The 3-dimensional (3D) imaging is an important area which can be applied to face detection, gesture recognition, and 3D reconstruction. Many techniques have been reported for 3D imaging using various methods such as time of fight (TOF), stereo vision, and structured light. These methods have limitations such as use of light source, multi-camera, or complex camera system. In this paper, we propose the offset pixel aperture (OPA) technique which is implemented on a single chip so that the depth can be obtained without increasing hardware cost and adding extra light sources. 3 types of pixels including red (R), blue (B), and white (W) pixels were used for OPA technique. The aperture is located on the W pixel, which does not have a color filter. Depth performance can be increased with a higher sensitivity because we use white (W) pixels for OPA with red (R) and blue (B) pixels for imaging. The RB pixels produce a defocused image with blur, while W pixels produce a focused image. The focused image is used as a reference image to extract the depth information for 3D imaging. This image can be compared with the defocused image from RB pixels. Therefore, depth information can be extracted by comparing defocused image with focused image using the depth from defocus (DFD) method. Previously, we proposed the pixel aperture (PA) technique based on the depth from defocus (DFD). The OPA technique is expected to enable a higher depth resolution and range compared to the PA technique. The pixels with a right OPA and a left OPA are used to generate stereo image with a single chip. The pixel structure was designed and simulated. Optical performances of various offset pixel aperture structures were evaluated using optical simulation with finite-difference time-domain (FDTD) method.
A 3dimensional (3D) imaging is an important area which can be applied to face detection, gesture recognition, and 3D reconstruction. In this paper, extraction of depth information for 3D imaging using pixel aperture technique is presented. An active pixel sensor (APS) with in-pixel aperture has been developed for this purpose. In the conventional camera systems using a complementary metal-oxide-semiconductor (CMOS) image sensor, an aperture is located behind the camera lens. However, in our proposed camera system, the aperture implemented by metal layer of CMOS process is located on the White (W) pixel which means a pixel without any color filter on top of the pixel. 4 types of pixels including Red (R), Green (G), Blue (B), and White (W) pixels were used for pixel aperture technique. The RGB pixels produce a defocused image with blur, while W pixels produce a focused image. The focused image is used as a reference image to extract the depth information for 3D imaging. This image can be compared with the defocused image from RGB pixels. Therefore, depth information can be extracted by comparing defocused image with focused image using the depth from defocus (DFD) method. Size of the pixel for 4-tr APS is 2.8 μm × 2.8 μm and the pixel structure was designed and simulated based on 0.11 μm CMOS image sensor (CIS) process. Optical performances of the pixel aperture technique were evaluated using optical simulation with finite-difference time-domain (FDTD) method and electrical performances were evaluated using TCAD.
TMA-based obstruction-free off-axis three-mirror systems became popular recently. Although they provide good performance over wide field of view by employing freeform mirrors, the overall dimension and the size of the system are relatively large considering their aperture size and focal length. More compact design is possible in off-axis two-mirror systems combined with field-correcting lens. A linear-astigmatism-free two-mirror system with correcting lens provides a wide field of view in relatively small size. In this paper, design examples of compact wide field two-mirror systems with correcting lens are presented.
A simple closed-form equation for the elimination of linear astigmatism in off-axis three-mirror telescope and imaging
system is presented. Several practical design examples of telescope and auxiliary optics based on the equation are also
presented and compared to the similar designs reported previously.
The basic concept and fundamental result of a recently developed geometric aberration theory for classical off-axis
reflecting telescopes and imaging systems are presented. It is shown that a classical off-axis reflecting telescope can be
designed to have practically axially-symmetric optical property by eliminating the dominant aberration (linear
astigmatism) caused by the asymmetric geometry. A simple closed-form equation for elimination of linear astigmatism
is presented. Also, to show how the developed aberration theory can be applied to current and future telescopes, several
off-axis reflecting telescopes and imaging systems are designed and analyzed.