Bremsstrahlung & Synchrotron Radiation Pattern

This interactive simulator explores Bremsstrahlung & Synchrotron Radiation Pattern in Astronomy & The Sky. Polar plot of dP/dΩ for an accelerating charge: a ∥ v (linear / brems) and a ⊥ v (circular / synchrotron). Pull β = v/c toward 1 — Larmor donut collapses into a forward beam of half-angle ≈ 1/γ; ω_g, ω_c shown for given B. Use the controls to change the scenario; watch the visualization and any graphs or readouts to connect the model with lectures, labs, and homework.

Who it's for: For learners comfortable with heavier math or second-level detail. Typical context: Astronomy & The Sky.

Key terms

bremsstrahlung
synchrotron
radiation
pattern
bremsstrahlung synchrotron
astronomy

How it works

Angular radiation pattern of an accelerating charge — switch between bremsstrahlung-style acceleration parallel to velocity (a ∥ v) and synchrotron-style circular motion (a ⊥ v), and watch the Larmor donut at β → 0 collapse into a forward-pointing relativistic beam of half-angle ≈ 1/γ as β → 1. The polar plot is dP/dΩ in arbitrary units; the right panel cartoons the charge in linear motion or in a circular orbit (with toy magnetic field B giving the gyrofrequency ω_g = qB/(γm) and synchrotron critical frequency ω_c ≈ (3/2)γ³ω_g — the workhorse of synchrotron light sources and astrophysical jets).