Magnetic field, field lines and flux
A compass needle always turns north — because of the Earth's magnetic field. Link to earlier classes : magnets, field lines and the compass of classes 9-10 now extend to dipoles, fields and torque formulas.
A magnetic field (B) is the region around a magnet where it exerts a force on other magnets or currents.
In the figure : Field lines on the left, flux on the right.
Magnetic field, field lines and flux
In the app you can move this figure with your finger.
Open in the appRule 1: Field lines — Lines leave N, enter S; inside the magnet S → N; closed loops; never cross; dense = stronger B.
- Easy : The tangent to a line gives the direction of B.
- Medium : Two lines crossing would give two directions at a point — impossible.
- Exam (CET) : Field lines are? (1) closed (2) open (3) crossing (4) straight only → answer 1)
Rule 2: Magnetic flux — Φ = B A cos θ; unit weber (Wb) = T m²; θ = angle between B and the area normal.
- Easy : B = 0.2 T, A = 0.05 m², θ = 0 ⇒ Φ = 0.01 Wb.
- Medium : θ = 60° ⇒ Φ = 0.005 Wb.
- Exam (CET) : Φ is maximum at? (1) 0° (2) 90° (3) 45° (4) 60° → answer 1) Trick : area perpendicular to B ⇒ maximum.
Rule 3: Units and dimensions — Unit of B is tesla (T) = Wb/m²; 1 T = 10⁴ gauss. [B] = M T⁻² A⁻¹; [Φ] = M L² T⁻² A⁻¹.
- Easy : 0.5 T = 5000 gauss.
- Medium : 2 × 10⁻⁴ Wb ÷ 0.01 m² = 0.02 T.
- Exam (CET) : 1 T = ? (1) 10⁴ G (2) 10² G (3) 10⁻⁴ G (4) 1 G → answer 1)
Derivation : Φ = B A cos θ
- Step 1 : Area normal n̂; angle θ with B.
- Step 2 : Component of B normal to the surface is B cos θ.
- Step 3 : Φ = (normal component) × A.
- Step 4 : Φ = B A cos θ.
Φ = BA cos θ; 1 Wb = 1 T m²; lines are closed.
Flux depends on angle; θ is measured from the normal.
Memory clue : "Normal = maximum (cos 0)".
Spot the difference
| Quantity | Unit | Dimensions |
|---|---|---|
| B | T | M T⁻² A⁻¹ |
| Φ | Wb | M L² T⁻² A⁻¹ |
Practice questions
- 1What is a magnetic field?
- 2Unit of Φ?
- 3Do field lines cross?
- 4B = 0.4 T, A = 0.02 m², θ = 0 : Φ?
- 5Same, θ = 90° : Φ?
- 63 × 10⁻³ Wb, A = 0.06 m² : B?
- 7By what factor does Φ change at θ = 60°?
- 8What do dense lines mean?
Show answers (try them yourself first)
- 1The space around a magnet where its force is felt
- 2Wb
- 3No
- 48 × 10⁻³ Wb
- 50
- 60.05 T
- 7½
- 8Stronger B
Bar magnet as a magnetic dipole
However you cut a magnet, it still has two ends.
A magnetic dipole is two equal opposite poles close together; m = pole strength × separation.
In the figure : m points from S to N.
Rule 1: Dipole moment — m = q_m × 2l; direction S → N; unit A m² (or J/T); [m] = L² A.
- Easy : q_m = 5 A m, 2l = 0.1 m ⇒ m = 0.5 A m².
- Medium : m = 0.5, 2l = 0.2 m ⇒ q_m = 2.5 A m.
- Exam (CET) : Direction of m? (1) S → N (2) N → S (3) outward (4) zero → answer 1)
Rule 2: Current loop — The m of a loop = N I A; a current loop is a magnetic dipole.
- Easy : I = 2 A, A = 0.01 m², N = 1 ⇒ m = 0.02 A m².
- Medium : N = 50 ⇒ m = 1 A m².
- Exam (CET) : m of a loop? (1) NIA (2) I/A (3) NI/A (4) IA² → answer 1)
Rule 3: Cutting a magnet — However a magnet is cut, each piece keeps N and S (no monopole). Cut across the length : m halves, q_m same.
- Easy : m = 0.8 A m²; cut across the middle ⇒ m = 0.4.
- Medium : Cut across : q_m same, 2l halves.
