- DOI
- 10.26302/SSHADE/EXPERIMENT_ZED_20250127_01
- Data reference
- Caminiti, Emma; Lantz, Cateline (2024): MIR spectra of Mercury terrestrial analogues irradiated by $He^+$ ions. SSHADE/DAYSY (OSUG Data Center). Dataset/Spectral Data. https://doi.org/10.26302/SSHADE/EXPERIMENT_ZED_20250127_01
- Database(s)
- Experimentalists
- Type(s)
- laboratory measurement
- Description
- Mid-IR spectra of Mercury terrestrial analogues pellets: unirradiated area and area irradiated by $He^+$ ions at 20 keV and a fluence up to $5.10^{17} ions.cm{-2}$.
- Number of spectra
- 12
- Variable type(s)
-
- sample composition
- irradiation dose
- Comments
- We irradiated pellets of Mercury terrestrial analogues on the SIDONIE isotope separator at IJCLab (Orsay, France) using $He^+$ ions at 20 keV and a fluence up to $5.10^{17}$ $ions.cm^{-2}$ .Two pellets were measured for each type of analogues. For each pellet, half of the samples was measured unirradiated and the other half was measured after irration with He+ with a fluence of $1.10^{17}$ $ions.cm^{-2}$ for the first samples and $5.10^{17}$ $ions.cm^{-2}$ for the second sample (bis).
- Laboratory
- Institut d'Astrophysique Spatiale (IAS)
- Instrument
- SMIS Cary 670 - confocal reflection Mid-IR
- Standard medium
- vacuum
- Observation mode
- spectrum
- Spectral range type(s)
- MIR
- Valid spectral range(s)
-
Min - Max (${\mu}m$) Sampling (${\mu}m$) Resolution (${\mu}m$) Position accuracy (${\mu}m$) Absorption edge #1 7.0 - 15.4 4.0 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
- specular
- Observation mode
- fixed angles
- Incidence angle
- 0.0°
- Emergence angle
- 0.0°
- Azimuth angle
- 180.0°
- Phase angle
- 0.0°
- Comments
- numerical aperture of 0.62
- Observation mode
- averaged
- Spots number
- 4
- Objective type
- x15
- Image size
- 200.0 x 200.0 ${\mu}m$
- Comments
- The spot size was between 160 and 400 μm^2. The resolution changes with the wavelength according to the Abbe's equation.
- Date begin
- 2024-01-01
Versions
- Release date
- 2025-02-17 11:25:33 UTC+0000
- Version (Date)
- #1 (2025-02-17 11:25:33 UTC+0000, Updated: 2025-02-17 11:25:33 UTC+0000)
