The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful arts — John Shaqi
The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful artsBrewster, David
Science
The kaleidoscope : $b its history, theory and construction. With its application to the fine and useful arts
Brewster, David
Kaleidoscopes
Before we proceed to investigate the effects produced by a variation in
the length of the reflecting planes, it will be necessary to consider
the variation of the intensity of the light in different parts of the
reflected sectors. In the direct sector =A O B=, Fig. 2, the intensity
of the light is uniform in every part of its surface; but this is far
from being the case in the images formed by reflexion. In Fig. 17, take
any two points _m_, _o_, and draw the lines _m n_, _o p_, perpendicular
to =A O=, and meeting =β O= in _n_ and _p_. Let =O E=, Fig. 18, be a
section of the reflector =A O= seen edgewise, and let =O _p_=, =O _n_=,
be taken equal to the lines _m n_, _o p_, or the height of the points
_n_, _p_, above the plane of the reflector =A O=. Make =O R= to =R E=
as =O _p_= is to =E _e_= the constant height of the eye above the
reflecting plane, and =O _r_= to =_r_ E= as =O _n_= to =E _e_=, and the
points =R, _r_=, will be the points of incidence of the rays issuing
from _p_ and _n_; for in this case =O R _p_ = E R _e_=, and =O _r n_ =
E _r e_=. Hence it is obvious, that =E R _e_= is less than =E _r e_=,
and that the rays issuing from _p_, by falling more obliquely upon
the reflecting surface, will be more copiously reflected. It follows,
therefore, that the intensity of the light in the reflected sector =A
O β= is not uniform, the lines of equal brightness, or the _isophotal_
lines, as they may be called, being parallel to the reflecting surface
=A O=, and in every sector parallel to the radius, between the given
sector and the reflecting surface by which the sector is formed.
As it is easy from the preceding construction to determine the angles
at which the light from any points _m_, _n_, is reflected, when the
length =O E= of the reflectors, and the position of the eye at =E= is
given, we may calculate the intensity of the light in any point of
the circular field by means of the following table, which shows the
number of rays reflected at various angles of incidence, the number
of incident rays being supposed to be 1000. Part of this table was
computed by Bouguer for plate glass not quicksilvered, by means of a
formula deduced from his experiments. By the aid of the same formula I
have extended the table considerably.
_Table showing the quantity of light reflected at various angles of
incidence from plate glass._
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