advanced33 min studyLesson 293 in Physics

Cyclotron motion and magnetic moment

Track signed gyromotion, perpendicular energy, and the assumptions behind a magnetic adiabatic invariant.

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What you’ll understand

  • Determine gyration direction from the charge sign.
  • Calculate gyrofrequency, radius, and magnetic moment.
  • Distinguish exact energy conservation from approximate magnetic-moment conservation.

A magnetic force bends a charged particle's velocity without directly doing work. Its perpendicular motion therefore circles while its parallel motion advances freely in a uniform field. Plasma theory often replaces that fast orbit by a slowly moving guiding centre. The replacement becomes reliable only when the particle sees little change during one turn; magnetic-moment conservation records that separation of scales.

A signed frequency fixes the direction

Let B=Bz^\mathbf B=B\hat{\mathbf z} with B>0B>0 and no electric field. Cartesian Lorentz-force components give v˙x=Ωcvy\dot v_x=\Omega_c v_y and v˙y=−Ωcvx\dot v_y=-\Omega_c v_x, where Ωc=qB/m\Omega_c=qB/m is signed. With initial perpendicular velocity along positive x, a positive charge initially accelerates toward negative y. Viewed from positive z toward the origin, its orbit is clockwise; changing the charge sign reverses that direction without changing the speed.

The positive gyration rate is ∣Ωc∣|\Omega_c|, its period is 2π/∣Ωc∣2\pi/|\Omega_c|, and the Larmor radius uses the velocity perpendicular to the field. Parallel velocity instead sets the helix pitch per turn. The magnetic force is always orthogonal to the instantaneous total velocity, so kinetic energy is exactly constant in a static magnetic field, even when that field varies in space. That exact statement does not by itself establish a circular orbit in a nonuniform field.

Ωc=qBm,ρL=v⊥∣Ωc∣,ddt(mv22)=qv⋅E\Omega_c=\frac{qB}{m},\qquad \rho_L=\frac{v_\perp}{|\Omega_c|},\qquad \frac{d}{dt}\left(\frac{mv^2}{2}\right)=q\mathbf v\cdot\mathbf E
For a nonrelativistic particle, q is signed charge in C, B magnetic-field magnitude in T, m mass in kg, ρ_L radius in m, and Ω_c angular frequency in rad/s. Uniform B gives the exact circular perpendicular orbit. The energy equation also applies to nonuniform fields.↔ Scroll wide equations horizontally.

The invariant is positive, the dipole vector is diamagnetic

Define the scalar magnetic moment μ=mv⊥2/(2B)\mu=mv_\perp^2/(2B) using the fast gyration relative to the guiding centre. This positive quantity is perpendicular kinetic energy divided by field magnitude. It is independent of the sign of charge for given mass, speed, and field. The associated orbital magnetic dipole vector points opposite to B\mathbf B for either charge sign: reversing the orbit and reversing charge cancel in the current-loop orientation. Do not replace this scalar by signed charge.

In a slowly varying field, the gyro-averaged scalar is approximately conserved. Require ρL/LB≪1\rho_L/L_B\ll1 and a fractional field change during a gyrotime much smaller than unity, with the latter measured along the particle's motion as well as at a fixed location. Collisions and resonant fluctuations can invalidate the averaging. A small laboratory time derivative alone is insufficient if the particle traverses a sharp spatial gradient during one turn.

μ=mv⊥22B=K⊥B,ρLLB≪1,∣dB/dt∣B∣Ωc∣≪1,dμdt≃0\mu=\frac{mv_\perp^2}{2B}=\frac{K_\perp}{B},\qquad \frac{\rho_L}{L_B}\ll1,\qquad \frac{|dB/dt|}{B|\Omega_c|}\ll1,\qquad \frac{d\mu}{dt}\simeq0
μ has units J/T; L_B is a representative field-variation length, and dB/dt follows the sampled field along the guiding centre. These inequalities state a leading-order adiabatic regime away from field nulls and resonances. They do not claim exact conservation through arbitrary changes.↔ Scroll wide equations horizontally.

Follow energy as well as moment

In a static nonuniform magnetic field with negligible electric field, total kinetic energy stays fixed while conserved μ\mu makes perpendicular energy increase as the particle reaches stronger field. Parallel energy must decrease by the same amount. The resulting mirror force is an averaged consequence of the Lorentz dynamics, not work by the magnetic force. This explains how a particle can slow along a field even though its total speed remains constant.

