Displaying reports 70841-70860 of 77046.Go to page Start 3539 3540 3541 3542 3543 3544 3545 3546 3547 End
Reports until 15:15, Thursday 16 May 2013
H1 SUS
szymon.steplewski@LIGO.ORG - posted 15:15, Thursday 16 May 2013 (6400)
ETMY and ITMY Optical Lever power fluctuations

Thomas V. & Szymon S.

Over the last couple weeks we have noticed that the ETMY optical lever power monitored on the channel H1:SUS-ETMY_L3_OPLEV_SUM_OUTPUT has been periodically fluctuating. The monitored power level has been dropping from a nominal 10,000 counts to 0 counts on a regular interval. Exchanging the power supply on May 3 seemed to have slightly improved the situation with the power level dropping to 6,000 counts from 10,000, but still on a very regular schedule. I tried another spare power supply as well as using a different cable connecting the laser with the power supply. Attached is a plot of how the power level read from the quad photodiode varies after the last change on May 15, still fluctuating.

Testing the power supply pins with a voltmeter I saw the voltage at a steady 5 volts, and no regular power glitch as seen on the oplev sum. Additionally, the laser module for ETMY optical lever is loudly buzzing most likely due to the cooling fan interfering with something inside the chassis.

The ITMY optical lever was installed and aligned a week ago, but has drifted significantly since initial alignment. One theory is that the cables for the electric micrometer stage are forcing the stage holding the QPD to move around. ITMY optical lever plots show that the laser power is wandering in a sawtooth pattern, probably due to drift of the stage.

Images attached to this report
H1 INS
jodi.fauver@LIGO.ORG - posted 14:43, Thursday 16 May 2013 (6399)
HAM4 ISI Install Prep
The Apollo crew flew the forklift from the West Bay to the near side of the LVEA so that it would be available to remove doors. Christina and crew took care of second cleaning by ~9:00 am. Then, the Apollo guys started the assembly of the A-frames used in ISI install. There was also some Apollo help on HEPI actuators.
H1 SUS
jeffrey.kissel@LIGO.ORG - posted 13:52, Thursday 16 May 2013 (6392)
BSFM Damping Loops Commissioned to Reduce Sensor Noise Contribution to Optic Displacement
J. Kissel

In preparation for the HIFO-Y and DRMI integration phases, I've redesigned the H1SUSBS (a BSFM) damping loops in a similar vein as those for the QUAD (see LLO aLOG 6949 and G1300537). I've tried my best to make the figures of merit identical to that of the QUAD, so if you understand those figures of merit, you'll understand these. Unlike the QUAD, however, one can in-almost-all-cases beat the aLIGO requirements with the same, only-slightly-more-complicated, level/style of filters. Vertical turns out to be the trickiest DOF, if you can believe it; it's the only one that I couldn't get below that DOF's requirements at all frequencies. However, as can be seen on pg 1 of dampingfilters_BSFM_2013-05-15.pdf, the vertical noise projected onto DARM is still a factor of ~10 below even the best aLIGO sensitivity (if all coupling factors are correct). Details below!

Note, I've captured a new safe.snap, copied, and committed both the snap and the newly modified filter file to the userapps repo:
${userapps}/sus/h1/burtfiles/h1susbs_safe.snap
and 
${userapps}/sus/h1/filterfiles/H1SUSBS.txt

Details:
--------
Since most of the figures of merit are either self-explanatory or the exact same as what's described in detail in the QUAD design (again, see (see LLO aLOG 6949 and G1300537)), I won't go through them in detail, but instead highlight the interesting points where the BSFM differed from the QUAD.

