
Physics II course sequence · Interactive lesson
Faraday's law
Flux on its own drives nothing. What a circuit feels is how fast that flux is moving, and Faraday's law is the sentence that turns one into the other. Learn to differentiate a flux, count the turns, and read a voltage waveform straight off a flux-time graph.
UPII-10.02 · Lesson 2 of 8 in this unit. Position is not a completion score.Build the model
A steady flux drives nothing; only a changing one does.
The key idea
Faraday's law states that the emf induced around a closed loop equals minus the rate at which the magnetic flux through that loop changes, and that a coil of N identical turns gives N times as much.
Example. A 200-turn coil whose flux per turn falls steadily from 4.0 × 10⁻⁴ Wb to zero in 25 ms gives |ε| = 200 × (4.0 × 10⁻⁴ Wb) ÷ (0.025 s) = 3.2 V, and only during those 25 ms.
The complete physical model and assumptions
Faraday's law says a circuit responds not to magnetic flux but to its rate of change: ε = −dΦB/dt around a closed loop, and N times that for a coil of N identical turns. It is an experimental law before it is anything else — a galvanometer twitches while a magnet moves and sits dead while the magnet rests, and the twitch grows with the speed of the motion rather than with the strength of the field alone. Writing it as a derivative absorbs every way the flux can change at once: the field can vary, the loop can change area, the loop can turn, and the product rule sorts out the separate contributions, which may add or cancel. The minus sign is bookkeeping tied to the convention that links the chosen sense of circulation to the area vector; the next topic turns it into a physical statement about opposition. Three limits are worth knowing now. The law gives the emf around a whole loop, not a voltage at a point, so in an induced circuit a voltmeter's reading depends on where its leads run. It needs a loop whose boundary you can actually name, so sliding or ambiguous circuits need care. And it never says where the energy comes from: that always traces back to whatever is doing work to change the flux.
1Rate, not amount
Faraday's experiments settled one question: a circuit feels the motion of flux, not its size. A 500-turn coil of area 20 cm² held still in a 0.80 T field links Φ = 0.80 T × 20 × 10⁻⁴ m² = 1.6 × 10⁻³ Wb per turn, a flux linkage of 0.80 Wb, and produces no emf whatsoever. Pull the same coil clear of the field in 40 ms and the average emf is NΔΦ/Δt = 0.80 Wb ÷ 0.040 s = 20 V. Nothing about the coil changed; only the clock entered. So the quantity to compute is always a derivative, and the units say so: one weber per second is one volt. A useful habit follows. Before reaching for a formula, ask what is changing and how fast, because if the answer is nothing, the emf is zero no matter how impressive the field.
2Fix a sense of circulation before you differentiate
Faraday's law has a sign, and a sign needs a convention. Choose a direction to walk around the loop. Curl the right hand that way and the thumb gives the positive normal, which fixes the area vector and therefore the sign of Φ = ∫B⋅dA. Then ε = −dΦ/dt is positive when it drives current in the direction you chose. Choose the opposite sense and both Φ and ε flip together, so the physical current is unchanged — the convention never affects the answer, only its label. Two practical consequences: keep the same normal for the whole calculation, since flipping it midway is the commonest sign error, and remember that the flux may be negative to start with, in which case a flux becoming less negative is still a positive dΦ/dt. Turning that sign into the statement that the induced effect opposes the change is the job of Lenz's law.
3Differentiate the flux term by term
For a flat loop in a uniform field, Φ = BA cos θ is a product of three things that can each move in time. The product rule gives dΦ/dt = A cos θ (dB/dt) + B cos θ (dA/dt) − BA sin θ (dθ/dt): a changing field, a changing area, a turning loop. Most problems switch on one term. A fixed 0.040 m² loop facing a field rising at 1.5 T s⁻¹ has dΦ/dt = 0.040 m² × 1.5 T s⁻¹ = 0.060 Wb s⁻¹, so one turn develops 60 mV. But the terms are signed and they can fight: a loop being squeezed while the field grows has a positive first term and a negative second, and at the right squeeze rate the emf is exactly zero while both the field and the area are changing fast. When the field is not uniform over the loop, go back to Φ = ∫B⋅dA, integrate first with the geometry frozen, then differentiate the result.
