Academy
Formulas/physics/Moving Charges/Helical Motion — Pitch

Helical Motion — Pitch

When v has a component parallel to B, that component is unaffected by B. The particle traces a helix: radius r = mv⊥/qB from the perpendicular component, pitch p from the parallel component.
Class 12
Derivation

Setup

A charged particle enters a uniform field B\vec{B} (along zz-axis) with velocity v\vec{v} at angle α\alpha to B\vec{B}.

Resolve:

  • v=vcosαv_{\parallel} = v\cos\alpha — component along B\vec{B}
  • v=vsinαv_{\perp} = v\sin\alpha — component perpendicular to B\vec{B}

Motion in Each Component

Perpendicular component: B\vec{B} exerts force, causing circular motion in the xyxy-plane.

r=mvqB=mvsinαqBr = \frac{mv_{\perp}}{qB} = \frac{mv\sin\alpha}{qB}

Parallel component: B\vec{B} exerts no force on vv_{\parallel} (since vBv_{\parallel} \parallel \vec{B}, sin0°=0\sin 0° = 0). The particle moves at constant vv_{\parallel} along zz.

Helical Path

The combination of circular motion in xyxy and uniform motion in zz gives a helix.

Period of one circular revolution: T=2πm/qBT = 2\pi m / qB

Distance advanced along zz in one revolution — the pitch:

p=vT=2πmvqB=2πmvcosαqB\boxed{p = v_{\parallel}\,T = \frac{2\pi m\,v_{\parallel}}{qB} = \frac{2\pi m v\cos\alpha}{qB}}

Summary

QuantityExpression
Radiusr=mvsinα/qBr = mv\sin\alpha\,/\,qB
Pitchp=2πmvcosα/qBp = 2\pi mv\cos\alpha\,/\,qB
PeriodT=2πm/qBT = 2\pi m / qB
Note
Charged particles in Earth's magnetic field follow helical paths along field lines — this is why cosmic rays funnel toward the poles and cause the aurora.