The Au site in Er + Au-implanted silica has been investigated by X-ray absorption spectroscopy, after annealing at 600 Β°C in either neutral N 2 or reducing H 2 (4%):N 2 (95%) atmosphere. High-resolution X-ray fluorescence spectra collected near the Au L III -edge indicate the presence of oxidized Au
The effect of line-mixing in near 15  on the emission of Mars atmosphere
β Scribed by F. Niro; C. Boulet; J.-M. Hartmann; E. Lellouch
- Publisher
- Elsevier Science
- Year
- 2005
- Tongue
- English
- Weight
- 291 KB
- Volume
- 95
- Category
- Article
- ISSN
- 0022-4073
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
I review our current understanding of positron sources in the Galaxy, on the basis of the reported properties of the observed 511 keV annihilation line. It is argued here that most of the disk positrons propagate away from the disk (due to the low density environment) and the resulting low surface b
The density, refractive index on mixing, and speed of sound at T = 298.15 K and atmospheric pressure have been measured over the whole composition range for {dimethyl carbonate (DMC), or diethyl carbonate (DEC) + methanol + toluene}, (diethyl carbonate + methanol), (dimethyl carbonate, or diethyl ca