The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomyDick, Thomas
Science
The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomy
Dick, Thomas
Astronomical instruments; Astronomy; Telescopes
We have just now alluded to an experiment with a glass globe:--If,
then, we take either a solid glass globe, or a hollow globe filled with
water, and suspend it so high in the solar rays above the eye, that
the spectator, with his back to the sun, can see the globe _red_;--if
it be lowered slowly, he will see it orange, then yellow, then green,
then blue, then indigo, and then violet; so that the drop at different
heights, shall present to the eye the seven primitive colours in
succession. In this case, the globe, from its form, will act in some
measure like a prism, and the ray will be separated into its component
parts. The following figure will more particularly illustrate this
point. Suppose A (fig. 35.) to represent a drop of rain--which may be
considered as a globe of glass in miniature, and will produce the same
effect on the rays of light--and let SD represent a ray from
the sun falling upon the upper part of the drop at D. At the
point of entering the drop, it will suffer a refraction, and instead
of going forward to C, it will be bent to N. From
N a part of the light will be reflected to Q--some
part of it will, of course, pass through the drop. By the obliquity
with which it falls on the side of the drop at Q, that part
becomes a kind of prism, and separates the ray into its primitive
colours. It is found by computation that, after a ray has suffered
two refractions and one reflection, as here represented, the least
refrangible part of it, namely the _red_ ray, will make an angle with
the incident solar ray of 42° 2´, as SFQ; and the violet, or
greatest refrangible ray will make with the solar ray, an angle of 40°
17´, as SCQ; and thus all the particles of water within the
difference of those two angles, namely 1° 45´--(supposing the ray to
proceed merely from the centre of the sun)--will exhibit severally the
colours of the prism, and constitute the _interior_ bow of the cloud.
This holds good at whatever height the sun may chance to be in a shower
of rain. If he be at a high altitude, the rainbow will be low; if he be
at a low elevation, the rainbow must be high; and if a shower happen
in a vale, when the spectator is on a mountain, he will sometimes see
the bow in the form of a _complete circle_ below him. We have at
present described the phenomena only of a single drop; but it is to be
considered that in a shower of rain there are drops at all heights and
at all distances; and therefore the eye situated at G will see all the
different colours. All those drops that are in a certain position with
respect to the spectator will reflect the red rays, all those in the
next station the orange, those in the next the green, and so on with
regard to all the other colours.
[Illustration: _figure 35._]
Public-domain text, read in full here on John Shaqi.
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