Wiki source code of Amadee-18-FieldSpectrometry
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1.1 | 1 | === Details === |
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3.1 | 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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1.1 | 7 | |
| 8 | === Summary === | ||
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3.1 | 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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1.1 | 11 | |
| 12 | === Objectives === | ||
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3.1 | 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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1.1 | 15 | |
| 16 | === Experiment Data === | ||
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| 18 | |=Date|=Files | ||
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2.1 | 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 |