Electromagnetism

The field outside the solenoid, which is not zero

Ampère's law says the field outside a solenoid vanishes, and every step of that argument is exact — for a winding of infinite length. A real one is a bar magnet seen from outside, its external field falls as the inverse square of its length rather than to nothing, and the "exactly zero" that makes the derivation so satisfying is the one part of it a laboratory cannot have.

Assumes: The field that wraps a current · The field with no ends, and the force that does no work

The derivation is one of the tidiest in the subject. Take a rectangular loop with one side inside the solenoid and one outside, apply Ampère’s law, note that the two short sides contribute nothing because the field there is perpendicular to them, and conclude that the difference between the inside and outside fields is μ0nI\mu_0 n I. Then argue that the outside field must fall to zero far away and is the same everywhere outside by symmetry, so it is zero everywhere outside, so the inside field is μ0nI\mu_0 n I and is uniform.

Nothing in that is wrong. It is a proof about an object that does not exist.

Every line that goes in has to come out. Field lines of a 5:1 solenoid in the plane through its axis, each traced by stepping along the local direction of a field summed turn by turn from Biot–Savart. Inside the winding they are parallel and evenly spaced, which is the picture the textbook argument is about. Outside they are not absent: they are spread over the whole of the rest of space, which is why the field there is small — 1.60e-2 of the centre value at 2 radii off the axis — and why it cannot be zero. A line has no end, so every one of the lines through the bore returns outside, and a field with no outside would be a field whose lines stop.
Fig. 1 The field of a solenoid five times as long as it is wide, traced by stepping along the direction of a field summed turn by turn from Biot–Savart, with no Ampère’s law used anywhere. Inside, the lines are parallel and evenly spaced, which is the picture the derivation is about. Outside, they are not missing: they are spread over the whole of the rest of space, which is why the field there is small — 1.6 × 10⁻² of the centre value two radii off the axis — and exactly why it cannot be zero. A field line has no end, so every line through the bore has to come back somehow.

This essay computes what a finite winding actually does, and the interest is not that the textbook answer is wrong. It is that the three quantities the answer is usually quoted with — zero outside, uniform inside, half at the mouth — approach their ideal values at three different rates, and one of them cannot approach it at all without destroying the thing that makes a solenoid a magnet.

Where the infinity gets in

The rectangular-loop argument uses Ampère’s law twice, and Ampère’s law is exact both times. What it also uses, silently — as every symmetry argument in electrostatics does, is that the field outside is the same at every distance — otherwise a loop entirely outside the winding, with its two long sides at different radii, would enclose no current and yet return a nonzero circulation.

Four paths, one answer. The field of a straight wire carrying 10 A, summed step by step around four closed paths in 4000 pieces each. Three of them enclose the wire and each returns 12.566 µT·m, which is μ₀I; the fourth does not enclose it and returns zero, because the outward stretch of the path and the return stretch cross the same field lines in opposite senses. Nothing about the shape survives into the answer — not the radius, not the centring, not the corners — which is what makes the law usable and also what makes it useless without a symmetry to hand.
Fig. 2 The law itself, on the case where it does everything asked of it. Four different closed paths round one straight wire, with the circulation of B summed along each: all four return μ₀I to five decimal places, and nothing else about the path survives into the answer. That indifference to the path is what makes the law so powerful and also what makes it so easy to misuse — it constrains one number per loop, and turning one number into a field everywhere requires a symmetry argument that the law itself does not supply.

That sameness is a translation symmetry along the axis, and a finite winding does not have it. Slide a rectangular loop along a real solenoid and the field it encloses changes, because the loop gets nearer an end. So the step that turns “the difference between inside and outside is μ0nI\mu_0 nI” into “the outside is nothing” is the step that assumes the answer, and it is available only in the limit.

It is worth being precise about where the residue outside comes from, because “the field cancels” is the sentence that does the damage. Each turn on its own makes a field that wraps it, and outside the winding the contributions from neighbouring turns point in nearly opposite directions. Nearly, and not exactly: the cancellation between a turn and its neighbour is a subtraction of two large numbers that differ slightly, because the two turns are at slightly different distances from the point being asked about. What survives is a small residue rather than nothing, and it is largest near the ends, where a turn has a neighbour on one side only and so has nothing to cancel against on the other. That is the whole mechanism, and it is why the leak is an end effect: the middle of a long winding really is quiet, and the mouths are where the field gets out.

