• 제목/요약/키워드: Kolmogorov-smirnov

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일수문량의 RUN-LENGTH 및 RUN-SUM의 SIMULATION (Simulation of Run-Length and Run-Sum of Daily Rainfall and Streamflow)

  • 이순택;지홍기
    • 물과 미래
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    • 제10권1호
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    • pp.79-94
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    • 1977
  • 본 연구는 Run-Length와 Run-Sum에 의한 강우량과 하천유량을 분석하여 그 특성을 구명하고, 이로부터 모의발생 모델(Simulation Model)을 설정하여 검토하는데 목적을 두고 있다. 분석에 있어서는 우리나라의 주요도시(서울, 대구 및 부산)의 일강우량과 주요하천(한강, 낙동강 및 금강)의 일류량 자료들을 사용하였다. 또한 해석에 있어서는 Run-Length와 Run-Sum에 대한 각각의 분포형 분석으로부터 Weibull 분포 및 1-변수지수 분포를 하고 있음을 알았으며, 이로부터 Monte Carlo 기법(Monte Carlo technique)을 기초로 하는 Weibull모델(Weibull model)과 1-변수지수 모델(One-Parameter Exponential Model)에 의해서 Run-Length와 Run-Sum을 모의발생 시켰다. 그 결과 기록치(Historical Data)에 근사한 모의발생 자료(Simulation Data)를 얻었다.

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우리나라의 확률적설량 산정에 관한 연구 (A Study on the Evaluation of Probable Snowfall Depth in Korea)

  • 이재준;정영훈;이상원
    • 한국방재학회 논문집
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    • 제7권2호통권25호
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    • pp.53-63
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    • 2007
  • 국내의 경우 매년 발생하는 홍수에 대해서는 많은 분석과 대비를 하고 있지만, 겨울철 폭설에 대한 연구는 미비한 실정이다. 본 연구에서는 기상청 산하 52개 관측지점의 30년 이상의 최심신적설량 자료를 수집하고 각 지점별 적설량의 최적분포형을 결정하여 확률적설량을 산정하였으며, 지역별 확률적설량의 분포를 파악하기 쉽게 재현기간별 확률적설량도를 작성 제시하였다. 지점별 최심신적설량의 적정분포형으로는 2모수 gamma분포가 우세하였고, 과거 주요폭설기록의 재현기간은 약 500년 내외를 보인 2005년, 재현기간 약 200년 정도를 보인 2004년의 확률적 규모를 볼 때 설하중에 대한 설계기준의 확립이 긴요하다. 우리나라의 확률적설량은 남부지방인 영 호남 지역 보다 중부지방으로 올라 갈수록 증가하고 있으며, 특히 태백산맥과 소백산맥을 경계로 서쪽과 동쪽의 편차가 뚜렷한 차이를 보이고 있다.

LH-모멘트의 적정 차수 결정에 의한 설계홍수량 추정(II) (Estimation of Design Flood by the Determination of Best Fitting Order of LH-Moments(II))

  • 맹승진;이순혁
    • 한국농공학회지
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    • 제45권1호
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    • pp.33-44
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    • 2003
  • This study was conducted to estimate the design flood by the determination of best fitting order for LH-moments of the annual maximum series at fifteen watersheds. Using the LH-moment ratios and Kolmogorov-Smirnov test, the optimal regional probability distribution was identified to be the Generalized Extreme Value (GEV) in the first report of this project. Parameters of GEV distribution and flood flows of return period n years were derived by the methods of L, L1, L2, L3 and L4-moments. Frequency analysis of flood flow data generated by Monte Carlo simulation was performed by the methods of L, L1, L2, L3 and L4-moments using GEV distribution. Relative Root Mean Square Error. (RRMSE), Relative Bias (RBIAS) and Relative Efficiency (RE.) using methods of L, Ll , L2, L3 and L4-moments for GEV distribution were computed and compared with those resulting from Monte Carlo simulation. At almost all of the watersheds, the more the order of LH-moments and the return periods increased, the more RE became, while the less RRMSE and RBIAS became. The Absolute Relative Reduction (ARR) for the design flood was computed. The more the order of LH-moments increased, the less ARR of all applied watershed became It was confirmed that confidence efficiency of estimated design flood was increased as the order of LH-moments increased. Consequently, design floods for the appled watersheds were derived by the methods of L3 and L4-moments among LH-moments in view of high confidence efficiency.

경험모의기법을 이용한 한반도 주변 해역에서의 극치해면 분석 (Extreme Sea Level Analysis in Coastal Waters around Korean Peninsula Using Empirical Simulation Technique)

  • 서경덕;양영철;전기천;이동영
    • 한국해안·해양공학회논문집
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    • 제21권3호
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    • pp.254-265
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    • 2009
  • 해양 및 해안의 구조물 설계 시 극치해면 연구가 필수적이다. 본 논문에서는 한반도 주변의 무역항과 연안항 총 52개 항에서 수치모의 된 폭풍해일 자료를 연최대치 시계열 방법, 부분 시계열 방법, 경험모의기법을 이용하여 빈도분석을 수행한 후 비교하였다. 연최대치 시계열 방법과 부분 시계열 방법에서 매개변수 추정을 위해 최우도법을 사용하였다. 분포는 Generalized Pareto 분포를 사용하였고 적합성은 5% 유의수준으로 $\chi^2$ 및 K-S 검정을 수행하였다. 또한, 경험모의기법에 조석을 추가하여 극치해면을 산정하였으며 정 등(2008)이 제시한 극치 해면과 비슷한 값을 나타내었다.

