• 제목/요약/키워드: z-order curve

검색결과 23건 처리시간 0.03초

초음파현미경에서 V(z) 곡선을 이용한 세라믹/금속 접합계면의 비파괴평가 (Nondestructive Evaluation of Ceramic/Metal Interface Using the V(z) Curve of Scanning Acoustic Microscope)

  • 박익근;이철구;조동수;김용권
    • Journal of Welding and Joining
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    • 제23권2호
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    • pp.59-65
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    • 2005
  • A leaky surface acoustic wave (LSAW) velocity was measured using a scanning acoustic microscope on the ceramic/metal interface in order to investigate material properties. The inverse Fourier transform (IFFT) of the V(z) curve contains the reflectance function of a liquid-specimen interface. So, the longitudinal, transverse, and Rayleigh wave velocities for each layer are obtained by the inversion of the V(z) curve at the same time. This paper contains mainly the experimental procedure for measurements of the LSAW velocity, and the results obtained for the velocity variation of individual layer after the thermal shock. It is shown that this method is useful in measuring the material properties under external stress.

정상인의 교합 만곡 분석에 관한 연구 (A STUDY ON THE ANALYSIS OF OCCLUSAL CURVE OF THE NORMAL SUBJECTS)

  • 최명식;계기성;강동완
    • 대한치과보철학회지
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    • 제28권1호
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    • pp.95-122
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    • 1990
  • This study was done to analyze the occlusal curve as one of the factors to be considered for maintenance of occlusal stability in the orthodontic and prosthodontic treatments. Sixty gnathological casts we.e obtained from 43 subjects with normal occlusion and 17 subjects with some of temporomandibular disorders. The occlusal surfaces of gnathologic casts were duplicated by using a Color kit SK-700 and tile reference points of X, Y coordinates were digitized by using the Summagraphic digitizer and 18AT computer system. The Z coordinates of cusp height were measured by 0.01mm measurable caliper. The mathematical computer program of least square method was used to analyze the occlusal curve arranged by three dimensional coordinates of X, Y, Z. The following results were obtained : 1. The occlusal curve of buccal and lingual cusp tips was fitted to the ellipse, and the occlusal curve of anterior teeth was fitted to a part of the circle in the analysis of conic sections. 2. The radius of Spee's curve showed individual differences, but was average 98.7mm in male subjects and 93.7mm in female subjects. 3. The radius fo Spee's curve according to the half of canine width showed the least coefficient of variation. 4. The radius of Spee's curve was not significantly relative to the lateral occlusal contacts on laterotrusion and the absence or presence of temporomandibular disorders. 5. The radius of Wilson's curve showed individual difference and the size of radius was followed by the order of 1st premolar, 2nd premolar, 2nd molar and 1st molar.

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비정규 공정의 극소 불량률 관리를 위한 Zp 관리도 적용 방안 연구 (On the Application of Zp Control Charts for Very Small Fraction of Nonconforming under Non-normal Process)

  • 김종걸;최성원;김혜미;엄상준
    • 품질경영학회지
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    • 제44권1호
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    • pp.167-180
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    • 2016
  • Purpose: The problem for the traditional control chart is that it is unable to monitor the very small fraction of nonconforming and the underlying distribution is the normal distribution. $Z_p$ control chart is useful where it controls the vert small fraction on nonconforming. In this study, we will design the $Z_p$ control chart in order to use under non-normal process. Methods: $Z_p$ is calculated not by failure rate based on attribute data but using variable data. Control limit for non-normal $Z_p$ control chart is designed based on ${\alpha}$-risk calculated by cumulative distribution function of Burr distribution. ${\beta}$-risk, which is for performance evaluation, obtains in the Burr distribution's cumulative distribution function and control limit. Results: The control limit for non-normal $Z_p$ control chart is designed based on Burr distribution. The sensitivity can be checked through ARL table and OC curve. Conclusion: Non-normal $Z_p$ control chart is able to control not only the very small fraction of nonconforming, but it is also useful when $Z_p$ distribution is non-normal distribution.

z변환을 이용한 시간영역에서의 승차감 평가 (Evaluation of Ride Comfort in Time Domain by Using z-Transform)