4Turns multiply the emf, not automatically the current
A coil of N identical turns is N loops in series, each threaded by the same flux Φ, so their emfs add: ε = −N dΦ/dt. The bookkeeping is tidier in terms of the flux linkage λ = NΦ, since then ε = −dλ/dt for any coil. Two cautions. The word identical is doing work: near the ends of a short solenoid, or in a coil wider than the magnet that feeds it, the outer turns link less flux and the sum must be done turn by turn. And a coil with more turns is not automatically a better current source. Winding twice as many turns of the same wire round the same former doubles the emf but also doubles the length of wire, hence the resistance, so I = ε/R barely moves. More turns buy voltage; a lower-resistance circuit buys current.
5Read the emf straight off the flux-time graph
Since ε = −N dΦ/dt, the emf waveform is the negative slope of the flux waveform, scaled by N. A flat stretch of flux gives zero emf however high it sits. A straight ramp gives a constant emf, so a triangular flux gives a square-wave emf, and the sharp corner where the ramp reverses appears as an instantaneous jump in the emf. A steeper ramp in half the time gives twice the emf, which is why short, fast changes are the violent ones. The sinusoidal case runs the whole course: Φ = Φ₀ sin ωt gives ε = −NΦ₀ω cos ωt, an emf a quarter cycle behind the flux with amplitude NΦ₀ω. With N = 250 turns, Φ₀ = 2.0 mWb and f = 10 Hz, ω = 2π(10) = 62.8 rad s⁻¹ and the peak emf is 250 × 2.0 × 10⁻³ Wb × 62.8 s⁻¹ = 31 V. Double the frequency and the peak doubles, though the flux curve keeps its height.
6Integrate it back: charge, and the timing that cancels
Faraday's law can also be run in reverse. With a total circuit resistance R the current is I = −N(dΦ/dt)/R, and integrating over a flux change gives the charge q = ∫I dt = N|ΔΦ|/R. Every trace of the timing has gone: the same charge circulates whether the change takes a millisecond or an hour, which is exactly why a fluxmeter measures charge in order to get ΔΦ. Calculus handles the smooth cases the same way. A search coil of 350 turns and area 4.0 cm² in a field decaying as B = (0.60 T) e(−t/τ) with τ = 12 ms sees ε = NAB₀ e(−t/τ)/τ, which starts at 350 × 4.0 × 10⁻⁴ m² × 0.60 T ÷ 0.012 s = 7.0 V and then decays with that same τ. Integrating the emf over all time recovers NAB₀, so with R = 22 Ω the total charge is 0.14 m² × 0.60 T ÷ 22 Ω = 3.8 mC.
Key equations
Read the units, assumptions and limits before substituting.
Faraday's law for one loop
ε = −dΦB/dt
The emf follows the slope of the flux-time graph and never its height.
ε in volts (V), ΦB in webers (Wb = T m²), t in seconds; 1 Wb s⁻¹ = 1 VFlux linkage of N turns
ε = −N dΦB/dt = −dλ/dt, with λ = NΦB
Identical turns are emf sources in series, so the coil multiplies the emf by N.
N is the turn count, a pure number; λ is the flux linkage in weber-turns (Wb)Three ways the flux can change
dΦB/dt = A cos θ (dB/dt) + B cos θ (dA/dt) − B A sin θ (dθ/dt)
Names the three drives — changing field, changing area, turning loop — and lets them cancel.
flat loop in a uniform field; A in m², θ in rad between B and the area vectorAverage emf across an interval
εavg = −N ΔΦB/Δt
What a before-and-after measurement gives when the shape of the curve is unknown.
