Page 168 - Electromagnetics
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while the point forms are
                                                       ∇× H(r) = J(r),                        (3.120)
                                                        ∇· B(r) = 0.                          (3.121)

                        Note the interesting dichotomy between the electrostatic field equations and the magne-
                        tostatic field equations. Whereas the electrostatic field exhibits zero curl and a divergence
                        proportional to the source (charge), the magnetostatic field has zero divergence and a
                        curl proportional to the source (current). Because the vector relationship between the
                        magnetostatic field and its source is of a more complicated nature than the scalar rela-
                        tionship between the electrostatic field and its source, more effort is required to develop a
                        strong understanding of magnetic phenomena. Also, it must always be remembered that
                        although the equations describing the electrostatic and magnetostatic field sets decou-
                        ple, the phenomena themselves remain linked. Since current is moving charge, electrical
                        phenomena are associated with the establishment of the current that supports a magne-
                        tostatic field. We know, for example, that in order to have current in a wire an electric
                        field must be present to drive electrons through the wire.

                        The magnetic scalar potential.   Under certain conditions the equations of magne-
                        tostatics have the same form as those of electrostatics. If J = 0 in a region V , the
                        magnetostatic equations are
                                                        ∇× H(r) = 0,                          (3.122)
                                                         ∇· B(r) = 0;                         (3.123)
                        compare with (3.5)–(3.6) when ρ = 0. Using (3.122)we can define a magnetic scalar
                        potential   m :
                                                         H =−∇  m .                           (3.124)
                        The negative sign is chosen for consistency with (3.30). We can then define a magnetic
                        potential difference between two points as

                                       P 2          P 2               P 2
                             V m21 =−    H · dl =−    −∇  m (r) · dl =  d  m (r) =   m (r 2 ) −   m (r 1 ).
                                      P 1          P 1               P 1
                        Unlike the electrostatic potential difference, V m21  is not unique. Consider Figure 3.17,
                        which shows a plane passing through the cross-section of a wire carrying total current I.
                        Although there is no current within the region V (external to the wire), equation (3.118)
                        still gives

                                                      H · dl −  H · dl = I.
                                                      2         3
                        Thus

                                                      H · dl =  H · dl + I,
                                                      2         3

                        and the integral  H · dl is not path-independent. However,


                                                        H · dl =  H · dl
                                                        1         2
                        since no current passes through the surface bounded by   1 −   2 . So we can artificially
                        impose uniqueness by demanding that no path cross a cut such as that indicated by the
                        line L in the figure.




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