Propagation of Electromagnetic Waves in Media & Plasmas
Rigorous analytical treatment of classical electromagnetic wave propagation: the vector wave equation derivation from Maxwell's field equations, monochromatic plane waves, orthogonality and transverse nature of electric and magnetic fields, intrinsic wave impedance of free space, lossy propagation in conducting media, attenuation constant, skin depth and phase delay in metals, and dispersion relations and plasma cutoff frequencies in ionized gases.
§2.1 The Electromagnetic Wave Equations in Vacuum & Media
Derivation of the Vector Wave Equation
Consider source-free vacuum where charge density $\rho = 0$ and conduction current density $\mathbf{J} = 0$. Maxwell's equations reduce to:
- $\nabla \cdot \mathbf{E} = 0$
- $\nabla \cdot \mathbf{B} = 0$
- $\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t}$
- $\nabla \times \mathbf{B} = \mu_0 \epsilon_0 \frac{\partial \mathbf{E}}{\partial t}$
To decouple these coupled first-order partial differential equations, take the curl of Faraday's law:
Using the fundamental vector identity $\nabla \times (\nabla \times \mathbf{A}) \equiv \nabla(\nabla \cdot \mathbf{A}) - \nabla^2 \mathbf{A}$ on the left-hand side:
Since $\nabla \cdot \mathbf{E} = 0$ in vacuum, and substituting Ampère-Maxwell's law for $\nabla \times \mathbf{B}$:
Rearranging gives the celebrated homogeneous vector wave equation for the electric field:
Taking the curl of Ampère-Maxwell's law in identical fashion yields the wave equation for the magnetic field:
The Speed of Light and Maxwell's Synthesis
Comparing these to the standard 3D scalar wave equation $\nabla^2 \psi - \frac{1}{v^2} \frac{\partial^2 \psi}{\partial t^2} = 0$, the wave propagation speed $v$ is determined strictly by electromagnetic constants:
Substituting experimental values:
This exact match between the derived velocity of electromagnetic waves and the measured speed of light led James Clerk Maxwell to declare: "Light is an electromagnetic disturbance in the form of waves propagating through the electromagnetic field according to electromagnetic laws."
§2.2 Plane Waves, Transverse Nature, and Orthogonality of Fields
Monochromatic Plane Wave Solutions
A plane wave traveling in direction $\hat{\mathbf{k}}$ with wavevector $\mathbf{k} = k \hat{\mathbf{k}}$ and angular frequency $\omega$ is described in complex exponential notation by:
where physical fields are the real parts $\text{Re}\{\mathbf{E}\}$.
Substituting into the wave equation gives the vacuum dispersion relation:
Rigorous Proof of Transverse Nature (No Longitudinal Component)
Apply Gauss's law $\nabla \cdot \mathbf{E} = 0$:
Similarly, applying $\nabla \cdot \mathbf{B} = 0$:
Conclusion: Both $\mathbf{E}$ and $\mathbf{B}$ are strictly perpendicular to the propagation vector $\mathbf{k}$. Electromagnetic waves in unbounded homogeneous media are purely transverse waves ($E_k = 0, B_k = 0$).
Orthogonality and Phase Relationship
Applying Faraday's law $\nabla \times \mathbf{E} = -\frac{\partial \mathbf{B}}{\partial t}$:
This fundamental vector relation establishes that:
- $\mathbf{B}$ is perpendicular to $\mathbf{E}$ ($\mathbf{E} \cdot \mathbf{B} = 0$).
- $\mathbf{E}$, $\mathbf{B}$, and $\hat{\mathbf{k}}$ form an orthogonal right-handed triad:
- The magnitudes are related by $B_0 = \frac{E_0}{c}$.
- In vacuum, $\mathbf{E}$ and $\mathbf{B}$ oscillate exactly in phase, reaching crests and nodes at identical positions and times.
§2.3 Wave Impedance, Energy Flow, and Time-Averaged Poynting Flux
Intrinsic Wave Impedance of Free Space
The ratio of the transverse electric field to the transverse magnetic intensity $H = B/\mu_0$ defines the wave impedance:
Evaluating numerically:
The wave impedance of free space represents the resistance of vacuum to the generation of electric and magnetic flux. In a linear medium with permittivity $\epsilon$ and permeability $\mu$, the intrinsic impedance is $\eta = \sqrt{\mu / \epsilon}$.
Time-Averaged Energy Flux (Intensity)
For real sinusoidal fields traveling along $+z$:
The instantaneous Poynting vector is:
Since the time average of $\cos^2(\theta)$ over a full cycle is $\frac{1}{2}$, the time-averaged Poynting vector (wave intensity $I$) is:
Energy Density Distribution
The time-averaged electric energy density is:
The time-averaged magnetic energy density is:
Thus, $\langle u_E \rangle = \langle u_B \rangle$: electromagnetic energy is partitioned equally between electric and magnetic fields at all times in a plane wave.