  • 김영국;김석원;박찬경;김상수;김기환
    • 한국철도학회논문집
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    • 제14권6호
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    • pp.495-500
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    • 2011
  • 철도차량의 승차감은 승객이 느끼는 감정이므로 물리적인 진동의 크기뿐만 아니라 인간의 감응도(느낌)도 고려하여야 하며, 이러한 진동에 대한 인간의 감응도를 나타낸 것이 주파수 보정곡선이다. 주파수 보정곡선은 라플라스 변환형태의 전달함수이기 때문에 이 전달함수를 직접 사용하여 시간 영역에서의 승차감의 평가가 불가능하다. 이를 해결하기 위해서 본 논문에서는 라플라스 변환형태의 전달함수를 시간 영역에서 사용할 수 있는 전달함수로 변환하는 방법을 제시하고 다양한 예제를 통해 이 방법에 대한 타당성을 입증하였다.

Density-based Outlier Detection in Multi-dimensional Datasets

  • Wang, Xite;Cao, Zhixin;Zhan, Rongjuan;Bai, Mei;Ma, Qian;Li, Guanyu
    • KSII Transactions on Internet and Information Systems (TIIS)
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    • 제16권12호
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    • pp.3815-3835
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    • 2022
  • Density-based outlier detection is one of the hot issues in data mining. A point is determined as outlier on basis of the density of points near them. The existing density-based detection algorithms have high time complexity, in order to reduce the time complexity, a new outlier detection algorithm DODMD (Density-based Outlier Detection in Multidimensional Datasets) is proposed. Firstly, on the basis of ZH-tree, the concept of micro-cluster is introduced. Each leaf node is regarded as a micro-cluster, and the micro-cluster is calculated to achieve the purpose of batch filtering. In order to obtain n sets of approximate outliers quickly, a greedy method is used to calculate the boundary of LOF and mark the minimum value as LOFmin. Secondly, the outliers can filtered out by LOFmin, the real outliers are calculated, and then the result set is updated to make the boundary closer. Finally, the accuracy and efficiency of DODMD algorithm are verified on real dataset and synthetic dataset respectively.

w 변환에 의한 기계-유압식 조속기를 가진 선박용 디젤기관의 속도제어 시스템 설계 (The velocity control system design of marine diesel engine with mechanical-hydraulic governor using w transformation method)

  • 강창남;박진길;정주윤;노영오
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 1997년도 하계학술대회 논문집 B
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    • pp.696-698
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    • 1997
  • The marine diesel engine have been widely applied with a mechanical hydraulic governor to control the ship speed for long time. But it was recently very difficult for the mechanical hydraulic governor to control the speed of engine under the condition of low speed and low load because of jiggling by rough fluctuation of rotating torque and hunting by dead time of diesel engine. In order to analyze the speed control system the transfer function was converted from z to w transformation. The author proposed velocity control system with feedback loop by PID controller in order to stabilize for unstable area. The influence of dead time was discussed by Nichols chart and unit step response curve. It was confirmed through computer simulation that the performance improvement of a mechanical hydraulic governor can be obtained by PID controller.

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정밀도로지도의 대용량 공간데이터 교환을 위한 직렬화 기법 설계 (Serialization Method for large spatial data transmission of High Definition Map)

  • 이은일;김덕호
    • 한국지리정보학회지
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    • 제25권4호
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    • pp.32-48
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    • 2022
  • 공간데이터의 활용 범위와 서비스가 늘어나면서 정밀한 공간데이터를 필요로 하는 기술들이 많아지고 있다. 특히 정밀도로지도는 3차원 공간데이터를 수집, 가공, 처리하는 것이 필수적이며 이를 통해 자율주행 지원이 가능하다. 본 연구에서는 정밀도로지도를 대상으로 대용량의 공간데이터를 효율적으로 저장 및 전송할 수 있는 공간데이터 직렬화 기법을 설계하고 구현하였다. 효율적인 직렬화를 위해 바이너리 형태의 공간데이터 구조를 정의하였으며 Zigzag-Z-order 곡선을 활용하여 정보의 손실 없는 좌표 값 인코딩 기법을 설계하였다. 설계한 공간데이터 직렬화 기법을 정밀도로지도 대상으로 구현 및 적용하여 Protocol buffer, Geobuf와 인코딩 후 데이터 크기, 인코딩/디코딩 속도를 비교하였다. 그 결과 경량화 성능과 인코딩 속도는 모든 유형의 공간데이터에서 설계한 직렬화 방식이 우수한 것을 확인하였다. 하지만 디코딩 속도는 선과 면 유형의 공간데이터에서 다른 직렬화 기법의 성능이 우수하였다. 본 연구를 통해 바이너리 형식의 직렬화 기법으로 공간데이터를 효율적으로 인코딩하여 저장 및 전송할 수 있다는 것을 확인하였다.

