TY - GEN
T1 - Process development for adjustable X-ray mirrors
AU - Tendulkar, Mohit
AU - Liu, Tianning
AU - Kirchner-Hall, Nicole
AU - Bishop, Nathan
AU - Tran, Quyen
AU - Deroo, Casey T.
AU - Cotroneo, Vincenzo
AU - Kradinov, Vladimir
AU - Marquez, Vanessa
AU - Reid, Paul B.
AU - Trolier-Mckinstry, Susan
AU - Jackson, Thomas N.
N1 - Funding Information:
This work was supported by National Aeronautics and Space Administration (NASA) award number 80NSSC19K0234 and NNX17AF66G. Internal funding from the Smithsonian Astrophysical Observatory is also gratefully acknowledged.
Publisher Copyright:
© 2021 SPIE.
PY - 2021
Y1 - 2021
N2 - Thin adjustable X-ray mirrors can correct deformations generated from fabrication, gravity release, mounting stresses, drifting stresses in the reflecting layer(s) and thermal variations while maintaining high angular resolution (< 0.5 arcsecond) and large effective area (< 2 m2) required for future X-ray missions. This work presents fabrication process developments for adjustable mirror segments with actuators for the Lynx X-ray observatory mission concept. Piezoelectric actuator arrays were fabricated on the convex side of precision slumped glass or curved silicon mirror segments using a 1.5 μm thick lead zirconate titanate (PZT) film. A two-layer metal routing scheme with a polymeric insulator was used to independently address 288 actuators on the mirror. The two-layer metal allows narrow kerfs between actuators and increased actuator density. Anisotropic conductive film was used to bond thin flexible copper cables to flat edges of the mirror to interface with external control electronics. This prototype mirror has eight cables with a total of 290 connections to access the array. To reduce the cabling complexity for future mirrors, thin film transistors have been fabricated on the curved mirror to function as access switches. To facilitate this, a mask aligner that allows precision alignment on curved mirror segments was developed and arrays of thin film transistors (TFT) on curved substrates have been tested. TFT and actuator integration on future mirrors will reduce external connections to just two cables with a total of 30 connections. Keywords: Lynx, adjustable optics, X-ray optics, thin film piezoelectric, curved substrate aligner.
AB - Thin adjustable X-ray mirrors can correct deformations generated from fabrication, gravity release, mounting stresses, drifting stresses in the reflecting layer(s) and thermal variations while maintaining high angular resolution (< 0.5 arcsecond) and large effective area (< 2 m2) required for future X-ray missions. This work presents fabrication process developments for adjustable mirror segments with actuators for the Lynx X-ray observatory mission concept. Piezoelectric actuator arrays were fabricated on the convex side of precision slumped glass or curved silicon mirror segments using a 1.5 μm thick lead zirconate titanate (PZT) film. A two-layer metal routing scheme with a polymeric insulator was used to independently address 288 actuators on the mirror. The two-layer metal allows narrow kerfs between actuators and increased actuator density. Anisotropic conductive film was used to bond thin flexible copper cables to flat edges of the mirror to interface with external control electronics. This prototype mirror has eight cables with a total of 290 connections to access the array. To reduce the cabling complexity for future mirrors, thin film transistors have been fabricated on the curved mirror to function as access switches. To facilitate this, a mask aligner that allows precision alignment on curved mirror segments was developed and arrays of thin film transistors (TFT) on curved substrates have been tested. TFT and actuator integration on future mirrors will reduce external connections to just two cables with a total of 30 connections. Keywords: Lynx, adjustable optics, X-ray optics, thin film piezoelectric, curved substrate aligner.
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U2 - 10.1117/12.2595316
DO - 10.1117/12.2595316
M3 - Conference contribution
AN - SCOPUS:85117803195
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Optics for EUV, X-Ray, and Gamma-Ray Astronomy X
A2 - O'Dell, Stephen L.
A2 - Gaskin, Jessica A.
A2 - Pareschi, Giovanni
PB - SPIE
T2 - Optics for EUV, X-Ray, and Gamma-Ray Astronomy X 2021
Y2 - 1 August 2021 through 5 August 2021
ER -