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).
Key equations
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