If the field is instead increased slowly in time, Faraday's law generally supplies an induced electric field. That field can do work on the gyromotion, increasing perpendicular energy while approximately preserving μ\mu. Confusing these two situations leads to an apparent contradiction about magnetic work. Always distinguish spatial travel through a static field from temporal field compression, and check whether electric forces, collisions, or a vanishing field destroy the assumptions before using the invariant.

A proton orbit and its scale separation

A proton with q=1.60×10−19 Cq=1.60\times10^{-19}\,\mathrm C and m=1.67×10−27 kgm=1.67\times10^{-27}\,\mathrm{kg} has perpendicular speed 105 m/s10^5\,\mathrm{m/s} in B=0.10 TB=0.10\,\mathrm T. Calculate its positive gyrofrequency, radius, and scalar moment. Compare its radius with a 1 m field-gradient scale.

  1. Compute ∣Ωc∣=qB/m=9.58×106 rad/s|\Omega_c|=qB/m=9.58\times10^6\,\mathrm{rad/s}. For an initial velocity along positive x and field along positive z, the positive proton bends toward negative y, fixing the orientation independently of the magnitude calculation.

  2. The radius is 105/(9.58×106)=1.04×10−2 m10^5/(9.58\times10^6)=1.04\times10^{-2}\,\mathrm m. Thus ρL/LB=0.0104\rho_L/L_B=0.0104 for the specified metre-scale variation, a favourable spatial ordering for a guiding-centre description.

  3. The perpendicular energy is mv⊥2/2=8.35×10−18 Jmv_\perp^2/2=8.35\times10^{-18}\,\mathrm J, so μ=8.35×10−17 J/T\mu=8.35\times10^{-17}\,\mathrm{J/T}. Temporal variation and collisions still need separate checks; a small radius does not establish those conditions.

The result

The proton gyrates at 9.58 million rad/s with radius 1.04 cm and scalar moment 8.35 × 10⁻¹⁷ J/T. Its radius is about one percent of the proposed gradient scale.

Explore the model

Interactive lab

Interactive lab · vectors

Resolve a pitch angle

Use the x projection as parallel speed and y as perpendicular speed in normalized units. Reset and set both controls to angle 30° and magnitude 2; predict a perpendicular projection of 1. Reset and set both controls to angle 60° and magnitude 2; predict √3. This static vector decomposition does not integrate a helical trajectory or test adiabatic conservation.

Resolve a pitch anglePlayback traces a fixed vector and its projections. Angle and magnitude set the geometry; the moving marker does not change them. Current readings: x component: 1.393; y component: 0.975; Magnitude: 1.7. All parameters are adjustable with the labeled controls below.−7.46−3.7303.737.46−3.5−1.7501.753.5xyvvₓ = 1.39
Vectorx / y projectionsTrace marker
x component
1.393
y component
0.975
Magnitude
1.7
t = 0 s

Playback traces a fixed vector and its projections. Angle and magnitude set the geometry; the moving marker does not change them. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.

Look forPitch angle changes the perpendicular-energy fraction while holding total speed fixed; gyromotion requires additional dynamics.

Check your understanding

A particle moves into stronger static magnetic field with no electric field while magnetic-moment conservation is valid. What happens before it reaches a mirror point?

Try it yourself

In a static magnetic field a particle starts with perpendicular energy 20 eV and parallel energy 80 eV at 0.20 T. It reaches 0.50 T while the adiabatic approximation holds and electric fields are negligible. Find both energies there and decide whether it has already mirrored.

Take a moment to make a prediction or work it out on paper. Open a hint when you need one.

Give me a hint

Scale perpendicular energy with B, then subtract it from the conserved total energy.

Compare with the solution

The field increases by 2.5, so perpendicular energy becomes 20(2.5)=50 eV20(2.5)=50\,\mathrm{eV}. Total energy remains 100 eV, leaving 50 eV parallel energy. The particle has not yet mirrored because its parallel energy is positive. Its formal turning field is Bm=0.20(100/20)=1.0 TB_m=0.20(100/20)=1.0\,\mathrm T, provided the field can reach that value and adiabatic ordering remains valid along the path. A temporally increasing field would require a different energy calculation because induced electric fields can supply work.

Take it with you

  • Use signed gyrofrequency for direction and its magnitude for radius and period.
  • Magnetic-moment conservation requires spatial and temporal scale separation.
  • Static magnetic fields redistribute parallel and perpendicular energy without changing their sum.

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