Each LISA PathFinder test mass (TM) will be sensitive to forces along all its 6 Degrees of Freedom (DoFs). Extensive ground testing is required in order to evaluate the influence of cross-talks from the read-out and actuator channels. In the INFN laboratory of Firenze we have developed a facility for a good representation of the free fall conditions of the TM on flight. A hollow replica of a TM hanging from a double torsion pendulum can move inside a Gravitational Reference Sensor (GRS) with quasi free fall condition on two Dofs, in the frequency band (0.1 ÷ 100)mHz. On both DoFs, the target residual accelerations (yet to be achieved) at the low end frequency range are ≤ 3 10−13ms−2, limited by the thermal noise of the fibres. At higher frequencies, the sensitivity is limited by the readout noise of the readout, a replica of the flight electronics. After a long commissioning, we are now in operating conditions, and can carry out a series of experiments to better qualify the interaction between TM and GRS. In this paper we will show some significant qualification measurements and a first scientific measurements, i.e. the measurement and compensation of the DC bias in the GRS using two independent channels, as well as a measurement of the residual acceleration of the translational DoF, with the feedback loop closed on the rotational one, and viceversa.

Marconi, L., Stanga, R., Bassan, M., De Marchi, F., Pucacco, G., Visco, M., et al. (2013). PETER: A Hardware Simulator for the Test Mass-GRS System of LISA Pathfinder. In 9th LISA Symposium, Paris ASP Conference Series, Vol. 467 G. Auger, P. Bine ́truy and E. Plagnol, eds. ⃝c 2013 Astronomical Society of the Pacific (pp.303-307). San Francisco : Astronomical Society of the Pacific.

PETER: A Hardware Simulator for the Test Mass-GRS System of LISA Pathfinder

BASSAN, MASSIMO;PUCACCO, GIUSEPPE;
2013-01-01

Abstract

Each LISA PathFinder test mass (TM) will be sensitive to forces along all its 6 Degrees of Freedom (DoFs). Extensive ground testing is required in order to evaluate the influence of cross-talks from the read-out and actuator channels. In the INFN laboratory of Firenze we have developed a facility for a good representation of the free fall conditions of the TM on flight. A hollow replica of a TM hanging from a double torsion pendulum can move inside a Gravitational Reference Sensor (GRS) with quasi free fall condition on two Dofs, in the frequency band (0.1 ÷ 100)mHz. On both DoFs, the target residual accelerations (yet to be achieved) at the low end frequency range are ≤ 3 10−13ms−2, limited by the thermal noise of the fibres. At higher frequencies, the sensitivity is limited by the readout noise of the readout, a replica of the flight electronics. After a long commissioning, we are now in operating conditions, and can carry out a series of experiments to better qualify the interaction between TM and GRS. In this paper we will show some significant qualification measurements and a first scientific measurements, i.e. the measurement and compensation of the DC bias in the GRS using two independent channels, as well as a measurement of the residual acceleration of the translational DoF, with the feedback loop closed on the rotational one, and viceversa.
9th LISA Symposium
Paris, France
2012
9th
APC Paris
Rilevanza internazionale
contributo
23-mag-2012
2013
Settore FIS/01 - FISICA SPERIMENTALE
English
Pendulum; torsion; small forces; inertial motion; LISA;
Intervento a convegno
Marconi, L., Stanga, R., Bassan, M., De Marchi, F., Pucacco, G., Visco, M., et al. (2013). PETER: A Hardware Simulator for the Test Mass-GRS System of LISA Pathfinder. In 9th LISA Symposium, Paris ASP Conference Series, Vol. 467 G. Auger, P. Bine ́truy and E. Plagnol, eds. ⃝c 2013 Astronomical Society of the Pacific (pp.303-307). San Francisco : Astronomical Society of the Pacific.
Marconi, L; Stanga, R; Bassan, M; De Marchi, F; Pucacco, G; Visco, M; Di Fiore, L; De Rosa, R; Garufi, F
File in questo prodotto:
File Dimensione Formato  
13_Lisa9_PETER.pdf

accesso aperto

Dimensione 1.05 MB
Formato Adobe PDF
1.05 MB Adobe PDF Visualizza/Apri

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/102673
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus ND
  • ???jsp.display-item.citation.isi??? 0
social impact