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Reports until 19:15, Friday 08 July 2016
H1 PSL
keita.kawabe@LIGO.ORG - posted 19:15, Friday 08 July 2016 - last comment - 11:29, Monday 11 July 2016(28294)
PSL ISS 2nd loop MEDM madness

Summary:

As reported before (28236), ISS 2nd loop MEDM screen appears as if it sometimes doesn't agree with reality. Turns out that it never truly agreed with reality. For example, in the first attachment, both SERVO ON/OFF indicator and additional 20 dB gain indicator are red while these are ON.

I was bothered enough to investigate and found that the MEDM screen has numerous nonsense logic and that the guardians are not written MEDM-friendly. I made a quick dirty fix for MEDM as well as guardians.

What was wrong:

Before going into details, you need to know that ALL of PSL 2nd loop I/O that are binary in nature is done via 16 bit DAC (don't ask me why). The output of DAC is sent to optical coupler via a resistor (see e.g. D1300439). To make anything ON, you want some large positive voltage to drive the LED in the coupler. To make anything OFF, you want to send sufficiently small (e.g. zero-ish) voltage or negative voltage.

As you can easily guess, one of the problems is the lack of convention. People sometimes send +32000 and other times +32700 to make the same thing ON. Sometimes -32000 and other times 0 to turn it OFF.

On top of that, there are many bugs in MEDM screen such that color indicators check some nonsense bits that never change, value set on pressing button but changed to a different number on releasing the button, that kind of things.

What was done:

I changed most everything in MEDM as well as IMC_LOCK and lsclibrary such that:

  1. OFF is 0 so MEDM switch graphics using "if zero" and "if not zero" works correctly,
  2. ON is 32000 for the sake of consistency but the color indicators check if the value is positive (instead of looking at some specific bit).

It seems as if it's working for now.

Madness example:

Just as an example. Manually pressing CHANGE PDs button could have made you believe that you selected PD1-4 when PD5-8 (3rd loop) was selected in reality.

In the second attachment, you can see that the CHANGE PDs "1-4" button sent 32000 (40V-ish differential) when pressed, but then 1 (less than 1 mV) when released.

PD1-4 is selected with large positive voltage (or ON or HIGH or whatever), otherwise PD5-8 is selected.

When you manually pressed and released "1-4",  the DAC output momentarilly went +40V differential, but immediately went down to some tiny voltage, so PD5-8 was selected in the end.

But the switch graphics was implemented assuming that non-zero output means PD1-4. Since the DAC output was 1 after pressing the "1-4" button, the graphics showed that PD1-4 was connected instead of 5-8. The PD indicator color box didn't help either as it checked the bit 2 of the DAC output, and it only turned to orange (CH5-8) only when DAC output was 32700.

The story was different for guardian as it used +32000 and -32000 for PD1-4 and PD5-8, respectively. When guardian did something, it looked as if PD1-4 was selected no matter what.

Images attached to this report
Comments related to this report
keita.kawabe@LIGO.ORG - 11:29, Monday 11 July 2016 (28321)

Addendum:

"The story was different for guardian as it used +32000 and -32000 for PD1-4 and PD5-8, respectively. When guardian did something, it looked as if PD1-4 was selected no matter what."

The above was incorrect, it turns out that the MEDM screen PD14/PD58 graphics happened to agree with reality when the guardian was doing it.

ISC_LOCK lets IMC_LOCK handle most of the 2nd loop board switching except for closing the third loop (i.e. selecting PD5-8) when ISC_LOCK bypasses IMC_LOCK and uses lockISS in ISC_library to send 0 to DAC. MEDM looked correct.

When selecting PD1-4, ISC_LOCK uses IMC_LOCK which sends +32000 to the DAC and again the graphics looked correct.

H1 AOS (SEI)
conor.mow-lowry@LIGO.ORG - posted 18:23, Friday 08 July 2016 (28291)
Stage 1 Sensor correction with BRS
Conor, Jeff, Jim

Short summary:
- BRS results in a factor of three reduction in arm-length RMS velocity with moderate wind.
- BRS does no measurable harm at low frequencies.
- In moderate wind, all test-mass sensor corrections show the same RMS in the beam axis.
- Identical broadband sensor correction results in rejection of the primary microseism in arm-length


Moving one step further down the ISI chain, I looked at the sensor correction of the Stage 1 CPSs from the ground STS2s.

To do this, I fetched Ground and BRS data along the beamlines (ITMY_X, ITMY_Y, ETMX_X, ETMY_Y, ETMX_RY, and ETMY_RX) and
filtered the BRS using fetched zpk from Foton to tilt-correct the End-station STS2s (one could also grab the corrected channel now).

The STS2 outputs were then filtered for broadband sensor correction (using a filter very similar to the installed version). This is 
now the signal sent directly to the CPSs and at low frequency (f<0.1 Hz) is a good estimate of the relative motion of the optics.

Attachment 1 shows the CPS sensor correction inputs (in m/s/rtHz) for each test mass in the beam axis. End test masses are shown with and without 
BRS tilt correction. The RMS for each curve from 0.2Hz down is dashed. The RMS velocity is the thing I think we want to minimise at low-f.