The flux has to come back

The rectangular-loop argument uses one of the four equations and never touches the one that settles the question. B=0\nabla\cdot\mathbf{B}=0 says the flux out of any closed surface is nothing at all. Wrap a cylinder round the middle of the winding, its two flat lids far out along the axis on either side and its curved wall at some radius outside the turns. The lids sit where the field has already become a dipole’s, falling as the inverse cube while their area grows only as the square, so what crosses them can be made as small as one likes by pushing them further out. Everything else leaves through the wall.

That is a conservation law, and it fixes a quantity rather than a shape. The flux running up the bore at the middle is BcentreπR2B_{\text{centre}}\pi R^2 — for a 5:1 winding, 0.9806μ0nI0.9806\,\mu_0 n I times the bore area — and every line of it is outside the winding somewhere. The aspect ratio decides how much room that return has, and nothing else. Lengthening a coil deletes no line; it hands the same bundle a longer object to get round, so the same flux is spread over more of the wall and the field at any one place on it is smaller. An inverse square is what that spreading looks like when it is written down, which is why the exponent measured below is a piece of geometry rather than a fitted curiosity.

The infinite solenoid escapes the constraint by having no outside in the sense that matters. Its return path has been sent to infinite radius, where unlimited room holds a finite flux at zero density, and a field of zero over an infinite area is a perfectly good way to carry μ0nIπR2\mu_0 n I \pi R^2. That is a legitimate limit and it is not a small idealisation: it is the whole of the difference between the derivation and the object. The same accounting is what makes a field’s energy something stored in space rather than in the wire, and the energy outside a real winding is the same flux counted a second way.

What the sum gives on the axis

Nothing below uses Ampère’s law. Each turn is a circular current, its field at a point is Biot–Savart integrated round the ring, and the winding’s field is the sum. On the axis the result can be checked against a closed form got by integrating the single-loop expression along the winding — a route that shares no arithmetic with a sum of three-dimensional cross products — and the two agree to five hundredths of a per cent.

The end of the winding is where the field is half. Field on the axis of a solenoid, in units of the infinite-solenoid value μ₀nI, with distance measured in half-lengths so that ±1 is the mouth of the winding whatever its length. At 1:1 the centre reaches 0.7075 of μ₀nI and the end plane 0.4472, a ratio of 0.6322; At 2.5:1 the centre reaches 0.9285 of μ₀nI and the end plane 0.4903, a ratio of 0.5280; At 5:1 the centre reaches 0.9806 of μ₀nI and the end plane 0.4975, a ratio of 0.5074; At 10:1 the centre reaches 0.9950 of μ₀nI and the end plane 0.4994, a ratio of 0.5019. Every point is a sum of Biot–Savart contributions from each of the turns, and the centre value agrees with the closed form for a continuous winding to 0.049 per cent. The half is exact only in the limit: a winding as long as it is wide gives 0.63, and the familiar rule is a statement about a solenoid nobody has.
Fig. 3 Field on the axis, in units of μ₀nI, with distance in half-lengths so that ±1 is the mouth whatever the length. The centre value approaches μ₀nI from below — 0.7075 at 1:1, 0.9285 at 2.5:1, 0.9806 at 5:1, 0.9950 at 10:1 — so even the famous interior value is an approximation, and a short coil is fifteen per cent under it. The end-plane value approaches half the centre value from above: 0.632, 0.528, 0.507, 0.502.

Two familiar statements come out of that figure with their conditions attached.

“The field inside is μ0nI\mu_0 n I is good to a per cent at five to one and to five parts in a thousand at ten to one. It is a statement about the middle: near the mouth the field is falling, and it has fallen to half by the time it reaches the end plane.

“The field at the end is half the field in the middle” is exact only in the limit and approached from above. At one to one it is 0.632, which is not half by any reading. The reason the half is so nearly right so quickly is that it comes from a symmetry rather than from a size: at the end plane the winding subtends a solid angle on one side and nothing on the other, so a long solenoid’s end sees exactly half of what its middle sees.

