• 제목/요약/키워드: k-space trajectory

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Impact of Human Mobility on Social Networks

  • Wang, Dashun;Song, Chaoming
    • Journal of Communications and Networks
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    • 제17권2호
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    • pp.100-109
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    • 2015
  • Mobile phone carriers face challenges from three synergistic dimensions: Wireless, social, and mobile. Despite significant advances that have been made about social networks and human mobility, respectively, our knowledge about the interplay between two layers remains largely limited, partly due to the difficulty in obtaining large-scale datasets that could offer at the same time social and mobile information across a substantial population over an extended period of time. In this paper, we take advantage of a massive, longitudinal mobile phone dataset that consists of human mobility and social network information simultaneously, allowing us to explore the impact of human mobility patterns on the underlying social network. We find that human mobility plays an important role in shaping both local and global structural properties of social network. In contrast to the lack of scale in social networks and human movements, we discovered a characteristic distance in physical space between 10 and 20 km that impacts both local clustering and modular structure in social network. We also find a surprising distinction in trajectory overlap that segments social ties into two categories. Our results are of fundamental relevance to quantitative studies of human behavior, and could serve as the basis of anchoring potential theoretical models of human behavior and building and developing new applications using social and mobile technologies.

상지 외골격 로봇 제어를 위한 인체 팔 동작의 기구학 및 동역학적 분석 - 파트 2: 제한조건의 선형 결합 (Analysis on the Kinematics and Dynamics of Human Arm Movement Toward Upper Limb Exoskeleton Robot Control - Part 2: Combination of Kinematic and Dynamic Constraints)

  • 김현철;이춘영
    • 제어로봇시스템학회논문지
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    • 제20권8호
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    • pp.875-881
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    • 2014
  • The redundancy resolution of the seven DOF (Degree of Freedom) upper limb exoskeleton is key to the synchronous motion between a robot and a human user. According to the seven DOF human arm model, positioning and orientating the wrist can be completed by multiple arm configurations that results in the non-unique solution to the inverse kinematics. This paper presents analysis on the kinematic and dynamic aspect of the human arm movement and its effect on the redundancy resolution of the seven DOF human arm model. The redundancy of the arm is expressed mathematically by defining the swivel angle. The final form of swivel angle can be represented as a linear combination of two different swivel angles achieved by optimizing two cost functions based on kinematic and dynamic criteria. The kinematic criterion is to maximize the projection of the longest principal axis of the manipulability ellipsoid of the human arm on the vector connecting the wrist and the virtual target on the head region. The dynamic criterion is to minimize the mechanical work done in the joint space for each of two consecutive points along the task space trajectory. The contribution of each criterion on the redundancy was verified by the post processing of experimental data collected with a motion capture system. Results indicate that the bimodal redundancy resolution approach improved the accuracy of the predicted swivel angle. Statistical testing of the dynamic constraint contribution shows that under moderate speeds and no load, the dynamic component of the human arm is not dominant, and it is enough to resolve the redundancy without dynamic constraint for the realtime application.

에너지와 대기시간을 고려한 우주비행체 랑데부 (Spacecraft Rendezvous Considering Orbital Energy and Wait Time)

  • 오승렬;이현재
    • 한국항공우주학회지
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    • 제45권9호
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    • pp.775-783
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    • 2017
  • 본 논문에서는 서로 다른 궤도상에 있는 두 우주비행체의 랑데부를 위한 최소 에너지 순간추력을 구하는 문제를 다룬다. 두 우주비행체의 궤도는 공면 궤도나 원 궤도 같이 특정 지어진 궤도가 아닌 일반적인 궤도이다. 이러한 최적화 문제를 다루기 위해 범용변수를 사용한 케플러 방정식과 두 우주비행체의 최종 위치 및 속도를 구속조건으로 사용하며, 전이 궤도의 정보를 얻기 위해 라그랑지 계수를 이용한다. 이 방법은 최소 에너지를 고려한 예시와 대기시간까지 고려한 예시를 통해 보여 지며, 최소 에너지 궤도로 알려진 호만 궤도와 비교함으로써 검증된다. 비록 닫힌 형태의 해를 얻을 수는 없었지만, 수치해석적 방식을 적용함으로써 다양한 궤도 전이 문제의 해를 구할 수 있음을 보여준다.

