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Learn/Module 1

Electromagnetic FundamentalsModule 1

Foundation module for RF learning. Covers electromagnetic radiation, the EM spectrum, sine wave properties, bandwidth, and the Doppler effect — with interactive demos throughout. All other modules depend on concepts introduced here.

1.4

What is Electromagnetic Radiation?

Electromagnetic (EM) radiation is energy that propagates through space as coupled oscillating electric and magnetic fields, perpendicular to each other and to the direction of travel. Unlike sound, EM waves require no medium — they travel through a vacuum at the speed of light.

The fields are inseparable: a changing electric field generates a magnetic field, and vice versa. This self-sustaining cycle was first described mathematically by James Clerk Maxwell in 1865 — one of the most important equations in physics.

Key insight: EM waves carry energy (and momentum) without moving any matter. They are how the Sun's energy reaches Earth across 150 million km of vacuum.
Electric field (E)

Oscillates in a plane perpendicular to the direction of travel. Drives free electrons in antennas.

🧲Magnetic field (B)

Perpendicular to E and to direction of travel. Generated by the changing E field.

1.5

Electromagnetic Spectrum

The electromagnetic spectrum is the complete range of all EM radiation, ordered by frequency (or equivalently, wavelength). All EM waves travel at c = 299,792,458 m/s in a vacuum, but they differ enormously in frequency — from a few kilohertz (long-wave radio) to 10²⁵ Hz (gamma rays).

The relationship between frequency, wavelength, and speed of light is: λ = c / f. Higher frequency means shorter wavelength and more energy per photon.

Click a band to explore — increasing frequency →

3 kHzFrequency →300 EHz
Click any band above to see details, frequency range, wavelength, and real-world examples.
🌊All the same physics

Every EM wave travels at c = 299,792,458 m/s in a vacuum. Only frequency and wavelength differ.

λ = c / f

Higher frequency → shorter wavelength. Radio waves are metres long; gamma rays are sub-atomic.

👁️Visible is tiny

The entire visible spectrum spans only 400–700 nm — a sliver of the full EM spectrum.

1.6

Creating an EM Wave

An EM wave is created whenever an electric charge accelerates. In a radio transmitter, alternating current drives electrons back and forth in an antenna, creating oscillating electric and magnetic fields that propagate outward at the speed of light.

The frequency of the transmitted wave equals the frequency of the alternating current driving the antenna. This is why an FM radio transmitter at 100 MHz drives its antenna at exactly 100,000,000 oscillations per second.

Wave structure: The E-field and B-field are always perpendicular to each other and to the direction of propagation. This transverse nature is what allows EM waves to be polarised.
1

AC drives current in the antenna — electrons accelerate

2

Oscillating charge creates oscillating E and B fields

3

Fields propagate outward at c, carrying energy

1.7

Sine Waves & EM Waves

The electric (and magnetic) field of a simple, single-frequency EM wave varies sinusoidally in both space and time — it follows the shape of a sine wave. This is the simplest and most fundamental waveform; any real signal can be decomposed into sine waves (Fourier analysis).

The mathematical form is: E(x,t) = A·sin(2πft − kx + φ), where A is amplitude, f frequency, k the wavenumber (= 2π/λ), and φ phase.

1.8

Sine Wave Characteristics

Understanding these six parameters is essential for all RF engineering:

Cycle
One complete oscillation — from zero, through positive peak, back through zero, through negative peak, and back to zero.
Period (T)
Time in seconds for one complete cycle. T = 1/f.
Frequency (f)
Cycles per second, measured in Hertz (Hz). f = 1/T.
Amplitude (A)
Peak value of the wave — how strong or intense the field is at its maximum.
Phase (φ)
Horizontal shift of the wave, measured in degrees or radians. Two waves at the same frequency can be out of phase.
Wavelength (λ)
Distance in metres between two identical points on consecutive cycles. λ = c/f.

Use the interactive visualiser to see how each parameter shapes the wave:

2.0 Hz
0.70
0°

Derived values

Period (T)0.500 s
Wavelength (λ)150 m
🔁Cycle

One complete oscillation — from zero, up, back through zero, down, and back.

⏱️Period

Time T for one full cycle (seconds). T = 1 / f.

↕️Amplitude

Peak displacement from zero. Represents signal strength or field intensity.

↔️Phase

Horizontal shift of the wave (degrees or radians). Matters in interference.

1.9

Sine Wave Calculations

Three fundamental relationships let you derive any parameter from the others, given the speed of light c:

f = 1 / T// frequency = 1 / period

λ = c / f// wavelength = speed of light / frequency

ω = 2πf// angular frequency (rad/s)

Quick reference — speed of light

c = 299,792,458 m/s ≈ 3 × 10⁸ m/s

1.10

Bandwidth & Channel Bandwidth

Bandwidth is the range of frequencies a signal or system occupies, measured in Hz. A pure sine wave (a single tone) has zero bandwidth — it occupies exactly one frequency. Real signals, which carry information, always occupy a band.

Channel bandwidth is the frequency range allocated to one communication channel by a regulator or standard. For example, an FM radio station is assigned a 200 kHz channel; a 5G NR carrier might use 100 MHz.

Shannon's theorem: Channel capacity C = B · log₂(1 + SNR). More bandwidth means more capacity to carry data — doubling bandwidth (B) doubles the maximum bit rate (all else equal).
📶Occupied bandwidth

The actual frequency range a transmitted signal uses. A 1080p video stream uses far more bandwidth than a voice call.

📡Channel bandwidth

The regulatory or standard-defined "lane" assigned to a communication link. Unused bandwidth within the channel is wasted spectrum.

1.11

Doppler Effect & Doppler Shift

The Doppler effect is the change in observed frequency of a wave when the source and observer move relative to each other. When a source approaches, wavefronts bunch up — the observer receives them more frequently (higher observed frequency). When it recedes, wavefronts spread out — lower frequency.

For electromagnetic waves the Doppler-shifted frequency is: f_obs = f_src · c / (c − v_s) where v_s is the source speed toward the observer (positive = approaching).

Emitted

1.00 kHz

Observed

1.00 kHz

0 m/s (stationary)
🔵Blueshift (approaching)

Source approaching → wavefronts compress → higher observed frequency.

🔴Redshift (receding)

Source receding → wavefronts stretch → lower observed frequency.

📡Real uses

Police radar, weather Doppler radar, astronomy redshift, and air traffic control.

Up next

Module 2 — Modulation

Learn how information is encoded onto a carrier wave using AM, FM, and digital modulation schemes.

Start Module 2