So much for the eye and ear method of transit observation. There is
another which has now to a very large extent superseded it. This is
called the “chronographic method”; we owe it to Sir Charles Wheatstone,
who made it possible about 1840.
Figs. 124-7 are from drawings of the chronograph in use at Greenwich,
and by their means we hope to make the principle of the instrument
clear. In this chronograph, _g_ is a long conical pendulum which
regulates the driving clock in the case below it, through the gearing of
wheel-work, as it turns the cylinder, E, gently and regularly round. On
the cylinder is placed paper to receive the mark registering the
observations; along the side of the cylinder or roller run two long
screws, K and N, Fig. 125, which are also turned by the clock, and on
them are carried electro-magnets, A, B, Fig. 125, and prickers, 35, Fig.
126; as the screws turn, the magnets and prickers are moved along the
roller, and, as the roller turns, the pointer, 36, Fig. 127, traces a
fine line on the paper like the worm of a screw on the surface; and it
is close to this line, which serves as a guide to the eye, that the
prickers make a mark each time a current is sent through the
electro-magnets; this turns each of them into a magnet, and they then
attract a piece of iron which, in moving upwards, presses down its
pricker by means of a lever, and registers the instant the current is
sent.
The different wires are brought, first from the transit circle to work
one pricker, and then from the clock to work the other, the clock
sending a current and producing a prick on the roller every second.
[Illustration:
FIG. 124.—The Greenwich chronograph. General view.
]
The observer, instead of depending upon the eye and ear as he had to do
before, has then the means of impressing a mark at any instant upon the
same cylinder, in exactly the same way that the pendulum of the clock
impresses the mark of any second, so that as each wire in the eyepiece
of the transit instrument is passed by the star, he is able, by the same
method as the clock, to record on this same revolving surface each
observation, which can afterwards be compared with the marks
representing the seconds, and so the exact time of each observation is
read off more accurately and with less trouble than by the old method.
Let us suppose we are making a transit observation: the clock will be
diligently pricking sidereal seconds, while we, by a contact-maker held
in the hand, are as diligently recording the moments at which the star
passes each wire.
[Illustration:
FIG. 125.—Details of the travelling carriage which carries the magnets
and prickers. Side view and view from above.
]
[Illustration:
FIG. 126.—Showing how on the passage of a current round the soft iron
the pricker is made to make a mark on the spiral line on the
cylinder.
]
[Illustration:
FIG. 127.—Side view of the carriage carrying the magnets and the
pointer that draws the spiral.
]
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