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Stokes Shift Calculator

The Stokes shift between absorption and emission maxima in nm, cm⁻¹ and eV.

Model: Exact

Stokes shift Δλ

40.00 nm

Stokes shift Δν̃

1602.6 cm⁻¹

= 4.804e+4 GHz

Energy difference ΔE

0.1987 eV

= 198.7 meV

Quote the shift in cm⁻¹ or eV: the same Δλ means a larger energy gap in the blue than in the red. The widths only shape the chart; the bands are drawn as Gaussians in wavelength for illustration.

Absorption and emission bands

00.20.40.60.81.0450500550600Wavelength (nm)Normalised intensity
  • Absorption
  • Emission
  • Shift between the maxima

Δλ = λ_em − λ_abs

Δν̃ = 10⁷ (1/λ_abs − 1/λ_em) cm⁻¹ (λ in nm)

ΔE = hc (1/λ_abs − 1/λ_em), hc = 1239.84 eV·nm

The Stokes shift is the gap between the absorption and emission maxima. After excitation the molecule relaxes vibrationally, and its surroundings reorganise, before it emits, so emission comes from a lower energy. Solvent polarity adds to the shift (Lippert–Mataga). Compare maxima taken on the same axis: a band's maximum moves when a spectrum per nm is converted to one per cm⁻¹. The vibronic model on the band-model page shows how the shift follows from the Huang–Rhys factor.

Model and references

Exact. The equations are exact within the stated assumptions, or are a standard's tabulated values. The results are as good as the inputs. About the tiers

Exact conversion between the two maxima (vacuum wavelengths). The band shapes in the chart are Gaussians in wavelength, for illustration only.

  1. Lakowicz J. R. (2006). Principles of Fluorescence Spectroscopy, 3rd ed., ch. 1. Springer.
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Spectral Deconvolution & Band Model

Overlapping Gaussian, Lorentzian or pseudo-Voigt bands: areas, band width and centroid, whether neighbours resolve, and least-squares heights with standard errors from a simulated noisy spectrum; or a vibronic (Huang–Rhys) absorption and emission band with its Stokes shift.