Survey of the use of statistical methods in Journal of the Korean Association of Oral and Maxillofacial Surgeons

  • Choi, Yong-Geun
    • Journal of the Korean Association of Oral and Maxillofacial Surgeons
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    • 제44권1호
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    • pp.25-28
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    • 2018
  • Objectives: This study aimed to describe recent patterns in the types of statistical test used in original articles that were published in Journal of the Korean Association of Oral and Maxillofacial Surgeons. Materials and Methods: Thirty-six original articles published in the Journal in 2015 and 2016 were ascertained. The type of statistical test was identified by one researcher. Descriptive statistics, such as frequency, rank, and proportion, were calculated. Graphical statistics, such as a histogram, were constructed to reveal the overall utilization pattern of statistical test types. Results: Twenty-two types of statistical test were used. Statistical test type was not reported in four original articles and classified as unclear in 5%. The four most frequently used statistical tests constituted 47% of the total tests and these were the chi-square test, Student's t-test, Fisher's exact test, and Mann-Whitney test in descending order. Regression models, such as the Cox proportional hazard model and multiple logistic regression to adjust for potential confounding variables, were used in only 6% of the studies. Normality tests, including the Kolmogorov-Smirnov test, Levene test, Shapiro-Wilk test, and $Scheff{\acute{e}}^{\prime}s$ test, were used diversely but in only 10% of the studies. Conclusion: A total of 22 statistical tests were identified, with four tests occupying almost half of the results. Adoption of a nonparametric test is recommended when the status of normality is vague. Adjustment for confounding variables should be pursued using a multiple regression model when the number of potential confounding variables is numerous.

한국 연안 퇴적물 내 중금속 원소의 자연적 배경농도 연구 (Natural Background Level Analysis of Heavy Metal Concentration in Korean Coastal Sediments)

  • 임동일;최진용;정회수;최현우;김영옥
    • Ocean and Polar Research
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    • 제29권4호
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    • pp.379-389
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    • 2007
  • This paper presents an attempt to determine natural background levels of heavy metals which could be used for assessing heavy metal contamination. For this study, a large archive dataset of heavy metal concentration (Cu, Cr, Ni, Pb, Zn) for more than 900 surface sediment samples from various Korean coastal environments was newly compiled. These data were normalized for aluminum (grain-size normalizer) concentration to isolate natural factors from anthropogenic ones. The normalization was based on the hypothesis that heavy metal concentrations vary consistently with the concentration of aluminum, unless these metals are of anthropogenic origin. So, the samples (outliers) suspected of receivingany anthropogenic input were removed from regression to ascertain the "background" relationship between the metals and aluminum. Identification of these outliers was tested using a model of predicted limits at 95%. The process of testing for normality (Kolmogorov-Smirnov Test) and selection of outliers was iterated until a normal distribution was achieved. On the basis of the linear regression analysis of the large archive (please check) dataset, background levels, which are applicable to heavy metal assessment of Korean coastal sediments, were successfully developed for Cu, Cr, Ni, Zn. As an example, we tested the applicability of this baseline level for metal pollution assessment of Masan Bay sediments.

Rotational Properties of the Maria Asteroid Family

  • Kim, Myung-Jin;Choi, Young-Jun;Moon, Hong-Kyu;Byun, Yong-Ik;Brosch, Noah;Kaplan, Murat;Kaynar, Suleyman;Uysal, Omer;Guzel, Eda;Behrend, Raoul;Yoon, Joh-Na;Mottola, Stefano;Hellmich, Stephan;Hinse, Tobias C.;Eker, Zeki;Park, Jang-Hyun
    • 천문학회보
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    • 제39권1호
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    • pp.66.2-66.2
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    • 2014
  • We carried out photometric observations of Maria family asteroids during 134 nights spanning from July 2008 to May 2013, and derived synodic rotational periods for 51 objects including obtained periods of 34 asteroids for the first time. In this study, we found that there is a significant excess of fast and slow rotators. The one-sample Kolmogorov-Smirnov test confirms that the spin rate distribution is not consistent with the Maxwellian at a 92% confidence level. From the correlations between rotational period, amplitude of lightcurve, and size, we conclude that rotational properties of Maria family have been changed considerably by the non-gravitational force such as the Yarkovsky and the YORP effect. Using the lightcurve inversion method, we successfully determined the pole orientation for the 13 Maria members, and found the excess of prograde objects versus retrograde with a ratio ($N_p/N_r$) of 3. This implies that retrograde rotators could have been ejected by the 3:1 resonance to the inner Solar System since the generation of Maria family. We estimate that approximately 37 - 75 kilometer-sized Maria asteroids have entered to near-Earth space every 100 Myr.

