• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2005년도 추계학술대회논문집
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• pp.620-628
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• 2005

Spatial control of sound is essential to deliver better sound to the listener's position in space. As it can be experienced in many listening environments, the quality of sound can not be manifested over every position in a hall. This motivates us to control sound in a region we select. The primary focus of the developed method has to do with the brightness and contrast of acoustic image in space. In particular, the acoustic brightness control seeks a way to increase loudness of sound over a chosen area, and the contrast control aims to enhance loudness difference between two neighboring regions. This enables us to make two different kinds of zone - the zone of quiet and the zone of loud sound - at the same time. The other perspective of this study is on the direction of sound. It is shown that we can control the direction of perceived sound source by focusing acoustic energy in wavenumber domain. To begin with, the proposed approaches are formulated for pure-tone case. Then the control methods are extended to a more general case, where the excitation signal has broadband spectrum. In order to control the broadband signal in time domain, an inverse filter design problem is defined and solved in frequency domain. Numerical and experimental results obtained in various conditions certainly validate that the acoustic brightness, acoustic contrast, direction of wave front can be manipulated for some finite region in space and time.

• 천문학회지
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• 제56권1호
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• pp.23-33
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• 2023

We investigate the diffusion process of Thomson-scattered line photons in both real space and frequency space through a Monte Carlo approach. The emission source is assumed to be monochromatic and point-like embedded at the center of a free electron region in the form of a sphere and a slab. In the case of a spherical region, the line profiles emergent at a location of Thomson optical depth τ_Th from the source exhibit the full width of the half maximum σ_λ ≃ τ^1.5_Th. In the slab case, we focus on the polarization behavior where the polarization direction flips from the normal direction of the slab to the parallel as the slab optical depth τ_Th increases from τ_Th ≪ 1 to τ_Th ≫ 1. We propose that the polarization flip to the parallel direction to the slab surface in optically thick slabs is attributed to the robustness of the Stokes parameter Q along the vertical axis with respect to the observer's line of sight whereas randomization dominates the remaining region as τ_Th increases. A brief discussion on the importance of our study is presented.

• 한국지능시스템학회논문지
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• 제24권5호
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• pp.518-528
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• 2014

본 논문에서는 4차원 시공간 (4D-ST, [x,y,z,t]) 특징을 이용하여 행동 방향을 인식하는 방법을 제안한다. 이를 위해 4차원 시공간 특징점 (4D-STIPs, [x,y,z,t])을 제안하였고, 이는 여러 다른 뷰에서 촬영한 이미지들로부터 복원된 3차원 공간 (3D-S, [x,y,z]) 볼륨으로부터 계산된다. 3차원 공간정보를 갖고 있는 3D-S 볼륨과 4D-STIPs는 2차원 공간 (2D-S, [x,y]) 뷰로 사영을 하여 임의의 2D-S 뷰에서의 특징을 생성해 낼 수 있다. 이 때, 사영 방향을 결정 할 수 있으므로, 학습 시 방향에 대한 정보를 포함하여 행동 방향을 인식 할 수 있다. 행동 방향을 인식하는 과정은 두 단계로 나눌 수 있는데, 우선 어떤 행동인지를 인식하고 그 후, 방향 정보를 이용하여 최종적으로 행동 방향을 인식한다. 행동 인식과 방향 인식을 위해, 사영된 3D-S 볼륨과 4D-STIPs은 각각 움직이는 부분과 움직이지 않는 부분에 대한 정보를 담고 있는 motion history images (MHIs)와 non-motion history images (NMHIs)로 구성된다. 이러한 특징들은 행동 인식을 위해, 방향 정보에 상관없이 같은 행동이면 같은 클래스로 분류되어 support vector data description (SVDD) 분류기로 학습되고, support vector domain density description (SVDDD)을 이용하여 인식된다. 인식된 행동에서 최종적으로 방향을 인식하기 위해 각 행동을 방향 클래스로 분류하여 SVDD 분류기로 학습하고 SVDDD로 인식한다. 제안된 방법의 성능을 보이기 위해서 INRIA Xmas Motion Acquisition Sequences (IXMAS) 데이터셋에서 제공하는 3D-S 볼륨을 사용하여 학습을 하고, 행동 방향 인식 실험이 가능한 SNU 데이터셋을 구축하여 인식 실험을 하였다.

