Inset: X-ray surface microanalysis of the PS GO structures.
Consequently, we could detect X-ray surface scattering of the order of 10−6.
The X-ray surface microanalysis (EDS) of the hybrid structures found the traces of silicon, carbon, and oxygen.
The X-ray surface brightness is generally anti-correlative with the IR and radio brightness.
Nanofabricated supported model catalyst systems can be probed with traditional scanning probe imaging techniques and synchrotron X-ray surface characterization tools.
The main scientific task of SCXM would be the mapping of the coronal X-ray emission, i.e. to resolve the radial distribution of the X-ray surface brightness around the Sun.
We present results of the study on the spatial asymmetric distribution of the X-ray surface brightness and the plasma temperature in distant clusters of galaxies (z>0.1) with ASCA.
The shaded area denotes the mass loss evolution derived by Wood et al. (2005), who used their power law fit to the X-ray surface flux (cf. Eq. (3)) and the evolution of the X-ray flux (FX ∝ t−1.74±0.34) of Sun-like stars (Ayres, 1997) to construct the scaling.
Characterisation of the apatites included elemental analysis, X-ray diffraction, surface roughness, specific surface area, density, and solubility.
Micronized SFL powders were characterized by X-ray diffraction, surface area, scanning and transmission electron microscopy, contact angle and dissolution.
The treated samples were characterized by X-ray diffraction, surface area, pore volume, and pore size distribution measurements.
