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Unit 5: Magnetic Fields and Electromagnetism

Physics C E&M cheatsheet

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Magnetism describes forces on moving charges and currents. Unlike electric fields, magnetic fields do no work on a point charge because the magnetic force is always perpendicular to the charge’s velocity. This unit focuses on Lorentz forces, fields produced by currents, and Ampere’s law.



A charge moving through a magnetic field feels the magnetic part of the Lorentz force:

F⃗B=qv⃗×B⃗.\vec{F}_B = q\vec{v}\times\vec{B}.

The magnitude is

FB=∣q∣vBsin⁡θ.F_B = \lvert q \rvert vB\sin\theta.

The force is perpendicular to both v⃗\vec{v} and B⃗\vec{B}. For positive charges, use the right-hand rule for v⃗×B⃗\vec{v}\times\vec{B}. For negative charges, reverse the direction.

The full electric and magnetic force is

F⃗=qE⃗+qv⃗×B⃗.\vec{F}=q\vec{E}+q\vec{v}\times\vec{B}.

Since F⃗B\vec{F}_B is always perpendicular to v⃗\vec{v}, it does no work: P=F⃗B⋅v⃗=q(v⃗×B⃗)⋅v⃗=0P = \vec{F}_B\cdot\vec{v} = q(\vec{v}\times\vec{B})\cdot\vec{v} = 0, since v⃗×B⃗\vec{v}\times\vec{B} is perpendicular to v⃗\vec{v}. A magnetic field can change a charge’s direction but never its speed.

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Example. A proton (q=+1.6×10−19 Cq = +1.6\times10^{-19}\ \text{C}) moves at v=4.0×105 m/sv = 4.0\times10^5\ \text{m/s} in the +x+x direction through a uniform field B⃗=0.50 T\vec{B} = 0.50\ \text{T} pointing in the +y+y direction. Find the magnitude and direction of the magnetic force.

The velocity is perpendicular to the field (θ=90∘\theta = 90^\circ), so the magnitude is

FB=∣q∣vBsin⁡90∘=(1.6×10−19)(4.0×105)(0.50)=3.2×10−14 N.F_B = \lvert q\rvert vB\sin 90^\circ = (1.6\times10^{-19})(4.0\times10^5)(0.50) = 3.2\times10^{-14}\ \text{N}.

For the direction, evaluate v⃗×B⃗=(vx^)×(By^)=vB (x^×y^)=vB z^\vec{v}\times\vec{B} = (v\hat{x})\times(B\hat{y}) = vB\,(\hat{x}\times\hat{y}) = vB\,\hat{z}. Since the charge is positive, F⃗B\vec{F}_B points in +z+z (out of the page if xx is right and yy is up). For an electron with the same velocity, the force would point in −z-z.


Charged Particles in Uniform Magnetic Fields

Section titled “Charged Particles in Uniform Magnetic Fields”

If a charge moves perpendicular to a uniform magnetic field, the magnetic force provides centripetal force:

∣q∣vB=mv2r.\lvert q \rvert vB=\frac{mv^2}{r}.

Thus

r=mv∣q∣B.r=\frac{mv}{\lvert q\rvert B}.

The angular frequency is

ω=∣q∣Bm,\omega=\frac{\lvert q \rvert B}{m},

and the period is

T=2πm∣q∣B.T=\frac{2\pi m}{\lvert q \rvert B}.

If the velocity has a component parallel to B⃗\vec{B}, that component is unchanged and the path becomes a helix.

Notice that the period T=2πm/(∣q∣B)T = 2\pi m/(\lvert q\rvert B) does not depend on the speed or the radius: a faster particle simply travels a proportionally larger circle in the same time. This speed-independence is the principle behind the cyclotron.

Example. An electron (m=9.11×10−31 kgm = 9.11\times10^{-31}\ \text{kg}, ∣q∣=1.6×10−19 C\lvert q\rvert = 1.6\times10^{-19}\ \text{C}) moves at v=2.0×106 m/sv = 2.0\times10^6\ \text{m/s} perpendicular to a uniform field B=1.5×10−3 TB = 1.5\times10^{-3}\ \text{T}. Find the radius of its circular path, the period, and the frequency.