The end of the winding is where the field is half. Field on the axis of a solenoid, in units of the infinite-solenoid value μ₀nI, with distance measured in half-lengths so that ±1 is the mouth of the winding whatever its length. At 0.5:1 the centre reaches 0.4476 of μ₀nI and the end plane 0.3537, a ratio of 0.7902; At 1:1 the centre reaches 0.7073 of μ₀nI and the end plane 0.4472, a ratio of 0.6323; At 20:1 the centre reaches 0.9988 of μ₀nI and the end plane 0.4998, a ratio of 0.5005. Every point is a sum of Biot–Savart contributions from each of the turns, and the centre value agrees with the closed form for a continuous winding to 0.080 per cent. The half is exact only in the limit: a winding as long as it is wide gives 0.63, and the familiar rule is a statement about a solenoid nobody has.
Fig. 4 The same construction taken to both extremes. At 0.5:1 the object is a thick pancake of wire and the “plateau” is a single rounded peak reaching 0.447 of μ₀nI, with no uniform region anywhere in it; at 20:1 the plateau is flat to a part in a thousand across most of the length. The transition between those two pictures is entirely a matter of aspect ratio, and nothing about the current, the winding density or the radius appears in it separately.

Outside: not zero, and falling as the inverse square of the length

The quantity the derivation gets most wrong is the one it is most confident about. Sampling the mid-plane at a fixed number of radii off the axis, and asking how the field there depends on how long the winding is, gives a power law rather than a vanishing.

Outside the winding the field is small, and it is not zero. The field 2 radii off the axis, at the mid-plane, as a fraction of the field at the centre of the same solenoid, against the winding's aspect ratio, on logarithmic axes. At 1:1 it is 7.34e-2; At 2.21:1 it is 4.61e-2; At 4.9:1 it is 1.66e-2; At 10.8:1 it is 4.07e-3; At 24:1 it is 8.59e-4. The fitted exponent beyond 6:1 is -1.918 and the local slope between the last two points is -1.967, so it is on its way to −2 rather than at it. That is the two-pole answer: from outside, a solenoid is a pair of ends of fixed strength B∞πR²/μ₀, and at the mid-plane each of them is a distance L/2 away, which needs the probe to be near the mid-plane compared with the length before it holds. Nothing here ever reaches zero — the textbook exactness is a limit, and a 24:1 winding realises it to about a part in a thousand.
Fig. 5 Field two radii off the axis at the mid-plane, as a fraction of the centre field, against aspect ratio, on logarithmic axes. It falls from 7.3 × 10⁻² at 1:1 to 8.6 × 10⁻⁴ at 24:1, with a fitted exponent of −1.918 beyond 6:1 and −1.967 between the last two points. The limit is −2, and the reason is a picture rather than an integral: from outside, a solenoid is two ends of fixed strength B∞πR²/μ₀, and at the mid-plane each of them is a distance L/2 away.

An inverse square is a slow way to reach zero. Doubling the length of a winding buys a factor of four in how quiet it is outside; getting from a part in a hundred to a part in a million takes a factor of a thousand in length. That is the honest cost of magnetic screening by geometry alone, and it is why real apparatus screens with iron or with a return path instead.

Outside the winding the field is small, and it is not zero. The field 4 radii off the axis, at the mid-plane, as a fraction of the field at the centre of the same solenoid, against the winding's aspect ratio, on logarithmic axes. At 1:1 it is 1.07e-2; At 2.51:1 it is 1.32e-2; At 6.32:1 it is 7.62e-3; At 15.9:1 it is 1.80e-3; At 40:1 it is 3.08e-4. The fitted exponent beyond 12:1 is -1.916 and the local slope between the last two points is -1.951, so it is on its way to −2 rather than at it. That is the two-pole answer: from outside, a solenoid is a pair of ends of fixed strength B∞πR²/μ₀, and at the mid-plane each of them is a distance L/2 away, which needs the probe to be near the mid-plane compared with the length before it holds. Nothing here ever reaches zero — the textbook exactness is a limit, and a 24:1 winding realises it to about a part in a thousand.
Fig. 6 The same measurement four radii out rather than two, and over a longer range of windings, because the two-pole picture needs the probe to be close to the mid-plane compared with the length: the fitting window starts at 12:1 here rather than 6:1, and the generator refuses to fit outside it. The exponent comes back the same, −1.916, while every value is smaller — 3.1 × 10⁻⁴ at 40:1. What the two figures together say is that the outside field has two independent knobs, how far away and how long the winding is, and the textbook derivation sets the second to infinity and then reports the answer as though it were about the first.

