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The Digital Imaging and Remote Sensing Group at RIT has constructed an imaging
spectrometer called the Modular Imaging Spectrometer Instrument which is a line
scanner with a 6" rotating mirror coupled to a Cassegrain telescope of focal
ratio f/3.3. Two 0.5mm square silicon detectors (broad-band visible) and two
1.5mm fiber optics are placed at the primary focal plane to give a GIFOV of
0.3 m and 1.0 m respectively at 0.3 km of altitude. The fibers lead to two
separate 36-channel spectrometers to cover the EM spectrum from 0.440µm to
1.020µm in 0.010µm spectral bands. A pyramid mirror diverts some photons from
the primary focal plane to five HgCdTe detectors for the long-wave infrared
region; secondary focal planes are available in the SWIR and MWIR for future use
(Feng, 1995). An on-board calibration system consisting of two blackbodies for
the LWIR and a tungsten source for the visible completes this imaging system
for gathering
absolute radiometrically calibrated data
for remote sensing
applications.
The system is designed to serve as:
The Spectral Calibration of MISI
The Thermal Calibration of MISI
Web Reference:
Feng, Xiaofan., "Design and Performance of a Modular Imaging Spectrometer
Instrument", Rochester Institute of Technology Ph.D. Dissertation, (1995).
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The Modular Imaging Spectrometer Instrument (MISI) An AutoCad schematic of MISI First Line-Scan Image Taken by the Broad-Band Visible Detectors on the MISI of the Rochester Skyline (12/02/95). First Line-Scan Image Taken by the Broad-Band Visible Detectors on the MISI of the RIT Dormitories (12/02/95). |