Design Philosophy / Comments:
(These notes are entirely focused on the dampingfilters_BSFM_2013-05-15.pdf attachment)
- Initially, the focus was on reducing the sensor noise for the L degree of freedom. However, because the BSFM is a very long Triple suspension, the L/P modes are relatively low in frequency. This meant that there's plenty of room between the last L/P mode and the goal frequency of 10 [Hz]. 
- Because the BSFM's blades are not diagonally oriented like they are in the QUAD, there is no fundamental cross-coupling between (T/R) motion and (L/P) motion. (L/P), (R/T), V, and Y are entirely independent of each other.
- These two features of the plant (the highest resonances are at lower frequency, and DOFs are much better decoupled) makes rolling of the sensor noise by 10 Hz relatively easy for these degrees of freedom. 
- Even in the fundamentally cross-coupled degrees of freedom, (L/P) and (R/T), the MIMO interaction between them makes it easy to isolate certain modes, and damp them in DOFs where the noise requirement is less stringent. For example, the highest (R/T) modes at 2.1 and 3.2 [Hz], which are the only substantial modes that show up in the R2R plant, can be almost entirely taken care of in R where there is no requirement. This offloads damping authority from the what-would-be-difficult T design. (That being said, the T requirements are so loose, that even the Level 1 controllers beat the requirement by several orders of magnitude).
- The point at which I stopped tuning the L, P, and Y loops was when the sensor noise was reduced to a factor of a few below the M2 actuator noise (as shown on pgs 2/10, 34, and 40). They probably could be made more aggressive, but until the M2 actuator noise is reduced, there's no point. (Remember, there are no actuators on the M3 / optic stage of the BSFM).
- An interesting diversion from the QUAD design for these DOFs was that for R and Y (see pgs 23 and 35), I've moved the boost to reasonably high frequencies, "skipping" the first few modes. They're Qs are reduced enough by the "velocity damping" portion of the controller, and in the case of R, by the T loop as well. Because the boost was so close to the elliptic filter, the phase is evolving a little faster than ideal, but I think I've still managed to squeak out a good looking loop that is fairly insensitive to small changes in gain. 


- Vertical, it turns out was the most difficult to design (see pgs 17-22 of dampingfilters_BSFM_2013-05-15.pdf). The last V mode visible from the top/M1 stage is at 3.8 [Hz], very close to the 10 [Hz] requirements. As such, there's very little phase left for the elliptic filter. 
- On top of this, the last vertical mode at 17.5 [Hz] is invisible at the top stage. This meant that, regardless of whether I could see it in the M1 V2V plant, I needed to get rid of the sensor noise in that region between the two modes, since it shows up in the M1 to M3 V2V transfer function.
- As such, I used a 4th order elliptic instead of the 3rd order I'd used for all of the QUAD DOFs and other BSFM DOFs. In doing so, I tried to get the second notch of the filter as close to 17.5 [Hz] as possible, while still having enough gain to evenly damp the 1st and 2nd V modes, and have enough phase to be stable. 
- In summary, what you see here in this Level 2 V filter is a comprimise between 4 things:
    - The resulting Q of the 1st and 2nd V modes, both in the M1-to-M1 TF (pg 17) and in the GND-to-M3 TF (pg 22)
    - The phase and gain margins (i.e. the stability of the loop)
    - The sensor noise level between 10 Hz and the 3rd V resonance at 17.5 [Hz] as shown on (pg 22) with respect to the specifically-defined, beam splitter vertical requirements (from T010007-v5)
    - The assumed 0.001 V2L cross coupling into DARM as shown on (pg 1) with respect to the BS L requirements (again in T010007) and the current predictions of interferometer sensitivity
- While this compromise does not meet the requirements for the T010007-defined, BSFM vertical, the noise is still a factor of 10-20 away from even the best expected DARM curve, assuming the 
BS2DARM = pi / (sqrt(2) * F)
factor from T080192 is correct (Note, I've used F = 450 for the arm cavity finesse, found in T010075, and T070303).

The configuration:
------
For all degrees of freedom,
FMs 1 ("rolloff_*"),2 ("boost_*"),5 ("norm*"), and 10 (ellip_*)
should be engaged. After discussing it with Arnuad, we've decided to fold the overall gains of the loop into the boost_* filter, so that all the EPICs gains are an easy-to-remember -1. Note that this deviates from traditional SUS gains, but it's time for a new era of not-just-velocity-damping-anymore. <gullable, annoying pre-teen voice> Seismic is doing it </gullable, annoying pre-teen voice>. Hence, the new EPICs gains are:
L = T = V = R = P = Y = -1.
In the fullness of time, we intended to go back to QUAD filters and do the same.

