Removed these channels until Beckhoff issue is resolved.

The dmtviewer process on projector0 had used up all available memory on projector0 and had quit running.  I rebooted the computer and restarted the dmtviewer shortly after 9 AM this morning.

Laser Status: 
SysStat is good
Output power is 33.3 W (should be around 30 W)
FRONTEND WATCHdog is Active
HPO WATCH is RED

PMC:
It has been locked 13 day, 1 hr 26 minutes (should be days/weeks)
Reflected power is 2.0 Watts  and PowerSum = 25.8 Watts.
(Reflected Power should be <= 10% of PowerSum)

FSS:
It has been locked for 3 days, 21 h and 33 min (should be days/weeks)
Threshold on transmitted photo-detector PD = 2.265V (should be 0.9V)

ISS:
The diffracted power is around 7.4% (should be 5-15%)
Last saturation event was 3 days, 21 h and 38 minutes ago (should be days/weeks)

David B., Jim B., Patrick T.

We looked at H1:ALS-Y_REFL_SERVO_IN1EN from '00:00:00 Nov 2 PDT' to '03:00:00 Nov 2 PST'. The correct behavior is observed:

...
11/02/2014 01:59:59.005479920 PDT 	Off 	NO_ALARM 	NO_ALARM
11/02/2014 01:59:59.055615806 PDT 	On 	NO_ALARM 	NO_ALARM
11/02/2014 01:00:01.060458106 PST 	Off 	NO_ALARM 	NO_ALARM
11/02/2014 01:00:01.110599290 PST 	On 	NO_ALARM 	NO_ALARM
...

Note that PDT and PST should be specified for searches covering times of the changeover.

Here is the list of commissioning task for the next 7-14 days:

Locking team:

1. Fix ALS DIFF feedback path (ESD/SUS crossover).
2. DRMI stability with new 3f detector modification.
3. Check RF power on 2f detectors.
4. Carrier sweeps with DRMI locked o new 3f.
5. Common hand-off to transmitted power.
6. Lock interferometer.
7. Resolve down stream clipping issues in the SRC.

Modecleaner team:

1. Investigate long-term alignment stability of mode cleaner.
2. Minimize intensity noise coupling through mode cleaner.
3. Optimized auto alignment scheme to minimize coupling.

Alignment team:

1. Revisit EY green WFS beam path and look for ghost beams.
2. Make EY green WFS work again.
3. Install EX green WFS auto-centering hardware.
4. Commission an arm alignment controls topology which can be used for initial alignment.
5. Integrate green WFS into initial alignment.

RF:

1. Make an assessment of RF cross talk into the IMC AOM.
2. Investigate EMI radiation by the VCOs and the fixed frequency OCXO.

The question of whether Operators have been checking the Observation Intent button came up this morning (basically we have).  I was curious to see how much this button is being used and how quick Operators are to Unclick it at the beginning of our shifts.   

I went ahead and trended/Conlog-ed the channel (H1:ODC-GRD_OPERATOR_OBSERVATION_READY).  Attached is a trend of the channel over the last 60 days.  Over this time we've had (6) "Undisturbed" segments (only counting segments over 30min):

1. 9/18
2. 10/2
3. 10/5
4. 10/8
5. 10/11 (over a weekend)
6. 11/7

In all of these instances, the Button was taken to "Commissioning" within the first few minutes-hour of the Operator shift. 

Note for Operators: 

• Please make sure this is one of the first things you check at the beginning of your shift!
• If there was an Undisturbed Segment overnight, please check the Access System for any incursions during the segment and make an alog entry stating when these incursions were (this has been added to the Operator Checksheet).

Note On Overnight Measurements & Request To Limit Early Morning Access (i.e. Cleaning)

With Operator shfits starting at 8am, there can be instances when the cleaning crew can enter the VEAs when we are in an "Undisturbed" Observation Intent state.  Now if there is ever a need  to limit cleaning activity due to overnight measurements:  please send an email to Jodi and/or Christina so they have a heads up for the cleaning team.  Otherwise, one can do what was suggested by Ed M. in his alog last week (i.e. post signs on doors requesting to postpone cleaning in the morning).

I manually added H1:LSC-PD_DOF_MTRX_LOAD_MATRIX to Conlog. The script that generates the channel list needs to be modified to add this channel. Otherwise if a new channel list is generated by the script and used, this channel will be removed. I will plan to make the change to the script on Tuesday as part of maintenance.

This morning ISS diff power was at ~11.6%. REFSIGNAL was @ -2.02V. I adjusted REFSIGNAL to -2.11. diff power is currenly at ~7%.

Attached is ten days of minute trends for some channels at EndX and EndY for the HEPI Pump systems.

