Near ultraviolet visible infrared mapping spectrometer (NU-VIMS)

Details Near ultraviolet visible infrared mapping spectrometer (NU-VIMS) Near ultraviolet visible infrared mapping spectrometer (NU-VIMS)

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2209..332r&link_type=abstract

Proc. SPIE Vol. 2209, p. 332-344, Space Optics 1994: Earth Observation and Astronomy, M. G. Cerutti-Maori; Philippe Roussel; Eds

Physics

Optics

2

Scientific paper

The NU-VIMS is a new instrument concept for high resolution spectral imaging within the spectral band of 0.25 to 5.0 micrometers . The concept utilizes state-of-the-art detector and grating technologies to extend the capabilities of the Cassini/VIMS-V prototype while maintaining its compact and lightweight format. The NU-VIMS optical design achieves remarkable performance while relying only on spherical surfaces in a single optical channel with only one grating and either one or two detector arrays. Though the concept was developed in anticipation of the MORO, Rosetta, and Pluto-Charon deep space missions, the instrument could also be mounted on a lightweight satellite for low cost remote sensing of the earth.

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