Paper
22 June 2000 Microprecision interferometer: pointing system solutions for on-orbit disturbance environment
Frank G. Dekens, Gregory W. Neat
Author Affiliations +
Abstract
The Space Interferometer Mission (SIM) is required to point each arm of its science interferometer to better than 30 milli-arcseconds (mas) RMS residual jitter using a 0.01 Hz bandwidth optical sensor on the star. We address the residual pointing error due to the spinning spacecraft reaction wheel assemblies which emit disturbances from 2 Hz to 1 kHz. The vibration attenuation strategy for this 'blind' pointing problem is to isolate each reaction wheel assembly with a vibration isolation system and to possibly augment the low bandwidth closed loop system with an internal high bandwidth sensor. Central to estimating the high frequency pointing error is the Micro-Precision Interferometer (MPI) testbed which is a softly suspended hardware model of a spaceborne optical interferometer and is dimensionally representative of SIM. Using the testbed and a transfer function-based performance prediction algorithm, we show that the 30 mas requirement is missed by a factor of six when only employing a six-axis active vibration isolator made by TRW. In preparation for augmenting the vibration attenuation strategy, we also show that the primary contributor to the tip-tilt jitter error is the first optic in the interferometer's optical train.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Frank G. Dekens and Gregory W. Neat "Microprecision interferometer: pointing system solutions for on-orbit disturbance environment", Proc. SPIE 3985, Smart Structures and Materials 2000: Smart Structures and Integrated Systems, (22 June 2000); https://doi.org/10.1117/12.388841
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Cited by 1 scholarly publication.
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KEYWORDS
Optical isolators

Interferometers

Sensors

Stars

Signal attenuation

Vibration isolation

Electronics

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