
ustt-4
The first version of the High-Speed Interferometer was used to measure Webb mirror segment responses to very small dynamic stimulus (left). The resulting data (right) showed reliable identification of aberrations (depicted as Zernike content) on picometer scales because of the disturbance.
Image Credit: NASA GSFC
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https://science.nasa.gov/image-detail/ustt-4/
Image CreditNASA GSFC
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