• Title/Summary/Keyword: pseudo-radial

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An Efficient Computation Method of Zernike Moments Using Symmetric Properties of the Basis Function (기저 함수의 대칭성을 이용한 저니키 모멘트의 효율적인 계산 방법)

  • 황선규;김회율
    • Journal of KIISE:Software and Applications
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    • v.31 no.5
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    • pp.563-569
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    • 2004
  • A set of Zernike moments has been successfully used for object recognition or content-based image retrieval systems. Real time applications using Zernike moments, however, have been limited due to its complicated definition. Conventional methods to compute Zernike moments fast have focused mainly on the radial components of the moments. In this paper, utilizing symmetric/anti-symmetric properties of Zernike basis functions, we propose a fast and efficient method for Zernike moments. By reducing the number of operations to one quarter of the conventional methods in the proposed method, the computation time to generate Zernike basis functions was reduced to about 20% compared with conventional methods. In addition, the amount of memory required for efficient computation of the moments is also reduced to a quarter. We also showed that the algorithm can be extended to compute the similar classes of rotational moments, such as pseudo-Zernike moments, and ART descriptors in same manner.

Performance Analysis of GPS and QZSS Orbit Determination using Pseudo Ranges and Precise Dynamic Model (의사거리 관측값과 정밀동역학모델을 이용한 GPS와 QZSS 궤도결정 성능 분석)

  • Beomsoo Kim;Jeongrae Kim;Sungchun Bu;Chulsoo Lee
    • Journal of Advanced Navigation Technology
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    • v.26 no.6
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    • pp.404-411
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    • 2022
  • The main function in operating the satellite navigation system is to accurately determine the orbit of the navigation satellite and transmit it as a navigation message. In this study, we developed software to determine the orbit of a navigation satellite by combining an extended Kalman filter and an accurate dynamic model. Global positioning system (GPS) and quasi-zenith satellite system (QZSS) orbit determination was performed using international gnss system (IGS) ground station observations and user range error (URE), a key performance indicator of the navigation system, was calculated by comparison with IGS precise ephemeris. When estimating the clock error mounted on the navigation satellite, the radial orbital error and the clock error have a high inverse correlation, which cancel each other out, and the standard deviations of the URE of GPS and QZSS are small namely 1.99 m and 3.47 m, respectively. Instead of estimating the clock error of the navigation satellite, the orbit was determined by replacing the clock error of the navigation message with a modeled value, and the regional correlation with URE and the effect of the ground station arrangement were analyzed.

THE MULTIPLE PROTO STELLAR SYSTEM L1551 IRS5 AT 5 AU RESOLUTION

  • LIM JEREMY;TAKAKUWA SHIGEHISA
    • Journal of The Korean Astronomical Society
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    • v.38 no.2
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    • pp.237-240
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    • 2005
  • We present images of L1551 IRS5 at angular resolutions as high as ${\~}$30 mas, corresponding to a spatial resolution of ${\~}$5 AU, made at 7 mm with the VLA. Previously known to be a binary protostellar system, we show that L1551 IRS5 is likely a triple protostellar system. The primary and secondary components have a projected separation of ${\~}$46 AU, whereas the tertiary component has a projected separation of ${\~}$11 AU from the primary component. The circumstellar dust disks of the primary and secondary components have dimensions of ${\~}$15 AU, whereas that of the tertiary component has a dimension of ${\~}$10 AU. Their major axes are closely, but not perfectly, aligned with each other, as well as the major axis of the surrounding flattened, rotating, and contracting molecular condensation (pseudodisk). Furthermore, the orbital motion of the primary and secondary components is in the same direction as the rotational motion of this pseudodisk. We suggest that all three protostellar components formed as a result of the fragmentation of the central region of the molecular pseudo disk. The primary and secondary components, but apparently not the tertiary component, each exhibits a bipolar ionized jet that is centered on and which emergers perpendicular to its associated dust disk. Neither jets are resolved along their base, implying that they are driven within a radial distance of ${\~}$2.5 AU from their central protostars. Finally, we show evidence for what may be dusty matter streams feeding the two main protostellar components.

Effect of Discrete Walsh Transform in Metamodel-assisted Genetic Algorithms (이산 월시 변환이 메타모델을 사용한 유전 알고리즘에 미치는 영향)

  • Yu, Dong-Pil;Kim, Yong-Hyuk
    • Journal of the Korea Convergence Society
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    • v.10 no.12
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    • pp.29-34
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    • 2019
  • If it takes much time to calculate the fitness of the solution in genetic algorithms, it is essential to create a metamodel. Much research has been completed to improve the performance of metamodels. In this study, we tried to get a better performance of metamotel using discrete Walsh transform in discrete domain. We transforms the basis of the solution and creates a metamodel using the transformed solution. We experimented with NK-landscape, a representative function of the pseudo-boolean function, and provided empirical evidence on the performance of the proposed model. When we performed the genetic algorithm using the proposed model, we confirmed that the genetic algorithm found a better solution. In particular, our metamodel showed better performance than that using the radial basis function network that modified the similarity function for the discrete domain.

