- Title
- Vis-NIR reflectance spectra of JSC Mars 1 or Dark basalt powders pure, and/or mixed with H2O ice (with ice particles ~4 or ~67 µm, or in a slab), and/or covered with H2O frost
- DOI
- 10.26302/SSHADE/EXPERIMENT_OP_20201104_001
- Data reference
- Yoldi, Zuriñe (2016): Vis-NIR reflectance spectra of JSC Mars 1 or Dark basalt powders pure, and/or mixed with H2O ice (with ice particles ~4 or ~67 µm, or in a slab), and/or covered with H2O frost. SSHADE/BYPASS (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_OP_20201104_001
- Publications
- Database(s)
- Experimentalists
- Type(s)
- laboratory measurement
- Number of spectra
- 47
- Variable type(s)
-
- sample composition
- Standard medium
- air
- Observation mode
- spectrum
- Spectral range type(s)
- Vis, NIR
- Valid spectral range(s)
-
Min - Max (${\mu}m$) Sampling (${\mu}m$) Resolution (${\mu}m$) Position accuracy (${\mu}m$) Absorption edge #1 0.38 - 0.96 0.02 0.015 #2 0.96 - 2.404 0.01 0.03
Definition: incidence and emergence angles are positive with origin at nadir, and vary in same direction. Azimuth origin (increasing clockwise) is for i = e (opposition geometry).
- Observation geometry
- biconical
- Observation mode
- fixed angles
- Emergence angle
- 13.0°
- Azimuth angle
- 0.0°
- Comments
- The light beam emitted from the extremity of the fibre bundle positionned about 300 mm above the sample surface has a divergence half-angle of 12.7°. The light source incidence and azimuth angles are slightly variable from pixel to pixel.
- Observation mode
- roi averaged
- Comments
- Note to the provider: Complete the "image" observation_mode when fully implemented in SSHADE. Because SCITEAS data are hyperspectral images.
- Date begin - end
- 2016-11-18 - 2019-07-10
Versions
- Release date
- 2020-11-13 21:44:36 UTC+0000
- Version (Date)
- #1 (2020-11-13 21:44:36 UTC+0000, Updated: 2020-11-13 21:44:36 UTC+0000)