Empirical range scale
Energy is in keV, density in grams per cubic centimetre. Atomic mass uses tabulated C, Si and Au values or an explicit proxy. The low-energy end is an extrapolation.
E05 · Electron microscopy / specimen physics
Change beam energy, atomic number, density and specimen thickness. Follow seeded primary-electron walks through the cutaway sample, switch emission pathways, and compare their source depths. Keep secondary electrons surface sensitive while transmitting at least half the primary beam.
Physics tutorial
BackgroundChange beam energy, atomic number, density and specimen thickness. Follow seeded primary-electron walks through the cutaway sample, switch emission pathways, and compare their source depths. Keep secondary electrons surface sensitive while transmitting at least half the primary beam.
Why it mattersSeparate specimen physics from detector appearance before interpreting an electron image.
Start with the essentials
Energy is in keV, density in grams per cubic centimetre. Atomic mass uses tabulated C, Si and Au values or an explicit proxy. The low-energy end is an extrapolation.
Generated signal and escape probability are separate. The depth plot compares kernels normalized to their peaks, not absolute yields.
Typical misconceptionA schematic image is a calibrated material prediction.
Better mental modelTeaching Monte Carlo: empirical Kanaya–Okayama range sets a continuous-slowing path budget; scattering is an invented random-walk kernel, not measured cross sections. Signal branches are schematic, not calibrated yields. SE and Auger escape lengths are assumed; CL requires a luminescent material. X-ray excitation uses a rough shell threshold. No quantitative compositional analysis.
Predict which will transmit more: a silicon block or a thin foil. Compare their detected end-point fractions.
What to observe: A signal generated deep inside the specimen can be absorbed before reaching a detector. Transmission changes with thickness; surface escape remains shallow.Transmit at least 50 percent of primary histories while keeping the modeled SE 90-percent source depth below 15 nm.
What to observe: The task checks quantitative readouts rather than visual brightness.Compare silicon and gold, then switch off each signal pathway. Explain why depth distributions differ even under the same beam.
What to observe: Teaching Monte Carlo: empirical Kanaya–Okayama range sets a continuous-slowing path budget; scattering is an invented random-walk kernel, not measured cross sections. Signal branches are schematic, not calibrated yields. SE and Auger escape lengths are assumed; CL requires a luminescent material. X-ray excitation uses a rough shell threshold. No quantitative compositional analysis.