• Title/Summary/Keyword: motion parallax

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AN EMPHASIZED HIGHLIGHT MODEL OF METALLIC OBJECT ON CAVE SYSTEM IN CONSIDERATION OF CONTRAST AND PARALLAX

  • Watanabe, Yasuji;Makino, Mitsunori
    • Proceedings of the Korean Society of Broadcast Engineers Conference
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    • 2009.01a
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    • pp.644-648
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    • 2009
  • Accurate rendering of a virtual scene in real time has been one of important issues for virtual reality (VR) technology. Specular reflection of light has been studied a long time, which is always seen on a metallic object and causes occasionally very strong brightness (highlight). Due to restriction of number of gradation of brightness (usually 256), maximum brightness and contrast ratio, the highlight is relatively weakly represented by displays and projectors. In addition, specular reflection will be take influence of binocular parallax and motion parallax, because it is light to reflect in a specific course. Therefore in this paper, an emphasized highlight model of a metallic object on the CAVE system is proposed. Decreasing brightness slightly on neighbor area of highlighted area, the proposed method increases contrast ratio between the highlighted area and neighbor area. Furthermore, using features of CAVE, the proposed method also represents glance (blink). When a metallic object moves, the method alternatively represents images with highlight and without highlight for both eyes. Since the difference of images for both eyes influences binocular parallax and motion parallax, a userfeels glance more realistically.

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Stereoscopic Image Conversion Algorithm using Object Segmentation and Motion Parallax (객체 분할과 운동 시차를 이용한 입체 영상 변환 알고리즘)

  • Jung, Jae-Sung;Cho, Hwa-Hyun;Yoon, Jong-Ho;Choi, Myung-Ryul
    • Proceedings of the IEEK Conference
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    • 2005.11a
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    • pp.1129-1132
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    • 2005
  • In this paper, we proposed real-time stereoscopic image conversion algorithm using object segmentation and motion parallax. The proposed algorithm separates objects using luminance of image, extracts moving object among objects of the image using motion parallax and generates depth map. Parallax process is done based on the depth map. The proposed method has been evaluated using visual test and APD(Absolute Parallx Difference) for comparing the stereoscopic image of the proposed method with that of MTD. The proposed method offers realistic stereoscopic conversion effect regardless of the direction and velocity of the 2-D image.

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Super-multiview windshield display for driving assistance

  • Urano, Yohei;Kashiwada, Shinji;Ando, Hiroshi;Nakamura, Koji;Takaki, Yasuhiro
    • Journal of Information Display
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    • v.12 no.1
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    • pp.43-46
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    • 2011
  • A three-dimensional windshield display (3D-WSD) can present driving information at the same depth as the objects in the outside scene. Herein, a super-multiview 3D-WSD is proposed because the super-multiview display technique provides smooth motion parallax. Motion parallax is the only physiological cue for perceiving the depth of a 3D image displayed at a far distance, which cannot be perceived by vergence and binocular parallax. A prototype system with 36 views was constructed, and the discontinuity of motion parallax and accuracy of depth perception were evaluated.

A Real-Time Stereoscopic Image Conversion Method Using Motion Parallax (운동 시차를 이용한 실시간 입체 영상 변환 방법)

  • Choi, Chul-Ho;Kwon, Byong-Heon;Choi, Myung-Ryul
    • The KIPS Transactions:PartB
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    • v.10B no.4
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    • pp.359-366
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    • 2003
  • We propose a real-time stereoscopic image conversion method that can generate stereoscopic image with different perspective depth using motion parallax from 2-D image and offer realistic 3-D effect regardless of the direction and velocity of the moving object in the 2-D image. The stereoscopic image is generated by computing the motion parallax between adjacent two 2-D images using the proposed method for motion detection, region segmentation and depth map generation. The proposed method is suitable for real-time stereoscopic conversion processing on various image formats. It has been verified the proposed method by comparing between the stereoscopic image of the proposed method and that of MTD.

Development of Mobile-type Full Parallax 3D Display using High-Density Directional Images

  • Tsuboi, Masashi;Takaki, Yasuhiro;Horikoshi, Tsutomu
    • 한국정보디스플레이학회:학술대회논문집
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    • 2007.08b
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    • pp.1729-1732
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    • 2007
  • We introduce a mobile-type 3D display that achieves a full directional motion parallax and the real time interactions between the observer and the 3D image at the same time. These effects can be unique specified to the mobile-type 3D display.

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Universal Stereoscopic Display Using 64 LCD's

  • Takaki, Yasuhiro
    • 한국정보디스플레이학회:학술대회논문집
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    • 2002.08a
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    • pp.289-292
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    • 2002
  • A new technique to construct an auto-stereoscopic display that offers massive horizontal parallax images is proposed Multiple telecetnric imaging systems are arranged in a modified 2D array. The horizontal parallax images displayed by LCD panels are imaged to be superimposed on a 3D screen. All parallax images are displayed in the different horizontal directions because all imaging systems have different horizontal positions. The difference of the vertical display directions due to the imaging system's vertical positions is canceled by a vertical diffuser placed at the 3D screen. Observers can percept 3D images with the binocular disparity, the vergence, and the smooth motion parallax. In addition, the accommodation function may also work because a number of parallax images are displayed with a very small angle interval in the horizontal direction. A prototype 3D display including 64 color LCD panels was constructed.

