Wave Frequency Calculator: v = f·λ (velocity, frequency, wavelength)
Wave calculator v=f·λ: find velocity, frequency, or wavelength. Light (c=299,792,458), sound (343 m/s), seismic presets. Period, angular frequency, E=hf. Audio, FM MHz, 5G GHz, X-ray examples.
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Disclaimer: this calculation is for informational purposes only. For important decisions, consult a qualified professional.
Waves: the fundamental relation v = f·λ
All waves — light, sound, radio, water, seismic — obey the same simple relation: v = f·λ, where v is propagation speed (m/s), f is frequency (Hz, cycles per second), and λ is wavelength (m, distance between two crests). This calculator solves v, f, or λ given the other two, plus period T, angular frequency ω, wavenumber k, photon energy (light), and real-world context (AM radio, FM, 5G, visible, X-ray, etc.).
Fundamental formulas
- v = f · λ — speed = frequency × wavelength
- f = v / λ
- λ = v / f
- T = 1 / f — period (s)
- ω = 2π·f — angular frequency (rad/s)
- k = 2π/λ — wavenumber (rad/m)
- E = h·f — photon energy (light), h = 6.626×10⁻³⁴ J·s
Typical propagation speeds
| Wave type | Speed (m/s) | Context |
|---|---|---|
| Light in vacuum (c) | 299,792,458 | Universal constant |
| Light in water | 225,000,000 | n=1.33 |
| Light in glass | ~200,000,000 | n=1.5 typical |
| Light in diamond | 124,000,000 | n=2.42 very high |
| Sound in air (20°C) | 343 | Increases with T |
| Sound in helium | 972 | "Cartoon" voice |
| Sound in water | 1,480 | Sonar |
| Sound in steel | 5,100 | Trains audible far |
| P seismic waves | 5,000-8,000 | First after earthquake |
| S seismic waves | 3,000-5,000 | Slower, more destructive |
| Deep water waves | 15-25 | Depth-dependent |
| Radio in vacuum | 299,792,458 | Like light (EM) |
Practical numerical examples
Example 1: A4 musical note
A4 = 440 Hz in air at 20°C (v=343):
- λ = v/f = 343/440 = 0.780 m = 78 cm
- Period T = 2.27 ms
- Order of size of a guitar or transverse flute
Example 2: FM radio
FM station at 100 MHz in vacuum:
- λ = c/f = 3×10⁸ / 10⁸ = 3 m
- FM antennas typically 75 cm (λ/4) or 1.5 m (λ/2)
- Period T = 10 ns
Example 3: 2.4 GHz WiFi
- λ = 3×10⁸ / 2.4×10⁹ = 0.125 m = 12.5 cm
- WiFi antennas ~3-6 cm (λ/4 or λ/2)
- Passes thin walls well, blocked by metal or thick walls
Example 4: 5G mmWave
5G at 28 GHz:
- λ = 3×10⁸ / 2.8×10¹⁰ = 1.07 cm
- Hence "mmWave" name
- High bandwidth but short range (100-300 m), blocked by walls
Example 5: green visible light
Green at λ = 550 nm in vacuum:
- f = c/λ = 3×10⁸ / 5.5×10⁻⁷ = 5.45×10¹⁴ Hz = 545 THz
- Photon energy E = h·f = 3.6×10⁻¹⁹ J ≈ 2.25 eV
- Typical visible photon energy
Example 6: ocean wave
8 s period wave in deep water (v ≈ 12.5 m/s):
- f = 1/T = 0.125 Hz
- λ = v·T = 12.5 × 8 = 100 m
- Ocean waves have very long λ
The complete EM spectrum
| Band | Frequency | Wavelength | Use |
|---|---|---|---|
| ELF radio | < 3 kHz | > 100 km | Underwater comm |
| VLF/LF | 3-300 kHz | 1-100 km | Navigation |
| AM radio | 540-1700 kHz | 180-560 m | AM radio |
| Shortwave | 3-30 MHz | 10-100 m | HF international |
| FM/VHF TV | 30-300 MHz | 1-10 m | FM 88-108, TV |
| UHF | 300 MHz-3 GHz | 10 cm-1 m | TV UHF, mobile, GPS |
| Microwave | 3-300 GHz | 1 mm-10 cm | WiFi, 5G, oven, radar |
| Infrared | 300 GHz-430 THz | 700 nm-1 mm | Remotes, heat |
| Visible | 430-750 THz | 400-700 nm | Human eye |
| Ultraviolet | 750 THz-30 PHz | 10-400 nm | Sterilization, UV |
| X-rays | 30 PHz-30 EHz | 0.01-10 nm | Radiography |
| Gamma rays | > 30 EHz | < 0.01 nm | Nuclear medicine |
All EM radiation travels at the same speed in vacuum: c = 299,792,458 m/s (exact value, meter definition since 1983).
