• Title/Summary/Keyword: Optics Design

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The property of WC(Co 0.5%) Ultra precision turning for Glass Lens molding (Glass Lens 성형용 초경합금(Co 0.5%)의 초정밀 절삭특성)

  • Kim, Min-Jae;Lee, Jun-Key;Kim, Tae-Kyoung;Hwang, Yeon;Kim, Hye-Jeong;Kim, Jeong-Ho
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2010.06a
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    • pp.41-41
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    • 2010
  • In this research, to study tungsten carbide alloy(Co 0.5%) ultra precision turning possibility that is used Glass Molding Press(GMP) using conventional (Rake angle $-25^{\circ}$) single crystal diamond bite observed machining surface condition, surface roughness($R_a$), diamond bite cutting edge after tungsten carbide alloy ultra precision turning. Suggested and designed optimum chamfer bite shape to suggest ultra precision optimum bite using Finite Element Analysis(FEM). After machining tungsten carbide alloy ultra precision turning using optimum chamfer bite and comparing with conventional bite machine result and studied optimum chamfer bite design inspection and also tungsten carbide ultra precision turning possibility for high temperature compression glass lens molding.

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Auto detect inspection system for single lens product of mobile phone camera (휴대폰 카메라용 렌즈단품 이물 자동검사장비)

  • Song C.H.;Jung Y.W.;Bae S.S.;Song J.Y.;Kim Y.G.
    • Proceedings of the Korean Society of Precision Engineering Conference
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    • 2005.10a
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    • pp.432-435
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    • 2005
  • The Mega-pixel camera phones become main trends in mobile phone market. The lens modules used in mesa-pixel camera phones need high resolution. One of the main factors of resolution drop is the defects of bare lens. Though there are many advantages in auto-inspection of defects of bare lens, high technical problems take the defect inspections to be done with manual process. In this paper, the type and the source of defects were described and bare lens defect auto-inspection system design was explained. The designed auto-inspection system is composed of illumination optics part, focusing optics part and auto-moving system. With the proposed auto-inspection system, fast and uniform inspection of bare lens can be achieved.

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Fabry-Perot Filter Constructed with Anisotropic Space Layer and Isotropic Mirrors

  • Qi, Hongji;Hou, Yongqiang;Yi, Kui;Shao, Jianda
    • Journal of the Optical Society of Korea
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    • v.17 no.1
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    • pp.33-37
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    • 2013
  • In this study a new design concept of the Fabry-Perot filter, constructed with an anisotropic space layer and a couple of isotropic mirrors, was proposed based on the Maxwell equations and the characteristic matrix method. The single- and double-cavity Fabry-Perot filters were designed, and their optical properties were investigated with a developed software package. In addition, the dependence of the transmittance and phase shift for two orthogonal polarization states on the column angle of the anisotropic space layer and the incidence angle were discussed. We demonstrated that the polarization state of electromagnetic waves and phase shifts can be modulated by exploiting an anisotropic space layer in a polarization F-P filter. Birefringence of the anisotropic space layer provided a sophisticated phase modulation with varied incidence angles over a broad range, resulting in a wide-angle phase shift. This new concept would be useful for designing optical components with isotropic and anisotropic materials.

Optical Design of CubeSat Reflecting Telescope

  • Jin, Ho;Pak, Soojong;Kim, Sanghyuk;Kim, Youngju
    • The Bulletin of The Korean Astronomical Society
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    • v.39 no.2
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    • pp.110.1-110.1
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    • 2014
  • The optics of Space telescope is one of the major parts of space mission used for imaging observation of astronomical targets and the Earth. These kinds of space mission have a bulky and complex opto-mechanics with a long optical tube, but there are attempts have been made to observe a target with a small satellite in many ways. In this paper, we describe an optical design of a reflecting telescope for use in a CubeSat mission. For this design, we adopt the off-axis segmented method of astronomical observation techniques based on the Ritchey-Chr$\acute{e}$tien type telescope. The primary mirror shape is a rectangle with dimensions of $8cm{\times}8cm$, and a secondary mirror has dimensions of $2.4cm{\times}4.1cm$. The focal ratio is 3 which can obtain a $0.3{\times}0.2$ degree diagonal angle in a $1280{\times}800$ CMOS color image sensor with a pixel size of $3{\mu}m{\times}3{\mu}m$. This optical design can capture a ${\sim}4km{\times}{\sim}2.3km$ area of the earth's surface at 700 km altitude operation. Based on this conceptual design, we will keep trying to study more for astronomical observation with Attitude control system.

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General Numerical Calculation Method for Paraxial Zoom Loci of Zoom Lenses with Finite Object Distance by Using Gaussian Bracket Method (가우스 괄호법을 이용한 유한 물점을 갖는 줌 렌즈에 대한 일반적인 수치해석적 근축광선 줌 궤적 추적)

  • Lee, Do-Kyung;Yoo, Nam-Jun;Jo, Jae-Heung;Ryu, Jae-Myung;Kang, Geon-Mo;Lee, Hae-Jin
    • Korean Journal of Optics and Photonics
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    • v.20 no.3
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    • pp.156-165
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    • 2009
  • We theoretically derive the set of general paraxial zoom locus equations for all zoom lens systems with finite object distance, including the infinite object distance case, by using the Gaussian bracket method and matrix representation of paraxial ray tracing. We make the zoom locus program by means of a numerical calculation method according to these equations in Visual Basic Language. Consequently, the solutions of this method can be consistently and flexibly used in all types of zoom lens in the step of initial design about zoom loci. Finally, in order to verify the justification and usefulness of this method, we show that two examples, such as $M_{4a}$ and $M_{4h}$ types of 4 groups, and one example, $M_{5n}$ type of 5 groups, which are very complicated zoom lens systems, can be rapidly and diversely traced through various interpolations by using this program.

