ISC Meeting on 2015/11/30
14:00 - 15:15 on SeeVogh
Participants: H. Yamamoto, Michimura, Aso, Akutsu, Okutomi, Hirose, Somiya
- Requests for coating requirements from LMA (Aso)
- We got requests to relax requirments for coating of various mirrors from LMA.
- The following changes will be made
- Green transmission for TMs
- Finesse of the arm for green should be higher than 6 to avoid unwanted resonances of higher order modes. For safety, we decided to make it 50. With the relaxed transmission error, the finesse will be in the range of 40 - 60, which is still fine.
- Old: 6% +/- 0.5%
- New: 6% +/- 1%
- ITM AR reflectivity
- ITM AR reflection will be used as POX and POY. Therefore, we need non-zero reflectivity. The PRC cavity can tolerate a loss of 1000ppm.
- Old: 200ppm +100/-0
- New: 300ppm +/-100ppm
- ETM AR reflectivity
- The ghost beam from the ETM AR will be separated inside the BRT when the beam size becomes small.
Old: <50ppm
New: < 100ppm
Reference: LIGO requirement is < 500ppm. Actually measured value vary a lot from 20ppm to 700ppm.
- The difference between 50ppm and 100ppm is insignificant
- PRM/SRM AR reflectivity
- Separation of the PRM ghost beam was not yet considered.
Old: < 50ppm
New: < 100ppm
- SRM HR transmission
- Old: 15.36% +/-0.1%
- New: 15%+/-1%
- The linear range of the SRCL signal is fine with this relaxed error range.
- The WFS shot noise change only about 5% with the above error.
- Somiya-san will check the effect on the sensitivity.
- Green transmission for TMs
- Electronics Preparation Status (Michimura, Aso)
- Cable (Michimura)
- Delivered to the site. Now in the tunnel (低温機械室)
- RF flexible cables are also included, but some RF flexible cables are in NAOJ room at Kamioka.
See this ISC cable list.
- RF distribution (Komori, Michimura)
- The panel should have been delivered to Kamioka
- Need to arrange people to assemble the box
- RFPD/QPD (Aso, Doi)
- The first delivery will be in the middle of Dec.
- For MC lock, we need one extra RFPD. We have the stuffed PCB but no box. Fujisawa-san at Toyama University is now making a box. Asked Doi-san to supervise her and finish the box production by the end of the week of 11/30.
- Diff-to-Single converter
- For bKAGRA, we need to make official converters.
- For iKAGRA, we can use a passive conversion boxes. Just connect the cold line to GND through a resistor (1kOhm or so).
- The above box needs to be made
- Cable (Michimura)
- Magnet Noise (Michimura)
- Decided to reduce the size of BS magnets by a factor of 30 from the current design. IM magnets will also be smaller (1/3 to 1/10).
- VIS members (Mark and Fabian) will design new flags for the BS and SR
- OMC (Somiya)
- We need to decide where to level the beam in the output chain: Befoer OFI ?, after OFI ?
Do we need steering mirrors before OFI ? -> Needs to be discussed with quantitative assesment of scattering noise from various optical components.
How much light power will be picked off for the AS WFS ? -> 1%
- FFT Simulation (Hirose, H. Yamamoto)
- No update