Category: Featured

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    Photography basics: Shutter angle and shutter speed and motion blur

    http://www.shutterangle.com/2012/cinematic-look-frame-rate-shutter-speed/

     

    https://www.cinema5d.com/global-vs-rolling-shutter/

     

    https://www.wikihow.com/Choose-a-Camera-Shutter-Speed

     

    https://www.provideocoalition.com/shutter-speed-vs-shutter-angle/

     

     

    Shutter is the device that controls the amount of light through a lens. Basically in general it controls the amount of time a film is exposed.

     

    Shutter speed is how long this device is open for, which also defines motion blur… the longer it stays open the blurrier the image captured.

     

    The number refers to the amount of light actually allowed through.

     

    As a reference, shooting at 24fps, at 180 shutter angle or 1/48th of shutter speed (0.0208 exposure time) will produce motion blur which is similar to what we perceive at naked eye

     

    Talked of as in (shutter) angles, for historical reasons, as the original exposure mechanism was controlled through a pie shaped mirror in front of the lens.

     

     

    A shutter of 180 degrees is blocking/allowing light for half circle.  (half blocked, half open). 270 degrees is one quarter pie shaped, which would allow for a higher exposure time (3 quarter pie open, vs one quarter closed) 90 degrees is three quarter pie shaped, which would allow for a lower exposure (one quarter open, three quarters closed)

     

    The shutter angle can be converted back and fort with shutter speed with the following formulas:
    https://www.provideocoalition.com/shutter-speed-vs-shutter-angle/

     

    shutter angle =
    (360 * fps) * (1/shutter speed)
    or
    (360 * fps) / shutter speed

     

    shutter speed =
    (360 * fps) * (1/shutter angle)
    or
    (360 * fps) / shutter angle

     

    For example here is a chart from shutter angle to shutter speed at 24 fps:
    270 = 1/32
    180 = 1/48
    172.8 = 1/50
    144 = 1/60
    90 = 1/96
    72 = 1/120
    45 = 1/198
    22.5 = 1/348
    11 = 1/696
    8.6 = 1/1000

     

    The above is basically the relation between the way a video camera calculates shutter (fractions of a second) and the way a film camera calculates shutter (in degrees).

    Smaller shutter angles show strobing artifacts. As the camera only ever sees at least half of the time (for a typical 180 degree shutter). Due to being obscured by the shutter during that period, it doesn’t capture the scene continuously.

     

    This means that fast moving objects, and especially objects moving across the frame, will exhibit jerky movement. This is called strobing. The defect is also very noticeable during pans.  Smaller shutter angles (shorter exposure) exhibit more pronounced strobing effects.

     

    Larger shutter angles show more motion blur. As the longer exposure captures more motion.

    Note that in 3D you want to first sum the total of the shutter open and shutter close values, than compare that to the shutter angle aperture, ie:

     

    shutter open -0.0625
    shutter close 0.0625
    Total shutter = 0.0625+0.0625 = 0.125
    Shutter angle = 360*0.125 = 45

     

    shutter open -0.125
    shutter close 0.125
    Total shutter = 0.125+0.125 = 0.25
    Shutter angle = 360*0.25 = 90

     

    shutter open -0.25
    shutter close 0.25
    Total shutter = 0.25+0.25 = 0.5
    Shutter angle = 360*0.5 = 180

     

    shutter open -0.375
    shutter close 0.375
    Total shutter = 0.375+0.375 = 0.75
    Shutter angle = 360*0.75 = 270

     

     

    Faster frame rates can resolve both these issues.

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    Black Body color aka the Planckian Locus curve for white point eye perception

    http://en.wikipedia.org/wiki/Black-body_radiation

     

    Black-body radiation is the type of electromagnetic radiation within or surrounding a body in thermodynamic equilibrium with its environment, or emitted by a black body (an opaque and non-reflective body) held at constant, uniform temperature. The radiation has a specific spectrum and intensity that depends only on the temperature of the body.

     

    A black-body at room temperature appears black, as most of the energy it radiates is infra-red and cannot be perceived by the human eye. At higher temperatures, black bodies glow with increasing intensity and colors that range from dull red to blindingly brilliant blue-white as the temperature increases.

    The Black Body Ultraviolet Catastrophe Experiment

     

    In photography, color temperature describes the spectrum of light which is radiated from a “blackbody” with that surface temperature. A blackbody is an object which absorbs all incident light — neither reflecting it nor allowing it to pass through.

     

    The Sun closely approximates a black-body radiator. Another rough analogue of blackbody radiation in our day to day experience might be in heating a metal or stone: these are said to become “red hot” when they attain one temperature, and then “white hot” for even higher temperatures. Similarly, black bodies at different temperatures also have varying color temperatures of “white light.”

     

    Despite its name, light which may appear white does not necessarily contain an even distribution of colors across the visible spectrum.

     

    Although planets and stars are neither in thermal equilibrium with their surroundings nor perfect black bodies, black-body radiation is used as a first approximation for the energy they emit. Black holes are near-perfect black bodies, and it is believed that they emit black-body radiation (called Hawking radiation), with a temperature that depends on the mass of the hole.