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Title: Multimedia 113 Video


1
Multimedia 113Video
2
The Birth of Photography JOSEPH NICEPHORE
NIEPCE (1765-1833) In 1826 Niepce took the very
first photograph using a camera and an 8-hour
exposure
3
LOUIS JACQUES MANDE DAGUERRE (1787-1851) In
1837, Daguerre alone perfected the method of
sensitizing the silver plates with the fumes of
iodine. In 1839, the Paris Observatory
announces his invention to the entire
world. WILLIAM H. FOX TALBOT (1800-1877) Succee
ded in securing images on plain writing paper,
which he sensitized with silver chloride.
4
Paris

Auguste Louis-Jean Lumière First public
screening in 1895?
Talking films are a very interesting invention,
but I do not believe that they will remain very
long in fashion - Louis-Jean Lumière
5
Edison

Thomas Edison develops the first commercially
successful projector, The Vitascope, in late 1896
6
Why do we love films and videos?
  • screenings
  • Edison Actualities (1890-early 1900s)
  • The Great Train Robbery
  • Run Lola Run

7
Filmic Vocabulary
  • What is different between these films?
  • What type of evolution do you see?
  • What about the films structures?
  • What about the films content?
  • What about the films technologies?

8
What are the components of film and video?
  • screenwriting or story structure-- what is the
    idea behind the work
  • mise-en-scene
  • production design
  • cinematography
  • performance
  • editorial
  • sound
  • picture
  • effects
  • delivery mechanism
  • film
  • tape
  • DVD

9
What is a genre?
  • types of films (name one in each category)
  • Action
  • Adventure
  • Comedy
  • Crime
  • Drama
  • Documentary
  • Epics
  • Horror
  • Musicals
  • Science Fiction
  • War
  • Western
  • how do we type films?
  • think about the components we discussed earlier

10
Goals for Class Today
  • Camera operation
  • Getting a proper exposure
  • Film ASA
  • Color Temperature
  • Aperture
  • Shutter Speed
  • Light

11
Color Temperature
  • Color temperature is a term that is borrowed from
    physics. In physics we learn that a so called
    "black body" will radiate light when it is
    heated. The spectrum of this light, and therefore
    its color, depends on the temperature of the
    body. You probably know this effect from everyday
    life if you heat an iron bar, say, it will
    eventually start to glow dark red ("red hot").
    Continue to heat it and it turns yellow (like the
    filament in a light-bulb) and eventually
    blue-white.
  • Be careful with the terminology here! The hotter
    the body gets (measured as the temperature in
    degrees Kelvin) the more the color moves from red
    to wards blue. But we say that red is a "warmer"
    color than blue! So a warm body radiates a cold
    color and a (comparatively) cold body radiates
    warm colors.
  • The photographic color temperature is not the
    same as the color temperature defined in physics
    or colorimetry. As mentioned above, the
    photographic color temperature is measured only
    on the relative intensity of blue to red.
    However, we borrow the basic measurement scale
    from physics and we will measure the photographic
    color temperature in degrees Kelvin (K).

12
Color Temperature
  • daylight balanced film and CCDs (5500 K)
  • tungsten balanced films and CCDs (3200 K).
  • This gives the color of the light balanced to
    white

13
Part Two of Proper ExposureAperture
  • Aperture is measured by f-stops
  • smaller f-numbers (f2, f2.8 etc.) represent wider
    apertures (i.e. more light can pass through the
    lens in a given time) and higher f-numbers (f11,
    f16, f22 etc.) give narrower apertures (meaning
    that less light passes through in a given time).
  • f-stops are calibrated to allow exactly half as
    much light through as the previous setting and
    twice as much light through as the next setting
    (in a given time of course)

14
Aperture Continued
  • For example, a lens set at f8 will allow twice as
    much light through as one set at f11 but only
    half as much as one set as f5.6. It's no
    coincidence that shutter speeds are also
    calibrated to be twice as fast or slow as the
    next or previous setting which allows us to see
    how changing the aperture affects the shutter
    speed required and vice versa.

15
Aperture Continued
  • The technical definition of aperture value, or
    f-stop as it is often known, is the ratio of the
    focal length of the lens to the diameter of the
    lens opening. In other words, it is the number of
    times the diameter of the hole through which the
    light has to pass will fit into the focal length
    of the lens. The size of this hole, known as the
    aperture, may be controlled by turning a collar
    usually located at the base of the lens. On
    automatic cameras, aperture priority mode is
    often denoted by Av which means "Aperture value".
    Typical values may be f2, f2.8, f5.6 and f16
    where the "f" denotes the f-stop, often referred
    to as f-numbers.

16
Part Three of Proper ExposureShutter Speed
  • Shutter speed is a measure of how long the
    shutter remains open when the picture is taken.
  • On manual cameras, it is usually set by means of
    a dial on the top of the camera or, less
    commonly, a ring around the base of the lens.
    Automatic cameras usually denote shutter priority
    mode with the symbol Tv which simply means "Time
    value".
  • Typical shutter speeds are 1/1000s, 1/250s, 1/15s
    and 1s. Note that shutter speeds are calibrated
    to be approximately twice as fast as the previous
    setting and twice as slow as the next setting.
    For example, 1/250s is twice as fast as the
    previous setting 1/125s but is twice as slow as
    the next setting 1/500s.

17
Shutter Speed Continued
  • Shutter speed plays an important role in avoiding
    camera shake which happens when the camera moves
    relative to the subject while the shutter is
    open, causing an overall blur.
  • To avoid this, a good rule of thumb is select a
    shutter speed which is near to, or faster than,
    one divided by the focal length of the lens. For
    example, with a 50mm lens the slowest hand-held
    shutter speed would be 1/60s and with a 300mm
    lens it would be 1/500s.

18
Part Four of Proper ExposureLight
  • This is the most important part of taking great
    pictures and is the most difficult to master
  • Light is measured in footcandles

19
Other Elements of Image MakingFocal Length
  • Focal Length
  • focal length is the angle of view obtained. The
    longer the focal length, the narrower the angle
    of view and the more magnified the image is (at a
    fixed distance). Short focal length lenses are
    known as wide-angle with typical focal lengths of
    20mm, 24mm and 35mm. Standard focal length lenses
    are around the 50mm mark and the range 80mm-300mm
    are considered telephoto lenses. Anything above
    300mm is regarded as super-telephoto.
  • Telephoto lenses tend to compress perspective
    making objects look closer together, while
    wide-angle lenses distort and can make fairly
    close objects seem very distant.

20
Other Elements of Image MakingDepth of Field
  • Depth of field can be thought of as the amount of
    the image which has acceptable sharpness. This
    means that either side of the selected point of
    focus, there is a region in which the image
    remains in focus. Moving outside of this band of
    focus (towards or away from the lens), the image
    becomes progressively more unsharp and out of
    focus.
  • The amount of depth of field is controlled solely
    by magnification and aperture. Since the
    magnification is normally fixed for a given
    subject, the depth of field is usually controlled
    by aperture alone. Wide apertures (such as f2,
    f2.8) give less depth of field while narrow
    apertures (such as f16, f22) give much more depth
    of field.
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