§2.4 Propagation in Isotropic Non-Conducting Media
In a linear, homogeneous, isotropic dielectric medium with permittivity $\epsilon = \epsilon_r \epsilon_0$, permeability $\mu = \mu_r \mu_0$, and conductivity $\sigma = 0$:
Maxwell's equations yield the modified wave velocity:
where $n \equiv \sqrt{\epsilon_r \mu_r}$ is the index of refraction of the medium. For non-magnetic optical materials ($\mu_r \approx 1$), Maxwell's relation gives:
Wavelength and Wavevector in Matter
Because frequency $\omega$ is fixed by the driving source, the wavelength in the dielectric shrinks:
The wavevector increases:
The wave impedance becomes:
The time-averaged intensity in the dielectric is:
§2.5 Propagation in Conducting Media: Loss Tangent & Complex Wavevector
The Telegrapher-Type Wave Equation in Conductors
In an ohmic conducting medium with electric conductivity $\sigma$, free conduction currents flow according to Ohm's Law: $\mathbf{J}_f = \sigma \mathbf{E}$. There are no static free charges ($\rho_f = 0$).
Maxwell's curl equations become:
Taking the curl of Faraday's law:
Since $\nabla \cdot \mathbf{E} = 0$:
The first-order time derivative term $\mu \sigma \frac{\partial \mathbf{E}}{\partial t}$ acts as a dissipative frictional damping term that extracts energy from the wave and converts it into Joule heat.
Complex Wavevector Formulation
Substitute a monochromatic plane wave $\mathbf{E} = \mathbf{E}_0 e^{i(\tilde{k} z - \omega t)}$:
The ratio $\tan \delta \equiv \frac{\sigma}{\omega \epsilon}$ is known as the loss tangent. It quantifies the relative magnitude of conduction current compared to displacement current:
Let the complex wavevector be $\tilde{k} \equiv \beta + i \alpha$:
Equating real and imaginary parts:
Solving this system yields the exact analytical expressions:
The spatial electric field in the conductor is therefore:
The wave amplitude decays exponentially with distance into the conductor.
§2.6 Attenuation Constant, Phase Shift, and the Skin Depth (δ)
The Good Conductor Limit ($\sigma \gg \omega \epsilon$)
For metals and good conductors (such as copper, silver, aluminum, and sea water at radio frequencies), conduction current dwarfs displacement current:
Under this approximation, the term $\sqrt{1 + (\sigma/\omega\epsilon)^2} \approx \frac{\sigma}{\omega \epsilon}$, and the formulas for $\alpha$ and $\beta$ simplify dramatically:
Definition of Skin Depth ($\delta$)
The skin depth $\delta$ (also called penetration depth) is defined as the distance over which the wave amplitude drops by a factor of $1/e \approx 0.3679$ (36.8% of its surface value):
Over a depth of $z = 5\delta$, the wave amplitude decays to $e^{-5} \approx 0.0067$ (under 0.7%), meaning high-frequency currents are confined almost entirely to a microscopically thin outer shell of a conductor.
Table: Practical Skin Depths Across Frequencies
For pure copper ($\sigma = 5.8 \times 10^7 \text{ S/m}$, $\mu = \mu_0$):
| Frequency ($f$) | Skin Depth $\delta$ in Copper | Application / Impact | | :--- | :--- | :--- | | 50 Hz / 60 Hz | $9.38 \text{ mm}$ | AC mains power transmission (large cables require hollow or stranded conductors). | | 10 kHz | $0.66 \text{ mm}$ | Audio and induction heating frequencies. | | 1 MHz | $66 \, \mu\text{m}$ | AM radio broadcast frequencies. | | 100 MHz | $6.6 \, \mu\text{m}$ | FM radio and VHF communications. | | 10 GHz | $0.66 \, \mu\text{m}$ | X-band radar and microwave waveguides (requires surface silver plating). |
Phase Delay Between $\mathbf{E}$ and $\mathbf{B}$
From Faraday's law in a good conductor:
Since $\tilde{k} = \beta + i \alpha = \alpha(1 + i) = \alpha \sqrt{2} e^{i\pi/4}$:
Physical Result: In a good conductor, the magnetic field lags the electric field by a phase angle of $45^\circ$ ($\pi/4$ radians), and the magnetic energy density dramatically exceeds the electric energy density:
§2.7 Electromagnetic Waves in Ionized Gases (Plasmas) and Ionospheric Propagation
The Cold Plasma Dielectric Function
Consider an ionized gas (such as the Earth's ionosphere or interstellar plasma) consisting of free electrons (mass $m_e$, charge $-e$, density $n_e$) and heavy, immobile positive ions. In the presence of a monochromatic electric field $\mathbf{E}(t) = \mathbf{E}_0 e^{-i\omega t}$, the equation of motion for a conduction electron (neglecting damping collisions) is:
The induced macroscopic dipole polarization density is:
The electric displacement is:
The Plasma Frequency ($\omega_p$)
We define the characteristic electron plasma frequency:
In terms of frequency in Hertz:
where $n_e$ is in $\text{electrons/m}^3$.