The magnetic force supplies the centripetal force, ∣q∣vB=mv2/r\lvert q\rvert vB = mv^2/r, so

r=mv∣q∣B=(9.11×10−31)(2.0×106)(1.6×10−19)(1.5×10−3)=1.82×10−242.4×10−22≈7.6×10−3 m.r = \frac{mv}{\lvert q\rvert B} = \frac{(9.11\times10^{-31})(2.0\times10^6)}{(1.6\times10^{-19})(1.5\times10^{-3})} = \frac{1.82\times10^{-24}}{2.4\times10^{-22}} \approx 7.6\times10^{-3}\ \text{m}.

The period is independent of vv:

T=2πm∣q∣B=2π(9.11×10−31)(1.6×10−19)(1.5×10−3)=5.72×10−302.4×10−22≈2.4×10−8 s.T = \frac{2\pi m}{\lvert q\rvert B} = \frac{2\pi(9.11\times10^{-31})}{(1.6\times10^{-19})(1.5\times10^{-3})} = \frac{5.72\times10^{-30}}{2.4\times10^{-22}} \approx 2.4\times10^{-8}\ \text{s}.

The frequency (the cyclotron frequency) is

f=1T=∣q∣B2πm≈4.2×107 Hz.f = \frac{1}{T} = \frac{\lvert q\rvert B}{2\pi m} \approx 4.2\times10^{7}\ \text{Hz}.

When electric and magnetic forces oppose each other,

qE=qvB.qE=qvB.

Only particles with speed

v=EBv=\frac{E}{B}

pass through undeflected. This is the basic idea of a velocity selector.

After velocity selection, a magnetic field can separate particles by mass-to-charge ratio because

r=mv∣q∣B.r=\frac{mv}{\lvert q \rvert B}.
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Example. A velocity selector uses crossed fields E=3.0×104 V/mE = 3.0\times10^4\ \text{V/m} and B1=0.10 TB_1 = 0.10\ \text{T}. The selected beam (singly charged ions, q=1.6×10−19 Cq = 1.6\times10^{-19}\ \text{C}) then enters a mass-spectrometer region with field B2=0.20 TB_2 = 0.20\ \text{T}. Find the selected speed, and the radii of two isotopes of mass m1=3.32×10−26 kgm_1 = 3.32\times10^{-26}\ \text{kg} and m2=3.65×10−26 kgm_2 = 3.65\times10^{-26}\ \text{kg}.

In the selector, the electric and magnetic forces balance, qE=qvB1qE = qvB_1, so only ions with

v=EB1=3.0×1040.10=3.0×105 m/sv = \frac{E}{B_1} = \frac{3.0\times10^4}{0.10} = 3.0\times10^5\ \text{m/s}

pass straight through. In the spectrometer the path radius is r=mv/(qB2)r = mv/(qB_2):

r1=(3.32×10−26)(3.0×105)(1.6×10−19)(0.20)=9.96×10−213.2×10−20≈0.311 m,r_1 = \frac{(3.32\times10^{-26})(3.0\times10^5)}{(1.6\times10^{-19})(0.20)} = \frac{9.96\times10^{-21}}{3.2\times10^{-20}} \approx 0.311\ \text{m}, r2=(3.65×10−26)(3.0×105)(1.6×10−19)(0.20)=1.095×10−203.2×10−20≈0.342 m.r_2 = \frac{(3.65\times10^{-26})(3.0\times10^5)}{(1.6\times10^{-19})(0.20)} = \frac{1.095\times10^{-20}}{3.2\times10^{-20}} \approx 0.342\ \text{m}.

The heavier isotope curves on the larger circle. The two beams land 2(r2−r1)≈6.2 cm2(r_2 - r_1) \approx 6.2\ \text{cm} apart on the detector, which is how a mass spectrometer resolves isotopes.


A wire segment carrying current II in a magnetic field feels

F⃗=IL⃗×B⃗,\vec{F}=I\vec{L}\times\vec{B},

where L⃗\vec{L} points in the direction of conventional current and has magnitude equal to the length of wire in the field.

The magnitude is

F=ILBsin⁡θ.F=ILB\sin\theta.

This force comes from the magnetic forces on the moving charges inside the wire: each carrier feels qv⃗d×B⃗q\vec{v}_d\times\vec{B}, and summing over all carriers in a length LL (with I=nqvdAcrossI = nqv_d A_{\text{cross}}) gives F⃗=IL⃗×B⃗\vec{F} = I\vec{L}\times\vec{B}.

