= 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 a[[http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/private/DocDB/ShowDocument?docid=872|large 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.