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
=Formation of Real Images.=--Let A B (Fig. 13) be an object in front
of a lens, at a distance less than the principal focal length. It will
have a real image on the other side of the lens. To determine the
position of the image by construction, draw through any point A of the
object a line parallel to the principal axis, meeting the lens in A′.
The ray represented by this line will, after refraction, pass through
the principal focus, F, and its intersection with the secondary axis,
A O, determines the position of _a_, the focus conjugate to A. We can
in like manner determine the position of _b_, the focus conjugate to B,
another point of the object; and the joining line _a b_ will then be
the magnified image of the line A B. It is evident that if _a b_ were
the object, A B would be the image.
[Illustration: Fig. 13.--Real and Magnified Image.]
The figures 12 and 13 represent the cases in which the distance of the
object is respectively greater and less than twice the focal length of
the lens.
The focal length of a lens is determined by the convexity of its
surfaces and the refractive power of the material of which it is
composed, being shortened either by an increase of refractive power,
or diminution of the radii of curvature of the faces of the lens. The
increase or decrease of spherical aberration is determined by the
shape or curvature of the lens; it is less in the bi-convex than in
other forms. When a lamp or other source of light is placed at the
focus of the rays constituting that portion of its light which falls
upon the lens, the light is so refracted as to become parallel. Should
the source of light be brought nearer to the lens than the focus the
refracted rays are still divergent, though not to the same extent;
on the other hand, if the source be beyond the focus, the refracted
rays are rendered convergent so as to meet at a point which is
mathematically related to the distance of the luminous source from the
focus. The former arrangement is that with which we are most familiar,
since it is the ordinary magnifying glass.
Concave Lenses.
The refracting influence of a _concave_ lens (Fig. 14) will be
precisely the opposite of that of a convex. Rays which fall upon it in
a parallel direction will be made to diverge as if from the principal
focus, which is here called the _negative_ focus. This will be, for a
_plano-concave_ lens, at the distance of the diameter of the sphere of
curvature; and for a _double-concave_, in the centre of that sphere.
[Illustration: Fig. 14.--A Virtual Image formed by Concave Lens.]
In Fig. 14 A B is the object and _a b_ the image. Rays incident from A
and B parallel to the principal axis will emerge as if they came from
the principal focus F; hence, the points _a b_ are determined by the
intersections of the dotted lines in the figure with the secondary
axis, O A, O B. An eye on the other side of the lens sees the image _a
b_, which is always virtual, erect and diminished.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account