• 제목/요약/키워드: vacuum system design

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IGRINS First Light Instrumental Performance

  • Park, Chan;Yuk, In-Soo;Chun, Moo-Young;Pak, Soojong;Kim, Kang-Min;Pavel, Michael;Lee, Hanshin;Oh, Heeyoung;Jeong, Ueejeong;Sim, Chae Kyung;Lee, Hye-In;Le, Huynh Anh Nguyen;Strubhar, Joseph;Gully-Santiago, Michael;Oh, Jae Sok;Cha, Sang-Mok;Moon, Bongkon;Park, Kwijong;Brooks, Cynthia;Ko, Kyeongyeon;Han, Jeong-Yeol;Nah, Jakyuong;Hill, Peter C.;Lee, Sungho;Barnes, Stuart;Park, Byeong-Gon;T., Daniel
    • 천문학회보
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    • 제39권1호
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    • pp.52.2-52.2
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    • 2014
  • The Immersion Grating Infrared Spectrometer (IGRINS) is an unprecedentedly minimized infrared cross-dispersed echelle spectrograph with a high-resolution and high-sensitivity optical performance. A silicon immersion grating features the instrument for the first time in this field. IGRINS will cover the entire portion of the wavelength range between 1.45 and $2.45{\mu}m$ accessible from the ground in a single exposure with spectral resolution of 40,000. Individual volume phase holographic (VPH) gratings serve as cross-dispersing elements for separate spectrograph arms covering the H and K bands. On the 2.7m Harlan J. Smith telescope at the McDonald Observatory, the slit size is $1^{\prime\prime}{\times}15^{\prime\prime}$. IGRINS has a $0.27^{\prime\prime}$ pixel-1 plate scale on a $2048{\times}2048$ pixel Teledyne Scientific & Imaging HAWAII-2RG detector with SIDECAR ASIC cryogenic controller. The instrument includes four subsystems; a calibration unit, an input relay optics module, a slit-viewing camera, and nearly identical H and K spectrograph modules. The use of a silicon immersion grating and a compact white pupil design allows the spectrograph collimated beam size to be 25mm, which permits the entire cryogenic system to be contained in a moderately sized rectangular vacuum chamber. The fabrication and assembly of the optical and mechanical hardware components were completed in 2013. In this presentation, we describe the major design characteristics of the instrument and the early performance estimated from the first light commissioning at the McDonald Observatory.

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이산화탄소 분리를 위한 순환식 중공사 막흡수기에 관한 모델링 연구 (Modeling Study on a Circulatory Hollow-Fiber Membrane Absorber for $CO_{2}$ Separation)

  • Chun, Myung-Suk;Lee, Kew-Ho
    • 멤브레인
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    • 제5권1호
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    • pp.35-43
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    • 1995
  • 이산화탄소를 포함하는 기체혼합물의 분리를 위해 액체막을 기반으로 하여 관련된 많은 연구가 시도되어 왔다. 폐가스로부터 이산화탄소를 분리하기 위해 본 연구에서는, 흡수제(absorbent)가 흡수(absoption)모듈과 전공조작식 탈착(desorption)모듈간을 계속 순환하는, 보다 개선된 형식의 순환식 중공사 막흡수기(circulatory HFMA)를 새로이 구성하고 분리성능에 관한 기초적인 해석을 하였다. 기-액 물질전달 모델식에 수치해를 적용하여 중공사 막 내부에서의 액상에 대한 농도분포를 정량적으로 예측하였고, 순환하는 흡수제의 유속에 따른 투과플럭스와 선택도의 변화거동을 살펴보았다. $CO_{2}/N_{2}$ 원료혼합기체와 흡수제로서 반응이 없는 순수(pure water)에 대해 계산을 수행하였다. 결과로 흡수제의 유량이 증가함에 따라 투과플럭스는 증가하는 반면에 종전 방식에 비해 졸은 값을 나타낸 선택도의 경우는 점차 감소하였다. 한편 투과플럭스는 진공조작변수인 탈착모듈에서의 기상압력($p_{4}$)에 크게 좌우됨을 보았다. 기존의 평판형 막모듈과의 비교로부터 예상했던 바와 같이 본 연구에서의 중공사 막모듈이 우수한 투과율을 나타냄을 확인할 수 있었다. Circulatory HFMA의 실제 설계를 위한 기초해석이 본 연구가 갖는 의의이다.

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RTP 공정을 통한 태양전지용 AZO 박막의 후열처리 특성연구 (A Study on Properites of PV Solar cell AZO thin films post-annealing by RTP technique)

