Picometer stable scan mechanism for gravitational wave detection in space: LISA PAAM

J. A. C. M. Pijnenburg; N. Rijnveld

doi:10.1117/12.2309235

20 November 2017 Picometer stable scan mechanism for gravitational wave detection in space: LISA PAAM

J. A. C. M. Pijnenburg, N. Rijnveld

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Proceedings Volume 10565, International Conference on Space Optics — ICSO 2010; 105652Z (2017) https://doi.org/10.1117/12.2309235
Event: International Conference on Space Optics—ICSO 2010, 2010, Rhodes Island, Greece

Abstract

Detection and observation of gravitational waves requires extreme stability in the frequency range 0.03 mHz to 1 Hz. The Laser Interferometer Space Antenna (LISA) mission will attain this by creating a giant interferometer in space, based on free floating proof masses in three spacecrafts. Due to orbit evolution and time delay in the interferometer arms, the direction of transmitted light changes. To solve this problem, a picometer stable Point-Ahead Angle Mechanism (PAAM) was designed, realized and successfully tested. The PAAM concept is based on a rotatable mirror. The critical requirements are the contribution to the optical path length (less than 1.4 pm / rt Hz) and the angular jitter (less than 8 nrad / rt Hz). Extreme dimensional stability is achieved by manufacturing a monolithical Haberland hinge mechanism out of Ti₆Al₄V, through high precision wire erosion. Extreme thermal stability is realized by placing the thermal center on the surface of the mirror. Because of piezo actuator noise and leakage, the PAAM has to be controlled in closed-loop. To meet the requirements in the low frequencies, an active target capacitance-to-digital converter is used. Interferometric measurements with a triangular resonant cavity in vacuum proved that the PAAM meets the requirements.

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J. A. C. M. Pijnenburg and N. Rijnveld "Picometer stable scan mechanism for gravitational wave detection in space: LISA PAAM", Proc. SPIE 10565, International Conference on Space Optics — ICSO 2010, 105652Z (20 November 2017); https://doi.org/10.1117/12.2309235

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