ID¼
n
2 l 0 cEtotalEtotal¼n
2 l 0 cE^2 s0þE^2 r0þ2Es0Er0cos2ðkzrkzsÞð 10 : 5 ÞHere n is the refractive index of the transmission medium (e.g., n≈1.5 for
glass),μ 0 is the magnetic permeability, and the asterisk (*) denotes the complex
conjugate. Letting the intensity from the sample be
Is0¼
n
2 l 0 cE^2 so ð 10 : 6 Þand letting the intensity from the reference mirror be
Ir0¼n
2 l 0 cE^2 ro ð 10 : 7 Þthen the intensity at the detector can be expressed as
ID¼Is0þIr0þ 2ffiffiffiffiffiffiffiffiffiffi
Is0Ir0p
cos 22 p
kðzrzsÞð 10 : 8 Þwhereλ=2π/k is the wavelength of the optical source. The factor zr−zsis the
path length difference between the reference and the sample arms.
Alternatively, Eq. (10.8) can be written in terms of the optical power received at
the detector as
PD¼Ps0þPr0þ 2ffiffiffiffiffiffiffiffiffiffiffiffi
Ps0Pr0p
cos 22 p
k
ðzrzsÞð 10 : 9 Þwhere Pr0and Ps0are the monochromatic powers from the reference and sample
arms, respectively. In Eqs. (10.8) and (10.9) thefirst two terms are constants for
particular reflection values, whereas the third term represents the wave interference.
When the factor in square brackets in the cosine term is 0 or a multiple of± 2 πthe
cosine value is a maximum of 1, thereby yielding a maximum optical power at the
detector.
For an actual OCT setup, the source is not monochromatic. In fact, as described
below, to increase the axial resolution it is desirable to have a coherent light source
with a wide spectral width. In this case the total optical power falling on the detector
is found by integrating over the entire spectrum of the light source, thereby yielding
PD¼PsþPrþ 2ffiffiffiffiffiffiffiffiffi
PsPrp
sincpðzrzsÞ
lccos 22 p
kðzrzsÞð 10 : 10 ÞHere Prand Psare the wideband spectral optical powers from the reference and
sample arms, respectively,λ 0 is the center wavelength of the optical source,lcis the
source coherence length, and thesinc functionis defined by sinc x = (sin x)/x.
10.1 Optical Coherence Tomography 297