EM wave 3D

Watch an electromagnetic wave travel: the electric field waves up and down, the magnetic field side to side, both at right angles to the direction of travel and in step. Change the wavelength from gamma rays to radio and the field strength, turn the view, and get the frequency, B₀ = E₀/c, the intensity and c = 1/√(µ₀ε₀).

Keep it one tap away for everyday use.

Bookmark EM wave 3D?

Press Ctrl + D now. Your browser opens its own bookmark box, where you choose the name and folder.

  1. See E and B
  2. Wavelength
  3. f, B₀, I
  4. Check
Nothing is uploadedWorks offline once open

Electromagnetic wave

electric field Emagnetic field Bdirection of travel

Try this

  • Watch E and B: they peak together and pass through zero together. They are in phase.
  • Turn the view: E stays up and down, B stays side to side, and both are at right angles to the travel.
  • Slide the wavelength from radio to gamma rays: the picture looks the same, because all of them are the same kind of wave. Only λ and f change.
  • Make E₀ ten times bigger: B₀ goes up ten times, and the intensity a hundred times.
  • B₀ is tiny compared with E₀ because B₀ = E₀/c, and c is huge.

Check yourself

What it does

Maxwell showed that a changing electric field makes a magnetic field and a changing magnetic field makes an electric field, so the two can keep each other going and travel through empty space as a wave. Light, radio and X-rays are all such electromagnetic (EM) waves.

In an EM wave in empty space:

  • the electric field E and the magnetic field B are at right angles to each other,
  • both are at right angles to the direction the wave travels (it is a transverse wave),
  • they rise and fall together (in phase), with B₀ = E₀/c,
  • and the wave travels at c = 1/√(µ₀ε₀), about 3 × 10⁸ m/s, whatever its wavelength.

This page draws two wavelengths of the wave in 3D and keeps it moving. The electric field is drawn up and down, the magnetic field side to side. Turn the view to see that they stay at right angles. Slide the wavelength from 1 nm to 1 km, and the page names the band and gives the frequency and period; set the peak electric field and it gives the peak magnetic field, the intensity and the energy density.

It follows the electromagnetic waves chapter of Class 12 Physics (displacement current, sources and nature of EM waves, the EM spectrum). See where the wave’s magnetic field comes from in displacement current, place your wavelength among all the others in the electromagnetic spectrum explorer, and compare with waves on a string in travelling wave.

How to use it

  1. Slide the wavelength (a log scale from 1 nm to 1 km). The picture always shows two wavelengths, so it looks the same for every band.
  2. Slide the peak electric field E₀ (1 to 1000 V/m).
  3. Turn the view to look from the side, from above at an angle, or along the wave.
  4. Pause and Play the wave. If your device asks for reduced motion, it starts paused.

Worked example

The page opens with λ = 3.02 m (an FM radio wave) and E₀ = 10 V/m.

  • f = c / λ = 3 × 10⁸ / 3.02 = 99.3 MHz, and one cycle takes T = 1/f = 10.1 ns.
  • B₀ = E₀ / c = 10 / 3 × 10⁸ = 3.34 × 10⁻⁸ T, far smaller than the Earth’s field (about 5 × 10⁻⁵ T).
  • I = ½ c ε₀ E₀² = ½ × 3 × 10⁸ × 8.85 × 10⁻¹² × 10² = 0.133 W/m².
  • c = 1/√(µ₀ε₀) = 1/√(1.257 × 10⁻⁶ × 8.854 × 10⁻¹²) = 3 × 10⁸ m/s.

Tips

  • Doubling E₀ doubles B₀ but makes the intensity four times bigger, because I ∝ E₀².
  • The direction of travel is along E × B: turn E towards B with your right hand and your thumb points the way the wave goes.
  • In a material, EM waves travel slower than c, by the refractive index. This page is for empty space.

FAQ

Why is the magnetic field drawn the same size as the electric field? They have different units, so they cannot be drawn to one scale. Both are drawn to show their shape and timing; the numbers give their real sizes.

Does the wave need a medium? No. EM waves travel through empty space, which is how sunlight reaches us.

Is anything saved? No. Everything is worked out on this page and nothing leaves your device.

Where the numbers come from

  • Plane electromagnetic wave in vacuum: E ⊥ B ⊥ direction of travel, B₀ = E₀/c, c = 1/√(µ₀ε₀), f = c/λ, intensity I = ½cε₀E₀², average energy density ½ε₀E₀². Standard physics results. ε₀ = 8.8541878188 × 10⁻¹² F/m and µ₀ = 1.25663706127 × 10⁻⁶ N/A² (CODATA 2022, NIST); c = 299 792 458 m/s exactly.
  • Checked against an independent Python script, including c computed from ε₀ and µ₀.

Standard scientific values, such as constants, atomic weights and melting points, are facts found in every textbook; we name where ours were checked. If you are an author or publisher and want a value, a credit or a table changed or removed, tell us and we will act quickly.

Last updated 2026-11-09.

Change log for EM wave 3D

  1. Add #1418 Electromagnetic wave in 3D Details on GitHub

Every change to fibub

Related tools

Travelling wave #L27 Watch a wave move along a string while one particle just goes up and down. Change the amplitude, wavelength, period and direction; add a second wave to see superposition and standing waves; and hear beats between two close tones. Photoelectric effect lab #L31 Shine light on caesium, sodium, zinc and other metals. Change the frequency, brightness and collector voltage, watch the current, and record the stopping potential at several frequencies to measure Planck's constant and the work function from a straight line. Electromagnetic spectrum explorer #L273 Drag along the electromagnetic spectrum from gamma rays to radio waves and see the band, what it is used for, the frequency f = c/λ and the energy of one photon in joules and electronvolts. Jump to everyday examples such as a TV remote, Wi-Fi, a microwave oven or FM radio. Displacement current #L274 Charge a round parallel-plate capacitor through a resistor and watch the current fall while the field between the plates grows. See why Maxwell added the displacement current I_d = ε₀ dΦ_E/dt, and why the magnetic field on a loop comes out the same whichever surface you pick. Mirror ray diagram #L1 Drag an object in front of a concave or convex mirror and watch the principal rays find the image: where it forms, how big it is, real or virtual, with the mirror formula and magnification worked out with signs. Lens ray diagram #L2 Drag an object in front of a convex or concave lens and watch the principal rays find the image: where it forms, how big it is, real or virtual, with the lens formula, magnification and power worked out with signs.