- DOI
- 10.26302/SSHADE/EXPERIMENT_ZD_20160831_01
- Data reference
- Dionnet, Zélia (2016): MIR spectrocopy of Paris meteorite. SSHADE/DAYSY (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_ZD_20160831_01
- Publications
- Database(s)
- Experimentalists
- Type(s)
- laboratory measurement
- Description
- Hyper-spectrale MIR spectroscopy of Paris meteorite in tranmission (sample crushed in a diamand compression cell)
- Number of spectra
- 4
- Variable type(s)
-
- no
- Laboratory
- Institut d'Astrophysique Spatiale (IAS)
- Instrument
- SMIS Cary 670 - trans Mid-IR
- Sample holder
- The sample was crushed in a diamond compression cell, which is transparent in the IR range
- Standard medium
- air
- Observation mode
- spectrum
- Spectral range type(s)
- MIR
- Valid spectral range(s)
-
Min - Max ($cm^{-1}$) Sampling ($cm^{-1}$) Resolution ($cm^{-1}$) Position accuracy ($cm^{-1}$) Absorption edge #1 849.0 - 3750.0 4.0 4.0 1.0
Definition: incidence and emergence angles are positive with origin at nadir. Emergence angle in transmission is larger than 90° (=180°-i).
- Observation geometry
- direct
- Observation mode
- fixed angles
- Observation mode
- image
- Objective type
- x25
- Pixels separation
- 0.66 x 0.66 ${\mu}m$
- Pixels number
- 128 x 128
- Image size
- 85.0 x 85.0 ${\mu}m$
- Spatial resolution
- 3.0 ${\pm}$ 1.0 ${\mu}m$ (3.0 $cm^{-1}$)
- Comments
- The resolution changes with the wavelenght according to the Abbe's equation.
- Date begin - end
- 2016-08-31 - 2016-08-31
Versions
- Release date
- 2022-05-18 18:52:30 UTC+0000
- Version (Date)
- #1 (2022-05-18 18:52:30 UTC+0000, Updated: 2022-05-18 18:52:30 UTC+0000)
