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NCERT Exemplar · Q26

Q.A metallic ring of mass mm and radius ll (ring being horizontal) is falling under gravity in a region having a magnetic field. If zz is the vertical direction, the zz-component of the magnetic field is Bz=B0(1+λz)B_z = B_0(1 + \lambda z). If RR is the resistance of the ring and if the ring falls with a velocity vv, find the energy lost in the resistance. If the ring has reached a constant velocity, use the conservation of energy to determine vv in terms of mm, BB, λ\lambda and acceleration due to gravity gg.

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The falling ring experiences a changing magnetic flux due to the vertical gradient in BzB_z, inducing an emf and current. The energy lost in resistance per unit time is I2RI^2 R, and at terminal velocity, the gravitational power mgvmgv equals the Joule heating power, giving v=mgRπ2B02λ2l4v = \frac{mgR}{\pi^2 B_0^2 \lambda^2 l^4}.

Why Motional Emf Works Here

The ring falls through a magnetic field that varies linearly with height: Bz=B0(1+λz)B_z = B_0(1 + \lambda z). Even though the field is not uniform, the key is that the ring moves — so the magnetic flux through its area changes with time. That change induces an emf, which drives a current, and the resistance dissipates energy as heat.

The standard motional emf formula E=Blv\mathcal{E} = Blv applies to a straight wire cutting field lines. Here we have a circular loop, but the same physics holds: the emf around the loop equals the rate of change of magnetic flux through it.

E=−dΦdt\mathcal{E} = -\frac{d\Phi}{dt}

Step-by-step solution

1. Find the magnetic flux through the ring

The ring is horizontal, so its area vector points vertically. The flux is:

Φ=∫B⋅dA=Bz⋅(πl2)\Phi = \int \mathbf{B} \cdot d\mathbf{A} = B_z \cdot (\pi l^2)

Since Bz=B0(1+λz)B_z = B_0(1 + \lambda z) and the ring is small enough that BzB_z is essentially constant over its area (the field varies only with zz, and the ring’s radius is fixed), we get:

Φ=B0(1+λz)⋅πl2\Phi = B_0(1 + \lambda z) \cdot \pi l^2

2. Induced emf from motion

As the ring falls, zz changes at rate v=dz/dtv = dz/dt. So:

E=−dΦdt=−B0πl2⋅λdzdt=−B0πl2λv\mathcal{E} = -\frac{d\Phi}{dt} = -B_0 \pi l^2 \cdot \lambda \frac{dz}{dt} = -B_0 \pi l^2 \lambda v

The magnitude of the induced emf is:

E=B0πl2λv\mathcal{E} = B_0 \pi l^2 \lambda v

Tip

The minus sign tells us the direction (Lenz’s law), but for energy calculations we only need the magnitude — the current will oppose the change, but the power dissipated depends on ∣E∣|\mathcal{E}|.

3. Current and power dissipated

Ohm’s law gives the induced current:

I=ER=B0πl2λvRI = \frac{\mathcal{E}}{R} = \frac{B_0 \pi l^2 \lambda v}{R}

The power lost as heat in the resistance is:

Plost=I2R=(B0πl2λvR)2R=B02π2l4λ2v2RP_{\text{lost}} = I^2 R = \left( \frac{B_0 \pi l^2 \lambda v}{R} \right)^2 R = \frac{B_0^2 \pi^2 l^4 \lambda^2 v^2}{R}

This is the energy lost per unit time. …

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