Displaying reports 50521-50540 of 75211.Go to page Start 2523 2524 2525 2526 2527 2528 2529 2530 2531 End
Reports until 12:30, Wednesday 03 February 2016
H1 TCS (TCS)
aidan.brooks@LIGO.ORG - posted 12:30, Wednesday 03 February 2016 (25353)
TCS CO2Y aligned to center of ITMY - position uncertainty ~ 20 mm, thermal tilt uncertainty ~ 400 nrad

[Aidan, Alastair]

Per the discussion on the position dependent coupling of CO2 noise to DARM, we injected a 23.8Hz line into CO2Y yesterday (using a function generator) yielding a 1.5E-2 /sqrtHz line in RIN for that laser.

We turned the laser on to inject 100mW onto ITMY. A line appeared in DARM at 23.8Hz

We used PICO_G Motor 3 to steer the TCSY beam around on ITMY and observed the magnitude of the line in DARM. By eyeballing the live spectra, I could roughly maximize the line around PICO motor counts [-1E4, 3E4]. Then we swept the beam in the vertical direction on the mirror until the line disappeared in DARM. We reversed the direction of the sweep, moving the beam through maximum coupling through to minimum coupling again. We returned the beam to the rough position of maximum coupling and repeated the procedure in the horizontal direction.

The results were a bit noisy. We used the following channels to track the position of the PICO_G mirror and the line magnitude vs time.

We left the mirror at position [-1E4, 3E4] last night.

Following the scanning, I analyzed the data this morning and found that the, despite being noisy, we could estimate the maximum coupling point as [-5E3, 3.1E4] with an uncertainty of approximately +/- 3000 counts. I moved the mirror to this position this morning.

----

A word on the uncertainty:

We can estimate the maximum single-pass thermal tilt we should see because of the uncertainty in the alignment:

If we operate the TCS in the range [0, 500mW], then we should anticipate up to 400nrad of thermal tilt induced in the IFO beam

Non-image files attached to this report
H1 PSL
jeffrey.bartlett@LIGO.ORG - posted 12:19, Wednesday 03 February 2016 (25355)
FAMIS #4136 Weekly PSL Chiller Top-Off
Added 200ml water to Crystal Chiller. 

Peter K. added 350ml water to the Diode chiller (see aLOG #25343)  
H1 AOS
jeffrey.bartlett@LIGO.ORG - posted 12:05, Wednesday 03 February 2016 (25354)
FAMIS #1935 Monthly HEPI Pump Trends
Ran HEPI Pump Trends per FAMIS #1935. End-Y showed a cavitation after the power outage, which was corrected.  
Images attached to this report
H1 General
jeffrey.bartlett@LIGO.ORG - posted 10:57, Wednesday 03 February 2016 (25349)
FAMIS # 4341 STS Centering Check
Results from STS Centering Script:

All STSs prrof masses that within healthy range (< 2.0 [V]). Great!


Here's a list of how they're doing just in case you care:
STS A DOF X/U = 0.426 [V]
STS A DOF Y/V = -1.085 [V]
STS A DOF Z/W = -0.267 [V]
STS B DOF X/U = 0.688 [V]
STS B DOF Y/V = 0.468 [V]
STS B DOF Z/W = 0.405 [V]
STS C DOF X/U = 0.533 [V]
STS C DOF Y/V = -0.546 [V]
STS C DOF Z/W = -0.956 [V]
STS EX DOF X/U = 0.521 [V]
STS EX DOF Y/V = -1.057 [V]
STS EX DOF Z/W = 0.456 [V]
STS EY DOF X/U = 0.519 [V]
STS EY DOF Y/V = 0.741 [V]
STS EY DOF Z/W = -0.28 [V]

H1 GRD
thomas.shaffer@LIGO.ORG - posted 10:56, Wednesday 03 February 2016 (25348)
Guardian Manager Map Script

I forgot to alog this, its been usable for a few weeks now.

I made a script that will create a map of all the nodes and who is managed by whom. It uses the same packages as the normal Guardian maps for a similar look, and the same colors as the medms. The script will only map the current management, so if managers change, it will have to be re-ran for a new map. I will try to make this better later, but for now this will have to work.

Location: /opt/rtcds/userapps/release/guardian/manager_map.py

I attached a sample output.

