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Electromagnetic Waves and Materials

In a source-free, linear, homogeneous medium,

∇×E=−μ∂H∂t,∇×H=σE+ε∂E∂t.\nabla\times\mathbf{E}=-\mu\frac{\partial\mathbf{H}}{\partial t}, \qquad \nabla\times\mathbf{H}=\sigma\mathbf{E}+\varepsilon\frac{\partial\mathbf{E}}{\partial t}.

For a source-free homogeneous medium, Gauss’s laws and the constant material parameters imply

∇⋅E=0,∇⋅H=0.\nabla\cdot\mathbf E=0, \qquad \nabla\cdot\mathbf H=0.

These conditions remove the gradient-divergence terms when the double-curl identity is applied.

The resulting electric-field wave equation is

∇2E=μσ∂E∂t+με∂2E∂t2.\boxed{ \nabla^2\mathbf{E}=\mu\sigma\frac{\partial\mathbf{E}}{\partial t} +\mu\varepsilon\frac{\partial^2\mathbf{E}}{\partial t^2}. }

For a lossless medium, σ=0\sigma=0:

∇2E−με∂2E∂t2=0.\nabla^2\mathbf{E}-\mu\varepsilon\frac{\partial^2\mathbf{E}}{\partial t^2}=0.

Therefore,

∇2H=μσ∂H∂t+με∂2H∂t2.\boxed{ \nabla^2\mathbf{H} =\mu\sigma\frac{\partial\mathbf{H}}{\partial t} +\mu\varepsilon\frac{\partial^2\mathbf{H}}{\partial t^2} }.

For a lossless medium, σ=0\sigma=0:

∇2H−με∂2H∂t2=0.\boxed{ \nabla^2\mathbf{H} -\mu\varepsilon\frac{\partial^2\mathbf{H}}{\partial t^2}=0 }.

For a wave travelling in the +z+z direction,

E=E0cos⁡(ωt−βz)ax,H=H0cos⁡(ωt−βz)ay.\mathbf{E}=E_0\cos(\omega t-\beta z)\mathbf{a}_x, \qquad \mathbf{H}=H_0\cos(\omega t-\beta z)\mathbf{a}_y.

Symbols used:

SymbolMeaningSI unit
E(z,t)\mathbf{E}(z,t)Instantaneous electric-field vectorV/m\mathrm{V/m}
H(z,t)\mathbf{H}(z,t)Instantaneous magnetic-field-intensity vectorA/m\mathrm{A/m}
E0E_0Peak electric-field amplitudeV/m\mathrm{V/m}
H0H_0Peak magnetic-field amplitudeA/m\mathrm{A/m}
ω=2πf\omega=2\pi fAngular frequency, where ff is frequencyrad/s\mathrm{rad/s}
ttTimes\mathrm{s}
β=2π/λ\beta=2\pi/\lambdaPhase constant, where λ\lambda is wavelengthrad/m\mathrm{rad/m}
zzPosition measured along the propagation axism\mathrm{m}
ax\mathbf{a}_xUnit vector in the +x+x direction; direction of E\mathbf Edimensionless
ay\mathbf{a}_yUnit vector in the +y+y direction; direction of H\mathbf Hdimensionless
ωt−βz\omega t-\beta zWave phase; the minus sign indicates propagation in +z+zrad\mathrm{rad}

Time-domain snapshots of a propagating sinusoidal wave.

Time-domain snapshots of a propagating sinusoidal wave.

How to read the figure. The left panel holds time fixed and shows the spatial waveform at successive instants; the right panel holds position fixed and shows the field oscillating in time. The spatial period is λ=2π/β\lambda=2\pi/\beta, the time period is T=2π/ωT=2\pi/\omega, and the phase ωt−βz\omega t-\beta z advances in the +z+z direction.

The propagation direction is

E×H.\mathbf{E}\times\mathbf{H}.

Uniform plane wave with mutually perpendicular electric field, magnetic field and propagation direction.

