next up previous
Next: Magnetic Mirrors: the effects Up: Single Particle Motions: ``Orbit Previous: Applications

Adiabatic invariants

For periodic motions the theory of mechanics shows that quantities called actions can remain invariant for slow changes in the system. An action J can be defined in terms of generalized coordinates qgen and conjugate momenta pgen by

\begin{displaymath}J = \oint p_{gen} d q_{gen} \ ,
\end{displaymath} (2.31)

where the integral is over one period of the motion. A particle's gyromotion is one example of a periodic motion amenable to the construction of an approximate constant of the motion (or invariant). Defining qgen to be the gyrophase $\phi$, then the angular momentum $p_{gen} = l = m v_{\perp} r_{L}$ is the conjugate momentum. Inserting these variables into (2.31) and integrating one finds

\begin{displaymath}J = 2\pi \frac{m}{q} \frac{v_{\perp}^{2}}{B} = \frac{4\pi m}{q} \mu
\end{displaymath} (2.32)

for slowly varying B. The quantity

\begin{displaymath}\mu = \frac{v_{\perp}^{2}}{2 B}
\end{displaymath} (2.33)

is known as the first adiabatic invariant of a plasma particle. This implies that a particle's perpendicular energy $W_{\perp} = 1/2 m v_{\perp}^{2}$ is proportional to B if $\mu$ is constant.

Another, perhaps more obvious derivation of the first adiabatic invariant is as follows. Assume that the particle sees a small change in ${\bf B}$ during a gyroperiod, whether due to temporal or spatial variations in ${\bf B}$. I.E.,

\begin{displaymath}\frac{1}{\Omega_{c}} \vert \frac{\partial B}{\partial t} B^{-1} \vert \ll 1 \ .
\end{displaymath} (2.34)

The change in $W_{\perp}$ in one gyroperiod is
$\displaystyle \Delta W_{\perp}$ = $\displaystyle q \oint {\bf E} . {\bf d}l$ (2.35)
  = $\displaystyle \frac{1}{c} \frac{\partial }{\partial t} \left( q \int_{S} {\bf B} . d{\bf S} \right) \ .$ (2.36)

Assuming the orbit size changes very little in one gyroperiod then

\begin{displaymath}\Delta W_{\perp} \approx q \pi r_{L}^{2} \frac{1}{c} \frac{\partial B}{\partial t} .
\end{displaymath} (2.37)

Since the change in B in one gyroperiod is

\begin{displaymath}\Delta B = \frac{2\pi}{\Omega_{c}} \frac{\partial B}{\partial t}
\end{displaymath} (2.38)

then $\Delta W_{\perp} = W_{\perp} \Delta B / B$ or

\begin{displaymath}\Delta \left( \frac{W}{B} \right) = 0 = \Delta( \mu )\ .
\end{displaymath} (2.39)

That is, $\mu$ is a constant.

Other adiabatic invariants also exist. The second or longitudinal adiabatic invariant is associated with the periodic bouncing of particles in magnetic flux tubes and magnetic bottles:

\begin{displaymath}J_{L} = m \oint v_{\parallel} d z
\end{displaymath} (2.40)

A third adiabatic invariant can be associated with the periodic drift of a particle (due to $\nabla B$ and curvature drifts) around a dipole magnetic field. It is useful for studying particle motions in Earth's magnetosphere but is not addressed further here.


next up previous
Next: Magnetic Mirrors: the effects Up: Single Particle Motions: ``Orbit Previous: Applications
Iver Cairns
1999-08-04