3 May 1988 Data Processing Assessment For The Lunar Geoscience Observer Imaging Spectrometer
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Proceedings Volume 0890, Infrared Systems and Components II; (1988); doi: 10.1117/12.944281
Event: 1988 Los Angeles Symposium: O-E/LASE '88, 1988, Los Angeles, CA, United States
Abstract
On the Lunar Geoscience Observer (LGO) project a Visible and Infrared Mapping Spectrom-eter (VIMS) instrument has been proposed. This instrument will have science data input rates in the hundreds of kilobits per second (kbps) and an average telemetry output data rate of 4 kbps. Techniques that can be used to reduce the throughput of the instrument are editing, summing and averaging, data compression, data preprocessing, pattern recognition and snapshot data taking. Due to instrument limitations in the buffer memory size and processing speeds, a careful selection of the available techniques must be made.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
R. E. Irigoyen, H. M. Liaw, "Data Processing Assessment For The Lunar Geoscience Observer Imaging Spectrometer", Proc. SPIE 0890, Infrared Systems and Components II, (3 May 1988); doi: 10.1117/12.944281; https://doi.org/10.1117/12.944281
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KEYWORDS
Data compression

Infrared radiation

Data acquisition

Infrared imaging

Spectroscopy

Pattern recognition

Earth sciences

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