Popular lectures on scientific subjects : $b Second series, with an autobiography of the authorHelmholtz, Hermann von
Science
Popular lectures on scientific subjects : $b Second series, with an autobiography of the author
Helmholtz, Hermann von
Science; Universities and colleges -- Germany
The easiest method of producing accurately measurable differences in
the brightness of two white surfaces, depends on the use of rapidly
rotating disks. If a disk, like the adjacent one in Fig. 3, is made to
rotate very rapidly (that is, 20 to 30 times in a second), it appears
to the eye to be covered with three grey rings as in Fig. 4. The
reader must, however, figure to himself the grey of these rings, as
it appears on the rotating disk of Fig. 3, as a scarcely perceptible
shade of the ground. When the rotation is rapid each ring of the disk
appears illuminated, as if all the light which fell upon it had been
uniformly distributed over its entire surface. Those rings, in which
are the black bands, have somewhat less light than the quite white
ones, and if the breadth of the marks is compared with the length of
half the circumference of the corresponding ring, we get the fraction
by which the intensity of the light in the white ground of the disk is
diminished in the ring in question. If the bands are all equally broad,
as in Fig. 3, the inner rings appear darker than the outer ones, for in
this latter case the same loss of light is distributed over a larger
area than in the former. In this way extremely delicate shades of
brightness may be obtained, and by this method, when the strength of
the illumination varies, the brightness always diminishes by the _same
proportion_ of its total value. Now it is found, in accordance with
Fechner’s law, that the distinctness of the rings is nearly constant
for very different strengths of light. We exclude, of course, the
cases of too dazzling or of too dim a light. In both cases the finer
distinctions can no longer be perceived by the eye.
The case is quite different when for different strengths of
illumination we produce differences which always correspond to the same
quantity of light. If, for instance, we close the shutter of a room
at daytime, so that it is quite dark, and now light it by a candle,
we can discriminate without difficulty the shadows, such as that of
the hand, thrown by the candle on a sheet of white paper. If, however,
the shutters are again opened, so that daylight enters the room, for
the same position of the hand we can no longer recognise the shadow,
although there falls on that part of the white sheet, which is not
struck by this shadow, the same excess of candle-light as upon the
parts shaded by the hand. But this small quantity of light disappears
in comparison with the newly added daylight, provided that this strikes
all parts of the white sheet uniformly. You see then that, while the
difference between candle-light and darkness can be easily perceived,
the equally great difference between daylight, on the one hand, and
daylight plus candle-light on the other, can be no longer recognised.
Public-domain text, read in full here on John Shaqi.
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