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Example. A straight wire of length L=0.40 mL = 0.40\ \text{m} carries current I=8.0 AI = 8.0\ \text{A} in the +x+x direction. It sits in a uniform field B⃗=0.25 T\vec{B} = 0.25\ \text{T} pointing into the page (−z-z, with xx to the right and yy up). Find the magnitude and direction of the force.

The current direction (+x+x) is perpendicular to B⃗\vec{B} (−z-z), so θ=90∘\theta = 90^\circ and

F=ILBsin⁡90∘=(8.0)(0.40)(0.25)=0.80 N.F = ILB\sin 90^\circ = (8.0)(0.40)(0.25) = 0.80\ \text{N}.

For the direction, L⃗×B⃗=(Lx^)×(−Bz^)=−LB (x^×z^)=−LB(−y^)=+LB y^\vec{L}\times\vec{B} = (L\hat{x})\times(-B\hat{z}) = -LB\,(\hat{x}\times\hat{z}) = -LB(-\hat{y}) = +LB\,\hat{y}. So the force points in +y+y (upward). Check with the right-hand rule: fingers point along the current (+x+x), curl toward B⃗\vec{B} (into page), thumb points up. The force is 0.80 N0.80\ \text{N} upward.


A current loop in a magnetic field experiences a torque. For a loop with NN turns, current II, area AA, and magnetic moment

μ⃗=NIA⃗,\vec{\mu}=NI\vec{A},

the torque is

τ⃗=μ⃗×B⃗.\vec{\tau}=\vec{\mu}\times\vec{B}.

Its magnitude is

τ=NIABsin⁡θ.\tau=NIAB\sin\theta.

The potential energy of a magnetic dipole in a uniform magnetic field is

U=−μ⃗⋅B⃗=−μBcos⁡θ.U=-\vec{\mu}\cdot\vec{B} = -\mu B\cos\theta.

Here θ\theta is the angle between μ⃗\vec{\mu} (the loop’s normal, by the right-hand rule) and B⃗\vec{B}. The energy is lowest when μ⃗\vec{\mu} is aligned with B⃗\vec{B} (θ=0\theta = 0, U=−μBU = -\mu B, stable) and highest when anti-aligned (θ=180∘\theta = 180^\circ, U=+μBU = +\mu B, unstable). The torque always tries to rotate μ⃗\vec{\mu} into alignment with B⃗\vec{B}.

Example. A rectangular coil with N=50N = 50 turns, sides 0.080 m×0.050 m0.080\ \text{m}\times0.050\ \text{m}, carries I=2.0 AI = 2.0\ \text{A} in a uniform field B=0.30 TB = 0.30\ \text{T}. (a) Find the magnetic moment and the maximum torque. (b) Find the dipole energy when μ⃗\vec{\mu} is aligned with B⃗\vec{B} and when it is perpendicular to B⃗\vec{B}.

The loop area is A=(0.080)(0.050)=4.0×10−3 m2A = (0.080)(0.050) = 4.0\times10^{-3}\ \text{m}^2, so the magnetic moment is

μ=NIA=(50)(2.0)(4.0×10−3)=0.40 A⋅m2.\mu = NIA = (50)(2.0)(4.0\times10^{-3}) = 0.40\ \text{A}\cdot\text{m}^2.

The torque τ=NIABsin⁡θ=μBsin⁡θ\tau = NIAB\sin\theta = \mu B\sin\theta is maximum at θ=90∘\theta = 90^\circ (plane of the loop parallel to B⃗\vec{B}):

τmax⁡=μB=(0.40)(0.30)=0.12 N⋅m.\tau_{\max} = \mu B = (0.40)(0.30) = 0.12\ \text{N}\cdot\text{m}.

For the energy U=−μBcos⁡θU = -\mu B\cos\theta: when μ⃗∥B⃗\vec{\mu}\parallel\vec{B} (θ=0\theta = 0),

U∥=−μB=−(0.40)(0.30)=−0.12 J,U_{\parallel} = -\mu B = -(0.40)(0.30) = -0.12\ \text{J},

and when μ⃗⊥B⃗\vec{\mu}\perp\vec{B} (θ=90∘\theta = 90^\circ),

U⊥=−μBcos⁡90∘=0 J.U_{\perp} = -\mu B\cos 90^\circ = 0\ \text{J}.

Rotating the dipole from aligned to perpendicular requires an external agent to supply ΔU=0−(−0.12)=+0.12 J\Delta U = 0 - (-0.12) = +0.12\ \text{J}.


