LIGO-G050485-00-R Inverted pendulum studies for seismic attenuation Ilaria Taurasi University of Sannio at Benevento, Italy September 20, 2005 Supervisor.

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Presentation transcript:

LIGO-G R Inverted pendulum studies for seismic attenuation Ilaria Taurasi University of Sannio at Benevento, Italy September 20, 2005 Supervisor Riccardo De Salvo Mentor Calum Torrie

LIGO-G R Introduction Seismic noise is one of the most important noise sources that will affect the detector at low frequencies There is the necessity to design an adequate isolation system An inverted pendulum (IP) is implemented to provide attenuation at frequencies extending down to the micro- seismic peak and to realize a mean to position the entire system without requiring large force

LIGO-G R Inverted Pendulum IP is a horizontal pre- isolation stage with ultra-low resonant frequency, typically 30 mHz Small flex joint Main flex joint

LIGO-G R IP in ANSYS: First step Draw in each detail the individual legs of the inverted pendulum in Solid Solid Works ©

LIGO-G R Second step Import the pendulum in Ansys © First operation: meshing Ansys is ageneral purpose finite element modeling The body can be sub-divided up into small discrete regions known as finite elements Calculate stress and strain propagated through the mesh

LIGO-G R Second step Import the pendulum in Ansys © Second operation: convergence test to check that the model finds stable resonance frequencies NO problem of convergence Convergence test for the first 6 frequencies up to 22 MHz

LIGO-G R Third step Assembly 4 legs into in Solid Works

LIGO-G R Fourth Step Solve model and analyze first 20 modes in ANSYS

LIGO-G R Table normal modes Third frequency: transversal motion f = Hz Second frequency: longitudinal motion f = Hz First frequency: yaw motion f = Hz

LIGO-G R Table normal modes (2) Frequency vs load: I changed the mass of the table on the top of the 4 legs Longitudinal and trasversal frequencies are identical Zero frequency point is the same for all 3 main modes

LIGO-G R Validation Ansys results are fully validated by the measurement results

LIGO-G R Rigid leg resonances Small flex joint: S- stress Main flex joint: C- stress Eight degenerate resonances: each leg has 2 resonances

LIGO-G R Rigid leg resonances Eight degenerate resonances: each leg has 2 resonances Leg is not stressed

LIGO-G R Rigid leg resonances (2) Resonance frequency with counterweight Resonance frequency without counterweight ~110.6 Hz ~122 Hz ~178.3 Hz ~235.3 Hz Diameter of small flex joint: 1.5 mm Diameter of small flex joint: 3 mm Mass of counter weight: Kg

LIGO-G R Rigid leg resonances (2) Resonance frequency with counterweight Resonance frequency without counterweight ~110.6 Hz ~122 Hz ~178.3 Hz ~235.3 Hz Diameter of small flex joint: 1.5 mm Diameter of small flex joint: 3 mm Mass of counter weight: Kg Measurement of prototype: 103 Hz 20% of discrepance between measurement and Ansys results, within tube tolerancies

LIGO-G R Rigid leg resonances (3) Resonance frequency with counterweight Resonance frequency without counterweight ~110.6 Hz ~122 Hz ~178.3 Hz ~235.3 Hz Diameter of small flex joint: 1.5 mm Diameter of small flex joint: 3 mm Mass of counter weight: Kg Ansys shows that counter weight doesn’t reduce significantly the resonance, that are dangerous. They can be damped

LIGO-G R Eddy current dampers Solution: Eddy current dampers Before installation t = 4.3 s After installation t = 35 ms Measured and succesfully damped in a prototype without counter weight

LIGO-G R Banana leg resonances Each IP leg has 2 banana resonances Small flex joint: S- stress Main flex joint: S- stress

LIGO-G R Banana resonances (2) Resonance frequency with counterweight Resonance frequency without counterweight ~210.6 Hz ~415 Hz ~253.3 Hz ~424 Hz Diameter of small flex joint: 1.5 mm Diameter of small flex joint: 3 mm Mass of counter weight: Kg

LIGO-G R Banana resonances (3) Higher frequencies Resonances move the head of the leg The damper will be even more effective

LIGO-G R Spring box resonances Fourth frequency: pitch motion f = 38 Hz Fifth frequency: roll motion f = 45 Hz Sixth frequency: up-down motion f = 38 Hz

LIGO-G R Leg magnetic dampers may be still effective Complementary resonant dampers may be required Spring box resonances(2) Spring box effective mass 320 Kg

LIGO-G R IP Transfer Function Excitation Output: monitor resulting movement

LIGO-G R IP Transfer Function The aim is to determine the counter weight that neutralize the percussion point effect of the legs Prototype measurements indicate that the transfer function saturates at 80 dB without counterweight A proper counter weight should allow 100 dB attenuation

LIGO-G R Future Find a counter weight which allow an attenuation of 100 dB Export TF to Sym Mechanic model

LIGO-G R Acknowledgments Riccardo De Salvo and Calum Torrie for their help, encouragments and patience Juri Agresti and Virginio Sannibale for answering my quick questions Innocenzo Pinto for the opportunity he gave me

LIGO-G R And… The sun of California…