• 제목/요약/키워드: vFo

검색결과 128건 처리시간 0.025초

A 12-b Asynchronous SAR Type ADC for Bio Signal Detection

  • Lim, Shin-Il;Kim, Jin Woo;Yoon, Kwang-Sub;Lee, Sangmin
    • JSTS:Journal of Semiconductor Technology and Science
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    • 제13권2호
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    • pp.108-113
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    • 2013
  • This paper describes a low power asynchronous successive approximation register (SAR) type 12b analog-to-digital converter (ADC) for biomedical applications in a 0.35 ${\mu}m$ CMOS technology. The digital-to-analog converter (DAC) uses a capacitive split-arrays consisting of 6-b main array, an attenuation capacitor C and a 5-b sub array for low power consumption and small die area. Moreover, splitting the MSB capacitor into sub-capacitors and an asynchronous SAR reduce power consumption. The measurement results show that the proposed ADC achieved the SNDR of 68.32 dB, the SFDR of 79 dB, and the ENOB (effective number of bits) of 11.05 bits. The measured INL and DNL were 1.9LSB and 1.5LSB, respectively. The power consumption including all the digital circuits is 6.7 ${\mu}W$ at the sampling frequency of 100 KHz under 3.3 V supply voltage and the FoM (figure of merit) is 49 fJ/conversion-step.

MIRIS 환경시험 준비현황 및 시스템 최적화

  • 문봉곤;박영식;이대희;차상목;박성준;이창희;남욱원;정웅섭;표정현;이덕행;이승우;박종오;;한원용
    • 천문학회보
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    • 제36권1호
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    • pp.64.2-64.2
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    • 2011
  • MIRIS (Multi-purpose InfraRed Imaging System), 다목적 적외선 영상시스템은 한국천문연구원에서 개발하고 있는 과학위성 3호의 주 탑재체이다. MIRIS 우주관측카메라는 한국에서 최초로 발사되는 천문우주관측용 적외선 우주망원경이다. 그 유효 구경은 80mm 이고, 탑재되는 검출기는 Teledyne사의 PICNIC $256{\times}256$ Array 이며, 이 검출기를 적용한 관측 화각(FoV)은 $3.67 deg{\times}3.67 deg$, Pixel Scale은 51.6 arcsec/pixel 이다. MIRIS는 현재 비행모델의 납품을 앞두고 우주환경 시험을 준비 및 진행하고 있으며, 시스템의 최적화 작업을 함께 수행하고 있다. 최근에 과학기술위성 3호의 발사체가 러시아 Dnepr로 결정되면서 시험 조건이 변경된 시험 항목에 대해서 EQM의 Sine진동, 충격 시험이 Qualification level로 진행되었다. 그리고 MIRIS 비행모델의 열진공 환경 시험 및 진동시험에 대한 준비 현황을 보고한다. MIRIS 비행 모델의 환경시험은 실제 위성이 겪는 acceptance level로 진행되며, 모든 시험을 통과하면 최종 납품이 이뤄질 예정이다. 또한 시스템의 최적화를 위해 수행했던 조립의 수정 항목들도 함께 보고한다.

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Korean Participation in All-sky Infrared Spectro-Photomeric Survey Mission, SPHEREx

  • Jeong, Woong-Seob;Yang, Yujin;Park, Sung-Joon;Pyo, Jeonghyun;Jo, Youngsoo;Kim, Il-Joong;Ko, Jongwan;Hwang, Hoseong;Song, Yong-Seon
    • 천문학회보
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    • 제44권2호
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    • pp.45.3-45.3
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    • 2019
  • Since the high throughput for diffuse objects and the wide-area survey even with a small telescope can be achieved in space, infrared (IR) obervations have been tried through small missions in Korea. Based upon the previous technical development for infrared spectro-photometric instrument, NISS (Near-infrared Imaging Spectrometer for Star formation history) onboard NEXTSat-1, we participated in the all-sky infrared spectro-photometric survey mission, SPHEREx. The SPEHREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) was selected as the NASA MIDEX (Medium-class Explorer) mission (PI Institute: Caltech) in this February. As an international partner, KASI will take part in the hardware development, the operation and the science for the SPHEREx. The SPHEREx will perform the first all-sky infrared spectro-photometric survey to probe the origin of our Universe, to explore the origin and evolution of galaxies, and to explore whether planets around other stars could harbor life. For the purpose of the all-sky survey, the SPHEREx is designed to have a wide FoV of 3.5 × 11.3 deg. as well as wide spectral range from 0.75 to 5.0㎛. Here, we report the status of the SPHEREx project and the progress in the Korean participation.