Community Type and Stand Structure of the Korean Pine(Pinus koraiensis) Natural Forest in Seoraksan National Park (설악산 국립공원 잣나무 천연림의 군락유형 및 임분구조)

  • Song, Youn-Hee;Yun, Chung-Weon
    • Korean Journal of Environment and Ecology
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    • v.20 no.1
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    • pp.29-40
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    • 2006
  • This study was conducted to obtain the fundamental data for the ecological management in the Pinus koraiensis natural forest in Seoraksan National Park. The community types of the P. koraiensis forest were divided into Ainsliaea acerifolia group and Rhododendron schlippenbachii group. A. acerifolia group was subdivided into Acer tschonoskii var. rubripes subgroup and Calamagrostis arundinacea subgroup. The importance value of major species showed higher value in the order like Pinus koraienses, Abies nephrolepis, Acer barbinerve, Betula ermani, Acer pseudo-sieboldianum, Sorbus commixta and Quercus mongolica. The value of species diversify ranged from 0.44 to 0.86, and showed stronger competition in the interspecific association than in the intraspecific one. The number of individuals of P. koraiensis below 10 centimeters in the 15 study sites was 35, and it was considered that the population of P. koraiensis could be succeeded to the other species in the present situation because of lower frequency in the low layer though the canopy of tree layer was dominated with P. koraiensis. The radial growth patterns of P. koraiensis individuals were mainly fluctuated for the entire life time, which was considered to be caused by frequent disturbance.

Is there a stellar companion in hybrid star HD 81817?

  • Bang, Tae-Yang;Lee, Byeong-Cheol;Perdelwitz, V.;Jeong, Gwang-Hui;Han, Inwoo;Oh, Hyeong-il;Park, Myeong-Gu
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.2
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    • pp.64.2-64.2
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    • 2019
  • HD 81817 is known as a hybrid star. Hybrid stars have both cool stellar wind properties and UV or even X-ray emission features of highly ionized atoms in their spectra. A white dwarf companion has been suggested as the source of UV or X-ray features. HD 81817 has been observed since 2004 as a part of our radial velocity (RV) survey program to search for exoplanets around K giant stars using the Bohyunsan Observatory Echelle Spectrograph (BOES) at the 1.8 m telescope of Bohyunsan Optical Astronomy Observatory (BOAO) in Korea. We obtained 84 RV measurements between 2004 and 2018 for HD 81817 and found two periodic RV variations. The obtained amplitudes of RV periods are around 200 m/s, which are significantly lower than that expected from a white dwarf companion. Furthermore, our re-analysis of the IUE spectra used by Reimers (1984) shows that the excess in UV emission can easily be explained by a pseudo-continuum of unresolved emission lines originating in the extended chromosphere of the star. We thus conclude that there are no companions of stellar mass to HD 81817. Meanwhile, we analyzed two periodicities in RV measurements and conclude that the period of 627.9 days is caused by intrinsic stellar activities based on H alpha equivalent width (EW) variations of a similar period. On the other hand, the period of 1047.8 days is likely to be caused by substellar companion which has a minimum mass of 27.6 MJUP, a semi-major axis of 3.3 AU, and an eccentricity of 0.17 assuming the stellar mass of 4.3 M for HD 81817. The inferred mass puts HD 81817 b in the brown dwarf desert.

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Ecological Examinations of the Radial Growth of Pine Trees (Pinus densiflora S. et Z.) on Mt. Namsan and the Potential Effects of Current Level of Air Pollutants to the Growth of the Trees in Central Seoul, Korea.

  • Kim, Eun-Shik
    • Journal of Korean Society for Atmospheric Environment
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    • v.10 no.E
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    • pp.371-386
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    • 1994
  • Ecological examinations of the radial growth Patterns of pine trees(Pinus densiflora Sieb. et Zucc) growing on Mt. Namsan in central Seoul were made to test a Proposition that the pine trees decline due to the influence of air pollution and acid rain, which was proposed by some researchers in Korea, and the potential effects of current level of air pollutants to the growth of the Pine trees in central Seoul have been speculated. Tree-rings of 40 trees sampled at 3 sites of Mt. Namsan were prepared and examined using a Computer-aided Tree-Ring Measuring System at Kookmin University, Korea. Air Pollutant data collected by the Ministry of Environment( MOE ) and the Forestry Research Institute(FRI) were used to infer the general conditions of the environment. Correlation analysis was applied to the data set of tree growth and the other environmental factors. General information derived from the close examination of the tree-rings and the data on air pollution, drought and the other biological conditions suggested that the growth of the pine trees was severely affected by the occurrence of drought(climatic variation), the prevalence of the pine leaf gall midges(insects), and the suppression by the black locust trees(Robinia pseudo-acacia L.) (competition among trees). While the current condition of air pollution in Seoul cannot be categorized as good, the concentrations of air pollutants are not so high as to cause acute damages to the trees. In addition, while the data of rain acidity showed episodic low PHs of under 4.0, the average of them is far less acidic than those which were observed in either northeastern United States or central Europe, where the decline of trees were not solely attributed to any of the air pollutants. Considering the sequential facts that one of the most important environmental factors that affect the growth of trees is weather condition of the forest that the proposition of the decline of the pine trees was made without careful examination of the growth patterns and past growth history of them as well as the complex influences of many other factors including the weather conditions to the growth of trees, and that no objective explanation has been made on the causal relationships between the current condition of air pollution and the growth of the trees, such a proposition should be evaluated as invalid for the explanation of tree growth on Mt. Namsan in central Seoul, Korea. The author evaluates the factors of air pollution (including acid rain) as the predisposing factors, which may have the Potentials to chronically affect the tree growth at the forest ecosystem on Mt. Namsan for a long period of time. Ecosystem ecological studies should be further carried out to carefully explain both the functional and the structural aspects of the ecosystem processes, which include the biogeochemistry and the long-term changes of soil conditions as well as the growth of the other tree species on the mountain.

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