• Journal of Astronomy and Space Sciences
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• 제23권1호
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• pp.29-38
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• 2006

이 논문에서는 통신해양기상위성 1호기의 영상위치유지를 위한 영상오차보상 알고리즘을 설계하였다. 영상오차보상 알고리즘은 관측영상의 위치결정 및 위치유지를 위한 INR시스템의 핵심요소이다. 궤도와 자세에 대한 다양한 섭동 때문에 위성체의 움직임에 변화가 생기고, 이로 인해 영상기의 포인팅 어긋남이 발생하며, 그 결과로 관측영상의 일그러짐이 유발된다. 포인팅 어긋남을 바로잡기 위하여 보정해 야할 스캔 거울의 각도를 GEOS 위성과 다른 방법으로 계산하였다. 새로 설계된 영상오차보상 알고리즘의 성능을 검증하기 위해 미국의 기상위성 GOES의 INR시스템에 적용된 영상오차보상 알고리즘과 비교평가를 하였다. 설계된 영상오차보상 알고리즘은 영상기의 포인팅 어긋남을 효과적으로 보상함으로써 약 40% 이상의 지향정밀도를 향상시킬 수 있었다.

• 한국실내디자인학회논문집
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• 제18권6호
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• pp.104-114
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• 2009

The purpose of study was understanding necessity of environment design for underground parking lot in residential design plan and grasping design plans of 'Activity Support' that considerate women, exclude women's unsecured feeling at underground parking lot. The inquiry analyzed 6 design plan in design competition that considerate women according to precede studies, a theory of CPTED, a design guide for wayfinding, and survey. A ramp, circulation, entrance, lighting, ventilation, and space design plan are proceed on this study The result are as below. First, a rectilinear figure ramp suits entrance plan on the circulation, but if it is not possible, cross-using of rectilinear and curvilinear figure ramp plan is desirable. Second, on the circulation plan, vehicles circulation plan and equality parking distribution plan got accomplished generally, and help senses of direction because it is planed network systemize. On a large scale underground parking lot, simplify parking circulation to convenience entrance and exit for weak in sense of direction. Third, the shape and material that‘s environmentally conscious will be in use to the entrance plan. As the first stage to the underground, artwork that women prefer can modulate the rejection of underground space. Forth, natural lighting system and ventilation can make the environment-friendly space, decrease the women’s rejection to the underground, it can also keep a natural watch on the space. Fifth, on the space design plan, it can use bright and comfortable design of wall and ground to decrease the women‘s rejection, also it is useful to the sense of direction. LED indirect lighting plan that 58.7% of women prefers on survey reflects women’s state of desire that bright and atmosphere. In addition, proper use of plans that subsidiary facilities, rest area with Sunken, and nature-friendly material can minimize differences of underground and ground parking lot.

• 대한치과보철학회지
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• 제13권1호
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• pp.11-22
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• 1975

This study is to determine the severity and direction of the movement of the adjacent tooth into the created space by tooth or teeth loss. The random samples 387 cases (upper; 121 cases, lower; 266 cases) were selected with surveying record under some criteria. Edentulous area is grouped into the free end type and the tooth borne type. The following results were obtained. In the tooth borne type, slight distal movement of the adjacent tooth into the edentulous space was obtained. And the tooth distal to the edentulous space moved into the space in proportion to the duration of the edentulous state. Elongation of the opposing tooth of the free end type was more severe than that of the tooth borne type. And no inter-relationship between the severity of the elongation and the duration of the edentulous state In general, adjacent teeth had normal and mesial inclination. Lower teeth migrated mesially and lingually (especially in the distal tooth to the edentulous space in the tooth borne type). Upper adjacent teeth usually moved into the normal direction.

