• 제목/요약/키워드: line-of-sight

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Location Error Compensation in indoor environment by using MST-based Topology Control (MST 토폴로지를 이용한 실내 환경에서의 위치측정에러의 보상기법)

  • Jeon, Jong-Hyeok;Kwon, Young-Goo
    • Journal of the Korea Institute of Information and Communication Engineering
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    • v.17 no.8
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    • pp.1926-1933
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    • 2013
  • Many localization algorithms have been proposed for Wireless Sensor Networks (WSNs). The IEEE 802.15.4a-based location-aware-system can provide precise ranging distance between two mobile nodes. The mobile nodes can obtain their exact locations by using accurate ranging distances. However, the indoor environments contain various obstacles which cause non-line-of-sight (NLOS) conditions. In NLOS condition, the IEEE 802.15.4a-based location-aware system has a large scale location error. To solve the problem, we propose location error compensation in indoor environment by using MST-based topology control. Experimental and simulation results show that the proposed algorithm improves location accuracy in NLOS conditions.

Line-of-Sight Rate for Off-axis Seeker on a 2-axis Gimbal (2축 김발 위에 장착된 비축탐색기를 위한 시선각속도 계산)

  • Kim, Jeong-Hun;Park, Kuk-Kwon;Ryoo, Chang-Kyung
    • Journal of the Korean Society for Aeronautical & Space Sciences
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    • v.47 no.3
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    • pp.187-194
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    • 2019
  • The off-axis Infra-Red(IR) seeker is mounted on the nose cone side of the anti-air high speed missile to alleviate thermal shield effect due to aerodynamic heating. The seeker output can not be regarded as the Line-of-Sight(LOS) rate any more as missile's roll motion to keep the target tracking is associated. In this paper, we propose a method to calculate the LOS rate for off-axis seeker on a 2-axis gimbal. Firstly, true LOS rate equations are analytically derived but not implementable because boresight error rate is not measurable. And then the first order lag approximation to obtain boresight error rate is proposed. The proposed LOS rate calculation method can compensate the coupling effect by considering the rotations of missile and gimbal. The performance of the proposed method is verified via full nonlinear 6-DOF(Degree of Freedom) simulations.

Performance analysis of UWB receiver using PPM and BPSK modulation scheme in the LR-WPAN System (LR-WPAN 시스템에서 PPM+BPSK 변조 방식을 사용하는 UWB 송수신기의 성능 분석)

  • Lee, Kyoung-Tak;Lim, Dong-Guk;Sohn, Sung-Hwan;Kim, Jae-Moung
    • The Journal of The Korea Institute of Intelligent Transport Systems
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    • v.5 no.2 s.10
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    • pp.19-28
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    • 2006
  • In the IEEE 802.15.4a system, they require simple, economical and low power consumption transmitter and receiver to transmit low rate data and to identify distance and location. To meet these requirements, LR-WPAN system use transmitter and receiver with simple modulation and demodulation scheme. In this paper, use PPM+BPSK modulation and windowing scheme to overcome multipath fading effect. Then we apply this channel estimation scheme to LR-WPAN system and compare performance depends on transmitter scheme. Proposed method using preamble to find channel characteristic out and we compensate distorted data with that information. Therefore we can detect signal easily at the demodulation part. Simulation result shows that performance evaluation is greater at the NLOS channel than LOS channel no matter what the receiver scheme.

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DGNSS-CP Performance Comparison of Each Observation Matrix Calculation Method (관측 행렬 산출 기법 별 DGNSS-CP 성능 비교)

  • Shin, Dong-hyun;Lim, Cheol-soon;Seok, Hyo-jeong;Yoon, Dong-hwan;Park, Byungwoon
    • Journal of Advanced Navigation Technology
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    • v.20 no.5
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    • pp.433-439
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    • 2016
  • Several low-cost global navigation satellite system (GNSS) receivers do not support general range-domain correction, and DGNSS-CP (differential GNSS) method had been suggested to solve this problem. It improves its position accuracy by projecting range-domain corrections to the position-domain and then differentiating the stand-alone position by the projected correction. To project the range-domain correction, line-of-sight vectors from the receiver to each satellite should be calculated. The line-of-sight vectors can be obtained from GNSS broadcast ephemeris data or satellite direction information, and this paper shows positioning performance for the two methods. Stand-alone positioning result provided from Septentrio PolaRx4 Pro receiver was used to show the difference. The satellite direction information can reduce the computing load for the DGNSS-CP by 1/15, even though its root mean square(RMS) of position error is bigger than that of ephemeris data by 0.1m.

A Studyu on the Waveguide Running Condition Inspection of Radar (레이다 도파관의 작동상태점검법에 관한 연구)

  • 류대근
    • Journal of the Korean Institute of Navigation
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    • v.5 no.2
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    • pp.41-47
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    • 1981
  • Many new radar techniques have appeared on the electronic scene in recent years, such as a variety of automatic computer processing. However, even with the advent of these sophisticated radar techniques, an old problem continues to plague all radars: the problem of transmission line losses. With the higher performance required today, the Waveguide testing and trouble-shooting techniques remain essentially unchanged in principle. This paper dealt with the rf pulse "Time-domain Reflectometry" to inspect radar wave-guide system and compared with the conventional methods. During the investigation, it was verified that the pulsed TDR for wave-guide is superior to the conventional methods; 1. Disassembling is not needed to locate the discontinity points and measure the reflections of trobled points. 2. The results of the data are more precise. 3. The condition of individual component is able to the photographed and recorded permanently. 4. Since rf pulse TDR is based on the well-known basic radar principle, such a test set requires the minimum of training to operate. With the level of transmission line problems, the prospect of increasing complexity of equipment, and no relief in sight, the benifits must be emphasizied to adopt such a testing procedure.procedure.

