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124

C.E. Riva

 

 

fast development of this device and optical techniques associated with it, this principle has led over the last 35 years to the measurement of blood ßow in a number of tissues of the body [1]. In 1972, the retina provided the Þrst measurements of blood velocity obtained by means of the Doppler shift [2]. LDV measurement of blood velocity in human retinal vessels was published 2 years later [3]. Subsequent to the pioneering work of Stern [4], who assessed blood ßow in the tissue of the skin, Riva et al. [5] described a method to measure blood velocity in the human optic nerve microcirculation. This method was then extended to the measurement of blood ßow in the vascular bed of the cat optic nerve head (ONH) [6], the human ONH [7, 8], and the subfoveal choroid [9]. In 1995, Michelson and Schmauss Þrst reported mapping of blood ßow in the microcirculation of the human retina by means of scanning LDF [10].

The present chapter is by no means an exhaustive description of LDV and LDF. Regrettably, due to limitation of space, a choice of papers and reviews among the extensive laser Doppler literature related to the eye had to be made. Part of the material of this chapter has been reproduced with permission from previous publications [11Ð14].

7.2Retinal Laser Doppler Velocimetry

7.2.1The Doppler Effect

The basis of LDV and LDF is the Doppler effect, Þrst described in 1842 by the Austrian physicist Christian Doppler in an article entitled ÒOn the Colored Light of Double Stars and Some Other Heavenly Bodies.Ó Doppler describes the frequency shift that a sound or a light wave undergoes when emitted from an object that is moving away or towards an observer. It manifests itself, for example, in the increase in the pitch of the siren of an approaching ambulance.

Consider a particle, such as a red blood cell (RBC), moving at velocity V (Fig. 7.1). A laser

fo + f

fo

ai

aS

RBC

V

Fig. 7.1 The Doppler effect: The frequency of the light scattered by the particle moving at the velocity V in the direction deÞned by as is shifted in frequency by an amount Df compared to that of the incident light (frequency f0 and direction deÞned by ai with V)

beam of single frequency, f0, is incident on this particle. This beam, which is deÞned by the wave vector Ki, will be scattered by the particle in vari-

ous directions. The beam scattered in the direc-

tion of the detector, deÞned by Ks , is shifted in frequency by an amount:

 

1

 

 

1

 

 

Df =

(Ks

- Ki ) ·V =

(K) ·V

(7.1)

2p

2p

where the symbol (¥) represents the scalar prod-

 

 

 

 

 

 

uct and K = Ks

- Ki ¥

Ks

@

Ki

@ 2π n / λ ¥ n is the

refractive index of the medium and λ is the wavelength in vacuo of the incident laser light.

In order to determine Df , the scattered light must be detected by a sensor, which transforms the electric Þeld of the scattered light incident upon it into a current. This current is in turn processed to determine its frequency content. The technique by which Df is determined from the scattered Þeld is known as Òoptical mixing spectroscopy (OMS)Ó or Òlight beating spectroscopyÓ [15, 16].

Understanding the application of OMS to the measurement of RBC velocity in retinal vessels requires a description of the electric Þeld of the scattered light, followed by that of the current at the output of the detector. This description will be Þrst carried out in the simpliÞed case of singly scattering particles moving in a glass capillary tube and then extended to multiply scattering RBCs.

7 Laser Doppler Techniques for Ocular Blood Velocity and Flow

125

 

 

Fig. 7.2 (a) Schematic representation of a volume of a

capillary tube illuminated by an

incident wave deÞned by

 

cosω

t and with the wave

E

o

o

 

vector Ki . The light scattered by the particles moving in the tube and the vessel wall is deÞned by Ks . (b) Assumed parabolic velocity proÞle of the particles in the capillary tube. The cylindrical shell DR contains particles moving at velocity V, the value of which is given by PoiseuilleÕs law (Adapted from Riva and Feke [13] with permission from the Publisher)

E0 (Kit ) cosw0t

Es (Ks‚t ) a

b

v

R

R

7.2.2Electric Field Scattered by Singly Scattering Particles Moving in a Capillary Tube

The electric Þeld,

 

 

,t), of the light scattered in

E (K

 

s

s

 

direction Ks at time t by a dilute solution of singly scattering particles moving at constant velocity through a glass capillary tube (Fig. 7.2) consists of light scattered by both the particles and the glass

wall. The incident monochromatic beam (single

frequency, f0), Eo cosωot (ωo = 2π / f0 ), is assumed to illuminate uniformly the entire cross section of the tube.