- Exam (CET) : A piece with one pole only? (1) never (2) always (3) sometimes (4) in small pieces → answer 1)
Derivation : Loop as a dipole
- Step 1 : Far from a loop, its field looks like that of a dipole.
- Step 2 : A dipole has m = q_m × 2l.
- Step 3 : For a loop m = I A.
- Step 4 : m = N I A.
m = q_m 2l = NIA; unit A m².
Cutting never gives a monopole.
Memory clue : "S to N = m".
Spot the difference
| Feature | Bar magnet | Electric dipole |
|---|---|---|
| Poles | N, S (no monopole) | +q, −q (can be separated) |
| Moment | m = q_m 2l | p = q 2l |
| Direction | S → N | −q → +q |
Practice questions
- 1Unit of m?
- 2Direction of m?
- 3Do monopoles exist?
- 4q_m = 4 A m, 2l = 0.05 m : m?
- 5I = 3 A, A = 0.02 m², N = 10 : m?
- 6A magnet of m = 1.2 cut across the middle : m?
- 7Why is a loop a dipole?
- 8Dimensions of m?
Show answers (try them yourself first)
- 1A m²
- 2S → N
- 3No
- 40.2 A m²
- 50.6 A m²
- 60.6
- 7Same far field
- 8L² A
Axial and equatorial fields of a short magnet
Move away from a magnet and its effect falls quickly.
Axial = along the magnet's line; equatorial = on the perpendicular bisector.
In the figure : Green axial, purple equatorial.
Rule 1: Axial line — B = (μ₀/4π) · 2m / r³; along m.
- Easy : m = 0.5, r = 0.2 m ⇒ B = 1.25 × 10⁻⁵ T.
- Medium : r doubled ⇒ B becomes ⅛.
- Exam (CET) : B ∝ ? (1) 1/r³ (2) 1/r² (3) 1/r (4) r → answer 1)
Rule 2: Equatorial line — B = (μ₀/4π) · m / r³; opposite to m. B_axial = 2 B_eq.
- Easy : Same m, r : B = 6.250 × 10⁻⁶ T.
- Medium : Axial : equatorial = 2 : 1.
- Exam (CET) : B_axial / B_eq = ? (1) 2 (2) 1 (3) ½ (4) 4 → answer 1)
Rule 3: Short magnet — Valid only when r ≫ l; μ₀/4π = 10⁻⁷ T m/A.
- Easy : l = 1 cm, r = 50 cm ⇒ r ≫ l, the formula works.
- Medium : m = 2, r = 1 m ⇒ B_ax = 4 × 10⁻⁷ T.
- Exam (CET) : μ₀/4π = ? (1) 10⁻⁷ (2) 10⁻⁵ (3) 4π×10⁻⁷ (4) 10⁷ → answer 1)
Derivation : Axial field
- Step 1 : Point at r from the centre; r − l from N, r + l from S.
- Step 2 : B = (μ₀/4π) q_m [1/(r − l)² − 1/(r + l)²].
- Step 3 : = (μ₀/4π) q_m · 4 r l / (r² − l²)².
- Step 4 : r ≫ l, m = q_m 2l ⇒ B = (μ₀/4π) 2m / r³.
B_ax = (μ₀/4π) 2m/r³; B_eq = (μ₀/4π) m/r³.
B_eq is opposite to m; axial is double.
Memory clue : "Axis = 2, equator = 1".
Spot the difference
| Line | B | Direction |
|---|---|---|
| Axial | (μ₀/4π) 2m/r³ | Along m |
| Equatorial | (μ₀/4π) m/r³ | Opposite to m |
Practice questions
- 1Formula for axial B?
- 2Direction of equatorial B?
- 3How does B vary with r?
- 4m = 1, r = 0.1 m : B_axial?
- 5Same : B_eq?
- 6r tripled ⇒ B?
- 7B_ax = 8 × 10⁻⁶ T at r; at 2r?
- 8Why r ≫ l in the formula?
Show answers (try them yourself first)
- 1(μ₀/4π) 2m/r³
- 2Opposite to m
- 31/r³
- 42 × 10⁻⁴ T
- 51 × 10⁻⁴ T
- 61/27
- 710⁻⁶ T
- 8Because r² − l² ≈ r²
Field at any point, torque and neutral points
A compass needle turns and settles in a field — because of torque.
Torque τ turns m in a field; a neutral point is where the net B is zero.