As mentioned above, I've already captured a new safe.snap.

The files:
------
The 2013-05-15 loops were designed using 
${SusSVN}/sus/trunk/BSFM/Common/FilterDesign/design_damping_BSFM_20130515.m
which saves the .mat file of the filters,
${SusSVN}/sus/trunk/BSFM/Common/FilterDesign/dampingfilters_BSFM_2013-05-15.mat
and produces the dampingfilters_BSFM_2013-05-15 set of plots,  as well as saving the model itself in an additional .mat file,
${SusSVN}/sus/trunk/BSFM/Common/FilterDesign/dampingfilters_BSFM_2013-05-15_model.mat

These were compared with the previous filters, (whose figures of merits were plotted with the similar
${SusSVN}/sus/trunk/BSFM/Common/FilterDesign/design_damping_BSFM_20130130.m
and saved to ${SusSVN}/sus/trunk/BSFM/Common/FilterDesign/dampingfilters_BSFM_20130130.mat)
using the script,
${SusSVN}/sus/trunk/BSFM/Common/FilterDesign/compare_bsfm_dampfilter_design.m

The performance measurement was taken using the DTT template
${SusSVN}/sus/trunk/BSFM/H1/BS/SAGM1/Data/2013-05-15_H1SUSBS_M1_DAMPOUT_Spectra.xml

Note, because of the experience taking the open loop gain transfer functions of the QUAD (low SNR, confusing results at low frequency, but otherwise confirming the MIMO nature of the plant, and the ability for my models to predict it), I did *not* take open loop gain transfer functions.

-------
As of this edit, all of the above mentioned files are committed to their respective repository, whether it be the userapps, or SUS repos.


-------
Edit: Replaced the dampingfilters_BSFM_2013*.pdf plot sets because there was a bug in the Title and Legend of the DARM coupling plots -- I'd writting BS2DARM as 2*F instead of sqrt(2)*F. Note, the code that processed the data did/does not have this bug, it was just the plot labels.
Non-image files attached to this report
LHO VE
john.worden@LIGO.ORG - posted 11:33, Thursday 16 May 2013 (6398)
LVEA Pumpdown

Annuli continue to be pumped with a few more transferred to ion pumps this week.

The attached plot shows a step up in pressure and a possible slope reduction. This is currently unexplained but could indicate a leak or a gauge artifact .

We currently have only one operating gauge on the volume so nothing to compare to.

Images attached to this report
H1 SEI
vincent.lhuillier@LIGO.ORG - posted 11:15, Thursday 16 May 2013 (6397)
Coherence Ground STS-2 (installed by BSC4) to BSC1 and BSC2

The STS-2 at the corner station is currently installed by BSC4 (under the stairs). Since the STS-2 is relatively "far appart" from the BSC1 and BSC2 chambers, I checked the coherence from the STS-2 and the T240s installed in stage 1 of the ISIs. Plots of coherence are presented in attachment. Coherence is really good (in the 100mHz to 3Hz frequency band) but not as good as the end station where the STS-2 is closer from the chamber. Coherence between the stage 1 of the 2 ISIs is also presented.

Images attached to this report
H1 SEI
vincent.lhuillier@LIGO.ORG - posted 10:12, Thursday 16 May 2013 (6396)
Tilt T240 - Saturation test - ISI - BSC6

The isolation filters are ramped up with no DC offsets on the super sensor. Once the platform is isolated, it will be translated and rotated as desired. Tests were performed on ISI-BSC6 to evaluate the risk of saturation on the T240s when tilting the platform. Tests were performed with damping loops on every DOFs. Isolation filter (with BOOST to lock the platform to the ground at DC) was engaged in the RX direction with a blend at 750mHz. Then, the platform was tilted by 100nrad in the RX direction. Time series of all T240s signals were recorded during 600s and presented in attachment.
A 100nrad rotation in RX creates a 5000 count peak on the local inputs and a 22000nm/s velocity peak in the Y direction.

