Consider \(\mathbf{E}\) and \(\mathbf{B}\) wave fields whose only dependence on \(z\) and \(t\) is included in the factor \(e^{i\left(\omega t-x_{1} \theta\right)}\). Further assume TE waves such that \(E_{z}=0\). Write out Maxwell's curl equations \((82.2)\) and \((8.2 .4)\) in cartesian components and show \((a)\) that all four transverse field components can be obtained from \(B_{t}\) by first-order partial differentiation and \((b)\) that \(B_{*}\) must be a solution of the Helmholtz equation \((8.7 .16)\). Thus the scalar function \(\phi\) of the text may be interpreted as proportional to \(B_{z}\) for TE waves or proportional to \(E_{s}\) for TM waves.

Short Answer

Expert verified
Short Answer: Using Maxwell's curl equations, we showed that all four transverse field components can be obtained from \(B_{t}\) by first-order partial differentiation with respect to \(x\), \(y\), and \(z\). Furthermore, we showed that \(B_{*}\) must be a solution of the Helmholtz equation, which implies that the scalar function \(\phi\) in the text may be interpreted as proportional to \(B_{z}\) for TE waves or proportional to \(E_{s}\) for TM waves.

Step by step solution

01

1. Rewrite the wave fields with the given dependence on \(z\) and \(t\)

The given dependence on \(z\) and \(t\) is included in the factor \(e^{i(\omega t-x_{1}\theta)}\). So, we can represent the electric and magnetic fields as follows: \(\mathbf{E} = \mathbf{E}_{t}(x,y)e^{i(\omega t-x_{1}\theta)}\) \(\mathbf{B} = \mathbf{B}_{t}(x,y)e^{i(\omega t-x_{1}\theta)}\) Where \(\mathbf{E}_{t}(x,y)\) and \(\mathbf{B}_{t}(x,y)\) are the transverse components of the electric and magnetic fields.
02

2. Write Maxwell's curl equations in cartesian components

Maxwell's curl equations are: (8.2.2) \(\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t}\) (8.2.4) \(\nabla \times \mathbf{B} = \mu_0 \varepsilon_0 \frac{\partial \mathbf{E}}{\partial t}\) We need to write these equations in cartesian components. Since we are dealing with TE waves, \(E_z=0\). Therefore, the equations become: \(\frac{\partial E_y}{\partial x} - \frac{\partial E_x}{\partial y} = -\frac{\partial B_z}{\partial t}\) \(\frac{\partial B_z}{\partial x} - \frac{\partial B_x}{\partial z} = \mu_0 \varepsilon_0 \frac{\partial E_y}{\partial t}\) \(\frac{\partial B_y}{\partial z} - \frac{\partial B_z}{\partial y} = \mu_0 \varepsilon_0 \frac{\partial E_x}{\partial t}\) Now, we will use these equations to prove the required conditions for both (a) and (b).
03

3. Show that all four transverse field components can be obtained from \(B_{t}\)

Using the given dependence on \(z\) and \(t\) for \(\mathbf{E}\) and \(\mathbf{B}\), we can differentiate Maxwell's curl equations in Cartesian components with respect to \(t\) and \(z\). We get: (1) \(\frac{\partial E_y}{\partial x} - \frac{\partial E_x}{\partial y} = -i\omega B_z e^{i(\omega t-x_{1}\theta)}\) (2) \(\frac{\partial B_z}{\partial x} - \frac{\partial B_x}{\partial z} = -i x_{1}\theta E_y e^{i(\omega t-x_{1}\theta)}\) (3) \(\frac{\partial B_y}{\partial z} - \frac{\partial B_z}{\partial y} = -i x_{1}\theta E_x e^{i(\omega t-x_{1}\theta)}\) We can see from equations (1), (2), and (3) that all four transverse field components (\(E_y\), \(E_x\), \(B_y\), and \(B_x\)) can be obtained from the transverse field component \(B_{t}\) by first-order partial differentiation with respect to \(x\), \(y\), and \(z\).
04

4. Show that \(B_{*}\) must be a solution of the Helmholtz equation (8.7.16)

The Helmholtz equation is given by: (8.7.16) \((\nabla^2 + k^2)B_{*} = 0\) where \(k=\omega\sqrt{\mu_0 \varepsilon_0}\) is the wave number. To show that \(B_{*}\) must be a solution of the Helmholtz equation, we need to substitute the given dependence on \(z\), \(t\), and use Maxwell's curl equations. Using the curl of (8.2.4) equation, we get: \(\nabla \times (\nabla \times \mathbf{B}) = \nabla \times (\mu_0 \varepsilon_0 \frac{\partial \mathbf{E}}{\partial t})\) Simplifying and writing in cartesian components, we get: (4) \(\nabla^2 B_z = \mu_0 \varepsilon_0 \frac{\partial^2 B_z}{\partial t^2}\) Now we substitute the given dependence on \(z\) and \(t\) in equation (4): \((\nabla^2 + k^2) B_z e^{i(\omega t-x_{1}\theta)} = 0\) This implies that the \(B_{*}\) must be a solution of the Helmholtz equation \((8.7.16)\). In conclusion, we have shown that all four transverse field components can be obtained from \(B_{t}\) by first-order partial differentiation and that \(B_{*}\) must be a solution of the Helmholtz equation. This means that the scalar function \(\phi\) in the text may be interpreted as proportional to \(B_{z}\) for TE waves or proportional to \(E_{s}\) for TM waves.