Acoustic spectrum: human ear
| Frequency (Hz) | Description | Example |
|---|---|---|
| < 20 | Infrasound | Earthquakes |
| 20-60 | Deep bass | Subwoofer, cannons |
| 60-250 | Bass | Bass guitar, male voice |
| 250-2000 | Mids | Speech, guitar |
| 2000-6000 | Upper mids | Singing voice, violin |
| 6000-20000 | Highs | Cymbals, whistles |
| > 20000 | Ultrasound | Dogs hear to 45 kHz |
Human hearing declines with age: children to 20 kHz, adults ~15 kHz, elderly 8-10 kHz. Animals: dolphins 150 kHz, bats 200 kHz.
Musical notes and frequencies
| Note | Frequency (Hz) | λ in air (cm) |
|---|---|---|
| C4 (middle C) | 261.63 | 131 |
| D4 | 293.66 | 117 |
| E4 | 329.63 | 104 |
| F4 | 349.23 | 98 |
| G4 | 392.00 | 87 |
| A4 (tuning) | 440.00 | 78 |
| B4 | 493.88 | 69 |
| C5 | 523.25 | 65 |
One octave = doubling of frequency. Guitar string length halves per octave.
Physical derivation
A wave is a periodic disturbance propagating in space. In one period T the wave advances one wavelength λ. Speed = distance/time:
v = λ / T = λ · (1/T) = λ · f
Universal, applies to mechanical (sound, strings, water) and electromagnetic (light, radio, X) waves.
The wave equation
Traveling wave mathematical form:
y(x,t) = A·sin(k·x − ω·t + φ)
A amplitude, k = 2π/λ wavenumber, ω = 2π·f angular frequency, φ initial phase. Phase velocity v = ω/k = f·λ.
Applications
Music and acoustics
- Musical instrument design (organ pipe length, strings)
- Tuning: A4 440 Hz standard
- Concert halls: room length vs λ for unwanted reflections
- Microphones and speakers: bandwidth
Telecommunications
- Antenna sizing: L ≈ λ/4 or λ/2
- Band choice: low f penetrates obstacles; high f more bandwidth
- Propagation: ionosphere reflects HF, UHF is line-of-sight
- 5G mmWave: small λ → compact antennas but short range
Medicine
- Ultrasound: 2-15 MHz; higher f = better resolution but lower penetration
- X-rays (f ~10¹⁸ Hz): radiography, CT
- MRI: radio frequencies 60-300 MHz in magnetic field
Radar and sonar
- Radar: microwaves 1-40 GHz, aircraft and ships
- Sonar: acoustic 10-100 kHz in water
- Distance: t=2d/v → d=v·t/2
Astronomy
- Radio telescopes: detect stellar emissions at various λ
- Cosmological Doppler: galaxy redshift
- Gravitational waves (LIGO): f ~ 100 Hz, detected 2015
Seismology
- P waves (compression): faster, arrive first
- S waves (shear): slower, don't cross liquids
- P-S time difference → epicenter distance
Sound speed and temperature
Sound speed in air depends on temperature:
v ≈ 331.3 + 0.606·T(°C) m/s
At 0°C: 331 m/s. At 20°C: 343 m/s. At 40°C: 355 m/s. Kinetic theory: v ∝ √T. Why musical instruments go out of tune with temperature.