What can be seen is that after correction and with moderate wind (~17mph), all channels except ETMX_X have identical RMS. With lower tilt and BRS correction, EX performs better.
Also note that even though there is a spectral 'bump' of BRS noise around and below 10mHz, it makes no difference at all to the RMS. BRS does no 
measurable harm after the Ground-to-CPS sensor correction filters.

Attachments 2 and 3 show the ARM DoF sensor correction, by taking the subtractions: ITMX_X - ETMX_X, and ITMY_Y - ETMY_Y. What this shows is that 
by using identical sensor correction filters, we get some (not insignificant) common-mode rejection of the primary microseism, which is *amplified*
by the sensor correction filter. This rejection will improve as the microseism increases. Additionally, in the important degree of freedom for the
interferometer, there is a factor of 3 improvement in RMS using the BRS.

Attachment 4 is the script used to produce these plots, it should be self-contained apart from an NDS fetch, Foton fetching, and these path entries:
addpath /ligo/svncommon/NbSVN/aligonoisebudget/trunk/Externals/SimulinkNb/Utils/
addpath /ligo/svncommon/SeiSVN/seismic/Common/MatlabTools/
Images attached to this report
Non-image files attached to this report
H1 ISC (Lockloss, OpsInfo)
sheila.dwyer@LIGO.ORG - posted 17:42, Friday 08 July 2016 - last comment - 19:13, Friday 08 July 2016(28292)
please watch ITMX bounce

Our first lockloss from 40 Watts today (2016-07-08 19:36:59  ISC_LOCK  NOMINAL_LOW_NOISE -> LOCKLOSS)  was caused by bounce modes.  ITMX bounce mode rang up ( I don't know why).  After this rang up I turned off all the bounce mode damping (because of confusion about which mode it was) which caused all the modes to grow and break the lock. 

This lock I have been watching and the settings we used damped the ITMX mode well when we first locked, and it has not rung up at all.  My advice to operators would be to keep open the StripTool (/ligo/home/ops/BOUNCE_DAMPING.stp).  If ITMX starts ringing up open up the damping filters (sitemap> sus> BOUCNE_ROLL>DAMPING filters)  and try a different phase for ITMX by turning on or off some of the filters like +60, -60 ect.  If it starts damping that's good, if it starts ringing up faster because of your change you can use a negative gain with that phase. 

Comments related to this report
patrick.thomas@LIGO.ORG - 19:13, Friday 08 July 2016 (28295)
There does not appear to be a file named BOUNCE_DAMPING.stp at /ligo/home/ops/. I found /ligo/home/ops/Templates/StripTool/BOUNCE_DAMPING.stp.
H1 PSL (PSL)
cheryl.vorvick@LIGO.ORG - posted 16:08, Friday 08 July 2016 (28289)
"Weekly PSL Chiller Reservoir Top-Off

FAMIS task 6478: PSL DIode and Crystal chilller top-off:  assigned 11PM 7/6, read by me in the morning on 7/7, on 7/8 JeffB noticed the Crystal chiller was in alarm, I trended and it went into alarm on 7/7, was previously filled on 6/30, so only lasted 8 days

H1 INJ (CAL, CDS, DetChar)
jeffrey.kissel@LIGO.ORG - posted 16:06, Friday 08 July 2016 (28284)
ODC EPICs Records Set to Match New PINJX Inverse Actuation Filter Scheme
J. Kissel, D. Macleod

Via the ODC Team's "internal status checking webpage," Duncan found that several ODC EPICs records that define good settings for the PCALX's hardware injection path were errantly all zeros. In short: I've fixed the problem and the ODC summary bit for PINJX is happy and green.

-------------
Details of how I made the summary bit green:
The subpage for PINJX shows three columns: "ini" "safe" and "current", and I *think* that the "ini" coulmn is what they want the value to be (reported in decimal), the "safe" is what the SDF system's safe.snap has stored, and "current" is the current EPICs value. 

These channels were "not monitored" in the SDF system, and the safe.snap file that the front end loads upon restart had them set to zero, so it's not surprising that no one noticed these had gone bad. 

However, given the recent rearrangement of the hardware injection path (see LHO aLOG 27383) the values listed in the "ini" column are also incorrect. 

The channels in question are
    H1:CAL-PINJX_ODC_HARDWARE_CTRL_EQ
    H1:CAL-PINJX_ODC_HARDWARE_GAIN_EQ
    H1:CAL-PINJX_ODC_CW_CTRL_EQ
    H1:CAL-PINJX_ODC_CW_GAIN_EQ
    H1:CAL-PINJX_ODC_TRANSIENT_CTRL_EQ
    H1:CAL-PINJX_ODC_TRANSIENT_GAIN_EQ
    H1:CAL-PINJX_ODC_CHANNEL_BITMASK
After digging through the h1calex front-end model to figure out what these ODC channels listed on the web actually *are*, I found the following (see first two attachments for visual aide):
- the three _GAIN_EQ records are compared against the *actual* gain of each of the three hardware injection filter banks (H1:CAL-PINJX_CW_GAIN, H1:CAL-PINJX_TRANSIENT_GAIN, H1:CAL-PINJX_HARDWARE_GAIN). These records are just standard decimal values, and since the filter bank gains are currently all +1.0, all of these records should be +1.0.