ΔΦB is the change in flux per turn in Wb, Δt the interval in sInduced current in the loop
I = |ε|/R
The emf is the source; the resistance alone decides the current it pushes.
I in amperes, R in ohms for the whole loop, the winding's own resistance includedCharge moved by one flux change
q = ∫I dt = N|ΔΦB|/R
A fluxmeter measures charge precisely because the timing drops out of it.
q in coulombs; no Δt appears, so the duration of the change cancels outInteractive lab
Predict first. Explore the model. Compare the result.
Explore the model
Try this. Drag the instant to a crest: the flux is largest there and the tangent is flat, so the emf is zero. Slide it to a zero crossing for the peak, {0.25*2*π*f*φ|1} V. Doubling f halves the period and doubles that peak without raising the curve at all.
Live results
- FLUX Φ NOW
- 1.37 mWb
- SLOPE dΦ/dt
- 92 mWb s⁻¹
- EMF ε = −N dΦ/dt
- -22.9 V
- PEAK EMF NΦ₀ω
- 31.4 V
Results follow this lesson’s model and assumptions. Displayed values are rounded.
Predict → change one variable → check
Plan a change before running it. Every other input stays at the saved baseline.
Saved baseline. Flux amplitude Φ₀ per turn: 2.0 mWb; Frequency f: 10 Hz; Instant t on the graph: 12 ms
This experiment is kept only while this page is open. It does not change saved course progress.
Catch the common trap
The commonest error is to treat the emf as proportional to the flux itself, so that a strong field or a tightly linked coil must give a large emf. Faraday's law contains no Φ, only dΦ/dt. A 250-turn coil resting inside the 3 T bore of an MRI magnet links an enormous flux and generates exactly nothing, because nothing is changing; the same coil pulled out in 0.20 s gives a healthy emf from a far smaller field. The sinusoidal case makes the point sharply: with Φ = Φ₀ sin ωt the emf is −NωΦ₀ cos ωt, so the instant the flux is largest is precisely the instant the emf vanishes, and the emf peaks as the flux passes through zero. Flux and emf run a quarter cycle apart, never in step.
Practice & worked examples
3 authored examples. Make an attempt, then reveal the reasoning one step at a time.
EasyExample 1
A single square loop of side 12.0 cm lies with its plane perpendicular to a uniform magnetic field. The field is reduced steadily from 0.850 T to 0.250 T in 40.0 ms. The loop's total resistance is 0.150 Ω. Find the magnitude of the induced emf and of the induced current.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 4 steps revealed.
- The plane is perpendicular to the field, so the area vector lies along B, θ = 0 and Φ = BA for the one turn. The area is A = (0.120 m)² = 0.0144 m².
- Only B changes, so dΦ/dt = A (dB/dt), and a steady reduction means dB/dt = (0.250 − 0.850) T ÷ 0.0400 s = −15.0 T s⁻¹.
- Magnitude of the emf: |ε| = A |dB/dt| = 0.0144 m² × 15.0 T s⁻¹ = 0.216 V. Because the ramp is straight, this value holds for the whole 40.0 ms and then stops dead.
- Current: I = |ε|/R = 0.216 V ÷ 0.150 Ω = 1.44 A.
Answer. |ε| = 0.216 V, constant throughout the 40.0 ms ramp, and I = 1.44 A.
MediumExample 2
A 240-turn coil of cross-sectional area 25.0 cm² has its axis along a uniform field. B rises linearly from 0 to 0.400 T in the first 20.0 ms, holds at 0.400 T until 50.0 ms, then falls linearly to zero by 60.0 ms. The coil circuit has resistance 8.00 Ω. Find the emf in each stage, and the charge that flows during the rise and during the fall.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 5 steps revealed.
