Wave Velocity Calculator

Calculate phase velocity and group velocity of waves. Explore dispersion in ocean waves, plasma, optical fiber, and custom media with frequency sweeps.

Presets

Hz
Hz
Phase Velocity (vₚ)
343.00 m/s
vₚ = ω/k
Group Velocity (vg)
343.00 m/s
Signal/energy propagation speed
vg / vₚ Ratio
1.0000
Non-dispersive
Phase Wavelength
343.00 mm
λ = vₚ/f = 0.3430 m
Wave Number (k)
18.3183 rad/m
k = 2π/λ
Angular Frequency (ω)
6,283.19 rad/s
ω = 2πf

Phase vs Group Velocity

Phase (vₚ)
Group (vg)

Media Properties Comparison

MediumPhase VelocityGroup VelocityDispersive
Vacuum (EM)299.8M m/s299.8M m/s✗ No
Air (sound, 20°C)343 m/s343 m/s✗ No
Water (sound)1,497 m/s1,490 m/s✓ Yes
Glass (optical)199.9M m/s196.0M m/s✓ Yes
Optical fiber204.1M m/s200.0M m/s✓ Yes
Planning notes, formulas, and examples

About the Wave Velocity Calculator

The wave velocity calculator computes both phase velocity and group velocity for waves in different media, revealing the critical phenomenon of dispersion. While the phase velocity describes how fast individual wave crests move, the group velocity tells you how fast energy and information actually travel — a distinction that becomes crucial in dispersive media.

In non-dispersive media like sound in air, both velocities are equal. But in dispersive media — optical fibers, ocean surfaces, plasma — the two speeds diverge. Deep-ocean swells have a group velocity exactly half their phase velocity, which is why surfers see waves approaching faster than the wave groups that carry them. In plasma, the phase velocity can exceed the speed of light (without violating relativity, since no information travels faster than vg < c).

This calculator models real dispersion relations for deep-water gravity waves, ionospheric plasma, and optical media. Enter a frequency, choose your medium, and see how phase and group velocities differ across a range of frequencies.

When This Page Helps

Understanding the difference between phase and group velocity is essential whenever waves travel through a real medium. Optical engineers must manage dispersion to maintain signal integrity over thousands of kilometers of fiber. Naval engineers predict wave energy arrival times for coastal structures. Atmospheric scientists track radio wave propagation through the ionosphere.

This calculator goes beyond simple v = fλ to reveal the rich physics of dispersion, showing how phase and group velocities diverge in real-world media and how that divergence varies with frequency.

How to Use the Inputs

  1. Select the propagation medium from the dropdown — options include vacuum, air, water, glass, fiber, ocean surface, and plasma
  2. Choose the input mode: standard frequency (Hz) or angular frequency (rad/s)
  3. Enter the wave frequency for your scenario
  4. For custom media, enter both phase and group velocities manually
  5. Read phase velocity, group velocity, and their ratio from the output cards
  6. Compare the visual bars to see the relative magnitude of phase vs group velocity
  7. For dispersive media (ocean, plasma), check the dispersion table to see how speeds vary with frequency
Formula used
Phase velocity: vₚ = ω/k = fλ Group velocity: vg = dω/dk Specific dispersion relations: • Deep-water gravity waves: ω² = gk → vₚ = √(g/k), vg = vₚ/2 • Plasma waves: ω² = ωₚ² + c²k² → vₚ = c/√(1-(fₚ/f)²), vg = c·√(1-(fₚ/f)²) • Non-dispersive: vₚ = vg = constant Where: • ω = angular frequency (rad/s), k = wave number (rad/m) • g = 9.81 m/s² (gravitational acceleration) • ωₚ = plasma frequency, c = speed of light

Example Calculation

Result: Phase velocity ≈ 15.6 m/s, Group velocity ≈ 7.8 m/s

A 10-second ocean swell (f = 0.1 Hz) has phase velocity vₚ = √(g/k) ≈ 15.6 m/s and group velocity vg = vₚ/2 ≈ 7.8 m/s. Wave crests move twice as fast as the wave packet (energy), which is why individual crests appear to emerge from the back of a swell group and vanish at the front.

Tips & Best Practices

  • For non-dispersive media (air, vacuum), phase and group velocity are identical — use the simpler wave speed calculator instead
  • The vg/vₚ ratio immediately tells you the dispersion type: <1 is normal, >1 is anomalous, =1 is non-dispersive
  • Ocean swell prediction: group velocity determines when wave energy from a distant storm arrives at shore
  • In plasma, signals near the plasma frequency are heavily distorted — keep carrier frequency well above fₚ
  • For fiber optics at 1550 nm, group velocity delay is about 5 µs/km — multiply by fiber length for signal timing
  • Remember: only group velocity is limited by c for information transfer; phase velocity exceeding c is physically allowed

Phase Velocity vs Group Velocity

The distinction between phase and group velocity is one of the most profound concepts in wave physics. Phase velocity vₚ = ω/k describes the speed of individual wave crests — the rate at which a surface of constant phase moves through space. Group velocity vg = dω/dk describes the speed of the wave envelope — the rate at which energy, information, and wave packets propagate.

In a non-dispersive medium where ω = vk (linear dispersion), phase and group velocities are identical. This is the familiar case for sound in air or light in vacuum. But most real media are dispersive: glass slows blue light more than red (normal dispersion), while the ionosphere slows low-frequency radio waves more than high-frequency ones (also normal dispersion by a different mechanism).

Deep-Water Wave Dispersion

Ocean surface waves provide one of the most intuitive examples of dispersion. For deep-water gravity waves (depth > half the wavelength), the dispersion relation is ω² = gk, giving vₚ = √(g/k) = gT/(2π). Longer-period swells travel faster.

The group velocity for these waves is exactly vₚ/2 — a beautiful result that means wave energy propagates at half the speed of visible wave crests. Watch ocean swells carefully and you'll see individual crests form at the back of a group, propagate forward through the group, and disappear at the front. This has practical importance: when a storm generates ocean swell, the energy arrives at a distant coast at the group speed, not the (faster) phase speed.

Dispersion in Technology

Modern telecommunications depend on managing dispersion. In an optical fiber carrying 100 Gbps of data, each data pulse occupies roughly 10 picoseconds. Standard single-mode fiber has chromatic dispersion of about 17 ps/(nm·km) at 1550 nm. Over 1000 km, a pulse with 0.1 nm spectral width spreads by 1.7 ns — far wider than the original 10 ps — destroying the data stream unless compensated.

Engineers use dispersion-compensating fiber, dispersion-shifted fiber, and digital signal processing to combat this effect. The entire field of ultrafast optics—generating and manipulating femtosecond laser pulses—requires precise control of dispersion through prisms, gratings, and chirped mirrors.

Sources & Methodology

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Frequently Asked Questions

  • Yes. In plasma and other anomalous-dispersion media, phase velocity can exceed c. This doesn't violate relativity because phase velocity doesn't carry information or energy — the group velocity (always ≤ c in these cases) is what matters for causality. The superluminal vₚ simply means wavefronts don't represent signal propagation.