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Controlling surface composition of bimetallic catalysts is of significance in energy conversion and storage.
Here we present the spectral parameter maps used in this Surface Composition of Vesta Special Issue.
The X-ray photoelectron spectroscopy was used to study the surface composition of the films.
Moreover, the surface wettability can be tuning by varying the surface composition of the coating.
The surface composition of the solid phases were analysed by X-ray Photoelectron Spectroscopy (XPS).
Thus, little is known about it, but reflectivity data returned by the U.S. Voyager 2 space probe in 1989 suggest a surface composition of ices and silicates.
The first mineralogical determination of the surface composition of an asteroid was made in 1969 when spectral reflectance measurements (see below Composition) identified the mineral pyroxene in the surface material of Vesta.
Further, the chemical environment of the surface composition of NiCo2O4/NiO is identified by X-ray Photoelectron spectroscopy.
These results suggested that the surface composition of PDMS influenced the adhesion, morphology and CYP450IA1 activity of hepatocyte.
Thus in each zone, the land surface composition of those excessively hot places can be compared to the zonal standard.
In this work, we tuned the surface composition of Pt3Co nanocatalysts by heat treatment under different atmosphere.
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