Open Workbench w/ All Tools
By SpectralBench Editorial Team6 min read

Absorbance, Transmittance & Reflectance Explained

Every spectroscopy measurement ultimately records how light interacts with a sample. The three fundamental quantities — transmittance, absorbance, and reflectance — describe this interaction from different perspectives. Understanding what each one means, how they relate to each other, and when to use each representation is essential for interpreting spectra correctly and making quantitative measurements.

Transmittance

Transmittance (T) is the fraction of incident light that passes through a sample without being absorbed or scattered. It is defined as:

T = I / I₀

where I₀ is the incident intensity and I is the transmitted intensity

Transmittance ranges from 0 (complete absorption) to 1 (no absorption). In practice, spectra are usually displayed as percent transmittance (%T), which is simply T × 100. A sample with 50%T absorbs half the light; a sample with 10%T absorbs 90%.

FTIR instruments traditionally display spectra in %T because this is the natural output of the measurement — the detector measures how much light reaches it. Peaks in a transmittance spectrum point downward (toward lower %T) at absorption frequencies.

Absorbance

Absorbance (A) is the base-10 logarithm of the reciprocal of transmittance:

A = −log₁₀(T) = log₁₀(1/T)

A = 2 − log₁₀(%T)

Absorbance is dimensionless and ranges from 0 (no absorption) upward with no theoretical maximum, though in practice values above 2.0 are unreliable.

The key advantage of absorbance is its linear relationship with concentration via the Beer-Lambert law (A = εlc). Doubling the concentration doubles the absorbance. This linearity makes absorbance the preferred representation for quantitative work, calibration curves, and any analysis where you need to relate spectral intensity to amount.

%TAbsorbanceLight Absorbed
100%0.000None
50%0.30150%
10%1.00090%
1%2.00099%
0.1%3.00099.9% — unreliable measurement range

Absorbance ↔ Transmittance Converter

A = −log₁₀(T/100)  |  %T = 10⁻ᴬ × 100

Transmittance (fraction): T = 0.5000

Light absorbed: 50.00%

Convert units in bulk — the Spectroscopy Unit Converter handles absorbance, transmittance, wavenumber, wavelength, and energy conversions. The Spectral Viewer can switch display mode between absorbance and transmittance for uploaded spectra.

Reflectance

Reflectance (R) is the fraction of incident light that is reflected from a sample surface. Like transmittance, it ranges from 0 to 1 (or 0% to 100%). Reflectance spectroscopy is used when the sample is opaque, highly absorbing, or when non-destructive surface analysis is needed.

There are two main types of reflectance:

  • Specular reflectance — mirror-like reflection from a smooth surface at the angle of incidence. The reflected spectrum is related to the refractive index and absorption coefficient of the material. Used for thin films and polished surfaces.
  • Diffuse reflectance — scattered reflection from a rough or powdered surface. Light penetrates the sample, undergoes multiple scattering and absorption events, and exits at various angles. The most common reflectance technique for powders and rough solids. DRIFTS (Diffuse Reflectance Infrared Fourier Transform Spectroscopy) is the standard FTIR implementation.

Kubelka-Munk Transform

Raw diffuse reflectance spectra cannot be directly used for quantitative analysis because reflectance is not linearly related to concentration. The Kubelka-Munk (K-M) function transforms reflectance into a quantity that is proportional to concentration:

f(R∞) = (1 − R∞)² / (2R∞) = K/S

where R∞ is the absolute reflectance, K is the absorption coefficient, and S is the scattering coefficient

The K-M function is the reflectance analog of the Beer-Lambert law. It is valid when the sample is optically thick (infinitely thick relative to penetration depth), the particle size is uniform, and scattering is isotropic. In practice, diluting the sample in a non-absorbing matrix like KBr improves linearity.

ATR and Pseudo-Absorbance

Attenuated Total Reflectance (ATR) is the most common sampling technique in modern FTIR. It is technically a reflectance method — the infrared beam reflects off the internal surface of a high-refractive-index crystal while an evanescent wave penetrates into the sample. However, ATR spectra are displayed in absorbance-like units and are routinely treated as absorption spectra.

ATR spectra differ from true transmission spectra in two ways: relative peak intensities change because the evanescent wave penetration depth increases at lower wavenumbers, and peak positions can shift slightly due to anomalous dispersion. ATR correction algorithms compensate for the wavelength-dependent penetration depth.

When to Use Each Representation

Use CaseRepresentationWhy
Quantitative analysisAbsorbanceLinear with concentration (Beer-Lambert law)
Qualitative FTIR identification%TransmittanceTraditional display; most reference libraries use %T
Spectral subtractionAbsorbanceAbsorbances are additive; transmittances are multiplicative
Powders / rough solids (DRIFTS)Kubelka-MunkLinearizes the reflectance–concentration relationship
NIR chemometricsAbsorbance or log(1/R)Linearity required for PLS/PCA models
ATR-FTIR routine analysisAbsorbance (ATR)Instrument default; compatible with most search algorithms

Related Resources

Frequently Asked Questions

How do you convert transmittance to absorbance?

Absorbance = −log₁₀(T), where T is the transmittance as a fraction (0 to 1). If you have percent transmittance: A = −log₁₀(%T/100) = 2 − log₁₀(%T). For example, 50%T = 0.301 absorbance, 10%T = 1.000 absorbance, and 1%T = 2.000 absorbance.

What is the difference between absorbance and transmittance?

Transmittance (T) is the fraction of light that passes through a sample (T = I/I₀). Absorbance (A) is the negative logarithm of transmittance (A = −log₁₀T). The key difference for analytical work: absorbance is linearly proportional to concentration (Beer-Lambert law), while transmittance has an exponential relationship. This is why absorbance is preferred for quantitative measurements.

What is the Kubelka-Munk function?

The Kubelka-Munk function f(R) = (1−R)²/(2R) transforms diffuse reflectance data into a quantity proportional to the ratio of absorption coefficient (K) to scattering coefficient (S). It is the reflectance analog of the Beer-Lambert law, linearizing the relationship between reflectance and concentration for powdered or rough-surface samples measured by DRIFTS.

Try It Yourself

Apply what you've learned — open your spectra and use all the analysis tools in one place.

Open Workbench
w/ All Tools

No download · No account required · Works on any device