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.

 

 

Helios mirrors

 

IµS for Mo-radiation

 

IµS for Ag-radiation