I think you should use the current actual PRC & SRC cavity lengths as measured, as it would be simplest to simply replace the folding mirror optics without changing the macroscopic lengths / optic positions. (EDIT: Gautam rightly points out that we have to move things around regardless, since our current lengths include propagation through the folding mirror subtrates)

Moreover, the recycling cavity lengths you posted are not the right "ideal" lengths to use, as they do not account for the complex reflectivities of the sidebands off of the arm cavities (I have made this mistake myself). See this 40m wiki page for details.

In short, given our current modulation frequency, the ideal lengths to use would be:

• Ideal arm length of 37.795 m
• Ideal PRC length of 6.753 m
• Ideal SRC length of 5.399 m

These are the lengths that the recycling cavity optics were positioned for (though we did not achieve them perfectly). If you do a finer PRC/SRC length scan around the DRFPMI resonance of your model, you would presumably see some undesired sideband splitting. 

WFS locking point seemed degraded; I hand aligned and reset the WFS offsets as usual.

ITMX oplev recentered. While doing so, I noticed an ETMX excursion rear its head for the first time in a long while :

There was no active length control on ETMX, only OSEM damping + oplevs. Afterwards, its still moving around with only local damping on. I'm leaving the oplevs off for now.

Local EQ 3.5 mag  at 2:28 UTC May 24, 2016 Rancho Cucamonga, Ca.....no damage

Varun has received 40m specific basic safety training today.

I have modified the c1summary.ini and c1lsc.ini configuration files slightly to avoid overloading the system and remove the errors that were preventing plots from being updated after certain time in the day.

The changes made are the following:
1- all high-resolution spectra from the Summary and LSC tabs are now computed for each state (X-arm locked, Y-arm locked, IFO locked, all);
2- I've removed MICH, PRCL & SRCL from the summary spectrum (those can still be found in the LSC tab);
3- I've split LSC into two subtabs.

The reason for these changes is that having high resolution (raw channels, 16kHz) spectra for multiple (>3) channels on a single tab requires a *lot* of memory to process. As a result, those jobs were failing in a way that blocked the queue, so even other "healthy" tabs could not be updated.

My changes, reflected from May 25 on, should hopefully fix this. As always, feel free to re organize the ini files to make the pages more useful to you, but keep in mind that we cannot support multiple high resolution spectra on a single tab, as explained above.

Edited the AGC to include overlapping frames yesterday. forgot to put an elog on it!

Wrote and tested a function for downconversion. It contains a mixer with a sinusoidal input for modulation with the desired frequency and a 2nd order butterworth low pass filter to remove the higher frequency-shifted part of the modulated signal. I have tested this with input of 2kHz giving a good output of 200 Hz on the speaker. Codes are uploaded on github, will update the real time document tomorrow.

-Varun

I've been futzing with the common mode servo, trying to engage the AO path with POY for high bandwidth control of a single arm lock. I'm able to pull in the crossover and get a nice loop shape, but keep getting tripped up by the offset glitches from the CM board gain steps, so can't get much more than a 1kHz UGF.

As yutaro measured, these can be especially nasty at the major carrier transitions (i.e. something like 0111->1000). This happens at the +15->+16dB input gain step; the offset step is ~200x larger than the in-loop error signal RMS, so obviously there is no hope of keeping the loop engaged when recieving this kind of kick. Neither of the CM board inputs are immune from this, as I have empirically discovered. I can turn down the initial input gain to try and avoid this step occuring anywhere in the sequence, but then the SNR at high frequencies get terrible and I inject all kinds of crud into the mode cleaner, making the PC drive furious.

I think we're able to escape this when locking the full IFO because the voltages coming out of REFL11 are so much larger than the puny POY signals so the input-referred glitches aren't as bad. I think in the past, we used AS55 with a misaligned ITMX for this kind of single arm thing, which probably gives better SNR, but the whole point of this is to keep the X arm aligned and lock it to the Y-arm stabilized PSL. 

A package labelled 'UPS Ground' has arrived.

-Varun

I noticed that the TRY button in the ASS main screen was linking to LSC_TRX instead of LSC_TRY. Gautam fixed it.

Please do not place anything on the top of the cabinets that is not tied down. It will end up on our head in an earth quake.

