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Wavelength is the spatial period of a wave — the distance over which the wave's shape repeats. For electromagnetic radiation, wavelength λ and frequency f are related by λ = c/f, where c = 299,792,458 m/s (speed of light in vacuum, exact). This converter spans the entire electromagnetic spectrum, from radio waves (metres) to gamma rays (femtometres), and also converts between wavelength, frequency, photon energy, and wavenumber.
The electromagnetic spectrum by wavelength: radio waves >1 mm; microwaves 1 mm-1 m; millimetre waves 1-10 mm; infrared 780 nm-1 mm; visible light 380-780 nm; ultraviolet 10-380 nm; X-rays 0.01-10 nm (10 pm-10 nm); gamma rays <10 pm. These boundaries are approximate and overlap.
In spectroscopy and photonics, nanometres are the standard unit for visible and UV/NIR light. The visible range (380-780 nm) corresponds to photon energies 1.59-3.26 eV. The infrared range (780 nm-1 mm = 0.78-1000 μm) is important for thermal imaging, fiber optic communications (1310 nm and 1550 nm telecom windows), and infrared spectroscopy.
In X-ray crystallography, wavelengths are in the Angstrom range (0.1-10 Å = 10-1000 pm), comparable to atomic spacings in crystals. CuKα X-rays (λ = 1.5418 Å = 154.18 pm) are the most common source for powder diffraction. Photon energies are 1.24-12.4 keV. The relationship E(keV) × λ(Å) = 12.4 is a useful quick conversion.
At nuclear scales, gamma rays have wavelengths in the femtometre (fm) range, comparable to nuclear diameters (~1-10 fm). A 1 MeV gamma ray has λ = hc/E = 1.24 × 10⁻¹² m = 1.24 pm. The proton Compton wavelength (h/m_p c = 1.321 fm) and nuclear size (~1 fm) are in the same range.
Select the input unit — wavelength (m, cm, mm, μm, nm, Å, pm, fm) or electromagnetic property (frequency in Hz, or photon energy in eV, keV, MeV). All conversions use λ = c/f and E = hc/λ with exact SI values of c and h. Output includes wavelength in all units, frequency, photon energy in eV, and wavenumber in cm⁻¹.
Quick reference: 550 nm = green light = 2.25 eV = 545 THz = 18,182 cm⁻¹. 1550 nm = fiber optic telecom C-band = 0.80 eV = 193 THz. 0.154 nm = 1.54 Å = CuKα X-ray = 8.05 keV. 1.24 pm = 1 MeV gamma ray = 2.42 × 10²⁰ Hz.
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Sodium D-line at 589.3 nm = 2.105 eV = 509 THz = 16,970 cm⁻¹. The characteristic yellow color of sodium vapor lamps and one of the most famous spectral lines — first analyzed by Fraunhofer in 1814.
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CuKα radiation: 1.5418 Å = 8.047 keV. This wavelength is ideal for X-ray crystallography because it is comparable to chemical bond lengths (1-2 Å), giving diffraction angles in the range 10-80° for common crystal spacings.
The human eye detects electromagnetic radiation from approximately 380 nm (violet) to 780 nm (deep red), with peak sensitivity at about 555 nm (green) for photopic (daytime, cone) vision and 507 nm (blue-green) for scotopic (dark-adapted, rod) vision. The exact limits vary between individuals; some people can detect down to 350 nm UV. Bees see down to 300 nm UV but cannot see red above ~650 nm.
Every particle has an associated quantum wavelength λ = h/p = h/(mv) for non-relativistic particles. For an electron at v = 10⁶ m/s: λ = 6.626 × 10⁻³⁴ / (9.109 × 10⁻³¹ × 10⁶) = 0.727 nm = 7.27 Å — comparable to atomic spacings, explaining electron diffraction in crystals. For a 1 kg ball at 10 m/s: λ = 6.626 × 10⁻³⁵ m — utterly undetectable, explaining why large objects don't exhibit wave behavior.
