• Title/Summary/Keyword: Eclipse-II

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Development of the Virtual Test Path for Eclipse-II, A Parallel Mechanism Motion Simulator (병렬구조 모션 시뮬레이터 이클립스-II 를 위한 가상현실 시험경로 개발)

  • 인우성;김종원
    • Proceedings of the Korean Society of Precision Engineering Conference
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    • 2004.10a
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    • pp.965-968
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    • 2004
  • This paper describes the development of the test path for Eclipse-II, a parallel mechanism motion simulator. Eclipse-II which can be used as a base for general motion simulators, enables unlimited continuous 360-degree spinning in any rotational axes plus finite X, Y, and Z translation motions. The advantage of enabling continuous 360-degree spinning allows various motions for virtual reality. In this paper, the development of the test path to verify the robustness of the Eclipse-II motion simulator is described. The test motions, which satisfy the requirements of test path, are suggested and washout filter enables these motions reproduced in the limited workspace. The trial run is conducted to verify the robustness of the Eclipse-II motion simulator. Additionally the standard data format of virtual reality for Eclipse-II One Man Ride is suggested.

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Optimal Home Positioning Algorithm for a 6-DOF Eclipse-II Motion Simulator (6-자유도 Eclipse-II 모션 시뮬레이터의 최적 원점 복귀 알고리즘)

  • Shin, Hyun-Pyo;Kim, Jong-Won
    • Journal of the Korean Society for Precision Engineering
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    • v.29 no.4
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    • pp.441-448
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    • 2012
  • This paper describes the optimal home positioning algorithm of Eclipse-II, a new conceptual parallel mechanism for motion simulator. Eclipse-II is capable of translation and 360 degrees continuous rotation in all directions. In unexpected situations such as emergency stop, riders have to be resituated as soon as possible through a shortest translational and rotational path because the return paths are not unique in view of inverse kinematic solution. Eclipse-II is man riding. Therefore, the home positioning is directly related to the safety of riders. To ensure a least elapsed time, ZYX Euler angle inverse kinematics is applied to find an optimal home orientation. In addition, the subsequent decrease of maximum acceleration and jerk values is achieved by combining the optimal return path function with cubic spline, which consequently reduces delivery force and vibration to riders.

Mg II LINE VARIATION OF 32 CYGNI

  • Kang, Young-Woon
    • Journal of Astronomy and Space Sciences
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    • v.9 no.2
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    • pp.154-164
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    • 1992
  • The Mg II lines been extracted from the IUE archival spectra of 32 Cygni to investigate the effect of the atmospheric eclipse. The UV light curve has been reduced from the continuum flux at the center wavelength of 2807.5 ${\AA}$ in the IUE spectra. The equivalent width of the Mg II k absoption line has been measured for each spectra. The results of the light variation and flux tracing of the absorption line at the vicinity of the primary eclipse confirmed the atmospheric eclipse. The atmospheric effect lasted until the phase 0.06 in the absorptin line tracing, while it lasted until the phase 0.02 in the UV light curve, respectively.

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The Eclipse-II Parallel Mechanism for Motion Simulators

  • Kim, Jongwon;Hwang, Jae-Chul;Kim, Jin-Sung;Park, Frank C.;Cho, Young-Man
    • Proceedings of the Korean Society of Machine Tool Engineers Conference
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    • 2002.10a
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    • pp.286-291
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    • 2002
  • We present the analysis and design of a new six degree-of-freedom parallel mechanism, Eclipse-II, which can be used as a basis for general motion simulators. This mechanism allows x, y and z-axis translations and a, b and c-axis rotations. Most significantly, it presents the advantage of enabling continuous 360 degrees spinning of the platform. We first describe the computational procedures for the forward and in inverse kinematics of the Eclipse-II. Next, the complete singularity analysis is presented for the two cases of end-effector and actuator singularities. Two additional actuators are added to the original mechanism to eliminate both types of singularities with in the workspace. Some practical aspects of the prototype development are introduced.

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ATMOSPHERIC ECLIPSING BINARY ZETA AURIGAE IN THE 1987-1988 ECLIPSE (II)

  • Nha, Il-Seong
    • Journal of Astronomy and Space Sciences
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    • v.8 no.2
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    • pp.125-131
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    • 1991
  • UBV observations at Yonsei University Observatory (500 and 537 observations each at Ilsan Station and at Campus Station) were made for the latest eclipse of $\zeta$ Aur in 1987-1988. Orbital period of Saijo and Saito has been confirmed and the light and color variations on the night JD 244730 are found.

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Design and Analysis of Korean Lunar Orbiter Mission using Direct Transfer Trajectory (직접 전이궤적을 이용한 한국형 달 궤도선 임무설계 및 분석)

  • Choi, Su-Jin;Song, Young-Joo;Bae, Jonghee;Kim, Eunhyeuk;Ju, Gwanghyeok
    • Journal of the Korean Society for Aeronautical & Space Sciences
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    • v.41 no.12
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    • pp.950-958
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    • 2013
  • The Lunar orbiter is expected to be inserted into a ~300km low Earth orbit using Korea Space Launch Vehicle-II(KSLV-II). After the states are successfully determined with obtained tracking data, the Trans Lunar Injection(TLI) burn has to be done at appropriate epoch to send the lunar orbiter to the Moon. In this study, we describe in detail the mission scenario of the Korean lunar orbiter from the launch at NARO Space Center to lunar orbit insertion(LOI) stage following direct transfer trajectory. We investigate the launch window including launch azimuth, delta-V profile according to TLI and LOI burn positions. We also depict the visibility conditions of ground stations and solar eclipse duration to understand the characteristics of the direct transfer trajectory. This paper can be also helpful not only for overall understanding of ${\Delta}V$ trend by changing TOF and coasting time but for selecting launch epoch and control parameters to decrease fuel consumption.

A STUDY ON THE TRACKING AND POSITION PREDICTIONS OF ARTIFICIAL SATELLITE(II) - A Study on the Orbit Prediction - (인공위성 궤도의 추적과 예보의 기술개발(II) -궤도예보에 관하여-)

  • 박필호;김천휘;신종섭;이정숙;최규홍;박재우
    • Journal of Astronomy and Space Sciences
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    • v.8 no.1
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    • pp.99-113
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    • 1991
  • We developed a software system called IODS(ISSA Orbit Determination System), which can predict the orbit of arbitary artificial satellite using the numerical method. For evaluating the orbit prediction accuracy of IODS, the orbital data predicted for the meteorological satellite NOAA-11 and the stationary satellite INTELSAT-V are intercompared with those tracked at the Central Bureau of Meterology and the Kum-San Satellite Communication Station. And the Perturbations affecting the orbit of these artificial satellites are quantitatively analyzed. The orbital variation and the eclipse phenomina due to the shadow are analyzed for a hypothetical geostationary satellite called KORSAT-1 which is assumed to be located in longitude $110^{circ}E$.

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