• Title/Summary/Keyword: TLE(TLE)

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Ictal Cerebral Perfusion Patterns in Partial Epilepsy: SPECT Subtraction (부분적 간질에서 SPECT Subtraction을 이용한 발작 중 뇌혈류 변화에 대한 연구)

  • Lee, Hyang-Woon;Hong, Seung-Bong;Tae, Woo-Suk;Kim, Sang-Eun;Seo, Dae-Won;Jeong, Seung-Cheol;Yi, Ji-Young;Hong, Seung-Chyul
    • The Korean Journal of Nuclear Medicine
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    • v.34 no.3
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    • pp.169-182
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    • 2000
  • Purpose: To investigate the various ictal perfusion patterns and find the relationships between clinical factors and different perfusion patterns. Materials and Methods: Interictal and ictal SPECT and SPECT subtraction were performed in 61 patients with partial epilepsy. Both positive images showing ictal hyperperfusion and negative images revealing ictal hypoperfusion were obtained by SPECT subtraction The ictal perfusion patterns of subtracted SPECT were classified into focal hyperperfusion, hyperperfusion-plus, combined hyperperfusion-hypoperfusion, and focal hypoperfusion only. Results: The concordance rates with epileptic focus were 91.8% in combined analysis of ictal hyperperfusion and hypoperfusion images of subtracted SPECT, 85.2% in hyperperfusion images only of subtracted SPECT, and 68.9% in conventional ictal SPECT analysis. Ictal hypoperfusion occurred less frequently in temporal lobe epilepsy (TLE) than extratemporal lobe epilepsy. Mesial temporal hyperperfusion alone was seen only in mesial TLE while lateral temporal hyperperfusion alone was observed only in neocortical TLE. Hippocampal sclerosis had much lower incidence of ictal hypoperfusion than any other pathology. Some patients showed ictal hypoperfusion at epileptic focus with ictal hyperperfusion in the neighboring brain regions where ictal discharges propagated. Conclusion: Hypoperfusion as well as hyperperfusion in ictal SPECT should be considered for localizing epileptic focus. Although the mechanism of ictal hypoperfusion could be an intra-ictal early exhaustion of seizure focus or a steal phenomenon by the propagation of ictal discharges to adjacent brain areas, further study is needed to elucidate it.

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Minimum Number of Observation Points for LEO Satellite Orbit Estimation by OWL Network

  • Park, Maru;Jo, Jung Hyun;Cho, Sungki;Choi, Jin;Kim, Chun-Hwey;Park, Jang-Hyun;Yim, Hong-Suh;Choi, Young-Jun;Moon, Hong-Kyu;Bae, Young-Ho;Park, Sun-Youp;Kim, Ji-Hye;Roh, Dong-Goo;Jang, Hyun-Jung;Park, Young-Sik;Jeong, Min-Ji
    • Journal of Astronomy and Space Sciences
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    • v.32 no.4
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    • pp.357-366
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    • 2015
  • By using the Optical Wide-field Patrol (OWL) network developed by the Korea Astronomy and Space Science Institute (KASI) we generated the right ascension and declination angle data from optical observation of Low Earth Orbit (LEO) satellites. We performed an analysis to verify the optimum number of observations needed per arc for successful estimation of orbit. The currently functioning OWL observatories are located in Daejeon (South Korea), Songino (Mongolia), and Oukaïmeden (Morocco). The Daejeon Observatory is functioning as a test bed. In this study, the observed targets were Gravity Probe B, COSMOS 1455, COSMOS 1726, COSMOS 2428, SEASAT 1, ATV-5, and CryoSat-2 (all in LEO). These satellites were observed from the test bed and the Songino Observatory of the OWL network during 21 nights in 2014 and 2015. After we estimated the orbit from systematically selected sets of observation points (20, 50, 100, and 150) for each pass, we compared the difference between the orbit estimates for each case, and the Two Line Element set (TLE) from the Joint Space Operation Center (JSpOC). Then, we determined the average of the difference and selected the optimal observation points by comparing the average values.

