this and will post as a comment to this alog.  Even still, we managed to almost immediately dislodge one of the OSEM magnets (the one near the lone +X/+Y OSEM) as soon as we started trying to remove the KTP wedge assembly (the magnet is still stuck to the flag on the OFI, will need to have its polarity checked and be put back in place).

We first placed a teflon sheet in between the KTP wedge and the quartz rotator assembly.  Using non-magnetic tools (a titanium hex key that had been bent so it would fit in the space between the KTP and FS wedges, and a beryllium copper one that had been cut short) we attempted to remove the beam dump assembly from the KTP wedge assembly.  Camilla held the OFI and I tried to loosen the bolts holding the beam dump on the KTP wedge.  I say "tried" because the bolts are frozen in place.  We were unable to get them to move, at all.  Pivoting again, we found that the beryllium copper hex key was short enough to fit under the beam dump assembly, so we began loosening the two bolts on the +Y side of the KTP wedge assembly; Camilla had to crawl in the -X door to access the -X bolt while I held the OFI.  This worked until the -X bolt was loose enough that we could no longer fit the hex key under the beam dump assembly.  At this point Sheila used a T-shaped titanium hex key to loosen the -Y bolt on the KTP wedge (the bolt directly under the quartz rotator) while I held the OFI, and then I loosened the +X bolt.  With these 2 bolts loose we were able to lift the KTP wedge assembly enough that Camilla could fit the hex key under the beam dump assembly again.  In this way were able to slowly work the -X bolt free.  With all bolts free I carefully removed the KTP wedge assembly while Sheila held the OFI.  We Ooohh'd and Ahhhh'd at the craters in the KTP wedge for a bit and took some photos (see attached), and Camilla and Sheila grabbed some more pictures of the back side of the FS wedge (more access, and therefore better viewing, with the KTP assembly out of the way).  We also removed the teflon sheet from in front of the quartz rotator.

We ensured all of the non-magnetic tools were separate from other tools in the cleanroom, safely wrapped up the tools we would need as well as the KTP wedge assembly, and moved everything to the optics lab to start prepping for swapping and realigning the KTP wedge assembly (the beam dump assembly will have to be removed in the Optics Lab).  I've attached a few closeup pictures of the KTP; 2 are viewing the front surface and one is viewing the back surface (better view of the coating damage around the craters).  Camilla has several other pictures that she'll attach as a comment to this alog.

Images attached to this report
Comments related to this report
camilla.compton@LIGO.ORG - 16:02, Thursday 25 July 2024 (79316)

Note on the  D1300098 OFI Transport shims, looking at 3.1.2 and 4.2.1 of E1300056-v4, it appears we were trying to use them incorrectly and should replace the Earthquake Stop Posts with 1/4-20 bolts. We could try this next week but it would involve removing another shroud panel to get clearance... 

The first three photos attached show the OFI with the KTP removed, and looking through the FS towards the magnets. Third one shows splatter on FS.

Forth/fifth photos show the dog clamps we used to help support the sled and the osem magnet that got turned over: photo

Images attached to this comment
corey.gray@LIGO.ORG - 10:19, Thursday 01 August 2024 (79403)EPO

Tagging for EPO.

H1 General
anthony.sanchez@LIGO.ORG - posted 13:48, Thursday 25 July 2024 (79314)
PCAL Lab Log From Spring 2023 to Summer of 2024

PCAL has had a Paper Log of all the measurements taken from Spring2023 to Summer2024.
Since Jun24, We have switched over to a google Doc PCAL-Lab-Log, a new log will likely be made by the scripts in the near future.

Non-image files attached to this report
H1 TCS
oli.patane@LIGO.ORG - posted 08:48, Thursday 25 July 2024 (79312)
TCS Chiller Water Level Top-Off FAMIS

Closes FAMIS#27794, last checked 79168

TCSX: At 30.3. No water added.

TCSY: At 10.5. No water added.

