• 제목/요약/키워드: Features in the Vicinity

검색결과 62건 처리시간 0.03초

Simulation of JERS-1 SAR Images with Map Information

  • Sato, Yuko;Sakurai Amano, Takako;Takagi, Mikio;Kobayashi, Shigeki;Fujii, Naoyuki
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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    • pp.207-212
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    • 1998
  • It is not easy to identify a ground control point (GCP) or even locate its vicinity from a SAR image. Although simulated SAR images may be useful to interpret mountain areas, they are not useful in flat areas because they do not show ground coverage or key features such as rivers, lakes and roads. In this study, we developed a method to simulate SAR images integrating geographical features to DEM to facilitate to locate ground control features from SAR images.

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한국산 사미류의 계통분류학적 연구 II. 제주도 (A Systematic Skdy on the Ophiuroidea in Korea II. Cheiu Island)

  • Shin, Sook
    • 한국동물학회지
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    • 제35권3호
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    • pp.350-361
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    • 1992
  • The ophiuroids collected from 13 localities in the vicinity of Cheiu Island during the period from July, 1965 to October, 1991 were observed for the systematic study on the basis of external features. As a result 26 species belonging to 11 families and 2 orders were identified, of which 5 species are neurly reported in Korean fauna and 6ey are as follows: Ophiomyxa austrolis, Ophioccnfho leuispino, Ophiactis dyscrita, Ophiocentws uenicillotus, Ophiorochnella infemolis. The ophiuroids distributed so far in Cheiu Island turned out to be 30 species.

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Gamma-ray emission from millisecond pulsars - an Outergap perspective

  • Cheng, Kwong Sang
    • Journal of Astronomy and Space Sciences
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    • 제30권3호
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    • pp.153-158
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    • 2013
  • In this review paper we explain the following gamma-ray emission features from the millisecond pulsars. (1) Why is the dipolar field of millisecond pulsars so weak but the magnetic pair creation process may still be able to control the size of the outergap? (2) A sub-GeV pulse component could occur in the vicinity of the radio pulse of millisecond pulsars. (3) Orbital modulated gamma-rays should exist in the black widow systems for large viewing angle.

위상 공액 거울에 흡착된 분자의 광학적 성질 (Optical Properties of Admolecules near a Phase -Conjugate Mirror)

  • 김영식
    • 한국진공학회지
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    • 제5권1호
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    • pp.33-38
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    • 1996
  • The induced linewidth, frequency shift and absorption spectrum for a molecular dipole in the vicinity of a phase -conjugate mirror have been investgated within a classical phenomenological model, with particularreference to the technique of optical phase conjugation by a surface. While the shifts and the widths show similar characteristics as those obtained recently by Bochove who considered the problem within the context of four-wave mixing, the results obtained in the present model can be defined uniquely with the possibility of an infinite lifetime for the excited admolecule . Furthermore, the absorption lineshape obtained here some interesting features which depend on both the magnitude and the phase of the complex reflectivity of the mirror.

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Shear Layer and Wave Structure Over Partially Spanning Cavities

  • Das, Rajarshi;Kim, Heuy Dong;Kurian, Job
    • 한국가시화정보학회지
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    • 제11권2호
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    • pp.46-54
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    • 2013
  • Study of the wave structure and shear layer in the vicinity of a wall mounted cavity is done by time averaged colour schlieren and time resolved instantaneous shadowgraph technique in an M=1.7 flowfield. Effect of change of cavity width on flow structure is investigated by using constant length to depth (L/D) ratio cavity models with varying length to width (L/W) ratio of 0.83 to 4. The time averaged shock wave structure was observed to change with change in cavity width. Dependence of the shock angle at the leading edge on the shear layer width is also evident from the images obtained. Unsteadiness in the flow field in terms of shear layer dynamics and quasi steady nature of shock waves was evident from the images obtained during instantaneous shadowgraph experiments. Apart from the leading and trailing edge shocks, several other waves and flow features were observed. These flow features and the associated physical phenomena are discussed in details and presented in the paper.