Images attached to this report
H1 SEI
hugo.paris@LIGO.ORG - posted 09:36, Thursday 16 May 2013 (6394)
HAM-ISI - Macro Substitution Text Files Moved

The macro substitution text files of the HAM-ISIs were moved from:

/opt/rtcds/userapps/release/isi/common/medm/hamisi/           (now at revision 4499)

into:

/opt/rtcds/userapps/release/isi/h1/medm/hamisi/                      (now at revision 4498)

 

The $(IFO) part of the name of those text files was removed to avoid redundancy: i.e. H1_isiham2_overview_macro.txt became: isiham2_overview_macro.txt 

The sitemap was updated to reflect those changes.                 (now at revision 4500)

H1 ISC
kiwamu.izumi@LIGO.ORG - posted 19:14, Wednesday 15 May 2013 (6382)
h1iscey updated, recomplied and restarted

[Chris W. and Kiwamu]

We have updated, recompiled, reinstalled and restarted the h1iscey model ( per WP#3893). It still runs fine so far.

Main update:

QPDs remain the same

The QPD libraries were upgraded to QPD_WITH_WHITEN_CONTROL, but besides it nothing was changed. Since we haven't edited the rest of the QPD chains, they basically stay the same as before. This is good because we don't have to recover all the servo parameters and so on. I burt-restored the h1iscey and hence the settings came back to what they were in this morning as far as QPDs and their servos are concerned.

DCPDs became different

On the other hand the DCPDs were updated to something almost equivalent to new channels as some of them were renamed and some were deleted and added. Looking at the past DCPD setting Keita and I didn't see any special filters such as anti-whitening. Therefore we decided to abandon whatever the past signal conditioning settings. In case someone wants to remind what they used to be, I took a snapshot of the signal conditioning settings (see the attached). Also I modified the DAQ list so that the output of the DCPD filters are acquired in to DAQ correctly.

Images attached to this report
H1 SEI
vincent.lhuillier@LIGO.ORG - posted 18:14, Wednesday 15 May 2013 (6391)
Sensor Correction – Ground to Stage 1 vs Stage 1 to Stage 2

Following previous aLOGs related to the sensor correction:
-          Coherence ground to ISI https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=6274
-          Master model modifications + Modification routines + Installation filters + Sensor correction from ground (first results) https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=6319
-          Installation of aggressive controllers https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=6351
-          Coherence Stage 1 to stage 2 https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=6360

I tried to evaluate the contribution of each sensor correction on the suppression. For this test, I used the level 3 controllers (the aggressive ones) on both stages, blend at 250mHz in all DOFs. I measured spectra in the following configurations:
-          No sensor corrections
-          Isolation filters only (blend 250mHz – T240s - Level 3 isolation filters)
-          Only the sensor correction from stage 0 to stage 1 using the STS-2
-          Only the sensor correction from stage 1 to stage 2 using the T240s
-          The sensor correction on both stages.

Spectra of translations and rotations of both stages are presented in attachment.

On the translation DOFs:
Isolation provided by the sensor correction from the ground to stage 1 and from stage 1 to stage 2 are quite similar (red vs cyan). In both cases, the sensor correction improves the isolation from 100mHz to 3Hz. The motion around the blend frequency is also reduced (the CPS low pass filters considerably increase the motion below 250mHz – Blue vs green). When the sensor correction is engaged on both stages (red), the individual suppressions are multiplied.
We can notice some amplification between 40mHz and 100mHz due to the aggressive high pass used for the sensor correction.

On the rotation DOFs:
We can notice on stage 1 in the RZ direction:
- around 250mHz, a huge amplification of the inertial motion when engaging the isolation loops (green vs blue).
- between 40mHz and 100mHz, a huge amplification (x100) due to the sensor correction (red, cyan, purple)
The important amplification is particularly visible  in the RZ direction since the sensor correction  is realized in the X and Y directions (only 1 sensor correction with vertical sensor). The low frequency amplifications are less visible on stage 2 since the GS13s are in their noise floor at low frequency.
Isolation performances on stage 2 seem limited by the noise floor of the super sensor.

