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Reports until 14:49, Wednesday 18 May 2022
H1 ISC (CAL, CDS)
jeffrey.kissel@LIGO.ORG - posted 14:49, Wednesday 18 May 2022 - last comment - 10:59, Thursday 19 May 2022(63210)
Clean up of OMC DCPD Input Filtering banks ... Somehow that improved glitchiness?
J. Kissel

It's been on the to-do list for several years now to move the EPICs gain of 1000 in to a filter module, such that H1's and L1's rough calibration into millamperes [mA] is done in a similar fashion (see comparison of how it's been done for years in G1700316, Appendix A, Slide 19). 

As such, I took the IFO down time this afternoon to
    (a) Clean up all the now obsolete O3-era whitening and transimpedance filter banks, and 
    (b) Move the EPICs gain of 1000 into a filter module, FM10, called "A2mA"

In doing so -- to sanity check that moving the gain into a filter bank produces the same output I compared an ndscope of the raw data, 
    H1:OMC-DCPD_A_OUT_DQ
    H1:OMC-DCPD_B_OUT_DQ
before and after the change. 

I was very surprised to see that there was a difference in gain on the DCPD B channel and even crazier, a cleaner character (less high frequency spikes) on both channels.

Unfortunately, as seems to be my life, a "quick sanity check" must now turn into a full fledged investigation as to what's going on.
Stay tuned on that.

In the mean time, I post screenshots (in order of appearance) of 
    - the "before" configuration of the banks, 
    - the design of the new "A2mA" filter, 
    - the diff of what changed in the filter backs according to the front-end, 
    - the "after" configuration of the banks,
    - the sanity check time series before vs. after (where the off-chart time in the middle is when both the A2mA gain of 1000 and the EPICs gain of 1000 are unphysically on for a moment while I switched)
    - the SDF acceptance of this new configuration.
Images attached to this report
Comments related to this report
jeffrey.kissel@LIGO.ORG - 14:57, Wednesday 18 May 2022 (63212)CDS, CSWG, SEI
WUT

Reference traces are in the before configuration.
Live traces are in the after configuration.
Images attached to this comment
daniel.sigg@LIGO.ORG - 15:03, Wednesday 18 May 2022 (63213)

Was the shutter closed? If not, you may just see some flashing in the OMC. I found a flashing OMC to produce a rather non stationary signal.

jeffrey.kissel@LIGO.ORG - 15:12, Wednesday 18 May 2022 (63214)CSWG
@Daniel, the OMC was flashing transmitted light on the DCPDs, but the same character of incoming light was on both sides of the change. There were no less or more flashes before vs. after the change.

Definitely worth a test with no light, or with stable amounts of light, for sure, though.
jenne.driggers@LIGO.ORG - 10:59, Thursday 19 May 2022 (63232)

The OMC guardian had a hard-coded gain value of 1000.  With this move of that gain to the filter bank, I have changed OMC guardian to set the gain to 1.

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