Only depends on position. Taking the curl,
The field reverses across . Its divergence is zero, as required for a magnetic field; the vanishing field on the midplane is important for the crossing and separatrix trajectories below.
With zero scalar potential, the nonrelativistic charged-particle Lagrangian in SI units is kinetic energy plus . Thus
The velocity-dependent magnetic term changes canonical momentum but does not contribute to the mechanical energy.
Define . Differentiating the Lagrangian with respect to each generalized velocity gives
The coordinates and are cyclic, so and are conserved. The momentum is generally not conserved: its equation is . In particular, conserved canonical is not the same as conserved mechanical , which changes as the particle moves across the magnetic-field gradient.
The Legendre transform cancels the term linear in velocity and gives
It equals the mechanical kinetic energy. The Hamiltonian has no explicit time dependence, so is conserved. This is also a direct consequence of the magnetic force doing no work: .
Since initially and remains constant, the motion stays in a plane of constant . Setting and gives
The allowed interval obeys . The sign of is set by the initial direction and changes at a turning point. The specified fixes the starting position on the energy orbit, but the data do not specify which sign of the initial transverse velocity is chosen.
Dividing the two velocities gives
Here : the orbit always advances toward increasing , except for instantaneous zeros at each midplane crossing . The transverse motion oscillates between and . At these outer turning points and the trajectory is tangent to the direction; at the midplane while , so the tangent is along . The sign of the initial only chooses the phase or reflected trace.
Figure 1.
Crossing and separatrix orbits in a reversing magnetic field
. The left panel shows the orbit with zero conserved axial canonical momentum, advancing monotonically in z. The right panel shows a positive-x separatrix with the negative extreme canonical momentum; its arrows and marked axial-velocity zeros distinguish it from an ordinary periodic orbit. Both panels use dimensionless coordinates. Details.
With , the allowed range is , where . But an orbit starting with never crosses the midplane in finite time, because
One positive-side separatrix, with and , is
The negative-side orbit is its reflection in . For the positive branch, rises from zero asymptotically, reaches at , then returns asymptotically to zero. Thus the infimum is zero but it is not attained in finite time on this nontrivial branch. Since , the two axial-velocity zeros occur at . Motion is toward decreasing near either asymptotic midplane tail and toward increasing near the outer excursion. These directions are marked in part i.
The exactly midplane initial state , is a separate straight trajectory with ; it must not be described as a finite-time crossing of the separatrix.

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