Account of the Skerryvore lighthouse : $b with notes on the illumination of lighthousesStevenson, Alan
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Account of the Skerryvore lighthouse : $b with notes on the illumination of lighthouses
Stevenson, Alan
Skerryvore Lighthouse (Hebrides, Scotland)
It is still more obvious that a perfect paraboloïdal figure, and a
luminous _point_ mathematically true, would render the illumination
of the whole horizon by means of a fixed light _impossible_; and it
is only from the divergence caused by the size of the flame which
is substituted for the _point_, that we are enabled to render even
revolving lights practically useful. But for this aberration, the
slowest revolution in a revolving light would be inconsistent with a
continued observable series, such as the practical seamen could follow,
and would, as we have seen, render the flashes of a revolving light too
transient for any useful purpose; whilst fixed lights, being visible
in the azimuths only in which the mirrors are placed, would, over the
greater part of the distant horizon, be altogether invisible. The size
of the flame, therefore, which is placed in the focus of a paraboloïdal
mirror, when taken in connexion with the form of the mirror itself,
leads to those important modifications in the paths of the rays and the
form of the resultant beam of light, which have rendered the catoptric
system of lights so great a benefit to the benighted seamen.
In order to obtain a mirror capable of producing a given divergence of
the reflected beam, therefore, we must proportion its focal distance to
the diameter of the flame in such a manner, that the sine of _one-half_
of the whole effective divergence of the mirror, may be equal to the
_quotient of the radius of the flame, divided by the distance of a
given point on the surface of the mirror from the focus_. The best
proportions for paraboloïdal mirrors depend on the objects which they
are meant to attain. Those which are intended to give great divergence
to the resultant beams, as in fixed lights, capable of illuminating
the whole horizon at one time, should have a short focal distance;
while those mirrors which are designed to produce a nearer approach to
parallelism (as in the case of revolving lights which illuminate but a
few degrees of the horizon at any one instant of time), will have the
opposite form. Those two objects may, no doubt, be attained with the
same mirror, by increasing or diminishing the size of the burner; but
that is by no means desirable, as any change on the size of a burner,
which is found to be the best in other respects, must be considered as
to some extent disadvantageous.
Public-domain text, read in full here on John Shaqi.
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