• 천문학회보
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• 제44권1호
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• pp.34.3-34.3
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• 2019

We report our discovery of observational evidence for the coherence between galaxy rotation and the average motion of neighbors. Using the Calar Alto Legacy Integral Field Area (CALIFA) survey data analyzed with the Python CALIFA STARLIGHT Synthesis Organizer (PyCASSO) platform, and the NASA-Sloan Atlas (NSA) catalog, we estimate the angular momentum vectors of 445 CALIFA galaxies and build composite maps of their neighbor galaxies on the parameter space of velocity versus distance. The composite radial profiles of the luminosity-weighted mean velocity of neighbors show striking evidence for dynamical coherence between the rotational direction of the CALIFA galaxies and the average moving direction of their neighbor galaxies. The signal of such dynamical coherence is significant for the neighbors within 800 kpc distance from the CALIFA galaxies with a confidence level of $3.5{\sigma}$, when the angular momentum is measured at the outskirt ($Re<R{\leq}2Re$) of each CALIFA galaxy. We also find that faint or kinematically misaligned galaxies show stronger coherence with neighbor motions than bright or kinematically well-aligned galaxies do. Our results show that the rotation of a galaxy, particularly at its outskirt, may be significantly influenced by recent interactions with its neighbors.

• 한국실내디자인학회논문집
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• 제14권5호
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• pp.159-166
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• 2005

This study is focused on Resider's Preference of Residential Space to improve Residence Unit Plan. Three Rental Housing Complexes in Jeju which supplied by Korea National Housing Corporation(KNHC) were selected for more detailed Resider's Preference research, which were constructed within 5years. Questionnaire of Total 360 sheets were distributed for each Rental Housing Complexes and total 299 sheets were returned. The results of research are as the followings. Generally satisfaction of environment and living area of home is not high. And also it seem that many residers want to live in housing of average 25.87 pyeong in housing scale. In view and direction of housing Especially, many residers tend to select housing that view is better than direction. With based on like this results, it is proposed housing plan's develop and political supports reflected Jeju's culture condition, life style, climate and so on.

• Journal of Astronomy and Space Sciences
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• 제29권1호
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• pp.11-21
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• 2012

In this paper, the authors introduced a new approach to find the optimal collision avoidance maneuver considering multi threatening objects within short period, while satisfying constraints on the fuel limit and the acceptable collision probability. A preliminary effort in applying a genetic algorithm (GA) to those kinds of problems has also been demonstrated through a simulation study with a simple case problem and various fitness functions. And then, GA is applied to the complex case problem including multi-threatening objects. Two distinct collision avoidance maneuvers are dealt with: the first is in-track direction of collision avoidance maneuver. The second considers radial, in-track, cross-track direction maneuver. The results show that the first case violates the collision probability threshold, while the second case does not violate the threshold with satisfaction of all conditions. Various factors for analyzing and planning the optimal collision avoidance maneuver are also presented.

• 천문학회지
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• 제40권4호
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• pp.91-97
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• 2007

The Fokker-Planck (FP) model is one of the commonly used methods for studies of the dynamical evolution of dense spherical stellar systems such as globular clusters and galactic nuclei. The FP model is numerically stable in most cases, but we find that it encounters numerical difficulties rather often when the effects of tidal shocks are included in two-dimensional (energy and angular momentum space) version of the FP model or when the initial condition is extreme (e.g., a very large cluster mass and a small cluster radius). To avoid such a problem, we have developed a new integration scheme for a two-dimensional FP equation by adopting an Alternating Direction Implicit (ADI) method given in the Douglas-Rachford split form. We find that our ADI method reduces the computing time by a factor of ${\sim}2$ compared to the fully implicit method, and resolves problems of numerical instability.