Machined from I-beam 6061 T6 Aluminum 5" x 0.5 x 3.25

Atm2, version 2 "pdstand" will allow you to clamp from any direction ( Koji was right )

Completed:

Wrote and tested a code for AGC using cavity transmission signal and length error signal.

Wrote and tested a code for frequency shifting (downconversion) using mixing and LPF

Wrote a code for whitening using FFT.

Altium working on cit40m iMac

Plans:

Writing codes for Frequency warping and whitening in time domain.

Implement AGC and frequency shifting on the real time control system.

Calculate requirements for Anti-aliasing filter.

There are some issues with 5 mm sapphire prism Atm5. It will cause  interference between one of the prisms and the Side OSEM.

Here are some drawings to see the issues with larger wire standoff.

The 2 mm prism will work.with a 1 mm longer dumbell.

Quotes requested from http://photomachining.com/laser-micromachining-photomachining-contact.html and http://www.optocity.com/ 

I used a Eurocard extension board to peek at the inputs and outputs of each of the gain-ladder AD829s on input B of the CM board in the +31dB configuration with the input terminated. (i.e with the following stages active in this order: +16dB, +8dB, +4dB, +2dB, +1dB).

The voltages I observed imply that the +8dB stage has an input voltage offset of -2mV, whereas all the other positive gain stages show around +-0.5mV. This could explain the shift observed at the +15->+16 transition. (However, since both input channels show a jump here, maybe its something more systemic about the board...)

In any case, it should be simple enough to swap out a new AD829 in place of U9B and see if it improves things, before getting too deep into the muck. (In principle, the AD829 has offset nulling pins, but I'm not sure how to do it in a non-hacky way since the board doesn't have any pads for it.)

Gap of the prism from the mirror

Sag: s = R(1-Cos[ArcSin[d/2/R]])

- Mirror curvature sag for 2mm prism (R=37.75mm): s=13um

- Minimum gap: 20um => s=33um => R=15mm

- Nominal gap: 35um => s=48um => R=10mm

- Maximum gap: 50um => s=63um => R=8mm

The second figure shows somewhat realistic arrangement of the pieces

I replaced some of the AD829s with other AD829s, but the offset situation didn't improve.

However, I figured that we don't really need the ~100MHZ bandwidth of the AD829, since the IMC loop limits us to a ~10kHz CARM bandwidth. Also, since we don't routinely use IN2 for anything, I felt free to try something else. 

Specifically, I replaced all of the positive gain AD829s in the input 2 gain ladder with OP27s (U8B->U12B on D1500308), which should have input offset voltages ~30x lower than the AD829s. 

Here is a comparison of the outputs these configurations perform, normalized to the output at the +0dB gain setting - where all of the op amps in the gain ladder are bypassed. 

So, most of the transitions now result in an output offset change of less than 0.5mV, which is nice.

The exception seems to be where the +8dB stage is switched in or out. I may try replacing this one, as these transitions cause a lock loss now when trying to lock the arm with high bandwidth using POY.

Some CDS related things:

Keith Thorne has told us about a potential fix for our framebuilder woes. Jamie is going to be at the 40m next week to implement this, which could interfere with normal interferometer operation - so plan accordingly. 

I spent a little time doing some plumbing in the realtime models for Varun's audio processing work. Specifically, I tried to spin up a new model (C1DAF), running on the c1lsc machine. This included:

• Removing the unused TT3 and TT4 parts from the IOO block in c1ass.mdl, freeing up some DAC outputs on the LSC rack
• Adding an output row to the LSC input matrix which pipes to a shared memory IPC block. (This seemed like the simplest way for the DAFI model to have access to lots of signals with minimal overhead).
• Removing two unused ADC inputs from c1lsc.mdl (that went to things like PD_XXX), to give c1daf.mdl the required two ADC inputs - and to give us the option of feeding in some analog signals.
• Editing the rtsystab file to include c1daf in the list of models that run on c1lsc
• Editing the existing DAFI .mdl file (which just looked like an old recolored cut-n-paste of c1ioo.mdl) to accept the IPC and ADC connections, and one DAC output that would go to the fibox. 

The simple DAFI model compiled and installed without complaint, but doesn't succesfully start. For some reason, the frontend never takes the CPU offline. Jamie will help with this next week. Since things aren't working, these changes have not been commited to the userapps svn. 

Local EQ 3.1 mag at Jun 2, 2016 11:06:16 PM UTC, Muscoy CA........no damage

Our STS should seen this shake.

