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
_Ramsden’s eye-piece._--There is another modification of lenses,
known by the name of the _Positive_, or Ramsden’s eye-piece, which is
much used in Transit instruments, and telescopes which are furnished
with micrometers, and which affords equally good vision as the other
eye-piece. In this construction the lenses are plano-convex, and
nearly of the same focus, but are placed at a distance from each other
less than the focal distance of the glass next the eye, so that the
image of the object viewed is beyond both the lenses, when measuring
from the eye. The flat faces of the two lenses are turned into
contrary directions in this eye-piece--one facing the object-glass,
and the other the eye of the observer; and as the image formed at
the focus of the object-glass, lies parallel to the flat face of the
contiguous lens, every part of the field of view is distinct at the
same adjustment, or, as opticians say, there is a _flat field_, which,
without a diaphragm, prevents distortion of the object. This eye-piece
is represented in fig. 74, where AB and CD are two plano-convex
lenses, with their convex sides inwards. They have nearly the same
focal length, and are placed at a distance from each other, equal to
about two thirds of the focal length of either. The focal length of
an equivalent single lens is equal to three fourths the focal length
of either lens, supposing them to have equal focal distances. This
eye-piece is generally applied, when wires of spider’s lines are used
in the common focus; as the piece containing the lenses can be taken
out without disturbing the lines, and is adjustable for distinct
vision; and whatever may be the measure of any object given by the
wire micrometer, at the solar focus, it is not altered by a change of
the magnifying power, when a second eye-piece of this construction is
substituted.
[Illustration: _figure 74._]
[Illustration: _figure 75._]
[Illustration: _figure 76._]
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