Data Processing Assessment For The Lunar Geoscience Observer Imaging Spectrometer

R. E. Irigoyen; H. M. Liaw

doi:10.1117/12.944281

3 May 1988 Data Processing Assessment For The Lunar Geoscience Observer Imaging Spectrometer

R. E. Irigoyen, H. M. Liaw

Proceedings Volume 0890, Infrared Systems and Components II; (1988) https://doi.org/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.

Citation Download Citation

R. E. Irigoyen and H. M. Liaw "Data Processing Assessment For The Lunar Geoscience Observer Imaging Spectrometer", Proc. SPIE 0890, Infrared Systems and Components II, (3 May 1988); https://doi.org/10.1117/12.944281

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