Topographic Changes of Ictal Hyperperfusion During Progression of Clinical Seizures (간질발작의 진행에 따른 발작기 SPECT의 혈류증가 양상)

  • Shin, Won-Chul;Hong, Seung-Bong;Tae, Woo-Suk;Shon, Young-Min;Seo, Dae-Won;Kim, Byoung-Joon;Hong, Seung-Chyul;Kim, Sang-Eun
    • The Korean Journal of Nuclear Medicine
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    • v.35 no.6
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    • pp.352-363
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    • 2001
  • Purpose: To investigate ictal hyperperfusion patterns during semiologic progression of seizures, we performed SPECT subfraction in 50 patients with temporal lobe epilepsy (TLE). Materials and Methods: The patients were categorized Into five groups according to semiologic progression during ictal SPECT (group-1 having only aura; group-2 haying motionless staling with or without aura; group-3 having motionless staring and then automatism with or without aura; group-4 having motionless staring and then dystonic posturing with or without aura and automatism; group-5 having motionless staring, automatism, then head version and generalized seizures with or without aura and dystonic posturing). Results: In group-1, three patients showed ipsilateral temporal hyperperfusion and two had bilateral temporal hyperperfusion with ipsilateral predominance. In group-2, three (42.9%) patients showed bilateral temporal hyperperfusion with unilateral predominance and four (57.1%) revealed insular hyperperfusion of epileptic side. In group-3, 15 patients (88.2%) showed bilateral temporal hyperperfusion with unilateral predominance and 12 (70.6%) insular hyperperfusion. In group-4, 11 patients (84.6%) showed basal ganglia hyperperfusion on the opposite hemisphere to the side of the dystonic posturing. en group-5, there were multiple hyperperfusion areas in the frontal, temporal and basal ganglia regions. However, the injection times of radiotracer in five groups were relatively short and similar. Conclusions: The semiologic progression in TLE seizures were related to the propagation of hyperperfusion from ipsilateral temporal lobe to contralateral temporal lobe, insula, basal ganglia, and frontal lobe. Not only the radiotracer injection time but also semiologic progression after the Injection was significant in determining hyperperfusion pattern of ictal SPECT.

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Feasibility of Using Norad Orbital Elements for Pass Programming and Catalog Generation for High Resolution Satellite Images (고해상도 위성영상 촬영계획 수립 및 카탈로그 생성을 위한 NORAD 궤도 데이터의 이용 가능성 연구)

  • 신동석;김탁곤;곽성희;이영란
    • Korean Journal of Remote Sensing
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    • v.15 no.2
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    • pp.119-130
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    • 1999
  • At present, many ground stations all over the world are using NORAD orbit element data in order to track and communicate with Earth orbiting satellites. The North American Aerospace Defense Command (NORAD) observes thousands of Earth orbiting objects on daily basis and provides their orbital information via internet. The orbital data provided by NORAD, which is also called two line element (TLE) sets, allows ground stations to predict the time-varying positions of satellites accurately enough to communicate with the satellites. In order to complete the mission of a high resolution remote sensing satellite which requires very high positional determination and control accuracy, however, a mission control and tracking ground station is dedicated for the observation and positional determination of the satellite rather than using NORAD orbital sets. In the case of KITSAT-3, NORAD orbital elements are currently used for image acquisition planning and for the processing of acquired images due to the absence of a dedicated KITSAT-3 tracking ground system. In this paper, we tested and analyzed the accuracy of NORAD orbital elements and the appropriate prediction model to determine how accurately a satellite acquisites an image of the location of interest and how accurately a ground processing system can generate the catalog of the images.

Research and Application of Satellite Orbit Simulation for Analysis of Optimal Satellite Images by Disaster Type : Case of Typhoon MITAG (2019) (재난유형별 최적 위성영상 분석을 위한 위성 궤도 시뮬레이션 연구 및 적용 : 태풍 미탁(2019) 사례)

  • So-Mang, LIM;Ki-Mook, KANG;Eui-Ho, HWANG;Wan-Sik, YU
    • Journal of the Korean Association of Geographic Information Studies
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    • v.25 no.4
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    • pp.210-221
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    • 2022
  • In order to promptly respond to disasters, the era of new spaces has opened where satellite images with various characteristics can be used. As the number of satellites in operation at home and abroad increases and the characteristics of satellite sensors vary, it is necessary to find satellite images optimized for disaster types. Disaster types were divided into typhoons, heavy rains, droughts, forest fires, etc., and the optimal satellite images were selected for each type of disaster considering satellite orbits, active/passive sensors, spatial resolution, wavelength bands, and revisit cycles. Each satellite orbit TLE (Two Line Element) information was applied to the SGP4 (Simplified General Perturbations version 4) model to develop a satellite orbit simulation algorithm. The developed algorithm simulated the satellite orbit at 10-second intervals and selected an accurate observation area by considering the angle of incidence of each sensor. The satellite orbit simulation algorithm was applied to the case of Typhoon Mitag in 2019 and compared with the actual satellite list. Through the analyzed results, the time and area of the captured image and the image to be recorded were analyzed within a few seconds to select the optimal satellite image according to the type of disaster. In the future, it is intended to serve as a basis for building a system that can promptly request and secure satellite images in the event of a disaster.

