The story of the universe. Volume 2 (of 4) : $b The earth : land and sea
History
The story of the universe. Volume 2 (of 4) : $b The earth : land and sea
Astronomy; Earth (Planet); Natural history
Descartes proved that, according to the principles of refraction, a
circular band of light must appear in the heavens exactly where the
rainbow is seen. But how are the colors of the bow to be accounted
for? Here his penetrative mind came to the very verge of the
solution, but the limits of knowledge at the time barred his further
progress. He connected the colors of the rainbow with those produced
by a prism; but then these latter needed explanation just as much as
the colors of the bow itself. The solution, indeed, was not possible
until the composite nature of white light had been demonstrated by
Newton. Applying the law of Snell to the different colors of the
spectrum, Newton proved that the primary bow must consist of a series
of concentric circular bands, the largest of which is red and the
smallest violet; while in the secondary bow these colors must be
reversed. The main secret of the rainbow, if I may use such language,
was thus revealed.
I have said that each color of the rainbow is carried to the eye by
a sheaf of approximately parallel rays. But what determines this
parallelism? Here our real difficulties begin. Let us endeavor to
follow the course of the solar rays before and after they impinge
upon a spherical drop of water. Take, first of all, the ray that
passes through the centre of the drop. This particular ray strikes
the back of the drop as a perpendicular, its reflected portion
returning along its own course. Take another ray close to this
central one and parallel to it--for the sun’s rays when they reach
the earth are parallel. When this second ray enters the drop it is
refracted; on reaching the back of the drop it is there reflected,
being a second time refracted on its emergence from the drop. Here
the incident and the emergent rays inclose a small angle with each
other. Take, again, a third ray a little further from the central
one than the last. The drop will act upon it as it acted upon its
neighbor, the incident and the emergent rays inclosing in this
instance a larger angle than before. As we retreat further from the
central ray the enlargement of this angle continues up to a certain
point, where it reaches a maximum, after which further retreat
from the central ray diminishes the angle. Now, a maximum resembles
the ridge of a hill, or a watershed, from which the land falls in a
slope at each side. In the case before us the divergence of the rays
when they quit the raindrop would be represented by the steepness
of the slope. On the top of the watershed--that is to say, in the
neighborhood of our maximum--is a kind of summit-level, where the
slope for some distance almost disappears. But the disappearance of
the slope indicates, as in the case of our raindrop, the absence of
divergence. Hence we find that at our maximum, and close to it, there
issues from the drop a sheaf of rays which are nearly, if not quite,
parallel to each other. They are the so-called “effective rays” of
the rainbow.
Public-domain text, read in full here on John Shaqi.
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