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From version < 2.1 >
edited by Barry Bishop
on 2018/02/11 12:49
To version < 4.1 >
edited by ahirtl
on 2018/02/14 12:03
>
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Summary

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1 -XWiki.bbishop
1 +XWiki.ahirtl
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1 1  === Details ===
2 2  
3 -|**Acronym**|
4 -|**Description**|
5 -|**Principal Investigator (PI)**|
6 -|**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
7 7  
8 8  === Summary ===
9 9  
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.
10 10  
11 11  === Objectives ===
12 12  
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.
13 13  
14 14  === Experiment Data ===
15 15  
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17 17  |[[2018-02-03>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-03]]|8 'asd' files
18 18  |[[2018-02-04>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-04]]|6 'asd' files
19 19  |[[2018-02-09>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-09]]|21 'asd' files
22 +|[[2018-02-13>>https://mission.oewf.org/archive_downloads/amadee18/06-FieldSpectrometry/2018-02-13]]|15 'asd' files (1 directory)
23 +
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