Uniform plane wave with mutually perpendicular electric field, magnetic field and propagation direction.

How to read the figure. The wave travels along +z+z, while E\mathbf E points along xx and H\mathbf H points along yy. Thus E⊥H\mathbf E\perp\mathbf H, both fields are transverse to the propagation axis, and E×H\mathbf E\times\mathbf H points in the direction of travel.

In a lossless medium,

v=1με,β=ωμε,η=EH=με.v=\frac{1}{\sqrt{\mu\varepsilon}}, \qquad \beta=\omega\sqrt{\mu\varepsilon}, \qquad \eta=\frac{E}{H}=\sqrt{\frac{\mu}{\varepsilon}}.

In free space,

c=1μ0ε0,η0=μ0ε0≈377 Ω.c=\frac{1}{\sqrt{\mu_0\varepsilon_0}}, \qquad \eta_0=\sqrt{\frac{\mu_0}{\varepsilon_0}}\approx377\ \Omega.

Its instantaneous value is

S=E×H.\mathbf{S}=\mathbf{E}\times\mathbf{H}.

For phasors,

Sav=12Re⁡(E×H∗).\mathbf{S}_{\text{av}}=\frac{1}{2}\operatorname{Re}\left(\mathbf{E}\times\mathbf{H}^*\right).

The average power crossing a surface AA is the normal flux of Sav\mathbf S_{\text{av}}:

Pav=∫ASav⋅dS.P_{\text{av}}=\int_A\mathbf S_{\text{av}}\cdot d\mathbf S.

For a uniform wave incident at angle θ\theta to the surface normal,

Pav=SavAcos⁡θ.P_{\text{av}}=S_{\text{av}}A\cos\theta.

Power flow for oblique fields.

Power flow for oblique fields.

How to read the figure. Only the component of Sav\mathbf S_{\text{av}} parallel to the area normal crosses the receiving surface. The collected power is maximum at normal incidence and decreases by the projection factor cos⁡θ\cos\theta.

A coaxial line gives a practical example of the cross product S=E×H\mathbf S=\mathbf E\times\mathbf H.

Power flow in a coaxial line.

Power flow in a coaxial line.

How to read the figure. Between the conductors, E\mathbf E is radial and H\mathbf H is azimuthal, so their cross product points along the cable. Electromagnetic energy is transported through the dielectric between the conductors.

For linear media,

we=12εE2,wm=12μH2.w_e=\frac{1}{2}\varepsilon E^2, \qquad w_m=\frac{1}{2}\mu H^2.

With dSd\mathbf S directed outward,

−∮∂VS⋅dS=ddt∫V(we+wm) dV+∫VJ⋅E dV.-\oint_{\partial V}\mathbf S\cdot d\mathbf S =\frac{d}{dt}\int_V(w_e+w_m)\,dV +\int_V\mathbf J\cdot\mathbf E\,dV.

Equivalently,

Pin−Pout=dWemdt+PJ.P_{\text{in}}-P_{\text{out}} =\frac{dW_{\text{em}}}{dt}+P_J.

Poynting theorem control volume.

Poynting theorem control volume.

How to read the figure. Power entering the control volume either increases the stored electric and magnetic energy or is transferred to matter through PJ=∫VJ⋅E dVP_J=\int_V\mathbf J\cdot\mathbf E\,dV; any remaining power leaves the volume.

AspectPermittivityPermeability
Quantity and field relationε\varepsilon; D=εE\mathbf D=\varepsilon\mathbf Eμ\mu; B=μH\mathbf B=\mu\mathbf H
Physical meaningRelates electric flux density to electric field and indicates how strongly the medium polarizesRelates magnetic flux density to magnetic field and indicates how strongly the medium supports magnetic flux
SI unitfarad per metre, F/m\mathrm{F/m}henry per metre, H/m\mathrm{H/m}
Relative value and meaningεr=ε/ε0\varepsilon_r=\varepsilon/\varepsilon_0: electric response relative to vacuum; for the same E\mathbf E, the material has εr\varepsilon_r times the vacuum electric flux densityμr=μ/μ0\mu_r=\mu/\mu_0: magnetic response relative to vacuum; for the same H\mathbf H, the material has μr\mu_r times the vacuum magnetic flux density
Free-space referenceε0≈8.854×10−12 F/m\varepsilon_0\approx8.854\times10^{-12}\ \mathrm{F/m} and εr=1\varepsilon_r=1μ0≈1.257×10−6 H/m\mu_0\approx1.257\times10^{-6}\ \mathrm{H/m} and μr=1\mu_r=1

