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20 RAYS OF POSITIVE ELECTRICITY
the tube is big the walls are far away from the cathode and
the pressure has to be exceedingly low before the dark space reaches the sides of the tube. We can work with much lower pressures with these large tubes and therefore reduce the ob- struction which the positive rays meet with in their passage from the cathode to the screen. Using vessels of about 2 litres capacity I have observed1 on a willemite screen the parabolas corresponding to carbon, oxygen, neon, and mercury vapour as well as those corresponding to the atom and molecule of hydrogen and the atom of helium. The photo- graphic plate is, however, for most purposes a much more |
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FIG. 10.
convenient detector than a willemite screen. It is more sensi-
tive, it gives a permanent record, and measurements can be made with much greater accuracy on the plate than they can oil the screen. Before entering into the discussion of the theory of the positive rays it is desirable to describe the results obtained with the photographic method, as well as the experimental details by which these results have been pro- cured.
The apparatus now in use at the Cavendish Laboratory is
represented in Fig. 10. The discharge takes place in a large
1J. J. Thomson, " PML Mag.," VI, xx, p. 752, 1910,
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