The relative permittivity of the plasma is:
Dispersion Relation and Propagation Regimes
The wavevector in the plasma satisfies:
1. High Frequency Regime ($\omega > \omega_p$):
$k$ is purely real:
The wave propagates freely without attenuation. The phase velocity exceeds the speed of light:
The group velocity (signal energy velocity) is strictly less than $c$:
Notice that $v_p \cdot v_g = c^2$, satisfying special relativity.
2. Low Frequency Cutoff Regime ($\omega < \omega_p$):
$k$ becomes purely imaginary:
The fields decay exponentially: $\mathbf{E}(z, t) = \mathbf{E}_0 e^{-\kappa z} e^{-i\omega t}$. No real energy is propagated; instead, the wave undergoes total reflection at the plasma boundary.
Application to Radio Communications: The Earth's ionosphere has peak electron density $n_e \approx 10^{12} \text{ m}^{-3}$, giving a plasma critical frequency $f_p \approx 9 \text{ MHz}$. Shortwave radio signals ($3 - 30 \text{ MHz}$) below the critical frequency are totally reflected back to Earth, enabling global intercontinental communication without satellites. Satellite transmissions (GPS, 1.5 GHz) easily exceed $f_p$ and pass through the ionosphere unhindered.
📝 Chapter Worked Examples & Exercises
Complete analytical solutions & proofsA focused Nd:YAG laser beam ($\lambda = 1064\text{ nm}$) operates at an average output power of $P = 150\text{ W}$. It is focused down to a circular spot of radius $w_0 = 25\,\mu\text{m}$ in air. Calculate: (a) the laser beam intensity $I$, (b) the peak electric field amplitude $E_0$, (c) the peak magnetic field amplitude $B_0$, and (d) the radiation pressure $P_{\text{rad}}$ on a totally absorbing target placed at the focal spot.
Focusing the laser concentrates 150 watts into a flux of over 76 gigawatts per square meter.
The electric field exceeds the dielectric breakdown threshold of ambient air ($3\text{ MV/m}$), ionizing air molecules and generating a visible optical plasma spark.
The magnetic induction reaches 253 Gauss, illustrating the immense strength of focused optical fields.
Radiation pressure reaches several millibars, easily enough to trap and levitate microscopic dielectric beads in optical tweezers.
Seawater has electrical conductivity $\sigma = 4.0\text{ S/m}$, relative permittivity $\epsilon_r = 81$, and $\mu_r = 1$. (a) Determine whether seawater behaves as a good conductor or dielectric at $f = 75\text{ Hz}$ (Extremely Low Frequency, ELF) and at $f = 2.4\text{ GHz}$ (Wi-Fi). (b) Calculate the skin depth $\delta$ at $75\text{ Hz}$. (c) Calculate the depth $z$ at which a $75\text{ Hz}$ submarine communications signal is attenuated by $60\text{ dB}$ (power factor of $10^{-6}$).
At 75 Hz, seawater is an exceptional conductor (conduction current dominates by 7 orders of magnitude). At 2.4 GHz, seawater is a lossy dielectric.
The electromagnetic field amplitude decays by a factor of $1/e$ every 29 meters of seawater depth.
ELF signals at 75 Hz can successfully reach nuclear submarines operating submerged at depths up to 200 meters (660 feet) without surfacing.
For a microwave frequency of $f = 10\text{ GHz}$ propagating in copper ($\sigma = 5.8 \times 10^7\text{ S/m}$, $\mu = \mu_0$): (a) calculate the skin depth $\delta$, (b) calculate the phase velocity $v_p$ and wavelength $\lambda$ inside the copper, and (c) find the surface resistance $R_s = \frac{1}{\sigma \delta}$ per square.
At 10 GHz, the entire microwave current flows in an ultra-thin surface skin of just 661 nanometers.
In free space, a 10 GHz wave has $\lambda_0 = 3\text{ cm}$ and $v_p = c$. Inside the metal, the wave slows down to 41.5 km/s (a factor of 7200 slower), and its wavelength compresses to just 4.15 micrometers.
This non-zero surface resistance causes wall conduction loss and attenuation in microwave waveguides and cavity resonators.
The daytime ionospheric F2 layer has an electron density of $n_e = 1.5 \times 10^{12}\text{ m}^{-3}$. (a) Calculate the critical plasma frequency $f_p$. (b) For radio waves incident on the ionosphere at an angle of incidence $\theta_i = 65^\circ$ relative to the normal, use Snell's law to derive and calculate the Maximum Usable Frequency (MUF) that can still be reflected back to Earth (secant law).
Vertical incidence signals ($0^\circ$) at frequencies above 11.0 MHz will penetrate straight through the ionosphere into outer space.
This celebrated relation is known as Martyn's Secant Law for ionospheric radio reflection.
Because oblique incidence glances off the ionosphere, shortwave radio operators can communicate across continents at frequencies up to 26 MHz, well above the 11 MHz vertical critical frequency.