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In-vitro development of a temporal abutment screw to protect osseointegration in immediate loaded implants

  • Garcia-Roncero, Herminio;Caballe-Serrano, Jordi;Cano-Batalla, Jordi;Cabratosa-Termes, Josep;Figueras-Alvarez, Oscar
    • The Journal of Advanced Prosthodontics
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    • 제7권2호
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    • pp.160-165
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    • 2015
  • PURPOSE. In this study, a temporal abutment fixation screw, designed to fracture in a controlled way upon application of an occlusal force sufficient to produce critical micromotion was developed. The purpose of the screw was to protect the osseointegration of immediate loaded single implants. MATERIALS AND METHODS. Seven different screw prototypes were examined by fixing titanium abutments to 112 Mozo-Grau external hexagon implants (MG Osseous$^{(R)}$; Mozo-Grau, S.A., Valladolid, Spain). Fracture strength was tested at $30^{\circ}$ in two subgroups per screw: one under dynamic loading and the other without prior dynamic loading. Dynamic loading was performed in a single-axis chewing simulator using 150,000 load cycles at 50 N. After normal distribution of obtained data was verified by Kolmogorov-Smirnov test, fracture resistance between samples submitted and not submitted to dynamic loading was compared by the use of Student's t-test. Comparison of fracture resistance among different screw designs was performed by the use of one-way analysis of variance. Confidence interval was set at 95%. RESULTS. Fractures occurred in all screws, allowing easy retrieval. Screw Prototypes 2, 5 and 6 failed during dynamic loading and exhibited statistically significant differences from the other prototypes. CONCLUSION. Prototypes 2, 5 and 6 may offer a useful protective mechanism during occlusal overload in immediate loaded implants.

Effect of different provisional cement remnant cleaning procedures including Er:YAG laser on shear bond strength of ceramics

  • Zortuk, Mustafa;Gumus, Hasan Onder;Kilinc, Halil Ibrahim;Tuncdemir, Ali Riza
    • The Journal of Advanced Prosthodontics
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    • 제4권4호
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    • pp.192-196
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    • 2012
  • PURPOSE. The purpose of this study was to evaluate the effect of provisional cement removal by different dentin cleaning protocols (dental explorer, pumice, cleaning bur, Er:YAG laser) on the shear bond strength between ceramic and dentin. MATERIALS AND METHODS. In total, 36 caries-free unrestored human third molars were selected as tooth specimens. Provisional restorations were fabricated and cemented with eugenol-free provisional cement. Then, disc-shaped ceramic specimens were fabricated and randomly assigned to four groups of dentin cleaning protocols (n = 9). Group 1 (control): Provisional cements were mechanically removed with a dental explorer. Group 2: The dentin surfaces were treated with a cleaning brush with pumice Group 3: The dentin surfaces were treated with a cleaning bur. Group 4: The provisional cements were removed by an Er:YAG laser. Self-adhesive luting cement was used to bond ceramic discs to dentin surfaces. Shear bond strength (SBS) was measured using a universal testing machine at a 0.05 mm/min crosshead speed. The data were analyzed using a Kolmogorov Smirnov, One-way ANOVA and Tukey HSD tests to perform multiple comparisons (${\alpha}$=0.05). RESULTS. The dentin cleaning methods did not significantly affect the SBS of ceramic discs to dentin as follows: dental explorer, pumice, cleaning bur, and Er:YAG laser. CONCLUSION. The use of different cleaning protocols did not affect the SBS between dentin and ceramic surfaces.

Detailed Abundance Analysis for Plant Host Stars

  • 강원석;이상각;김강민
    • 천문학회보
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    • 제36권1호
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    • pp.27.1-27.1
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    • 2011
  • We obtained the spectra of 93 Planet host stars and 73 normal field stars in F, G, K type using BOES at BOAO. We measured the equivalent width of Fe and 25 elements lines using the automatic EW measurement program, TAME(Tools for Automatic Measurement of Equivalent-widths) and estimated the elemental abundances by synth and abfind driver of MOOG code. Since the absence of planets in the normal field stars cannot be "completely" proved, this work focused on the chemical abundances and planet properties of planet host stars, which have the massive planets close to the parent star relatively. We carried out an investigation for the difference of abundances between stars with "Hot Jupiter" and normal field stars with no known planets. We examined the chemical composition of 25 elements, such as C, N, O, S, Na, Mg, Al, Si, K, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Cu, Zn, Sr, Y, Zr, Ba, Ce, Nd, and Eu by EW measurements, and the S abundances were estimated using synthetic spectrum. We have found that [Mg/Fe] and [Al/Fe] for planet host stars have lower limit comparing with those of comparison stars, and [Ca/Fe] of host star with Neptunian planets is relatively lower than the other host stars with massive planets. We have performed the Kolmogorov-Smirnov test, and examined the ratio of planet host stars to all stars for each bin of [X/H]. As a result, we noted that the O, Si, and Ca abfor undances are strongly related with the presence of planets.

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