Title
Comparison Of Relative Signal-To-Noise Ratios Of Different Classes Of Imaging Spectrometer
Abstract
The continued development of new and fiindamentally different classes of imaging spectrometer has increased both the scope and the complexity of comparisons of their relative signal-to-noise ratios. Although the throughput and multiplex advantages of Fourier-transform spectrometers were established in the early 1950s, the application of this terminology to imaging spectrometers is often ambiguous and has led to some confusion and debate. For comparisons of signal-collection abilities to be useful to a system designer, they must be based on identical requirements and constraints. We present unambiguous definitions of terminology for application to imaging spectrometers and comparisons of signal-collection abilities and signal-to-noise-ratios on a basis that is useful to a systems designer and inclusive of six fundamentally different classes (both traditional and novel) of imaging spectrometers. © 2005 Optical Society of America.
Publication Date
3-20-2005
Publication Title
Applied Optics
Volume
44
Issue
9
Number of Pages
1614-1624
Document Type
Article
Personal Identifier
scopus
DOI Link
https://doi.org/10.1364/AO.44.001614
Copyright Status
Unknown
Socpus ID
15944418580 (Scopus)
Source API URL
https://api.elsevier.com/content/abstract/scopus_id/15944418580
STARS Citation
Sellar, R. Glenn and Boreman, Glenn D., "Comparison Of Relative Signal-To-Noise Ratios Of Different Classes Of Imaging Spectrometer" (2005). Scopus Export 2000s. 4059.
https://stars.library.ucf.edu/scopus2000/4059