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absorptance

Absorptance is the fraction of incident radiant energy that is absorbed by a material or surface. It is defined for a specific wavelength, incidence angle, and polarization, and is typically expressed as a dimensionless quantity between 0 and 1. Absorptance is complementary to the fractions that are reflected and transmitted.

In general, for a planar surface or homogeneous medium, absorptance A, reflectance R, and transmittance T satisfy

Spectral absorptance a(λ) expresses dependence on wavelength. A can also depend on incidence angle θ and polarization.

Measurement and applications: Absorptance is measured with integrating spheres and spectrometers to determine A(λ); it is

A
=
1
−
R
−
T.
For
opaque,
non-scattering
materials,
T
is
approximately
zero
and
A
≈
1
−
R.
In
a
homogeneous
slab
with
absorption
coefficient
α
and
thickness
d,
A
=
1
−
e^(−α
d).
For
thin
films,
neglecting
reflections,
A
≈
α
d
when
α
d
is
small.
Kirchhoff's
law
states
that,
at
thermal
equilibrium,
the
emissivity
ε(λ,
θ)
equals
the
absorptivity
for
the
same
wavelength
and
direction
in
opaque
bodies,
linking
absorptance
to
radiative
emission.
central
to
the
design
of
optical
coatings,
solar
cells,
detectors,
and
radiative
heat
transfer
control.
It
is
common
to
distinguish
this
optical
absorptance
from
absorbance
used
in
chemistry,
where
absorbance
A
is
defined
by
A
=
log10(I0/I)
in
Beer-Lambert
applications,
a
different
concept
from
optical
absorptance.