Quieter nearby, louder far away

The two measurements this essay makes outside the winding pull in opposite directions, and the pull is worth stating plainly, because “a longer solenoid leaks less” is true only in the region where it was measured.

At the mid-plane, a couple of radii off the axis, the field falls as L2L^{-2}. Far away on the axis, the same winding is a point dipole of moment NIπR2NI\pi R^2; at a fixed turn density N=nLN = nL, so the moment is proportional to the length, and a dipole’s field at a fixed distance is proportional to its moment. Doubling the length of a winding at constant nn, II and RR therefore divides the near-outside field by four and multiplies the far field by two. Both numbers are in the figures above, arrived at independently, and neither is a correction to the other.

There is no contradiction because there is one conserved quantity behind both. The return flux is being reshaped and not removed. Pushing it further from the mid-plane is what makes the near outside quiet; stretching the two ends further apart is precisely what makes the dipole moment large. So a coil built to be magnetically inconspicuous is built against a distance, and the distance has to be named before the design question means anything. The measurement two radii out and the measurement forty lengths out are not two estimates of one number.

The crossover between them is where the probe stops being close compared with the length and starts being far. The second leak figure shows its near edge directly: at four radii out the two-pole fit does not begin until 12:1, where at two radii it began at 6:1, because what the fit needs is ρL\rho \ll L. That the generator refuses to fit outside its window rather than returning a number is the same discipline a falloff exponent needs everywhere — an exponent read off the wrong range of distances is a measurement of the range.

Every line that goes in has to come out. Field lines of a 1.2:1 solenoid in the plane through its axis, each traced by stepping along the local direction of a field summed turn by turn from Biot–Savart. Inside the winding they are parallel and evenly spaced, which is the picture the textbook argument is about. Outside they are not absent: they are spread over the whole of the rest of space, which is why the field there is small — 6.87e-2 of the centre value at 2 radii off the axis — and why it cannot be zero. A line has no end, so every one of the lines through the bore returns outside, and a field with no outside would be a field whose lines stop.
Fig. 7 And the field of a winding barely longer than it is wide, where the “small” outside field is 6.9 × 10⁻² of the centre — one part in fifteen. The lines through the bore turn round within a couple of radii and the object is visibly a bar magnet with a hole in it. This is the same generator, the same physics and the same code as the 5:1 picture at the top; only the aspect ratio has changed.

What the loop argument does prove

Throwing the derivation away would be the wrong lesson, because the rectangular loop still constrains a finite winding. It constrains it more weakly, and the weaker statement is exact.

Take a closed loop lying entirely outside the winding, enclosing no turns. Ampère’s law returns zero circulation round it, for a real solenoid of any length whatever. That is not a claim that the field vanishes. It is a claim that the external field is conservative — that throughout the current-free region it is the gradient of a single scalar, in the way an electrostatic field is, so that one number at every point carries all of it. Which is what licenses the two-end picture used above: poles are sources of a potential, and without the circulation result there would be no potential for them to be sources of.

What the infinite case adds on top is the translation symmetry, and the symmetry is doing all of the remaining work. It says the gradient cannot depend on where along the axis it is measured, and a gradient that is the same everywhere and dies at large radius is zero everywhere. Remove the symmetry and the first half survives untouched while the second half has nothing left to stand on. A finite solenoid still has a scalar potential outside it. The potential simply has structure, and the structure is the two ends.

That is the standard shape of the mistake, and it is not particular to magnetism: the law is exact, the symmetry is an extra assumption smuggled in beside it, and the sentence that fails is the one after the law rather than the law itself. Gauss’s law has the same character — true for every charge distribution there is, and useful only where something independent of it says the field is constant over the surface.

Far away it is exactly a dipole, and that is the point

Follow the axis out past the end and the winding’s identity dissolves into a single number.

Far enough away it is a bar magnet, and nothing else. Field on the axis beyond the end of a 5:1 solenoid, against distance from its centre, on logarithmic axes, with a point dipole of the same magnetic moment NIπR² drawn beside it. The two agree to 0.08 per cent beyond forty solenoid lengths, and the fitted exponent of the summed field there is -3.001. Whatever the winding is doing inside itself, from far enough away it has exactly one number: its moment. That is the same statement as the outside field not being zero — a solenoid with no external field would have no moment either, and could not be a magnet.
Fig. 8 Field on the axis beyond the end of a 5:1 solenoid, against a point dipole of moment NIπR², on logarithmic axes. Beyond forty solenoid lengths the two agree to 0.08 per cent and the fitted exponent of the summed field is −3.001. Whatever the winding is doing inside itself, from far enough away it has exactly one property, and that property is the same one a current loop has.

