Changes for page Amadee-18-FieldSpectrometry

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Details

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1	1	=== Details ===
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3		-|**Acronym**|Field spectrometry
4		-|**Description**|Acquisition of reflectance and radiance spectra in an environment analogous to Mars
5		-|**Principal Investigator (PI)**|Eleonora Ammannito
6		-|**Organisation** |Agenzia Spaziale Italiana
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8	8	=== Summary ===
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10		-VIS-NIR reflectance spectroscopy is the major technique used so far to identify mineralogical phases present on the surface of Mars. However, the interpretation of reflectance spectra is subject to a deep understanding of the contest in which the measurements have been acquired. The co-existence of different minerals (Brossard et al. 2016), the temperature (Singer & Roush 1985) and illumination (Mustard & Pieters, 1989) - just to cite few examples - can significantly alter the shape of absorption features of minerals leading to mistakes in the determination of the composition of the site under analysis.
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12	12	=== Objectives ===
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14		-The scope of our proposal is to acquire spectra in a realistic Martian-like environment along with ancillary information like temperature and illumination conditions to check the reliability of mineralogical interpretation.
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16	16	=== Experiment Data ===
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