If the particles are much smaller than the cap-

illary radius, R

, their

velocity proÞle

obeys

0

 

 

 

 

 

PoiseuilleÕ law,

i.e., V (R)

(for

simpliÞcation,

V (R) =

 

) is a parabolic function of the radial

V (R)

distance,

R,

from the axis of the tube:

 

 

 

 

ì

æ

2

ü

 

 

 

 

ï

R ö

ï

 

 

 

V (R) = Vmax í1- ç

 

÷

ý

(7.2)

 

 

 

 

 

 

ï

è

R0 ø

ï

 

 

 

 

î

 

 

 

þ

 

Vmax is the centerline (maximum) velocity of the particles. Due to this distribution of velocities, the scattered light consists of a range of Dopplershifted frequencies.

With Poiseuille ßow, if one divides the range of velocities (0 to Vmax) into N equal increments, DV, (Fig. 7.2) the particles with speeds between V and V+DV are located in a shell of radial thick-

ness DR, where from Eq. 7.2, DR=R02DV/2RVmax. Furthermore, if the concentration of particles across

the tube is uniform, there will be equal numbers of

particles ßowing at each velocity range [2].

The Þeld Es (K,t) is the sum of the Þeld scattered by the particles and the Þeld scattered by the vessel wall:

 

 

 

 

 

N

 

 

 

 

 

 

 

 

 

 

Es(K,t) = å

E

(K,t) + E

LO

(K,t)

 

(7.3)

 

 

 

 

 

i=0

i

 

 

 

 

 

 

 

 

, the Þeld scattered by the particles with

Ei (K,t)

velocity

V

i

has

the

frequency 2p(f

0

+ Df

).

 

 

 

 

 

 

 

 

 

 

i

 

ELO (K,t) is the Þeld of the light scattered from the tube wall. It has the same frequency as the incident light since the tube is not moving and acts as a reference beam, conventionally called Òlocal oscillator (LO).Ó

Under the conditions of both uniform concen-

tration of the particles and laser illumination of

the tube, each

 

has the same amplitude,

Ei (K,t)

 

 

 

 

 

A(K) and thus:

 

 

 

 

 

 

 

(7.4)

Ei (K,t) = A(K)cos 2π ( f0 + Dfi )t

 

 

 

 

 

Similarly, ELO (K,t)

can be written as:

 

 

 

 

 

 

 

ELO (K,t) = ALO (K)cos 2π f0t

(7.5)

Therefore:

 

 

 

 

 

 

 

 

Es (K,t) = ALO (K)cos 2π f0t

(7.6)

 

 

 

N

 

 

+ A(K)åcos 2π ( f0 + Dfi )t

 

i=0

126

C.E. Riva

 

 

The power spectral density of the scattered

light P ( f )

 

detected for the scattering geometry

 

Es

 

 

is obtained by applying Fourier

deÞned by

K

analysis:

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

P ( f ) =

A 2

δ ( f - f

 

 

 

 

 

 

 

 

 

LO

 

 

 

)

 

 

 

 

 

 

 

 

 

 

0

 

 

 

 

 

Es

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

ù (7.7)

 

 

 

 

A

 

 

A

N

 

é

 

 

iDf

 

 

+

 

LO

 

åδ

ê f - ( f0 +

 

 

max

)ú

 

2

 

 

N

 

 

 

 

i=0

ë

 

 

 

û

with

f0 £ f

 

£ f0 + Dfmax

 

 

 

 

 

Dfmax

corresponds

to

 

the

maximum

velocity

Vmax , and δ ( f

- f0 )

is the delta function at f0.

Thus,

for our

model,

the

optical

spectrum of

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Es (K,t) consists of a d function at f0, a ßat part of

magnitude ALO A/2 from f0 to f0 + Dfmax and zero

beyond f0 + Dfmax.