This is where the “confinement” claim and the “it is a magnet” claim collide. A magnetic moment is defined by the far field, in the way a dipole’s own lines define it; a body with no external field has no moment; a body with no moment feels no torque in an applied field and exerts none on anything else. So a solenoid that really had zero field outside could not be used as a magnet at all — could not deflect a compass, could not attract iron, could not be weighed in a gradient. The external field is not a leak from an otherwise perfect device. It is the device’s output.

A torque, and no force at all. A loop of 1 turn enclosing 20 cm² and carrying 10 A has a magnetic moment of 0.02 A m². In a uniform field of 0.05 T the torque on it is m B sin θ, drawn here against the angle between the moment and the field: zero when they are aligned, largest at 0.001 N m across, and zero again when they are opposed. The second curve is the energy, −m·B, whose minimum is the aligned position and whose maximum is the opposed one — which is why a compass needle settles one way round and not the other. The net force is zero at every angle on this axis, exactly and not approximately: the force is I dl × B summed round the loop, the sum of dl round any closed path is zero, and a constant B comes outside the sum. The inset shows the four forces on a rectangular loop; the pair across the axis is the couple, and the pair along it cancels.
Fig. 9 The moment itself, as a torque. A loop of area A carrying I in a field B feels a torque IAB·sinθ, which is what defines the moment IA and is what a compass needle responds to. A solenoid of N turns is N such loops in series, so its moment is NIA — the same number that appeared in the far-field comparison above, arrived at from a torque rather than from a distance.

What the ideal picture is still for

None of this makes the infinite solenoid a bad idealisation. It makes it a good one with a stated domain, which is the more useful object.

Start from a single loop and the point makes itself. One loop’s field is a dipole almost everywhere: there is no interior region where anything is uniform, and no aspect ratio to improve, because a loop has no length to be long compared with. Stacking loops is the entire manoeuvre, and what it buys is the uniform interior. What it does not buy, at anything like the same rate, is the absence of an exterior. The uniformity arrives long before the outside field becomes negligible — at five to one the interior is already within two per cent of μ0nI\mu_0 nI while the exterior is still 1.6 per cent of the centre value — so a winding that is plainly “long enough” by the measure a designer usually has in mind is nothing of the kind by the other.

The two errors have different sizes and different signs, and knowing which matters decides the design. Both fall as roughly the inverse square of the aspect ratio — the interior shortfall runs 0.29, 0.019, 0.0050, 0.0013 at 1:1, 5:1, 10:1 and 20:1, and the exterior field runs 0.073, 0.017, 0.0041, 0.00086 — so a winding built long enough for one purpose is usually long enough for the other, and the design question is which of the two numbers the application can actually afford. What no amount of care in the winding changes is the exponent. Screening by length alone is an inverse square, and an inverse square is a slow road to a part in a million. A coil that has to produce a known field inside — a calibration coil, a magnetic-resonance bore, a Zeeman slower — cares about the interior number and can reach a part in a thousand at 20:1. A coil that must not disturb something nearby cares about the exterior number, which at 20:1 is still a part in a thousand of the centre field and falls only as the square of any further lengthening.

There is a practical consequence when a winding has to share its flux with something else, and it is the same arithmetic seen from the other end. The flux rule relates the emf in a coil to the flux threading it, and it carries no term at all for flux that got away — so any line that leaves one winding without entering the other is simply absent from the calculation. On a transformer that absence has a name and a number: it is the leakage inductance, and its size is set by exactly the geometry measured above. The rule is not wrong about the coil it is applied to. It is silent about where the rest of the field went, which is a different failing and a harder one to notice, because nothing in the calculation is missing — the calculation is complete and describes a smaller object than the one on the bench.

