
Proceedings Paper
ZnO thin film transistors and electronic connections for adjustable x-ray mirrors: SMART-X telescopeFormat | Member Price | Non-Member Price |
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Paper Abstract
The proposed SMART-X telescope consists of a pixelated array of a piezoelectric lead zirconate titanate (PZT) thin film
deposited on flexible glass substrates. These cells or pixels are used to actively control the overall shape of the mirror
surface. It is anticipated that the telescope will consist of 8,000 mirror panels with 400-800 cells on each panel. This
creates an enormous number (6.4 million) of traces and contacts needed to address the PZT. In order to simplify the
design, a row/column addressing scheme using ZnO thin film transistors (TFTs) is proposed. In addition, connection of
the gate and drain lines on the mirror segment to an external supply via a flexible cable was investigated through use of
an anisotropic conductive film (ACF). This paper outlines the design of the ZnO TFTs, use of ACF for bonding, and
describes a specially designed electronics box with associated software to address the desired cells.
Paper Details
Date Published: 5 September 2014
PDF: 9 pages
Proc. SPIE 9208, Adaptive X-Ray Optics III, 920809 (5 September 2014); doi: 10.1117/12.2063369
Published in SPIE Proceedings Vol. 9208:
Adaptive X-Ray Optics III
Stephen L. O'Dell; Ali M. Khounsary, Editor(s)
PDF: 9 pages
Proc. SPIE 9208, Adaptive X-Ray Optics III, 920809 (5 September 2014); doi: 10.1117/12.2063369
Show Author Affiliations
R. L. Johnson-Wilke, The Pennsylvania State Univ. (United States)
R. H. T. Wilke, The Pennsylvania State Univ. (United States)
M. Wallace, The Pennsylvania State Univ. (United States)
J. I. Ramirez, The Pennsylvania State Univ. (United States)
Z. Prieskorn, The Pennsylvania State Univ. (United States)
J. Nikoleyczik, The Pennsylvania State Univ. (United States)
V. Cotroneo, Harvard-Smithsonian Ctr. for Astrophysics (United States)
R. H. T. Wilke, The Pennsylvania State Univ. (United States)
M. Wallace, The Pennsylvania State Univ. (United States)
J. I. Ramirez, The Pennsylvania State Univ. (United States)
Z. Prieskorn, The Pennsylvania State Univ. (United States)
J. Nikoleyczik, The Pennsylvania State Univ. (United States)
V. Cotroneo, Harvard-Smithsonian Ctr. for Astrophysics (United States)
R. Allured, Harvard-Smithsonian Ctr. for Astrophysics (United States)
D. A. Schwartz, Harvard-Smithsonian Ctr. for Astrophysics (United States)
S. McMuldroch, Harvard-Smithsonian Ctr. for Astrophysics (United States)
P. B. Reid, Harvard-Smithsonian Ctr. for Astrophysics (United States)
D. N. Burrows, The Pennsylvania State Univ. (United States)
T. N. Jackson, The Pennsylvania State Univ. (United States)
S. Trolier-McKinstry, The Pennsylvania State Univ. (United States)
D. A. Schwartz, Harvard-Smithsonian Ctr. for Astrophysics (United States)
S. McMuldroch, Harvard-Smithsonian Ctr. for Astrophysics (United States)
P. B. Reid, Harvard-Smithsonian Ctr. for Astrophysics (United States)
D. N. Burrows, The Pennsylvania State Univ. (United States)
T. N. Jackson, The Pennsylvania State Univ. (United States)
S. Trolier-McKinstry, The Pennsylvania State Univ. (United States)
Published in SPIE Proceedings Vol. 9208:
Adaptive X-Ray Optics III
Stephen L. O'Dell; Ali M. Khounsary, Editor(s)
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