Images attached to this report
H1 General
jeffrey.bartlett@LIGO.ORG - posted 10:23, Wednesday 03 February 2016 - last comment - 11:39, Wednesday 03 February 2016(25347)
FAMIS #4365 T240 Centering
T240 Centering script results:

There are 18 T240 proof masses out of range ( > 0.3 [V] )!
ITMX T240 1 DOF X/U = -3.297 [V]
ITMX T240 1 DOF Z/W = 0.439 [V]
ITMX T240 2 DOF Y/V = 0.505 [V]
ITMX T240 3 DOF X/U = -3.301 [V]
ITMX T240 3 DOF Z/W = -0.341 [V]
ITMY T240 1 DOF X/U = -0.433 [V]
ITMY T240 1 DOF Y/V = 0.359 [V]
ITMY T240 1 DOF Z/W = 0.34 [V]
ITMY T240 2 DOF Y/V = 0.43 [V]
ITMY T240 2 DOF Z/W = -0.345 [V]
ITMY T240 3 DOF X/U = -0.941 [V]
ITMY T240 3 DOF Y/V = -0.319 [V]
ITMY T240 3 DOF Z/W = -3.275 [V]
BS T240 1 DOF Y/V = 0.904 [V]
BS T240 1 DOF Z/W = 0.384 [V]
BS T240 2 DOF X/U = 0.96 [V]
BS T240 2 DOF Z/W = 0.481 [V]
BS T240 3 DOF Z/W = 0.927 [V]


All other proof masses are within range ( < 0.3 [V] ):
ETMX T240 1 DOF X/U = 0.158 [V]
ETMX T240 1 DOF Y/V = 0.143 [V]
ETMX T240 1 DOF Z/W = 0.19 [V]
ETMX T240 2 DOF X/U = 0.061 [V]
ETMX T240 2 DOF Y/V = -0.052 [V]
ETMX T240 2 DOF Z/W = 0.168 [V]
ETMX T240 3 DOF X/U = 0.153 [V]
ETMX T240 3 DOF Y/V = 0.008 [V]
ETMX T240 3 DOF Z/W = 0.113 [V]
ETMY T240 1 DOF X/U = 0.066 [V]
ETMY T240 1 DOF Y/V = 0.006 [V]
ETMY T240 1 DOF Z/W = 0.046 [V]
ETMY T240 2 DOF X/U = -0.126 [V]
ETMY T240 2 DOF Y/V = 0.059 [V]
ETMY T240 2 DOF Z/W = 0.148 [V]
ETMY T240 3 DOF X/U = 0.045 [V]
ETMY T240 3 DOF Y/V = 0.038 [V]
ETMY T240 3 DOF Z/W = 0.152 [V]
ITMX T240 1 DOF Y/V = -0.16 [V]
ITMX T240 2 DOF X/U = -0.227 [V]
ITMX T240 2 DOF Z/W = 0.219 [V]
ITMX T240 3 DOF Y/V = 0.18 [V]
ITMY T240 2 DOF X/U = 0.219 [V]
BS T240 1 DOF X/U = 0.207 [V]
BS T240 2 DOF Y/V = 0.182 [V]
BS T240 3 DOF X/U = 0.072 [V]
BS T240 3 DOF Y/V = 0.241 [V]

Comments related to this report
hugh.radkins@LIGO.ORG - 11:39, Wednesday 03 February 2016 (25351)

ITMX & ITMY T240 Masses Centered  WP 5719

JeffB's post of the Mass Positions prompted us to center the ITM ISI T240s.  This was successful.  The BS T240 masses are a bit above action level but not by much; we'll wait a few before we mess with it.

H1 CDS
patrick.thomas@LIGO.ORG - posted 08:41, Wednesday 03 February 2016 (25344)
Reconnected conlog-test-master to channels
Feb. 3 2016 16:38 UTC Reconnected conlog-test-master to the same 99,560 channels are h1conlog1-master.
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 08:20, Wednesday 03 February 2016 (25343)
H1 PSL Chiller
Added 350 ml of water to the diode chiller, as I noticed the red LED was on with the error
message about low water level.
H1 PSL (PSL)
peter.king@LIGO.ORG - posted 04:33, Wednesday 03 February 2016 (25323)
H1 PSL Maintenance
4f H4 looks clean except for a small wipe mark near 1 o'clock close to the
retaining ring.