Wrote and tested a phase vocoder, with two of its applications:

1) Time scaling: This enables change of time duration without affecting the pitch.

2) Frequency warping: This changes the pitch of the sound without affecting the time duration.

1 & 2 tested offline with cavity transmission signal. 1) gives speedup of 2, and 2 gives frequency warping (pitch lowering by a factor of 2)

codes uploaded on github repo

Barring objections, starting tomorrow morning, Jamie will be testing the new FB code. The IFO will not be available for other use while this is ongoing.

I am re-starting work on the daqd upgrade again now.  Expect the daqd to be offline for most of the day.  I will report progress.

Hi!

I am Aakash Patil. I will be working at the 40m lab as a SURF student with Gautam Venugopalan on enclosures for seismometers to shield them from thermal and magnetic fluctuations. This week I will be working on the development of hardware for four probe measurement along with a constant current source. It will effectively help us in accurate temperature measurement throughout the development of enclosure.

Tried to implement AGC on FE. Had some trouble bringing the code into the correct form. It looks okay now. However, this agc code as well as idenntity code (input = output) doesnt seem to build on the c1lsc FE. Have not tried too many debugging steps yet, will come and check the problem tomorrow. 

-Varun

Summary: new daqd code running overnight test on fb1.  Stability issues persist.

The code is from Keith's "tests/advLigoRTS-40m" branch, which is a branch of the current trunk.  It's supposed to include patches to fix the crashes when multiple frame types are written to disk at the same time.  However, the issue is not fixed:

2016-06-07_20:38:55 about to write frame @ 1149392336
2016-06-07_20:38:55 Begin Full WriteFrame()
2016-06-07_20:38:57 full frame write done in 2seconds
2016-06-07_20:39:11 about to write frame @ 1149392352
2016-06-07_20:39:11 Begin Full WriteFrame()
2016-06-07_20:39:13 full frame write done in 2seconds
2016-06-07_20:39:27 about to write frame @ 1149392368
2016-06-07_20:39:27 Begin Full WriteFrame()
2016-06-07_20:39:29 full frame write done in 2seconds
2016-06-07_20:39:43 about to write second trend frame @ 1149391800
2016-06-07_20:39:43 Begin second trend WriteFrame()
2016-06-07_20:39:43 about to write frame @ 1149392384
2016-06-07_20:39:43 Begin Full WriteFrame()
2016-06-07_20:39:44 full frame write done in 1seconds
2016-06-07_20:39:59 about to write frame @ 1149392400
2016-06-07_20:40:04 Begin Full WriteFrame()
2016-06-07_20:40:04 Second trend frame write done in 21 seconds
2016-06-07_20:40:14 [Tue Jun  7 20:40:14 2016] main profiler warning: 1 empty blocks in the buffer
2016-06-07_20:40:15 [Tue Jun  7 20:40:15 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:16 [Tue Jun  7 20:40:16 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:17 [Tue Jun  7 20:40:17 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:18 [Tue Jun  7 20:40:18 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:19 [Tue Jun  7 20:40:19 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:20 [Tue Jun  7 20:40:20 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:21 [Tue Jun  7 20:40:21 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:22 [Tue Jun  7 20:40:22 2016] main profiler warning: 0 empty blocks in the buffer
2016-06-07_20:40:23 [Tue Jun  7 20:40:23 2016] main profiler warning: 0 empty blocks in the buffer

This failure comes when a full frame (1149392384+16) is written to disk at the same time as a second trend (1149391800+600).  It seems like every time this happens daqd crashes.

I have seen other stability issues as well, maybe caused by mx flakiness, or some sort of GPS time synchronization issue caused by our lack of IRIG-B cards.  I'm going to look to see if I can get the GPS issue taken care of so we take that out of the picture.

For the last couple of hours I've only seen issues with the frame writing every 20 minutes, when the full and second trend frames happen to be written at the same time.  Running overnight to gather more statistics.

38 restarts overnight.  Problem definitely not fixed.  I'll be reverting back to old daqd and fb this morning.  Then regroup and evaluate options.

Aakash Patil received 40m specific basic safety training.

[EDIT: corrected name of installed card]

We just installed a Spectracom TSyc-PCIe timing card on fb1.  The hope is that this will help with the GPS timeing syncronization issues we've been seeing in the new daqd on fb1, hopefully elliminating some of the potential failure channels.

