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Magnetic flux and flux density: HSC Physics Module 6

Syllabus dot point

“Describe how magnetic flux can be sensed by the changing alignment of a magnet on a compass needle and quantitatively analyse the concept of magnetic flux density B and flux Phi = B A cos theta in a magnetic field”

14 min read

Quick answer

Magnetic flux density BB is the local field strength (tesla, T = Wb/m2^2), and magnetic flux Φ=BAcos⁡θ\Phi = B A \cos \theta (weber, Wb = T m2^2) is the total field threading a surface of area AA whose normal lies at angle θ\theta to B⃗\vec{B}.

Jump to a section
  1. What this dot point is asking
  2. The answer
  3. Examples in context
  4. Exam-style questions
  5. Practice questions

What this dot point is asking

NESA wants you to distinguish magnetic flux density BB (the field at a point, in tesla) from magnetic flux Φ\Phi (the total field through a surface, in weber), apply Φ=BAcos⁡θ\Phi = B A \cos \theta correctly, and connect this concept to the qualitative idea of a compass needle responding to field direction. Flux is the bridge to Faraday's law in the next dot point.

The answer

Magnetic flux density B

The magnetic flux density (often just called the magnetic field) B⃗\vec{B} at a point is a vector describing the strength and direction of the magnetic field there. It is what a compass needle aligns with, and it determines the force on a moving charge (F=qvBF = qvB) or on a current (F=BILsin⁡θF = BIL \sin \theta).

SI unit: the tesla (T). Equivalent forms:

1 T=1Wbm2=1NA m=1kgA s21 \text{ T} = 1 \frac{\text{Wb}}{\text{m}^2} = 1 \frac{\text{N}}{\text{A m}} = 1 \frac{\text{kg}}{\text{A s}^2}

Typical magnitudes:

  • Earth's surface field: about 5×10−55 \times 10^{-5} T.
  • Bar magnet near a pole: 0.01 to 0.1 T.
  • MRI scanner: 1.5 to 3 T (some research machines reach 7 T).
  • Strong laboratory electromagnet: up to 10 T.
  • Neutron star: 10810^8 T (and rising).

Magnetic flux

Magnetic flux through a tilted coil A flat rectangular coil of area A is tilted so that its normal vector n makes an angle theta with the uniform magnetic field B. Field lines pass through the coil; the flux equals B A cosine theta. When the normal is aligned with B (theta zero), flux is a maximum. When the normal is perpendicular to B (theta ninety), flux is zero. B n θ Φ = B A cos θ; θ is the angle between B and the area normal n.

For a flat surface of area AA placed in a uniform field B⃗\vec{B}, the magnetic flux through the surface is:

Φ=BAcos⁡θ\Phi = B A \cos \theta

where θ\theta is the angle between B⃗\vec{B} and the normal to the surface (the vector perpendicular to the surface). SI unit: the weber (Wb), where 1 Wb = 1 T m2^2.

Two ways to picture it:

  1. Flux is the "amount of field passing through" the surface. More field, more area, or more alignment with the surface normal all increase flux.
  2. Flux is the dot product Φ=B⃗⋅A⃗\Phi = \vec{B} \cdot \vec{A}, where A⃗\vec{A} is the area vector (magnitude AA, direction along the normal).

Special angles:

  • θ=0°\theta = 0° (field along the normal): Φ=BA\Phi = BA, maximum flux.
  • θ=90°\theta = 90° (field in the plane of the surface): Φ=0\Phi = 0, no flux through the surface.
  • θ=180°\theta = 180°: Φ=−BA\Phi = -BA, maximum negative flux (the field passes through the surface in the opposite sense).

The angle convention (watch this)

The θ\theta in Φ=BAcos⁡θ\Phi = B A \cos \theta is the angle between B⃗\vec{B} and the normal to the surface, not between B⃗\vec{B} and the surface itself. Questions sometimes give the angle between the field and the plane of a coil; you must take the complement.

"Plane at 30° to the field" ⇒\Rightarrow normal at 60° to the field ⇒\Rightarrow cos⁡60°=0.5\cos 60° = 0.5.

"Normal at 30° to the field" ⇒\Rightarrow cos⁡30°=0.866\cos 30° = 0.866.

