The motion of a charged particle in a magnetic field can be analyzed into two components of velocity:
1. A component \( v_{\perp} \) perpendicular to the magnetic field, causing circular motion.
2. A component \( v_{\parallel} \) parallel to the magnetic field, causing linear motion along the direction of the field.
The total velocity \( v \) is the vector sum of these two components:
\[
v_{\perp} = v \sin \theta, \quad v_{\parallel} = v \cos \theta.
\]
The perpendicular component causes circular motion, and the parallel component causes linear motion along the magnetic field direction, resulting in a helical path.
The magnetic force provides the centripetal force for the circular motion, which gives the radius \( r \) of the circular path:
\[
\frac{mv_{\perp}^2}{r} = q v_{\perp} B.
\]
Solving for \( r \):
\[
r = \frac{mv_{\perp}}{qB}.
\]
The time period \( T \) for one complete revolution is the circumference of the circle divided by the velocity:
\[
T = \frac{2\pi r}{v_{\perp}} = \frac{2\pi m}{qB}.
\]
The frequency of revolution \( \nu \) is the reciprocal of the time period:
\[
\nu = \frac{1}{T} = \frac{qB}{2\pi m}.
\]
Thus, the particle follows a helical path with a frequency of revolution \( \nu = \frac{qB}{2\pi m} \).