Ag(Ⅰ) Ion Selective Macrocyclic Ligands: The Complexation and Liquid Membrane Transport Phenomena of Benzylated Nitrogen-Oxygen Donor Macrocyclic Ligands (Ag(Ⅰ) 이온 선택성을 갖는 거대고리 리간드: 벤질 치환기를 갖는 질소-산소 주개 거대고리 리간드의 착물 형성과 액체막 이동 현상)

  • Kim, Jeong;Ahn, Tae Ho;Lee, Myoung Ro;Cho, Moon Hwan;Kim, Si Joong
    • Journal of the Korean Chemical Society
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    • v.43 no.2
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    • pp.167-171
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    • 1999
  • An investigation of the interaction of Co(II), Ni(II), Cu(II), Zn(II), Cd(II), Pb(II) and Ag(I) with two N,N'-dibenzylated nitrogen-oxygen mixed donor macrocyclic ligands, has been carried out. Tle log K values for the respective complexes in 95% methanol have been determined potentiometrically. Both ligands have formed stable complex with only Cu(II) and Ag(I) ion. Transport measurements in a bulk liquid membrane system exhibited a very high selectivity of Ag(I) ion over the other metal ions used.

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인공위성 추적을 위한 위성 궤도 계산 프로그램 개발

  • Song, Yong-Jun;Jin, Ho;Kim, Gap-Seong;Lee, Seong-Hwan
    • The Bulletin of The Korean Astronomical Society
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    • v.36 no.2
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    • pp.130.2-130.2
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    • 2011
  • 지상의 관측소에서 특정 인공위성을 찾아내기 위해서는 위성의 정밀궤도 계산이 필요하다. 궤도상의 인공위성의 위치는 시간에 따라 계속 변하므로 이러한 위성의 위치를 실시간으로 추적하기 위해서는 컴퓨터를 이용한 계산이 필수적이다. 정밀한 계산 결과를 얻기 위하여 태양과 지상 관측소의 위치는 Astronomical Almanac과 지구 타원체 모델을 이용하여 계산 하였다. 인공위성의 궤도는 미공군 북미방공사령부(NORAD)에서 발표하는 TLE를 초기값으로 이용하여 J2 섭동효과를 포함한 위성의 위치 및 속도의 변화를 계산하여 SkyView로 나타내었다. 이렇게 나타낸 SkyView의 결과를 실제 위성의 궤적과 비교하여 위성의 궤도를 검증하였으며, 시간에 따른 위성의 광도 곡선 변화 계산 루틴을 작성하여 실제 위성을 찾아내기 위한 기초자료로 활용이 가능하도록 하였다. 모든 계산을 위한 프로그램을 Visual Studio.net 2010 환경에서 C++ 언어를 이용하여 작성하였으며, 결과를 나타내기 위하여 Nokia 사의 Cross Platform 라이브러리인 Qt를 이용하여 UI 제작 및 Visualization을 수행하였다. Qt 라이브러리는 C++ 언어를 기반으로 작성된 플랫폼 독립적인 GUI 라이브러리로써 MS Windows, Linux, MacOS 환경에서 사용이 가능하다. 이를 통해 운영체제에 관계없이 모든 컴퓨터 환경에서 동일한 유저 인터페이스를 이용하여 계산을 할 수 있다. 본 연구는 향후 우주물체탐색에 있어 독자적인 운영을 위한 프로그램으로 활용할 예정이다.

