| Size: 8281 Comment:  | Size: 8268 Comment:  | 
| Deletions are marked like this. | Additions are marked like this. | 
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| * Geophysics Interferometer (GIF/GI): ''Baseline interferometer along KAGRA, and Arrangement of sensors and benchmarks''<<BR>> | * Geophysics Interferometer (GIF/GI): ''Baseline interferometer and Arrangement of sensors and benchmarks''<<BR>> | 
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| * The target duty factor of KAGRA is '''80%'''. Breakdown of the time loss is shown [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=***|here]]. | * The target duty factor of KAGRA is '''80%'''. Breakdown of the time loss is shown [[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=932|here]]. | 
KAGRA Interface Control
Contents
2. Table of the interface items between subsystems
3. Working groups for important interface issues
6. Duty factor
7. Reference
1. Scope of each subsystem
- Tunnel (TUN/TU): Tunnel design, Underground lab area, Access tunnel, and Safety 
 
- Facility (FCL/FA): TBD 
 
- Vacuum (VAC/VA): Two beam tubes, Chambers, Baffles, Beam targets, Layout, and Pumps 
 
- Cryogenic (CRY/CR): Cryostat, Shield, Cryo duct, Cryo-cooler; Cryo-suspension, and Heat link 
 
- Vibration Isolation (VIS/VI): Four Type-A systems, Seven Type-B systems, and Several Type-C systems 
 
- Mirror (MIR/MI): 23kg Sapphire mirrors, Silica BS, Small Silica mirrors for PRC, SRC, MC, OMC 
 
- Laser (LAS/LA): 180W laser, 10-50W laser for iKAGRA, Laser control system, and Optics for lasers 
 
- Main Interferometer (MIF/IF): MIF design (length, RoC, layout), LSC, ASC, Lock acquisition, and Commissioning 
 
- Input/Output Optics (IOO/IO): Input optics between laser and PRM, and Output optics including OMMT and OMC 
 
- Auxiliary Optics (AOS/AO): All the optical systems that are not included in MIF or IOO 
 
- Analog Electronics (AEL/EL): TBD 
 
- Digital (DGS/DG): Real-time control, Data acquisition, IFO tuning, Automatic operation, and Information collection 
 
- Data Analysis (DAS/DA): Management of observation data 
 
- Geophysics Interferometer (GIF/GI): Baseline interferometer and Arrangement of sensors and benchmarks 
 
| Allocation of items to each subsystem is here. | 
2. Table of the interface items between subsystems
| 
 | TU | FA | VA | CR | VI | MI | LA | IF | IO | AO | EL | DG | DA | GI | 
| TU | -- | |||||||||||||
| FA | -- | |||||||||||||
| VA | -- | |||||||||||||
| CR | -- | |||||||||||||
| VI | -- | |||||||||||||
| MI | -- | |||||||||||||
| LA | -- | |||||||||||||
| IF | -- | |||||||||||||
| IO | -- | |||||||||||||
| AO | -- | |||||||||||||
| EL | -- | |||||||||||||
| DG | -- | |||||||||||||
| DA | -- | |||||||||||||
| GI | -- | 
 
3. Working groups for important interface issues
- Layout (VAC,MIF,AOS,IOO, etc.) 
- Cabling (VIS,CRY, etc.) 
- Interlock (MIF,IOO,LAS, etc.) 
- Detector diagnostics (MIF,DAS, etc.) 
4. Parameter list
- Parameter list is here. 
5. Requirements and tolerance
- Requirements are given in the parameter list. Each parameter must be not so far from the required value as to deteriorate the sensitivity by less than 1%. 
- Tolerance is given for some of the parameters by calculating the robustness of the sensitivity. See here. 
6. Duty factor
- The target duty factor of KAGRA is 80%. Breakdown of the time loss is shown here. 