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Alkyl 급 Aryl thionocarbamate 류의 합성과 그 구충작용에 관한 연구 (Preparation of Alkyl and Aryl-thionocarbamate and their Anthelmintic action)

  • 국채호
    • 약학회지
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    • 제7권2_3호
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    • pp.58-66
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    • 1963
  • Alkyl-phenylthionocarbamates already have been investigated as anthelmintics. Especially ethyl-phenylthionocarbamate is noted for its anthelmintic action. Author studied methods for synthesizing Alkyl-phenylthionocarbamates, Alkyl-p-phenetyl thionocarbamates, Alkyl-cyclohexylthionocarbamates, 5 kinds for each. For alkyl radical $-CH_{3}$, $-C_{2}H_{5}$, -n-propyl, -isobuthyl, -n-buthyl, being chosen. Compounds VIII, X, XIII, XIV, and XV are new compounds. At the sametime author prepared 4 kinds of Arylthionocarbamates, among which XVII, and XIX being new compounds. (Table I) The anthelmintic action of these thionocarbamates has been examined through kymographic records indicating the action of neuromuscular preparation of Eisenia foetida Savigny in the various concentration fo above compounds: -Trendelenburg method. Santonine as the criterion of the estimation. (Table. II) 1. Compounds I-X could be prepared by method A or method B. method A in sealed tube brought on better yield and purity. 2. Compounds XI-XV couldn't be prepared by method A but by method B. 3. Arylthionocarbamates XVI, XVII, XVIII, and XIX couldn't be prepared by method A or method B but by method C. 4. Analyzed N. contained in all compounds. Analyzed C.H. and N. contained in unknown compounds, VIII, X, XIII, XIV, XV, XVII, and XIX. 5. Examination of anthelmintic action has been done under the advice of Prof. J.S.Oh medical college, Seoul Nat. University. 6. Compounds VI-X showed little action. 7. Compounds XVI-XIX showed almost no action. 8. Compounds XI-XV showed stronger action than compounds I-V, which was reported already as a usable anthelmintics. 9. Compounds XI, XII, XIII and XIV showed strongest actions, stronger than santonine as recorded on kymographion of the Trendelenburg method. Provided that, the toxity of these compounds found mild enough for human system, these compounds will serve as anthelmintics of greater powers than compounds I-V. 10. In Alkylthionocarbamates, R'NH-radical more influence on the anthelmintic action than ester radical(-OR).

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TWO-COLOR VR CCD PHOTOMETRY OF THE INTERMEDIATE POLAR `RXS J062518.2+733433

  • Kim, Yong-Gi;Andronov Ivan L.;Park, Sung-Su;Chinarova Lidia L.;Baklanov Alexey V.;Jeon, Young-Beom
    • Journal of Astronomy and Space Sciences
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    • 제22권3호
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    • pp.197-210
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    • 2005
  • Results of 7 nights of CCD VR photometry of the intermediate polar 1RXS J062518.2+733433 obtained at the Korean 1.8m telescope are reported. The corrected ephemeris for the orbital minimum is BJD (Orb.min) = 2453023.6159(42)+0.1966431(33) (E-1735). The corrected ephemeris for the spin maximum is BJD (spin max) = 2452893 78477 (10)+0.01374116815 (17) (E-15382) (cycle numbering corresponds to that of Staude et al.2003). The variations of the shape of the individual spin variations are highly correlated in V and R. The phase of the spin maximum is found to be dependent on the orbital phase. The corresponding semi-amplitude of sinusoidal variations of phase is $0.11{\pm}0.03.$ This new phenomenon is explained by the changing viewing conditions of the accreting magnetic white dwarf, and should be checked in further observations this star and for other intermediate polars. To avoid influence of this effect on the analysis of the long-term spin period variations, the runs of at least one orbital period are recommended. Results of time series analysis are presented in tables.

