Attenuation coefficient

The linear attenuation coefficient, attenuation coefficient, or narrow-beam attenuation coefficient characterizes how easily a volume of material can be penetrated by a beam of light, sound, particles, or other energy or matter.<ref name=GoldBook>IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version: (2006–) "Attenuation coefficient". doi:10.1351/goldbook.A00516</ref> A coefficient value that is large represents a beam becoming 'attenuated' as it passes through a given medium, while a small value represents that the medium had little effect on loss.<ref>Serway, Raymond; Moses, Clement; Moyer, Curt (2005). Modern Physics. California, USA: Brooks/Cole. p. 529. ISBN 978-0-534-49339-4.</ref> The (derived) SI unit of attenuation coefficient is the reciprocal metre (m⁻¹). Extinction coefficient is another term for this quantity,<ref name=GoldBook/> often used in meteorology and climatology.<ref name="AMSGlossary">"2nd Edition of the Glossary of Meteorology". American Meteorological Society. Retrieved 2015-11-03.</ref> Most commonly, the quantity measures the exponential decay of intensity, that is, the value of downward e-folding distance of the original intensity as the energy of the intensity passes through a unit (e.g. one meter) thickness of material, so that an attenuation coefficient of 1 m⁻¹ means that after passing through 1 metre, the radiation will be reduced by a factor of e, and for material with a coefficient of 2 m⁻¹, it will be reduced twice by e, or e². Other measures may use a different factor than e, such as the decadic attenuation coefficient below. The broad-beam attenuation coefficient counts forward-scattered radiation as transmitted rather than attenuated, and is more applicable to radiation shielding. The mass attenuation coefficient is the attenuation coefficient normalized by the density of the material.

Overview

The attenuation coefficient describes the extent to which the radiant flux of a beam is reduced as it passes through a specific material. It is used in the context of:

X-rays or gamma rays, where it is denoted μ and measured in cm⁻¹;
neutrons and nuclear reactors, where it is called macroscopic cross section (although actually it is not a section dimensionally speaking), denoted Σ and measured in m⁻¹;
ultrasound attenuation, where it is denoted α and measured in dB⋅cm⁻¹⋅MHz⁻¹;<ref name="ReferenceA">ISO 20998-1:2006 "Measurement and characterization of particles by acoustic methods"</ref><ref name="autogenerated2002">Dukhin, A.S. and Goetz, P.J. "Ultrasound for characterizing colloids", Elsevier, 2002</ref>
acoustics for characterizing particle size distribution, where it is denoted α and measured in m⁻¹.

The attenuation coefficient is called the "extinction coefficient" in the context of

solar and infrared radiative transfer in the atmosphere, albeit usually denoted with another symbol (given the standard use of μ = cos θ for slant paths);

A small attenuation coefficient indicates that the material in question is relatively transparent, while a larger value indicates greater degrees of opacity. The attenuation coefficient is dependent upon the type of material and the energy of the radiation. Generally, for electromagnetic radiation, the higher the energy of the incident photons and the less dense the material in question, the lower the corresponding attenuation coefficient will be.

Mathematical definitions

Attenuation coefficient

The attenuation coefficient of a volume, denoted μ, is defined as<ref name="ISO_9288-1989">"Thermal insulation — Heat transfer by radiation — Physical quantities and definitions". ISO 9288:1989. ISO catalogue. 1989. Retrieved 2015-03-15.</ref>

<math>\mu = -\frac{1}{\Phi_\mathrm{e}} \frac{\mathrm{d}\Phi_\mathrm{e}}{\mathrm{d}z},</math>

where

Φ_e is the radiant flux;
z is the path length of the beam.

