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Development of the imaging spectrometer - Technical challenges and solutionsThe imaging spectrometer (IS) is capable of performing direct identification of surface materials through their spectral signatures. This paper describes some of the system design and technology tradeoffs associated with the development of ISs; particular attention is given to optics, spectral dispersion, focal plane, and data handling,. Design examples for both earth and planetary remote-sensing applications are described, including AVIRIS, HIRIS, and VIMS.
Document ID
19880048738
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Herring, Mark (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Duval, James E. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Macenka, Steven A. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1987
Subject Category
Spacecraft Instrumentation
Meeting Information
Meeting: Optical systems for space applications
Location: The Hague
Country: Netherlands
Start Date: March 30, 1987
End Date: April 1, 1987
Sponsors: Comite Belge D'Optique, IEEE, NASA
Accession Number
88A35965
Distribution Limits
Public
Copyright
Other

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