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REAL - TIME ORBIT DETERMINATION OF LOW EARTH ORBIT SATELLITES USING RADAR SYSTEM AND SGP4 MODEL (RADAR 시스템과 SGP4 모델을 이용한 저궤도 위성의 실시간 궤도결정)

  • 이재광;이성섭;윤재철;최규홍
    • Journal of Astronomy and Space Sciences
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    • v.20 no.1
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    • pp.21-28
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    • 2003
  • In case that we independently obtain orbital informations about the low earth satellites of foreign countries using radar systems, we develop the orbit determination algorithm for this purpose using a SGP4 model with an analytical orbit model and the extended Kalman filter with a real-time processing method. When the state vector is Keplerian orbital elements, singularity problems happen to compute partial derivative with respect to inclination and eccentricity orbit elements. To cope with this problem, we set state vector osculating to mean equinox and true equator cartesian elements with coordinate transformation. The state transition matrix and the covariance matrix are numerically computed using a SGP4 model. Observational measurements are the type of azimuth, elevation and range, filter process to each measurement in a lump. After analyzing performance of the developed orbit determination algorithm using TOPEX/POSEIDON POE(precision 0.bit Ephemeris), its position error has about 1 km. To be similar to performance of NORAD system that has up to 3km position accuracy during 7 days need to radar system performance that have accuracy within 0.1 degree for azimuth and elevation and 50m for range.

The Surface Sidelobe Clutter and the False Alarm Probability of Target Detection for the HPRF Waveform of the Microwave Seeker (마이크로파 탐색기의 HPRF 파형에 대한 지표면 부엽클러터와 표적탐지 오류 확률)

  • Kim, Tae-Hyung;Yi, Jae-Woong;Byun, Young-Jin
    • The Journal of Korean Institute of Communications and Information Sciences
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    • v.34 no.4C
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    • pp.476-483
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    • 2009
  • Tracking and detecting targets by the microwave seeker is affected by the clutter reflecting from the earth's surface. In order to detect retreating targets in look-down scenario, which appear in the sidelobe clutter (SLC) region, in the microwave seeker of high pulse repetition frequency (HPRF) mode, it is necessary to understand statistical characteristics of the surface SLC. Statistical analysis of SLC has been conducted for several kinds of the surface using data obtained by the captive flight test of the microwave seeker in the HPRF mode. The probability density function (PDF) fitting is conducted for several kinds and conditions of the surface. PDFs and PDF parameters, which best describe statistical distribution of the SLC power, are estimated. By using the estimated PDFs and PDF parameters, analyses for setting the target-detection thresholds, which give a desired level of target-detection false alarm probability, are made. These analysis materials for statistical characteristics of SLC power and the target-detection threshold can be used in various fields, such as development of a target-detection method, the constant false alarm rate processing.

태양 주위에 있는 만기형 주계열성의 자전에 관한 연구

  • Yang, Eun-Su;Lee, Sang-Gak
    • Publications of The Korean Astronomical Society
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    • v.4 no.1
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    • pp.31-52
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    • 1989
  • The rotational properties of late-type main sequence stars in the solar neighborhood have been investigated. So rotation periods and stellar radii are determined for 104 field stars, 8 Ursa Major Group stars, and 20 Hyades cluster stars. Most of the rotation periods are derived using the Noyes et al. (1984)'s relation between chromospheric activity and rotation period. Stellar radii are calculated by the Stefan law for the nearby stars within 25 pc from the sun. Rotational velocities at equator are determined by the above rotation periods and stellar radii. Their distribution along the (B-V) color shows an upper boundary and an abrupt drop for the stars in the range of 0.4<(B-V)<0.8, as found from the apparent rotational velocity data. Furthermore, it is apparent that there is an lower boundary of rotational velocity. The inclination of rotation axis to line-of-sight is obtained by comparing the rotational velocity at equator with the apparent rotational velocity given by the analysis of the line profiles. For the field stars, it is found that the inclination has no correlation with the galactic lattitude and follows random distribution.