AN ANALOGUE OF THE HILTON-MILNER THEOREM FOR WEAK COMPOSITIONS

  • Ku, Cheng Yeaw;Wong, Kok Bin
    • 대한수학회보
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    • 제52권3호
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    • pp.1007-1025
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    • 2015
  • Let $\mathbb{N}_0$ be the set of non-negative integers, and let P(n, l) denote the set of all weak compositions of n with l parts, i.e., $P(n,l)=\{(x_1,x_2,{\cdots},x_l){\in}\mathbb{N}^l_0\;:\;x_1+x_2+{\cdots}+x_l=n\}$. For any element $u=(u_1,u_2,{\cdots},u_l){\in}P(n,l)$, denote its ith-coordinate by u(i), i.e., $u(i)=u_i$. A family $A{\subseteq}P(n,l)$ is said to be t-intersecting if ${\mid}\{i:u(i)=v(i)\}{\mid}{\geq}t$ for all $u,v{\epsilon}A$. A family $A{\subseteq}P(n,l)$ is said to be trivially t-intersecting if there is a t-set T of $[l]=\{1,2,{\cdots},l\}$ and elements $y_s{\in}\mathbb{N}_0(s{\in}T)$ such that $A=\{u{\in}P(n,l):u(j)=yj\;for\;all\;j{\in}T\}$. We prove that given any positive integers l, t with $l{\geq}2t+3$, there exists a constant $n_0(l,t)$ depending only on l and t, such that for all $n{\geq}n_0(l,t)$, if $A{\subseteq}P(n,l)$ is non-trivially t-intersecting, then $${\mid}A{\mid}{\leq}(^{n+l-t-l}_{l-t-1})-(^{n-1}_{l-t-1})+t$$. Moreover, equality holds if and only if there is a t-set T of [l] such that $$A=\bigcup_{s{\in}[l]{\backslash}T}\;A_s{\cup}\{q_i:i{\in}T\}$$, where $$A_s=\{u{\in}P(n,l):u(j)=0\;for\;all\;j{\in}T\;and\;u(s)=0\}$$ and $$q_i{\in}P(n,l)\;with\;q_i(j)=0\;fo\;all\;j{\in}[l]{\backslash}\{i\}\;and\;q_i(i)=n$$.

Single-Pass VDD 심파를 위한 자동화된 심장 박동기 탈분극파 검출 알고리즘의 효용성 (Behavior of an Automatic Pacemaker Sensing Algorithm for Single-Pass VDD Atrial Electrograms)

  • 김정국;이승한;허웅
    • 전기전자학회논문지
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    • 제5권2호
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    • pp.182-189
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    • 2001
  • Single-pass VDD 심장 박동기(pacemaker)는 하나의 리드만 이식하는 수술 과정의 단순함과 하나의 리드만으로 심방 탈분극파를 적절히 검출하여 심방-심실 탈분극의 연속성(A-V sequence)을 이를 수 있다는 이유로 널리 사용되고 있으나, 검출의 신뢰도에 대해서는 여전히 논의의 대상이 되고 있다. 본 논문에서는 논의의 대상이 되고 있는 심방 탈분극파 검출을 개선하기 위하여 자동화된 심장 박동기 심파 검출 알고리즘을 9명의 환자로부터 얻은 Single-pass VDD 심파에 적용하고, 실제 심파 검출과정에서의 동작 특성을 관찰하였다. 자동화된 검출 알고리즘은 최근에 검출된 두 개의 intrinsic 탈분극파 진폭의 평균치를 계산하여 그 평균치의 50%로 검출 문턱치를 매 박동마다 조정하는 매우 단순한 방법으로, 자동화된 검출 알고리즘의 핵심인 문턱 전압 검출치의 자동적 조정만으로도 Single-pass VDD 심방 탈분극파 검출을 개선할 수 있음을 확인하였다.

