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Intensity Stabilization Servo Plan Yuta Michimura Department of Physics, University of Tokyo November 23, 2015.

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Presentation on theme: "Intensity Stabilization Servo Plan Yuta Michimura Department of Physics, University of Tokyo November 23, 2015."— Presentation transcript:

1 Intensity Stabilization Servo Plan Yuta Michimura Department of Physics, University of Tokyo November 23, 2015

2 Start discussion on the sevo topology of the bKAGRA intensity stabilization servo (ISS) Start from following the aLIGO design Related documents: - Optics Express 20, 10617 (2012) (aLIGO ISS/FSS paper) - Optics Letters 34, 2912 (2009) (aLIGO ISS paper) - LIGO-T0900649 (aLIGO PSL Final Design) - JGW-G1503293 (bKAGRA laser development status) - JGW-T1200913 (requirement from MIF; Fig. 4.8, 4.9)Optics Express 20, 10617 (2012)Optics Letters 34, 2912 (2009)LIGO-T0900649JGW-G1503293JGW-T1200913 Scope 2

3 see related documents for the real spectra Requirement 3

4 aLIGO Topology 4 NPRO FI AOM FI PMC Finesse: 130 Round trip length: 2.02 m high power oscillator medium power amplifier IMC Finesse: 475 Round trip length: 32.9 m

5 bKAGRA Topology Plan 5 NPRO AOM FI solid state amplifier fiber amplifier IMC Finesse: 500 Round trip length: 53.3 m PMC Finesse: 155 ? Round trip length: 1.95 m ? PMC design not fixed yet We can implement noise eater servo (pick off right after NPRO and feedback to NPRO) Any feedback to the current to the fiber amps and/or the solid state amps?


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