- the H1:CAL-PINJX_ODC_CHANNEL_BITMASK is a binary bit-word that masks which of the ODC bits are used to determine the summary status bit. Of course you know, in EPICs, binary bitwords must be entered in as hexidecimal. Also you know that, in ODC Bit 0 is reserved for the summary, so the mask starts functioning at bit 1. Since there are 6 comparison channels that we want to inform the summary bit, we need six bits, so the value should be
                                           Bit# 6 5 4 3 2 1 0   Decimal   Hex   What Goes In EPICs
     H1:CAL-PINJX_ODC_CHANNEL_BITMASK           1 1 1 1 1 1 0 = 126     = 7e    = 0x7e

- the three _CTRL_EQ records are compared against the output of "CtrlOut" spigot of each of the three hardware injection filter banks, respectively, which cdsCtrlFilt2 filter modules. According to the doc text inside the CDS_PARTS.mdl library, this cdsCtrlFilt2 output is a 13-bit bitword indicative of the state of all switches in the filter module: FM1's status is the least significant bit (Bit 0), FM2 through FM10's status are Bits 1 through 9, and Bits 10, 11, and 12 are the input, offset, and output switch status respectively. Because the _CTRL_EQ records are bit-wise compared to the front end's bitword, the record's value must also be a binary bit word. 

So, here's the table to translates this mess for each of the three filter banks, given the current, correct status of these filter banks (see third attached screen shot).
                                         Bit# 13 12 11 10 09 08 07 06 05 04 03 02 01     Decimal    Hex       What Goes In EPICs 
     H1:CAL-PINJX_ODC_HARDWARE_CTRL_EQ         1  0  1  0  0  0  0  0  0  0  0  0  0   = 5120     = 1400    = 0x1400
     H1:CAL-PINJX_ODC_CW_CTRL_EQ               1  0  1  1  1  1  1  1  1  1  1  1  1   = 6143     = 17FF    = 0x17ff
     H1:CAL-PINJX_ODC_TRANSIENT_CTRL_EQ        1  0  1  0  0  0  0  0  0  0  0  0  0   = 5120     = 1400    = 0x1400
                                 Switch Name  OT OF IN F1 F2 F3 F4 F5 F6 F7 F8 F9 F10
 

All of the bits are now green, and the mask is lights are on as expected, and the summary bit is green. I've switched ON the monitoring of these channels in the SDF system, and accepted these new values. I trust that Duncan will update the ODC team's page such that the "ini" column is correct.

I've also re-installed (and SDF monitored) all of the appropriate strings in each H1:CAL-PINJX_ODC_BITn channel (where n is the bit number from 0 to 13), as defined again by this ODC Team webpage.

-------------
Critiques of this instantiation of ODC:
- This ODC system is essential identically recreating the SDF system. There's really no need for this. The SDF system is required to be reconciled before going into any observational stretch, so if the hardware injection path's filter banks are monitored by the SDF system (and they are), then they by default confirmed to be correct every observation stretch.
- If someone decides that this is worth keeping, 
    - these EPICS records should be much more clearly labeled and explained on the ODC MEDM screen.
    - The actual output of the CtrlOut from each of the cdsFiltCtrl2 banks should be fed into an EPICs record as well. This way one can easily take the current value and copy it into the comparator, such that the novice doesn't have to go through the binary to EPICs hex translation game that I had to above.
Images attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 15:53, Friday 08 July 2016 (28288)
Ops Day Summary: H1 locked at 40W and in Observe

State of H1: Locked at 40W and in Observe

Today's H1 Commissioners: Keita, Sheila, Kiwamu

Locking:

Site Activities:

Current Plans for continuing ER9 (may change): continue the run the rest of today, and continue the run 8AM-midnight tomorrow

H1 ISC (SUS)
christopher.wipf@LIGO.ORG - posted 15:49, Friday 08 July 2016 (28264)
PUM noise vs dewhitening

Coil drivers for the quad L2 (penultimate) stage have four dewhitening filter states, of which state 2 has the largest range and state 3 the lowest noise.

State 2 is meant for lock acquisition, and is not compatible with low noise data taking (unless some form of subtraction is used). As shown in the plot below, the DAC noise in state 2 would be expected to limit the historic DARM sensitivity in the 10-50 Hz band. (For ER9 sensitivity the state 2 noise is apparently low enough to be out of the way, as noted in alog 28107.)

Images attached to this report
Non-image files attached to this report
H1 General
cheryl.vorvick@LIGO.ORG - posted 15:05, Friday 08 July 2016 (28286)
H1 in Observe at 22:04UTC at 40W
H1 ISC
edward.daw@LIGO.ORG - posted 14:38, Friday 08 July 2016 (28272)
Parametric Instability Doublet Control with IWAVE - cross-subtraction technique - Ed Daw, Tega Edo
Here are results on a study of using iwave to control closely spaced doublets of sinusoids. This study was conducted on test data at 16384Hz sampling rate, of 100 second duration. The dataset consisted of two sine waves at 27.8 and 27.9Hz, each of amplitude 1, on a background of Gaussian white noise of RMS 0.1. Two iwave configurations were used to try and subtract the two components. In both schemes, iwave was running with a tau parameter of 5 seconds and initial guess frequencies at exactly the line frequencies. Iwave was running in phaselocked mode. The loops on the lower and upper frequency lines were set to close 5 and 6 seconds into the dataset, respectively, although these time delays are unimportant; they could both have been set to zero just as well and I mention them for completeness.