Doppler effect
When source and observer move relative to each other, perceived frequency changes:
f' = f · (v ± v_obs) / (v ∓ v_source)
Example: ambulance at 40 m/s with 700 Hz siren approaching stationary observer:
f' = 700 · 343/(343-40) = 792 Hz (higher)
After passing: f' = 626 Hz (lower). 166 Hz jump.
Refraction: waves crossing media
When a wave enters a new medium, speed changes but frequency stays constant (set by source). Wavelength changes:
λ₂/λ₁ = v₂/v₁ = n₁/n₂
with n = c/v refractive index. Vacuum (n=1) to water (n=1.33): λ reduced by 1.33×. Green light 550 nm in vacuum → 414 nm in water (still appears green!).
Standing waves and harmonics
On a string fixed at both ends, standing waves form at discrete wavelengths:
- λ_n = 2L/n for n = 1, 2, 3, ...
- f_n = n·v/(2L)
n=1 fundamental, n=2 first harmonic (octave), n=3 second harmonic. Instrument timbre comes from harmonic mixture.
History of wave theory
Huygens (1678, Netherlands): wave theory of light. Huygens' principle.
Thomas Young (1801): double-slit experiment proves wave nature of light.
Maxwell (1865): electromagnetism equations predict EM waves at light speed — light = EM wave!
Heinrich Hertz (1887): generates and detects radio waves, confirming Maxwell.
Planck (1900): E = h·f explains blackbody radiation.
Einstein (1905): photon as energy quantum h·f. Wave-particle duality.
De Broglie (1924): matter has wave properties λ = h/p.
FAQ
What is the fundamental wave formula?
v = f·λ, where v is speed (m/s), f frequency (Hz), λ wavelength (m). Universal for all waves.
Why is light speed constant?
From Maxwell's equations, c = 1/√(ε₀·μ₀), universal constants. Einstein (1905) deduced it's the same for all observers, founding special relativity.
Does frequency change when wave enters new medium?
No. Frequency stays constant (set by source). Speed v changes, so wavelength λ changes. Light vacuum → glass: f same, λ reduced.
What is Doppler effect?
Frequency change when source and observer move. Approaching: higher frequency (sound higher, light blue-shift); receding: lower (red-shift). f' = f·(v ± v_obs)/(v ∓ v_source).
How to calculate antenna length?
Typically L = λ/4 or λ/2. WiFi 2.4 GHz (λ=12.5 cm): L = 3.1 cm. FM 100 MHz (λ=3 m): L = 75 cm. AM 1 MHz (λ=300 m): large towers needed.
Difference longitudinal vs transverse waves?
Longitudinal: oscillation parallel to propagation (sound in air). Transverse: perpendicular (guitar string, light). EM waves are transverse; sound in fluids is longitudinal.
What is a photon?
Energy quantum of EM wave. Energy E = h·f (h = Planck constant). Wave-like (interference) and particle-like (photoelectric effect) — wave-particle duality.
Gravitational waves: new frontier
Predicted by Einstein (1916), first detected by LIGO (2015): oscillations of spacetime curvature from accelerating masses. Observed frequencies 10-1000 Hz, spacetime deformations 10⁻²¹ — equivalent to measuring a hair's width over Earth-Sun distance.
Common errors
- Forgetting frequency units: Hz = cycles/s
- Confusing f and ω: ω = 2π·f, differ by 6.28
- Applying v=fλ to relativistic particles: phase vs group velocity
- Using c in non-vacuum media: light in water travels at c/n
- Confusing vacuum λ with medium λ: light entering water: λ → λ/n
Updated July 2026
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