In the figure : θ between m and B.
Rule 1: B at any point — B = (μ₀/4π)(m/r³) √(1 + 3cos²θ); θ = angle from the axis.
- Easy : m = 0.5, r = 0.2, θ = 60° ⇒ B = 8.27 × 10⁻⁶ T.
- Medium : θ = 0 ⇒ 2m/r³ ; θ = 90° ⇒ m/r³.
- Exam (CET) : B at θ = 90°? (1) m/r³ (2) 2m/r³ (3) 0 (4) 3m/r³ (times μ₀/4π) → answer 1)
Rule 2: Torque and potential energy — τ = m B sin θ (m × B); U = − m B cos θ. θ = 0 stable equilibrium; θ = 180° unstable.
- Easy : m = 0.5, B = 0.2 T, θ = 30° ⇒ τ = 0.05 N m.
- Medium : θ = 0 ⇒ U = − 0.1 J; θ = 180° ⇒ + 0.1 J; difference 0.2 J.
- Exam (CET) : τ maximum at? (1) 90° (2) 0° (3) 180° (4) 45° → answer 1) Trick : sin 90° = 1.
Rule 3: Neutral points — Where the magnet's B equals the Earth's B_H. N pointing north ⇒ on the equatorial line (μ₀/4π)m/d³ = B_H; N pointing south ⇒ on the axial line (μ₀/4π)2m/d³ = B_H.
- Easy : m = 0.35, B_H = 3.5 × 10⁻⁵ ⇒ d = 0.10 m.
- Medium : N pointing south ⇒ same m gives d = 0.126 m.
- Exam (CET) : N pointing north ⇒ neutral points lie on? (1) equatorial (2) axial (3) anywhere (4) none → answer 1)
Derivation : τ = m B sin θ
- Step 1 : +q_m B on N, −q_m B on S; a couple.
- Step 2 : Arm = 2l sin θ.
- Step 3 : τ = q_m B × 2l sin θ.
- Step 4 : τ = m B sin θ.
τ = mB sin θ; U = −mB cos θ; neutral : B_d = B_H.
N north ⇒ equatorial points; N south ⇒ axial points.
Memory clue : "North → equatorial; south → axial".
Spot the difference
| State | θ | τ | U |
|---|---|---|---|
| Stable | 0 | 0 | −mB |
| Max τ | 90° | mB | 0 |
| Unstable | 180° | 0 | +mB |
Practice questions
- 1Formula for τ?
- 2When is equilibrium stable?
- 3What is a neutral point?
- 4m = 2, B = 0.1, θ = 90° : τ?
- 5Same, θ = 0 : U?
- 6Work to turn θ = 0 to 180°?
- 7τ = 0.05 N m, m = 0.5, B = 0.2 : θ?
- 8N north : where are neutral points?
Show answers (try them yourself first)
- 1m B sin θ
- 2θ = 0
- 3A point where the net field is zero
- 40.2 N m
- 5−0.2 J
- 60.4 J
- 730° (or 150°)
- 8On the equatorial line
Gauss's law for magnetism
A single pole of a magnet never comes alone.
Gauss for magnetism : the net magnetic flux through a closed surface is 0.
In the figure : Flux in = flux out.
Rule 1: Gauss for magnetism — ∮ B · dA = 0 — the net magnetic flux through any closed surface is zero.
- Easy : A sphere around a bar magnet : flux in = flux out.
- Medium : Φ_out = 3 × 10⁻³ Wb ⇒ Φ_in = 3 × 10⁻³ Wb.
- Exam (CET) : Net Φ through a closed surface? (1) 0 (2) B A (3) q/ε₀ (4) μ₀I → answer 1)
Rule 2: Electric vs magnetic Gauss — Electric : ∮E·dA = q/ε₀ (isolated charges exist). Magnetic : 0 (no isolated pole).
- Easy : Closed surface around an electric dipole : q_net = 0 ⇒ Φ_E = 0.
- Medium : For a magnet it is always 0.
- Exam (CET) : Magnetic monopole? (1) never found (2) found (3) proven (4) of iron → answer 1)
Rule 3: Why closed lines — Lines leave N, enter S and return inside — no start or end.
- Easy : Outside N → S; inside S → N.
- Medium : Electric lines run from +q to −q (not closed).