CONFIGURATION 1: the raw data is injected into iwave1 set to track the lower frequency (27.8Hz). The D phase output of iwave1 is subtracted from the raw data, and the result is injected into iwave2, set to track the upper frequency (27.9Hz).  The D phase output of iwave2 is subtracted from the input to iwave2, and the difference is the final output. In other words, the two iwave filters are cascaded.

CONFIGURATION 2: the raw data minus the D phase output of iwave2, set to track the upper frequency line (27.9Hz) is used as the input for iwave1, set to track the lower frequency line (27.8Hz). The raw data minus the D phase output of iwave1 is used as the input for iwave2. In other words, for each iwave, the input is the result of the raw data with the D phase output of the other iwave subtracted. 

The first attached pdf shows the results of studies of the the two configurations; the first two pages are for configuration 1 and the pages 3 and 4 are for configuration 2. In each case, there are three plots - the extracted line amplitudes and frequencies (together on the same page), and amplitude spectral densities of the raw data, the data after the subtraction of the first line, and the the output data after both lines are subtracted. 

The 'cross-subtraction' technique is superior, having much better line attenuation and markedly less sidebands introduced. This is because iwave uses the product of the input data and the Q phase output to sense phase shifts, but when the input data is polluted by a close by line, this causes residual beats between this line and the q phase output in the phase measurement. You can see this on page 1, where both the inferred frequency of the line and its amplitude oscillate at the difference frequency between the two lines, which is 0.1Hz, or a 10 second beat. When each iwave input has the inferred line from iwave outputs on other loud lines removed before input, this distortion goes away. 

I have attached a schematic of the cross subtraction configuration, 2, as a second attached figure, in case the written description above is not clear enough. One detail is, the output of iwave2 which is then subtracted from the input data before injection into iwave1 must be derived from the previous sample of iwave2 output, and hence has to be phase shifted forward by one sample period to accurately subtract the line. This is easy to do using both the Q and the D phase outputs of iwave2, and the cos and sin of the phase shift per sample for the frequency of the line tracked by iwave2.
Non-image files attached to this report
LHO VE
kyle.ryan@LIGO.ORG - posted 14:30, Friday 08 July 2016 (28281)
Manually over-filled CP3
1315 -1400 hrs. local -> To and from Y-mid (then X-mid, unrelated)

Opened exhaust check-valve bypass-valve.  Opened LLCV bypass-valve 1/2 turn -> LN2 @ exhaust in 55 seconds -> Restored valves to as found configuration.  

Next CP3 overfill to be Monday, July 11th.  
H1 GRD
jameson.rollins@LIGO.ORG - posted 12:15, Friday 08 July 2016 - last comment - 16:30, Friday 08 July 2016(28275)
IFO top node not monitoring some nodes

The IFO top node appears to be not monitoring some SEI BS and ALS nodes.  The IFO top node is reporting OK, even though multiple nodes are not reporting OK:

This is an indication of two issue:

The USERAPPS/h1/guardian/IFO_NODE_LIST.py that is in the SVN shows that those nodes should be managed, so my guess is that what's currently running has not been committed to the SVN.

Images attached to this report
Comments related to this report
jameson.rollins@LIGO.ORG - 14:52, Friday 08 July 2016 (28283)

My advice would be to not focus too much on a potential O2 configuration, but focus instead right now on the ER9 configuration.  There's no problem in updating the NOMINAL states as needed.  They should be set to whatever is appropriate for ER9, and make sure they're all monitored by the top node.  We can then adjust things as needed for O2.

In other words, IFO should always be monitoring all nodes, and we should just adjust the NOMINAL state for each node to reflect whatever is the ideal IFO configuration at the moment.

jameson.rollins@LIGO.ORG - 12:23, Friday 08 July 2016 (28277)

I confirmed that the USERAPPS/sys/h1/guardian/IFO_NODE_LIST.py file has indeed been modified locally to remove monitoring of the SEI BS and ALS nodes, and that those changes have not been committed to the SVN.

jameson.rollins@LIGO.ORG - 12:31, Friday 08 July 2016 (28278)

Many guardian files have local modifications that have not been committed to the SVN:

jameson.rollins@operator1:~ 0$ guardlog list | xargs -l guardutil files 2>/dev/null | sort | uniq | xargs -l svn status
M       /opt/rtcds/userapps/release/als/common/guardian/ALS_COMM.py
M       /opt/rtcds/userapps/release/als/common/guardian/ALS_DIFF.py
M       /opt/rtcds/userapps/release/als/common/guardian/ALS_YARM.py
M       /opt/rtcds/userapps/release/ioo/common/guardian/IMC_LOCK.py
M       /opt/rtcds/userapps/release/isc/common/guardian/VIOLIN_DAMPER.py
M       /opt/rtcds/userapps/release/isc/h1/guardian/BOUNCE_ROLL.py
M       /opt/rtcds/userapps/release/isc/h1/guardian/ISC_DRMI.py
M       /opt/rtcds/userapps/release/isc/h1/guardian/ISC_library.py
M       /opt/rtcds/userapps/release/isc/h1/guardian/ISC_LOCK.py
M       /opt/rtcds/userapps/release/isc/h1/guardian/lscparams.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_BS_ST1_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_BS_ST1.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_BS_ST2.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ETMX_ST1_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ETMX_ST1.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ETMX_ST2.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ETMY_ST1_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ETMY_ST1.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ETMY_ST2.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_HAM2_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_HAM3_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_HAM4_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_HAM5_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_HAM6_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ITMX_ST1_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ITMX_ST1.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ITMX_ST2.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ITMY_ST1_CONF.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ITMY_ST1.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/ISI_ITMY_ST2.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/SEI_CONFIG/const.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/SEI_CONFIG/CS_states.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/SEI_CONFIG/HAM_states.py
M       /opt/rtcds/userapps/release/isi/h1/guardian/SEI_CONFIG/manager.py
M       /opt/rtcds/userapps/release/omc/common/guardian/OMC_LOCK.py
M       /opt/rtcds/userapps/release/sus/common/guardian/SUS_PI.py
M       /opt/rtcds/userapps/release/sys/common/guardian/IFO.py
M       /opt/rtcds/userapps/release/sys/h1/guardian/DIAG_MAIN.py
M       /opt/rtcds/userapps/release/sys/h1/guardian/IFO_NODE_LIST.py
jameson.rollins@operator1:~ 0$ 

jenne.driggers@LIGO.ORG - 14:15, Friday 08 July 2016 (28280)

The lack of monitoring some nodes was at my request.  These are nodes that currently are requested to be different from their true nominal state so that we can get diagnostic information (ALS nodes), or to avoid unneccessary potential locklosses (BS ISI node).  For O2, these will be placed back in their low noise nominal modes.  We removed them from the monitoring so that we would be able to set the Intent bit to Observe for the ER run.  Once ER9 is complete, we will uncomment the nodes so that they are back to being monitored.

We should indeed be better about checking things into the svn.

sheila.dwyer@LIGO.ORG - 16:30, Friday 08 July 2016 (28290)

I comitted these except for the isi ones

H1 General
vernon.sandberg@LIGO.ORG - posted 11:01, Friday 08 July 2016 - last comment - 15:07, Friday 08 July 2016(28273)
Return to 40 W Commissioning

We have operated for over 10 hours in "nominal low noise, observation, intent bit set" condition.  This was a temporary configuration to allow locking, after the laser diode box failure, for the purposes of testing ER9 pipelines. We are returning to 40W operation.  

Comments related to this report
keita.kawabe@LIGO.ORG - 15:07, Friday 08 July 2016 (28287)

(Cheryl, Sheila, Kiwamu, Haocun, Ross, Keita)

ISC_LOCK.py and lscparams.py were reverted so the target power is 40W and SOFT offsets are set correctly.

ISS offset was remeasured at 40W and set to -0.932693 (instead of the original -0.9826934814453125).

IMC_LOCK.py was changed to set this offset, and  also the final ISS 2nd loop gain was set back to 20dB for 40W  (instead of 24dB for 25W).

No change was made to TCS as nobody touched the TCS CO2 guardian yesterday.

IFO got back to the correct 40W nominal low noise state after the above change.

After this, SUS_PI was also changed (yesterday it was accidentally changed such that QPD and OMC-based damping were enabled for the same mode at the same time).

H1 General
sheila.dwyer@LIGO.ORG - posted 01:07, Friday 08 July 2016 - last comment - 14:12, Friday 08 July 2016(28261)
Joint summary

Patrick, Sheila, Carl and Ross damping PIs

After Keita's ISS fixes we had a few hours of bad weather and earthquakes that contributed to dificulty locking.  Once things calmed down we locked and sat at several stages to see if the lock was stable, DC readout, 25 Watts, ISS 2nd loop engaged, and now we have made it to some kind of "nominal low noise" state.  Patrick hit the intent bit.  

There are several things wrong with this spectrum, some of which could be solved by going back to 40 Watts in the morning:

The last attached screenshot is just to show how many locking attempts everyone made in the last 14 hours. The range displayed by the DMT viewer in the control room seems to have a problem, it should be stable at some low range but on the DMT viewer it looks like we lost lock in the last half hour.  

Images attached to this report
Comments related to this report
sheila.dwyer@LIGO.ORG - 01:38, Friday 08 July 2016 (28262)

Sheila's comment

There were several things which had to be done today because of the change to run ER9 at 25 Watts.  

  • Getting rid of soft loop offsets that were tuned to improve recycling gain at 40 Watts
  • setting ISS 2nd loop offsets
  • commenting out low noise ASC states
  • changing TCS CO2 guardians by hand

We should remember to undo these things as soon as we go back to 40 Watts.  According to Ross and Carl, there isn't a reason to think our PI situation has gotten worse than it was for the last 2 weeks where we had stable locks more than 4 hours long, but the PI damping would need to be babysat at 40 Watts.  Maybe an engineering run is a good time for detector engineers and operators to learn how to do this.  