High Resolution Spectroscopy of Raman Features in Symbiotic Stars and Young Planetary Nebulae Using the BOES

  • Lee, Hee-Won
    • 천문학회보
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    • 제41권1호
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    • pp.59.4-60
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    • 2016
  • One important aspect of the late stage stellar evolution is the mass loss processes, where a significant amount of stellar material will be returned to the interstellar space to be used for stars of the next generation. Raman scattered O VI and He II by atomic hydrogen in symbiotic stars and young planetary nebulae are found to be excellent tools to investigate the mass loss processes and estimate the mass loss rate. These features appear near hydrogen Balmer emission lines due to the huge cross section in the vicinity of Lyman resonance transitions. With the capability of high spectral resolution and broad spectral coverage, BOES is an ideal instrument to perform Raman spectroscopy of these objects. In this talk, a cursory overview of our research activities on Raman spectroscopy of symbiotics and PNe using the BOES is presented.

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ACCRETION FLOW AND DISPARATE PROFILES OF RAMAN SCATTERED O VI λλ 1032, 1038 IN THE SYMBIOTIC STAR V1016 CYGNI

  • Heo, Jeong-Eun;Lee, Hee-Won
    • 천문학회지
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    • 제48권2호
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    • pp.105-112
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    • 2015
  • The symbiotic star V1016 Cygni, a detached binary system consisting of a hot white dwarf and a mass-losing Mira variable, shows very broad emission features at around 6825 Å and 7082 Å, which are Raman scattered O vi λλ 1032, 1038 by atomic hydrogen. In the high resolution spectrum of V1016 Cyg obtained with the Bohyunsan Optical Echelle Spectrograph these broad features exhibit double peak profiles with the red peak stronger than the blue counterpart. However, their profiles differ in such a way that the blue peak of the 7082 feature is relatively weaker than the 6825 counterpart when the two Raman features are normalized to exhibit an equal red peak strength in the Doppler factor space. Assuming that an accretion flow around the white dwarf is responsible for the double peak profiles, we attribute this disparity in the profiles to the local variation of the flux ratio of O vi λλ 1032, 1038 in the accretion flow. A Monte Carlo technique is adopted to provide emissivity maps showing the local emissivity of O vi λ1032 and O vi λ1038 in the vicinity of the white dwarf. We also present a map indicating the differing flux ratios of O vi λλ 1032 and 1038. Our result shows that the flux ratio reaches its maximum of 2 in the emission region responsible for the central trough of the Raman feature and that the flux ratio in the inner red emission region is almost 1. The blue emission region and the outer red emission region exhibit an intermediate ratio around 1.5. We conclude that the disparity in the profiles of the two Raman O vi features strongly implies accretion flow around the white dwarf, which is azimuthally asymmetric.

제주도 지역 거주자의 주거 행태에 관한 연구 (A Study on the Residential Behavior of Cheju Province)

  • 이정림;김봉애
    • 한국주거학회논문집
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    • 제8권3호
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    • pp.81-90
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    • 1997
  • Cheju province exposes a separated residential culture compared to the mainland area. since it has its own unique climate, natural features. Therefore, this study tried to grasp the residential behavior. was based on the questionnaire to Cheju province people, using the approach by statistic verification. This study also focused and aimed on suggesting the basic data about housing plan which is appropriate to the climate. natural features requirement from inhabitants through the comparison and analysis between the mainland area and Cheju province. The results of the study are as follows; Firstly. the diversified applicative study on ‘Ol-rae’. ‘Ma-dang’, ‘Yoo-young’ and so forth that is traditional outside garden of Cheju is imperative, because in urban area people think traffics, vicinity, etc. are more significant, and in rural area people think occupying large outside space is more significant. Secondly. in the study of the degree of satisfaction on the housing, most of the people's was ‘neutral’ and in rural area quite a lot of negative reaction exposed. This is owing to the uniform introduction on residential style of the mainland area. Thirdly, housing plan should be considered family members' housing needs and provincial characteristics, meanwhile most of the people answered positively about the residential value which is considered very significant lately, for instance, security of privacy. appropriate plan for child's room.

