☄️ Cosmic Ray Air Showers
Interactive 3D atmosphere column where adjusting a primary cosmic ray's energy shows it cascading into a shower of secondary particles branching down through simulated atmospheric layers.
A primary cosmic ray enters the top of a simulated 20 km atmosphere column and cascades generation by generation into a branching shower of secondary particles that rains down toward a ground detector array.
🔬 What It Demonstrates
Using a Heitler-style cascade model, particle count roughly doubles each generation while energy per particle halves, until the critical energy is reached — the point of shower maximum, Xmax, which shifts with primary energy, particle type, and arrival angle.
🎮 How to Use
Raise the primary energy to watch the cascade grow deeper and wider, switch between a proton, an iron nucleus, and a gamma ray to compare how Xmax shifts, tilt the zenith angle, and toggle the muon component to see which secondaries punch through to the ground.
💡 Did You Know?
The highest-energy cosmic ray ever recorded, the "Oh-My-God" particle (~3 × 10²⁰ eV), struck the atmosphere with roughly the kinetic energy of a fast-pitched baseball packed into a single subatomic particle.
Interactive 3D atmosphere column where adjusting a primary cosmic ray's energy shows it cascading into a shower of secondary particles branching down through simulated atmospheric layers.
3D · Three.js / WebGL renderer · 60 FPS target · runs fully client-side, no install