Flux through multiple turns

A coil of NN turns links flux NN times (each turn intercepts the same flux, in series). The flux linkage is:

Ψ=NΦ=NBAcos⁡θ\Psi = N \Phi = N B A \cos \theta

Faraday's law uses flux linkage: ε=−N dΦ/dt\varepsilon = - N \, d\Phi / dt, not just dΦ/dtd\Phi / dt. We treat this in the induction dot point.

Compass needles and flux qualitatively

A compass needle is a small magnetic dipole. It aligns with the local field direction so that its north pole points along B⃗\vec{B}. By placing compasses (or sprinkling iron filings) over a region you can map the direction of B⃗\vec{B} at every point, hence the field line pattern. The density of the lines (lines per unit area perpendicular to them) is proportional to the flux density BB, hence the name.

If you tilt a small loop of wire in a uniform field while watching the field lines, the number of lines threading the loop changes as cos⁡θ\cos \theta. That is the geometric content of Φ=BAcos⁡θ\Phi = BA \cos \theta.

Worked example: rotating coil

A square coil of side 0.200.20 m and 5050 turns is rotated in a uniform field of 0.300.30 T. Find the maximum flux linkage and the flux linkage when the coil normal is at 45°45° to the field.

Area: A=0.202=0.040A = 0.20^2 = 0.040 m2^2.

Maximum flux linkage (normal aligned with field, θ=0°\theta = 0°):

Ψmax⁡=NBA=50×0.30×0.040=0.60\Psi_{\max} = N B A = 50 \times 0.30 \times 0.040 = 0.60 Wb.

At θ=45°\theta = 45°:

Ψ=NBAcos⁡45°=0.60×0.707=0.42\Psi = N B A \cos 45° = 0.60 \times 0.707 = 0.42 Wb.

As the coil rotates, the flux linkage oscillates between +0.60+0.60 Wb and −0.60-0.60 Wb, with the rate of change driving the induced EMF in a generator (Faraday's law).

Reading a flux-versus-angle graph

Because Φ=BAcos⁡θ\Phi = BA\cos\theta and BB, AA are fixed for a given coil in a given field, plotting Φ\Phi against cos⁡θ\cos\theta (rather than against θ\theta itself) turns the relationship into a straight line through the origin, with gradient BABA. This is the practical way an exam graph tests the equation: read two points off the line, find the gradient, and either check it against a known BABA or use it to find an unknown BB or AA.

Magnetic flux versus cosine theta for a coil of fixed area in a fixed field A straight line through the origin rising to the right, showing that the magnetic flux Phi through a coil is directly proportional to cosine theta when the flux density B and area A are fixed. Five data points sit on the line at cosine theta equals zero point two, zero point four, zero point six, zero point eight and one point zero. The gradient of the line equals B times A. cos θ flux Φ (×10⁻³ Wb) 0.20.40.6 0.81.0 2468 gradient = B A Φ ∝ cos θ: a line through the origin.

Common traps
Confusing BB and Φ\Phi
BB is a field strength per unit area; Φ\Phi is a total field through an area. They have different units (T vs Wb).
Using the angle to the surface instead of to the normal
Questions love to phrase the geometry as "the coil is at 60 degrees to the field," meaning the plane of the coil is at 60 degrees, so the normal is at 30 degrees. Always check what θ\theta refers to before substituting into cos⁡\cos.
Forgetting the NN for a multi-turn coil
A 100-turn coil with 1 Wb through each turn has 100 Wb of flux linkage, not 1 Wb. For Faraday's law, you must use NΦN \Phi or apply the NN outside the derivative.
Treating flux as a vector
Flux Φ\Phi is a scalar. The direction information is buried in the sign through cos⁡θ\cos \theta (positive or negative depending on orientation).
Quoting flux as the dot product without specifying the area direction
Always state which way the area normal points; a flipped normal flips the sign of flux but does not change physics.
The must-know equations

Flux density (field at a point): BB, unit tesla, 1 T=1 Wb m−2=1 N A−1m−11\ \text{T} = 1\ \text{Wb m}^{-2} = 1\ \text{N A}^{-1}\text{m}^{-1}.

Flux (total field through a surface): Φ=BAcos⁡θ\Phi = BA\cos\theta, unit weber, 1 Wb=1 T m21\ \text{Wb} = 1\ \text{T m}^2, with θ\theta measured from the normal.