Spectral hemispherical attenuation coefficient

The spectral hemispherical attenuation coefficient in frequency and spectral hemispherical attenuation coefficient in wavelength of a volume, denoted μ_ν and μ_λ respectively, are defined as:<ref name="ISO_9288-1989"/>

<math>\mu_\nu = -\frac{1}{\Phi_{\mathrm{e},\nu}} \frac{\mathrm{d}\Phi_{\mathrm{e},\nu}}{\mathrm{d}z},</math>

<math>\mu_\lambda = -\frac{1}{\Phi_{\mathrm{e},\lambda}} \frac{\mathrm{d}\Phi_{\mathrm{e},\lambda}}{\mathrm{d}z},</math>

where

Φ_e,ν is the spectral radiant flux in frequency;
Φ_e,λ is the spectral radiant flux in wavelength.

Directional attenuation coefficient

The directional attenuation coefficient of a volume, denoted μ_Ω, is defined as<ref name="ISO_9288-1989"/>

<math>\mu_\Omega = -\frac{1}{L_{\mathrm{e},\Omega}} \frac{\mathrm{d}L_{\mathrm{e},\Omega}}{\mathrm{d}z},</math>

where L_e,Ω is the radiance.

Spectral directional attenuation coefficient

The spectral directional attenuation coefficient in frequency and spectral directional attenuation coefficient in wavelength of a volume, denoted μ_Ω,ν and μ_Ω,λ respectively, are defined as<ref name="ISO_9288-1989"/>

<math>\begin{align}

     \mu_{\Omega,\nu} &= -\frac{1}{L_{\mathrm{e},\Omega,\nu}} \frac{\mathrm{d}L_{\mathrm{e},\Omega,\nu}}{\mathrm{d}z}, \\
 \mu_{\Omega,\lambda} &= -\frac{1}{L_{\mathrm{e},\Omega,\lambda}} \frac{\mathrm{d}L_{\mathrm{e},\Omega,\lambda}}{\mathrm{d}z},

\end{align}</math> where

L_e,Ω,ν is the spectral radiance in frequency;
L_e,Ω,λ is the spectral radiance in wavelength.

Absorption and scattering coefficients

When a narrow (collimated) beam passes through a volume, the beam will lose intensity due to two processes: absorption and scattering. Absorption indicates energy that is lost from the beam, while scattering indicates light that is redirected in a (random) direction, and hence is no longer in the beam, but still present, resulting in diffuse light.

The absorption coefficient of a volume, denoted μ_a, and the scattering coefficient of a volume, denoted μ_s, are defined the same way as the attenuation coefficient.<ref name="ISO_9288-1989"/>

The attenuation coefficient of a volume is the sum of absorption coefficient and scattering coefficients:<ref name="ISO_9288-1989"/>

<math>\begin{align}

                  \mu &= \mu_\mathrm{a} + \mu_\mathrm{s}, \\
              \mu_\nu &= \mu_{\mathrm{a},\nu} + \mu_{\mathrm{s},\nu}, \\
          \mu_\lambda &= \mu_{\mathrm{a},\lambda} + \mu_{\mathrm{s},\lambda}, \\
           \mu_\Omega &= \mu_{\mathrm{a},\Omega} + \mu_{\mathrm{s},\Omega}, \\
     \mu_{\Omega,\nu} &= \mu_{\mathrm{a},\Omega,\nu} + \mu_{\mathrm{s},\Omega,\nu}, \\
 \mu_{\Omega,\lambda} &= \mu_{\mathrm{a},\Omega,\lambda} + \mu_{\mathrm{s},\Omega,\lambda}.

\end{align}</math>

Just looking at the narrow beam itself, the two processes cannot be distinguished. However, if a detector is set up to measure beam leaving in different directions, or conversely using a non-narrow beam, one can measure how much of the lost radiant flux was scattered, and how much was absorbed.

In this context, the "absorption coefficient" measures how quickly the beam would lose radiant flux due to the absorption alone, while "attenuation coefficient" measures the total loss of narrow-beam intensity, including scattering as well. "Narrow-beam attenuation coefficient" always unambiguously refers to the latter. The attenuation coefficient is at least as large as the absorption coefficient; they are equal in the idealized case of no scattering.