I have started measurements to look at the cross coupling at low frequency.

Original file (spectra) can be found at:
https://svn.ligo.caltech.edu/svn/seismic/BSC-ISI/H1/ETMY/Data/Spectra/Isolated/
H1_ISI_ETMY_20130514_152000.xml

H1_ISI_ETMY_Spectra_RX_RY_RZ_Comparison_Sensor_Correction_20130514_152000.txt H1_ISI_ETMY_Spectra_XYZ_Comparison_Sensor_Correction_20130514_152000.txt

With :
Ref 0-14: No control
Ref 15-29: Isolation filters only
Ref 30-44: Isolation filters + Sensor correction using STS-2
Ref 45-59: Isolation filters + Sensor correction using T240
Ref 60-74: Isolation filters + Sensor correction using STS-2 and T240s

Images attached to this report
H1 ISC
sheila.dwyer@LIGO.ORG - posted 17:17, Wednesday 15 May 2013 (6389)
end station Phase frequency discriminator
This afternoon I tried to lock the PLL at end Y.  One problem was that the phase frequency discriminator was not working, I watched Imon on a scope while I changed the laser temperature to move the beat note from above to below the locking frequency, and saw no change in Imon.  I swapped all the cables over to the PFD on the right side of the board, as you are looking at it from the front, which responded as I thought it would.  The chassis has serial number S1000761, I got a spare (S1000764) from the midstation and swapped them, I've brought the broken chassis into the EE shop.  

I don't know what might have happened, we saw that the power supplied to the whole rack was not right earlier in the afternoon, the power that should have been +18V was +25V, which Daniel has now fixed.  
LHO General
patrick.thomas@LIGO.ORG - posted 16:29, Wednesday 15 May 2013 (6375)
Ops Summary
The prefilter on one of the fan filter units on the northernmost small clean room between HAM 2 and 3 is not in place. (see attached photo)
Michael R., Pablo D. working on PCAL in the H2 laser room. H2 LEA in laser hazard.
Apollo craned a forklift over the X arm for use with the ISI test stand.
Corey G. installed a light pipe for the MC Trans path between HAM2 and IOT2L.
Arnaud P. took spectrum of the ETMY suspension.
Kiwamu I. rebuilt the h1iscey model.
Dave B. removed the corner station weather station channels from the EDCU and restarted the DAQ for this and Kiwamu's changes to h1iscey.
notification from driver that he would arrive in ~ 15 min for LN2 delivery, later alarms at EX CP8
Thomas V. aligning optical lever on top of HAM 3
Cheryl V. installing video camera on west door of HAM 2
Szymon S. running excitations on top mass of ETMY
Corey G. dropping off equipment in the squeezer bay
Michael R., Pablo D. and Laetitia working in the H2 laser room, H2 LEA NOT in laser hazard
PSL shutter opened ~ 4:22 PM
Images attached to this report
H1 IOO
cheryl.vorvick@LIGO.ORG - posted 15:25, Wednesday 15 May 2013 - last comment - 17:17, Wednesday 15 May 2013(6387)
Camera installed on HAM2 West door to look at REFL as it goes through it's baffle to HAM1:
Looking at the REFL baffle will tell me if our current alignment is sufficient to get the REFL beam from the first surface of PRM into HAM1.  When I looked at the beam before, it was slightly clipped on the East side of the aperture of the baffle, so misaligned in yaw.  I have no knowledge of the alignment state of PRM at the time I saw this clipping.  When I have the beam back and a locked IMC, I'll be able to evaluate the REFL/PRM alignment.

FYI - there is currently a yellow viewport cover without stickers on the East HAM2 door - this is not an invitation to remove the viewport cover without a work permit or contacting the Control Room!  I will either switch the viewport cover to one that has stickers, or get the proper stickers for this cover, before we open the PSL shutter.
Comments related to this report
keita.kawabe@LIGO.ORG - 17:17, Wednesday 15 May 2013 (6390)

I and Cheryl went to the floor, MC was locked, and PRM was aligned so the IFO REFL is centered on the baffle hole before HAM1.

