The
Widescreen Revolution (1952-1970)
One of a series describing each
of the major wide screen processes of the era
by Rick Mitchell
The basic standards of motion picture photography
and presentation were set 100 years ago and have only been
altered significantly twice: With the introduction of sound
in the late Twenties and of wide screen in the early Fifties.
This series of articles on the latter alteration
gives a chronological overview of notable techniques and processes
introduced during those times, the events and situations within
the industry which precipitated their introduction and the
subsequent loss of popularity of some of them and their effect
on production, post-production and exhibition.
On the evening of September 30, 1952, a first
night audience at the Broadway Theater in New York City was
treated to an event that would have as shattering an effect
on motion pictures as sound had almost 25 years earlier.
The theater itself had been altered; some
side seats removed and a huge curved curtained proscenium installed.
When the film started, if seemed rather unimpressive: Lowell
Thomas seen in an almost Lilliputian size in relation to the
proscenium in the standard 1.37:1 ratio image, giving a lecture
on the history of motion pictures.
But when he said, "Ladies and gentlemen,
this is CINERAMA!" his image faded out and the curtains parted
to the full width of the screen as the famous roller coaster
ride came on. Accompanied by directional stereophonic sound,
everyone in the audience was aghast. At that moment, the shape
of theatrical motion pictures would be changed forever.
WHAT WENT BEFORE
Exactly why W. K. L. Dickson chose the 1.33:1
aspect ratio for the motion picture system he was developing
for Thomas Edison is still a subject of controversy and conjecture.
However, by 1895, when a number of inventors were tinkering
with motion picture projection, the Edison Company had generated
a sufficient library of subjects for its Kinetoscope peepshow
device that these films were used in projection experiments.
Although other film and frame sizes were
experimented with, the 35mm 4 perforation per frame 1.33:1
image became the official standard in 1908.
The original 35mm 4-perf aspect ratio established
by Dickson with a perforation-to-perforation image is 1.33:1.
When the frame dimensions were reduced to allow for the optical
soundtrack, the new dimensions were 1.37:1, though 1.33:1 is
often commonly used to refer to the Academy aperture.
As the production and presentation of motion
pictures developed into a multimillion dollar industry, no
serious thought was given to changing this standard until after
World War I.
Theater chains began erecting huge picture
palaces in major cities around the world. Increasing the seating
capacity of the auditoriums meant increasing the size of the
projected picture. The extent to which this could be done was
limited by the available negative and print stocks, projection
lenses, light sources, as well as the balcony overhang which
might cut off the top of the picture for those in the back
rows of the first floor.
However, despite complaints from exhibitors,
nothing was really done until the adoption of optical sound
tracks in 1927. Recorded along the left side of the film inside
the perforations, it cut the image aspect ratio down to about
1.22:1 which in many theaters projected as unnaturally higher
than square.
Some theaters compensated by cutting new
projector aperture plates which restored the squarer image
even if the head and feet of actors were sometimes cut off.
By the early Thirties, cameramen began compensating
for such projection and it became an official standard in 1934.
In the impetus of the conversion to sound, serious thought
was for the first time given to changing the shape and size
of films, at least those for the first run picture palaces.
William Fox, then trying to take over the
industry (he owned both the Fox Film Corp. and MGM during the
summer of 1929), saw the establishment of a new format for
first runs as a further way of extending his control. Fox
opted for a 70mm system in which his company made four features
and a couple of newsreels. The Big Trail (1930) and
one of the newsreels was restored to 35mm anamorphic in 1985.
Paramount experimented first with a 56mm
system in which it filmed one short and then with a 65mm system
similar to today's except for an optical sound track. Pioneering
producer George K. S poor had a 63mm system in which one feature
was made. The film was distributed by RKO, which licensed the
process.
Warner Bros. claimed to have a 65mm system
in which it filmed three features, however, no technical details
have been found on it. Roland West filmed The Bat Whispers (1931)
in a 65mm system which looks similar to Paramount's, it has
also been restored to 35mm anamorphic. Concurrent 35mm versions
of all these features were made.
MGM borrowed Fox's 70mm Grandeur cameras
to film two features which would be optically reduced to 35mm
but projected on wide screens with wide angle lenses! Nine
of these features are known to have been shown in their wide
film formats in New York, Chicago and Los Angeles.
Although exhibitor resistance, audience indifference
and the Depression doomed this Wide screen Revolution of the
early Thirties, many of the techniques and even some of the
equipment would be revived 25 years later.
CINERAMA
One of the studios briefly involved with
wide film experiments at this time was Paramount, primarily
at its East Coast Studios. It has never been documented whether
or not Fred Waller, a special effects cinematographer at that
studio, was ever involved in these experiments. Waller was
interested in developing a motion picture system which roughly
duplicated the wide view of human vision.
Beginning in 1936, with eleven 16mm cameras,
Waller built a rig he called Vitarama. Each camera recorded
a portion of a 146 degree field of view, and corresponding
projectors presented the results on a deep curved screen, an
idea he got from architect Ralph Walker.
Vitarama was demonstrated at the 1939 New
York World's Fair and during World War II was used by the military
to train aerial gunners, including Joseph W. Schmit, later
of Technicolor and an interviewee for this article.