4f H1 has streaks visible with green light.  Wipe spots between 3 and 6
o'clock.  Possible spot/damage mark in centre of optic.  Hard to see.
Try cleanroom cotton tip to wipe pump light side.  Drag wipe removed
centre smudge.

4f H2 has a streak mark around 6 o'clock near the edge.  Also has a
hard to spot streak lined up with 12 o'clock and is ~3 mm wide.  Not
visible with white light, only seen with green light.

4f H3 has a spot around 7 o'clock near the edge.  Does not blow off.
Spot is ~2-3 mm from the edge.  Possibly on the pump light side of
the optic.  Hard to get to with the quartz rotator in the way.

Re-examined 4f H4 with green light.  Smudge in middle visible.
Vague spot visible under green light from the pump light side.
Spots visible from the pump light side, not visible from the H3 side.
Drag wiped surface, spot is now gone.

Quartz rotator surfaces look good under white and green light.

Spot on resonator side of output coupler, a little more than half
way from the centre to the edge, around 2 o'clock.  Drag wiped
clean.

Perhaps out of an abundance of caution it was good that we examined
the surfaces with green light.  Certainly a few wipe marks that were
present and not visible under a bright light source, were just visible
in green.  It might be that the wipe marks are inconsequential but at
this moment, it seemed prudent to deal with them.

Replaced intra-cavity shutter blade with new model.  The shutter
blades shipped from Livingston do not fit the external shutter as
there is a handedness problem.  EXTERNAL SHUTTER STILL
NEEDS UPGRADING.

Front end laser beam centered through MM2 iris, slightly off
to the left of centre as you look at the MM1 iris.  It is not clear
whether or not the beam was centred in the first place.

12:46 (PT) Turned on front end laser power watchdog.

Original mode matching lens positions:
L02 = 13.38, L03 = 6.42
L02 = 14.26, L03 = 6.35

PMC we have an offset somewhere as it does not lock to the
maximum transmission level unless the power on the locking
photodiode is turned down below the nominal 1.5V unlocked.
Upon some navel gazing, the offset might be due to some light
in the wrong polarisation falling on the photodiode.

ISS - adjusted waveplate until PDA DC = -10.0V and 
PDB DC = -10.16V.  Zeroed ISS QPD; new readings are 
dX = 0.0005 mm, dY = 0.0013 mm.





Jason, Peter
H1 General
travis.sadecki@LIGO.ORG - posted 00:00, Wednesday 03 February 2016 (25342)
OPS Eve Shift Summary

Summary:  Fairly straightforward recovery from maintenance day activities, which didn't end until after 4pm PST.  Several locklosses due to commissioning effort. 

Activity log:

0:04 Kyle back from MY

0:30 PSL crew done

0:39 Fil done

1:07 Jeff K to turn on EY ESD driver

3:37 cleared H1SUSETMY tim error

H1 ISC
evan.hall@LIGO.ORG - posted 23:33, Tuesday 02 February 2016 - last comment - 06:54, Friday 05 February 2016(25341)
RF oddities

There seem to be two new rf oddities that appeared after maintenance today:

Comments related to this report
evan.hall@LIGO.ORG - 13:16, Wednesday 03 February 2016 (25357)

Nothing immediately obvious from either the PR or SR bottom-stage OSEMs during this time. Ditto the BS and ITM oplevs.

Nothing immediately obvious from distribution amp monitors or LO monitors.

Images attached to this comment
evan.hall@LIGO.ORG - 11:28, Thursday 04 February 2016 (25381)

A bit more methodically now: all the OSEM readbacks for DRMI optics, including the IMC mirrors and the input mirrors. No obvious correlation with POP90 fluctuations.

Images attached to this comment
Non-image files attached to this comment
evan.hall@LIGO.ORG - 23:39, Thursday 04 February 2016 (25400)

I am tagging detchar in this post. Betsy and I spent some more time looking at sus electronics channels, but nothing jumped out as problematic. (Although I attach the fast current monitors for the beamsplitter penultimate stage: UR looks like it has many fast glitches. I have not looked systematically at other current or voltage monitors on the suspensions.)

