Chemical Crystallography
Compared to Cu-Kα, shorter wavelength radiation, such as Mo-Kα or Ag-Kα, allows diffraction experiments with minimized absorption and higher crystallographic resolution. Therefore, Mo-Kα is the favored wavelength for home-laboratory crystallography on small molecules and inorganic compounds, while Ag-Kα radiation is favorable for diffraction experiments on strongly absorbing materials and for high pressure crystallography.
Today's deposition techniques enable the fabrication of high quality multilayer coatings with small d-spacings that reflect at relatively large Bragg angles. The resulting mirrors have large capture angles and produce intensive beams that are required for high-resolution single crystal diffraction analyses in home-laboratories.
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| Helios mirrors | IµS for Mo-radiation | IµS for Ag-radiation |