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PTB >> Optical Scanning Using Fast Steering Mirrors Targeting, surveillance, and free space laser-based communication systems for aircraft and spacecraft require systems for line of sight (LOS) stabilization. These LOS systems are required to compensate for the influences of vehicle motion, vibration, and drift so that images are not blurred. Such systems are often required to simultaneously manage both large angle, low frequency, and small angle, high frequency corrections. Fast steering mirrors (FSMs), broadly defined as a glass or metal mirror
mounted to a flexure support system that may be moved independent of the
natural frequency of the spring/mass system to direct a laser beam or
other light source, can be used as a complimentary LOS correction device
to a system that also tilts a large mirror or the entire optical payload.
In this event, the accuracy and bandwidth of the larger mechanism can
be significantly degraded and refined LOS corrections are relegated to
the FSM. Thus, the overall performance can be improved and the cost of
bearings, motors, and angle sensors for movement of a large mirror or
the entire optical payload can be reduced. Although it is tempting to make the mirror oversized in thickness and aperture in order to eliminate concerns about meeting the optical requirements, the addition of mass and moments of inertia run counter to the goals for the actuator design and the associated control system. In such cases, a sufficient design for the mirror can be determined by finite element analysis (FEA). Glass or metal mirrors can be used in the FSM design. Glass mirrors are inexpensive and can be very high quality but lack the design versatility of metal mirrors. In many cases mirror materials with an exceptional stiffness/mass ratio, such as beryllium or silicon carbide, can be used. These materials have a specific stiffness (Young’s modulus/density) that is four to six times greater than common optical glass materials, such as BK7 and fused silica, and common structural metals, like aluminum, magnesium, steel, and titanium. In addition to the type of mirror used, its mounting to the flexure support system is extremely critical. Use of a glass mirror typically requires applying an adhesive to the back and/or sides of the mirror for attachment to a metal structure that is then attached to the flexure and actuator system. Dissimilar coefficients of expansion among mirror and support materials can result in mirror figure distortion upon changes in temperature. Also, the use of adhesives often results in dimensional creep and reduction of the natural frequency of the suspended mirror system. On the other hand, metal mirrors are readily designed for direct fastening
(no adhesives) to the flexure and actuator system. The metal mirror may
also be designed with integrally machined flexures, light-weighted to
increase the structural efficiency and other features not attainable with
glass mirrors.
Two flexures are used in Figure 1b inorder to only allow translation
along the axis of the mirror. This type of design can be used to rapidly
modulate an interferometer cavity for FFT waveform analysis. The mirror
depicted in Figure 1c is mounted to a two-axis flexure system with a center
pivot flexure that allows only two axes of tilt adjustment. This design
is ideal for a number of beam stabilization and scanning applications,
including free space laser telecom systems. Spring rate in both the compliant and non-compliant directions must be
considered simultaneously. An ideal FSM flexure system would have the
following attributes: PZTs typically consist of laminated stacks of piezoelectric material encased in a steel cylinder. By application of a modulated high-voltage signal to the PZT, small increments of motion result. When compared to voice coils, PZT actuators can produce tremendous force in a smaller package at much greater frequency response. However, PZTs suffer from very limited range of travel, hysteresis, and they must be mechanically preloaded in compression to prevent delamination and to provide a restorative spring force. A combination of high frequency, high load, and small tilts or translations favors the use of a PZT to actuate the FSM. Large ranges of excursion and low load favor the voice coil actuator. Sample Applications Figure 2: A single axle fast steering mirror In this case the small angular range of motion and extreme stiffness required suggest the use of a small single-axis flexure- mounted mirror. By using a diamond- machined metal mirror, it is possible to integrally machine the flexures into the mirror substrate. The small range of motion and high frequency response favors the selection of a PZT-type linear actuator. The selection of a metal mirror substrate allows the mirror to be hard
mounted directly to the top of the PZT. Peak accelerations exceed 200
g’s. The rotating polygon is mounted on an extremely accurate self-acting
air bearing motor system. The final result is a highly responsive, compact,
and reliable FSM module with a repeatable tilting motion about a virtual
hinge axis defined by two integrally machined pivot flexures.
Since the dynamic response characteristics are not particularly demanding, a sufficient design can be developed without the use of exotic mirror materials, light-weighting of the mirror, or ultrahigh performance actuators. Systematic engineering analysis results in a spring suspension system that remains exceptionally stiff in three axes of translation and one axis of rotation. The remaining two degrees of freedom, reserved for tilt of the mirror surface, are designed to have a very low spring rate and are essentially uncoupled from one another.
The virtual pivot of rotation is maintained as close to the center of the mirror aperture as possible. Two pairs of voice coils, operating in a push/pull manner for each tilt axis, act directly upon the mirror mount and are suspended with the mirror on the flexure system. The voice coil magnets are fixed mounted in the base of the FSM. By maintaining very low, yet highly elastic spring rate in the desired
compliant directions, the energy required to hold the mirror at a given
location for extended periods of time is not excessive. By balancing the
mirror, its mount, and the actuator coils such that the center-of-gravity
of the mirror coincides with the virtual pivot of tilt, the FSM may be
mounted in universal orientations without significant change in mirror
angle relative to reference datums. This article was written by Michael Sweeney, Gerald Rynkowski, Mehrdad Ketabchi, and Robert Crowley of Axsys Technologies Imaging Systems, located in Rochester Hills, Michigan. For questions regarding this article, please contact George Murray at gmurray@axsys.com. Visit Axsys Technologies online at www.axsys.com. |
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