The magnetic field around a long straight wire is

B=μ0I2πr.B=\frac{\mu_0 I}{2\pi r}.

The direction follows the right-hand rule: thumb in the direction of conventional current, curled fingers show the magnetic field direction.

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At the center of a circular loop of radius RR,

B=μ0I2R.B=\frac{\mu_0 I}{2R}.

For NN identical turns,

B=μ0NI2R.B=\frac{\mu_0 NI}{2R}.

Inside a long ideal solenoid,

B=μ0nI,B=\mu_0 nI,

where n=N/Ln=N/L is turns per unit length.


For a current element, the magnetic field contribution is

dB⃗=μ04πI dℓ⃗×r^r2.d\vec{B}=\frac{\mu_0}{4\pi}\frac{I\,d\vec{\ell}\times\hat{r}}{r^2}.

Use Biot-Savart when symmetry is not enough for Ampere’s law but the current geometry is integrable. The cross product means only the component of dℓ⃗d\vec{\ell} perpendicular to the line from source to field point contributes.

Proof (Field of an infinite straight wire from Biot–Savart). Place the wire along the xx-axis carrying current II, and find the field at a point PP a perpendicular distance rr from the wire. Let a current element I dℓ⃗=I dx x^I\,d\vec{\ell} = I\,dx\,\hat{x} sit at position xx; the vector from the element to PP has magnitude x2+r2\sqrt{x^2 + r^2}.

The magnitude of dℓ⃗×r^d\vec{\ell}\times\hat{r} is dxsin⁡ϕdx\sin\phi, where ϕ\phi is the angle between the wire and the line to PP. From the geometry, sin⁡ϕ=r/x2+r2\sin\phi = r/\sqrt{x^2 + r^2}. Every element contributes field in the same direction (out of the page, by the right-hand rule), so the magnitudes add:

dB=μ0I4πdxsin⁡ϕx2+r2=μ0I4πr dx(x2+r2)3/2.dB = \frac{\mu_0 I}{4\pi}\frac{dx\sin\phi}{x^2 + r^2} = \frac{\mu_0 I}{4\pi}\frac{r\,dx}{(x^2 + r^2)^{3/2}}.

Integrate over the whole wire, xx from −∞-\infty to +∞+\infty:

B=μ0Ir4π∫−∞∞dx(x2+r2)3/2.B = \frac{\mu_0 I r}{4\pi}\int_{-\infty}^{\infty}\frac{dx}{(x^2 + r^2)^{3/2}}.

The standard integral is

∫dx(x2+r2)3/2=xr2x2+r2,\int\frac{dx}{(x^2 + r^2)^{3/2}} = \frac{x}{r^2\sqrt{x^2 + r^2}},

which you can verify by the substitution x=rtan⁡ϕx = r\tan\phi, dx=rsec⁡2ϕ dϕdx = r\sec^2\phi\,d\phi, giving ∫rsec⁡2ϕ dϕr3sec⁡3ϕ=1r2∫cos⁡ϕ dϕ=sin⁡ϕr2\int \frac{r\sec^2\phi\,d\phi}{r^3\sec^3\phi} = \frac{1}{r^2}\int\cos\phi\,d\phi = \frac{\sin\phi}{r^2}. Evaluating from −∞-\infty to +∞+\infty, the factor xx2+r2\dfrac{x}{\sqrt{x^2+r^2}} runs from −1-1 to +1+1:

∫−∞∞dx(x2+r2)3/2=1r2[1−(−1)]=2r2.\int_{-\infty}^{\infty}\frac{dx}{(x^2 + r^2)^{3/2}} = \frac{1}{r^2}\big[1 - (-1)\big] = \frac{2}{r^2}.

Therefore

B=μ0Ir4π⋅2r2=μ0I2πr.B = \frac{\mu_0 I r}{4\pi}\cdot\frac{2}{r^2} = \frac{\mu_0 I}{2\pi r}.

Proof (On-axis field of a circular loop from Biot–Savart). A circular loop of radius RR carries current II. Find B⃗\vec{B} at a point PP on the axis, a distance xx from the center. Each element I dℓ⃗I\,d\vec{\ell} is perpendicular to the line of length s=x2+R2s = \sqrt{x^2 + R^2} joining it to PP, so ∣dℓ⃗×r^∣=dℓ\lvert d\vec{\ell}\times\hat{r} \rvert = d\ell and

dB=μ0I4πdℓx2+R2.dB = \frac{\mu_0 I}{4\pi}\frac{d\ell}{x^2 + R^2}.

