**A Student Survives the Exam:
A Counter-Intuitive Particle Drift Problem**

Greg Hammett and Nat Fisch.

April 26, 2001 Draft

This is an intriguing little particle drift problem which is counter-intuitive at first to many people. To be a successful physicist, one needs to be able to think slowly--carefully and slowly.

The dialogue below is a composite (not meant to be any actual student) based on our experience in giving this problem to students in the introductory graduate course in plasma physics and in general oral exams (but we only gave it in the later stages of oral exams to students who were doing well, to try to avoid unncesessarily shaking their confidence).

The motion of particles in magnetic and electric fields is of course basic (but fundamental) physics. Understanding such motion is important for having good intuition, not just about various fusion plasma devices and astrophysical plasmas, but also about particle detectors and accelerators, microwave generators and plasma thrusters, and various electronic devices. In plasma physics (and in the dialogue below), we often make use of an implied guiding center approximation, in which the radius of gyration of a particle is small and one can consider the slower drifts of the ``guiding center'' about which the particle gyrates.

The problem:

Consider the magnetic field produced by a small ring of current enclosing thezaxis. The magnetic field far from the ring has a dipole structure, so on the midplane , whereRis the distance from the ring. Consider a small gyroradius particle deeply trapped (the component of the velocity parallel to is small) in this dipole magnetic field (this is similar to a particle that is trapped near the equatorial plane of the earth's magnetosphere). Sketch the particle's orbit (which the student does as follows, to illustrate the gyromotion, the bounce-motion, and the precession due to grad-B/curvature drifts).

The current in the ring is now slowly increased. Does the energy of the particle go up or down? (You can consider the limit to simplify the analysis.)

The eager young student assumes this is one of those simple ``quicky'' problems and says, ``well, assuming that the current in the ring changes slowly compared to the cyclotron period of the particle, then the magnetic moment of the particle is an adiabatic invariant. Since , the energy of the particle must go up because the magnetic field goes up.''

Then the examiner asks, ``Is that your final answer?'', and the fun begins.

Trying to be helpful, the examiner asks where *B* is evaluated in this
formula for . But the student just says ``at the guiding center
position'', and doesn't see at first why this would change the answer. The
examiner next asks, `What are the invariants of the motion?'' The student
replies, ``*E*, , and ,--no wait, that would mean that the
energy *E* is fixed. Sorry, those are the constants of the motion only in
static fields. With time-varying fields, there are the first, second, and
third adiabatic invariants, corresponding to , to the bounce motion
along the field line, and to the particle's precessional drift around the z
axis. But we are taking the limit of so the bounce motion is
probably irrelevant.'' Then the student asks, ``can we assume that the
magnetic field is changing slowly compared to the precession frequency of
the particle so that the third adiabatic invariant is conserved?''. She is
assured that yes, the problem states that the magnetic field is changing
slowly, so she can assume it is slow even compared to the precession
frequency.

Then the student explains the physics of the third adiabatic invariant
(using this to buy time to think about the problem and see if she missed
something). ``The third adiabatic invariant is similar in a way to the
first adiabatic invariant. The first adiabatic invariant corresponds to
conservation of magnetic flux inside the small gyroradius of the
particle. Because of the particle's rapid gyromotion, it can essentially be
treated as a small, ideally-conducting ring of current, which must conserve
the magnetic flux going through the ring (assuming the magnetic field is
changing slowly compared to the cyclotron period). It accomplishes this
conservation of flux by adjusting its gyroradius. (The general
interpretation of adiabatic invariants is what Einstein called
conservation of ``action'', but in our case we can think of them as related
to conservation of magnetic flux inside an ideally conducting loop). So
too the third adiabatic invariant corresponds to conservation of magnetic
flux inside the region enclosed by the particle as it undergoes grad-B and
curvature drifts around the *z*-axis. [These drifts are what cause the
precession around the earth of energetic particles trapped in the earth's
magnetosphere.] ''

``In this problem, since the magnetic field is everywhere going up, in
order for the precessional drift to enclose the same amount of magnetic
flux, the particle's orbit around the *z*-axis must shift in to smaller
*R*. So the energy () of this particle goes up even faster than I
first thought.''

But the examiner counters, ``shouldn't the particle also conserve the
amount of flux outside of its orbit?'' This is a bit disconcerting at
first. People don't usually talk about the flux outside of a loop. But
since , the flux outside of a loop must exactly
balance the flux inside of a loop, so the two ways of looking at it must be
equivalent. ``Yes,'', the fast-thinking student agrees, ``the flux outside
of its orbit should be conserved also.'' But if this is true, then as the
magnetic field increases, the particle's precession orbit would have to
expand to larger *R* to conserve this flux. The student knows there must
be a solution to this conundrum, and, after pondering for a moment,
realizes that she had forgotten about the magnetic flux coming up through
the center of the current ring, which has the opposite sign of the magnetic
flux coming down outside of the ring. The student now realizes that it
must be that as the current in the ring is increased and the magnetic field
everywhere is increased, then the particle's orbit must actually expand to
conserve the amount of flux outside (or inside) of its orbit.

Doing a quick blackboard calculation of the amount of magnetic flux outside
of the particle's orbit, assuming it is at large enough *R* that a dipole
approximation is accurate, the student finds that,
although *B* everywhere is going up, the particle moves far enough
out at the same time that the *B* it sees actually drops.

Thus the student arrives at the unsettling conclusion that even though the magnetic field everywhere went up, the particle's energy actually goes down.

Being a little unsure of this result, the student looks for a simpler
explanation to make sure it's true, saying ``I suppose another way of
looking at this is to consider the fact that the time-changing magnetic
field induces an electric field in the direction which would then
lead to an drift of the particle''. Doing a quick
calculation, the student verifies that indeed the sign of this
drift is outwards. ``I probably should have thought of this from the start
(meaning the fact that the particle doesn't stay at fixed *R* but moves
outwards), because the velocity can be thought of as the
velocity at which magnetic field lines move (related to the fact that
particles and magnetic fields move together in the ``frozen-in field
lines'' condition of ideal MHD). Increasing the current in the central
ring means that additional magnetic field lines are being generated and the
other magnetic field lines must move outwards to maintain magnetic force
balance.''

[In our experience, about half of the students have their intuition
backwards about which direction the magnetic field lines move as the
current in the dipole ring increases. They seem to think that since
magnetic field lines must move closer together in order for the magnetic
field strength to go up, the field lines must all squeeze in closer to the
dipole ring at the origin. But this would require a source of magnetic
field lines at infinity, and neglects the fact that every field line that
comes down through the midplane at large R also comes back up through the
midplane inside of the ring. The right way to think about this is to
realize that magnetic fields are being generated at the surface of the
current ring, and must then move outwards. This of course must be true to
satisfy causality: if you suddenly change the current in the ring, the
magnetic fields at large *R* can't change until at least the time it would
take for light to propagate that distance. Because our intuition can
sometimes be wrong, it is good to be able to check the answer in multiple
ways, as the student did here by calculating the drift and the
flux outside of the particle's orbit.]

Thus the student has arrived at the startling conclusion that, even though
the magnetic field everywhere went up and is conserved, the
particle's energy actually goes down, because it moves outwards to a region
of lower *B* faster than the *B* at a fixed position is increasing. The
examiner, being satisfied with the depth and carefulness of the student's
answers to this problem, now moves on to the next problem.

Thu Apr 26 19:03:54 EDT 2001