• 제목/요약/키워드: Intermediate band

검색결과 134건 처리시간 0.033초

Optical Characteristics of Oxygen-doped ZnTe Thin Films Deposited by Magnetron Sputtering Method

  • Kim, Seon-Pil;Pak, Sang-Woo;Kim, Eun-Kyu
    • 한국진공학회:학술대회논문집
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    • 한국진공학회 2011년도 제41회 하계 정기 학술대회 초록집
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    • pp.253-253
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    • 2011
  • ZnTe semiconductor is very attractive a material for optoelectronic devices in the visible green spectral region because of it has direct bandgap of 2.26 eV. The prototypes of ZnTe light emitting diodes (LEDs) have been reported [1], showing that their green emission peak closely matches the most sensitive region of the human eye. The optoelectronic properties of ZnTe:O film allow to expect a large optical gain in the intermediate emission band, which emission band lies about 0.4-0.6 eV below the conduction band of ZnTe [2]. So, the ZnTe system is useful for the production of high-efficiency multi-junction solar cells [2,3]. In this work, the ZnTe:O thin films were deposited on Al2O3 substrates by using the radio frequency magnetron sputtering system. Three sets of samples were prepared using argon and oxygen as the sputtering gas. The deposition chamber was pre-pumped down to a base pressure of 10-7 Torr before introducing gas. The deposition pressure was fixed at 10-3 Torr throughout this work. During the ZnTe deposition, the substrate temperature was 300 oC. The optical properties were also investigated by using the ultraviolte-visible (UV-Vis) spectrophotometer.

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IF 대역 SAW 필터 설계 및 제작 (A Study on Design and Fabricate of a Intermediate Frequency Band SAW Filter)

  • 유일현;권희두;정양희
    • 한국음향학회지
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    • 제18권1호
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    • pp.10-15
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    • 1999
  • 본 연구는 35° Y-X Quartz 기판에 낮은 형상 요소를 갖는 Code Division Multiple Access(CDMA)방식 기지국용 Intermediate Frequency (IF)단 통과대역 필터를 설계하고 제작하는 방법에 대해 연구하였다. 이 기판 위에 임펄스 모델링을 이용하여 낮은 형상 요소를 갖는 표면 탄성파 필터를 제작하기 위해 입력단에는 Apodization weighted형의 빗살무늬 변환기, 출력단에는 Withdrawal weighted형의 빗살무늬 변환기로 구성하였다. 그리고 입출력 IDT의 개수는 리플의 영향을 최소화하기 위해 Kaiser-Bessel 창함수를 이용하였으며, 각각 2200쌍과 1000쌍으로 하였다. IDT 전극의 폭은 3.6㎛, 간격은 3.5㎛였으며 두께는 파장과의 비를 고려해 6000Å으로 할 때 최적의 결과를 얻을 수 있었으며, 구경은 임피던스 정합을 위해 2mm로 하였다. 제작된 SAW필터는 중심 주파수 115.2MHz, 통과대역 폭은 1.27MHz이상, 형상 요소는 1.3이하, 삽입손실 -l5dB 및 저지대역 -45dB이하인 특성을 얻을 수 있었다.

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QSO Candidates in Leo Triplet Field

  • 신윤경;변용익
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
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    • 한국우주과학회 2003년도 한국우주과학회보 제12권2호
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    • pp.86-86
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    • 2003
  • We present intermediate-band spectral energy distribution (SED) of QSO candidates in Leo Triplet field. Leo Triplet is composed of three galaxies, NGC3623, 3627, and 3628 which appear to interact with each other. Based on X -ray information, Arp et al. (2002) selected QSO candidates and suggested that the known QSOs and these candidates might belong to the triplet system in spite of their apparent high redshift. Our photometry is based on BATC survey data, which consist of hundreds of 15 intermediate-band images. In order to derive SED of high signal to noise ratio for every sources in the field, we have combined images of the same filter and matched the sources in the combined images. QSO candidates were identified based on the shape of derived SED curves. We compare our results with Arp et al. (2002)'s QSO candidates.