Flux linkage through NN turns: Ψ=NΦ=NBAcos⁡θ\Psi = N\Phi = NBA\cos\theta. Special angles: Φ=BA\Phi = BA at θ=0∘\theta = 0^{\circ} (maximum); Φ=0\Phi = 0 at θ=90∘\theta = 90^{\circ}; Φ=−BA\Phi = -BA at θ=180∘\theta = 180^{\circ}.

Worked examples

Model 1 - flux with a "plane at angle" wording. A circular coil of radius 8.0×10−28.0 \times 10^{-2} m has its plane at 35∘35^{\circ} to a uniform field of 0.550.55 T. Calculate the magnetic flux through the coil.

Area: A=πr2=π(8.0×10−2)2=2.01×10−2 m2A = \pi r^2 = \pi (8.0 \times 10^{-2})^2 = 2.01 \times 10^{-2}\ \text{m}^2.

"Plane at 35∘35^{\circ} to the field" means the normal is at 90∘−35∘=55∘90^{\circ} - 35^{\circ} = 55^{\circ} to the field.

Φ=BAcos⁡θ=0.55×2.01×10−2×cos⁡55∘=0.55×2.01×10−2×0.574=6.3×10−3 Wb\Phi = BA\cos\theta = 0.55 \times 2.01 \times 10^{-2} \times \cos 55^{\circ} = 0.55 \times 2.01 \times 10^{-2} \times 0.574 = 6.3 \times 10^{-3}\ \text{Wb}.

Marker's note: the mark for "correctly identifying θ\theta" is separate from the arithmetic mark - state "normal at 55∘55^{\circ}" explicitly before substituting, since markers cannot award the geometry mark from a bare number.

Model 2 - flux linkage and a rotating coil. A rectangular coil 0.12 m×0.090 m0.12\ \text{m} \times 0.090\ \text{m} with 8080 turns sits in a uniform field of 0.450.45 T. Find the maximum flux linkage, and the flux linkage when the coil has rotated so its normal is at 70∘70^{\circ} to the field.

Area: A=0.12×0.090=1.08×10−2 m2A = 0.12 \times 0.090 = 1.08 \times 10^{-2}\ \text{m}^2.

Maximum flux linkage (normal parallel to B⃗\vec{B}, θ=0∘\theta = 0^{\circ}): Ψmax⁡=NBA=80×0.45×1.08×10−2=0.389 Wb\Psi_{\max} = NBA = 80 \times 0.45 \times 1.08 \times 10^{-2} = 0.389\ \text{Wb}.

At θ=70∘\theta = 70^{\circ}: Ψ=NBAcos⁡70∘=0.389×0.342=0.13 Wb\Psi = NBA\cos 70^{\circ} = 0.389 \times 0.342 = 0.13\ \text{Wb}.

Marker's note: compute Ψmax⁡=NBA\Psi_{\max} = NBA first (a clean, checkable intermediate result), then multiply by cos⁡θ\cos\theta - this two-step structure earns partial credit even if the final multiplication slips, and it is the same structure Faraday's law needs in the next dot point.

Exam technique

Command words: "state/define" wants the equation and units only; "calculate" wants full substitution with units and a final answer to two or three significant figures; "explain" wants the physical reasoning (why cos⁡θ\cos\theta, why flux is a scalar).

Always write down whether the given angle is to the normal or to the plane before you substitute - this is the single most common way marks are lost on this dot point. If the question says "the coil is at X∘X^{\circ} to the field" with no other qualifier, assume it means the plane, and use cos⁡(90∘−X)=sin⁡X\cos(90^{\circ} - X)= \sin X.

On a Φ\Phi-vs-cos⁡θ\cos\theta graph, the gradient is BABA (or NBANBA for flux linkage) - read two points well apart on the line, not adjacent grid squares, to minimise reading error.