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An effective method for detecting satellite orbital maneuvers and its application to LEO satellites

  • Ashurov, Abdikul E.
    • Advances in aircraft and spacecraft science
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    • v.9 no.4
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    • pp.279-300
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    • 2022
  • This paper analyzes the possibilities of a new method to using TLE data for detecting satellite maneuvers. The method has a number of advantages over other methods that are designed to detect maneuvers. It allows not only to detect maneuvers, but also to get a more complete picture of the maneuver. In particular, the method makes it possible to estimate the moments of the beginning and end of the maneuver, calculate the changes in the orbital elements, evaluate the tangential and binormal components of the impulse, and finally, calculate the impulse of the satellite obtained as a result of the maneuver. To demonstrate in detail the capabilities of the algorithm, the proposed method was applied to one of LEO satellites - TIANHUI-1 satellite. After the efficiency of the method was proved, this method was applied to the China Space Station - TIANHE-1 (CSS), Starlink-1095 and Starlink-2305 satellites. The maneuvers of the CSS and Starlink-1095 satellite during their close encounter on 1 July, 2021, and the CSS and Starlink-2305 satellite during their close encounter on 21 October, 2021 are analyzed in detail. The minimum distances between the CSS and Starlink satellites at the moments of their maximum approaches are estimated. An estimate of the computation time of this algorithm is given, and the possibility of its use for monitoring maneuvers or other anomalous orbital changes of a large number of satellites in near real-time is shown. It is assumed that on the basis of this method, a service for monitoring satellite maneuvers can be created.

Optical Monitoring Strategy for Avoiding Collisions of GEO Satellites with Close Approaching IGSO Objects

  • Choi, Jin;Jo, Jung Hyun;Yim, Hong-Suh;Choi, Young-Jun;Park, Maru;Park, Sun-Youp;Bae, Young-Ho;Roh, Dong-Goo;Cho, Sungki;Park, Young-Sik;Jang, Hyun-Jung;Kim, Ji-Hye;Park, Jang-Hyun
    • Journal of Astronomy and Space Sciences
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    • v.32 no.4
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    • pp.411-417
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    • 2015
  • Several optical monitoring strategies by a ground-based telescope to protect a Geostationary Earth Orbit (GEO) satellite from collisions with close approaching objects were investigated. Geostationary Transfer Orbit (GTO) objects, Inclined GeoSynchronous Orbit (IGSO) objects, and drifted GEO objects forced by natural perturbations are hazardous to operational GEO satellites regarding issues related to close approaches. The status of these objects was analyzed on the basis of their orbital characteristics in Two-Line Element (TLE) data from the Joint Space Operation Center (JSpOC). We confirmed the conjunction probability with all catalogued objects for the domestic operational GEO satellite, Communication, Ocean and Meteorological Satellite (COMS) using the Conjunction Analysis Tools by Analytical Graphics, Inc (AGI). The longitudinal drift rates of GeoSynchronous Orbit (GSO) objects were calculated, with an analytic method and they were confirmed using the Systems Tool Kit by AGI. The required monitoring area was determined from the expected drift duration and inclination of the simulated target. The optical monitoring strategy for the target area was analyzed through the orbit determination accuracy. For this purpose, the close approach of Russian satellite Raduga 1-7 to Korean COMS in 2011 was selected.

ANALYZING ISUAL SPECTROPHOTOMETER DATA USING A TWO-COLOR DIAGRAM METHOD

  • CHEN ALFRED BING-CHIH;CHIANG PO-SHIH;HUANG TIAN-HSIANG;KUO CHENG-LING;WANG SHI-CHUN;SU HAN-TZONG;HSU RUE-RoN;CHANG MING-HUI;CHANG YEOU-SHIN;LIU TIE-YUE;MENDE STEPHEN B.;FREY HARALD U.;FUKUNISHI HIROSHI
    • Journal of The Korean Astronomical Society
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    • v.38 no.2
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    • pp.303-306
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    • 2005
  • Transient luminous events (TLEs; sprites, elves, jets and etc.) are lightning-related optical flashes occurring above thunderstorms. Since the first discovery of sprites in 1989, scientists have learned a great deal about the morphological, spectroscopic and electromagnetic characteristics of TLEs through ground and spacecraft campaigns. However, most of the TLE studies were based on events recorded over US High Plains. To elucidate the possible biasing effects, space-borne observations are needed and have their merits. Imager of sprites and Upper Atmospheric Lightning (ISUAL) on the FORMOSAT-2 satellite is the first instrument to carry out a true global measurement of TLEs from a low- earth orbit. In this short paper, we apply a common astronomical data analysis technique, two-color diagram, on the ISUAL spectrophotometer (SP) data. By choosing appropriated bandpasses and converting the measured flux of TLEs into the unit of magnitude, two-color diagrams of TLEs can be constructed. We demonstrate that two-color diagrams, which were constructed from the narrow-band spectrophotometer data, can be used to classify different types of TLEs and trace their temporal evolution. The amount of reddening due to Earth's atmosphere can also be estimated from two-color diagrams assembled from the broad-band spectrophotometer data.