'Force noise' diaporamas de présentation

Free-fall and the observation of low frequency gravitational waves with LISA Bill Weber

605 views • 43 slides

System Identification for X-dynamics

System Identification for X-dynamics. Data Analysis 4. LTP dynamics. 2 measured and controlled Degrees of Freedom within Measurement Bandwidth 3 Actuators (1 redundant) 4 Signals (2 redundant) A 2 Input-2 Output system with redundant sensing and actuation 4 Measurable transfer functions

454 views • 33 slides

403 views • 23 slides

LISA Pathfinder Preventivi 2013 Gruppo di Trento

LISA Pathfinder Preventivi 2013 Gruppo di Trento. Principal investigator della missione LISA Pathfinder Testing a terra del sensore gravitazionale con pendoli di torsione Testing a terra della fase di rilascio in volo della test mass. Scopo di LISA PAthfinder. Sensitivity of LISA.

341 views • 20 slides

Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO)

Deci-hertz Interferometer Gravitational Wave Observatory (DECIGO). 7th Gravitational Wave Data Analysis Workshop December 17, 2002 @ International Institute for Advanced Studies, Japan Seiji Kawamura National Astronomical Observatory of Japan. Contents. Introduction What is DECIGO ?

346 views • 16 slides

Bridging the Gap between Terrestrial Detectors and LISA

Bridging the Gap between Terrestrial Detectors and LISA. Elba 2002 May 24, 2002 Seiji Kawamura National Astronomical Observatory of Japan. Contents. Introduction What is DECIGO ? Science obtained by DECIGO Sensitivity of DECIGO Current Status of DECIGO Summary. 10 -18. 10 -20.

300 views • 15 slides