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Figure 2.4: Non-deforming closed contour moving with velocity v through a magnetic
                        field B given in the laboratory (unprimed) coordinate system.



                        ways. A popular formulation of Faraday’s law, the emf formulation, revolves around the
                        concept of electromotive force. Unfortunately, various authors offer different definitions
                        of emf in a moving circuit.
                          Consider a non-deforming contour in space, moving with constant velocity v relative
                        to the laboratory frame (Figure 2.4). In terms of the laboratory fields we have the large-
                        scale form of Faraday’s law (2.141). The flux term on the right-hand side of this equation
                        can be written differently by employing the Helmholtz transport theorem (A.63). If a
                        non-deforming surface S moves with uniform velocity v relative to the laboratory frame,
                        and a vector field A(r, t) is expressed in the stationary frame, then the time derivative
                        of the flux of A through S is
                                       d                ∂A
                                            A · dS =      + v(∇· A) −∇ × (v × A) · dS.        (2.151)
                                       dt  S         S  ∂t

                        Using this with (2.141) we have

                                              d
                                     E · dl =−    B · dS +  v(∇· B) · dS −  ∇× (v × B) · dS.
                                              dt  S        S              S
                        Remembering that ∇· B = 0 and using Stokes’s theorem on the last term, we obtain
                                                               d            d (t)

                                             (E + v × B) · dl =−   B · dS =−                  (2.152)
                                                              dt  S           dt
                        where the magnetic flux


                                                         B · dS =  (t)
                                                        S
                        represents the flux of B through S. Following Sommerfeld [185], we may set

                                                       E = E + v × B
                                                         ∗
                        to obtain the kinematic form of Faraday’s law

                                                           d             d (t)

                                                  ∗
                                                 E · dl =−     B · dS =−      .               (2.153)
                                                          dt  S           dt

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