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| Figure
4: Dual-axis implementation using single laser source
and remote detectors. |
measurement, which in this example
are the X and Y axes. These beams are steered to the interferometer
optics and plane mirrors prior to their measurement at a remote
detector. The detector electronics are located in the same
housing as the interferometer optics, providing a compact
solution. Some existing laser interferometer solutions require
a signal processing board that interfaces directly to the
motion controller. In many cases this is done so as to provide
a parallel word directly to the motion controller, which allows
for high data rates. While this may be required in high speed,
high resolution applications, this solution has the distinct
disadvantage of making the laser interferometer a proprietary,
closed-architecture solution. Interfacing to both the interferometer
board and motion controller requires an in-depth knowledge
of both devices that is often impractical for most users.
Advances in motion controller
technology have nearly made this approach obsolete. Aerotech
LZR series laser interferometer output signals are standard
A-quad-B, and are electrically identical to the output of
a traditional incremental encoder. To the motion controller,
the interferometer appears to be a standard feedback device,
simplifying system implementation. Aerotech's UNIDEX®
family of stand-alone and PC-bus-based controllers employ
high-speed devices, resulting in serial data rates as high
as 32 MHz. For a system with a resolution of 6 nm, that
results in a speed of nearly 200 mm/s. While Aerotech also
manufactures a laser interferometer signal processing board
for high-speed applications, the need for this approach
has been greatly minimized and often the much simpler serial
approach proves to be the optimal solution.
While the position feedback may be straightforward
to process, there are other important considerations that
must be made when implementing a laser interferometer-based
system. Issues such as home-marker implementation, losses
of feedback signal, and error-source reduction require unique
solutions in an interferometer-based system.
Since the interferometer is strictly
an incremental device, there is no way to establish an accurate
home reference. Traditional home devices such as LVDTs and
optical |
proximity
switches are only adequate in establishing an approximate
home. For accurate wafer measurements, it is often necessary
to acquire a fiducial directly from the wafer to establish
a sufficiently accurate and repeatable home. Once the mark
is acquired, the motion controller counters can be reset to
zero (software homed) and the processing continues.
When implementing a laser interferometer
as a feedback device it is absolutely necessary for the
interferometer to provide a "beam blocked" signal.
Unlike a linear encoder that places the read head in close
proximity to the encoder glass, it is easy to block the
feedback signal (in this case the laser beam) in an interferometer
system. This condition requires the motion controller to
immediately generate a fault condition and disable the axes.
Aerotech's UNIDEX controller and LZR series interferometer
implement all fault handling automatically, greatly simplyfying
system operation.
Minimize
Potential Error Sources The
same requirements that necessitate the use of a laser interferometer
_ high resolution and high accuracy _ require that system-wide
error sources be minimized. While it is inherently more
accurate than alternate feedback schemes, without proper
understanding of the error sources, it will be no more effective
than a low-cost linear encoder. Environmental conditions,
mechanical design and optical alignment must be considered
in the design/implementation of any high-accuracy laser
interferometer based motion system.
Environmental
Errors The
wavelength of light emitted by a He-Ne laser is by definition
equal to 632.99072 nm in a vacuum. Interferometer accuracy
in a vacuum is accurate to ±0.1 ppm. However, most applications
require operation of the system in atmospheric conditions,
so this accuracy degrades. The index of refraction of air
effectively changes the frequency of the laser light which
appears as a path length difference. Fortunately, the effects
of temperature, pressure and humidity as they affect the
wavelength of light are well known and are related by Edlen's
equation. As a result, the LZR series interferometer systems
incorporate a "weather station" that samples the
environmental conditions. These signals are digitized and
processed to create a wavelength scale number that is used
to generate a correction factor. An environmentally corrected
system will have an accuracy ±1.5 ppm or better. The final
accuracy is largely a function of the stability of the environmental
conditions.
The most effective, and incidentally
also the most expensive, means of compensating for changes
in the refractive index of
Environmental
Effects on Accuracy
Temperature: 1 ppm / 1°C
Pressure: 1 ppm / 2.5 mm Hg
Humidity: 1 ppm / 85% change |