Optical characterization of parasitic motion in a long-stroke shaker

We present an optical scheme to simultaneously characterize the cross-axis and rotational parasitic motions of a long-stroke shaker. By leveraging the geometric properties of a corner cube retroreflector mounted on the shaker load table, we independently sample pitch, yaw, and horizontal and vertical displacements with sampling rates above 10 kHz. We have applied our optical apparatus to a 400-mm-stroke shaker operated from 0.1 Hz to 100 Hz and present two forms of analysis: (A) Frequency-domain data for the four measured parasitic degrees of freedom, with the resulting implications for accelerometer calibration uncertainties, and (B) extracted trajectories of the shaker table, allowing visualization of the bowed linear guide below 0.5 Hz and higher harmonics and hysteresis above 10 Hz. Our findings demonstrate our optical measurement scheme to be an effective tool for the characterization of parasitic motion for long-stroke shakers. As an example, we determine the "gravity error" in accelerometer calibration with our shaker to be (1.3 ± 0.1) % times the acceleration amplitude at 0.1 Hz, providing a correction to reduce uncertainty from this effect by an order of magnitude.

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Publication Details

Journal
Metrologia
Published
2024-11-11
DOI
https://doi.org/10.1088/1681-7575/ad90e6
Primary Topic
Astronomical Observations and Instrumentation
Type
article
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article

Optical characterization of parasitic motion in a long-stroke shaker

Richard A. Allen, Jared H. Strait
Metrologia
Astronomical Observations and Instrumentation
article

Optical characterization of parasitic motion in a long-stroke shaker

Richard A. Allen, Jared H. Strait
article en

Abstract

We present an optical scheme to simultaneously characterize the cross-axis and rotational parasitic motions of a long-stroke shaker. By leveraging the geometric properties of a corner cube retroreflector mounted on the shaker load table, we independently sample pitch, yaw, and horizontal and vertical displacements with sampling rates above 10 kHz. We have applied our optical apparatus to a 400-mm-stroke shaker operated from 0.1 Hz to 100 Hz and present two forms of analysis: (A) Frequency-domain data for the four measured parasitic degrees of freedom, with the resulting implications for accelerometer calibration uncertainties, and (B) extracted trajectories of the shaker table, allowing visualization of the bowed linear guide below 0.5 Hz and higher harmonics and hysteresis above 10 Hz. Our findings demonstrate our optical measurement scheme to be an effective tool for the characterization of parasitic motion for long-stroke shakers. As an example, we determine the "gravity error" in accelerometer calibration with our shaker to be (1.3 ± 0.1) % times the acceleration amplitude at 0.1 Hz, providing a correction to reduce uncertainty from this effect by an order of magnitude.

MetrologiaVol. 62(1)
National Institute of Standards and Technology (US), Physical Measurement Laboratory (US)
Openalex Percentile: Top 78%
Astronomical Observations and Instrumentation
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Optical characterization of parasitic motion in a long-stroke shaker — Richard A. Allen, Jared H. Strait · Metrologia (2024) | TGRS Research Map | TGRS