• Title/Summary/Keyword: good pair

검색결과 227건 처리시간 0.03초

부산지방에서의 오메가위상차의 재현성 (Reappearance of the Phase Difference of Omega at Busan)

  • 안장영
    • 수산해양기술연구
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    • 제18권2호
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    • pp.97-100
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    • 1982
  • 1980년 9월 1일부터 1981년 2월 28일까지와 1981년 9월 20일부터 1982년 2월 28일까지 부산수산대학(350$^{\circ}$ 07'.9N, 129$^{\circ}$ 06'.3E)에서 A-C pair 및 A-E pair의 오메가 전파의 위상차를 연속적으로 관속하여 년별, 월별, 일별의 재현성에 대해 검토하였다. 그 결과, 오메가전파의 이상전파로 인한 전후기의 실측 PPC 간의 차가 큰 10월을 제외하고는 양 pair 모두 같은 주기적인 변동을 하므로 년별의 재현성은 좋았다. 일별의 재현성에 있어서는 표준편차의 변동이 심한 일몰과도기는 재현성이 없었으며 주야간은 양호한 재현성을 나타내었다. 또한, 실측 PPC 간의 차의 월별변화가 컷으므로 양 pair 모두 월별의 재현성은 희박하였다

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Source-Coupled Backgate쌍을 이용한 CMOS 차동입력단의 특성 (Characteistics of a CMOS Differential Input-Stage Using a Source-Coupled Backgate Pair)

  • 강욱;이원형;한우종;김수원
    • 전자공학회논문지A
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    • 제28A권1호
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    • pp.40-45
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    • 1991
  • It is well known that the conventional differential source-coupled pair uses gates as its input terminals. This input pair provids a high open-loop gain, a large CMRR, and a good PSRR. For these reasons, the input pair has been used widely as an input stages of the differential amplifiers, but a narrow linear input range of this structurelimits its application in the area of some analog circuit design. A novel CMOS source-coupled backgate pair is proposed in this paper. The bulk of MOSFET is exploited and input devices are biased to operate in ohmic region. With this topology, the backgate pair of the wide linear input range and variable transconductance can be obtained. This backgate input differential stage is realized with the size of W/L=50/25 MOSFETs. The results show the nonlinear error is less than $\gamma$1% over 10V full-scale range for the bias current of 200$\mu$A with 10V single power-supply.

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A study of a tidally interacting BCD pair, ESO 435-IG20 and ESO 435-IG16

  • Kim, Jinhyub;Sung, Eon-Chang;Chung, Aeree
    • 천문학회보
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    • 제39권1호
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    • pp.44.1-44.1
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    • 2014
  • Blue Compact Dwarf galaxies (BCDs) are systems that recently have experienced the burst of star formation. As one of the causes for active star formation in BCDs, tidal interaction (fly-by or merger) has been suggested. A pair of BCDs, ESO 435-IG20 and ESO 435-IG16 are separated by only ~80 kpc in projection at a similar redshift (at a ~9 Mpc distance), and hence suspected to be a good example of such case. Intergalactic atomic hydrogen gas found in HIPASS survey is also suggestive of this hypothesis. In this study, we probe the HI morphology and kinematics of this BCD pair using ATCA HI data to study detailed interaction history. We investigate various star formation tracers of the pair to study how responsible tidal interaction is for triggering star formation in these galaxies.

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치형수정된 기어쌍의 치합전달오차 모델링 (Modeling of Transmission Error of A Gear Pair with Modified Teeth)

  • 주상훈;노오현;정동현;배명호;박노길
    • 소음진동
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    • 제8권5호
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    • pp.841-848
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    • 1998
  • In the gear manufacturing, tooth modification is usually applied for the prevention of tooth impact during the loading. In contrary, tooth profile error causes amplifying the whine noise which is cumbersome to reduce in the automobile gear box. So optimum quantity of the modifications must be obtained for the good performance in the vibrational sense. In this paper, a formulation to define the tooth curve by considering the profile manufacturing error and loading deformation of the gear tooth is suggested and the transmission error and loading deformation of the gear tooth is suggested and the transmission error with modified tooth in the gear system is evaluated. A pair of gear set is mathematically modelled. The equivalent excitation in the gear vibratonal model is formulated. For the experimental evaluaton on the derived transmission error function, a simple geared system is set up in which the gears are designed to give pre-designed tooth profile modification and manufactured by CNC Wire Cutting Machine. Under slow speed operaton, the transmission error of the gear pair is measured by using two rotational laser vibrometers, compared with the calculated one of which the result shows good agreement.