Propagation Constant and Intrinsic Impedance

Section titled “Propagation Constant and Intrinsic Impedance”

The propagation constant is

γ=α+jβ=jωμ(σ+jωε).\boxed{ \gamma=\alpha+j\beta =\sqrt{j\omega\mu(\sigma+j\omega\varepsilon)} }.

With the ejωte^{j\omega t} convention, the reusable phasor differentiation rules are

∂∂t⟶jω,∂2∂t2⟶−ω2.\frac{\partial}{\partial t}\longrightarrow j\omega, \qquad \frac{\partial^2}{\partial t^2}\longrightarrow-\omega^2.

For a passive medium, choose the square-root branch with α≥0\alpha\ge0 so that field amplitude does not grow with propagation distance. The general one-dimensional solution is

E~(z)=E0+e−γz+E0−eγz,\widetilde{\mathbf E}(z) =\mathbf E_0^+e^{-\gamma z}+\mathbf E_0^-e^{\gamma z},

where the first term travels in +z+z and the second travels in −z-z.

For propagation in the +z+z direction,

E~(z)=E0e−γz=E0e−αze−jβz,E(z,t)=E0e−αzcos⁡(ωt−βz).\widetilde E(z)=E_0e^{-\gamma z}=E_0e^{-\alpha z}e^{-j\beta z}, \qquad E(z,t)=E_0e^{-\alpha z}\cos(\omega t-\beta z).

Attenuating wave in a lossy medium.

Attenuating wave in a lossy medium.

How to read the figure. The sinusoid continues to advance in phase according to β\beta, while its upper and lower envelopes shrink as e−αze^{-\alpha z}. Thus α\alpha controls amplitude loss and β\beta controls phase change.

It is

ηc=jωμσ+jωε.\eta_c=\sqrt{\frac{j\omega\mu}{\sigma+j\omega\varepsilon}}.
MediumConditionMain result
Perfect dielectricσ=0\sigma=0α=0\alpha=0, η\eta real
Lossless mediumno conduction lossphase changes, amplitude constant
Lossy dielectricfinite σ\sigmaattenuation and phase shift both occur
Good conductorσ≫ωε\sigma\gg\omega\varepsilonfield decays rapidly with depth

Medium regimes classified by conductivity and frequency.

Medium regimes classified by conductivity and frequency.

How to read the figure. Move from left to right as p=σ/(ωε)=tan⁡δp=\sigma/(\omega\varepsilon)=\tan\delta increases: displacement current dominates for p≪1p\ll1, neither term may be neglected near p=1p=1, and conduction current dominates for p≫1p\gg1. If σ\sigma and ε\varepsilon remain constant, increasing frequency moves the material toward the left.

For a good conductor,

α≈β≈πfμσ,ηc≈(1+j)ωμ2σ.\alpha\approx\beta\approx\sqrt{\pi f\mu\sigma}, \qquad \eta_c\approx(1+j)\sqrt{\frac{\omega\mu}{2\sigma}}.

For a wave incident normally from medium 1 onto medium 2, the electric-field reflection and transmission coefficients are

Γ=Er0Ei0=η2−η1η2+η1,au=Et0Ei0=2η2η1+η2=1+Γ.\Gamma=\frac{E_{r0}}{E_{i0}} =\frac{\eta_2-\eta_1}{\eta_2+\eta_1}, \qquad au=\frac{E_{t0}}{E_{i0}} =\frac{2\eta_2}{\eta_1+\eta_2}=1+\Gamma.

