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Principles of Fluorescence Spectroscopy

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PRINCIPLES OF FLUORESCENCE SPECTROSCOPY 195<br />

one component allows the emission spectrum <strong>of</strong> the second<br />

component to be directly recorded. This procedure is experimentally<br />

simple and can be used to record the emission<br />

spectra <strong>of</strong> fluorophores with closely spaced lifetimes. PSDF<br />

is frequently used in fluorescence lifetime imaging microscopy<br />

(Chapter 22).<br />

5.12.1. Theory <strong>of</strong> Phase-Sensitive Detection <strong>of</strong><br />

<strong>Fluorescence</strong><br />

A phase fluorometer, when coupled with phase-sensitive<br />

detection <strong>of</strong> fluorescence, can be used in a simple manner<br />

to resolve heterogeneous fluorescence. Consider a sample<br />

containing a single fluorescent species with a lifetime τ.<br />

When excited with sinusoidally modulated light the emission<br />

is given by<br />

F(t) 1 m Lm sin (ωt φ)<br />

(5.66)<br />

where m L is the modulation <strong>of</strong> the exciting light. In this<br />

equation, m and φ are related to the lifetime by eqs. 5.3 and<br />

5.4. Since phase-sensitive spectra are typically measured at<br />

a single modulation frequency the subscript ω has been<br />

dropped for simplicity. If the sample contains more than<br />

one fluorophore then the modulated emission at each wavelength<br />

(λ) is given by<br />

F(λ,t) ∑ i<br />

(5.67)<br />

In this expression I i (λ) are the individual emission spectra,<br />

f i are the fractional intensities to the total steady-state intensity,<br />

Ef i = 1.0, m i is the modulation <strong>of</strong> the ith component,<br />

and φ i is its phase angle. Depending upon the needs <strong>of</strong> the<br />

experiment, the steady-state spectra <strong>of</strong> each species I i (λ)<br />

can be replaced by the steady-state spectra <strong>of</strong> the sample<br />

I(λ) and the wavelength-dependent fractional intensities:<br />

F(λ,t) I(λ) ∑ i<br />

I i(λ)f im i sin (ωt φ i)<br />

f i(λ)m i sin (ωt φ i)<br />

(5.68)<br />

In eqs. 5.67 and 5.68 we have assumed that the sample contains<br />

discrete lifetimes characterized by m i and φ i , rather<br />

than a non-exponential decay or a lifetime distribution.<br />

Phase-sensitive detection is accomplished by multiplying<br />

the emission F(λ,t) by a square wave, and integrating<br />

the result over time to yield a steady-state intensity. 1–9 The<br />

Figure 5.49. Phase-sensitive detection <strong>of</strong> fluorescence. The detector<br />

phase (φ D ) can be in phase with the emission φ D = φ (top), out <strong>of</strong> phase<br />

with the emission (φ D = φ + 90°, middle), or at some intermediate<br />

value (bottom).<br />

square wave is usually regarded as having a value <strong>of</strong> 0 or 1<br />

depending on the angle within a single period <strong>of</strong> 2π (Figure<br />

5.49):<br />

{ <br />

0 from 0 to φ D<br />

1 from φ D to φ D π<br />

0 from φ D to φ D 2π<br />

(5.69)<br />

Typically the phase angle <strong>of</strong> the detector (φ D) is varied to<br />

integrate the emission over various portions <strong>of</strong> the 0 to 2π<br />

cycle.<br />

The phase-sensitive detector yields a direct current signal<br />

proportional to the modulated amplitude and to the<br />

cosine <strong>of</strong> the phase difference between the detector phase<br />

φ D and the phase <strong>of</strong> the sample. If an emission spectrum <strong>of</strong><br />

a sample containing a single fluorophore (lifetime) is<br />

scanned using phase-sensitive detection, one observes a<br />

steady-state spectrum whose amplitude depends on the<br />

detector phase angle φ D and the phase angle <strong>of</strong> the fluorophore<br />

φ 1 :<br />

F(λ, φ D) kF(λ)m cos (φ D φ 1)<br />

(5.70)

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