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Tile-Based 360 Degree Video Streaming System with User's gaze Prediction (사용자 시선 예측을 통한 360 영상 타일 기반 스트리밍 시스템)

  • Lee, Soonbin;Jang, Dongmin;Jeong, Jong-Beom;Lee, Sangsoon;Ryu, Eun-Seok
    • Journal of Broadcast Engineering
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    • v.24 no.6
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    • pp.1053-1063
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    • 2019
  • Recently, tile-based streaming that transmits one 360 video in several tiles, is actively being studied in order to transmit these 360 video more efficiently. In this paper, for the transmission of high-definition 360 video corresponding to user's viewport in tile-based streaming scenarios, a system of assigning the quality of tiles at each tile by applying the saliency map generated by existing network models is proposed. As a result of usage of Motion-Constrained Tile Set (MCTS) technique to encode each tile independently, the user's viewport was rendered and tested based on Salient360! dataset, streaming 360 video based on the proposed system results in gain to 23% of the user's viewport compared to using the existing high-efficiency video coding (HEVC).

A SPECTROSCOPIC STUDY OF THE CLOSE BINARY AG VIRGINIS (근접쌍성 AG Virginis의 분광학적 연구)

  • Kim, Ho-Il;Lee, Chung-Uk;Lee, Jae-Woo;Sohn, Mi-Rim
    • Journal of Astronomy and Space Sciences
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    • v.22 no.4
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    • pp.353-362
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    • 2005
  • We performed a new high-resolution spectroscopy of AG Vir for 4 nights from 25 March 2004 using the BOES (Bohyunsan Optical Echelle Spectrograph) attached to the 1.8-m reflector at Bohyunsan Optical Astronomy Observatory, and obtained a total of 59 spectra where all orbital phases are covered. To get the radial velocities of the binary system, both method of the CCF (Cross-Co..elation Function)and the BF (Broadening Function) were applied to the analysis of all the observed spectra. From these, the CCF could calculate the radial velocities of the primary star alone, while the BF could determine those of the primary and the secondary components. New absolute dimensions were deduced with the combination of our spectroscopic orbital elements ($K_1=90.5km/s$$K_2=258.8$) and the photometric solutions of Bell, Rainger, & Hilditch (1990): $A_1,=1.99M_\bigodot,\;M_2=0.62M_\bigodot,\;R_1=2.21R_\bigodot,\;R_2=1.36R_\bigodot,\;L_1=13.17L_\bigodot,\;and\;L_2=3.47L_\bigodot$. Our absolute parameters are larger and brighter than those derived from Bell, Rainger, & Hilditch (1990). We re-analyzed all the previous radial-velocity curves of AG Vir and, as a result, can see that its system velocity scatters largely up to ${\pm}8km/s$. However, we, at present, cannot determine this as the light-time effect due to the third body, which was suggested as a cause of the orbital period changes by Qian (2001).

The effect of preference color of children's hospital lobby on the visual attention (어린이병원 로비공간에서 선호 색채가 시지각 주의집중에 미친 영향)

  • Cho, Eun Kil;Son, Kwang Ho
    • Korea Science and Art Forum
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    • v.23
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    • pp.347-358
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    • 2016
  • The design of children's hospitals is highly dependent on color schemes. As a space shared together by both adults and children, the design of children's hospitals require color coordination that takes account of the users' characteristics. However, because the majority of prior research on color perception has focused overly on the emotional aspects, there is a necessity for more rational and scientific analyses to identify the characteristics of the visual perception of colors. Adopting this perspective in analyzing the characteristics of the visual perception of colors, this study aims to move beyond the abstract to focus on more objective methods, such as eye-tracking experiments, to examine the characteristics of hospital visitors' visual attention with respect to colors. Visual perception tracking experiment was conducted on the 2 chosen experimental images with a target group made up of adults and children, the following results were found. Firstly, spaces created with the preference colors of the different groups were found to develop a characteristic of developing higher attention. Secondly, observing the common tendencies for attention for adults and children, the highest region for visual concentration was formed towards the middle, as attention progresses to lower stages visually focused area changes in the order of upper-middle, left and right, and lower regions and edge regions show characteristics of not triggering attention Thirdly, it is understood that children's level of attention drops a lot faster than adults when identifying space therefore it is suspected that children need more elaborate color coordination than adults.