By symmetry, the components of dB⃗d\vec{B} perpendicular to the axis cancel when summed around the loop; only the axial components survive. The axial component is dBx=dBcos⁡αdB_x = dB\cos\alpha, where cos⁡α=R/x2+R2\cos\alpha = R/\sqrt{x^2 + R^2} (the angle between dB⃗d\vec{B} and the axis). Thus

dBx=μ0I4πdℓx2+R2⋅Rx2+R2=μ0IR4π(x2+R2)3/2 dℓ.dB_x = \frac{\mu_0 I}{4\pi}\frac{d\ell}{x^2 + R^2}\cdot\frac{R}{\sqrt{x^2 + R^2}} = \frac{\mu_0 I R}{4\pi (x^2 + R^2)^{3/2}}\,d\ell.

Everything in front of dℓd\ell is constant around the loop, so the integral just gives the circumference ∮dℓ=2πR\oint d\ell = 2\pi R:

B=μ0IR4π(x2+R2)3/2(2πR)=μ0IR22(x2+R2)3/2.B = \frac{\mu_0 I R}{4\pi (x^2 + R^2)^{3/2}}(2\pi R) = \frac{\mu_0 I R^2}{2(x^2 + R^2)^{3/2}}.

At the center, x=0x = 0:

B=μ0IR22(R2)3/2=μ0IR22R3=μ0I2R,B = \frac{\mu_0 I R^2}{2(R^2)^{3/2}} = \frac{\mu_0 I R^2}{2R^3} = \frac{\mu_0 I}{2R},

recovering the center-of-loop result.


Ampere’s law relates magnetic field circulation to enclosed current:

∮B⃗⋅dℓ⃗=μ0Ienc.\oint \vec{B}\cdot d\vec{\ell}=\mu_0 I_{\text{enc}}.

It is most useful with high symmetry, such as long straight wires, solenoids, and toroids. Choose an Amperian loop so B⃗\vec{B} is either constant and parallel to dℓ⃗d\vec{\ell} or perpendicular to it.

For a toroid with NN turns,

B=μ0NI2πrB=\frac{\mu_0 NI}{2\pi r}

inside the core, under the ideal toroid approximation.

Proof (Straight-wire field as an Ampère’s-law check). For an infinite straight wire, symmetry tells us B⃗\vec{B} has constant magnitude on any circle of radius rr centered on the wire and points tangent to that circle (circular field lines). Choose such a circle as the Amperian loop. Then B⃗∥dℓ⃗\vec{B}\parallel d\vec{\ell} everywhere, and BB is constant, so

∮B⃗⋅dℓ⃗=B∮dℓ=B(2πr).\oint\vec{B}\cdot d\vec{\ell} = B\oint d\ell = B(2\pi r).

The loop encloses the full current II, so Ampère’s law gives

B(2πr)=μ0I  ⇒  B=μ0I2πr,B(2\pi r) = \mu_0 I \;\Rightarrow\; B = \frac{\mu_0 I}{2\pi r},

matching the Biot–Savart result with far less work — symmetry did the integral for us.

Proof (Solenoid field from Ampère’s law). An ideal solenoid has nn turns per unit length carrying current II, with a uniform axial field inside and (ideally) zero field outside. Choose a rectangular Amperian loop with one side of length ℓ\ell inside the solenoid parallel to the axis, the opposite side outside, and two short sides crossing the wall.

BAmperianloop

Split ∮B⃗⋅dℓ⃗\oint\vec{B}\cdot d\vec{\ell} into the four legs:

  • Inside leg (parallel to B⃗\vec{B}): contributes BℓB\ell.
  • Outside leg: B⃗=0\vec{B} = 0, contributes 00.
  • Two crossing legs: B⃗\vec{B} is either zero (outside) or perpendicular to dℓ⃗d\vec{\ell} (inside), so each contributes 00.

Therefore

∮B⃗⋅dℓ⃗=Bℓ.\oint\vec{B}\cdot d\vec{\ell} = B\ell.

The current enclosed is the number of turns threading the loop, nℓn\ell, each carrying II:

Ienc=nℓI.I_{\text{enc}} = n\ell I.

Ampère’s law then gives

Bℓ=μ0nℓI  ⇒  B=μ0nI,B\ell = \mu_0 n\ell I \;\Rightarrow\; B = \mu_0 n I,

independent of position inside — confirming the field is uniform.