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60 GHz 광대역 무선 LAN구현 연구 (Studies of a broadband transceiver for 60 GHz band wireless LAN)

  • 이문교;이지형;설우석;임병옥;김용호;이진구
    • 대한전자공학회:학술대회논문집
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    • 대한전자공학회 2001년도 하계종합학술대회 논문집(1)
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    • pp.417-420
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    • 2001
  • In this paper, a transceiver using waveguide modules for 60 GHz band wireless LAN is implemented and analyzed. The characteristics of millimeter-wave transmitter are 0 dbm output power, 10.5 dB gain and 38 dBc spurious emition. The receiver's are 3.16 dB noise figure, 8.8 dB gain, -86dBm sensitivity. Maximum communication distance is more than loom. Intermediate frequency comply with IEEE 802.11b. The transfer of multimedia files is performed. The transceiver's data rate can vary with intermediate frequency bandwidth and the transceiver is designed more than 200 Mbps.

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Structure of Direct RF Sampling Receivers for GNSS Signals

  • Won, Yu-Jun;Ahn, Woo-Hyun;Lee, MinJoon;Park, Chansik;Seo, Bo-Seok
    • Journal of Positioning, Navigation, and Timing
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    • 제3권3호
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    • pp.91-97
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    • 2014
  • A direct RF sampling method refers to a technique that directly converts a passband signal to an intermediate band or a baseband without using a mixer. This method is less complicated than an existing RF receiver because a mixer is not used. It uses digital processing after sampling, and thus can flexibly process signals in a number of bands using software. In this process, it is important to select an appropriate sampling frequency so that a number of signals can be converted to an intermediate band that is easy to process. In this study, going beyond previously studied direct RF sampling frequency selection methods, conditions that need to be additionally considered during receiver design were examined, and the structure of a direct RF sampling receiver that satisfies these conditions was suggested.

$K_s$-band luminosity evolution of AGB populations based on star clusters in the Large Magellanic Cloud

  • 고유경;이명균
    • 천문학회보
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    • 제37권1호
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    • pp.56.2-56.2
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    • 2012
  • We present a study of the asymptotic giant branch (AGB) contribution to the total Ks band luminosity of star clusters in the Large Magellanic Cloud (LMC) as a function of age. AGB stars, a representative intermediate-age population, are a strong source of NIR to MIR emission so that they are a critical component for understanding the near-to-mid infrared observation of galaxies. Current calibration of IR emission in evolutionary population synthesis (EPS) models for galaxies is mainly based on a small number of LMC star clusters. However, each LMC star cluster with intermediate age contains only a few AGB stars so that it suffers from a stochastic effect. Therefore a large number of them are needed for solid calibration of the EPS models. We study physical properties of a large number of LMC star clusters to estimate the Ks band luminosity fraction of AGB stars in star clusters as a function of age. We discuss the stochastic effect in calibrating models, and the importance of this calibration for studying the evolution of not only nearby galaxies but also of high-z galaxies.

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Dioxygen Binding to the Singly Alkoxo-Bridged Diferrous Complex: Properties of [$Fe^{Ⅱ}_2$(N-Et-HPTB)$Cl_2$]$BPh_4$

  • 김은석;이강봉;Jang, Ho G.
    • Bulletin of the Korean Chemical Society
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    • 제17권12호
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    • pp.1127-1131
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    • 1996
  • [FeⅡ2(N-Et-HPTB)Cl2]BPh4(1), where N-Et-HPTB is the anion of N,N,N',N'-tetrakis(N-ethyl-2-benzimidazolylmethyl)-2-hydroxy-l,3-diaminopropane, has been synthesized to model dioxygen binding to the diferrous centers of proteins. 1 has a singly bridged structure with a μ-alkoxo of N-Et-HPTB and contains two five-coordinate iron(Ⅱ) centers with two chloride ligands as exogenous ligands. 1 exhibits an electronic spectrum with a λmax at 336 nm in acetone. 1 in acetone exhibits no EPR signal at 4 K, indicating diiron(Ⅱ) centers are antiferromagnetically coupled. Exposure of acetone solution of 1 to O2 at -90 ℃ affords an intense blue color intermediate showing a broad band at 586 nm. This absorption maximum of the dioxygen adduct(1/O2) was found in the same region of μ-l,2-peroxo diiron(Ⅲ) intermediates in the related complexes with pendant pyridine or benzimidazole ligand systems. However, this blue intermediate exhibits EPR signals at g = 1.93, 1.76, and 1.59 at 4 K. These g values are characteristic of S = 1/2 system derived from an antiferromagnetically coupled high-spin Fe(Ⅱ)Fe(Ⅲ) units. 1 is the unique example of a (μ-alkoxo)diferrous complex which can bind dioxygen and form a metastable mixed-valence intermediate. At ambient temperature, most of 1/O2 intermediate decays to form a diamagnetic species. It suggests that the dacay reaction of the intermediate might be bimolecular, implying the formation of mixed-valence tetranuclear species in transition state.