유도포탄 저속 회전 시 안정성 분석 (Stability Analysis on Guided Munition at Slow Spin)

  • 김영주;방효충;서송원;박장호;김진원;서일원
    • 한국항공우주학회지
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    • 제46권9호
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    • pp.752-759
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    • 2018
  • 본 논문에서는 비선형 모델 시뮬레이션을 통해 저속 회전 중인 유도포탄의 비행 모습을 확인하고 외란으로써 여러 가지 방향과 크기의 돌풍을 작용하여 유도포탄의 비행 안정성을 분석한 방법과 결과를 소개한다. 돌풍은 3m/s, 7m/s, 10m/s, 15m/s 네 가지의 속력을 가지고 26가지의 방향에서 탄도 정점 부근부터 작용하도록 설정하였다. 초당 1회전 및 3회전으로 회전하는 경우에 대해 총 208회의 시뮬레이션을 수행한 결과를 분석하였다. 초당 3회전으로 회전할 때는 탄체가 전복되지 않았지만, 초당 1회전으로 회전할 때는 7m/s 이상의 돌풍이 작용할 때 비행 후반부에 탄체가 전복되는 경우가 발견되었다. 탄체 비행 방향 반대쪽으로 작용하여 비행 방향 대기속도를 증가하는 돌풍은 해로운 영향을 주지 않았다. 탄체 전복은 모두 탄체가 하강하는 후반부에 발생하였으며, 탄도 정점 부근에서는 자세가 크게 진동하거나 탄체가 전복되지 않았다.

푸리에-스펙트럴 법을 사용한 근접 편대비행 항공기의 와 거동 계산 (Computation of Wake Vortex Behavior Behind Airplanes in Close Formation Flight Using a Fourier-Spectral Method)

  • 지승환;한철희
    • 한국항공우주학회지
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    • 제48권1호
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    • pp.1-11
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    • 2020
  • 항공기에서 발생한 후류의 거동은 항공기의 성능과 비행안정성에 큰 영향을 미친다. 본 연구에서는 푸리에-스펙트럴법을 사용하여 근접 편대비행을 하고 있는 항공기 날개 후류 거동에 관하여 연구하였다. 초기와의 순환강도, 상대위치 등에 따라 와들의 거동이 복잡한 양상으로 나타났다. 와의 순환강도 값이 큰 경우 와들의 이동이 크게 나타났다. 초기에는 가까이 위치한 와의 영향을 받아 이동하지만 이동하는 과정에서 다른 와와 가깝게 되면 새로운 경로를 형성하였다. 점성이 클수록 와의 반경이 증가하여 와 반경 근처로 새롭게 진입하는 와와 상호작용이 강해진다. 향후 항공기가 이착륙 시에 발생하는 지면 효과를 고려한 후류 거동 해석 연구를 수행하고자 한다.

단일물체 조작을 위한 두 협조 로봇의 협조제어 (A Coordination Control Methodlolgy for Two Cooperating Arms Handling a Single Object)

  • 여희주
    • 제어로봇시스템학회논문지
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    • 제6권2호
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    • pp.190-196
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    • 2000
  • A hybrid position/force control scheme to regulate the force and position by dual arms is proposed where two arms are treated as one rm in a kinematic viewpoint. The force error calculated from the information of two force/torque sensors attached to the end of each arm is transferred to minimum configuration space coordinates and then is distributed to total system joint coordinates, The position adjustment at the total con-figuration coordinates is computed based on the effective compliance matrix with respect to total joint coordinates which is obtained by coordinate transformation between the task coordinates and the total joint coordinates. The proposed scheme is applied to sawing task. When the trajectory of the saw is planned to follow a line in a horizontal plane 2 position parameters are to be controlled(i.e., two translational positions) Also a certain level of contact force has to be controlled along the vertical direction(i.e. minus z-direction) not to loose the contact with the object to be sawn. We experimentally show that the performance of the velocity and force response are satisfactory. The proposed hybrid control scheme can be applied to arbitrary two cooperating arm system regardless of their kinematic structure and the number of actuated joints.

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모바일 애드-혹 망을 위한 퍼지 비정상 행위 탐지 알고리즘 (FADA: A fuzzy anomaly detection algorithm for MANETs)

  • 배인한
    • Journal of the Korean Data and Information Science Society
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    • 제21권6호
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    • pp.1125-1136
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    • 2010
  • 최근에 이동 객체 추적 장치로부터 얻어진 추적 스트림에 대한 온라인 비정상 행위 감시에 대한 요구가 증가하고 있다. 제한된 공간 비용 내에서 고속 데이터 처리의 요구사항에 기인하여 이 문제는 흥미를 끌고 있다. 이 논문에서, 우리는 모바일 애드 혹 망에서 모바일 장치의 위성항법장치 로그로부터 이동특징 정보를 계산하여 정상 프로파일을 구축하고, 모바일 장치의 현재 이동 특징 정보와 정상 프로파일내의 이동 특징 정보간의 퍼지 비유사도를 계산한다. 그 계산된 퍼지 비유사도를 기초로 그 모바일 장치의 비정상 행위를 효율적으로 탐지하는 퍼지 비정상 행위 탐지 알고리즘을 제안한다. 그리고 모의실험을 통하여 제안한 알고리즘의 성능을 평가한다.