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경사자장의 선형성 향상을 위한 핵자기공명 영상용 Z-방향 경사자기장 코일 설계 (Design of Z-directional gradient coil to improve gradient linearity for the nuclear magnetic resonace imaging(NMRI))

  • 고락길;이동훈;백승태;김송희;권영길;류강식
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 1998년도 하계학술대회 논문집 A
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    • pp.235-237
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    • 1998
  • Gradient coil offers the spatial informations of sample or patient in Nuclear Magnetic Resonance Imaging(NMRI) and its gradient field linearity over the field of view(FOV) has many influence on the MR imaging. Accurate and good quality MR imaging can be acquired by the high gradient field linearity over the FOV. So it is an important part to design of gradient coil with good linearity in the wide imaging range. Usually, Z-directional gradient field is generated by using the Helmholtz type coil which is consisted of one-pair loop with anti-current path. It gets less about 40% linearity of the diameter spherical volume(DSV). In this study, we calculated optimized geometrical parameters of two-pair loop system to cancel odd terms up to $B_7$ included effectively. we also analyzed and compared the gradient field distribution and linearity of the common Helmholtz coil with them of the two-pair loop system.

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Solvent Effect on $Rb^+$ to $K^+$ Iron Mutation: Monte Carlo Simulation Study

  • 김학성
    • Bulletin of the Korean Chemical Society
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    • 제21권5호
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    • pp.503-509
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    • 2000
  • The solvent effects on the relative free energies of solvation and the difference in partition coefficients (log P) for $Rb^+$ to $K^+$ mutation in several solvents have been investigated using Monte Carlo simulation (MCS) of statistical perturbation theory(SPT). In comparing the relative free energies for interconversion of one ion pair, $Rb^+$ to $K^+$, in $H_2O$(TIP4P) in this study with the relative free energies of the computer simulations and the experimental, we found that the figure in this study with the relative free energies of the computert simulations and the experimental, we found that the figure in this study is $-5.00\pm0.11$ kcal/mol and those of the computer simulations are $-5.40\pm1.9$, -5.5, and -5.4 kcal/mol. The experimental is -5.1 kcal/mol. There is good agreement among various studies, taking into account both methods used to obtain the hydration free energies and standard deviations. There is also good agreement between the calculated structural properties of this study and the simulations, ab initio and the experimental results. We have explained the deviation of the relationship between the free energy difference and the Onsager dielectric function of solvents by the electron pair donor properties of the solvents. For the $Rb^+$ and $K^+$ ion pair, the Onsager dielectric function of solvents (or solvent permittivity), donor number of solvent and the differences in solvation dominate the differences in the relative free energies of solvation and partition coefficients.

A Multi-wavelength Study of a Pair of Interacting BCDs: ESO 435-IG20 and ESO 435-IG16

  • Kim, Jinhyub;Chung, Aeree;Sung, Eon-Chang;Staveley-Smtih, Lister
    • 천문학회보
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    • 제39권2호
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    • pp.49-49
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    • 2014
  • Blue Compact Dwarf galaxies (BCDs) are low-mass galaxies with recently enhanced star formation activity. Since the discovery of old stellar population in the BCDs, a number of hypotheses have been suggested as the origin of the current active star formation. One theory is tidal interactions such as fly-by and merger. In this study we test this hypothesis using a pair of BCDs, ESO 435-IG20 and ESO 435-IG16 that are separate by only ~80 kpc in projection at a similar redshift (at a ~9 Mpc distance). In the HIPASS survey, intergalactic atomic hydrogen envelope has been found to be covering both galaxies, making the pair a good candidate for the case where the star formation has been triggered by tidal interaction. We probe the gas morphology and kinematics of the BCD pair using ATCA HI data in order to find the evidence of tidal interaction. We also estimate star formation rates in the pair based on Ha emission and UV continuum, and compare with other dwarf galaxies to investigate how responsible the tidal interaction is for the enhanced star formation in this case.

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Poisson's Ratio Measurement Using a Pair of PVDF Ultrasonic Transducer

  • Vargas, Enrique;Toral, Sergio;Gonzalez, Vicente
    • 비파괴검사학회지
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    • 제29권6호
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    • pp.519-524
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    • 2009
  • This work presents a simple technique to determine the Poisson's ratio of homogeneous solid material using a pair of low cost PVDF ultrasonic transducers. It is based on transducer's property of generating longitudinal and transversal waves depending on the excitation frequency. Mechanical tests were conducted to validate the proposed method, resulting in a good agreement between ultrasonic and mechanical techniques.