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단일 이온빔 스퍼터링법을 이용한 AIN 박막의 증착 (Deposition of AIN Thin Films by Single Ion Beam Sputtering)

  • 이재빈;주한용;이용의;김형준
    • 한국세라믹학회지
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    • 제34권2호
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    • pp.209-215
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    • 1997
  • Reactive Single Ion Beam Sputtering 방법을 이용하여 AIN박막을 증착하고 물성을 분석하였다. 반응성 가스로 질소 가스 또는 암모니아 가스를 이용하였다. 증착된 AIN박막의 구조적, 화학적, 광학적 물성을 분석하기 위해 XRD, GAXRD, TEM, SEM, XPS, UV/VIS spectrophotometer, FT-IR등을 이용하였다. XRD, GAXRD분석결과에 의하면 증착된 모든 AIN박막은 비정질이었으나 TEM분석결과에서는 비정질 속에 육방정의 AIN미세결정들이 분포해 있었다. 그리고 FT-IR과 XPS분석을 통하여 Al-N결합을 확인하였으며, 화학양론적인 조성이 됨에 따라 UV-VIS spectrophotometery 분석에서 투광성이 증가하며 광학적 밴드갭은 6.2eV까지 증가함을 확인하였다. 또한 단면과 표면 형상관찰에서는, 반응성 가스로 질소 가스나 암모니아 가스에 관계없이, 결정입계가 전혀 관찰되지 않는 아주 평활한 현상이었으며 굴절율은 1.6~1.7의 값을 갖는다.

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5.8GHz/5.2GHz/2.4GHz 무선 랜 응용을 위한 선형 이득 CMOS LC VCO의 설계 (Design of CMOS LC VCO with Linearized Gain for 5.8GHz/5.2GHz/2.4GHz WLAN Applications)

  • 안태원;문용
    • 대한전자공학회논문지SD
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    • 제42권6호
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    • pp.59-66
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    • 2005
  • 삼중 대역 무선 랜 응용을 위한 CMOS LC VCO를 1.8V 0.18$\mu$m CMOS 공정으로 설계하였다. 저잡음 특성을 얻기 위하여 VCO 코어는 PMOS 트랜지스터로 구성하였으며 인덕터와 캐패시터를 선택적으로 스위칭하는 기법을 적용하여 5.8GHz 대역 (5.725$\~$5.825GHz), 5.2GHz 대역 (5.150$\~$5.325GHz), 그리고 2.4GHz 대역 (2.412$\~$2.484GHz)에서 동작 가능한 것을 확인하였다. 또한 MOS 버랙터(varactor)에 다중 바이어스를 적용하고 최적화하여 캐패시턴스의 선형 특성을 개선함으로써 VCO의 이득을 선형화하고 PLL의 안정도를 크게 개선하였다. VCO 코어의 소모 전류는 2mA, 면적은 $570{\mu}m{\times}600{\mu}m$이며, 3가지 주파수 대역 모두 1MHz 옵셋에서 -110dBc/Hz 이하의 잡음 특성이 가능함을 확인하였다.

An Wideband GaN Low Noise Amplifier in a 3×3 mm2 Quad Flat Non-leaded Package

  • Park, Hyun-Woo;Ham, Sun-Jun;Lai, Ngoc-Duy-Hien;Kim, Nam-Yoon;Kim, Chang-Woo;Yoon, Sang-Woong
    • JSTS:Journal of Semiconductor Technology and Science
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    • 제15권2호
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    • pp.301-306
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    • 2015
  • An ultra-compact and wideband low noise amplifier (LNA) in a quad flat non-leaded (QFN) package is presented. The LNA monolithic microwave integrated circuit (MMIC) is implemented in a $0.25{\mu}m$ GaN IC technology on a Silicon Carbide (SiC) substrate provided by Triquint. A source degeneration inductor and a gate inductor are used to obtain the noise and input matching simultaneously. The resistive feedback and inductor peaking techniques are employed to achieve a wideband characteristic. The LNA chip is mounted in the $3{\times}3-mm^2$ QFN package and measured. The supply voltages for the first and second stages are 14 V and 7 V, respectively, and the total current is 70 mA. The highest gain is 13.5 dB around the mid-band, and -3 dB frequencies are observed at 0.7 and 12 GHz. Input and output return losses ($S_{11}$ and $S_{22}$) of less than -10 dB measure from 1 to 12 GHz; there is an absolute bandwidth of 11 GHz and a fractional bandwidth of 169%. Across the bandwidth, the noise figures (NFs) are between 3 and 5 dB, while the output-referred third-order intercept points (OIP3s) are between 26 and 28 dBm. The overall chip size with all bonding pads is $1.1{\times}0.9mm^2$. To the best of our knowledge, this LNA shows the best figure-of-merit (FoM) compared with other published GaN LNAs with the same gate length.