ENVIRONMENTAL DEPENDENCE OF TYPE IA SUPERNOVA LUMINOSITIES FROM THE YONSEI SUPERNOVA CATALOG

  • Kim, Young-Lo;Kang, Yijung;Lee, Young-Wook
    • 천문학회지
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    • 제52권5호
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    • pp.181-205
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    • 2019
  • There is evidence that the luminosities of Type Ia supernova (SN Ia) depend on their environments. While the impact of this trend on estimating cosmological parameters is widely acknowledged, the origin of this correlation is still under debate. In order to explore this problem, we first construct the YONSEI (YOnsei Nearby Supernova Evolution Investigation) SN catalog. The catalog consists of 1231 spectroscopically confirmed SNe Ia over a wide redshift range (0.01 < z < 1.37) from various SN surveys and includes light-curve fit data from two independent light-curve fitters, SALT2 and MLCS2k2. For a sample of 674 host galaxies, we use the stellar mass and the star formation rate data in Kim et al. (2018). We find that SNe Ia in low-mass and star-forming host galaxies are $0.062{\pm}0.009mag$ and $0.057{\pm}0.010mag$ fainter than those in high-mass and passive hosts, after light-curve corrections with SALT2 and MLCS2k2, respectively. When only local environments of SNe Ia (e.g., locally star-forming and locally passive) are considered, this luminosity difference increases to $0.081{\pm}0.018mag$ for SALT2 and $0.072{\pm}0.018mag$ for MLCS2k2. Considering the significant difference in the mean stellar population age between the two environments, this result suggests that the luminosity evolution of SNe Ia with redshift is most likely the origin of the environmental dependence.

On the Global and Local Environmental Dependence of Type Ia Supernova Luminosity from the Analysis of SALT2 and MLCS2k2 Light-Curve Fitters

  • Kim, Young-Lo;Lee, Young-Wook
    • 천문학회보
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    • 제44권1호
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    • pp.40.3-40.3
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    • 2019
  • There is growing evidence for the dependence of Type Ia supernova (SN Ia) luminosities on the environments. The origin of this correlation, however, is under debate. In order to explore the physical origin of the trend in detail, we analyze SN Ia light-curves by combining a sample of 1231 SNe Ia over a wide redshift range (0.01 < z < 1.37) in various SN surveys and employing two independent light-curve fitters of SALT2 and MLCS2k2. Although SALT2 is the most widely used fitter in the SN community, MLCS2k2 has a novelty in the context of an investigation of the luminosity evolution of SNe Ia. For this reason we use both fitters and analyze them separately. We also determine a stellar mass and a star formation rate (SFR) for a sample of ~600 host galaxies. In addition, because recent low-redshift studies suggest that this dependence manifests itself most strongly when using the local SFR at the SN location, we introduce a new method to infer the local environments by restricting the SN Ia sample in globally star-forming host galaxies to a low-mass host galaxy subset (${\leq}10^{10}M_{\odot}$). We find that SNe Ia in low-mass and star-forming host galaxies are fainter than those in high-mass and passive hosts, after light-curve corrections. Especially, for the first time in host studies, we show that SNe Ia in locally star-forming environments are $0.081{\pm}0.018$ mag fainter ($4.5{\sigma}$) than those in locally passive environments from the sample including SNe at the high-redshift range. Considering the significant difference in the mean stellar population age between these environments, the result would suggest that the origin of the environmental dependence is the luminosity evolution of SNe Ia.

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