  • 양현훈;김한울;한창준;소순열;박계춘;이진;정해덕;이석호;백수웅;나길주;정운조
    • 한국신재생에너지학회:학술대회논문집
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    • 한국신재생에너지학회 2011년도 춘계학술대회 초록집
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    • pp.127.1-127.1
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    • 2011
  • In this paper, ZnO:Al thin films with c-axis preferred orientation were prepared on Soda lime glass substrates by RF magnetron sputtering technique. AZO thin film were prepared in order to clarify optimum conditions for growth of the thin film depending upon process, and then by changing a number of deposition conditions and substrate temperature conditions variously, structural and electrical characteristics were measured. For the manufacture of the AZO were vapor-deposited in the named order. It is well-known that post-annealing is an important method to improve crystal quality. For the annealing process, the dislocation nd other defects arise in the material and adsorption/decomposition occurs. The XRD patterns of the AZO films deposited with grey theory prediction design, annealed in a vacuum ambient($2.0{\times}10-3$Torr)at temperatures of 200, 300, 400 and $500^{\circ}C$ for a period of 30min. The diffraction patterns of all the films show the AZO films had a hexagonal wurtzite structure with a preferential orientation along the c-axis perpendicular to the substrate surface. As can be seen, the (002)peak intensities of the AZO films became more intense and sharper when the annealing temperature increased. On the other hand, When the annealing temperature was $500^{\circ}C$ the peak intensity decreased. The surface morphologies and surface toughness of films were examined by atomic force microscopy(AFM, XE-100, PSIA). Electrical resistivity, Gall mobility and carrier concentration were measured by Hall effect measuring system (HL5500PC, Accent optical Technology, USA). The optical absorption spectra of films in the ultraviolet-visibleinfrared( UV-Vis-IR) region were recorder by the UV spectrophotometer(U-3501, Hitachi, Japan). The resistivity, carrier concentration, and Hall mobility of ZnS deposited on glass substrate as a function of post-annealing.

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Low Temperature Thermal Desorption (LTTD) Treatment of Contaminated Soil

  • Alistair Montgomery;Joo, Wan-Ho;Shin, Won-Sik
    • 한국지하수토양환경학회:학술대회논문집
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    • 한국지하수토양환경학회 2002년도 추계학술발표회
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    • pp.44-52
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    • 2002
  • Low temperature thermal desorption (LTTD) has become one of the cornerstone technologies used for the treatment of contaminated soils and sediments in the United States. LTTD technology was first used in the mid-1980s for soil treatment on sites managed under the Comprehensive Environmental Respones, Compensation and Liability Act (CERCLA) or Superfund. Implementation was facilitated by CERCLA regulations that require only that spplicable regulations shall be met thus avoiding the need for protracted and expensive permit applications for thermal treatment equipment. The initial equipment designs used typically came from technology transfer sources. Asphalt manufacturing plants were converted to direct-fired LTTD systems, and conventional calciners were adapted for use as indirect-fired LTTD systems. Other innovative designs included hot sand recycle technology (initially developed for synfuels production from tar sand and oil shale), recycle sweep gas, travelling belts and batch-charged vacuum chambers, among others. These systems were used to treat soil contaminated with total petroleum hydrocarbons (TPH), polycyclic aromatic hydrocarbons (PAHs), pesticides, polychlorinated biphenyls (PCBs) and dioxin with varying degrees of success. Ultimately, performance and cost considerations established the suite of systems that are used for LTTD soil treatment applications today. This paper briefly reviews the develpoment of LTTD systems and summarizes the design, performance and cost characteristics of the equipment in use today. Designs reviewed include continuous feed direct-fired and indirect-fired equipment, batch feed systems and in-situ equipment. Performance is compared in terms of before-and-after contaminant levels in the soil and permissible emissions levels in the stack gas vented to the atmosphere. The review of air emissions standards includes a review of regulations in the U.S. and the European Union (EU). Key cost centers for the mobilization and operation of LTTD equipment are identified and compared for the different types of LTTD systems in use today. A work chart is provided for the selection of the optmum LTTD system for site-specific applications. LTTD technology continues to be a cornerstone technology for soil treatment in the U.S. and elsewhere. Examples of leading-edge LTTD technologies developed in the U.S. that are now being delivered locally in global projects are described.

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STSAT-3 Main Payload, MIRIS Flight Model Developments

  • 한원용;이대희;박영식;정웅섭;이창희;문봉근;박성준;차상목;남욱원;박장현;이덕행;가능현;선광일;양순철;박종오;이승우;이형목
    • 천문학회보
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    • 제35권1호
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    • pp.40.1-40.1
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    • 2010
  • The Main payload of the STSAT-3 (Korea Science & Technology Satellite-3), MIRIS (Multipurpose Infra-Red Imaging System) has been developed for last 3 years by KASI, and its Flight Model (FM) is now being developed as the final stage. All optical lenses and the opto-mechanical components of the FM have been completely fabricated with slight modifications that have been made to some components based on the Engineering Qualification Model (EQM) performances. The components of the telescope have been assembled and the test results show its optical performances are acceptable for required specifications in visual wavelength (@633 nm) at room temperature. The ensuing focal plane integration and focus test will be made soon using the vacuum chamber. The MIRIS mechanical structure of the EQM has been modified to develop FM according to the performance and environment test results. The filter-wheel module in the cryostat was newly designed with Finite Element Analysis (FEM) in order to compensate for the vibration stress in the launching conditions. Surface finishing of all components were also modified to implement the thermal model for the passive cooling technique. The FM electronics design has been completed for final fabrication process. Some minor modifications of the electronics boards were made based on EQM test performances. The ground calibration tests of MIRIS FM will be made with the science grade Teledyne PICNIC IR-array.

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