Computer Science – Performance
Scientific paper
Jan 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981spie..268..140k&link_type=abstract
In: Imaging spectroscopy; Proceedings of the Seminar, Los Angeles, CA, February 10,11, 1981. (A82-32440 15-74) Bellingham, WA, S
Computer Science
Performance
Design Analysis, Infrared Telescopes, Remote Sensors, Signal To Noise Ratios, Spectral Sensitivity, Systems Simulation, Atmospheric Models, Focal Plane Devices, Optical Filters, Radiance, Signature Analysis, Spectral Bands, Spectral Signatures, Transmission Efficiency
Scientific paper
The operation of the Spectrally Agile Staring Sensor (SASS) involves the employment of a telescope system which uses variable spectral band information to detect and identify moving IR sources against the background radiance of the earth. A description is presented of SASS simulation studies. A signal-to-noise ratio (SNR) expression used as a measure of system performance is considered. Attention is given to the target trajectory generator, a target signature model, a background and atmospheric model, a Dual Tunable Fabry-Perot (DTFP) optical filter model, problems of out-of-band leakage transmission, a Focal Plane Array (FPA)/spot convolution model, SNR improvement with high filter transmission efficiency, system performance vs DTFP optical filter parameters, and system performance vs atmospheric conditions.
Cox Jonathan A.
Kollodge M. A.
Marshall W. C.
Solstad R. G.
Steadman S. S.
No associations
LandOfFree
Design studies for a spectrally agile staring sensor /SASS/ system does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Design studies for a spectrally agile staring sensor /SASS/ system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Design studies for a spectrally agile staring sensor /SASS/ system will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1054278