 

Since f0 is approximately

5 × 1014 Hz, and Df

i

for retinal vessels (see later)

 

 

ranges between 0 and @ 5´104 kHz , the required resolution (Df/f0) for its detection, namely <<l0−10, was far beyond the capability of spectroscopic techniques available until @ 1965 . However, with OMS, the information contained in the optical spectrum could be translated from the high frequencies of light waves down to sufÞciently low frequencies, where instruments operate with adequate resolution to resolve the spectrum of Doppler shifts.

spectral density

DSPS = Pi (Df )

of the photocur-

rent [13]:

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

β

2

 

2

é

 

2

 

2

ù2

 

 

 

 

Pi (Df ) =

4

 

S

 

ëALO

+ As û

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

é

 

2

 

2

ù

 

 

 

 

 

δ (Df ) +

 

 

 

 

 

 

+

 

 

 

 

 

 

 

eβS ëALO

As û +

 

 

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

N

 

æ

 

 

iDfmax ö

 

 

 

 

 

 

 

 

2

 

2

åδ

 

 

 

 

βSScohLO ALO

A

çDf

-

 

 

÷

 

 

N

 

 

 

 

 

 

 

 

 

 

 

 

i=1

 

è

 

 

ø

 

in the range 0 £ Df

£ Dfmax

and

 

 

 

 

 

 

1

é

 

 

2

 

 

2

ù

 

 

 

 

 

 

(7.9)

Pi

(Df ) =

 

 

 

 

+ As

 

for

 

Df

> Dfmax .

eβS ëALO

 

û

 

 

 

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Dfmax is deÞned as the cutoff frequency of Pi (Df ) .e

is the charge of the electron, and ScohLO is the coherence area of the local oscillator at the detec-

tor surface.

The third term of Pi (Df ) in Eq. 7.9 is a squared replica of the second term of PEs(f) in Eq. 7.7, but shifted down towards low frequencies, so that the particle velocities can be determined from measurements of Pi (Df ). Thus, the process of mixing at the detector surface of the light scattered by the particles with the light from the glass wall (local oscillator) results in the downshifting of the spectrum from optical frequencies to frequencies in the kHz range (Fig. 7.3), where high-resolution spectral analy-

7.2.3Doppler Shift Power Spectrum sis can be performed with conventional devices.

(DSPS) of the Photocurrent

In the application of OMS, Es (K,t) is directed

onto the surface (S) of a square wave photodetec-

tor. This Þeld generates a photocurrent, i(r,t) , where r is a point on S. The time average of this current is:

 

 

i(t) = òβ Es (K,t)dS

(7.8)

S

b is the responsivity of S. All the information on the particles velocities can be extracted from i(t) . This extraction, which is complex and beyond the scope of this chapter, leads to the following expression for the Doppler shift power

The term

1

eβ S éALO2 + A2

ù

is the photodetector

2

ë

û

 

shot noise, which is due to the stochastic nature

of the photon emission.

 

 

In general, the local oscillator is much more

intense than the Þeld scattered by the particles

so that ALO >> A. As a result, the shot noise is

 

1

eβ SALO

2 . In

practice, the ability to

measure

2

 

with

high resolution requires

that the

 

Pi (Df )

power spectral density of the signal term be larger than that of the shot noise term. A measure of this ability is the intrinsic signal-to-noise ratio (SNR), which is:

 

2b

2

N

æ

iDfmax ö

(7.10)

SNR(Df ) =

 

SScohLO A åδ ç Df -

 

÷

e

N

 

 

i=1

è

ø

 

Dfmax

7 Laser Doppler Techniques for Ocular Blood Velocity and Flow

127

 

 

Fig. 7.3 Theoretically predicted photocurrent power

spectral density, Pi(Df),

 

 

explicitly showing DC

 

 

component β 2 S 2

éA2LO + A2

ù2

at

4

ë

û

 

Df = 0, signal component,

 

β SScoh LO A2LO A2 , extending to fmax and shot noise component,

eβSA2LO (Adapted from Riva

2

and Feke [13] with permission from the Publisher)

Pi ( f )

b

2

S

2

 

[A2LO + A2 ]2

 

4

 

 

0

For given b, S, and Scoh LO , the only way to increase the SNR is to increase A2 , i.e., the intensity of the incident laser light.

7.2.4Absolute Vmax Measurements

To obtain V

 

=

 

V

 

from Df

max

using Eq. 7.1,

 

 

 

max

 

 

max

 

 

 

 

the angle between

 

Ki

and V max

and the one

 

 

 

 

V max

 

 

 

between Ks

and

 

must be known. This is

difÞcult in the living eye due mainly to the difÞculty of determining accurately the direction of blood ßow in a retinal vessel.

