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Performance of the QWIP focal plane arrays for NASA's Landsat Data Continuity Mission
Author(s) -
Murzy Jhabvala,
K. K. Choi,
Augustyn Waczynski,
A. La,
M. Sundaram,
E. Costard,
Christine A. Jhabvala,
Emily Kan,
Duncan M. Kahle,
Richard Foltz,
Nicholas Boehm,
Michael Hickey,
Jason Sun,
Takahiro ADACHI,
Nicholas Costen,
Larry A. Hess,
H. Facoetti,
Matthew Montanaro
Publication year - 2011
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.886274
Subject(s) - cardinal point , pixel , focal plane arrays , quantum well infrared photodetector , optics , remote sensing , detector , dot pitch , physics , infrared , large format , computer science , quantum well , geology , laser
The focal plane assembly for the Thermal Infrared Sensor (TIRS) instrument on NASA's Landsat Data Continuity Mission (LDCM) consists of three 512 x 640 GaAs Quantum Well Infrared Photodetector (QWIP) arrays. The three arrays are precisely mounted and aligned on a silicon carrier substrate to provide a continuous viewing swath of 1850 pixels in two spectral bands defined by filters placed in close proximity to the detector surfaces. The QWIP arrays are hybridized to Indigo ISC9803 readout integrated circuits (ROICs). QWIP arrays were evaluated from four laboratories; QmagiQ, (Nashua, NH), Army Research Laboratory, (Adelphi, MD), NASA/ Goddard Space Flight Center, (Greenbelt, MD) and Thales, (Palaiseau, France). All were found to be suitable. The final discriminating parameter was the spectral uniformity of individual pixels relative to each other. The performance of the QWIP arrays and the fully assembled, NASA flight-qualified, focal plane assembly will be reviewed. An overview of the focal plane assembly including the construction and test requirements of the focal plane will also be described.

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