No leak in water cup

H1 PSL
anthony.sanchez@LIGO.ORG - posted 08:36, Thursday 25 July 2024 (79311)
PSL Status weekly report

FAMIS 26270


Laser Status:
    NPRO output power is 1.822W (nominal ~2W)
    AMP1 output power is 65.16W (nominal ~70W)
    AMP2 output power is 138.0W (nominal 135-140W)
    NPRO watchdog is GREEN
    AMP1 watchdog is GREEN
    AMP2 watchdog is GREEN
    PDWD watchdog is GREEN

PMC:
    It has been locked 15 days, 21 hr 10 minutes
    Reflected power = 18.79W
    Transmitted power = 108.0W
    PowerSum = 126.8W

FSS:
    It has been locked for 7 days 17 hr and 43 min
    TPD[V] = 0.7268V

ISS:
    The diffracted power is around 2.4%
    Last saturation event was 8 days 18 hours and 55 minutes ago


Possible Issues:
    PMC reflected power is high

LHO VE
david.barker@LIGO.ORG - posted 08:11, Thursday 25 July 2024 (79310)
Thu CP1 Fill

Thu Jul 25 08:08:24 2024 INFO: Fill completed in 8min 20secs

Jordan confirmed a good fill curbside.

Images attached to this report
H1 General
oli.patane@LIGO.ORG - posted 07:33, Thursday 25 July 2024 (79309)
Ops Day Shift Start

TITLE: 07/25 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
OUTGOING OPERATOR: None
CURRENT ENVIRONMENT:
    SEI_ENV state: MAINTENANCE
    Wind: 4mph Gusts, 2mph 5min avg
    Primary useism: 0.01 μm/s
    Secondary useism: 0.06 μm/s
QUICK SUMMARY: We went to laser safe yesterday afternoon and are ready for today's work

Today's plan:

H1 ISC
sheila.dwyer@LIGO.ORG - posted 22:22, Wednesday 24 July 2024 (79308)
HAM5 alignment laser set up complete

Jason, Jenne, Camilla, Keita, Francisco, Naoki, Sheila. (Please see Francisco's alog for more details 79300)

Today we got the alignment laser set up and the sqz beam checks done in a way that we think is good enough to move forward with removal of the KTP tomorow.  There are more detailed notes in other alog drafts, and photos coming. 

We found this morning that the beams were not where they were left last night on the OM1 + retro reflection irises.  We decided that this was likely due to the wobbly mount with sticking knobs that the steering mirror was in, this would change the alignment from being touched, and sometimes turning the knob did not adjust the alignment because the knob wasn't engaged.  We decided to swap this mount out which took some time, but after that things went smoothly, and with about 3 iterations we were able to center the beam on SR2.  We then did a quick check of the squeezer beam, which goes through the OFI and returns to OM1.  We got some cool photos of showing a hole in the middle of the beam; we intentionally set it's alignment to go through the most recent crater. 

We are ready to go to laser safe, and the door crew plans to take HAM6 door off in the morning.  After that we will remove the KTP assembly.

H1 ISC
francisco.llamas@LIGO.ORG - posted 22:17, Wednesday 24 July 2024 - last comment - 10:18, Thursday 01 August 2024(79300)
HAM 5 laser alignment day 3

Camilla, Jason, Jenne, Keita, Sheila, Francisco, Naoki

Summary: We are done for AUX laser alignment and power measurement of AUX laser. SQZ beam got to OM1, but we did not do power measurement due to noisy seed dither lock. The following are a mixture of notes between Camilla, Francisco, and Naoki regarding the changes done today:

Aiming for 2 1/4" above EQ stop as 4" between vertical stops and the center of SR2 optic is 5.5mm above center line of EQ stops.

At start of the day, someting had drifted (mainly pitch), re-centered AUX laser on irises.

*Iterating moving auxiliary laser mirror and beamspiltter to center in om1 and retroreflection irises.*

Checking position at SR2:

Swapped the AUX laser steeing mirror to a better optic mount and not woberly perdistal, we are blaming this for our drift.

Jenne also adjusted SRM sliders to yesterdays values.

*Iterating moving auxiliary laser mirror and beamspiltter to center in om1 and retroreflection irises.*

Checking position at SR2:

Moved SRM osems from (175, 140) to (50,190). In pitch moved -125urad from 175 to 50 on osems. In yaw moved +50urad. this was 140 to 190 on osems
Aiming to center the beam on SR2


*Iterating moving auxiliary moving mirror to center in om1 and retroreflection irises.*

Checking position at SR2:

EQ stops are 2 1/2 in away from each other; center is 1 1/4 in from horizontal EQ stop

Will do 100 microrad in -YAW, then check retro in OM1. -100urad in yaw is 190 to 90 on osems

*Iterating moving auxiliary moving mirror to center in om1 and retroreflection irises.*

Checking positions at SR2:

In yaw going +300 urad. This is 90 to 390 on osems.

