The Microscope. Its History, Construction, and Application 15th ed.: Being a familiar introduction to the use of the instrument, and the study of microscopical scienceHogg, Jabez
History
The Microscope. Its History, Construction, and Application 15th ed.: Being a familiar introduction to the use of the instrument, and the study of microscopical science
Hogg, Jabez
Microscopy; Natural history
In the construction of the microscope, either simple or compound, the
curvature of the lenses employed is usually spherical. Convergent
lenses, with spherical curvatures, have the defect of not bringing all
the rays of light which pass through them to one and the same focus.
Each circle of rays from the axis of the lens to its circumference
has a different focus, as shown in Fig. 15. The rays _a a_, which
pass through the lens near its circumference, are seen to be _more
refracted_, or come to a focus at a shorter distance behind it than
the rays _b b_, which pass through near its centre or axis, and are
_less refracted_. The consequence of this defect of lenses with
spherical curvatures, which is called _spherical aberration_, is that
a well-defined image or picture is not formed by them, for when the
object is focussed, for the circumferential rays, the picture projected
to the eye is rendered indistinct by a halo or confusion produced by
the central rays falling in a circle of dissipation, before they have
come to a focus. On the other hand, when placed in the focus of the
central rays, the picture formed by them is rendered indistinct by the
halo produced by the circumferential rays, which have already come to
a focus and crossed, and now fall in a state of divergence, forming a
circle of dissipation. The grosser defects of spherical aberration are
corrected by cutting off the passage of the rays _a a_, through the
circumferences of the lens, by means of a stop diaphragm, so that the
central rays, _b b_, only are concerned in the formation of the image.
This defect is reduced to a minimum, by using the meniscus form of
lens, which is the segment of an ellipsoid instead of a sphere.
[Illustration: Fig. 15.--Spherical Aberration of Lens.]
The ellipse and the hyperbola are forms of lenses in which the
curvature diminishes from the central ray, or axis, to the
circumference _b_; and mathematicians have shown that spherical
aberration may be practically got rid of by employing lenses whose
sections are ellipses or hyperbolas. The remarkable discovery of
these forms of lenses is attributed to Descartes, who mathematically
demonstrated the fact.
If _a l_, _a l′_, for example (Fig. 16) be part of an ellipse whose
greater axis is to the distance between its foci _f f_ as the index of
refraction is to unity, then parallel rays _r l′_, _r′′ l_ incident
upon the elliptical surface _l′ a l_, will be refracted by the single
action of that surface into lines which would meet exactly in the
farther focus _f_, if there were no second surface intervening between
_l a l′_ and _f_. But as every useful lens must have two surfaces, we
have only to describe a circle _l a′ l′_ round _f_ as a centre, for the
second surface of the lens _l′ l_.
[Illustration: Fig. 16.--Converging Meniscus.]
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