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Size: 360
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← Revision 6 as of 2018-07-24 11:38:44 ⇥
Size: 1430
Comment:
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| Deletions are marked like this. | Additions are marked like this. |
| Line 5: | Line 5: |
| * Attendance: Miyakawa, Izumi, * eZuce: |
* Attendance: Miyakawa, Izumi, Ohishi * eZuce: Yamamoto, Nakano, Shoda, Suzuki |
| Line 9: | Line 9: |
| == LAS (Nakano) == * EOM and FI are being tested. * EOM: TF and modulation index were measured. * Fiber isolate reached and is being tested. * Installation to KAGRA started. == PSL, IOO == * MZ alignment is being proceeded, and MC has been already locked with single arm of MZ. * Mode matching ratio is still bad but it will be fixed soon. == ISS == * ISS loop locked again. OLG or RIM was measured, and they are being analyzed. == IMMT2 (Ohishi) == * On 7/9, we started take IMMT out from the chamber. * All the replacement of magnetized screws is done by the end of last week. * Mirror position (distance between mirror and coile) was shifted a ~mm, probably caused by tilt of optical. * TF will be measured soon. == ACC noise == * Old circuits are still used in TAMA era, and all the noise floor are high. |
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| Line 12: | Line 37: |
| == Geophone == | |
| Line 13: | Line 39: |
| == LAS == | * To fix BS GeoPhone, we should open the chamber. * TMS GeoPhone looks fine, but some strange coupling can be seen in the TF measurement. * Feedback bandwidth is limited ~10Hz. |
| Line 15: | Line 43: |
| == PSL == | |
| Line 27: | Line 54: |
| * Next meeting: 7/24. | * Next meeting: 7/31. |
Minute of KAGRA commissioning meeting
- Date: 2018/7/24 11AM~12PM
- Attendance: Miyakawa, Izumi, Ohishi
- eZuce: Yamamoto, Nakano, Shoda, Suzuki
LAS (Nakano)
- EOM and FI are being tested.
- EOM: TF and modulation index were measured.
- Fiber isolate reached and is being tested.
- Installation to KAGRA started.
PSL, IOO
- MZ alignment is being proceeded, and MC has been already locked with single arm of MZ.
- Mode matching ratio is still bad but it will be fixed soon.
ISS
- ISS loop locked again. OLG or RIM was measured, and they are being analyzed.
IMMT2 (Ohishi)
- On 7/9, we started take IMMT out from the chamber.
- All the replacement of magnetized screws is done by the end of last week.
- Mirror position (distance between mirror and coile) was shifted a ~mm, probably caused by tilt of optical.
- TF will be measured soon.
ACC noise
- Old circuits are still used in TAMA era, and all the noise floor are high.
ETMX (Miyamoto)
Geophone
To fix BS GeoPhone, we should open the chamber.
TMS GeoPhone looks fine, but some strange coupling can be seen in the TF measurement.
- Feedback bandwidth is limited ~10Hz.
DGS
- DAC is almost out of stock. We should think to start using old DAC used in CLIO.
rack cleaning
Others
- Next meeting: 7/31.