Exactly when Waller switched to 35mm has
not been documented, but by 1949 he had developed the basics
of what was to become Cinerama. The camera employed three synchronized
movements running at 26 fps. Three 27mm lenses were set at
slightly overlapping horizontal angles to each other and the
frame height was increased to 6 perfs. A common shutter in
front of the lenses insured equal exposure on all three negatives.
Projection was from three booths in positions
corresponding to the photographic setup. With vibrating shutters
at the edge of the overlapping frames to, in theory, improve
the blend into one huge, wide image. The aspect ratio of three
panel Cinerama has been listed as anywhere from 2.59:1 to 2.75:1;
in actual practice it may have varied from theater to theater.
Release printing of the subsequent three
panel films was by Technicolor. Initially on color positive
stock, later three matrix printers were modified to handle
the six perf frame and Dubray-Howell perforations.
A picture this big and wide needed more than
standard monaural sound. Bell Labs had been experimenting with
the recording of three discrete channels of stereophonic sound
on film as well as transmitting and disc recording two channels
of stereophonic sound since 1932. There are other documented
attempts at recording more than one channel of optical sound
on film prior to the
FantaSound used in road show engagements of Fantasia (1940).
With post-war access to the German experiments
with magnetic recording, practical high-fidelity stereo recording
techniques became possible. Hazard Reeves of New York's Reeves
Sound developed a special system for Waller that would run
in interlock with his pictures on a 35mm fullcoat.
Reeves chose five channels across and behind
the screen to allow the sound to flow smoothly across the picture.
A sixth track (later modified to seven) contained surround
information directed to speakers in the auditorium by a cue
track.
Although "how it works" illustrations show
six microphones being used for the production recording of
Cinerama Sound in true stereo, this obviously was not practical
in every situation. Tracks were expanded and panned in dub
sessions.
Waller set up his base of operations on a
converted tennis court in Oyster Bay, Long Island. He invited
various studio heads to demonstrations which they all found
impressive but impractical. There was no way Cinerama could
fit into the average neighborhood movie house.
Subrun booking would be necessary to amortize
the obvious high cost of producing films in such a process.
It took a unique visionary from outside the industry to see
the possibilities of Cinerama--Michael Todd.
During the late Thirties and Forties, Todd
had made a name for himself in theatrical circles for producing
flashy revues and stage shows. While he was strongly devoted
to the legitimate theater, Todd felt a need to also make a
name for himself in Hollywood. In Cinerama, he saw his way
of doing so.
He realized that here was a special and unique
form of film presentation, not something for the local Bijou.
An event to be presented in specially selected theaters around
the world under the same conditions as a legitimate stage show,
which people would come from miles around to see.
Forming a company with Lowell Thomas, through
whom he'd first learned of Cinerama, Todd first had his son
reshoot the highlight of Waller's demo film, a roller coaster
ride. To excite investors they used the new Eastman Color negative
film.
Just as Niagara Falls became the symbol
of the Thirties' wide film experiments, being used in practically
every demo film, the roller coaster came to symbolize the fifties
revolution. Used not only in early CinemaScope and Todd-AO
tests, but even for climactic sequences in two 3-D film, Man
in the Dark (1953) and Gorilla at Large (1954).
Todd then set off for Europe to film a series
of travelogue type vignettes in various countries. Worried
that Todd's work might be too highbrow, Thomas brought in veteran
filmmaker Merian C. Cooper to supervise a sequence to be shot
at Cypress Gardens in Florida and an aerial flyover of the
United States by Paul Mantz.
The results wowed that first night audience
and within days the Broadway Theater was sold out for the
next several months. Cinerama was launched in New York.
Though radio and print communications were
faster than 25 years earlier and in spite of increasing transcontinental
air service, the coasts were still far more isolated than today.
The full impact of Cinerama was not immediately felt in Hollywood.
Those executives who'd seen it still felt
it to be economically impractical. Their interest was excited
by a presentation of a more practical nature in their own backyards.
The premiere of Bwana Devil in 3-D, a process easily
adaptable to existing theaters.
3-D at that time was not a wide screen process
and is really outside the scope of this article except for
the following notes: By the time the studios' first 3-D films
were ready for release, the practice of masking off the 1.33:1
frame to achieve a wider look had been introduced.
The House of Wax was shown in many
situations at 1.66:1 and It Came from Outer Space at
1.85:1. 3-D films begun after April 1953 were composed for
their various studios' recommended aspect ratio. Warner Bros.
filmed spherical 3-D versions of The Command and Ring
of Fear (both 1954); though the 3-D negatives were cut,
these versions were never released. In 1960 20th Century-Fox
released the independently-made September Storm, advertised
as the "CinemaScope 3-D film" (the author was unable to locate
a print of this film to determine if it had been shot with
anamorphic lenses).
In the summer of 1954, as the 3-D boom was
declining, Col. Robert Bernier announced he'd developed a process
in which 3-D pairs would be recorded one above the other within
the full aperture frame. The resultant images having a 2.35:1
aspect ratio similar to unsqueezed CinemaScope with an optical
track.
This technique appeared 11 years later as
Bernier's SpaceVision process and is the basis for one of the
single film 3-D systems used extensively in the Seventies and
Eighties. Flat prints from these negatives are blown up and
squeezed for projection through anamorphic lenses.
The continuation of this article will present
CinemaScope and many of the anamorphic processes following
its public introduction by 20th Century-Fox in 1953.
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