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Charged Particle Motion

Understanding how individual charged particles move in electromagnetic fields is fundamental to plasma physics and fusion research. This single-particle picture provides insights into plasma confinement, heating, and transport.

The motion of a charged particle in electromagnetic fields is governed by the Lorentz force:

mdvdt=q(E+v×B)m\frac{d\mathbf{v}}{dt} = q(\mathbf{E} + \mathbf{v} \times \mathbf{B})

where mm is the particle mass, qq is the charge, v\mathbf{v} is the velocity, E\mathbf{E} is the electric field, and B\mathbf{B} is the magnetic field.

In a uniform magnetic field with no electric field, charged particles execute circular motion perpendicular to the field. This is called cyclotron motion or gyromotion.

The cyclotron frequency (gyrofrequency) is:

ωc=qBm\omega_c = \frac{|q|B}{m}

For electrons and ions in a 5 T magnetic field (typical for tokamaks):

  • Electron cyclotron frequency: ωce8.8×1011\omega_{ce} \approx 8.8 \times 10^{11} rad/s
  • Deuterium ion cyclotron frequency: ωci2.4×108\omega_{ci} \approx 2.4 \times 10^{8} rad/s

The cyclotron radius (Larmor radius or gyroradius) is:

ρL=vωc=mvqB\rho_L = \frac{v_\perp}{\omega_c} = \frac{mv_\perp}{|q|B}

where vv_\perp is the velocity component perpendicular to B\mathbf{B}.

For thermal particles with perpendicular velocity vvth=2kBT/mv_\perp \sim v_{th} = \sqrt{2k_BT/m}:

ρL=2mkBTqB\rho_L = \frac{\sqrt{2mk_BT}}{|q|B}

In a 10 keV, 5 T tokamak plasma:

  • Electron Larmor radius: ρLe0.1\rho_{Le} \approx 0.1 mm
  • Deuterium Larmor radius: ρLi4\rho_{Li} \approx 4 mm

The ion Larmor radius being larger than the electron Larmor radius has important consequences for plasma confinement and transport.

The guiding center is the center of the circular gyration. On timescales longer than the cyclotron period, particle motion can be described as the movement of this guiding center. This adiabatic approximation greatly simplifies the analysis of particle dynamics.

When additional forces or field gradients are present, particles drift perpendicular to both the magnetic field and the force. The general drift velocity for a force F\mathbf{F} is:

vd=F×BqB2\mathbf{v}_d = \frac{\mathbf{F} \times \mathbf{B}}{qB^2}

In crossed electric and magnetic fields, all particles (regardless of charge or mass) drift with:

vE=E×BB2\mathbf{v}_E = \frac{\mathbf{E} \times \mathbf{B}}{B^2}

This drift is independent of particle charge and mass, so both electrons and ions drift together, not causing any current.

In a non-uniform magnetic field, the drift due to the gradient in B|\mathbf{B}| is:

vB=mv22qB3(B×B)\mathbf{v}_{\nabla B} = \frac{mv_\perp^2}{2qB^3}(\mathbf{B} \times \nabla B)

This drift depends on the sign of the charge, so electrons and ions drift in opposite directions.

When magnetic field lines are curved, particles experience a centrifugal force that causes:

vc=mv2qB2Rc×BRc2\mathbf{v}_c = \frac{mv_\parallel^2}{qB^2}\frac{\mathbf{R}_c \times \mathbf{B}}{R_c^2}

where Rc\mathbf{R}_c is the radius of curvature vector and vv_\parallel is the velocity parallel to B\mathbf{B}.

In vacuum magnetic fields, these drifts often occur together. The combined drift can be written as:

vgc=mqB3(v22+v2)B×B\mathbf{v}_{gc} = \frac{m}{qB^3}\left(\frac{v_\perp^2}{2} + v_\parallel^2\right)\mathbf{B} \times \nabla B

When a charged particle moves along a magnetic field that increases in strength, it experiences a force opposing its motion:

F=μBF_\parallel = -\mu \nabla_\parallel B

where μ=mv22B\mu = \frac{mv_\perp^2}{2B} is the magnetic moment, an adiabatic invariant.

A particle is reflected (mirrored) if it enters a region where:

B>B0v2v2B > B_0 \frac{v^2}{v_\perp^2}

The mirror ratio R=Bmax/BminR = B_{max}/B_{min} determines the trapping condition. Particles with pitch angle α\alpha (angle between velocity and magnetic field) satisfying:

sin2α>1R\sin^2 \alpha > \frac{1}{R}

will be trapped between mirrors.

Particles that are not trapped escape through the “loss cone” in velocity space. In tokamaks, this effect creates trapped and passing particle populations that behave differently.

The small Larmor radius compared to device size (by factor of 10310410^3-10^4) is what makes magnetic confinement possible. Particles are “tied” to magnetic field lines.

The gradient-B and curvature drifts in a purely toroidal field would cause vertical separation of electrons and ions, leading to charge accumulation and loss. This is why the poloidal magnetic field component is essential in tokamaks.

In tokamaks, trapped particles execute “banana” shaped orbits due to the combination of parallel motion, mirror reflection, and drifts. The banana width:

ΔbqρLε\Delta_b \approx \frac{q \rho_L}{\sqrt{\varepsilon}}

(where qq is the safety factor and ε\varepsilon is the inverse aspect ratio) is larger than the Larmor radius and affects transport.

Understanding cyclotron motion enables resonant heating methods:

  • Ion cyclotron resonance heating (ICRH) at ωci\omega_{ci}
  • Electron cyclotron resonance heating (ECRH) at ωce\omega_{ce}