Size: 2498
Comment:
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Size: 1329
Comment:
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Deletions are marked like this. | Additions are marked like this. |
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* eZuce: Izumi, Inoue, Yamamoto(Toyama), Suzuki, Miyoki, Yokozawa, Ohashi, Izumi, Nakano, Stefan | * eZuce: Izumi, Inoue, Yamamoto(Toyama), Suzuki, Miyoki, Yokozawa, Ohashi, Izumi, Stefan |
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* [[https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0083/G1808352/001/G1808352_v1.pdf]] | |
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== MC realignment == * MC will be re-aligned today. |
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== MC realignment == | |
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* BO card was broken and it was replaced. * BO check card is still connected between BO card and circuit to break ground loop. |
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* [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5227]] * Trying to implement an offset using slow output into EXC. |
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== 1. X arm commissioning == * [[https://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=8343|JGW-T1808343]] * Do we need WFS?(Eleonora) -> Yes, with control system.(Izumi) * Gouy phase measurement for green is also necessary. (Akutsu) * Both mirrors are at the room temperature. (Uchiyama) * Needs preparation list. (Aso) * Loss measurement will performed mainly reflection light. (Izumi) * Simulation of loss? (Eleonora) -> Hirose, Hiro Yamamoto * Camera view? (Stefan) -> PCal camera, transmitted camera * Which port will be used for locking? (Miyakawa) -> REFL port == 2. New 40 W laser == * RIN measurement * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5055]] * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5124]] * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5126]] * Non-stational noise happens but it is not related water cooler. * This RIN level cannot reach shotnoise level with the first ISS loop. Current noise is 2 orders lager than NPRO noise. Needs 2nd loop to reach design level. * Beam profile * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5068]] * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5084]] - OSA measurement * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5139]] == 3. PMC electronic hack == * [[http://klog.icrr.u-tokyo.ac.jp/osl/?r=5155]] * MATSUSADA HV driver has 10uV/rHz, quite high. * Slow output can be used as offset, and 2nd EXC point will be used as input. * LIGO is not using temperature controller. (Stefan) |
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* Next meeting: 5/29. | * Next meeting: 6/19. |
Minute of KAGRA commissioning meeting
- Date: 2018/6/12 11AM~12PM
- Attendance: Miyakawa, Aso, Yamamoto, Tomura, Enomoto
- eZuce: Izumi, Inoue, Yamamoto(Toyama), Suzuki, Miyoki, Yokozawa, Ohashi, Izumi, Stefan
0. Schedule
- k1ix0 will be needed by September for NAB PD.
ETMX status
http://klog.icrr.u-tokyo.ac.jp/osl/?r=5224
- ring on f0 got lower and on the f1 by a few mm.
- f0 TF had no response. Line to coil was cut. It had been repaired before and it was used again.
- It will be fixed around September as 1week work. Whole coil will be replaced.
X arm commissioning/preparation
- WFS target: 10nrad.
Satellite box modification
https://gwdoc.icrr.u-tokyo.ac.jp/DocDB/0083/G1808352/001/G1808352_v1.pdf
- 100nF cap will be implemented to avoid an oscillation. It introduce 41Hz pole.
MC realignment
- MC will be re-aligned today.
FSS BO
- BO card was broken and it was replaced.
- BO check card is still connected between BO card and circuit to break ground loop.
PMC installation, circuits, adding offset
- Trying to implement an offset using slow output into EXC.
IOO schedule
Others
- Next meeting: 6/19.