Six Lectures on Light: Delivered In The United States In 1872-1873Tyndall, John
Science
Six Lectures on Light: Delivered In The United States In 1872-1873
Tyndall, John
Light
'It is well known that if a plate of selenite sufficiently thin be
placed between two Nicol's prisms, or, more technically speaking,
between a polarizer and analyzer, colour will be produced. And the
question proposed is, What is the nature of that colour? is it
simply a pure colour of the spectrum, or is it a compound, and if
so, what are its component parts? The answer given by the wave
theory is in brief this: In its passage through the selenite plate
the rays have been so separated in the direction of their vibrations
and in the velocity of their transmission, that, when re-compounded
by means of the analyzer, they have in some instances neutralized
one another. If this be the case, the fact ought to be visible when
the beam emerging from the analyzer is dispersed by the prism; for
then we have the rays of all the different colours ranged side by
side, and, if any be wanting, their absence will be shown by the
appearance of a dark band in their place in the spectrum. But not
only so; the spectrum ought also to give an account of the other
phenomena exhibited by the selenite when the analyzer is turned
round, viz. that when the angle of turning amounts to 45°, all trace
of colour disappears; and also that when the angle amounts to 90°,
colour reappears, not, however, the original colour, but one
complementary to it.
'You see in the spectrum of the reddish light produced by the
selenite a broad but dark band in the blue; when the analyzer is
turned round the band becomes less and less dark, until when the
angle of turning amounts to 45° it has entirely disappeared. At this
stage each part of the spectrum has its own proportional intensity,
and the whole produces the colourless image seen without the
spectroscope. Lastly, as the turning of the analyzer is continued, a
dark band appears in the red, the part of the spectrum complementary
to that occupied by the first band; and the darkness is most
complete when the turning amounts to 90°. Thus we have from the
spectroscope a complete account of what has taken place to produce
the original colour and its changes.
'It is further well known that the colour produced by a selenite, or
other crystal plate, is dependent upon the thickness of the plate.
And, in fact, if a series of plates be taken, giving different
colours, their spectra are found to show bands arranged in different
positions. The thinner plates show bands in the parts of the
spectrum nearest to the violet, where the waves are shorter, and
consequently give rise to redder colours; while the thicker show
bands nearer to the red, where the waves are longer and consequently
supply bluer tints.
Public-domain text, read in full here on John Shaqi.
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