The number that decides most designs is not either field on its own but the ratio between them, and that ratio is what an aspect ratio actually buys. At 5:1 the interior is within two per cent of μ0nI\mu_0 nI and the exterior two radii out is 1.6 per cent of the centre value, so the two are comparable; at 20:1 the interior shortfall is 0.0013 and the exterior 0.00086, so they have stayed comparable. Twenty-fold more winding has improved both by roughly the same factor and changed nothing about which of them dominates. A design that needs one of the two numbers three orders of magnitude better than the other cannot get there by lengthening at all, which is the practical content of the two errors sharing an exponent.

Where the model stops

Three limits, in increasing order of how easy they are to forget.

The winding is not a current sheet. Everything here treats each turn as a circular filament, which smooths the helical pitch away. A real helix carries a current along the axis as well as around it, and that component makes a field circling the solenoid outside — a component the sheet model has exactly zero of, and which does not fall with aspect ratio at all. It is cancelled in practice by a return wire brought back along the axis, which is why careful coils are wound that way.

The turns are evenly spaced. The uniformity of the interior is a statement about the winding density. A coil with a gap in it has a dip; a coil wound more densely at the ends can be made more uniform than an evenly wound one of the same length, which is the whole trick behind a compensated solenoid.

A “solenoid” long enough is a different object. The interior of a very long winding is uniform, and the ends are far away — but the field lines that leave one end still have to reach the other, and they do it through the whole of the surrounding space. The energy stored outside a 20:1 winding is a small fraction of the total and it is not a negligible one, and it is the reason the inductance of a finite solenoid is less than μ0n2V\mu_0 n^2 V: the standard correction, Nagaoka’s coefficient, is 0.92 at 5:1 and 0.98 at 20:1, and it is exactly the accounting for flux that does not thread every turn.

And nothing here has any matter in it. Put iron inside — a material whose own moments align, as a magnet’s do — and the interior field is no longer μ0nI\mu_0 nI but something set by the iron’s magnetisation, which is a material’s answer to a field rather than a geometric fact. The external field is then dominated by where the iron’s flux path goes, and the aspect-ratio argument above is replaced by a question about the magnetic circuit.

The end of the winding is where the field is half. Field on the axis of a solenoid, in units of the infinite-solenoid value μ₀nI, with distance measured in half-lengths so that ±1 is the mouth of the winding whatever its length. At 3:1 the centre reaches 0.9487 of μ₀nI and the end plane 0.4932, a ratio of 0.5199; At 6:1 the centre reaches 0.9864 of μ₀nI and the end plane 0.4983, a ratio of 0.5051; At 12:1 the centre reaches 0.9965 of μ₀nI and the end plane 0.4996, a ratio of 0.5013; At 24:1 the centre reaches 0.9991 of μ₀nI and the end plane 0.4999, a ratio of 0.5003. Every point is a sum of Biot–Savart contributions from each of the turns, and the centre value agrees with the closed form for a continuous winding to 0.00087 per cent. The half is exact only in the limit: a winding as long as it is wide gives 0.63, and the familiar rule is a statement about a solenoid nobody has.
Fig. 10 Four windings at a higher turn density, to show that the curve does not depend on it. Doubling the turns per radius doubles the field and changes none of the ratios: the centre approaches μ₀nI, the end plane approaches half of it, and the profile in units of μ₀nI is a function of aspect ratio alone. That is the sense in which the infinite solenoid is a limit rather than a special case — everything a finite one does is one number away from it.

The rung after this one

Ampère’s law has been used here on a static current and found to be exactly true and not quite enough. The next rung is the case where it is not exactly true: a current that stops, in a circuit with a gap in it, where two surfaces bounded by the same loop give two different answers. That contradiction has a repair, the repair adds a term, and the term turns four equations into a wave — which is the argument the neighbouring ladder starts from.

The difficulty never arose here because this essay’s solenoid was steady, and a steady current is the one case where the two surfaces cannot disagree. A solenoid being switched on has the problem in full — and it is worth carrying away that the field such a winding throws outside itself while switching is a great deal larger than the static residue computed here. Every number in this essay is a statement about a coil that has settled down.

Part 2 of 5

This essay is one argument about Ampere law. The others:

What links here

Essays that reach for this one mid-argument — the half of a link its own author cannot write down.

The objects named here

The third axis, after the field and the reading path: the things themselves, and every essay that touches each one.

Amperes lawBoundary conditionsDipole radiationField linesFluxIdealisationMagnetic fieldMagnetic fluxMagnetic momentSolenoidSuperpositionSymmetry