Summary:
We were able to lock the squeezing angle using the 3MHz signal from the OMC DCPD's, and we have caused a few lockloses. We have found that our locking scheme is introducing a lot of noise, so our next step is to lock the OPO length to the laser frequency.
Locklosses:
In our first attempt we used the interferometer locked at 2W DC readout to look for the LO error signal. We caused a lockloss then, and so we then changed to working with the interferometer locked on RF and the OMC locked. We caused a couple of other locklosses this afternoon, one when the interferometer was locked on RF and the OPO became unlocked with the beam diverter open. After this we added closing the beam diverter to the OPO guardian DOWN state, and the state CHECK_EOM (which we enter when the TTFSS EOM is railed).
After successfully locking the squeezer angle, we transitioned to DC readout. When we attempted to close the beam diverter we lost lock, which we also don't understand.
We have been injecting ~10uW of CLF (measured on SQZT6), which gives us about 10 dBm of RF on the 3MHz demod. We are wondering if this is too much and might be part of our lockloss problems. We tried reducing it by a factor of 2.
Locking:
Nutsinee will post details of the squeezing angle lock configuration that we used tonight, even though we don't plan to keep using this scheme.
The basic steps:
Uncontrolled squeezing:
I am not sure what the free-running plot represents. In this case, the 2 lasers differ in frequency by as much as tens of kHz. This would completely invalidate the correlations that are responsible for squeezing. Every now and then the frequencies will cross and one might catch a short glimpse of (anti) squeezing.
The first plot is somewhat of a mystery too. If we really suffer from excess phase noise (as we have measured), why doesn't it effect squeezing at all frequencies? Could it be seeding through the CLF instead?
For reference, at LLO the nominal CLF power (measured on SQZT6) was 50 uW, tests up to 200 uW didn't show a large amount of seeding ( LLO log 41270). So, in principle 10 uW should be well below the seeding threshold.
On the other hand, some "seed hunting" on the double AOM path on ISCT6 was done before injection in the intererferometer, see for example: LLO log 37945 . I don't recall if you have done a similar characterization at LHO.
Lisa- no we haven't done any seed hunting here.
Daniel- I agree that it isn't clear what is happening without the CLF injected, especially since the level of anti squeezing is way too high.
The 10µW is measured transmitted by the OPO, I believe the 50-200µW at L1 are incident to the OPO. The CLF LO signal is fairly high with ~6 dBm (in the quad phase) when we are locked.
So, about the CLF power: all of the numbers reported in the LLO log so far quote the CLF power as measured on the CLF REFL diode, so BEFORE entering the OPO. The OPO has a 4% transmission for the 3 MHz - so indeed the 10 uW quoted for this LHO attempt, measured AFTER the OPO, are 5 times higher than the 50 uW used at LLO, since 50 uW * 0.04 = 2 uW of CLF AFTER the OPO. So, as we all discussed today, the first test would be to lower this power and see if the extra noise is caused by that.