Reflecting mirror stereoscope invented by Wheatstone
Early 3D movies came out at the end of the nineteenth century. With the emergence of filming, scientists used two cameras to simulate human eyes and projected the film through polarized filters, while the audience watched the movie wearing polarized glasses. Stereoscopic glasses first appeared in the Hollywood movies on May 24, 1953, which marks the beginning of a new era of stereoscopic films. Then, the “stereoscopic TV adopting dual channel polarized imaging technology” and the “complementary color stereoscopic imaging technology” made black & white and color TV three-dimensional, respectively. Currently, the most advanced 3D TV is fractional liquid crystal glasses stereo TV, which can provide vivid stereoscopic color image. When the TV frequency becomes higher, the image is stable without flicker. It is compatible with current color TV system and computer screen, and can easily be transformed to digital TV system.
Ophthalmic operating microscope is also one form of stereovision. As early as in 1590, the Dutch Hans Jansen invented the first compound microscope composed by multiple prisms. OPMI-1 produced by Zeiss corp. in the 1950s was the first operating microscope of modern sense. The current ophthalmic operating microscope integrates illumiation, suspension, multi-optical path, synchronization, built-in inverter, and HD camera in one, which can greatly improve the quality of ophthalmic surgery and expand the scope of surgical indications.
1.2 Stereopsis
Physiological parallax (η) is the distance between the corresponding images on both retinas. The physiological parallax of objects with different distances is not the same, and this disparity then is transmitted to the cerebral cortex center to create the sense of distance. Physiological parallax is the basis of stereopsis.
The physiological parallax of fixation point F is zero, for the points further than F, η < 0, like point A, on the contrary, for the points nearer than F, η > 0, like point B.
The distance of objects is determined by the intersection angle α of the line of sight, the object with larger α is nearer, and the object with smaller α is more far away.
In general, the eye feels most comfortable when D is 25 cm, which is the distance of distinct vision. The eye loses the ability of discerning depth when α is less than 30′, equivalent to the distance of 450 m, which is the observation radius of human stereopsis.
The fovea is responsible for fine stereopsis and could detect the parallax ranging from 2″ to 1200″, suitable for high spatial frequency, static and colored objects. The peripheral retina is responsible for coarse stereopsis and could only detect the parallax ranging from 0.1° to 10°, suitable for low spatial frequency, dynamic and colorless objects. Stereoscopic vision is the resolution of the stereovision, that is, the minimal depth and diameter difference that can be detected. The stereoscopic vision is described in arc seconds.
Object method and picture method have been used to measure stereoscopic vision. Picture method uses a pair of stereo images simulating what both eyes would see. Stereo images can be divided into three types. The first type of stereo image is line stereogram, the individual elements seen by each eye such as edges and lines are matched but with horizontal parallax to make stereovision. The second type of stereo image is random-dot stereogram made by black and white dot matrix, which is disordered lattice seen by one eye and parallax image fused by both eyes. The third type is auto stereogram, a single image stereogram with repeated 2D images. The vergence function of eye will match and fuse similar objects with parallax to create stereoscopic (3D phosphenes).