Original Article by Dr. Robert C. Youngquist, Kennedy Space Center, NASA
Republished with permission

The wavefront measurement system is composed of a six-inch aperture phase shifting interferometer on a vibration isolation optical table with a 2D translation system for scanning large windows. This allows the optical path length to be measured across large spaceflight windows as well as individual panes.

In response to the revised requirement levied onto the Multi-Purpose Crew Vehicle (MPCV) Program to verify that uninstalled flight window assemblies have minimal wavefront variation, Kennedy Space Center's (KSC) Applied Physics Laboratory partnered with the NASA Engineering & Safety Center (NESC) in the development of a wavefront measurement capability at KSC, in close proximity to the MPCV crew module assembly site. The measurement required the construction of an optical interferometer-based wavefront measurement system consisting of an off-the-shelf ZYGO Verifire™ interferometer and a custom scanning system. Training, testing, analysis, and an engineering assessment were required to ensure adequate system operation and that the deliverables provided could allow certification of window assemblies.

The system utilizes a ZYGO phase shifting interferometer to provide optical path length measurements through an individual window pane or through a fully stacked window assembly. Variations in the window's optical path length lead to wavefront perturbations and can cause images seen through the window to be distorted. The revised NASA requirement on spacecraft windows sets maximum allowed values for the wavefront perturbation, but other organizations, such as the Department of Defense, place maximum allowable values on the window's distortion, a window attribute that can be difficult to quantify using ASTM or ISO methodologies. One of the breakthroughs of this work was the realization that the distortion of a window is easily calculated from the optical path length of the window, allowing phase shifting interferometry to replace some of the older less precise distortion measurement approaches (see references).

After establishing the window wavefront measurement system for MPCV, the International Space Station (ISS) Program requested that it be used to help evaluate new scratch panes to cover the inside of windows on the ISS. The successful operation of the system in that evaluation has led to further ISS requests for window/material evaluation, including a request to perform modulation transfer function (MTF) measurements. MTF evaluation is a common optical approach for determining the imaging resolution capability of an optical system. However, measuring the MTF of a window has previously required measuring the MTF of a camera system with and without the window and comparing the results. Using software already programmed into the ZYGO phase shifting interferometer, MTF measurements of just the window can be obtained from the optical path length data, greatly simplifying the measurement of this important parameter.

For more information, contact:
Dr. Robert Youngquist, Kennedy Space Center (robert.c.youngquist@nasa.gov)

[1] Youngquist, R. C.; Skow, M.; and Nurge, M. A.: Optical Distortion Evaluation in Large Area Windows Using Interferometry, 14th International Symposium on Nondestructive Characterization of Materials, Marina del Rey, CA, June 2015, published on-line in NDT.net Vol. 20, No. 9 September 2015.
[2] Youngquist, R. C.; Skow, M.; and Nurge, M. A.: A Comparison of Three Methods for Measuring Distortion in Optical Windows, NASA TM 2015-218822.

ZYGO gratefully acknowledges NASA for granting permission to republish this article and related technical papers. You can access the original article here: "Measuring Window Flatness using Optical Interferometry"

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