In plain English

Picture rain falling straight down and you holding a hula hoop. If you hold the hoop flat, facing straight up at the sky, the most rain possible falls through it - that is like the flux being at its maximum, because the "normal" (the direction the hoop faces) lines up exactly with the rain's direction, which is what physicists call B⃗\vec{B}. Now tilt the hoop on its side, edge-on to the rain: almost no drops pass through the opening any more, even though the rain itself has not changed at all. That is flux dropping to zero, even though the flux density - how heavy the rain is falling, everywhere - has stayed exactly the same. The two ideas are easy to blend, but they measure completely different things: flux density is "how strong is the field right here," like the rain's intensity, while flux is "how much of that field actually gets through this particular window I've set up," which depends on the window's size and the angle you hold it at. A weather vane, and a compass needle in exactly the same way, does not care about flux at all - it just swings to point along the flux density, showing you the field's direction.

Examples in context

Example 1. Flux through a Snowy 2.0 generator rotor pole face. Each salient pole of a Snowy 2.0 generator has a 0.40 m×0.30 m0.40 \text{ m} \times 0.30 \text{ m} face producing B=1.6 TB = 1.6 \text{ T} at the air gap. With the pole face perpendicular to B⃗\vec{B} (i.e. normal to the surface aligned with the field, θ=0\theta = 0), the flux through the pole face is Φ=BAcos⁡0∘=1.6×0.40×0.30=0.192 Wb\Phi = B A \cos 0^{\circ} = 1.6 \times 0.40 \times 0.30 = 0.192 \text{ Wb}. As the rotor spins past a stator coil, the flux linking that coil rises and falls sinusoidally between ±0.192 Wb\pm 0.192 \text{ Wb} at the rotation frequency, driving the induced AC EMF that feeds the NSW grid.

Example 2. Earth's flux through a Coffs Harbour orienteering compass. The Earth's magnetic field strength at Coffs Harbour is B≈5.5×10−5 TB \approx 5.5 \times 10^{-5} \text{ T}, inclined 60∘60^{\circ} to horizontal. A horizontal compass needle (A=2.0×10−4 m2A = 2.0 \times 10^{-4} \text{ m}^2) has flux Φ=BAcos⁡60∘\Phi = B A \cos 60^{\circ} (the vertical component of B⃗\vec{B} passes through the horizontal area) =5.5×10−5×2.0×10−4×0.50=5.5×10−9 Wb=5.5 nWb= 5.5 \times 10^{-5} \times 2.0 \times 10^{-4} \times 0.50 = 5.5 \times 10^{-9} \text{ Wb} = 5.5 \text{ nWb}. This minuscule flux is enough to align the needle with Earth's field. A 3D field sensor (e.g. in a smartphone) reads all three components and combines them.

Exam-style questions

Questions in the style of NESA exam questions on this dot point, each with a worked answer. They are written by ExamExplained unless tagged "Past paper"; the year shows the paper a question is modelled on.

2023 HSC-style3 marks
A circular loop of radius 0.10 m sits in a uniform magnetic field of 0.50 T. Calculate the magnetic flux through the loop when its plane is (a) perpendicular to the field and (b) at 30 degrees to the field.
Show worked answer →

Area of the loop:

A=πr2=π(0.10)2=3.14×10−2A = \pi r^2 = \pi (0.10)^2 = 3.14 \times 10^{-2} m2^2.

(a) Plane perpendicular to the field means the field passes through the loop along its normal, so θ=0°\theta = 0° between B⃗\vec{B} and the area vector:

Φ=BAcos⁡0°=0.50×3.14×10−2×1=1.57×10−2\Phi = B A \cos 0° = 0.50 \times 3.14 \times 10^{-2} \times 1 = 1.57 \times 10^{-2} Wb.

(b) "Plane at 30° to the field" means the field makes 30° with the plane, so the normal makes 60° with the field:

Φ=BAcos⁡60°=0.50×3.14×10−2×0.5=7.85×10−3\Phi = B A \cos 60° = 0.50 \times 3.14 \times 10^{-2} \times 0.5 = 7.85 \times 10^{-3} Wb.

Markers reward correct interpretation of "plane at X degrees to field" versus "normal at X degrees to field," correct area calculation, and units in webers.

2018 HSC-style2 marks
Explain the difference between magnetic flux density B and magnetic flux Phi, and state the SI units of each.
Show worked answer →

Magnetic flux density BB is a vector quantity describing the strength and direction of the magnetic field at a point. Its SI unit is the tesla (T), where 1 T = 1 Wb/m2^2 = 1 N/(A m). It tells you the force per unit current per unit length on a conductor placed at that point, or the force per unit charge per unit velocity on a moving charge.