- Exam (CET) : Magnetic lines are? (1) closed (2) from + pole (3) to infinity (4) straight → answer 1)
Derivation : No monopole
- Step 1 : Take any closed surface.
- Step 2 : As many lines enter as leave.
- Step 3 : ∴ Σ B·ΔA = 0.
- Step 4 : ∮ B · dA = 0.
∮ B·dA = 0.
Electric gives q/ε₀; magnetic gives 0 — do not mix.
Memory clue : "A magnet always comes in pairs".
Spot the difference
| Gauss's law | Electric | Magnetic |
|---|---|---|
| Net flux | q/ε₀ | 0 |
| Source | Isolated charge | Dipole |
| Lines | Open | Closed |
Practice questions
- 1Gauss's law for magnetism?
- 2Has a monopole been found?
- 3How are the lines?
- 4Φ in = 5 × 10⁻⁴ Wb : Φ out?
- 5Net Φ of a closed surface?
- 6Φ_E of an electric dipole?
- 7Why do new poles appear on cutting?
- 8Electric vs magnetic Gauss difference?
Show answers (try them yourself first)
- 1∮B·dA = 0
- 2No
- 3Closed
- 45 × 10⁻⁴ Wb
- 50
- 60
- 7Always dipoles; no monopole
- 8q/ε₀ versus 0
Earth's magnetism and its elements
In India a compass stays nearly flat; near the poles it is useless.
Earth's field is described by three elements : declination (α), dip (δ), horizontal component (B_H).
In the figure : Horizontal and vertical parts of B_E.
Rule 1: Three elements — Declination α = angle between geographic and magnetic meridians; dip δ = angle of B_E with the horizontal; B_H = horizontal component.
- Easy : δ = 0 at the equator; δ = 90° at the poles.
- Medium : B_H = 0 at the poles; B_V = 0 at the equator.
- Exam (CET) : δ at the magnetic equator? (1) 0 (2) 90° (3) 45° (4) 60° → answer 1)
Rule 2: Relations — B_H = B_E cos δ; B_V = B_E sin δ; tan δ = B_V / B_H; B_E = √(B_H² + B_V²).
- Easy : B_E = 5 × 10⁻⁵, δ = 60° ⇒ B_H = 2.5 × 10⁻⁵, B_V = 4.33 × 10⁻⁵ T.
- Medium : B_H = B_V = 3.5 × 10⁻⁵ ⇒ δ = 45°, B_E = 4.95 × 10⁻⁵ T.
- Exam (CET) : δ = 45° ⇒ B_V / B_H = ? (1) 1 (2) 0 (3) 2 (4) ∞ → answer 1) Trick : tan 45° = 1.
Rule 3: Dip circle — A dip circle measures δ; the needle is vertical at the poles and horizontal at the equator.
- Easy : δ is small in India (near the equator).
- Medium : Larger δ ⇒ larger B_V.
- Exam (CET) : Needle at the poles? (1) vertical (2) horizontal (3) at 45° (4) spins → answer 1)
Derivation : tan δ = B_V / B_H
- Step 1 : Resolve B_E : horizontal B_H, vertical B_V.
- Step 2 : B_H = B_E cos δ, B_V = B_E sin δ.
- Step 3 : Divide : B_V / B_H = tan δ.
- Step 4 : Square and add : B_E = √(B_H² + B_V²).
B_H = B_E cos δ; B_V = B_E sin δ; tan δ = B_V/B_H.
δ is 0 at the equator, 90° at the poles — do not swap.
Memory clue : "cos = horizontal, sin = vertical".
Spot the difference
| Place | δ | B_H | B_V |
|---|---|---|---|
| Magnetic equator | 0 | Max | 0 |
| Mid latitude | 0-90° | Medium | Medium |
| Magnetic pole | 90° | 0 | Max |
Practice questions
- 1What is declination?
- 2What is dip?
- 3Formula for B_H?
- 4B_E = 6 × 10⁻⁵, δ = 30° : B_H?
- 5B_H = 3 × 10⁻⁵, B_V = 3 × 10⁻⁵ : δ?
- 6B_H = 3, B_V = 4 (units) : B_E?
- 7δ = 60° : B_V / B_H?
- 8Why is a compass useless at the poles?
Show answers (try them yourself first)
- 1The angle between the geographic and magnetic meridians
- 2Angle of B_E with the horizontal
- 3B_E cos δ
- 45.2 × 10⁻⁵ T
- 545°
- 65
- 71.73
- 8B_H = 0
Magnetic maps and the Earth as a dipole
A ship's captain corrects the compass using a map of declination.