The driver, called "symmetricom" in the advLigoRTS source (name of product from competing vendor), was built/installed (from DCC T1500227):

Summary: I am implementing digital audio filtering on various interferometer signals in order to listen to the processed audio which will help in characterizing and noise reduction in the interferometer. Following is an implementation of an Automatic Gain control (AGC) block on an LSC input signal.

Details of AGC: Currently, the AGC code implemented on FE takes input to fill a frame, then calculates the power in each frame and gives an appropriate gain to it, so that the new power content is to the required level. It is then written to the output, frame by frame. The frame is currently a rectangular window. The frame length and hop size can be adjusted. Current values are as follows:

frame length is 512 samples

hop length is 128 samples.

The input and output are delayed by 1 frame.

Details of testing: Attachment 1 shows a simulink diagram of the DAF system. Eric made this and I modified it later on. Testing was done using signal from the "LSC1" channel. Attachments 2 and 3 show aquired input and output of the AGC respectively. Gain of the preamp of the LSC input signal was varied over a total time span of 200 s. Each gain value was kept for a duration of about 20 seconds. The varying power levels can be seen in the input plot.

The output shows a uniform power level throughout.

Me and Gautam yesterday opened the tilt-free seismometer enclosure to see if we could use the thermocouples and
other things previously used by Megan. But we are planning to get new four-wire RTDs for our work.
For the next day or two, I will be trying to set up Acromag Busworks terminal so that the data logging during
this enclosure development experiment becomes perfect and easy. Johannes has sent me the wiki page URL for the same.

Something is wrong with the timing we're getting out of the symmetricom driver, associated with the new spectracom card.

controls@fb1:~/rtscore/tests/advLigoRTS-40m/src/drv/symmetricom 127$ lalapps_tconvert 
1149538884
controls@fb1:~/rtscore/tests/advLigoRTS-40m/src/drv/symmetricom 0$ cat /proc/gps 
704637380.00
controls@fb1:~/rtscore/tests/advLigoRTS-40m/src/drv/symmetricom 0$ 

The GPS time is way off, and it's counting up at something like 900 seconds/second.  Something is misconfigured, but I haven't figured out what yet.

The timing distribution module we're using is spitting out what appears to be an IRIG B122 signal (amplitude moduled 1 kHz carrier), which I think is what we expect.  This is being fed into the "AM IRIG input" connector on the card.

Not sure why the driver is spinning so fast, though, with the wrong baseline time.  Reboot of the machine didn't help.

I've restarted the old daqd on fb until I can figure out what's going on with the symmetricom driver on fb1.

Steve:  Jamie with hair.... long time ago
 

Today I tried to setup Acromag Busworks card. I was able to calibrate and test it over USB but I couldn't test it over ethernet. I'll utilize a few hours tomorrow to test it over ethernet and see if I can make it work. I have also found a few RTDs which I want to use for temperature sensing via four probe method. So, tomorrow I'll get these RTD details revived by Gautam and Steve.

I was wondering if we have a basic DAQ card with maybe 4 channels which is simple to setup like NI DAQ cards.

Eric gave me a psd plot of a signal which would be the input of a channel of the AA filter. the Nyquist freq. is about 32.8kHz.

Following are plots depicting the ratio of the aliased downconverted signal and the signal below 32.8 kHz. The first plot is for (to-be) aliased signal frequencies from 32.8 to 65.5k, and the second plot is for (to-be) aliased signals from 65.5k to 98.3k. In case of the first plot, the 36kHz peak will alias to 29kHz, and is about 30 times (29.5dB) greater than the signal there. Hence, the filter should give about 70dB attenuation there. Since this attenuation is not required by most other frequencies up to 65.5k, an option could be to use a notch filter to remove the frequency peak at 36k, and put a requirement of 45-50 dB attenuation on other frequencies.

In case of the second plot, the frequencies between 90 to 100k again need to be attenuated by more than 70 dB. However, if there is a -20dB/decade slope in stop band, we already have about 10 dB attenuation here as compared to around 32k.

The X axis of both plots is in Hz.

EQ  5.2 mag at Jun 10, 8:04 am UTC, Borego Spring, CA  ~150 mi away.........no obvoius damage, damping restored, MC is locking, arms are flashing

Looks like we might have a problem with the IRIG-B output of the GPS receiver.