Magnetic flux Φ\Phi is a scalar quantity describing the total magnetic field passing through a surface of area AA. Its SI unit is the weber (Wb), where 1 Wb = 1 T m2^2. It is given by Φ=BAcos⁡θ\Phi = B A \cos \theta, where θ\theta is the angle between the field direction and the normal to the surface.

Markers reward correct units for both, the area dependence of flux, and a clear statement that BB is per unit area and Φ\Phi is over the whole area.

Practice questions

Original practice questions graded from foundation to exam level, each with a full worked solution. Try them before revealing the solution.

foundation2 marks
State the SI unit of magnetic flux density BB and the SI unit of magnetic flux Φ\Phi, and write the equation linking them for a flat area AA at angle θ\theta to the normal.
Show worked solution →

Flux density BB is measured in tesla (T); flux Φ\Phi is measured in weber (Wb), where 1 Wb=1 T m21\ \text{Wb} = 1\ \text{T m}^2.

Φ=BAcos⁡θ\Phi = BA\cos\theta.

Marks: one for both correct units (T and Wb), one for the correct equation with θ\theta identified as the angle to the normal.

foundation3 marks
A flat coil of area 2.5×10−2 m22.5 \times 10^{-2}\ \text{m}^2 is placed with its plane perpendicular to a uniform magnetic field of 0.400.40 T. Calculate the magnetic flux through the coil.
Show worked solution →

Plane perpendicular to B⃗\vec{B} means the normal is parallel to B⃗\vec{B}, so θ=0∘\theta = 0^{\circ} and cos⁡θ=1\cos\theta = 1.

Φ=BAcos⁡θ=0.40×2.5×10−2×1=1.0×10−2 Wb\Phi = BA\cos\theta = 0.40 \times 2.5 \times 10^{-2} \times 1 = 1.0 \times 10^{-2}\ \text{Wb}.

Marks: one for correctly identifying θ=0∘\theta = 0^{\circ} from "plane perpendicular to the field", one for the substitution, one for Φ=1.0×10−2 Wb\Phi = 1.0 \times 10^{-2}\ \text{Wb} with the correct unit.

foundation2 marks
A student rotates a coil in a uniform field from θ=0∘\theta = 0^{\circ} (normal parallel to B⃗\vec{B}) to θ=90∘\theta = 90^{\circ} (normal perpendicular to B⃗\vec{B}). Describe what happens to the flux through the coil.
Show worked solution →

The flux Φ=BAcos⁡θ\Phi = BA\cos\theta starts at its maximum value Φ=BA\Phi = BA when θ=0∘\theta = 0^{\circ} (all field lines thread the coil) and decreases smoothly, following a cosine curve, to zero at θ=90∘\theta = 90^{\circ} (the field lies entirely in the plane of the coil, so none of it "passes through" along the normal).

Marks: one for stating the flux decreases from BABA to zero, one for linking this to the cos⁡θ\cos\theta dependence rather than a linear decrease.

core4 marks
The graph shows the magnetic flux Φ\Phi through a coil of fixed area AA in a fixed field BB, plotted against cos⁡θ\cos\theta as the coil is rotated. **(a)** Explain why the graph is a straight line through the origin. **(b)** Using the points (cos⁡θ=0.20, Φ=2.0×10−3 Wb)(\cos\theta = 0.20,\ \Phi = 2.0 \times 10^{-3}\ \text{Wb}) and (cos⁡θ=0.80, Φ=8.0×10−3 Wb)(\cos\theta = 0.80,\ \Phi = 8.0 \times 10^{-3}\ \text{Wb}), find the gradient. **(c)** Given A=2.5×10−2 m2A = 2.5 \times 10^{-2}\ \text{m}^2, use the gradient to find BB.
Show worked solution →

(a) Φ=BAcos⁡θ\Phi = BA\cos\theta, and for a fixed coil in a fixed field, BB and AA are constants, so Φ\Phi is directly proportional to cos⁡θ\cos\theta: a straight line through the origin with gradient BABA.

