The electron, its isolation and measurement and the determination of some of its properties — John Stuart Mill — John Shaqi
The electron, its isolation and measurement and the determination of some of its properties
John Stuart Mill · en
My original plan for eliminating the evaporation error was to obtain,
if possible, an electric field strong enough exactly to balance the
force of gravity upon the cloud and then by means of a sliding contact
to vary the strength of this field so as to hold the cloud balanced
throughout its entire life. In this way it was thought that the whole
evaporation-history of the cloud might be recorded, and that suitable
allowances might then be made in the observations on the rate of fall
to eliminate entirely the error due to evaporation. It was not found
possible to balance the cloud, as had been originally planned, but
it was found possible to do something much better: namely, to hold
individual charged drops suspended by the field for periods varying
from 30 to 60 seconds. I have never actually timed drops which lasted
more than 45 seconds, although I have several times observed drops
which in my judgment lasted considerably longer than this. The drops
which it was found possible to balance by an electrical field always
carried multiple charges, and the difficulty experienced in balancing
such drops was less than had been anticipated.
The procedure is simply to form a cloud and throw on the field
immediately thereafter. The drops which have charges of the same sign
as that of the upper plate or too weak charges of the opposite sign
rapidly fall, while those which are charged with too many multiples of
the sign opposite to that of the upper plate are jerked up against
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gravity to this plate. The result is that after a lapse of 7 or 8
seconds the field of view has become quite clear save for a relatively
small number of drops which have just the right ratio of charge to mass
to be held suspended by the electric field. These appear as perfectly
distinct bright points. I have on several occasions obtained but one
single such “star” in the whole field and held it there for nearly a
minute. For the most part, however, the observations recorded below
were made with a considerable number of such points in view. Thin,
flocculent clouds, the production of which seemed to be facilitated by
keeping the water-jackets , and (Fig. 2) a degree or
two above the temperature of the room, were found to be particularly
favorable to observations of this kind.