KAGRA MIF Meeting
Date: 2012/9/25 13:30 - 15:00
Location: EVO
Participants: Tatsumi, Aso, Ando, Akutsu, Takahashi, Yamamoto, Miyoki, Shibata, Izumi, Miyakawa
Decided
- The first version of the FSS model will be built based on the servo topology of Telada-san.
- We will discuss how to proceed with the OMC development on the KAGRA side at the next meeting. (Somiya-san will make a presentation)
We want to buy alarge beam profiler.
Discussions
Multiple loop servo and cascade servo are compared for the FSS. http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/ShowDocument?docid=1286
- For the FSS modeling, the radiation pressure noise should be included in the CARM noise budget.
Next Meeting
2012/10/9 (Tue) 13:30 -14:30
Agenda: Status reports, Discussion on OMC.