Following up on this earlier observation of a change point in
DARM combs on March 14 and on comments added by Evan
and Ansel, I tried looking at possible correlations between
optical lever laser power levels and combs seen in EX and EY
magnetometers. The bottom line is that there are such
correlations, as documented in detail in the attached
annotated slides with posted spectra at a variety of power
levels (as measured by H1:SUS-ETMX/Y_L3_OPLEV_SUM_OUT_DQ).
The figures below show EX and EY before/after spectra.
In summary, the spectra show narrow lines before March 14
in combs of ~1-Hz spacing with various offsets (EX worse than EY). During
periods when the laser powers were lowered, the spectra were contaminated
by broadband noise (motivation for keeping the power high, I believe).
When the power was raised to higher than it was prior to March 14,
the broadband power dropped again, the lines persisted and were
joined by new lines with 1-Hz spacing offset from integer frequencies
by ~0.25 Hz, a comb observed to be present in DARM following March 14.
The apparent creation of a new comb in DARM from these lasers may
hint that other combs seen for a long time in DARM and in magnetometer
spectra may also arise from these lasers. Whether the mechanism is
though the optical lever damping, as suggested previously for glitches,
or through another coupling, such as ESD power supply contamination
from the laser supplies, is not clear to me.
Fig 1: EX magnetometer spectrum before maintenance work on March 14 (Interval "A" on 1st attached slide file)
Fig 2: EY magnetometer spectrum before maintenance work on March 14 (Interval "P" on 1st attached slide file)
Fig 3: EX magnetometer spectrum before maintenance work, on March 15 (Interval "Q" on 1st attached slide file)
Fig 3: EY magnetometer spectrum before maintenance work, on March 15 (Interval "V" on 1st attached slide file)
Attachment 1: Annotated slides showing spectra before / after many change points on March 14/15 of EX laser power
Attachment 2: Annotated slides showing spectra before / after a handful of change points on March 14/15 of EY laser power