The Earth is a large dipole; magnetic maps show lines of equal α, δ and B_H.
In the figure : Magnetic axis tilted about 11°.
Rule 1: Earth is a dipole — Treat the Earth as a huge magnet : its S pole is near the geographic north, its N pole near the south; the axis is tilted about 11° from the geographic axis.
- Easy : A compass N is drawn to the Earth's magnetic S pole.
- Medium : m ≈ 8 × 10²² A m².
- Exam (CET) : Near the geographic north the Earth's pole is? (1) S (2) N (3) both (4) none → answer 1)
Rule 2: Magnetic latitude — B_E = B₀ √(1 + 3 sin²λ); B₀ = (μ₀/4π) m/R³; tan δ = 2 tan λ.
- Easy : B₀ = 10⁻⁷ × 8 × 10²² ÷ (6.4 × 10⁶)³ = 3.05 × 10⁻⁵ T; at the pole 2B₀ = 6.10 × 10⁻⁵ T.
- Medium : λ = 45° ⇒ tan δ = 2 ⇒ δ = 63.4°.
- Exam (CET) : λ = 0 ⇒ δ? (1) 0 (2) 90° (3) 45° (4) 63° → answer 1)
Rule 3: Magnetic maps — Isogonic lines (equal α), agonic line (α = 0), isoclinic lines (equal δ), aclinic line = magnetic equator.
- Easy : Sailors correct for declination using such maps.
- Medium : δ = 0 on the aclinic line.
- Exam (CET) : The line of δ = 0? (1) aclinic (2) isogonic (3) agonic (4) isoclinic → answer 1)
Derivation : tan δ = 2 tan λ
- Step 1 : Dipole : radial and tangential parts B_r = 2B₀ sin λ, B_θ = B₀ cos λ.
- Step 2 : Vertical = B_r, horizontal = B_θ.
- Step 3 : tan δ = B_r / B_θ.
- Step 4 : tan δ = 2 tan λ.
B_E = B₀√(1 + 3sin²λ); tan δ = 2 tan λ; B₀ ≈ 3 × 10⁻⁵ T.
λ is magnetic latitude, not geographic.
Memory clue : "tan δ = twice tan λ".
Spot the difference
| Line | Meaning |
|---|---|
| Isogonic | Equal α |
| Agonic | α = 0 |
| Isoclinic | Equal δ |
| Aclinic | δ = 0 (magnetic equator) |
Practice questions
- 1Earth's pole near geographic north?
- 2What is an isoclinic line?
- 3Formula for B₀?
- 4λ = 30° : δ?
- 5λ = 0 : B_E?
- 6λ = 90° : B_E?
- 7Prove tan δ = 2 tan λ.
- 8m = 8 × 10²² : B₀?
Show answers (try them yourself first)
- 1Magnetic S
- 2A line joining places of equal dip
- 3(μ₀/4π) m/R³
- 449.1°
- 5B₀
- 62B₀
- 7Use B_r / B_θ
- 83.1 × 10⁻⁵ T
Quick revision of the whole lesson
| Concept | Key formula / fact | Unit / dimensions |
|---|---|---|
| Flux | Φ = BA cos θ | Wb; M L² T⁻² A⁻¹ |
| Field | B | T; M T⁻² A⁻¹ |
| Moment | m = q_m 2l = NIA | A m²; L² A |
| Axial | (μ₀/4π) 2m/r³ | T |
| Equatorial | (μ₀/4π) m/r³ | T |
| Torque | τ = mB sin θ | N m |
| Energy | U = −mB cos θ | J |
| Gauss | ∮B·dA = 0 | Wb |
| Earth | B_H = B_E cos δ; tan δ = 2 tan λ | T |
🎯 Most important points for the exam
- Φ = BA cos θ; lines are closed; 1 T = 10⁴ G.
- m = q_m 2l = NIA, S → N.
- Axial = 2 × equatorial; ∝ 1/r³.
- τ = mB sin θ; U = −mB cos θ.
- Neutral point : B_d = B_H.
- ∮B·dA = 0 — no monopole.
- B_H = B_E cos δ; tan δ = 2 tan λ.
B → Φ → m → axial/equatorial → τ, U → Gauss 0 → Earth (δ, B_H).