Numerical Calculation for Autofocus of Zoom Lenses by Using Gaussian Brackets (가우스 괄호법을 이용한 줌 렌즈의 조출량에 대한 수치해석 계산법)

  • Jo, Jae-Heung;Lee, Do-Kyung;Lee, Sang-On;Ryu, Jae-Myung;Kang, Geon-Mo;Lee, Hae-Jin
    • Korean Journal of Optics and Photonics
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    • v.20 no.3
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    • pp.166-174
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    • 2009
  • When the object distance of a zoom lens with finite object distances is varied, we can fix the image at a fixed image plane by moving only one zoom lens group (autofocus group) without moving all zoom lens groups for the autofocus. We theoretically formulated and numerically calculated the moving distances of the autofocus group by using Gaussian brackets and a paraxial ray tracing method. The solutions of this method can be consistently and flexibly used in the initial design for the moving distance of autofocus group within these zoom loci in all types of zoom lens. Finally, in order to verify the usefulness of this method, we show that the moving distance of an autofocus group can be rapidly and diversely obtained in one example of $M_{5n}$ zoom lens type.

A Study on the Electrical Design of a Multi-Beam Large Antenna for S-band Satellite Payload (S-대역 위성 탑재용 다중 빔 대형 안테나의 전기적 설계 연구)

  • Yun, So-Heyun;Uhm, Man-Suk;Yom, In-Bok
    • The Journal of Korean Institute of Electromagnetic Engineering and Science
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    • v.21 no.11
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    • pp.1240-1247
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    • 2010
  • This paper describes the study on the electrical design of a multi-beam large antenna for a satellite payload. This satellite antenna provides the universal communication and broadcasting services to personal portable terminals over the Korean Peninsula. The structure of the hybrid antenna fed by a feed array is proper to provide multi-beams. The amplitude and phase of each feed element should be optimized for a required beam and they can be obtained by GO (Geometrical Optics) and PO(Physical Optics) method. The number of feed elements are also optimized to meet the specification of EIRP(Effective Isotropically Radiated Power). The optimally designed antenna with the limited reflector size and minimum number of feed elements is shown in this paper.

The Characteristics on Ultra Precision Machining for Infrared Optical Materials (Infrared 광학초자의 초정밀 가공 특성)

  • Yang, Sun-Choel;Huh, Myung-Sang;Kim, Sang-Hyuk;Lee, Gil-Jae;Lee, Sang-Yong;Kook, Myung-Ho;Chang, Ki-Soo;Ryu, Seon-Young;Won, Jong-Ho;Kim, Geon-Hee
    • Journal of the Korean Society for Precision Engineering
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    • v.29 no.3
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    • pp.253-260
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    • 2012
  • In nowadays, the infrared optics is frequently employed to various fields such as military, aerospace, industry and medical. To develop the infrared optics, special glasses which can transmit infrared wave are required. Ge(Germanium), Si(silicon), and fluoride glasses are typically used for material of the infrared optics. Compared with Ge and Si glasses, fluoride glasses have high transmittance in infrared wavelength range. Additionally, UV(ultraviolet) and visible light can be transmitted through fluoride glasses. There characteristics of fluoride glasses makes it possible to evaluate optical performance with generally used visible testing equipment. In this paper, we used design of experiment to find ultra precision machining characteristic of Ge and fluoride glasses and optimized machining process to obtain required form accuracy of PV(Peak to Valley) $0.2\;{\mu}m$.

Optical System Design and Experimental Demonstration of Long-range Reflective-type Precision Displacement Sensors (반사형 장거리 정밀 변위 감지기용 광학계 설계 및 측정)

  • Lim, Jae-In;Kim, Seung-Hwan;Lee, Seoung-Hun;Jeong, Hae-Won;Lee, Min-Hee;Kim, Shung-Whan;Kim, Kyong-Hon
    • Korean Journal of Optics and Photonics
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    • v.22 no.3
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    • pp.151-158
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    • 2011
  • This paper reports design and demonstration of optical systems for reflective-type remote optical displacement sensors. Optical systems for light illumination sources and a position sensitive detector (PSD) for the displacement sensor were developed to sense displacement of bridges and instability of skyscrapers in a distance range from 10 m to 250 m to an accuracy better than a few mm. Performance of the optical systems was verified by composing a displacement sensor and by using it in measurement of displacement of a remote target with proper reflective optics depending on distance. The displacement sensor was composed of two LED light sources, each with collimating optics, and a two-dimensional PSD with telescope-type optics. Its displacement resolutions was measured to be 0.1 mm at a distance of 10 m and less than 3 mm at a distance of 250 m.