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FEASIBILITY ON GENERATING STEREO MOSAIC IMAGE

  • Noh, Myoung-Jong;Lee, Sung-Hun;Cho, Woo-Sug
    • Proceedings of the KSRS Conference
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    • 2005.10a
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    • pp.201-204
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    • 2005
  • Recently, the generation of panoramic images and high quality mosaic images from video sequences has been attempted by a variety of investigations. Among a matter of investigation, in this paper, left and right stereo mosaic image generation utilizing airborne-video sequence images is focused upon. The stereo mosaic image is generated by creating left and right mosaic image which is generated by front and rear slit having different viewing angle in consecutive video frame images. The generation of stereo mosaic image proposed in this paper consists of several processes: camera parameter estimation for each video frame image, rectification, slicing, motion parallax elimination and image mosaicking. However it is necessary to check the feasibility on generating stereo mosaic image as explained processes. Therefore, in this paper, we performed the feasibility test on generating stereo mosaic image using video frame images. In doing so, anaglyphic image for stereo mosaic images is generated and tested for feasibility check.

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Real-Time Stereoscopic Image Conversion Using Motion Detection and Region Segmentation (움직임 검출과 영역 분할을 이용한 실시간 입체 영상 변환)

  • Kwon Byong-Heon;Seo Burm-suk
    • Journal of Digital Contents Society
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    • v.6 no.3
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    • pp.157-162
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    • 2005
  • In this paper we propose real-time cocersion methods that can convert into stereoscopic image using depth map that is formed by motion detection extracted from 2-D moving image and region segmentation separated from image. Depth map which represents depth information of image and the proposed absolute parallax image are used as the measure of qualitative evaluation. We have compared depth information, parallax processing, and segmentation between objects with different depth for proposed and conventional method. As a result, we have confirmed the proposed method can offer realistic stereoscopic effect regardless of direction and velocity of moving object for a moving image.

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RIGOROUS "RICH ARGUMENT" IN MICROLENSING PARALLAX

  • Gould, Andrew
    • Journal of The Korean Astronomical Society
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    • v.53 no.5
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    • pp.99-102
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    • 2020
  • I show that when the observables (πE, tE, θE, πs, µs) are well measured up to a discrete degeneracy in the microlensing parallax vector πE, the relative likelihood of the different solutions can be written in closed form Pi = KHiBi, where Hi is the number of stars (potential lenses) having the mass and kinematics of the inferred parameters of solution i and Bi is an additional factor that is formally derived from the Jacobian of the transformation from Galactic to microlensing parameters. Here tE is the Einstein timescale, θE is the angular Einstein radius, and (πs, µs) are the (parallax, proper motion) of the microlensed source. The Jacobian term Bi constitutes an explicit evaluation of the "Rich Argument", i.e., that there is an extra geometric factor disfavoring large-parallax solutions in addition to the reduced frequency of lenses given by Hi. I also discuss how this analytic expression degrades in the presence of finite errors in the measured observables.

ASTROMETRY OF IRAS 22555+6213 WITH VERA: A 3-DIMENSIONAL VIEW OF SOURCES ALONG THE SAME LINE OF SIGHT

  • CHIBUEZE, JAMES O.;SAKANOUE, HIROFUMI;OMODAKA, TOSHIHIRO;HANDA, TOSHIHIRO;NAGAYAMA, TAKUMI;KAMEZAKI, TATSUYA;BURNS, ROSS
    • Publications of The Korean Astronomical Society
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    • v.30 no.2
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    • pp.119-120
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    • 2015
  • We report results of the measurement of the trigonometric parallax of an $H_2O$ maser source in IRAS 22555+6213 with the VLBI Exploration of Radio Astrometry (VERA). The annual parallax was determined to be $0.278{\pm}0.019$ mas, corresponding to a distance of $3.66^{+0.30}_{-0.26}kpc$. Our results confirm that IRAS 22555+6213 is located in the Perseus arm. We computed the peculiar motion of IRAS 22555+6213 to be ($U_{src}$, $V_{src}$, $W_{src}$) = ($0{\pm}1$, $-32{\pm}1$, $9{\pm}1$) $km\;s^{-1}$, where $U_{src}$, $V_{src}$, and $W_{src}$ are directed toward the Galactic center, in the direction of Galactic rotation and toward the Galactic north pole, respectively. IRAS 22555+6213, NGC7538 and Cepheus A lie along the same line of sight, and are within $2^{\circ}$ on the sky. Their parallax distances, with which we derived their absolute position in the Milky Way, show that IRAS 22555+6213 and NGC7538 are associated with the Perseus arm, while Cepheus A is located in the Local arm. We compared the kinematic distances of IRAS 22555+6213 derived with flat and non-flat rotation curve with its parallax distance and found the kinematic distance derived from the non-flat rotation assumption ($-32km\;s^{-1}$ lag) to be consistent with the parallax distance.