There are several things that should be done if we want to continue the ER at 25 Watts with a reasonable sensitivity:

  • run A2L
  • make 25 Watt low noise hard loops
  • get CO2 powers set to something OK in the guardian

none of these are all that hard to do, but to me it seems like it would be more productive to try continuing the ER at 40 Watts, to see what we can learn about the IFO in a state that is more similar to the configuration we would like to run at for O2.  

keita.kawabe@LIGO.ORG - 10:20, Friday 08 July 2016 (28271)

DARM-ISS 2nd loop coherence doesn't change by increasing the ISS 2nd loop gain by 6dB. Jitter or whatever, ISS is imprinting noise onto intensity.

Images attached to this comment
gabriele.vajente@LIGO.ORG - 12:18, Friday 08 July 2016 (28276)

Keita, this is something I think we saw in the past too:

https://alog.ligo-wa.caltech.edu/aLOG/index.php?callRep=20394

nutsinee.kijbunchoo@LIGO.ORG - 14:12, Friday 08 July 2016 (28279)

CO2 related comment:

  • CO2 Nominal state of the guardian gets turned on during Coil Driver state. If you have skipped Coil Driver (which you did according to the alog) then CO2 power guardian stays at pre-heating. This can be changed easily.
  • CO2 power at its Nominal state is calculated based in PSL input. There might be a message complaining that the CO2 setting is not nominal (since we used to operate at 20W) but the output CO2 power should be correct at 40W.
H1 ISC (ISC, SUS)
carl.blair@LIGO.ORG - posted 00:08, Friday 08 July 2016 - last comment - 14:59, Friday 08 July 2016(28259)
Summary 47.5kHz Instabilities
[Ross, Carl]
This is a summary of what we know about the 47.5kHz instabilities at present.
 
There are two modes whose aplitudes rise significantly during most locks, they appear in the 65536kSa/sec HF OMC transmission signals at approximately 18038Hz and 18056Hz.  
 
As reported in alog28088 they appear to be super-nyquist ETMY modes that are aliased from 47497Hz and  47480Hz.  
 
They caused lockloss several times when we had increased the ETMY ring heater in an attempt to split the15042Hz ETMX and ETMY modes that are problematic to damp.  They have also caused several lock losses over the last day.  However there has been a large transient in amplitude for several weeks.  Currently when we survive these modes it is by fast thermal transient through a large parametric gain regime.  If the transient is fast enough we do not spend enough time in the transient for the mode amplitude to grow to a level to unlock the interferometer.  Example amplitude transients can be found here.
 
The phase of the arm transmission QPDs quadrants relative to the OMC transmission signal was measured for the 18038 Hz mode to be ETMX_A UL 21.7 deg, LL -171deg, UR -129deg and LR 83deg and ETMY_A UL 67 deg, LL -141deg, UR -129deg and LR 66 deg indicating a 'pringle' type optical mode.  For reference the 15542Hz vertical mode phase is ETMY UL -178 deg, LL 33deg, UR -163deg and LR 6.5 deg.  The pringle shape is the expected shape of a HG11 which has a resonance at approximately 47500Hz in a single arm cavity. 
 
The Q has been estimated as 5.7 million from a ring down time constant of 38.3 sec.  This was done at 40W and the parametric gain was not estimated so this number is an upper limit.
 
My simulations of the test mass do not show me any very likely culprit resonant modes in a 1kHz band around the observed resonance frequency, many would interact with significant beam decentering but Marie's measurements do not indicate any particular ETMY decentering (to explain only seeing ETMY instabilities).  It appears the ears interact significantly at these frequencies. See the mode shape animations with and without ears.  The most likely in the group of modes in these animations appears to be the 47942Hz without ears.  With ears all modes look like they need some decentering to get significant overlap.  However there is a suspicious mode at 43kHz (separate image).  I am not confident in the simulation at these frequencies, we need more high frequency mode identification to increase confidence in the model.
 
The mode has now been excited and damped and the damping setting have been put into the SUS_PI guardian.  The current damping settings use the OMC HF signal down-converted on 17300Hz transmitted to the end station then up-converted.  The signal then passes through a 10Hz wide band-pass filter -30deg phase and -3000 control gain driving the LL quadrant.  The phase response of the 10Hz wide bandpass may not be adequate as this mode is likely to shift more than 1 Hz in the thermal transient, while the filters response is approximately 60 degrees per Hz.  The filter used is a normalised combination of cheby2, butter and a notch to reduce the phase gradient.
A narrow filter was compared to a wide filter when doing the phase optimisation.  There are 2 lines within +/-5Hz.  These lines beat and the result is a reduction the 'effective damping strength'.  The two plots show the phase optimisation with the narrow filter and the broad filter.  The optimums were found to be 150 deg (broad) and +90deg (narrow).  In this case the cost of the beat signal is a factor of ## reduction in the effective drive strength.
 
A narrow filter (2Hz) was compared to a wide (10Hz) filter when doing the phase optimisation.  There are 2 lines within +/-5Hz.  These lines are removed by the narrow filter but not by the wide filter, resulting in a reduction of the 'effective damping strength'.  The two last plots show the phase optimisation with the narrow filter and the broad filter.  The optimums were found to be 150 deg (wide) and +90deg (narrow).  In this case the cost of the beat signal is a factor of 2 reduction in the effective drive strength going from a damping time constant of 4.4 seconds (narrow) to 9 seconds (wide) at the optimum damping phase (with the same control gain and filter normalisation on resonance).
 
