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26 January 2016 Landsat swath imaging spectrometer design
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Abstract
This paper describes the design of a high-throughput and high-uniformity pushbroom imaging spectrometer and telescope system that is capable of Landsat swath and resolution while providing better than 10 nm per pixel spectral resolution over the full visible to short-wave infrared band. The design is based on a 3200×480  element×18  μm pixel size focal plane array, two of which are utilized to cover the full swath. At an optical speed of F/1.8, the system is the fastest proposed to date to our knowledge. The utilization of only two Dyson-type spectrometer modules fed from the same telescope reduces system complexity while providing a solution within achievable detector technology. Two telescope designs are shown to achieve the required swath and resolution from different altitudes. Predictions of complete system response are shown. Also, it is shown that detailed ghost analysis is a requirement for this type of spectrometer and forms an essential part of a complete design.
© 2016 Society of Photo-Optical Instrumentation Engineers (SPIE) 0091-3286/2016/$25.00 © 2016 SPIE
Pantazis Mouroulis, Robert O. Green, Byron Van Gorp, Lori B. Moore, Daniel W. Wilson, and Holly A. Bender "Landsat swath imaging spectrometer design," Optical Engineering 55(1), 015104 (26 January 2016). https://doi.org/10.1117/1.OE.55.1.015104
Published: 26 January 2016
JOURNAL ARTICLE
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