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)
In the combination of lenses with the flame of a lamp, similar
considerations must influence us in making the necessary arrangements,
as in the case of reflectors. We have already seen that the size of
the flame and its distance from the surface of reflecting instruments
have an important practical bearing on the utility of the instrument,
and that the divergence of the resultant beam materially affects its
fitness for the purpose of a Lighthouse. So also, in the case of the
lens, unless the diameter of the flame of the lamp has to the focal
distance of the instrument a relation such as may cause an appreciable
divergence of the rays refracted through it, it could not be usefully
applied to a Lighthouse; for, without this, the light would be in sight
during so short a time, that the seaman would have much difficulty
in observing it. To determine the amount of this divergence of the
refracted beam, therefore, is a matter of great practical importance,
and I shall briefly point out the conditions which regulate its amount,
as they are nearly identical with those which determine the divergence
of a paraboloïdal mirror illuminated by a lamp in its focus. The
divergence, in the case of lenses, may be described as _the angle which
the flame subtends at the principal focus of the lens_, the maximum of
which, produced at the vertex of FRESNEL’S great lens by the lamp of
four concentric wicks, is about 5° 9′.[60]
[60]
This will be easily seen by examining the annexed figure (64), in
which Q _q_ represents the lens. A its centre, F the principal
focus, _b_ F and _b′_ F the radius of the flame; then is the angle
_b_ A _b′_ equal to the maximum divergence of the lens.
_b_ F Rad. of flame
Sin _b_ AF = ----- = sin _b′_ AF = --------------;
AF Focal distance
and twice _b_ AF = the whole divergence at A. Then for the divergence
at the margin of the lens, or at any other point, we have, FQ = √(AQ²
+ AF²) and Q _x_ = √(QF² + F _x_²); and for any angle at Q, we have
F _x_
sin FQ _x_ = -----.
FQ
[Illustration: Fig. 64.]
~Illuminating Power of Lenses.~
Public-domain text, read in full here on John Shaqi.
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