New "aligned" value for PRM alignment slider is [P,Y]=[-730, 0] urad.

This used to be [-830, -50] in air, the change is quite small considering the fact that we're under vacuum now.

With this data even the most serious skeptic should agree that the IO alignment is OK. We should proceed to center IM4 and MC2 trans QPDs because they're quite off-center now.

H1 INS
jodi.fauver@LIGO.ORG - posted 15:09, Wednesday 15 May 2013 - last comment - 15:11, Wednesday 15 May 2013(6385)
HAM4 ISI Install Prep
The area between HAM4 and the high bay/LEA roll-up door was cleared in preparation for the ISI install.  The BSC ISI storage container was flown from that area to the North Bay.  First cleaning was done on HAM4 and its cleanroom (yesterday). The HAM storage container was moved away from HAM4's north side and the bolts were loosened on the south door. Second cleaning will take place ASAP.
Comments related to this report
jodi.fauver@LIGO.ORG - 15:11, Wednesday 15 May 2013 (6386)
Sorry for the double entry. The submit button stuck...
H1 INS
jodi.fauver@LIGO.ORG - posted 15:09, Wednesday 15 May 2013 (6384)
HAM4 ISI Install Prep
The area between HAM4 and the high bay/LEA roll-up door was cleared in preparation for the ISI install.  The BSC ISI storage container was flown from that area to the North Bay.  First cleaning was done on HAM4 and its cleanroom (yesterday). The HAM storage container was moved away from HAM4's north side and the bolts were loosened on the south door. Second cleaning will take place ASAP.
H1 INS
jodi.fauver@LIGO.ORG - posted 15:03, Wednesday 15 May 2013 (6383)
BSC3 ISI Build-up
The forklift was flown into the West Bay so that SEI could use it for adding mass to the ISI.
LHO FMCS
patrick.thomas@LIGO.ORG - posted 12:29, Wednesday 15 May 2013 (6381)
Raised alarm levels for mid station temperatures
Raised HIGH alarms to 85 deg F

ops@operator0:~ 0$ caput H0:FMC-MY_AH_COOLTEMP_2_DEGF.HIGH 85
Old : H0:FMC-MY_AH_COOLTEMP_2_DEGF.HIGH 75
New : H0:FMC-MY_AH_COOLTEMP_2_DEGF.HIGH 85
ops@operator0:~ 0$ caput H0:FMC-MY_AH_COOLTEMP_1_DEGF.HIGH 85
Old : H0:FMC-MY_AH_COOLTEMP_1_DEGF.HIGH 75
New : H0:FMC-MY_AH_COOLTEMP_1_DEGF.HIGH 85

ops@operator0:~ 0$ caput H0:FMC-MX_AH_COOLTEMP_1_DEGF.HIGH 85
Old : H0:FMC-MX_AH_COOLTEMP_1_DEGF.HIGH 80
New : H0:FMC-MX_AH_COOLTEMP_1_DEGF.HIGH 85
ops@operator0:~ 0$ caput H0:FMC-MX_AH_COOLTEMP_2_DEGF.HIGH 85
Old : H0:FMC-MX_AH_COOLTEMP_2_DEGF.HIGH 80
New : H0:FMC-MX_AH_COOLTEMP_2_DEGF.HIGH 85

ops@operator0:~ 0$ caput H0:FMC-MY_VEA_202A_DEGF.HIGH 85
Old : H0:FMC-MY_VEA_202A_DEGF.HIGH   75
New : H0:FMC-MY_VEA_202A_DEGF.HIGH   85
ops@operator0:~ 0$ caput H0:FMC-MY_VEA_202B_DEGF.HIGH 85
Old : H0:FMC-MY_VEA_202B_DEGF.HIGH   75
New : H0:FMC-MY_VEA_202B_DEGF.HIGH   85
ops@operator0:~ 0$ caput H0:FMC-MY_VEA_202C_DEGF.HIGH 85
Old : H0:FMC-MY_VEA_202C_DEGF.HIGH   75
New : H0:FMC-MY_VEA_202C_DEGF.HIGH   85
ops@operator0:~ 0$ caput H0:FMC-MY_VEA_202D_DEGF.HIGH 85
Old : H0:FMC-MY_VEA_202D_DEGF.HIGH   75
New : H0:FMC-MY_VEA_202D_DEGF.HIGH   85

