SCI from Apre Measures Optical Domes Faster and More Accurately
Dome optics are the last component in a growing number of imaging and guidance applications. Domes protect the imaging optics from the surrounding environment without degrading optical performance. Therefore the dome’s transmitted wavefront quality is important to control since it directly influences the final image quality. Dome applications include:
- Underwater cameras
- Submersibles for robotic and manned exploration
- Unmanned aerial vehicles
- Remotely piloted vehicles
- Space applications
- Missile guidance systems
- Security systems
Manufacturing Parameters to Control
The transmitted wavefront is degraded by several parameters which must be controlled during manufacture:
- Individual surface irregularity
- Front-to-back surface thickness variation (TTV)
- Front-to-back surface decenter (X-Y)
- Center of radii shift in Z
- Transmitted wavefront
Typical Metrology Methods
Laser Fizeau Interferometer
A laser Fizeau interferometer appears as an obvious choice to measure domes. Transmitted wavefront and surface irregularity are typical parameters measured with a Fizeau interferometer. The long coherence of the laser Fizeau frustrates these measurements as both surfaces mutually interfere with the reference sphere as well as the front and back surfaces creating three interference patterns overlaid making accurate surface measurement impossible. [Optically a dome is equivalent to a flat parallel plate and encounter the same measurement difficulties] Tilt can be introduced in an attempt to visually separate the surfaces, or one surface is painted black to lower the fringe contrast from that surface, but in the end the measurements are not reliable.
5-Axis CMM with Point Probe or Depth Probe
5-Axis Coordinate Measuring Machines (CMM) swings a probe around the dome, measuring as it moves (Figure 1).
Figure 1: 5 Axis CMM Geometry [Vahidi Pashaki, Pooyan & Pouya, Milad. (2016). Volumetric Error Compensation in Five-Axis CNC Machining Center through Kinematics Modeling of Geometric Error. Advances in Science and Technology Research Journal. 10. 207-217. 10.12913/22998624/62921.]
If the CMM has ample range in the B Axis it can measure the full dome hemisphere. Two types of probes for surface sensing are used: A surface probe or a depth probe. The surface probe only measures one surface at a time and thus does not measure TTV or decenter. The depth probe measures both surfaces simultaneously, providing measurement of all parameters except transmitted wavefront.
The measurement reference or metrology frame is created by controlling the CMM’s motions. Motion control of a point in space (the probe) is technically difficult, especially when 5 non-orthogonal axes are concerned. Therefore the measurement accuracy is degraded compared to a Fizeau interferometer that has a fixed reference (metrology frame).
The 5-Axis CMM is slow to measure (minutes to hours depending on the resolution of data to acquire), typically expensive if state-of-the-art measurement uncertainty is achieved (~$750,000 [ USD]) and even then does not approach the optical metrology accuracy required.
SCI Fizeau: Fixed Metrology Frame all Parameters Measured
The Fizeau configuration is optimal considering accuracy. With Spectrally Controlled Interferometry (SCI) from Äpre, the coherence is controlled enabling the measurement of all parameters (Figure 2).
Figure 2: Dome setup in Fizeau measurement configuration
Just like for a plane parallel plate, the SCI coherence can be adjusted to create fringes on each surface individually and between the front and back surfaces. In this way an accurate, fast method exists to measure all dome parameters. The following interference cavities provide the required results (Figure 3):
- Surface Irregularity 1: Fizeau Sphere Reference to Surface 1 (PVr & RMS: Tilt & Power removed)
- Surface Irregularity 2: Fizeau Sphere Reference to Surface 2 (PVr & RMS: Tilt & Power removed)
- TTV: Surface 1 to 2 (PVr result)
- Decenter (X & Y): Surface 1 to 2 (Tilt result)
- Center of radii shift in Z: Surface 1 to 2 (Power result)
- Transmitted Wavefront: Fizeau Sphere Reference to Additional Reference Sphere (PVr & RMS: Tilt & Power removed)
Figure 3: Typical SCI Dome results without the multiple interference which frustrates measurement
The region of measurement is determined by the Fizeau sphere f#. A faster (lower number) sphere provides more coverage. To cover a full hemisphere an f# of 0.5 is required, but this does not exist. Tilting the sphere to the edges enables coverage of the full hemisphere over a series of measurements.