Example. A long cylindrical wire of radius aa carries a total current II spread uniformly over its cross-section, so the current density is J=I/(πa2)J = I/(\pi a^2). Find BB at radius r<ar < a inside the conductor.

By symmetry the field is again circular, so for an Amperian circle of radius r<ar < a, ∮B⃗⋅dℓ⃗=B(2πr)\oint\vec{B}\cdot d\vec{\ell} = B(2\pi r). But this loop encloses only the fraction of current inside radius rr:

Ienc=J (πr2)=Iπa2 πr2=Ir2a2.I_{\text{enc}} = J\,(\pi r^2) = \frac{I}{\pi a^2}\,\pi r^2 = I\frac{r^2}{a^2}.

Ampère’s law gives

B(2πr)=μ0Ir2a2  ⇒  B=μ0Ir2πa2.B(2\pi r) = \mu_0 I\frac{r^2}{a^2} \;\Rightarrow\; B = \frac{\mu_0 I r}{2\pi a^2}.

So inside the conductor B∝rB\propto r (rising linearly from zero on the axis), and at the surface r=ar = a this matches B=μ0I/(2πa)B = \mu_0 I/(2\pi a), the external field, as it must.


Two long parallel wires carrying currents I1I_1 and I2I_2 separated by distance dd exert forces on each other. The force per unit length is

FL=μ0I1I22πd.\frac{F}{L}=\frac{\mu_0 I_1I_2}{2\pi d}.

Currents in the same direction attract. Currents in opposite directions repel.

I1I2same-directioncurrentsattract

Proof (Force per length between parallel wires). Wire 1 carries I1I_1 and produces, at the location of wire 2 (distance dd away), a field of magnitude

B1=μ0I12πd.B_1 = \frac{\mu_0 I_1}{2\pi d}.

This field is perpendicular to wire 2. The force on a length LL of wire 2 (carrying I2I_2) is F⃗=I2L⃗×B⃗1\vec{F} = I_2\vec{L}\times\vec{B}_1, with magnitude (since L⃗⊥B⃗1\vec{L}\perp\vec{B}_1, sin⁡θ=1\sin\theta = 1):

F=I2LB1=I2Lμ0I12πd.F = I_2 L B_1 = I_2 L\frac{\mu_0 I_1}{2\pi d}.

Dividing by LL,

FL=μ0I1I22πd.\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi d}.

The result is symmetric in I1I_1 and I2I_2, as Newton’s third law requires. For the direction, apply the right-hand rule: if the currents are parallel (same direction), L⃗×B⃗1\vec{L}\times\vec{B}_1 points from wire 2 toward wire 1, so they attract; antiparallel currents repel.

Example. Two parallel wires d=0.020 md = 0.020\ \text{m} apart carry I1=10 AI_1 = 10\ \text{A} and I2=15 AI_2 = 15\ \text{A} in the same direction. Find the force per unit length and state whether it is attractive or repulsive.

FL=μ0I1I22πd=(4π×10−7)(10)(15)2π(0.020)=(2×10−7)(10)(15)0.020=3.0×10−50.020=1.5×10−3 N/m.\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi d} = \frac{(4\pi\times10^{-7})(10)(15)}{2\pi(0.020)} = \frac{(2\times10^{-7})(10)(15)}{0.020} = \frac{3.0\times10^{-5}}{0.020} = 1.5\times10^{-3}\ \text{N/m}.

Here I used μ02π=4π×10−72π=2×10−7 T⋅m/A\dfrac{\mu_0}{2\pi} = \dfrac{4\pi\times10^{-7}}{2\pi} = 2\times10^{-7}\ \text{T}\cdot\text{m/A}. Since the currents run the same direction, the force is attractive: 1.5×10−3 N1.5\times10^{-3}\ \text{N} per meter pulling the wires together.


Magnetic flux through a surface is

ΦB=∫B⃗⋅dA⃗.\Phi_B=\int \vec{B}\cdot d\vec{A}.

For a uniform field through a flat surface,

ΦB=BAcos⁡θ.\Phi_B=BA\cos\theta.

Magnetic flux becomes central in electromagnetic induction.


  1. Temporary placeholder FRQ for wiring/testing — replace with a real free-response question for this unit.

    (A)(A) State one key idea from this unit and explain it in your own words.

    (B)(B) Give a worked example or application of that idea.