Mass attenuation, absorption, and scattering coefficients

The mass attenuation coefficient, mass absorption coefficient, and mass scattering coefficient are defined as<ref name="ISO_9288-1989"/>

<math>\frac{\mu}{\rho_m},\quad \frac{\mu_\mathrm{a}}{\rho_m},\quad \frac{\mu_\mathrm{s}}{\rho_m},</math>

where ρ_m is the mass density.

Napierian and decadic attenuation coefficients

Decibels

Engineering applications often express attenuation in the logarithmic units of decibels, or "dB", where 10 dB represents attenuation by a factor of 10. The units for attenuation coefficient are thus dB/m (or, in general, dB per unit distance). Note that in logarithmic units such as dB, the attenuation is a linear function of distance, rather than exponential. This has the advantage that the result of multiple attenuation layers can be found by simply adding up the dB loss for each individual passage. However, if intensity is desired, the logarithms must be converted back into linear units by using an exponential: <math>I = I_o 10^{-(dB/10)}.</math>

Naperian attenuation

The decadic attenuation coefficient or decadic narrow beam attenuation coefficient, denoted μ₁₀, is defined as

Just as the usual attenuation coefficient measures the number of e-fold reductions that occur over a unit length of material, this coefficient measures how many 10-fold reductions occur: a decadic coefficient of 1 m⁻¹ means 1 m of material reduces the radiation once by a factor of 10.

μ is sometimes called Napierian attenuation coefficient or Napierian narrow beam attenuation coefficient rather than just simply "attenuation coefficient". The terms "decadic" and "Napierian" come from the base used for the exponential in the Beer–Lambert law for a material sample, in which the two attenuation coefficients take part:

<math>T = e^{-\int_0^\ell \mu(z)\mathrm{d}z} = 10^{-\int_0^\ell \mu_{10}(z)\mathrm{d}z},</math>

where

T is the transmittance of the material sample;
ℓ is the path length of the beam of light through the material sample.

In case of uniform attenuation, these relations become

Cases of non-uniform attenuation occur in atmospheric science applications and radiation shielding theory for instance.

The (Napierian) attenuation coefficient and the decadic attenuation coefficient of a material sample are related to the number densities and the amount concentrations of its N attenuating species as

<math>\begin{align}

      \mu(z) &= \sum_{i = 1}^N \mu_i(z) = \sum_{i = 1}^N \sigma_i n_i(z), \\
 \mu_{10}(z) &= \sum_{i = 1}^N \mu_{10,i}(z) = \sum_{i = 1}^N \varepsilon_i c_i(z),

\end{align}</math> where

σ_i is the attenuation cross section of the attenuating species i in the material sample;
n_i is the number density of the attenuating species i in the material sample;
ε_i is the molar attenuation coefficient of the attenuating species i in the material sample;
c_i is the amount concentration of the attenuating species i in the material sample,

by definition of attenuation cross section and molar attenuation coefficient.

Attenuation cross section and molar attenuation coefficient are related by

<math>\varepsilon_i = \frac{N_\text{A}}{\ln{10}}\,\sigma_i,</math>

and number density and amount concentration by

where N_A is the Avogadro constant.

The half-value layer (HVL) is the thickness of a layer of material required to reduce the radiant flux of the transmitted radiation to half its incident magnitude. The half-value layer is about 69% (ln 2) of the penetration depth. Engineers use these equations predict how much shielding thickness is required to attenuate radiation to acceptable or regulatory limits.

Attenuation coefficient is also inversely related to mean free path. Moreover, it is very closely related to the attenuation cross section.