- Convert the area: A = 25.0 cm² = 25.0 × 10⁻⁴ m² = 2.50 × 10⁻³ m². The axis lies along B, so Φ = BA per turn and ε = −NA (dB/dt) at every stage.
- Rise: dB/dt = 0.400 T ÷ 0.0200 s = 20.0 T s⁻¹, so |ε| = 240 × 2.50 × 10⁻³ m² × 20.0 T s⁻¹ = 12.0 V, flat for 20.0 ms.
- Hold: dB/dt = 0, so ε = 0 for the next 30.0 ms, even though the flux linkage is at its largest, NΦ = 240 × 1.00 × 10⁻³ Wb = 0.240 Wb.
- Fall: dB/dt = −0.400 T ÷ 0.0100 s = −40.0 T s⁻¹, so |ε| = 24.0 V with the sign reversed. The waveform is a 12.0 V block lasting 20.0 ms, a flat zero for the next 30.0 ms, then a 24.0 V block the other way for 10.0 ms.
- Charge: q = N|ΔΦ|/R = 0.240 Wb ÷ 8.00 Ω = 0.0300 C for the rise, and the identical 0.0300 C for the fall, because q depends on the size of the flux change and not on how long it took.
Answer. ε = 12.0 V during the rise, 0 during the hold, and 24.0 V reversed during the fall; q = 30.0 mC through each transition.
HardExample 3
A flexible single-turn loop of resistance 0.120 Ω lies flat in a uniform field perpendicular to its plane. At one instant its radius is 0.150 m and it is being squeezed inwards at 0.0200 m s⁻¹, while the field is 0.300 T and rising at 0.400 T s⁻¹. (a) Find the emf and the current at that instant. (b) Find the inward squeeze rate that would make the emf zero there.
Sketch your answer or reasoning, then compare it with the authored solution. Your writing is not automatically graded or saved.
0 of 6 steps revealed.
- With θ = 0 the flux is Φ = BA and both factors are moving, so the product rule gives dΦ/dt = A (dB/dt) + B (dA/dt).
- Area and its rate: A = πr² = π(0.150 m)² = 0.0707 m², and dA/dt = 2πr (dr/dt) = 2π(0.150 m)(−0.0200 m s⁻¹) = −0.0188 m² s⁻¹.
- Field term: A (dB/dt) = 0.0707 m² × 0.400 T s⁻¹ = +0.0283 Wb s⁻¹. Area term: B (dA/dt) = 0.300 T × (−0.0188 m² s⁻¹) = −0.00565 Wb s⁻¹. They pull opposite ways, since the field is growing while the loop is shrinking.
- Sum: dΦ/dt = 0.0283 − 0.00565 = 0.0226 Wb s⁻¹, so |ε| = 22.6 mV and I = 0.0226 V ÷ 0.120 Ω = 0.188 A.
- (b) Zero emf needs the two terms to cancel: πr²(dB/dt) + 2πrB (dr/dt) = 0, so dr/dt = −r (dB/dt) ÷ (2B) = −(0.150 m)(0.400 T s⁻¹) ÷ (2 × 0.300 T) = −0.100 m s⁻¹.
- Squeezing inwards at 0.100 m s⁻¹ would hold the flux constant at that instant. The real rate is five times slower, so the field term wins and the emf keeps its sign, exactly as the two signed terms already showed.
Answer. (a) |ε| = 22.6 mV and I = 0.188 A. (b) An inward rate of 0.100 m s⁻¹ would give zero emf.
Quick check
Select an answer and explain it before checking.
Review & continue
Faraday's law states that the emf induced around a closed loop equals minus the rate at which the magnetic flux through that loop changes, and that a coil of N identical turns gives N times as much.
- Explain the relationship without looking at the equation.
- Check a sign, a unit and a model assumption in your working.
- Return to the lab or worked example if a step is still unclear.
Optional supporting lessons
These chapter resources can help with earlier ideas; they are not additional required Physics II completion tasks.