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피로 검출을 위한 능동적 얼굴 추적 (Active Facial Tracking for Fatigue Detection)

  • 박호식;정연숙;손동주;나상동;배철수
    • 한국정보통신학회:학술대회논문집
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    • 한국해양정보통신학회 2004년도 춘계종합학술대회
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    • pp.603-607
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    • 2004
  • 본 논문에서는 얼굴 특징을 추출하는 새로운 능동적 방식을 제안하고자 한다. 운전자의 피로 상태를 검출하기 위한 얼굴 표정 인식을 위해 얼굴 특징을 추적하고자 하였다. 그러나 대다수의 얼굴 특징 추적 방법은 다양한 조명 조건과 얼굴 움직임, 회전등으로 얼굴의 특징점이 검출하지 못하는 경우가 발생한다. 그러므로 본 논문에서는 얼굴 특징을 추출하는 새로운 능동적 방식을 제안하고자 한다. 제안된 방법은 우선, 능동적 적외선 감지기를 사용하여 다양한 조명 조건 하에서 동공을 검출하고, 검출된 동공은 얼굴 움직임을 예측하는데 사용되어진다. 얼굴 움직임에 따라 특징이 국부적으로 부드럽게 변화한다고 할 때, 칼만 필터로 얼굴 특징을 추적할 수 있다. 제한된 동공 위치와 칼만 필터를 동시에 사용함으로 각각의 특징 지점을 정확하게 예상 할 수 있었고, Gabor 공간에서 예측 지점에 인접한 지점을 특징으로 추적할 수 있다. 패턴은 검출된 특징에서 공간적 연관성에서 추출한 특징들로 구성된다. 실험을 통하여 다양한 조명과 얼굴 방향, 표정 하에서 제안된 능동적 방법의 얼굴 추적의 실효성을 입증하였다.

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피로 검출을 위한 능동적 얼굴 추적 (Active Facial Tracking for Fatigue Detection)

  • 김태우;강용석
    • 한국정보전자통신기술학회논문지
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    • 제2권3호
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    • pp.53-60
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    • 2009
  • 본 논문에서는 얼굴 특징을 추출하는 새로운 능동적 방식을 제안하고자 한다. 운전자의 피로 상태를 검출하기 위한 얼굴 표정 인식을 위해 얼굴 특징을 추적하고자 하였다. 그러나 대다수의 얼굴 특징 추적 방법은 다양한 조명 조건과 얼굴 움직임, 회전등으로 얼굴의 특징점이 검출하지 못하는 경우가 발생한다. 본 논문에서는 얼굴 특징을 추출하는 새로운 능동적 방식을 제안하고자 한다. 제안된 방법은 우선, 능동적 적외선 감지기를 사용하여 다양한 조명 조건하에서 동공을 검출하고, 검출된 동공은 얼굴 움직임을 예측하는데 사용되어진다. 얼굴 움직임에 따라 특징이 국부적으로 부드럽게 변화한다고 할 때, 칼만 필터로 얼굴 특징을 추적할 수 있다. 제한된 동공 위치와 칼만 필터를 동시에 사용함으로 각각의 특징 지점을 정확하게 예상할 수 있었고, Gabor 공간에서 예측 지점에 인접한 지점을 특징으로 추적할 수 있다. 패턴은 검출된 특징에서 공간적 연관성에서 추출한 특징들로 구성된다. 실험을 통하여 다양한 조명과 얼굴 방향, 표정 하에서 제안된 능동적 방법의 얼굴 추적의 실효성을 입증하였다.

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