Other radiometric coefficients

Radiometry coefficients
v
t
e
Quantity		SI units	Notes
Name	Sym.	SI units	Notes
Hemispherical emissivity	$ε$	—	Radiant exitance of a surface, divided by that of a black body at the same temperature as that surface.
Spectral hemispherical emissivity	$ε ν$ $ε λ$	—	Spectral exitance of a surface, divided by that of a black body at the same temperature as that surface.
Directional emissivity	$ε Ω$	—	Radiance emitted by a surface, divided by that emitted by a black body at the same temperature as that surface.
Spectral directional emissivity	$ε Ω, ν$ $ε Ω, λ$	—	Spectral radiance emitted by a surface, divided by that of a black body at the same temperature as that surface.
Hemispherical absorptance	$A$	—	Radiant flux absorbed by a surface, divided by that received by that surface. This should not be confused with "absorbance".
Spectral hemispherical absorptance	$A ν$ $A λ$	—	Spectral flux absorbed by a surface, divided by that received by that surface. This should not be confused with "spectral absorbance".
Directional absorptance	$A Ω$	—	Radiance absorbed by a surface, divided by the radiance incident onto that surface. This should not be confused with "absorbance".
Spectral directional absorptance	$A Ω, ν$ $A Ω, λ$	—	Spectral radiance absorbed by a surface, divided by the spectral radiance incident onto that surface. This should not be confused with "spectral absorbance".
Hemispherical reflectance	$R$	—	Radiant flux reflected by a surface, divided by that received by that surface.
Spectral hemispherical reflectance	$R ν$ $R λ$	—	Spectral flux reflected by a surface, divided by that received by that surface.
Directional reflectance	$R Ω$	—	Radiance reflected by a surface, divided by that received by that surface.
Spectral directional reflectance	$R Ω, ν$ $R Ω, λ$	—	Spectral radiance reflected by a surface, divided by that received by that surface.
Hemispherical transmittance	$T$	—	Radiant flux transmitted by a surface, divided by that received by that surface.
Spectral hemispherical transmittance	$T ν$ $T λ$	—	Spectral flux transmitted by a surface, divided by that received by that surface.
Directional transmittance	$T Ω$	—	Radiance transmitted by a surface, divided by that received by that surface.
Spectral directional transmittance	$T Ω,ν$ $T Ω, λ$	—	Spectral radiance transmitted by a surface, divided by that received by that surface.
Hemispherical attenuation coefficient	$μ$	m⁻¹	Radiant flux absorbed and scattered by a volume per unit length, divided by that received by that volume.
Spectral hemispherical attenuation coefficient	$μ ν$ $μ λ$	m⁻¹	Spectral radiant flux absorbed and scattered by a volume per unit length, divided by that received by that volume.
Directional attenuation coefficient	$μ Ω$	m⁻¹	Radiance absorbed and scattered by a volume per unit length, divided by that received by that volume.
Spectral directional attenuation coefficient	$μ Ω, ν$ $μ Ω, λ$	m⁻¹	Spectral radiance absorbed and scattered by a volume per unit length, divided by that received by that volume.

References

External links

Absorption Coefficients α of Building Materials and Finishes
Sound Absorption Coefficients for Some Common Materials
Tables of X-Ray Mass Attenuation Coefficients and Mass Energy-Absorption Coefficients from 1 keV to 20 MeV for Elements Z = 1 to 92 and 48 Additional Substances of Dosimetric Interest
IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version: (2006–) "Absorption coefficient". doi:10.1351/goldbook.A00037

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Attenuation coefficient

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Contents

Overview

Mathematical definitions

Attenuation coefficient

Spectral hemispherical attenuation coefficient

Directional attenuation coefficient

Spectral directional attenuation coefficient

Absorption and scattering coefficients

Mass attenuation, absorption, and scattering coefficients

Napierian and decadic attenuation coefficients

Decibels

Naperian attenuation

Other radiometric coefficients

See also

References

External links

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Attenuation coefficient

Overview

Mathematical definitions

Attenuation coefficient

Spectral hemispherical attenuation coefficient

Directional attenuation coefficient

Spectral directional attenuation coefficient

Absorption and scattering coefficients

Mass attenuation, absorption, and scattering coefficients

Napierian and decadic attenuation coefficients

Decibels

Naperian attenuation

Other radiometric coefficients

See also

References

External links

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