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Duval, James E.

Publications and source records attributed to Duval, James E..

Visible and infrared mapping spectrometer for exploration of comets, asteroids, and the Saturnian system of rings and moons

Consideration is given to a visible and infrared mapping spectrometer (VIMS) developed by American, Italian, and French scientists and engineers as a facility instrument for the Comet Rendezvous Asteroid Flyby (CRAF) mission and as a candidate facility instrument for the Cassini mission to explore Saturn and its rings and moons. VIMS is characterized by 0.35-5.2 micron spectral range with a nominal spatial resolution of 0.5 mrad and spectral resolutions of 7 nm at 0.35-1.0 micron wavelength and 16 nm at 1.0-5.2 micron wavelength.

Juergens, David W.↗

Development of the imaging spectrometer - Technical challenges and solutions

The imaging spectrometer (IS) is capable of performing direct identification of surface materials through their spectral signatures. This paper describes some of the system design and technology tradeoffs associated with the development of ISs; particular attention is given to optics, spectral dispersion, focal plane, and data handling,. Design examples for both earth and planetary remote-sensing applications are described, including AVIRIS, HIRIS, and VIMS.

Herring, Mark↗

An imaging spectrometer for the investigation of Mars

Unmanned misions to Mars will employ imaging spectrometry to yield compositional data about the target body, through visual and IR measurements of the intensity and distribution of characteristic spectral signature features in the radiation that is emitted and reflected by surface materials. Attention is presently given to a modular imaging spectrometer design with applicability to a diverse range of planetary missions. This visual and IR mapping spectrometer has been tentatively selected for NASA's recently approved Mars Observer mission. Detailed optical characteristics and capabilities of the instrument are presented.

Duval, James E.↗