A narrow filter was compared to a wide filter when doing the phase optimisation.  There are 2 lines within +/-5Hz.  These lines beat and the result is a reduction the 'effective damping strength'.  The two plots show the phase optimisation with the narrow filter and the broad filter. [Ross, Carl]
This is a summary of what we know about the 47kHz instabilities at present.
 
There are two modes whose alpitudes rise significantly during most locks, they appear in the 65536kSa/sec HF OMC transmission signals at approximately 18038Hz and 18056Hz.  
 
As reported in alog @@@ they appear to be super-nyquist modes that are aliased from 47333 47333.  
 
They caused the interferometer to unlock several times when we had increased the ETMY ring heater in an attempt to split the 15042Hz ETMX and ETMY modes that are problematic to damp.  They have also caused several lock losses over the last day where the interferometer was being locked from a cold state.  Currently when we survive these modes it is by fast thermal tranisent through a large parametric gain regime.  If the transient is fast enough we do not spend enough time in the transient for the mode amplitude to grow to a level to unlock the interferometer.
 
The phase of the arm transmission QPDs relative to the OMC transmission signal was measured for the 18039 Hz mode to be ETMX UL 21.7 deg, LL -171deg, UR -129deg and LR 83deg and ETMY UL 67 deg, LL -141deg, UR -129deg and LR 66 deg indicating a 'pringle' type optical mode.  For reference the 15542Hz vertical mode phase is ETMY UL -178 deg, LL 33deg, UR -163deg and LR 6.5 deg.  The pringle shapes is the expected shape of a HG11, which has a resonance at approximately 47500Hz in a single arm cavity. 
 
The Q has been estimated as 5.7 million from a ring down time constant of 38.3 sec.  This was done at 40W and the parametric gain was not estimated.
 
My simulations of the test mass do not show me any very likely culprit resonant modes in a 1kHz band around the observed resonance frequency.  It appears the ears interact significantly at these frequencies. See the mode shape animations with and without ears.  The most likely in the group of modes in tha animation appears to be the 47942Hz.  However there is a suspicious mode at 43kHz.  I am not confident in the COMSOL simulation at these frequencies, we need more high frequency mode identification to increase confidence in the model.
 
The mode has now been excited and damped and the damping setting have been put into the SUS_PI guardian.  The current damping settings use the OMC HF signal downconverted on 17300 transmitted to the end station then upconverted.  The signal then passes through a 10Hz wide bandpass filter -30deg phase and -3000 control gain driving the LL quadrant.  The phase response of the 10Hz wide bandpass may not be adequate as this mode is likely to shift more than 1 Hz in the thermal transient, while the filters response is approximately 60 degrees per Hz.  The filter used is a normalised combination of cheby2, butter and a notch to reduce the phase gradient.
 
A narrow filter was compared to a wide filter when doing the phase optimisation.  There are 2 lines within +/-5Hz.  These lines beat and the result is a reduction the 'effective damping strength'.  The two plots show the phase optimisation with the narrow filter and the broad filter. 
Images attached to this report
Comments related to this report
carl.blair@LIGO.ORG - 03:32, Friday 08 July 2016 (28263)

The phase of the 18040Hz mode flipped during this lock stretch.  The damping has been switched to the arm transmission QPDs gain 10,000 phase + 60 deg.
The 18056Hz mode also became unstable and was succesffully damped with settings in SUS_PI guardian.

The ETMX 15541.8Hz mode and ETMY 15542.6Hz modes that have been difficult to damp were damped well tonight with the arm tranmssion QPD signals.  The rational was that the arm transmission QPD's differentiate the arm the mode is in to some extent reducing the beat effect.  These settings are in the SUS_PI guardian.  The revert comment out the ETM QPD gain settings and uncomment the OMC gain settings for these modes.

edward.daw@LIGO.ORG - 14:59, Friday 08 July 2016 (28285)
Carl - I'm wondering if the width and apparent double nature of each mode could be due to the same mode being excited in 
the coating-bearing mass and in the reaction mass - could the reaction mass body modes be getting rung up as well? Just a thought.
Might be nonsense.
LHO VE
kyle.ryan@LIGO.ORG - posted 15:25, Thursday 07 July 2016 - last comment - 14:32, Friday 08 July 2016(28248)
Ran rotating vacuum pumps at X-mid
Started and ran the purge-air skid, Turbo, QDP80 and newly added scroll pump.  Tested the functionality of the Turbo's Safety Valve with the control cable connected to the scroll pump's relay box - demonstrating that the Safety Valve closes upon the loss of scroll pump motor AC and thus mimicking the "QDP80 Running" 
signal.

Note: The purge-air skid has developed some problems from lack of use over these past few years, namely the radiator fan never came on while running the compressors, the drying tower never cycled and the low pressure alarm never sounded.  These features worked fine when last this unit was run.  Now they don't.  Also, the Turbo spun-up normally even with the locally mounted scroll pump running (new vibration source) but tripped into EMERGENCY OPERATION upon BRAKING and when at ~1/3 NORMAL rpm.  This behavior is seen on other Turbos (XBM for example) and might be an age related issue?  