This problem is solved by means of a bidirectional detection scheme [17, 18], in which

is measured for two directions of the scattered light. Vmax is then obtained from the formula:

Vmax

=

λD* fmax

 

(7.11)

ncos b

 

 

 

In this equation, D* fmax = Dfmax,2 - Dfmax,1 .

is

the intraocular angle between the two scattering

directions, K1 , K2 , which can be obtained from the corresponding extraocular angle [17Ð19]. The calculation of requires the measurement of the axial length of the eye, a routine

procedure in ophthalmology [18, 20]. b is the

angle between V max and the plane deÞned by

the vectors (K1, K2 ) . n is the index of refraction of the medium. Implementation of the bidirectional scheme to a fundus camera is shown in Fig. 7.4, top.

bSS cohLO A2 LO A2

ebSA2Lo

2

fmax

f

7.2.5Experimental Test of the Bidirectional LDV Technique

With the aim of testing the validity of the bidirectional scheme [11], polystyrene latex spheres (diameter=0.3 mm) suspended in water were passed at known V max through a glass capillary tube (diameter=200 mm) placed in the retinal plane of a Topcon model eye. The incident laser beam (helium-neon, 632.8 nm) was focused on the tube which was placed at different locations of the fundus. The direction of the ßow was also varied stepwise from 0¡ (tube horizontal) to 180¡. Measurements were performed for an emmetropic and an axially ametropic (± 4 diopters) eye. DSPS were recorded for two scattering directions by means of a two-channel digital signal spectrum analyzer (Fig. 7.4, bottom). These DSPS are characterized by sharp cutoffs from

which Dfmax,1 and Dfmax,2 can be accurately determined. The value of Vmax calculated using Eq. 7.11

was found to be in good agreement (<3% difference) with the value obtained from the known ßow through the tube and the cross section of the tube. The difference was attributed to errors in and D* fmax . Feke et al. demonstrated similar results and

also

conÞrmed

the linear relationship between

D* f

max

and cos b

for a given V

and scattering

 

 

max

 

geometry ( ) [19].

The increase in spectral power in the region of the cutoff frequencies for the DSPS shown in Fig. 7.4 bottom is probably due to a nonuniform illumination of the tube by the laser beam, which was smaller than the tube internal diameter. As a

Pi (Df )

128

C.E. Riva

 

 

Vmax

 

A1

Vmax

 

 

 

K1

P1

 

 

 

 

K2

 

P2

Retinal

 

 

 

 

Laser

vessel

 

 

Prism

A2

Fundus camera optics

Fig. 7.4 Top: Fundus-camera-based scheme for the detection of light scattered from blood moving with velocity Vmax along two directions K1 and K2 deÞned by apertures A1 and A2 in the plane of the eye pupil. The beam through A2 is focused at P2 after deßection by a prism in the collecting optics. The direction P1 −P2 is aligned with that of A1 A2. The direction A1 A2 can be rotated in the plane of the pupil

for alignment with the direction of the vessel (Adapted from Riva et al. [25] with permission from the Publisher). Bottom: DSPS obtained simultaneously along two directions of the scattered light from a suspension of polystyrene spheres in water through a 200-mm-internal-diameter glass capillary tube mounted in the ÒretinalÓ plane of a model eye (Adapted from Riva et al. [18] with permission from the Publisher)

result, the faster particles received more light relative to the slower ones located close to the vessel wall. The effects of laser beam size, eccentricity, as well as absorption of light by the ßowing medium, have been reported by Petrig and Follonier [21].

7.2.6The Output Signal-to-Noise Ratio of the DSPS and Its Dependence on the Recording Time

Due to the stochastic nature of the photodetector emission process, the photocurrent is a ßuctuating quantity so that there is an uncertainty in the

measurement of the DSPS when the measurement is performed in a Þnite time. This phenomenon is illustrated by four DSPS recorded in different times from a 0.1 suspension of 1-mm-

diameter

polystyrene spheres

ßowing with a

Vmax = 3.61 cm / s

through a 200-mm-internal-

diameter

glass

capillary tube

(Fig. 7.5). As

expected, the ßuctuations of decrease as the measurement time increase. It can be shown that, based on a previous analysis [13, 16], if

Dν ´T 1,

 

 

 

1

μ

T

(7.12)

 

 

 

σ (P(Df )

 

i

 

 

 

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