At EndX, the Pump is still controlled(Ch2) by the last pressure sensor on the Pump Station skid(Ch1.)  At EndY, the control was switched early Thursday to the actual differential pressure across the actuators measured in the VEA (Ch5.)  On Friday, you can see where I smoothed the Supply & Return pressures and the Max/Mins of the differential pressure and the subsequent drive to the Pump Motor.  It looks like the diurnal temperature fluctuations are increased significantly when the daily fluctuations or the daily minimum exceed some threshold.

We still have room to improve the grounds noise but I don't believe there is any reason not to switch all the Pump Stations to the differential control.

• 3IFO work:  NO craning, but LVEA bifurcated for laser state in LVEA (and will go until noon)
• SEI--tomorrow HAM2/3 matrices change. 
• HAM oplevs were re-installed (suresh)
• EX cabling, and then EY cabling (Filiberto & crew)
• Talk about whether
• OFI measurement in H2 enclosure (Gerardo)
• Vacuum rack investigations (Richard)
• Preparing for cold snap

no restarts reported

model restarts logged for Sat 08/Nov/2014
2014_11_08 00:27 h1fw1
2014_11_08 17:29 h1fw1

both unexpected restarts.

Nic, Evan

We have gotten DRMI to lock on the 3f signals using the new, modified BBPD serving as REFLAIR_B.

Some good UTC times for 3f locking: 2014-11-09 0:56:50, 01:13:10, 02:41:00

Judging by POPAIR_B_RF18_I_ERR, the lock is kind of ratty both on 1f and 3f.

I think the reason Alexa and I couldn't lock yesterday is that we had the wrong relative gain for RF135Q/RF45Q. Nic and I remeasured it today and got 2.0. It is still true, however, that the ramping matrix doesn't give the expected behavior; it seeems to approach the requested value almost asymptotically, taking far longer than the specified ramp time.

We then adjusted the gains in the 3f input matrix to reduce gain peaking in the demodulated spectra of RF27 and RF135. We have written the following matrix elements into the lscparams guardian file:

• RF27I → PRCL = −4.0
• RF135Q → MICH = 2.0
• RF27I → SRCL = −0.6
• RF135I → SRCL = 1.7

Attached are our measured OLTFs of PRCL, MICH, and SRCL while locked on 3f. The DTT files are in my directory under Public/2014/11/DRMI3f.

model restarts logged for Fri 07/Nov/2014
2014_11_07 06:28 h1fw1

unexpected restart of h1fw1, first one since Monday.

Alexa, Daniel, Evan

In order to use the new REFLAIR_B, we have made the following changes:

• The whitening gains are now 30 dB and 18 dB for RF27 and RF135, respectively.
• The dark offsets for RF27 and RF135 have been measured and nulled.
• The demod phases have been adjusted to 115.5° and 20° for RF27 and RF135, respectively. By driving PR2 at 131 Hz and SR2 at 184 Hz, we find that the PRCL and SRCL signals can now be made to appear in the correct quadratures (see first attachment).
• By driving a 5.75 Hz line in PRCL (and subsequently SRCL and MICH), we have measured the relative gains between the 1f and 3f signals:

  	PRCL	SRCL	MICH
  RF27I/RF9I	−0.49	−3.9
  RF135I/RF45I		2.4
  RF135Q/RF45Q			0.46 2.0

  The RF27I/RF9I measurement for SRCL is low SNR for some reason. [Edit, 2014-11-05: I think I must have taken the RF135Q/RF45Q measurement upside-down. I retook it today and got a magnitude of 2.0.]

By using these gain measurements to adjust the DRMI 1f matrix elements, we have tried to transition from DRMI 1f to DRMI 3f. Howver, so far it keeps dropping lock.

The demodulated 1f and 3f spectra (taken while DRMI is 1f locked) are attached (units are cts/rtHz).

(Keita Daniel)

A spare BBPD with serial number S1200247 has been modified by removing and bypassing U1, the first RF amplifier stage. The attached BBPD_tf1.pdf file shows the transfer function before and after. Plot tf2 shows the ratio.

We took a baseline intermodulation product measurement by sending a two tone signal into the AM laser. The first tone was at 45 MHz and generated a line with -15 dBm amplitude. The second tone was a 90 MHz line also at -15 dBm. Plot IP2.png shows IP2 and IP3 lines at 135 MHz and 180 MHz with amplitudes of -57 dBm and -60 dBm, respectively.

The plot labeled IP2M shows the same measurement after the removal of U1. Close-in plots IP2M135 and IP2M180 show spectra with lower resolution bandwidth. The intermodulation lines are visible at a level around -115 dBm. One might consider this an upper limit, since the dominant distortion could be in the AM laser head. The IP2M135A plots shows one of the lines moved by 100 Hz. This now separates IP2 (lower frequency) and IP3 lines.

Finally, the IP2Mplus plot includes 20 dB higher drive levels to bring the lines back to -15 dBm. The 135 MHz lines shows up at -90 dBm which seems puzzeling low compared to the above measurement.