I am leaving the Turbo energized overnight to ensure that the rotor is completely stopped.  I will de-energize it tomorrow.  
Comments related to this report
kyle.ryan@LIGO.ORG - 14:32, Friday 08 July 2016 (28282)
Friday, July 8th ~1345 hrs. local -> De-energized MTP controller
H1 CAL
kiwamu.izumi@LIGO.ORG - posted 11:36, Tuesday 05 July 2016 - last comment - 14:16, Friday 08 July 2016(28150)
Fit of sensing function completed

With the measured sensing function (28123) in hand, we did an MCMC-based numerical fitting for the sensing function (see E. Hall, T1500553).

The fitting results are


[New sensing function form]

As reported by Evan (27675), it seems that the extra roll off in the DARM response at low frequencies are due to an SRC detuning (or something equivalent). While such detuning should be suppressed by some control loop ideally, we decided to include the detuning-induced functional form in addition to the ordinary single-pole response. We use the following approximated form for the DARM response

S(f) = H / (1 + i f / fc ) * exp( -2 * pi * f * tau) * f^2/(f^2 + fs^2)

where H, fc, tau and fs are the optical gain, DARM cavity pole, time delay and spring frequency. Some details of the derivation will be reported later. Apparently, we now have an additional quantity (i.e., fs) to fit.

Note that since H1 seems to be in (unintentionally) an anti-spring detuning, fs should be a real number whereas it should be an imaginary number for a pro-spring case. Obviously, Q is set to infinity for simplicity.

[MCMC-based numerical fitting]

Following the work by Evan (T1500553), we adapted his code to include the spring frequency as well. In short, it is a Bayesian analysis to obtain posteriors for the parameters that we want to estimate. We gave a simple set of priors as follows for this particular analysis.

The quad plot below shows the fitting result. The estimated parameters are obtained by taking the mean values of the resutling probability distribution. As usual, the two plots on the left hand side show a bode plot of the measured and fitted data. The two plots on the right hand side show the residual of the fit. As shown in the residuals, there are several points which are as big as 20% in magnitude and 6 deg in phase below 10 Hz. Otherwise, the residual data points seem to be within 10-ish % and 4 deg. The code is attached in pdf format.

EDIT: I am attaching the actual code as well.

Images attached to this report
Non-image files attached to this report
Comments related to this report
kiwamu.izumi@LIGO.ORG - 15:15, Tuesday 05 July 2016 (28170)

A detailed derivation of the new functional form can be found at https://dcc.ligo.org/LIGO-T1600278

kiwamu.izumi@LIGO.ORG - 16:03, Tuesday 05 July 2016 (28171)

EvanG noticed that we have unintentionally included high frequency poles in the previous analysis (28157). So we made the same fitting for the data with all the high frequency poles removed.

Here are the fitting results for the latest data:

  • Optical gain = 9.070764e+05 +/- 8.071988e+02 [cnts/m]
  • Cavity pole = 3.287361e+02 +/- 5.692504e-01 [Hz]
  • Time delay = 5.554816e+00 +/- 3.424867e-01 [usec]
  • Spring frequency = 9.831483e+00 +/- 5.434934e-02 [Hz]

Since the bode plot looks very similar to the one posted above, I skip showing it here. Observe that the time delay is now smaller than it was because we now don't have the high frequency poles.

craig.cahillane@LIGO.ORG - 14:16, Friday 08 July 2016 (28274)CAL
C. Cahillane, K. Izumi

I have added in a new term to our sensing function fit, an optical spring Q factor to gain back phase information.

From the functional form f^2/(f^2 + f_s^2) we only get a magnitude correction from detuning, but we also expect detuning to slightly affect phase in the sensing function response.

This can be clearly seen in lower right subplot Figure 1 of this comment, where Kiwamu originally plotted the full RSE sensing function.  Here we see that when we have 1 degree of detuning we also have +1.5 degree phase difference at 10 Hz when compared to the sensing function without detuning. 

In the phase residual plot in the original post you can see this phase loss in the actual ER9 sensing measurement.  

In order to try and gain back some of this phase information, we have added in an additional term to the detuning function:

    f^2                        f^2
-----------    ===>  -----------------------
f^2 + f_s^2          f^2 + f_s^2 - i*f*f_s/Q

This adds another parameter to our fit, but lets us get back phase information lost to detuning.

**********

Figure 2 shows Kiwamu's original fit parameters posted above in red alongside my new results in green.
I argue that including the optical spring Q factor has improved the phase fit significantly.  
Quantitatively, here are the phase Χ-Square values:

With Optical Spring Q Χ-Square    = 85.104
Without Optical Spring Q Χ-Square = 819.28

**********

I have modified Kiwamu's SensingFunction.ipynb into a SensingFunctionSimulation.ipynb which fits to both phase and magnitude of the sensing function.  SensingFunctionSimulation.ipynb is attached as a zipped file in this aLOG and is also in a Git repo called RadiationPressureDARM owned by Kiwamu.

Fit parameters:

Optical gain = 9.124805e+05 +/- 8.152381e+02 [cnts/m]
Cavity pole = 3.234361e+02 +/- 5.545748e-01 [Hz]
Time delay = 5.460838e+00 +/- 3.475198e-01 [usec]
Spring frequency = 9.975837e+00 +/- 5.477828e-02 [Hz]
Spring Inverse Q = 1.369124e-01 +/- 3.522990e-03

(I choose to parametrize using inverse Q = Q^{-1} because Q^{-1} can be zero.)
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