(b) Gradient =ΔΦΔ(cos⁡θ)=(8.0−2.0)×10−3 Wb0.80−0.20=6.0×10−30.60=1.0×10−2 Wb= \dfrac{\Delta \Phi}{\Delta(\cos\theta)} = \dfrac{(8.0 - 2.0) \times 10^{-3}\ \text{Wb}}{0.80 - 0.20} = \dfrac{6.0 \times 10^{-3}}{0.60} = 1.0 \times 10^{-2}\ \text{Wb}.

(c) The gradient equals BABA, so B=gradientA=1.0×10−22.5×10−2=0.40 TB = \dfrac{\text{gradient}}{A} = \dfrac{1.0 \times 10^{-2}}{2.5 \times 10^{-2}} = 0.40\ \text{T}.

Marks: one for the direct-proportionality explanation with Φ=BAcos⁡θ\Phi = BA\cos\theta, one for a correctly calculated gradient with unit weber, one for identifying gradient =BA= BA, one for B=0.40 TB = 0.40\ \text{T}.

core3 marks
A rectangular coil measuring 0.15 m×0.080 m0.15\ \text{m} \times 0.080\ \text{m} has its plane at 50∘50^{\circ} to a uniform field of 0.600.60 T. Calculate the magnetic flux through the coil.
Show worked solution →

Area: A=0.15×0.080=1.2×10−2 m2A = 0.15 \times 0.080 = 1.2 \times 10^{-2}\ \text{m}^2.

"Plane at 50∘50^{\circ} to the field" means the normal is at 90∘−50∘=40∘90^{\circ} - 50^{\circ} = 40^{\circ} to the field.

Φ=BAcos⁡θ=0.60×1.2×10−2×cos⁡40∘=0.60×1.2×10−2×0.766=5.5×10−3 Wb\Phi = BA\cos\theta = 0.60 \times 1.2 \times 10^{-2} \times \cos 40^{\circ} = 0.60 \times 1.2 \times 10^{-2} \times 0.766 = 5.5 \times 10^{-3}\ \text{Wb}.

Marks: one for the correct area, one for correctly converting "plane at 50∘50^{\circ}" to "normal at 40∘40^{\circ}", one for Φ=5.5×10−3 Wb\Phi = 5.5 \times 10^{-3}\ \text{Wb} with the unit.

exam6 marks
A flat search coil of N=200N = 200 turns and area 1.5×10−3 m21.5 \times 10^{-3}\ \text{m}^2 is used to investigate the field between the poles of a large horseshoe magnet. Analyse how a student could use this coil, together with the concepts of flux density and flux, to determine both the direction and the magnitude of B⃗\vec{B} between the poles, and explain the limitations of the method.
Show worked solution →

Band-6 plan. (1) State the working definitions of BB and Φ=NBAcos⁡θ\Phi = NBA\cos\theta for the multi-turn coil. (2) Explain the direction-finding method (rotate the coil, flux linkage is maximum when the normal is along B⃗\vec{B}). (3) Explain the magnitude method (measure maximum flux linkage, then B=Φmax⁡/(NA)B = \Phi_{\max}/(NA), or use an induced-EMF search-coil technique). (4) Evaluate limitations (uniformity assumption, coil size relative to field region, alignment precision, whether a static or changing field is used). Finish with a judgement on reliability.

Model answer. The flux linked by the NN-turn coil is Ψ=NΦ=NBAcos⁡θ\Psi = N\Phi = NBA\cos\theta, where θ\theta is the angle between B⃗\vec{B} and the coil's normal. Because BB and AA are fixed for a given position, Ψ\Psi depends only on cos⁡θ\cos\theta, reaching its single maximum value Ψmax⁡=NBA\Psi_{\max} = NBA when the normal is exactly parallel to B⃗\vec{B} (θ=0∘\theta = 0^{\circ}).

To find the direction of B⃗\vec{B}, the student rotates the coil about a fixed point between the poles while monitoring the flux linkage (in practice, via the induced EMF as the coil is rotated or briefly withdrawn, since a static flux alone cannot be read directly without a sensor). The orientation that gives the maximum reading identifies the normal direction, and hence the field direction, at that point.

To find the magnitude, the student uses the coil in that maximum orientation. If the flux linkage Ψmax⁡\Psi_{\max} can be measured (for example, by suddenly removing the coil from the field and integrating the induced EMF, or with a calibrated Hall probe as a cross-check), then B=Ψmax⁡NAB = \dfrac{\Psi_{\max}}{NA}, using the known NN and AA of the coil.

