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Drift Motions

Source lecture(s): pc368_lec07_drift

Intuition

A charged particle gyrates rapidly around a magnetic field line. If the field has a gradient, or if there is an electric field perpendicular to B, the center of the gyration orbit moves slowly across B. These drift motions govern particle transport in non-uniform magnetized plasmas.

Formal Definition

A drift is the guiding-center motion perpendicular to the local magnetic field. For slowly varying fields (\(\omega/\Omega_c \ll 1\)) and \(v_\perp, v_\parallel\) constant over a gyroperiod, the average velocity is:

\[\mathbf{v}_d = \frac{\mathbf{F} \times \mathbf{B}}{q B^2}\]

where \(\mathbf{F}\) is any external force.

Mathematical Formulation

  1. \(\mathbf{E}\times\mathbf{B}\) drift:

$\(\mathbf{v}_{E\times B} = \frac{\mathbf{E}\times\mathbf{B}}{B^2}\)$

Independent of charge and mass.

  1. Gradient drift:

$\(\mathbf{v}_{\nabla B} = \frac{m v_\perp^2}{2 q B^3} (\mathbf{B} \times \nabla B)\)$

  1. Curvature drift:

$\(\mathbf{v}_c = \frac{m v_\parallel^2}{q B^3} \bigl[\mathbf{b} \times (\mathbf{b}\cdot\nabla)\mathbf{b}\bigr]\)$

  1. Gravity drift:

$\(\mathbf{v}_g = \frac{m \mathbf{g} \times \mathbf{B}}{q B^2}\)$

Derivation

Use the guiding-center expansion:

  1. Decompose \(\mathbf{r} = \mathbf{R} + \boldsymbol{\rho}\), where \(\mathbf{R}\) is the guiding center and \(\boldsymbol{\rho}\) is the gyration vector.
  2. Slow fields: \(\mathbf{E}(\mathbf{R}), \mathbf{B}(\mathbf{R})\).
  3. Average the Lorentz force over one cyclotron period.
  4. The drift velocity emerges from the \(\mathbf{E}\times\mathbf{B}\) advection and the polarization drift from time-varying E.

For the gradient drift, note that the orbital radius \(\rho_L = m v_\perp/|q|B\) changes as \(B\) varies, giving an net orbital excursion proportional to \(\nabla B\).

Worked Example

Tokamak ion gradient drift: In a tokamak with circular cross-section, the toroidal field \(B_\phi \sim 1/R\) has a gradient toward the center. Compute the drift direction for a co-going ion (\(v_\parallel\) along \(\hat{z}\)). Using \(\mathbf{v}_c \propto m v_\parallel^2 B^{-3}(\mathbf{b}\times\kappa)\), the curvature vector points outward (\(+\hat{r}\)), so the drift is vertically upward for ions (\(q>0\)).

Common Mistakes

  • Drift speed is set by \(v_\perp\) or \(v_\parallel\). Confusing them gives wrong scaling.
  • Drifts are NOT caused by \(\mathbf{E}\) alone. The gradient and curvature drifts persist even in vacuum B-fields.
  • Polarization drift is order \(\omega/\Omega_c\). It is often small but becomes important in time-dependent problems.

Quiz Questions

  1. Conceptual: Why do electrons and ions drift in the same direction under \(\mathbf{E}\times\mathbf{B}\) but in opposite directions under \(\nabla B\)?
  2. Computational: For a \(\nabla B\) drift in \(B = 1\) T with gradient \(\nabla B/B = 0.1/m\), find \(v_{\nabla B}\) for 1 keV protons with \(v_\perp = v_\parallel\).
  3. MCQ: Which drift is independent of the particle’s charge?
  4. A) \(\mathbf{E}\times\mathbf{B}\)
  5. B) Gradient
  6. C) Curvature
  7. D) Gravity

Further Reading

  • W. Baumjohann & R. A. Treumann, Basic Space Plasma Physics.