*Iterating moving auxiliary moving mirror to center in om1 and retroreflection irises.*

Checking positions at SR2:

*LUNCH BREAK*
 


Sheila back to SR2;

earlier today SRM P moved from 179 to 50. 1 1/4 inch move on SR2

Moved 1/4 inch backward. moved SRM P from 50 to 76

Sheila is happy with SR2 centering.

Jason is setting iris on OM1. Beam on OM1 ugly? due to crater on OFI?

ASC_AS_C P -0.6 Y -0.6

open GV for HAM7. send SQZ beam. seed dither lock is very noisy.

SQZ beam is close to AUX laser?

AUX power measurement

Comments related to this report
camilla.compton@LIGO.ORG - 13:49, Thursday 25 July 2024 (79313)

First three attached photos are of the aux laser steering mirror we swapped in, original mirror in 79253.

Fourth photo is the iris we places between the aux laser beamsplitter and SRM. Once we were finished with the alignment Jenne and Sheila recentered this iris on the beam. 

The power measurements recorded are with the AUX laser as we had trouble dither locking the SQZ seed beam. More details:

  • 1.72mW before SRM (SR2 side)
  • 0.605mW just after SRM (Good, expect 0.602mW =  35% transmitted = 0.35 x 1.72mW)
  • 0.45mW after KTP and TGG before TFP (expect 100% throughput so are loosing 25% through OFI)
  • 0.380mW before OM1 (some power lost through wring polarization to OFI rejected path? Didn't confirm).
Fifth image is the SQZ beam after passing through the OFI and SRM. Can see a big whole in the middle of the beam!! We expect this is from passing through the KTP crater! Still not easy to tell which crater the beam is passing though.
Note that the aux laser beam is too small to tell by eye if there is a hole in it, but once we got the alignment better, the beam quality seemed to decrease and the beam become dimmer.

Sixth image is the SQZ beam and aux laser beam (smaller) after SRM. They are misaligned in yaw. 

Seventh image is te  SQZ beam and aux laser beam (below) before OM1. They are misaligned in pitch.

Images attached to this comment
corey.gray@LIGO.ORG - 10:18, Thursday 01 August 2024 (79402)EPO

Tagging for EPO.

LHO VE (VE)
gerardo.moreno@LIGO.ORG - posted 17:38, Wednesday 24 July 2024 - last comment - 17:42, Wednesday 24 July 2024(79306)
Corner Station Dew Point Measurement

Dew point measurement taken this morning by Jordan, read at -43.9 oC.  Some demand by HAM5/6, small crew at work.

Images attached to this report
Comments related to this report
gerardo.moreno@LIGO.ORG - 17:42, Wednesday 24 July 2024 (79307)VE

End of the day dew point measurement, -43.6 oC.  No demand, all soft covers closed for HAM5/6 and HAM7 is under small pressure and isolated.

Note regarding HAM7: before the 10" gate valve is open, chamber needs a blow down, see a vacuum representative.

Images attached to this comment
H1 General
oli.patane@LIGO.ORG - posted 16:37, Wednesday 24 July 2024 (79305)
Ops Day Shift End

TITLE: 07/24 Day Shift: 1430-2330 UTC (0730-1630 PST), all times posted in UTC
STATE of H1: Corrective Maintenance
INCOMING OPERATOR: None
SHIFT SUMMARY: The OFI team was able to get the AUX laser aligned and verified that the SQZ beam can get to OM1. Tomorrow morning first thing we will be transitioning the LVEA to laser safe and continuing the OFI work by taking the KTP out and taking the HAM6 -X door off.
LOG:

- Continuing work on aligning AUX laser

- Aligning sqz beam

- Getting ready to transition to laser safe

Start Time System Name Location Lazer_Haz Task Time End
15:11 FAC Kim, Karen LVEA YES Tech clean, (Karen out at 1600) 16:23
15:20 VAC Jordan LVEA YES Checking purge air 15:31
15:41 OFI Camilla, Jason, Sheila HAM5 Y AUX laser work 19:41
16:10 OFI Keita LVEA YES OFI work 19:41
16:11 FAC Richard LVEA YES Checking in on OFI work 17:34
16:38 FAC Karen WoodShop n Tech clean 17:27
17:25 FAC Kim MX n Tech clean 18:27
18:09 FAC Karen EY n Tech clean 18:58
18:28 OFI Francisco LVEA YES Helping with OFI 19:41
19:12 ISI Jim EY n Recovering EY from HEPI/ISI trip 19:46
19:15   Richard LVEA YES Checking in on OFI peeps 19:41
20:41 OFI Camilla LVEA YES More AUX aligning for OFI 23:30
20:50 OFI Jenne, Naoki, Sheila, Jason LVEA YES Continue AUX alignment work for OFI (Sheila, Jenne out 22:55)(Naoki our 23:08)(Jason out 23:27) 23:27
21:51 VAC Gerardo LVEA YES Purge air for HAM7 22:02
21:29 VAC Janos EY n Purge air photos 21:48
21:49 FAC Tyler LVEA YES Prepping for HAM6 door removal 21:52
22:10 OFI Keita LVEA YES OFI help 22:55
23:08 EE Marc, Fil MY n Looking for parts ongoing
23:09 FAC Tyler LVEA YES More prep work for HAM6 door 23:13
H1 ISC
jennifer.wright@LIGO.ORG - posted 16:29, Wednesday 24 July 2024 (79304)
Mode-matching calculation for AUX laser injection from HAM6 to HAM5

Keita, Jennie W

Keita and I worked out the distance behind SRM we have to place the AUX launcher to match the beam radius the IFO beam normally has on SRM on its way into the OFI.

This is based on measurements of beam profile Keita made in the optics lab with the aux laser mounted with a collimator on it.

The code used to do this is saved in ligo/home/jennifer.wright/ModeMatching/beam_diverg.py

The graph attached shows the measured points in orange and the fitted points in blue.

Beam waist, w0 is 0.916 mm
Beam waist position in relation to front of launcher , z0 is -1.423 m
Rayliegh range for beam, z_R is 2.477 m
Move launcher 3.986 m away from SRM
Distance between OM1 and SRM is 3.646 m
 
Therefore we propose installing a steering mirror at right angles to OM1/SRM line to get this longer distance to SRM.
 
Images attached to this report
Non-image files attached to this report
H1 PSL
ryan.short@LIGO.ORG - posted 15:55, Wednesday 24 July 2024 (79303)
PSL 10-Day Trends

FAMIS 21009

The stabilization trends are especially interesting this week; PMC reflected power is steadily increasing while transmitted power (along with RefCav transmission and ISS diffracted power) is decreasing. This is particularly interesting as we thought this behavior might disappear when we swapped in the new PMC.

Images attached to this report
H1 PEM
genevieve.connolly@LIGO.ORG - posted 12:10, Wednesday 24 July 2024 - last comment - 13:47, Wednesday 24 July 2024(79284)
~40 Hz peak(s) investigation in HAM ISIs and PEM accelerometers

Sam and I have been investigating a ~40 Hz peak in the HAM ISIs and PEM accelerometers, first noticed by Camilla and Sheila in alogs 79001 and 78879. Jim also investigated and suggested the peak may be caused by gain peaking from the isolation loops (alog 79145). The peak is strongest in HAMs 2, 6, and the LVEAFLOOR YCRYO Z accelerometer. We tracked the first appearance of the peak to May 20th. We've found there are actually two peaks roughly 0.2 Hz apart, which drift a bit in frequency from ~39.45 Hz (20/05/24 16:00 UTC) to ~40.2 Hz (20/05/24 22:00 UTC), measured from the point between the two peaks (see 1st attachment). The peaks consistently remain about 0.2 Hz apart in frequency but they do not always have the same magnitude ratio, even between channels measured at the same time (see 2nd attachment). Overall, the peaks vary in magnitude, occasionally disappearing altogether, but we have yet to find a time when one peak disappears and the other doesn't (see 3rd & 4th attachments for peaks disappearing and reappearing, respectively). We'll continue looking into surrounding peaks and the coherence with DARM.

Images attached to this report
Comments related to this report
jim.warner@LIGO.ORG - 13:47, Wednesday 24 July 2024 (79302)SEI

The extra drive on HAM2 is likely from a very thin phase margin on the HAM2 X feedback loop. I measured this yester day and found that it had something like 5 deg of phase margin with a 32-ish hz ugf. I backed this off quite a bit, phase margin is now around 20deg and the ugf is more like 27 hz. Might be worth doing some quick checks on these for all the ISIs. Measurements of the X ugf and phase margin are attached. Red is the modified loop I installed yesterday, blue is the loop with the filters that have been running up to that point, not sure when the last measruements were run, it's been a while.

Images attached to this comment
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