Rolf came over this morning to help debug the strange symmetricom driver behavior on fb1 with the new Spectracom card.  We restarted the machine againt and this time when we loaded the drive rit was clocking at a normal rate (second/second).  However, the overall GPS time was still wrong, showing a time in October from this year.

The IRIG-B122 output is supposed to encode the time of year via amplitude modulation of a 1kHz carrier.  The current time of year is:

controls@fb1:~ 0$ TZ=utc date +'%j day, %T'
162 day, 18:57:35
controls@fb1:~ 0$ 

The absolute year is not encoded, though, so the symmetricon driver has the year offset hard coded into the driver (yuck), to which it adds the time of year from the IRIG-B signal to get the correct GPS time.

However, loading the symmetricom module shows the following:

...
[ 1601.607403] Spectracom GPS card on bus 1; device 0
[ 1601.607408] TSYNC PIC BASE 0 address = fb500000
[ 1601.607429] Remapped 0xffffc90017012000
[ 1606.606164] TSYNC NOT receiving YEAR info, defaulting to by year patch
[ 1606.606168] date = 299 days 18:28:1161455320
[ 1606.606169] bcd time = 1161455320 sec  959 milliseconds 398 microseconds  959398630 nanosec
[ 1606.606171] Board sync = 1
[ 1606.616076] TSYNC NOT receiving YEAR info, defaulting to by year patch
[ 1606.616079] date = 299 days 18:28:1161455320
[ 1606.616080] bcd time = 1161455320 sec  969 milliseconds 331 microseconds  969331350 nanosec
[ 1606.616081] Board sync = 1
controls@fb1:~ 0$ 

Apparently the symmetricom driver thinks it's the 299nth day of the year, which of course corresponds to some time in october, which jives with the GPS time the driver is spitting out.

Rolf then noticed that the timing module in the VME crate in the adjacent rack, which also receives an IRIG-B signal from the distribution box, was also showing day 299 on it's front panel display. We checked and confirmed that the symmetricom card and the VME timing module both agree on the wrong time of year, strongly suggesting that the GPS receiver is outputing bogus data on it's IRIG-B output, even though it's showing the correct time on it's front panel.  We played around with setting in the GPS receiver to no avail.  Finally we rebooted the GPS receiver, but it seemed to come up with the same bogus IRIG-B output (again both symmetricom driver and VME timing module agree on the wrong day).

So maybe our GPS receiver is busted?  Not sure what to try now.

The GPS receiver (EndRun Technologies box in 1Y5? (rack closest to door)) seems to not coming back up properly after the reboot.  The front pannel says that it's "LKD", but the "sync" LED is flashing instead of solid, and the time of year displayed on the front panel is showing day 6.  The fb1 symmetricom driver and VME timing module are still both seeing day 299, though.  So something may definitely be screwy with the GPS receiver.

ETMX has been jumping around again lately. Just now, I zeroed the ETMX alignment offsets in the SUS model, and centered the ETMX oplev spot via slow machine sliders. OSEM damping is on, oplev damping is off. Let's see how it moves around in the next day or so. 

GPS: 1149635923 

UTC: Jun 10 2016 23:18:26

The mode cleaner was misaligned probably due to the earthquake (the drop in the MC transmitted value slightly after utc 7:38:52 as seen in the second plot). The plots show PMC transmitted and MC sum signals from 10th june 07:10:08 UTC over a duration of 17 hrs. The PMC was realigned at about 4-4:15 pm today by rana. This can be seen in the first plot.

The PMC transmission slow degration or it's input beam is not stable.

About acquiring data: Initially I couldn't start with proper Acromag setup as the Raspberry pi had a faulty SD card slot. Then Gautam gave me a working pi on which I tried to install EPICS. I spent quite a time today but couldn't setup acromag over ethernet.  But, it would be great if we have a USB DAQ card. I have found a good one here http://www.mccdaq.com/PDFs/specs/USB-200-Series-data.pdf It costs around 106$ including shipping (It comes with some free softwares for acquiring data) . Also, I know an another python based 12bit DAQ card (with an inbuilt constant current source) which is made by IUAC, Delhi and more information can be found here http://www.iuac.res.in/~elab/expeyes/Documents/eyesj-progman.pdf  It costs around 60$ including shipping.