Bragg's law: nλ = 2d sin(θ), where d is crystal plane spacing, θ is the diffraction angle, λ is the X-ray wavelength, and n is the order. For CuKα (λ = 1.54 Å) diffracted from calcite (d = 3.036 Å): first-order peak at θ = arcsin(λ/2d) = arcsin(1.54/6.07) = 14.7°. X-ray crystallography maps atomic positions by solving the inverse problem: from measured diffraction pattern angles and intensities, determine the 3D arrangement of atoms.
Fiber optic communications use three low-loss windows of silica glass: O-band (1260-1360 nm), E-band (1360-1460 nm), S-band (1460-1530 nm), C-band (1530-1565 nm, lowest attenuation ~0.2 dB/km), and L-band (1565-1625 nm). The C-band is dominant for long-haul transmission. Each DWDM channel is ~0.8 nm wide, with up to 80 channels per fiber. WDM allows ~100 Tbps data rates per fiber.
The CMB is a nearly perfect blackbody spectrum at T = 2.725 K. The peak wavelength by Wien's law: λ_max = b/T = 2.898 × 10⁻³ / 2.725 = 1.063 mm (microwave). The photon energy at the peak is E = hc/λ = 1.166 meV. The CMB fills space isotropically with a photon number density of about 411 photons/cm³ and energy density 4.17 × 10⁻¹⁴ J/m³.
Shorter wavelengths (harder X-rays) penetrate more deeply. The attenuation coefficient μ ∝ λ³ × Z³ (photoelectric absorption, dominant below ~0.1 MeV), where Z is atomic number. Soft X-rays (1-10 nm): absorbed by air in millimeters, used for soft tissue contrast. Hard X-rays (0.01-0.1 nm, 12-120 keV): penetrate centimetres of soft tissue, used in medical imaging and industrial inspection. Mammography uses 17-35 keV (0.04-0.07 nm).
A photonic crystal is a periodic dielectric structure that creates a photonic bandgap — a range of wavelengths that cannot propagate through the structure (analogous to electronic bandgaps in semiconductors). The bandgap center wavelength is roughly twice the lattice period. Structural coloration in butterfly wings, opals, and peacock feathers arises from photonic crystal effects, creating iridescent colors that depend on viewing angle unlike pigment-based colors.
Sound at 440 Hz (concert pitch A) in air at 20°C (speed of sound = 343 m/s): λ = v/f = 343/440 = 0.780 m = 78.0 cm. Note that this is a sound wavelength (pressure wave in air), not electromagnetic. For comparison, radio waves at 440 Hz would have λ = c/f = 3×10⁸/440 = 682 km — far too large for conventional antennas. Extremely low frequency (ELF) radio at 76 Hz (used for submarine communication) has λ = 3947 km.
Laser wavelength is determined by the transition energy of the gain medium. For solid-state lasers: Nd:YAG at 1064 nm (near infrared), frequency-doubled to 532 nm (green); Ti:sapphire tunable 690-1080 nm. Diode lasers: InGaAs 780-1550 nm (telecom, CD, DVD). Gas lasers: HeNe at 632.8 nm (red), ArF at 193 nm (UV, semiconductor lithography), CO₂ at 10.6 μm (IR, cutting). Free electron lasers can tune from microwave to X-ray.
Resolving power R = λ/Δλ = f/Δf. Grating spectrometers: R = mN (m = diffraction order, N = number of grooves illuminated); a 1200 groove/mm grating at first order with 50 mm illuminated width gives R = 1200 × 50 = 60,000, resolving 550/60,000 = 0.009 nm = 9 pm at 550 nm. Fabry-Perot etalons: R up to 10⁶-10⁷. Fourier transform spectrometers (FTIR): R up to 10⁶. Atomic transition natural linewidth: R up to 10¹³.
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