Calculation Of Stem Dark-Field Images
Dark-field imaging is a promising procedure to visualize single atoms in high resolution electron microscopy. The quality of a dark-field micrograph depends to a large extent on the illumination mode for the CTEM or on the detector geometry for the STEM. The most commonly used dark-field modes are: CTEM with axial, tilted, or hollow-cone illumination and STEM with an annular detector limited by the angles and θ1-θ2. The STEM is equivalent to a CTEM which uses hollow-cone illumination of finite angular width (limiting angles θ1, θ2). the following we always assume θ2 = п/2.The three CTEM imaging modes have been investigated theoretically by several authors. Krakow (1) computed dark-field images of small organometallic molecules assuming tilted illumination. However, he could not achieve results for hollow-cone illumination because his computing method was too timeconsuming. Hoch (2) calculated images of model objects under axialy tilted, and hollow-cone illumination of infinitely small angular widthy applying the fast Fourier transform technique.