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Radio Age - 1944, January - 36 Pages, 3.3 MB ... - VacuumTubeEra

Radio Age - 1944, January - 36 Pages, 3.3 MB ... - VacuumTubeEra

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LARGER TELEVISION<br />

IMAGES<br />

RCA Scientists Solve Difficult Optica/ Problems in Projection— Develop<br />

Methods of Moldinii Plastic Lenses for Both Home and Theater Keceiuers.<br />

By I.<br />

G. Maloff<br />

RCA Victor Division,<br />

Camden, N. J.<br />

IMAGE<br />

size in television—for<br />

either the theater or the home<br />

— is no longer a serious problem in<br />

engineering or economics.<br />

It is possible to build, as was<br />

demonstrated experimentally by<br />

RCA just prior to the United<br />

States' entrance into the war, projection-type<br />

television receivers<br />

that reproduce images of any desired<br />

size up to full theater-screen<br />

dimensions.<br />

Not generally known, however, is<br />

the story of how certain features of<br />

one of the great instruments of<br />

astronomy — the Schmidt-Kellner<br />

camera—were adapted to television<br />

projection. The story concerns behind-the-scenes<br />

laboratory work,<br />

calling first for the solution of an<br />

unusually difficult mathematical<br />

problem in optical design, and<br />

finally, for development of a method<br />

to reduce the production cycle of a<br />

new lens from months to minutes.<br />

To those who have seen the allelectronic<br />

system of television in<br />

operation, it is well-known that<br />

images received from a television<br />

transmitter are reproduced on the<br />

broad, nearly-flat end of a tube<br />

called the kinescope. The kinescope<br />

can be built in various sizes, but<br />

when it is given a diameter much<br />

larger than 12 inches the cabinet<br />

in which it and its accompanying<br />

equipment are housed becomes undesirably<br />

bulky for practical home<br />

use.<br />

For this reason, it was apparent<br />

some years ago that if larger television<br />

images were to be available in<br />

homes, a system of optical projection<br />

must be developed. Tests with<br />

standard projection optics produced<br />

screen images that were much too<br />

dim for practical use. Thus, the<br />

situation called for a new approach<br />

—an original conception.<br />

It had been known for a long<br />

time that aspherical* lenses in combination<br />

with either spherical or<br />

aspherical mirrors may be arranged<br />

into<br />

optical systems of high definition<br />

combined with great light<br />

gathering power. Astronomers<br />

were first in making use of this<br />

principle, especially in an arrangement<br />

consisting of one spherical<br />

mirror and one aspherical lens. The<br />

high costs and difficulties in constructing<br />

aspherical lenses retarded<br />

more general utilization of such<br />

svstcms.<br />

Conceives Nen' System<br />

Quite a few years ago. D. O. Landis,<br />

an optician working in the<br />

laboratories of the RCA Manufacturing<br />

Company (now RCA Victor<br />

Division), and having contact with<br />

the needs and aims of men working<br />

on television research, conceived<br />

the idea that an optical system<br />

could be built using aspherical elements<br />

for projection of television<br />

images. He realized, too, that the<br />

shape of the aspherical lens in his<br />

new system would be different from<br />

that of the astronomical lens. This,<br />

he understood, was because the astronomical<br />

camera is focused on<br />

infinity but in his case a short and<br />

finite distance separated the optical<br />

system from the projection screen.<br />

Landis submitted his idea to<br />

E. W. Engstrom, now Research<br />

Director of the RCA Laboratories<br />

* Conventional lens design makes use of<br />

entirely spherical surfaces; in aspherical lens<br />

design, the surface has a variable curvature.<br />

R. LEUSCHNER TESTS AN ASPHERICAL<br />

LENS (ABOVE) FOR DEVIATIONS FROM<br />

THEORETICAL DESIGN; THE AUTHOR RE-<br />

MOVES A PLASTIC ASPHERICAL LENS<br />

(BELOW) FROM THE MOLD IN WHICH<br />

IT WAS MADE.<br />

(then heading the Research Division<br />

of RCA Manufacturing Company<br />

at Camden, New Jersey) and<br />

was encouraged to construct a<br />

working model. It may be mentioned<br />

here that Mr. Engstrom's<br />

action was not in accord with the<br />

more conservative opinions of some<br />

members of his stafi" at the time<br />

Landis commenced his work. The<br />

design of aspherical infinite focus<br />

systems seemed to oflFer little assistance<br />

to the evolution of aspherical<br />

finite focus projection systems.<br />

Landis went ahead struggling<br />

with his system and doing most of<br />

the work in the basement of his<br />

home, where he had a well equipped<br />

optical shop. He was then a well<br />

known figure among amateur astronomers<br />

as well as among amateur<br />

telescope makers. After a few<br />

months of long hours at the grinding<br />

and polishing machines his first<br />

[RADIO AGE 25]

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