Most likely, noise hunting cannot continue until this problem is fixed.

We would greatly appreciate some help from detchar in identifying which sus electronics channels (if any) are suspect.

In this case, data during any of the ISC_LOCK guardian states 101 through 104 is good to look at (these correspond to DRMI locking with arms off resonance). Higher-numbered guardian states will also show this POP90 problem. This problem only started after Tuesday afternoon local time.

I said above that nothing can be seen in the osems, but that is based only on second-trends of the time series. Perhaps something will be revealed in spectrograms, as when we went through this exercise several months before.

Images attached to this comment
andrew.lundgren@LIGO.ORG - 06:54, Friday 05 February 2016 (25403)DetChar, ISC, SUS
Comparing MASTER and NOISEMON spectra from a nominal low noise time on Feb 3 with Jan 10, the most suspicious change is SR2 M3 UL. Previously, this noisemon looked similar to the other quadrants, but with an extra forest of lines above 100 Hz. Now, the noisemon looks dead.

Attached are spectra of the UR quadrant, showing that it hasn't changed, and spectra of SR2 M3 UL, showing that something has failed - either the noisemon or the driver. Blue traces are from Feb 3 during a nominal low noise time, and red are a reference from science time on Jan 10. I'm also attaching two PDFs - the first is spectra of master and noisemon channels, and their coherence, from the reference time. The second is the same from the current bad time. Ignore the empty plots, they happen if the drive is zero. Also, it seems like the BS M2 noisemon channels have gone missing since the end of the run, so I had to take them out of the configuration. Also, I took out the ITMs, but I should probably check those too.
Images attached to this comment
Non-image files attached to this comment
H1 General (OpsInfo)
travis.sadecki@LIGO.ORG - posted 22:49, Tuesday 02 February 2016 - last comment - 11:51, Wednesday 03 February 2016(25339)
StripTool templates for monitoring Green WFS

Jeff Kissel graciously made 4 StripTool templates for OPS use when having issues with WFS running away during green locking, as happened today.  These templates are:

ALSX_GreenWFS_Pitch_Metrics.stp
ALSX_GreenWFS_Yaw_Metrics.stp   
ALSY_GreenWFS_Pitch_Metrics.stp 
ALSY_GreenWFS_Yaw_Metrics.stp

and can be found in the usual place for OPS templates: /ligo/home/ops/Templates/StripTool.

These will likely be used with the assistance of a commissioner since I didn't catch all the intricacies of manipulating the WFS enough to explain it here, but they are there to save some time when needed.

Comments related to this report
jeffrey.kissel@LIGO.ORG - 10:02, Wednesday 03 February 2016 (25346)ISC
J. Kissel, J. Driggers

A little more information / motivation here. 

There are 4 degrees of freedom when it comes to keeping the green arms aligned: X and Y arms, in both Pitch and Yaw. There are three optics involved in each of these systems -- each arm's ITM, ETM, and TMS. As such, we've constructed a sensor array that has three sensors for each arm: a green WFS A, a green WFS B, and that arm's ITM camera. We've arranged it such that WFS A (in the I phase) is "DOF 1" which is controlled by the ETM, WFS B (again in the I phase) is "DOF 2" controlled by the TMS, and the ITM camera is "DOF3," which is controlled by a little bit of all the optics; ETM, ITM, and TMS -- but mostly the ITM.

As such, each of these templates contain the error signals for each of these loops for the 4 degrees of green alignment. 

The goal during their use: 
Minimize (bring the absolute value toward zero) each of the sensor, or "error," signals, while maximizing the last signal in each template: the (normalized) power stored in the arms.

When you'll typically need these templates:
- Only when trouble shooting the green WFS alignment step of initial alignment, where the "trouble" is that every time the green WFS engage, it steers the arm (X or Y) off into the weeds (in Pitch or Yaw) and breaks the green arm lock. 
- We've found that this will only typically be after a particularly rough event on one (or several) of the chamber's isolation system, for example, an ISI or HEPI platform has tripped. (Or a maintenance day when the SEI platforms are brought down for a model change, or if there's been a site-wide power outage, etc.) 
- In such a case where you have to invoke this technique, it's likely that only one of the error signals is too large for the alignment system to handle.