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The Vertical Deviation of the Impact Point from and Aiming Point at an Inclined shooting Ranges (소총의 상하향 사격시 탄도학상의 수직편차)

  • ;;Chang, Won Hong
    • Transactions of the Korean Society of Mechanical Engineers
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    • v.2 no.2
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    • pp.47-51
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    • 1978
  • In order to improve the hitting rate in the shot of rifles, it is required that the analysis of exterior ballistics and the line of sight. One of the important factors influenced a marksman using a rifle obtained the zero-setting of a rifle at the horizontal range, is the deviation of the impact point from the aiming point when the shooting is performed in an inclined ranges. The deviation usually cccurs from the reaction force along the bore line, the characteristics of exterior ballistics, and the error of a shooting range judgement by the inclined range. This study is concerned with the problem of the vertical difference between the impact and aiming point in the inclined shooting ranges. The computing method to find the vertical difference is represented. This method is applied for and experimental rifle in three cases, (1) hofizontal shooting ranges, (2) upper inclined shooting ranges, and (3) lower inclined shooting ranges.

Revisiting the virial factor with the updated $M_{BH}-{\sigma}_*$ relation

  • Park, Dae-Seong;Woo, Jong-Hak
    • The Bulletin of The Korean Astronomical Society
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    • v.37 no.1
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    • pp.35.1-35.1
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    • 2012
  • Determining the virial factor of the broad-line region (BLR) gas is crucial in calibrating AGN black hole mass estimators, since the measured line-of-sight velocity needs to be converted into the representative velocity of the BLR gas. The unknown virial factor has been empirically calibrated based on the $M_{BH}-{\sigma}_*$ relation of non-AGN galaxies, but the claimed values are different by a factor of 2 in recent studies. We investigate the origin of the difference by measuring the $M_{BH}-{\sigma}_*$ relation using the most updated nearby galaxy sample, and explore the dependence of the virial factor on the various fitting methods. We find that the discrepancy is mostly caused by the sample bias while the difference stemming from various regression methods is marginal. Based on the best-determined virial factor, we present the updated $M_{BH}-{\sigma}_*$ relation of local active galaxies.

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Temperature Distribution Measurement of High-pressure Mercury Lamp using Spectroscopic Method (분광 분석법에 의한 고압 수은등의 온도분포 측정)

  • 김상용;김창섭;지철근
    • Proceedings of the Korean Institute of IIIuminating and Electrical Installation Engineers Conference
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    • 1989.10a
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    • pp.13-18
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    • 1989
  • Temperature distribution of 250W high-pressure mercury lamp has been measured by the spectroscopic method using relative intensities of spectral lines. To obtain radial temperature distribution, the measured intensity which was integrated along the line of sight was transformed into radial line intensity by Abel's inversion. Temperature was determined from relative intensities of spectral lines of the same atomic species. The measured temperature of 250W high-pressure mercury lamp is 6000K at the axis. In this experiment temperature profile of high-pressure arc is papabolic as known.

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A Study on the Spatial Factors in Traditional Retail Market Remodeling (재래시장 리모델링 사업에서의 공간 구성요소에 관한 연구)

  • Oh, Bong-Seok;Kim, Nam-Hyo
    • Proceedings of the Korean Institute of Interior Design Conference
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    • 2004.05a
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    • pp.112-115
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    • 2004
  • The government is in progress the traditional retail market redevelopment and remodeling due to atrophy of the traditional retail market in accordant to opening of the circulation market and changing of the consuming patterns. However, it seemed that primitive project was limited to the environment improvement scope. As the shopping environment which is comfortable to the consumers is provided and the design which considers a traditional retail market specific quality is applied from business plan early. It will be useful for the management normalization of traditional retail market actually. The spatial factors were analyzed as follows. 1. The circulation of consumer should be secured to make boundary line of the pass way. 2. The display booth should be standardized for the security of sight. 3. The signage panel should be consolidated in according to the plan. 4. The street vendor's handcart and tent should be arranged for circulations and the vision line.

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A pilot study of the two OB associations Cygnus OB2 and Carina OB1 using the Gaia data

  • Lim, Beomdu;Naze, Yael;Gosset, Eric;Rauw, Gregor
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.1
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    • pp.47.2-47.2
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    • 2019
  • We present a kinematic study of the two young OB associations Cygnus OB2 and Carina OB1 using the recently released Gaia astrometric data. The unimodal distributions of parallaxes of stars indicate that these associations are real stellar systems, rather than line-of-sight coincidences. The associations are found to comprise dense star clusters and a sparse halo which have different proper motions. Clusters have small spatial sizes with small dispersions in proper motion, while the haloes extending to tens of parsecs have a large dispersion in proper motion. We speculate that this aspect is related to that found in molecular clouds, the so-called "line width-size" relation. In this talk, the formation process of these associations is discussed, based on our findings.

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