Development of the Optimum Condition for Improving Retroreflection of Road Markings (노면표시 반사성능 향상을 위한 최적 조건 개발)

  • 여운웅
    • Proceedings of the KOR-KST Conference
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    • 1998.10a
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    • pp.342-351
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    • 1998
  • 노면표시는 운전자에게 시선유도와 각종 규제 및 지시에 대한 정보를 제공함으로써 교통안전 및 소통에 도움을 주는 시설로써 주야간의 시인성 확보가 중요하며 이를 위해서는 반사화가 필요하다. 노면표시의 반사성능은 유리알 (Glass Bead)의 함량 및 종류, 용융온도, 도료의 색도등 각 영향인자에 의해 결정되지만 현재는 시공법 및 관련 연구의 미흡으로 현행기준의 최하수준을 상회하는 정도로 제공되고 있다. 따라서 본 연구에서는 노면표시의 시공에 관계되는 각 요인중 반사성능가 내구성에 영향을 미치는 주요인자 및 반사성능을 최적화하기 위한 인자별 최적조합을 도출하였다. 연구결과 유리알 살포량이 중량비로 25%-30%, 용융시 온도가 $188^{\circ}C$$\pm$$10^{\circ}C$일 때 노면표면시의 반사성능이 최적화됨을 밝혀내었다. 또한 유리알의 품질개선과 함께 황색 노면표시의 재귀반사 휘도계수 기준을 현재 기준보다 상향조정할 필요성이 있음을 제안하였다.

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Radome Slope Estimation using Mode Parameter Renewal Method of IMM Algorithm (IMM 알고리듬의 모드 계수 갱신 방법을 통한 레이돔 굴절률 추정)

  • Kim, Young-Mo;Back, Ju-Hoon
    • The Journal of the Korea institute of electronic communication sciences
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    • v.12 no.5
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    • pp.763-770
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    • 2017
  • A radome mounted on the front of an aircraft can cause refraction errors for various reasons that occur during maneuver in seeking and tracking a target. This refraction error means that the microwave seeker is detecting apparent target. An Interactive Multiple Model (IMM) algorithm is applied to estimate radome slope mounted on an aircraft in 3D space. However, even though the parameter of uncertain system model such as radome slope can be estimated, the estimated performance can not be guaranteed when it exceeds the range of the predicted value. In this paper, we propose a method to update the predicted value by using the radome slope as the mode parameter of the IMM algorithm, and confirm the radome slope estimation performance of the proposed method.

A Study on the Transformation Motif in Animations (애니메이션의 변신(變身) 모티프 연구)

  • Cho, Mi-Ra
    • Cartoon and Animation Studies
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    • s.11
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    • pp.153-167
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    • 2007
  • This paper examined the immanent ideological bases in the transformation motif of animations, focusing on several leading animation works in which a human gets transformed into an animal, or vice versa, and also took a look at what meaning and function this transformation motif adds to their narrative. As a result of analyzing the animation texts centered on the transformation motif, transforming into an animal in is applied as a means for punishment. It shows the notion that the animals need men's care, that is, the anthropocentric point of view that the animals need to be overcome and conquered had a strong influence upon this work. However, in , a boy realizes that the animals(nature) are not the targets to conquer and learns to appreciate the principle of Mother Nature through the process of becoming a bear. By this description, this work shows deep reflection on nature and human being. Lastly, shows a desire to overpass the border to forbidden things, and describes the relationship between men and animals(nature) in a variety of perspectives. Furthermore, this study examined how the variety of attitudes toward the transformation targets is formed in each work.

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CORRECTION OF THE TRACKING DATA OF AN ARTIFICIAL SATELLITE CONSIDERING THE EARTH ATMOSPHERE AND LIGHT TIME EFFECTS (지구 대기와 광시간 효과를 고려한 인공위성 추적자료의 보정 S/W 개발)

  • 김경희;김천휘;김성규
    • Journal of Astronomy and Space Sciences
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    • v.12 no.1
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    • pp.123-132
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    • 1995
  • We developed a S/W system to simulate the orbit tracking data as nearly equal as the real data obtained at the tracking antenna by modeling various causes that could have effects on the tracking data (range, range rate, azimuth, elevation) of an artificial satellite. Using the S/W developed we produced delay values of tracking data due to the light-time effect and the terrestrial atmosphere. According to the simulation results due to the Earth atmosphere, the values delayed by the troposhpere were increased as the temperature, relative humidity, and pressure of the troposphere are more larger. However, delay values due to the ionosphere were dependent on both the maximum electron density and the frequencies used. They are more and more increased as the maximum electron density and frequency are more larger. And the delaying values by the light-time effect are more larger by the fast orbital motion as the altitude of an artificial satellite is more lower.

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