Strategy:
- Be sure to turn OFF the automatic alignment before getting started. It's the auto-alignment that's the problem, so you must be sure it's not fighting you while you're manually 6pushing the optics to the right place. Do this by heading to the ALS controls overview screen of which ever arm and angular DOF you're fighting (X or Y,  Pitch or Yaw), open each of the WFS "DOF" filters, and turn ON a limit of 0.0 for each. (If you turn OFF the input or output, guardian will fight you and automatically turn these things back ON. No good.)
- Keep the alignment adjustments small (0.1 micro radians on each optic's slider), and make sure to write down where you've started on each so you yourself don't get lost in the weeds.
- Be mindful of the optic indicated by the DOF which has a particularly large error signal. If WFS A error signal is large, it's likely that the ETM should be adjusted.
- The error signals only should be used when the cavity is locked on a zero-zero mode. That means you've got to get the alignment most of the way there *by hand* before using this system. Further, you have to make sure that the *automatic* green alignment system is OFF so that it's not fighting your manual alignment.
- Most typically, it's the camera error signal that's large. Unfortunately that error signal corresponds to a degree of freedom that is control by all three of the optics, so use your best judgement as to which optic to try first (based on your knowledge of what happened to the chambers and optics prior to you starting the alignment process). However, if no major alignment changing events have occured, start with the ITMs. As usual, if you change the alignment of an optic in either direction and it only seems to make all metrics worse, or break the lock, then that's not the problem optic!
- Once you have the error signals relatively small (Under +/- ~1000 - 2000 counts for the WFS, Under +/- ~0.1 to 0.2 counts for the Camera), re-engage the auto-alignment by releasing the limits of 0.0 in each of the "DOF" filter banks.
- Rinse and repeat until the arm cavity stays locked on the 00 mode with the auto-alignment engaged.
jenne.driggers@LIGO.ORG - 11:51, Wednesday 03 February 2016 (25352)

In Jeff's first paragraph, he forgot to include the other 2 degrees of freedom: the input beam pointing, which is defined by the TMS for the green lasers.  So, there are 6 degrees of freedom for each arm.

H1 General (GRD, SEI)
travis.sadecki@LIGO.ORG - posted 22:01, Tuesday 02 February 2016 - last comment - 08:54, Wednesday 03 February 2016(25338)
OPS: reset of HEPI L4C Accumulated WD Counters

I have reset all WD saturation counters for the platforms with warning. 

Also, I reset the HAM6 watchdog counter, which is not found on the OPS_HEPI_L4C_WD_SAT_CUSTOM.adl screen.  However, I was notified that HAM6 watchdogs were beyond 75% full via DIAG_MAIN.  Perhaps we should add HAM6 to this MEDM screen?  Or maybe not, since this seems to have been an ACT saturation, not an L4C??

See attached pics for details of what was reset.

Images attached to this report
Comments related to this report
travis.sadecki@LIGO.ORG - 23:28, Tuesday 02 February 2016 (25340)

I had to reset the HAM6 WD again after a lockloss.  Note: this happened the first time when I was clearing L4C counters, but I attributed it to the warning of 75% full.  Maybe something else is going on here.  Attached is another screenshot.

Images attached to this comment
jim.warner@LIGO.ORG - 08:54, Wednesday 03 February 2016 (25345)SEI

Hugh has noted in the past that this ISI seems to be holding an larger than normal offset in Z, based on actuator drives in alog 19528. The ISI tripped on a vertical actuator, so relieving this offset may make HAM6 trips less likely.  Of course this trip  was caused by drives way over the actuator limits, so something else may be going on.

Images attached to this comment
H1 SUS
jenne.driggers@LIGO.ORG - posted 20:35, Tuesday 02 February 2016 (25336)
BS coil driver lockloss - now with data!

[Jenne, JeffK, EvanH, Travis]

On our very first lock attempt (that made it past DRMI) after today's maintenence, we lost lock during the BS coil driver switching state.  Thanks to today's data saving work (see alog 25329), we now have some data to look at!

Attached are 2 figures of the same lockloss, one of which shows the whole time we were in the COIL_DRIVERS state, and the other zoomed in on the lockloss itself. On the top row of these figures, the left 3 plots are just power buildups, to indicate when the lock was actually lost.  The right-most plot is the ISC guardian state - state 505 is COIL_DRIVERS.  The bottom row of plots are the new FASTIMONs for each OSEM of the BS M2 stage.

