7 October 1996 The Visual and Infrared Mapping Spectrometer for Cassini
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Abstract
The visual and infrared mapping spectrometer (VIMS) is a remote sensing instrument developed for the Cassini mission to Saturn by an international team representing the national space agencies of the United States, Italy, and France. A dual imaging spectrometer, VIMS' unique design consists of two optical systems boresighted and operating in tandem, coordinated by a common electronics unit. The combined optical system generates 352 2D images simultaneously, each in a separate, contiguous waveband. These are combined by the electronics to produce 'image cubes' in which each image pixel represents a spectrum spanning 0.3 to 5.1 microns in 352 steps. VIMS images will be used to produce detailed spatial maps of the distribution of mineral and chemical species of Saturn's atmosphere, rings, and moons, and the atmosphere of Titan. At some wavelengths VIMS will penetrate Titan's atmosphere to map its surface, and image the night side of many Saturnian objects.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Edward A. Miller, Edward A. Miller, Gail Klein, Gail Klein, David W. Juergens, David W. Juergens, Kenneth Mehaffey, Kenneth Mehaffey, Jeffrey M. Oseas, Jeffrey M. Oseas, Ramon A. Garcia, Ramon A. Garcia, Anthony Giandomenico, Anthony Giandomenico, Robert E. Irigoyen, Robert E. Irigoyen, Roger Hickok, Roger Hickok, David Rosing, David Rosing, Harold R. Sobel, Harold R. Sobel, Carl F. Bruce, Carl F. Bruce, Enrico Flamini, Enrico Flamini, Romeo DeVidi, Romeo DeVidi, Francis M. Reininger, Francis M. Reininger, Michele Dami, Michele Dami, Alain Soufflot, Alain Soufflot, Yves Langevin, Yves Langevin, Gerard Huntzinger, Gerard Huntzinger, "The Visual and Infrared Mapping Spectrometer for Cassini", Proc. SPIE 2803, Cassini/Huygens: A Mission to the Saturnian Systems, (7 October 1996); doi: 10.1117/12.253421; https://doi.org/10.1117/12.253421
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