Normal incidence on an impedance discontinuity.

Normal incidence on an impedance discontinuity.

How to read the figure. The incident wave approaches the boundary in medium 1, the reflected wave returns through medium 1, and the transmitted wave continues through medium 2. The impedance change determines their amplitude ratios through Γ\Gamma and τ\tau.

For a perfect electric conductor, η2→0\eta_2\to0 and hence Γ=−1\Gamma=-1. The tangential electric field vanishes at the surface, and the incident and reflected waves form standing-wave envelopes:

∣E(d)∣Ei0=2∣sin⁡(β1d)∣,∣H(d)∣Ei0/η1=2∣cos⁡(β1d)∣.\frac{|E(d)|}{E_{i0}}=2|\sin(\beta_1d)|, \qquad \frac{|H(d)|}{E_{i0}/\eta_1}=2|\cos(\beta_1d)|.

Standing-wave envelopes at a perfect electric conductor.

Standing-wave envelopes at a perfect electric conductor.

How to read the figure. At the conductor surface, d=0d=0, the electric field has a node and the magnetic field has an antinode. Their neighboring extrema are separated by λ/4\lambda/4.

At oblique incidence, the law of reflection and Snell’s law are

θr=θi,n1sin⁡θi=n2sin⁡θt.\displaystyle\theta_r=\theta_i, \qquad n_1\sin\theta_i=n_2\sin\theta_t.

Oblique reflection and refraction at a plane boundary.

Oblique reflection and refraction at a plane boundary.

How to read the figure. The incident, reflected, and transmitted wave vectors lie in the plane of incidence. Every angle is measured from the interface normal, not from the interface itself.

Inside a conductor, field and current density decrease approximately as

J(z)=J0e−z/δs.J(z)=J_0e^{-z/\delta_s}.

For a good conductor, σ≫ωε\sigma\gg\omega\varepsilon, so its propagation constant reduces to

γ≈jωμσ=(1+j)ωμσ2.\gamma\approx\sqrt{j\omega\mu\sigma} =(1+j)\sqrt{\frac{\omega\mu\sigma}{2}}.

Hence

α≈β≈ωμσ2.\alpha\approx\beta\approx\sqrt{\frac{\omega\mu\sigma}{2}}.

Defining skin depth by e−αδs=e−1e^{-\alpha\delta_s}=e^{-1} gives

Skin depth is

δs=1α=2ωμσ=1πfμσ.\delta_s=\frac{1}{\alpha}=\sqrt{\frac{2}{\omega\mu\sigma}} =\frac{1}{\sqrt{\pi f\mu\sigma}}.

Higher frequency, permeability or conductivity gives smaller skin depth.

Skin depth in a conducting medium.

Skin depth in a conducting medium.

How to read the figure. At z=δsz=\delta_s, field and current-density amplitudes have fallen to e−1e^{-1} of their surface values. Power is proportional to field amplitude squared, so it falls as e−2z/δse^{-2z/\delta_s}.

For sinusoidal fields in a conductor, the average Joule-loss density is

pJ,av(z)=12σ∣E~(z)∣2∝e−2z/δs.p_{J,\text{av}}(z) =\frac{1}{2}\sigma|\widetilde E(z)|^2 \propto e^{-2z/\delta_s}.

Power penetration and loss under skin effect.

Power penetration and loss under skin effect.

How to read the figure. Average Poynting flux crosses the conductor surface and is converted to Joule heat. Because the fields decay rapidly with depth, most of this loss is concentrated within a few skin depths of the surface.

Because the effective current-carrying area shrinks with frequency, AC resistance, feeder attenuation, conductor heating and waveguide-wall loss all increase. RF conductors therefore use smooth, highly conductive surfaces, low-resistance joints and adequate circumference. Silver plating can reduce surface resistance, hollow conductors avoid unused bulk at microwave frequencies, and Litz wire can reduce skin and proximity effects at lower RF frequencies.