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An imaging spectrometer for planetary studies

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Il Nuovo Cimento C

Summary

VNIR, a Visible Near-Infrared Mapping Spectrometer, was developed at IFSI-CNR and it is the visible channel of an experiment, named OMEGA, to be flown on the Russian Mars 94 mission, that will provide detailed mineralogical and chemical maps of the Mars surface. We have tested and calibrated the instrument in our laboratory, using it to take images and spectra of meteorites and terrestrial rocks. In the present work a description of the camera with some preliminary results of this activity are given.

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References

  1. V. Formisano et al.: VNIR-OMEGA, A visible mapping spectrometer for Mars 94, Internal Report IFSI, Frascati 1991.

  2. F. Mastracci:Sistema di acquisizione di immagini multispettrali: studio di meteoriti, Thesis, Rome, 1992.

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Bellucci, G., Mastracci, F., Formisano, V. et al. An imaging spectrometer for planetary studies. Il Nuovo Cimento C 16, 589–595 (1993). https://doi.org/10.1007/BF02512039

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  • DOI: https://doi.org/10.1007/BF02512039

PACS 93.85

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