Learn Index · Waves, Electricity and Magnetism Grade 9–10

Wave properties and the electromagnetic spectrum

Electromagnetic waves travel at the speed of light and range from radio waves to gamma rays; higher frequency means shorter wavelength and more energy.

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Wave properties review

Property Symbol Unit Meaning
Wavelength λ m Distance between consecutive crests or compressions
Frequency f Hz Waves per second
Period T s Time for one wave; T = 1/f
Amplitude A m Maximum displacement; related to energy
Wave speed v m/s v = fλ

The speed of a wave depends on the medium, not on frequency or amplitude. When a wave enters a new medium, its speed and wavelength change, but its frequency stays the same.

Wave interactions

Reflection

Waves bounce off boundaries. A wave reflecting from a fixed end (like a rope tied to a wall) is inverted. From a free end, it isn’t.

Refraction

Waves change direction when they enter a medium at an angle and change speed. Ocean waves refract as they approach a beach, bending to arrive nearly parallel to the shore.

Diffraction

Diffraction is the spreading of waves around obstacles or through gaps. It is greatest when the gap is about the same size as the wavelength.

  • You can hear around corners because sound wavelengths (cm to m) are similar to doorways.
  • You can’t see around corners because visible light wavelengths are tiny (400–700 nm).
  • AM radio waves (hundreds of metres long) diffract around hills better than FM waves (about 3 m).

Interference and superposition

When waves overlap, their displacements add. This is the principle of superposition.

Type What happens Result
Constructive Crest meets crest Larger amplitude
Destructive Crest meets trough Smaller amplitude or cancellation

In 1801, Thomas Young shone light through two narrow slits and saw a pattern of bright and dark bands. This double-slit experiment proved light behaves as a wave.

Noise-cancelling headphones use destructive interference: they produce a sound wave that is the exact opposite of outside noise.

Standing waves

When two identical waves travel in opposite directions, they form a standing wave with:

  • nodes: points that never move
  • antinodes: points of maximum vibration

Guitar strings, organ pipes and microwaves all involve standing waves. For a string fixed at both ends, the fundamental wavelength is twice the string length.

Resonance

Every object has natural frequencies. If it’s pushed at one of them, its vibrations grow dramatically: resonance. Examples: a singer shattering a wine glass, pushing a swing at the right moment, and the 1940 Tacoma Narrows Bridge collapse (often attributed to resonance, though aerodynamic flutter was the main cause).

Polarization

Polarization restricts a transverse wave’s vibrations to one plane. Only transverse waves can be polarized. Polarized sunglasses block horizontally polarized glare reflected from water and roads.

The electromagnetic spectrum

Electromagnetic waves are transverse waves of oscillating electric and magnetic fields. All travel at the speed of light in a vacuum: c = 3.00 × 10⁸ m/s.

The electromagnetic spectrum, from longest to shortest wavelength (lowest to highest frequency and energy):

Type Wavelength range Uses Hazards
Radio waves > 1 m AM/FM radio, TV, MRI Generally safe
Microwaves 1 mm – 1 m Cooking, cell phones, Wi-Fi, radar Heating at high power
Infrared 700 nm – 1 mm Remote controls, thermal cameras, heat lamps Burns at high intensity
Visible light 400–700 nm Sight, photography, fibre optics Bright light can damage eyes
Ultraviolet 10–400 nm Sterilization, vitamin D, black lights Sunburn, skin cancer
X-rays 0.01–10 nm Medical imaging, airport security Ionizing; can damage DNA
Gamma rays < 0.01 nm Cancer treatment, sterilizing food Highly ionizing; very dangerous

Mnemonic: "Raging Martians Invaded Venus Using X-ray Guns."

Energy and frequency

Electromagnetic energy comes in packets called photons. Photon energy depends on frequency:

E = hf (h = 6.63 × 10⁻³⁴ J·s, Planck’s constant)

Higher frequency means more energetic photons. That’s why UV, X-rays and gamma rays can break chemical bonds and damage cells, but radio waves can’t.

Example: Find the wavelength of an FM radio station at 100 MHz.
λ = c ÷ f = 3.00 × 10⁸ ÷ 1.00 × 10⁸ = 3.00 m

Common mistakes

  • Thinking frequency changes when a wave enters a new medium. Speed and wavelength change; frequency doesn’t.
  • Thinking microwaves or radio waves are "radiation" in the dangerous, ionizing sense. Only high-frequency radiation is ionizing.
  • Thinking longitudinal waves can be polarized.

Try it yourself

  1. A wave has a frequency of 250 Hz and wavelength 1.4 m. Find its speed.
  2. Calculate the frequency of red light with λ = 700 nm.
  3. Explain why you can hear a radio in another room but not see it.
  4. Rank in order of increasing photon energy: X-rays, radio, visible, ultraviolet.

(Answers: 350 m/s; 4.3 × 10¹⁴ Hz; sound diffracts around doorways, light doesn’t; radio < visible < ultraviolet < X-rays)

Quick recap

  • v = fλ; speed depends on the medium.
  • Waves reflect, refract, diffract and interfere.
  • Superposition creates constructive and destructive interference and standing waves.
  • The EM spectrum ranges from radio waves to gamma rays, all at speed c in a vacuum.
  • Photon energy E = hf increases with frequency.