The principles of science : $b a treatise on logic and scientific methodJevons, William Stanley
Philosophy
The principles of science : $b a treatise on logic and scientific method
Jevons, William Stanley
Logic; Science -- Methodology
It is a great advantage in some instruments that they can be readily
made to manifest a phenomenon in a greater or less degree, by a very
slight change in the construction. Thus either by enlarging the bulb
or contracting the tube of the thermometer, we can make it give
more conspicuous indications of change of temperature. The ordinary
barometer, on the other hand, always gives the variations of pressure
on one scale. The torsion balance is remarkable for the extreme
delicacy which may be attained by increasing the length and lightness
of the rod, and the length and thinness of the supporting thread.
Forces so minute as the attraction of gravitation between two balls, or
the magnetic and diamagnetic attraction of common liquids and gases,
may thus be made apparent, and even measured. The common chemical
balance, too, is capable theoretically of unlimited sensibility.
The third mode of measurement, which may be called the Method of
Repetition, is of such great importance and interest that we must
consider it in a separate section. It consists in multiplying both
magnitudes to be compared until some multiple of the first is found
to coincide very nearly with some multiple of the second. If the
multiplication can be effected to an unlimited extent, without the
introduction of countervailing errors, the accuracy with which the
required ratio can be determined is unlimited, and we thus account for
the extraordinary precision with which intervals of time in astronomy
are compared together.
The fourth mode of measurement, in which we equate submultiples of
two magnitudes, is comparatively seldom employed, because it does not
conduce to accuracy. In the photometer, perhaps, we may be said to use
it; we compare the intensity of two sources of light, by placing them
both at such distances from a given surface, that the light falling
on the surface is tolerable to the eye, and equally intense from each
source. Since the intensity of light varies inversely as the square
of the distance, the relative intensities of the luminous bodies are
proportional to the squares of their distances. The equal intensity of
two rays of similarly coloured light may be most accurately ascertained
in the mode suggested by Arago, namely, by causing the rays to pass in
opposite directions through two nearly flat lenses pressed together.
There is an exact equation between the intensities of the beams when
Newton’s rings disappear, the ring created by one ray being exactly the
complement of that created by the other.
*The Method of Repetition.*
Public-domain text, read in full here on John Shaqi.
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