- Database
- Experimentalists
- Date
- 2013-01-01
- Provider
- IAS, Orsay
- Thickness
- 200.0 ± 100.0 μm
- Diameter
- 13000.0 μm
- Mass
- 0.1 ± 0.02 g
- Substrate material
- KBr
- Substrate comments
- KBr window, 2 mm thick, 13 mm diameter. The KBr is used as a substrate to avoid meteorite pellet break.
- Comments
- Pellet prepared by pressing (7 tons for 10 min) about 100 mg of the original dust (grain size 1–100 µm) on top of a KBr substrate pellet. The KBr is used as a substrate to avoid pellet break. Thickness of the meteorite pellet is large enough (>200 µm) to avoid contribution of KBr to the spectra.
Area D, irradiated with 3 1016 He+ cm−2
- Temperature
- 300.0 ± 5.0 K
- Temperature max
- 300.0 ± 5.0 K
- Type
- ambient air
- Fluid pressure
- 1.0 mbar
- Source
- ions accelerator
- Chronology
- before spectrum
- Comments
- Selected spectrum of the 3 1016 He+.cm−2 irradiated area, showing the most disordered (most irradiated) polyaromatic carbon (large D and G bands), thus representative of the irradiated layer (see Lantz et al., 2015, for details). We used ion currents in the 0.1–0.3 µA.cm−2 range to avoid macroscopic heating of the samples.
- Family
- atoms and molecules
- Type
- atomic ions
- Particle
- He+
- Energy
- 40.0 keV.particle−1
- Particle fluence
- 3e+16 particle.m−2
Particle
- Number
- 1
- Layers
-
- Pellet of Murchison powder , 200.0 μm
- Title
- Murchison pellet preparation
- Matters
- Sample
- Pellet of Murchison powder (n°2) (this sample)
- Processing steps
-
Step Chronology Date Type Process Changes #1 before layer formation 2013-01-01 mechanical pressing granular KBr to form the pellet substrate #2 during layer formation 2013-01-01 mechanical pressing Murchison powder on top of the KBr substrate (7 tons for 10 min)