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Thin-Layer Chromatography

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24 2 Physical Methods of Detection<br />

a)<br />

100<br />

50<br />

b)<br />

100<br />

^50<br />

200 300 100 500<br />

10<br />

200 300 (00<br />

X [nml<br />

Fig. 16: Relative intensity distribution of a mercury NK 4/4 low pressure lamp (A) and of a<br />

mercury St 41 or St 48 lamp (B).<br />

Detectors<br />

The commercial instruments employ detectors of various types. Their utility depends<br />

fundamentally on<br />

• the constancy with time of the photocurrent at constant radiation levels and<br />

constant external conditions,<br />

• the proportionality of the photocurrent to the intensity of illumination and<br />

• the signal to noise ratio of the photodetector.<br />

A role is also played by the temperature and frequency dependence of the<br />

photocurrent, the variable surface sensitivity at various parts of the cathode and<br />

the vector effect of polarized radiation [40]. All the detectors discussed below are<br />

electronic components whose electrical properties vary on irradiation. The effects<br />

depend on external (photocells, photomultipliers) or internal photo effects (photoelements,<br />

photodiodes).<br />

500<br />

Z.Z ueieciwn OJ Aosurum% ouusiurwa ij<br />

Photocells and photomultipliers (secondary electron multipliers, SEM) are mainly<br />

employed in photometry. These are detectors with an "external photo-effect".<br />

Photocells: The basic construction of a photocell is illustrated in Figure 17. A<br />

photocurrent flows when the photocathode is illuminated, this is proportional to<br />

the intensity of illumination if the supply potential has been chosen to be higher<br />

than the saturation potential. A minimal potential is required between the<br />

photocathode and the anode in order to be able to "collect" the electrons that are<br />

emitted. The sensitivity is independent of frequency up to 10 7 Hz. The temperature<br />

sensitivity of evacuated photocells is very small. The dark current (see below) is<br />

ca. 10~ n A[l].<br />

Cathode / Vs -<br />

l<br />

- 0<br />

r 0<br />

( fV 1 3-100 V<br />

Anode \T>J<br />

r 1<br />

Fig. 17: The construction of a photocell, schematic [1].<br />

Samples of analytical units with photocells :<br />

• TURNER fluorimeter, model III (CAMAG)<br />

• Quick Scan R & D densitometer (HELENA)<br />

• Fiber optic densitometer, model 800 (KONTES)<br />

Photomultipliers: Secondary electron multipliers, usually known as photomultipliers,<br />

are evacuated photocells incorporating an amplifier. The electrons emitted<br />

from the cathode are multiplied by 8 to 14 secondary electrodes (dynodes). A<br />

diagramatic representation for 9 dynodes is shown in Figure 18 [5]. Each electron<br />

impact results in the production of 2 to 4 and maximally 7 secondary electrons at<br />

each dynode. This results in an amplification of the photocurrent by a factor of 10 6<br />

to 10 8 . It is, however, still necessary to amplify the output of the photomultiplier.

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