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Chapter 2 Principles of Stereoscopic Depth Perception and ...

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2.3. <strong>Stereoscopic</strong> display techniques<br />

Figure 2.7: Display principle <strong>of</strong> Traub’s (1967) autostereoscopic display<br />

using rapid varifocal mirror oscillations.<br />

is the fact that coherent light is required during image recording, which<br />

means that holograms cannot be recorded with natural (incoherent) lighting.<br />

Also, the amount <strong>of</strong> data contained in a hologram is enormous 3 ,<br />

requiring specific data compression techniques. At present, only very<br />

small <strong>and</strong> monochromatic displays are feasible for video-based holography<br />

(Pastoor & Wöpking 1997).<br />

For television viewing, Smith & Dumbreck (1988) deem holography as<br />

unsuitable, not just on grounds <strong>of</strong> technical feasibility, but also from the<br />

point <strong>of</strong> view <strong>of</strong> artistic direction. They argue that exploration <strong>of</strong> a 3-D<br />

scene should be carried out by the director at the time <strong>of</strong> production, <strong>and</strong><br />

not by the individual viewer inspecting a hologram from different angles.<br />

Although it is certainly true that holographic filmmaking would require a<br />

different production grammar from traditional, or even 3-D, filmmaking,<br />

Smith & Dumbreck (1988) seem to overlook an important benefit <strong>of</strong> holography.<br />

Since holograms allow inspection from multiple viewpoints, they<br />

will also allow multiple viewers to enjoy the imagery at the same time, a<br />

feature that is clearly required for any successful 3-D television system, as<br />

will be discussed in the next section.<br />

3 The source rate is estimated to exceed 10 12 bit/sec (Pastoor & Wöpking 1997)<br />

67

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