- Title
- Vis-NIR reflectance spectroscopy of the meteorite Murchison with varying grain sizes from 1000µm to 45µm
- DOI
- 10.26302/SSHADE/EXPERIMENT_SP_20210420_1000
- Data reference
- Cloutis, Edward; Applin, Daniel (2014): Vis-NIR reflectance spectroscopy of the meteorite Murchison with varying grain sizes from 1000µm to 45µm. SSHADE/CHIPS (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_SP_20210420_1000
- Publications
- Database(s)
- Experimentalists
- Type(s)
- laboratory measurement
- Description
- 0.35 to 2.5µm reflectance spectroscopy of a powdered sample of the meteorite Murchison sieved to select grains sizes <1000µm, <500µm, <250µm, <150µm, <90µm and <45µm.
- Number of spectra
- 6
- Variable type(s)
-
- sample grain size
- Instrument
- ASD reflection VIS-NIR
- 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 #1 350.0 - 2500.0 1.0
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
- conical-directional
- Observation mode
- fixed angles
- Incidence angle
- 30.0°
- Emergence angle
- 0.0°
- Azimuth angle
- 0.0°
- Phase angle
- 30.0°
- Observation mode
- single spot
- Spatial resolution
- 5.0 $mm$
- Date begin
- 2014-07-03
Versions
- Release date
- 2021-04-22 14:45:05 UTC+0000
- Version (Date)
- #1 (2021-04-22 14:45:05 UTC+0000, Updated: 2021-04-22 14:45:05 UTC+0000)