ops@operator0:~ 0$ caput H0:FMC-MX_VEA_202A_DEGF.HIGH 85
Old : H0:FMC-MX_VEA_202A_DEGF.HIGH   75
New : H0:FMC-MX_VEA_202A_DEGF.HIGH   85
ops@operator0:~ 0$ caput H0:FMC-MX_VEA_202B_DEGF.HIGH 85
Old : H0:FMC-MX_VEA_202B_DEGF.HIGH   75
New : H0:FMC-MX_VEA_202B_DEGF.HIGH   85
ops@operator0:~ 0$ caput H0:FMC-MX_VEA_202C_DEGF.HIGH 85
Old : H0:FMC-MX_VEA_202C_DEGF.HIGH   75
New : H0:FMC-MX_VEA_202C_DEGF.HIGH   85
ops@operator0:~ 0$ caput H0:FMC-MX_VEA_202D_DEGF.HIGH 85
Old : H0:FMC-MX_VEA_202D_DEGF.HIGH   75
New : H0:FMC-MX_VEA_202D_DEGF.HIGH   85
LHO General
patrick.thomas@LIGO.ORG - posted 18:54, Tuesday 14 May 2013 - last comment - 15:54, Wednesday 15 May 2013(6358)
weather station code changes
Dave B., Patrick T.

This work falls under permit number 3887.

This morning I installed new EPICS IOC code for the weather stations in /ligo/apps/linux-x86_64/epics-3.14.12.2_long_sc. The module code is davis_weather_monitor_ii-1.0.0 and the IOC code is weather_davis_weather_monitor_ii-1.0.0. The targets are in /ligo/lho/h0/target. The IOCs are running in screen on h0epics2.

This was done primarily to change the channel names to reflect the aLIGO PEM standard in T1200221-v5.
I also hard coded the alarm severities for the wind speeds in the database files. The wind speed alarm levels are set by hand and stored in the autoBurt.req files.
The macro substituted database files are now generated from a template and substitutions files when the IOC is compiled.
An iocBoot directory named ioch0_weather_cs was created and the target named h0weatherms was changed to h0weathercs.

Dave renamed the minute trend files to reflect the channel name changes. his alog entry
New medm screens were linked to in the site map that incorporated the channel name changes.
The autoBurt.req files were updated.
Comments related to this report
patrick.thomas@LIGO.ORG - 15:54, Wednesday 15 May 2013 (6388)
The mapping for the channel name changes is attached.
Non-image files attached to this comment
H1 COC
gerardo.moreno@LIGO.ORG - posted 16:13, Friday 10 May 2013 - last comment - 21:38, Wednesday 15 May 2013(6335)
Ear Bonding Aborted

Ear Bonding of ETM08 was aborted after finding precipitates inside Sodium Silicate Solution bottles, I contacted manufacturer and was told items had expired.  Norna was notified and bonding was suspended, new solution is on its way to LHO, bonding will resume next week.

Images attached to this report
Comments related to this report
dennis.coyne@LIGO.ORG - 21:38, Wednesday 15 May 2013 (6393)
Measurements by Marielle van Veggel indicate that silicate bonds made with "old" sodium silicate solution do not have significantly lower strength or lower quality. For details see T1300482-v1:
https://dcc.ligo.org/LIGO-T1300482-v1
Nonetheless, with an abundance of caution, we should replace the commercial sodium silicate bonding solution every year. The silicate bonding procedure (https://dcc.ligo.org/LIGO-E050228-v3) will be changed to specifically note this shelf life limit.
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