An MMIC Broadband Image Rejection Downconverter Using an InGaP/GaAs HBT Process for X-band Application

  • Lee Jei-Young;Lee Young-Ho;Kennedy Gary P.;Kim Nam-Young
    • Journal of electromagnetic engineering and science
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    • 제6권1호
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    • pp.18-23
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    • 2006
  • In this paper, we demonstrate a fully integrated X-band image rejection down converter, which was developed using InGaP/GaAs HBT MMIC technology, consists of two single-balanced mixers, a differential buffer amplifier, a differential YCO, an LO quadratue generator, a three-stage polyphase filter, and a differential intermediate frequency(IF) amplifier. The X-band image rejection downconverter yields an image rejection ratio of over 25 dB, a conversion gain of over 2.5 dB, and an output-referred 1-dB compression power$(P_{1dB,OUT})$ of - 10 dBm. This downconverter achieves broadband image rejection characteristics over a frequency range of 1.1 GHz with a current consumption of 60 mA from a 3-V supply.

1[MHz] 대역의 자계 공명을 이용한 무선 전력 전송 장치에 관한 연구 (A Study on the Wireless Power Transfer System using Magnetic Resonance at the 1[MHz] Frequency Band)

  • 박정흠
    • 조명전기설비학회논문지
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    • 제26권1호
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    • pp.75-81
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    • 2012
  • In this paper, the wireless power transfer system using the magnetic resonance was designed, analyzed by circuit analysis methode and the calculated transfer function was compared with the measured one. The self-resonant coil was made up of the commonly used capacitor which had the lumped capacitance and it enabled the stable magnetic resonance not to be affected by the circumstance. The transmission efficiency of this system was 70[%] at the 15[cm] between the transmission and receiving coil and the measured transfer function was similar to the calculated one, which means the circuit analysis methode is valid in this system. When the intermediate coils were added between the transmission and receiving coil, the transmission efficiency was increased, which produced the increase of transfer distance. In the case of the five intermediate coils adding, the 35[%] transmission efficiency was achived at the 90[cm] distance.

Ka-band 위성방송수신용 저잡음 블록 변환기 구현 (Implementation of Ka-band Low Noise Block Converter For Satellite TVRO)

  • 임진원;김태진;박주남;이영철
    • 한국전자통신학회논문지
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    • 제3권2호
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    • pp.93-100
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    • 2008
  • 본 논문에서는 상업용 MMIC를 이용하여 Ka-대역 위성 텔레비전 방송 수신 전용(TVRO) 저 잡음 하향변환 증폭단을 설계하였다. 저 잡음 블록은 입력단에서 저 잡음 정합시킨 증폭기를 포함한 3단 증폭기, 이미지 제거용 대역통과필터, 주파수 혼합기, 주파수 체배기 및 IF단으로 구성하였다. 저 잡음블럭을 구성하는 모듈에 대한 감쇄와 전력이득에 대한 분석을 통하여 Ka-band LNB의 특성을 만족시키는 소자를 선정하였다. 설계된 저 잡음 블록에 대한 실험 결과 변환이득은 $58{\pm}1dB$, 잡음지수 1.5dB 이하, 위상잡음은 -94.6dBc@10KHz를 나타내었다.

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