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Most popular questions from this chapter

The treatment in the text tacitly assumes that the interior of the waveguide has the electromagnetic properties of vacuum. Show that if the waveguide is filled with a material of relative permittivity \(\pi_{e}\) and permeability \(\pi_{m}\), all equations remain valid if \(c\) is replaced by \(c^{\prime}\) of \((8.2 .21)\) and \(\lambda_{9}\) in \((8.7 .20)\) is replaced by \(\lambda^{\prime}=2 \pi c^{\prime} / \omega\).

For normal incidence and nonmagnetic materials show that the power coefficients \((8.6 .38)\) and \((8.6 .39)\) reduce to $$ \begin{aligned} &R_{p}=\left(\frac{n-1}{n+1}\right)^{x} \\ &T_{p}=\frac{4 n}{(n+1)^{2}} \end{aligned} $$ where \(n=c_{1} / c_{2}=Z_{01} / Z_{02}\) is the relative refractive index. Account for the difference in sign between the amplitude reflection coefficients \((8.6 .28)\) and \((8.6 .36)\) at normal incidence (see footnote, page 102). Compare with equations (1.9.6), (4.2.15), and (5.6.13).

Consider two unbounded plane waves whose vector wave numbers \(k_{1}\) and \(\kappa_{2}\left(\left.\right|_{1,2} \mid=\right.\) \(\omega / c)\) define a plane and whose electric fields are polarized normal to the plane. (a) Show that the superposition of these two plane waves is a wave traveling in the direction bisecting the angle \(\alpha\) between \({ }_{1}{ }_{1}\) and \({ }_{k}\) and that the \(\mathbf{E}\) field vanishes on a set of nodal planes spaced \(a=\) \(\lambda_{0} / 2 \sin \frac{1}{2} \alpha\) apart. \((b)\) Show that plane conducting walls can be placed at two adjacent nodal planes without violating the electromagnetic boundary conditions and likewise that a second pair of conducting walls of arbitrary separation \(b\) can be introduced to construct a rectangular waveguide of cross section \(a\) by \(b\), propagating the \(T E_{10}\) mode. Thus establish that the TE \(_{10}\) mode (more generally, the TE \(_{10}\) modes) may be interpreted as the superposition of two plane waves making the angle \(\frac{1}{2} \alpha\) with the waveguide axis and undergoing multiple reflections from the sidewalls. Note: The situation is directly analogous to that discussed in Sec. 2.4. Higherorder TE modes \((m>0)\) and TM modes may be described similarly as a superposition of four plane waves.

Use Gauss' and Stokes' theorems (Appendix A) to convert Maxwell's differential equations for vacuum, \((82.1)\) to \((8.2 .4)\), to their integral form $$ \begin{aligned} &\oint_{S} \mathbf{E} \cdot d \mathbf{S}=\frac{q}{\epsilon_{0}} \\ &\oint_{L} \mathbf{E} \cdot d \mathbf{l}=-\frac{d \Phi_{m}}{d t} \\ &\oint_{S} \mathbf{B} \cdot d \mathbf{S}=0 \\ &\oint_{L} \mathbf{B} \cdot d \mathbf{l}=\mu_{0} I+\mu_{0} \frac{d \Phi_{*}}{d t} \end{aligned} $$ † See Sec. \(5.4\) and Prob. 8.2.4. where the closed surface \(S\) contains the net charge \(q\) and the closed line (loop) \(L\) is linked by the net current \(I\), the magnetic flux \(\Phi_{m}=\int \mathbf{B} \cdot d \mathbf{S}\), and the electric flux \(\Phi_{e}=\epsilon_{0} \int \mathbf{E} \cdot d \mathbf{S}\). Note: The corresponding equations for a general electromagnetic medium are developed in Prob. \(8.6 .1 .\)

Show that the reflection coefficients for the magnetic field amplitudes (either B or H) are identical with \((8.6 .28)\) and \((8.6 .36)\), while the transmission coefficients differ from (8.6.29) and \((8.6 .37)\) by the ratio of the wave impedances of the two media, \((8.5 .18)\) or \((8.5 .19)\). Specifically, show that for the B field, $$ \frac{T_{B}}{T_{\boldsymbol{B}}}=\frac{c_{1}}{c_{2}}=\left(\frac{\kappa_{n k} k_{m 1}}{\kappa_{A 1} k_{m 1}}\right)^{1 / 2}, $$ which is the relative refractive index for the two media; for the \(\mathbf{H}\) field, $$ \frac{T_{H}}{T_{E}}=\frac{Z_{61}}{Z_{42}}=\left(\frac{\kappa_{A 1 \pi_{m 1}}}{\kappa_{A 1 K_{m 2}}}\right)^{1 / 2} $$ Justify the cosine ratio in (8.6.39).

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