These channels are plotted in units of ADC counts, but we have 40V/2^16 counts over a 40 ohm resistance, and the BS M2 actuation strength is about 1N/A.  The features in the LL channel are of order 100 counts, which corresponds to about 15 microNewtons.  For longitudinal, this is of order 60 nm of a kick to the BS.  The rms for MICH control above 10Hz is only 1e-14 m, so this is 6 orders of magnitude above the rms.  For pitch and yaw, this corresponds to about a 2 urad kick to the BS.  (Newtons to meters or radians from T1200404).

This seems like plenty to explain our locklosses. Next up: what to do about it?

Images attached to this report
H1 CDS
david.barker@LIGO.ORG - posted 17:57, Wednesday 27 January 2016 - last comment - 11:46, Wednesday 03 February 2016(25216)
Count of RFM IPC channels on H1 and L1

H1 has 30 sender RFM channels on each arm, of which only 26 have corresponding receiver(s). So 4 are being sent and no model is using the data.

L1 has 29 senders on the X-ARM (of which there are 26 receivers), and 30 senders on the Y-ARM (of which there are 26 receivers).

So the two sites are very close in number of sending channels.

Analysis details: The base number of potential senders was derived from the main IPC file, looking for RFM0 and RFM1 ipc types. This resulted in 30 for H1-X and H1-Y, and 42 for L1-X and L1-Y. Because the ipc file is only appended to during compilation, if it has not been cleanly regenerated recently it may overcount the number of sending channels.

For each channel, I searched the models' RCG generated IPC_STATUS.adl medm file for the channel name (e.g. H1LSC_IPC_STATUS.adl). Assuming that no two ipc channels share the same name, if I found the channel name in the adl file this means it is a running sender with a receiver. For the remaining possible senders without receivers (H1-X=4, H1-Y=4, L1-X=16, L1-Y=16) I looked for the channels in the top level simulink source files (e.g. /opt/rtcds/userapps/release/*/l1/models/l1*.mdl). This showed that all four channels on H1-X and H1-Y do have sending models, and for L1-X 3 of the 16 had sending models, and for L1-Y 4 of the 16 had sending models.

If we can possibly remove some of the RFM channels which are not being received, additional RFM channels can be added to the loop with no risk.

For H1 the sending channels with no receivers are:

Comments related to this report
jeffrey.kissel@LIGO.ORG - 11:03, Friday 29 January 2016 (25240)CAL, SEI
Tagging people interested in adding new (or rather, trading for) RFM channels.

SEI: IFO Basis SEI channels

CAL: Sending PCAL excitations to the corner.
brian.lantz@LIGO.ORG - 11:46, Wednesday 03 February 2016 (25350)
Dave,
Thanks for the count.
For the SUSpoint motion in the IFO basis, (see  ECR E1600028 , or  Integration Issue 1193 , or  Tech Doc T1500610 )

we need 2 RFM channels, 1 per arm for the ETMX SUS-WIT and ETMY SUS-WIT each to OAF in the corner.

For completeness, I note that we also need some PCIe channels from the top level of other 12
suspensions (3 IMCs, 3 SRMs, 3 PRMs, BS, ITMX, ITMY). 

These can replace the GS-13 X/Y signals now being used by OAF. Evidently the RFM senders for these are living in the PEM model at LLO. I do not know why it is done this way, but it may be related to the configuration of the FE machine for ISI at LLO.


ALSO (1) :

for more complete monitoring, it would be useful to also send the STS-2 X/Y signal from the end to OAF.

ALSO (2):
For Earthquake common mode control (still hypothetical) we would need to send the End X or Y STS-2 to the corner, and ALSO send the corner X/Y out to the ends.

Summary of RFM:
1 per arm from SUS to OAF (high priority) 
1 per arm from ISI-GND to OAF (med priority)
1 per arm from GND-ITMY X to End X and ITMY-Y to End Y (med priority)

NOTE- these signals don't need to be 16k. We want accurate data at 1 Hz and below, so 512 sample/sec would be fine. Thus, it is not crazy to think about ways to de-stress the RMF system (e.g. interleave several slow channels on one fast RFM connection, or something like this.)
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