About temperature sensing: The RTD which I found on Omega's list is having a temperature resolution of 0.1 deg C. I have also asked them for the one with good resolution. Also according to their reply, they have not performed any noise characteristics study for those RTDs.

 

Summary: I am implementing digital audio filtering on various interferometer signals in order to listen to the processed audio which will help in characterizing and noise reduction in the interferometer. following is a summary of the gui i have made towards a general purpose DAF module linked to the LSC. 

Details:  attachment 1 shows the top level overview of the daf module.

The "INPUTS" button shown redirects to the medm screen shown in attachment 2, which is a collection of inputs going into the module.

Each of the buttons shown in "C1DAFI_INPUTS.png" is further linked to various i/o boxes like adc1, adc2, lsc signal and exitation. An example is shown in attachment 3. This is the specific I/O box for the LSC signal.

The field labelled "INPUT_MTRX" is linked to a matrix which routes these 4 inputs to various DSP blocks. Similarly, the "OUTPUT_MTRX" tab is useful for choosing which output goes to the speaker. 

Time and computational load monitoring is done in the "GDS_TP" tab which links to the medm screen shown in attachment 4.

Currently the AGC is successfully implemented as one of the DSP block. The details of the AGC implementation were given in a previous elog: https://nodus.ligo.caltech.edu:8081/40m/12159

I need to make a few changes to the code for Frequency Shifting and Whitening before uploading them on the FE. I will put the details soon.

Some more things that I think need to be added: 

1) "Enable" buttons for each of the DSP blocks.

2) Labels for each of the matrix elements.

3) Further headers and other description for each of the tabs 

The drill room floor will be retiled Thursday, June 16. Temporary nitrogen line set up will allow emptying the hole area.

Ifo room entry will be through control room.

In preparation for the armloss map I checked the calibration of the Y-Arm ITM and ETM OpLevs with the method originally described in https://nodus.ligo.caltech.edu:8081/40m/1247. I was getting a little confused about the math though, so I attached a document at the end of this post in which I work it out for myself and posteriority. Stepping through an introduced offset in the control filter for the corresponding degree of freedom, I recorded the change in transmitted power and the reading of the OpLev channel with the current calibration. One thing I noticed is that the calibration for ITM PIT is inverted with respect to the others. This can of course be compensated at any point in any readout/feedback chain, but it might be nice to establish some sort of convention where positive feedback to the mirror will increase the OpLev reading.

The calibration factors I get are within ~10% of the currently stored values. The table (still incomplete, need to relate to the current values) summarizes the results:

The individual graphs:

ETM PIT

ETM YAW

ITM PIT

ITM YAW

The math:

We generally want to keep the configuration of the 40m close to that of the LIGO sites, which is why we chose BusWorks, and it is also being established as a standard in other labs on campus. Of course any suitable DAQ system can do the job, but to stay relevant we generally try to avoid patchwork solutions when possible. Did you follow Aidan's instructions to the book? I haven't set up a system myself, yet, so I cannot say how difficult this is. If it just won't work with the Raspberry Pi, you could still try using a traditional computer.

Alternatively, following Jamie's suggestions, I'm currently looking into using python for the modbus communications (there seem to be at least a few python packages that can do this), which would reportedly make the interfacing and integration a lot easier. I'll let you know when I make any progress on this.

Within two hours, it was already all over the place. 

It has been Decided: we will assemble a suspension with the spare ETM optic with the current-generation standoff for installation ASAP. I.e. no new custom parts. We will continue pursuing the new standoff design, but we need our interferometer back.

What about ETMY? and are these really microradians or just some made up cal?

I'm running another overnight test with new daqd software on fb1.  The normal daqd process on fb has been shutdown, and the front ends are sending their signals to fb1.

fb1 is running separate data concentrator (dc) and  frame writer (fw) processes, to see if this is a more stable configuration than the all-in-one framebuilder (fb) that we have been trying to run with.  I'll report on the test tomorrow.

I have added Enable buttons for each of the DSP blocks, and labels for the matrix elements. The input matrix takes inputs from each of the 4 channels: ADC1, ADC2, LSC and EXC, and routes them to the audio processing blocks (attachment 2). The output matrix (attachment 3) takes the outputs of the various DSP blocks and routes them to the output and then to the speakers.