3.0T 자기공명영상을 이용한 잡음전력스펙트럼 특성 평가 (Evaluation of Noise Power Spectrum Characteristics by Using Magnetic Resonance Imaging 3.0T)

  • 민정환;정회원;김승철
    • 대한방사선기술학회지:방사선기술과학
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    • 제44권1호
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    • pp.31-37
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    • 2021
  • This study aim of quantitative assessment of Noise Power Spectrum(NPS) and image characteristics of by acquired the optimal image for noise characteristics and quality assurance by using magnetic resonance imaging(MRI). MRI device was (MAGNETOM Vida 3.0T MRI; Siemense healthcare system; Germany) used and the head/neck shim MR receive coil were 20 channels coil and a diameter 200 mm hemisphere phantom. Frequency signal could be acquired the K-space trajectory image and white image for NPS. The T2 image highest quantitatively value for NPS finding of showed the best value of 0.026 based on the T2 frequency of 1.0 mm-1. The NPS acquired of showed that the T1 CE turbo image was 0.077, the T1 CE Conca2 turbo image was 0.056, T1 turbo image was 0.061, and the T1 Conca2 turbo image was 0.066. The assessment of NPS image characteristics of this study were to that could be used efficiently of the MRI and to present the quantitative evaluation methods and image noise characteristics of 3.0T MRI.

Accelerating Magnetic Resonance Fingerprinting Using Hybrid Deep Learning and Iterative Reconstruction

  • Cao, Peng;Cui, Di;Ming, Yanzhen;Vardhanabhuti, Varut;Lee, Elaine;Hui, Edward
    • Investigative Magnetic Resonance Imaging
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    • 제25권4호
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    • pp.293-299
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    • 2021
  • Purpose: To accelerate magnetic resonance fingerprinting (MRF) by developing a flexible deep learning reconstruction method. Materials and Methods: Synthetic data were used to train a deep learning model. The trained model was then applied to MRF for different organs and diseases. Iterative reconstruction was performed outside the deep learning model, allowing a changeable encoding matrix, i.e., with flexibility of choice for image resolution, radiofrequency coil, k-space trajectory, and undersampling mask. In vivo experiments were performed on normal brain and prostate cancer volunteers to demonstrate the model performance and generalizability. Results: In 400-dynamics brain MRF, direct nonuniform Fourier transform caused a slight increase of random fluctuations on the T2 map. These fluctuations were reduced with the proposed method. In prostate MRF, the proposed method suppressed fluctuations on both T1 and T2 maps. Conclusion: The deep learning and iterative MRF reconstruction method described in this study was flexible with different acquisition settings such as radiofrequency coils. It is generalizable for different in vivo applications.

The Flow of the Interstellar Plasmas surrounding the Heliopause estimated via IBEX-Lo Observations

  • 박지우
    • 천문학회보
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    • 제43권1호
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    • pp.51.3-52
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    • 2018
  • Since Voyager 1 passed the Heliopause in 2012, it has provided the observations of the charged particles in the local interstellar medium. However, Voyager 1 only provides the information along with its trajectory. In order to understand the global view of the interstellar plasma flow surrounding the Heliopause, we need another tool. When the interstellar plasmas approach the Heliopause, the ions are deflected around the Heliopause due to the draping of the interstellar magnetic field. The draping of the interstellar magnetic field is strongly connected with the shape of the Heliopause. A fraction of the diverted ions exchanges their charges with the undisturbed primary interstellar neutral atoms, and then the ions become neutral atoms called the secondary interstellar neutral atoms. The newly created neutral atoms carry information on the diverted flow of the interstellar ions, and a fraction of them can travel to the Sun. Therefore, the secondary component of the interstellar neutrals is an excellent diagnostic tool to provide important information to constrain the shape of the Heliopause. The secondary interstellar neutrals are observed by Interstellar Boundary Explorer (IBEX) at Earth's orbit. Since 2009, two energetic neutral atom cameras on IBEX have measured neutral atoms and it has provided sky maps of neutral atoms. In this presentation, we will discuss the directional distribution of the secondary interstellar neutrals at Earth's orbit. In the sky maps, the primary interstellar neutral gas is seen between $200^{\circ}$ and $260^{\circ}$ in ecliptic longitude and the secondary components are seen in the longitude range of $160^{\circ}-200^{\circ}$. We also present a simplified model of the outer heliosheath to help interpret the observations of interstellar neutrals by the IBEX-Lo instruments. We extract information on the large-scale shape of the Heliopause by comparing the neutral flux measured at IBEX along four different look directions with simple models of deflected plasma flow around hypothetical obstacles of different aspect ratios to the flow. Our comparisons between the model results and the observations indicate that the Heliopause is very blunt in the vicinity of the Heliospheric nose, especially compared to a Rankine half-body or cometary shape.

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