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Unformatted text preview: Working with potentials rather than electric and magnetic fields allows Maxwell’s equations in a vacuum to be recast into the following secondorder partial differential equations (in phasor notation): ∇ 2 A + k 2 A = − μ ◦ J ∇ 2 φ + k 2 φ = − ρ/ǫ ◦ where the time dependence is bound up in k , the free space wavenumber: k = ω/c = ω √ μ ◦ ǫ ◦ = 2 π/λ The potential equations are coupled only by the fact that the current density J and charge density ρ obey the continuity equation ∇· J + jωρ = 0 . These are all examples of the inhomogeneous Helmholtz equation, which has a wellknown solution. Notice that the equation for the vector potential separates into three scalar equations for the three vector components of A and J in Cartesian coordinates. In the case of the elemental dipole where the current flows in one Cartesian direction, it is sufficient therefore to solve one scalar equation. ∇ 2 A z + k 2 A z = − μ ◦ J z (2.1) We view the right side of (2.1) as a source and the left side as a response. The general method of solution involves finding the response to a point source excitation, called a Greens function, and then constructing the solution to a particular problem from an appropriate superposition of point sources. In this case, the excitation is already a point source, and the Greens function is itself the solution we seek. We first solve the homogeneous (source free) problem. The overall symmetry of the problem suggests that the solution should depend only on the variable r . In spherical coordinates, this implies the following ordinary differential equation: 1 r 2 d dr r 2 dA z dr + k 2 A z = The solution is facilitated with the change of variables given by A z = ψ/r , yielding d 2 ψ dr 2 + k 2 ψ = 28 with the solutions ψ ( r ) = c 1 e − jkr + c 2 e jkr The two solutions represent spherically expanding and contracting wavefronts, and while both are mathematically valid, only the former is physically meaningful. The solution to the homogeneous problem, which holds everywhere except the origin where the elemental electric dipole is located, is then A z = c 1 e − jkr r All that remains is to determine the constant c 1 . This is done by reconsidering the inhomogeneous equation (with the source restored). Integrating the equation over a small spherical volume surrounding the origin with a radius r ◦ yields contintegraldisplay s ∇ A z · ˆ rds + integraldisplay v k 2 A z dv = − μ ◦ Idl where the divergence theorem has been used to convert one volume integral to a surface integral over the sphere and where the volume integral over the totally enclosed current element is Idl . By considering the limit where the radius r ◦ is made arbitrarily small, it is possible to make the term immediately to the left of the equal sign vanish, since the product A z dV ∼ r 2 ◦ . The surface integral term meanwhile evaluates to − 4 πc 1 in the limit that r ◦ ≪ λ . The constant is thereby set, and the solution for the vector potential due to an elemental dipole at the origin is found to be...
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 Spring '13
 HYSELL
 The Land, power density, Solid angle

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