Reports until 02:40, Wednesday 31 October 2018
H1 ISC
sheila.dwyer@LIGO.ORG - posted 02:40, Wednesday 31 October 2018 - last comment - 15:40, Wednesday 31 October 2018(44938)
pico'd POP QPDs

Sheila, Georgia, Craig, Jamie, Keita

Summary:

We picomotored the POP QPDs so that we are now on both QPDs, we had some difficulties doing this but we think that we have recovered and reset the QPD offsets to a reasonable place. 

Details:

After we saw the coupling of HAM3 motion to PRCL and DARM that Georgia is writing about, Keita pointed out that scattered light in the POP QPD path could easily couple to the LSC POP path.  Since the beam was falling off POP B which we don't use in loop, I attempted to use the pico's while we were locked at low noise. 

Side note about PRC2 cut offs:

Comments related to this report
georgia.mansell@LIGO.ORG - 02:50, Wednesday 31 October 2018 (44940)

Attaching spectra of DARM and PRCL while HAM3 ISI RY is driven (bottom left and right plots). Dark blue is earlier tonight, before pico'ing onto the POP QPD. Mint green is later tonight, after pico'ing - note the IFO alignment changed between these measurements, we don't know the origin of the change in coupling. More details on this measurement in alog-44939.

Images attached to this comment
keita.kawabe@LIGO.ORG - 15:40, Wednesday 31 October 2018 (44949)

After pico-ing, POPA SUM increased by about 3%, POPB about 1%.

Images attached to this comment