Wave phase; the minus sign indicates propagation in +z
rad
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, the time period is T=2π/ω, and the phase ωt−βz advances in the +z direction.
The propagation direction is
E×H.
Uniform plane wave with mutually perpendicular electric field, magnetic field and propagation direction.
How to read the figure. The wave travels along +z, while E points along x and H points along y. Thus E⊥H, both fields are transverse to the propagation axis, and E×H points in the direction of travel.
The average power crossing a surface A is the normal flux of Sav:
Pav=∫ASav⋅dS.
For a uniform wave incident at angle θ to the surface normal,
Pav=SavAcosθ.
Power flow for oblique fields.
How to read the figure. Only the component of Sav parallel to the area normal crosses the receiving surface. The collected power is maximum at normal incidence and decreases by the projection factor cosθ.
A coaxial line gives a practical example of the cross product S=E×H.
Power flow in a coaxial line.
How to read the figure. Between the conductors, E is radial and 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=21εE2,wm=21μH2.
With dS directed outward,
−∮∂VS⋅dS=dtd∫V(we+wm)dV+∫VJ⋅EdV.
Equivalently,
Pin−Pout=dtdWem+PJ.
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⋅EdV; any remaining power leaves the volume.
With the ejωt convention, the reusable phasor differentiation rules are
∂t∂⟶jω,∂t2∂2⟶−ω2.
For a passive medium, choose the square-root branch with α≥0 so that field amplitude does not grow with propagation distance. The general one-dimensional solution is
E(z)=E0+e−γz+E0−eγz,
where the first term travels in +z and the second travels in −z.
How to read the figure. The sinusoid continues to advance in phase according to β, while its upper and lower envelopes shrink as e−αz. Thus α controls amplitude loss and β controls phase change.
Medium regimes classified by conductivity and frequency.
How to read the figure. Move from left to right as p=σ/(ωε)=tanδ increases: displacement current dominates for p≪1, neither term may be neglected near p=1, and conduction current dominates for p≫1. If σ and ε remain constant, increasing frequency moves the material toward the left.
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 and τ.
For a perfect electric conductor, η2→0 and hence Γ=−1. The tangential electric field vanishes at the surface, and the incident and reflected waves form standing-wave envelopes:
Standing-wave envelopes at a perfect electric conductor.
How to read the figure. At the conductor surface, d=0, the electric field has a node and the magnetic field has an antinode. Their neighboring extrema are separated by λ/4.
At oblique incidence, the law of reflection and Snell’s law are
θr=θi,n1sinθi=n2sinθt.
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.
For a good conductor, σ≫ωε, so its propagation constant reduces to
γ≈jωμσ=(1+j)2ωμσ.
Hence
α≈β≈2ωμσ.
Defining skin depth by e−αδs=e−1 gives
Skin depth is
δs=α1=ωμσ2=πfμσ1.
Higher frequency, permeability or conductivity gives smaller skin depth.
Skin depth in a conducting medium.
How to read the figure. At z=δs, field and current-density amplitudes have fallen to e−1 of their surface values. Power is proportional to field amplitude squared, so it falls as e−2z/δs.
For sinusoidal fields in a conductor, the average Joule-loss density is
pJ,av(z)=21σ∣E(z)∣2∝e−2z/δs.
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.