- Title
- VIS-NIR reflectance spectra of binary mixtures between the fine fraction of the JSC Lunar regolith simulant (JSC-1AF) and two types of spherical water ice particles
- DOI
- 10.26302/SSHADE/EXPERIMENT_ZY_20180110_002
- Data reference
- Yoldi, Zuriñe (2018): VIS-NIR reflectance spectra of binary mixtures between the fine fraction of the JSC Lunar regolith simulant (JSC-1AF) and two types of spherical water ice particles. SSHADE/BYPASS (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_ZY_20180110_002
- Publications
- Database(s)
- Experimentalists
- Type(s)
- laboratory measurement
- Description
- Intimate mixtures of two types of spherical water ice particles (SPIPA-A and -B, 4.5 and 67 µm average diameter, respectively) and the JSC-1AF fine-grained fraction of JSC Lunar Regolith Simulant.
- Number of spectra
- 11
- Variable type(s)
-
- sample composition
- sample grain size
- Standard medium
- vacuum
- Observation mode
- spectrum
- Spectral range type(s)
- Vis, NIR
- Valid spectral range(s)
-
Min - Max ($nm$) Sampling ($nm$) Resolution ($nm$) Position accuracy ($nm$) Absorption edge #1 400.0 - 940.0 15.0 6.5 #2 946.0 - 1294.0 6.0 6.5 #3 1300.0 - 2404.0 6.0 13.0
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
- Incidence angle
- 20.0°
- Emergence angle
- 30.0°
- Azimuth angle
- 180.0°
- Phase angle
- 50.0°
- Observation mode
- roi averaged
- Spots number
- 1
- Date begin - end
- 2018-01-10 - 2018-01-12
Versions
- Release date
- 2023-05-04 06:59:02 UTC+0000
- Version (Date)
- #1 (2023-05-04 06:59:02 UTC+0000, Updated: 2023-05-06 09:08:13 UTC+0000)
- Sponsors
-
- Swiss National Science Fundation (SNSF)