Changes for page Amadee-18-FieldSpectrometry

Summary

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3	3	=== Details ===
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5		-|**Acronym**|
6		-|**Description**|
7		-|**Principal Investigator (PI)**|
8		-|**Organisation** |
	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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10	10	=== 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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13	13	=== 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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18	18	|=Date|=Files
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	19	+|[[2018-02-03>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-03]]|8 'asd' files
	20	+|[[2018-02-04>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-04]]|6 'asd' files
	21	+|[[2018-02-09>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-09]]|21 'asd' files