• Title/Summary/Keyword: Automatic Optical Alignment System

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Robust PCB Image Alignment using SIFT (잡음과 회전에 강인한 SIFT 기반 PCB 영상 정렬 알고리즘 개발)

  • Kim, Jun-Chul;Cui, Xue-Nan;Park, Eun-Soo;Choi, Hyo-Hoon;Kim, Hak-Il
    • Journal of Institute of Control, Robotics and Systems
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    • v.16 no.7
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    • pp.695-702
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    • 2010
  • This paper presents an image alignment algorithm for application of AOI (Automatic Optical Inspection) based on SIFT. Since the correspondences result using SIFT descriptor have many wrong points for aligning, this paper modified and classified those points by five measures called the CCFMR (Cascade Classifier for False Matching Reduction) After reduced the false matching, rotation and translation are estimated by point selection method. Experimental results show that the proposed method has fewer fail matching in comparison to commercial software MIL 8.0, and specially, less than twice with the well-controlled environment’s data sets (such as AOI system). The rotation and translation accuracy is robust than MIL in the noise data sets, but the errors are higher than in a rotation variation data sets although that also meaningful result in the practical system. In addition to, the computational time consumed by the proposed method is four times shorter than that by MIL which increases linearly according to noise.

Development of Automatic Alignment Height and Cross-section Inspection System for Fiber Bragg Grating Embedded Field Assembly Connector (FBG Embedded 현장 조립형 커넥터의 자동 정렬 및 단면 자동 검사 시스템 개발)

  • Lee, Jung-Ho;Park, Chan-Hee;Yoon, Jae-Soon;Lee, Hee-Kwan;Kim, Cheol-Sang;Kim, Jae-Won;Kim, Kyung;Kim, Jae-Jun
    • Journal of the Korean Society of Manufacturing Technology Engineers
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    • v.23 no.1
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    • pp.94-101
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    • 2014
  • Recently, in order to reduce the time required to replace an optical jumper cord, many researchers are using a field-installable connector and applying the ferrule polishing method, ferrule mechanical contact method, or ferrule fusion contact method. However, the process of arranging the length of the optical fiber, i.e., inserting the optical fiber into the ferrule by hand and checking its cross section, takes 60% of the time required for the entire process, which increases the overall cost. Therefore, in order to make this task more cost-effective, we will develop an automated inspection system with automatic cross-sectional arrangement of a field-installable connector. This system will be able to decrease the failure rate from 10% to 2% compared with the conventional method when cutting the optical fiber inserted into the ferrule. It will also improve the productivity by decreasing the test time by 28% compared with the conventional method. Our studies showed that it was possible to reduce the production costs and improve the quality of a field-installable connector, and we expect it to dominate the market.

OPTICAL PROPERTY AND ALIGNMENT OF KAO WIDE FIELD TELESCOPE (NEOPAT-3) (광시야 망원경 3호기 (NEOPAT-3)의 광학계 특성 및 조정)

  • Yuk, In-Soo;Kyeong, Jae-Mann;Yoon, Joh-Na;Yoon, Jae-Hyuck;Yim, Hong-Suh;Moon, Hong-Kyu;Han, Won-Yong;Byun, Yon-Ik;Kang, Yong-Woo;Yu, Sung-Yeol
    • Journal of Astronomy and Space Sciences
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    • v.21 no.4
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    • pp.417-428
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    • 2004
  • We have investigated the optical property of the KAO(Korea Astronomy Observatory) wide field telescope (named NEOPAT-3; Near Earth Object and Satellite Patrol-3) and aligned optical system. The NEOPAT-3 is restricted to V,R,I-filters because of the refractive property of the correcting lens system. Because of the fast focal ratio, the optical performance of the NEOPAT-3 is very sensitive to its alignment factors of the optical system. To make the spot radius smaller than $8{\mu}m$ in rms over 2degree${\times}2$degree field, the optical system must satisfy the following conditions: 1) The tilt error between detector plane and focal plane should be less than 0.05degree. 2) The decenter error between the primary mirror and the correcting lens system should be less than 1mm. 3) The distance error between the primary mirror and the correcting lens system should be less than 2.3mm. In order to align the optical system accurately, we measured the aberrations of the telescope quantitatively by means of curvature sensing technique. NEOPAT-3 is installed temporary on the roof of the TRAO(Taeduk Radio Astronomy Observatory) main building to normalize system performance and to develop automatic observation.