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Frans_M_Everaerts_Isotachophoresis_378342.pdf

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UV ABSORPTION METER 165<br />

dicular to this hole, a hole is drilled of diameter 0.3 mm with a conical shape at the<br />

outside on both ends, so that the quartz rod (4) can approach the central hole as close<br />

as possible. The diameter of the quartz rods (optical quality) is 3 mm. The distance<br />

between the quartz rods and the narrowbore tube must be made as small as possible,<br />

otherwise some of the UV light is lost by absorption by oxygen. The quartz rods are<br />

fixed by brass holders (5,ll). Before mounting, the outside of the optical quartz rods<br />

and the inside of the brass holders must be cleaned carefully with cyclohexane in order<br />

to remove all UV-absorbing material. After ths procedure, the quartz rods must be<br />

handled with a pair of clean tweezers in order to prevent dirt from sticking on the surface.<br />

An adhesive must not be used to fix the quartz rods in the holders. Any resin on the<br />

surface of the rods absorbs large amounts of W light; when the rods were fixed in the<br />

holders with Cyanolite, the signal was reduced to 1% of its original value. The two brass<br />

holders, with the quartz rods fixed simply with an O-ring, clamp the slit holder (12) by<br />

means of a set of O-rings. The flanges fit the central housing (not shown in Fig.6.30)<br />

and fixes the slit holder at a pre-determined position.<br />

The edges on the ends of the holders of the quartz rods act as an important lock for<br />

daylight, together with components 10 and 12. This lock is not as important at the side<br />

of the W source because the combined interference filter and end fdter is mounted at<br />

the side of the UV detector (8). If this lock is not positioned in front of the photodiode<br />

(R 330) at least a noisy signal may be expected and too much daylight may even destroy<br />

the phototube.<br />

The holder 9 contains the combined interference filter and end filter. In the W source<br />

(14), the UV light is generated by the microwave-powered low-pressure mercury<br />

electrodeless lamp (6). A slide (13) makes it possible for the narrowbore tube not to be<br />

exposed constantly to the UV light, which may damage the PTFE. After a long exposure<br />

time, the quality of PTFE coloured by UV light is poor. For optimal stability of the UV<br />

lamp, it is preferable to have the lamp constantly in the bright mode. After switching on,<br />

it requires at least 1.5 h to attain full optimal stability. The slit holder (12) contains an<br />

extra hole that permits the conductivity detector to be mounted near the W detector<br />

cell. It has proved to be unimportant if the sequence of either the UV detector and the<br />

conductivity detector is altered. Of course, exceptional cases can occur.<br />

6.5.6. Experimental<br />

It does not need a long explanation about the way in which the UV detector will<br />

produce supplementary information about the isotachophoretic separation, because many<br />

ions lack W absorbance and so many successively moving zones that contain ions without<br />

any UV absorbance will not be detected. In some instances, minor UV-absorbing<br />

components (see Fig.6.15) are present in the electrolytes (the leading electrolyte, the<br />

sample and the terminating electrolyte). These impurities can ‘mark’ a zone boundary,<br />

because these components are also concentrated in zones, sandwiched between the<br />

sample zones.<br />

If a mixture of mainly non-UV-absorbing components is available, one can add to<br />

the sample an extra amount of UV-absorbing markers in such a concentration that, if<br />

these markers cannot be separated from the sample ions and form stable mixed zones, they

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