Limitations. The method assumes the field is uniform over the area of the coil; if the coil is large compared with the region between the poles, it averages the field rather than measuring it at a point, underestimating peak BB near the pole faces. Precisely aligning the normal with B⃗\vec{B} by eye introduces angular uncertainty, and since Φ∝cos⁡θ\Phi \propto \cos\theta is fairly flat near θ=0∘\theta = 0^{\circ}, small misalignments barely change the reading, making the maximum hard to pinpoint exactly. The method also only gives BB at the coil's location, not the full field map.

Marker's note: the top band gives both the direction method (rotate to find the flux-linkage maximum) and the magnitude method (measured Ψmax⁡\Psi_{\max} then B=Ψmax⁡/(NA)B = \Psi_{\max}/(NA)), explicitly uses Ψ=NBAcos⁡θ\Psi = NBA\cos\theta, and evaluates at least two genuine limitations (field non-uniformity over the coil area, angular alignment uncertainty near the flat top of the cosine curve). A response that only states the formula without the direction-finding reasoning caps in the middle band.

exam5 marks
Evaluate the claim that 'magnetic flux and magnetic flux density measure the same thing, just in different units.' In your answer, refer to the physical meaning of each quantity and to a specific scenario where treating them as interchangeable would lead to an incorrect conclusion.
Show worked solution →

Band-6 plan. (1) State the claim is false and why: give the precise definitions of BB (field per unit area, a vector, at a point) and Φ\Phi (total field through a whole surface, a scalar). (2) Show the unit mismatch is not just a scaling issue (T vs Wb are dimensionally different, differing by m2\text{m}^2). (3) Give a concrete scenario (two coils of different area, or one coil at different angles) where equal BB gives different Φ\Phi, or equal Φ\Phi arises from different BB. (4) Conclude with a precise, judged statement.

Model answer. The claim is incorrect. Magnetic flux density B⃗\vec{B} is a vector field quantity describing the strength and direction of the magnetic field at a single point in space, measured in tesla. Magnetic flux Φ\Phi is a scalar describing the total amount of field passing through a whole surface of finite area, measured in weber, and is calculated from BB by Φ=BAcos⁡θ\Phi = BA\cos\theta. These are not the same physical quantity measured in different units (like metres and centimetres); they differ by a factor of area and orientation, so their units are dimensionally different (1 Wb=1 T m21\ \text{Wb} = 1\ \text{T m}^2, not a pure numerical conversion).

A concrete case shows why the distinction matters. Two coils sit in the same uniform field B=0.50 TB = 0.50\ \text{T}, both with their normal aligned with the field (θ=0∘\theta = 0^{\circ}): a small coil of area 1.0×10−3 m21.0 \times 10^{-3}\ \text{m}^2 and a large coil of area 1.0×10−1 m21.0 \times 10^{-1}\ \text{m}^2. Both experience the identical flux density B=0.50 TB = 0.50\ \text{T}, yet their fluxes are Φ1=0.50×1.0×10−3=5.0×10−4 Wb\Phi_1 = 0.50 \times 1.0 \times 10^{-3} = 5.0 \times 10^{-4}\ \text{Wb} and Φ2=0.50×1.0×10−1=5.0×10−2 Wb\Phi_2 = 0.50 \times 1.0 \times 10^{-1} = 5.0 \times 10^{-2}\ \text{Wb}, a hundred-fold difference. If a student incorrectly treated BB and Φ\Phi as interchangeable, they would wrongly conclude the two coils experience "the same field effect," when in fact any induced EMF (which depends on the rate of change of Φ\Phi, not BB) would be a hundred times larger in the big coil for the same rate of rotation.

Treating BB and Φ\Phi as interchangeable would therefore lead directly to an incorrect prediction of induced EMF in a generator or search coil, since Faraday's law is stated in terms of Φ\Phi (or NΦN\Phi), not BB alone.

Marker's note: the top band gives both correct definitions with correct units, explicitly notes the dimensional difference (area factor), and uses a worked numerical scenario (not just an assertion) to show the claim fails, linking the consequence to Faraday's law. A response that only recites "B is tesla, Phi is weber" without the worked contrast or the EMF consequence caps in the middle band.

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