Count into angular bins
Each virtual image sums stored radial counts in its declared half-open angular interval.
E32 · Angular selection and column contrast
Move the collection bounds through bright field and three annular geometries, using the same stored counts to test contrast and noise.
Physics tutorial
BackgroundMove the collection bounds through bright field and three annular geometries, using the same stored counts to test contrast and noise.
Why it mattersTarget: inner angle at least twice the convergence semi-angle, heavier-column contrast at least 0.2, heavy/light ROI intensity ratio at least 1.5, pooled difference SNR at least 10 and assumed probe FWHM at most 0.15 nm.
Start with the essentials
Each virtual image sums stored radial counts in its declared half-open angular interval.
The isotropic Gaussian radial law is an assumed transport surrogate. Radius and angle share the displayed collector geometry.
This pooled difference uses count statistics in separately declared regions; it is not a per-pixel SNR or composition inversion.
Typical misconceptionAny annular image directly identifies atoms.
Better mental modelThickness, angular acceptance and probe overlap also change contrast. Low-angle phase effects require a coherent model absent here.
Compare the separate specimen input with bright field and the selected angular image.
What to observe: Known regions are an audit, not a recovered chemical map.Change inner and outer angles while watching the native histogram and outcome budget.
What to observe: Virtual images change; native radial counts stay fixed.Use the resolved preset and check the target. Compare the count-derived row profiles.
What to observe: Read the signed contrast and pooled difference SNR together.Try low exposure, a broad probe and reversed bounds. Compare BF, ABF and low-angle ADF.
What to observe: Gain changes appearance; it cannot recover missing counts or resolve a blurred probe.