• Journal of Astronomy and Space Sciences
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• 제38권3호
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• pp.157-164
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• 2021

We describe a method for the in-orbit calibration of body-mounted magnetometers based on the CHAOS-7 geomagnetic field model. The code is designed to find the true calibration parameters autonomously by using only the onboard magnetometer data and the corresponding CHAOS outputs. As the model output and satellite data have different coordinate systems, they are first transformed to a Star Tracker Coordinate (STC). Then, non-linear optimization processes are run to minimize the differences between the CHAOS-7 model and satellite data in the STC. The process finally searches out a suite of calibration parameters that can maximize the model-data agreement. These parameters include the instrument gain, offset, axis orthogonality, and Euler rotation matrices between the magnetometer frame and the STC. To validate the performance of the Python code, we first produce pseudo satellite data by convoluting CHAOS-7 model outputs with a prescribed set of the 'true' calibration parameters. Then, we let the code autonomously undistort the pseudo satellite data through optimization processes, which ultimately track down the initially prescribed calibration parameters. The reconstructed parameters are in good agreement with the prescribed (true) ones, which demonstrates that the code can be used for actual instrument data calibration. This study is performed using Python 3.8.5, NumPy 1.19.2, SciPy 1.6, AstroPy 4.2, SpacePy 0.2.1, and ChaosmagPy 0.5 including the CHAOS-7.6 geomagnetic field model. This code will be utilized for processing NextSat-1 and Small scale magNetospheric and Ionospheric Plasma Experiment (SNIPE) data in the future.

• 천문학회보
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• 제37권1호
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• pp.66.2-66.2
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• 2012

Building a relativistic magnetohydrodynamic (RMHD) code based on upwind scheme is a challenging project, because eigenvalues and eigenvectors are not yet analytically given. Here, we present analytic expressions for eigenvalues and eigenvectors in isothermal flows. And then we show tests performed with a code based on the total variation diminishing (TVD) scheme.

• 대한전자공학회:학술대회논문집
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• 대한전자공학회 2003년도 하계종합학술대회 논문집 I
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• pp.101-104
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• 2003

In this paper, we analyze the performance of transmitter and receiver of W-CDMA system using the space-time code in downlink over JTC realistic channel model. We can get a diversity gain by using the space time code. We also apply the RAKE receiver to improve a performance in multi-path fading channel environment.

• 천문학회보
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• 제37권2호
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• pp.101.1-101.1
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• 2012

Building a relativistic magnetohydrodynamic (RMHD) code based on upwind schemes has been a challenging project, because of the absence of analytic expressions of eigenvalues and eigenvectors. We found analytic expressions of eigenvalues and eigenvectors for adiabatic RMHD flows which are relatively simple and manageable. Especially, our eigenvectors can handle all degenerate points. Using these analytic forms, we built a code based on the total variation diminishing (TVD) scheme, and successfully performed one-dimensional shock tube tests.

• 한국정보통신학회논문지
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• 제10권10호
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• pp.1869-1876
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• 2006

최근에 시공간 부호화(Space-Time Code, STC)는 차세 대 이동 통신에서 고속의 신뢰성 있는 통신을 위 해 각광받고 있다. 본 논문에서는 다중경로 페이딩 채널에서 고속의 데이터를 전송하고자 할 경우에 성능을 향상시키고자 트렐리스 부호화된(Trellis-Coded, TC) 차동 시공간 변조(Differential Space Time Modulation, DSTM)를 사용한 MDPSK에서 다중 심벌 검파 시스템을 제안한다 차동 시공간 부호화된 MDPSK의 성능을 향상시키기 위해 DUSTM(differential unitary space-time modulation)을 이용하여 송신기를 설계하고 수신단에서 다중 심 벌 검파를 수행하는 수신기와 디코딩 알고리듬을 개발하며, 이를 위한 새로운 가지 메트릭을 유도한다.

• 융합신호처리학회논문지
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• 제5권3호
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• pp.223-229
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• 2004

최근에 OFDM과 시공간 부호화(Space-Time Code, STC)는 차세대 이동 통신에서 고속의 신뢰성 있는 통신을 위해 각광받고 있다. 본 논문에서는 다중경로 페이딩 채널에서 고속의 데이터를 전송하고자 할 경우에 성능을 향상시키고자 트렐리스 부호화된(Trellis-Coded, TC) 차동 시공간 변조(Differential Space Time Modulation, DSTM)를 사용한 OFDM에서 다증 심벌 검파 시스템을 제안한다. 차동 시공간 부호화된 OFDM의 성능을 향상시키기 위해 DUSTM(differential unitary space-time modulation)을 이용하여 송신기를 설계하고 수신단에서 다중 심벌 검파를 수행하는 수신기와 디코딩 알고리듬을 개발하며, 이를 위한 새로운 가지 메트릭을 유도한다.

• 한국통신학회논문지
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• 제12권4호
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• pp.347-356
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• 1987

本 論文에서는 高速 光 디지털 傳送시스템과 같은 高速 unipolar 信號 傳送시스템에 適合한 새로운 mBIZ 傳送路符號를 提案하였다. mBIZ符號는 情報信號系列 傳送速度를 $\frac{(m+1)}{m}$ 만큼 速度變換한 後 m 비트마다 補助 서어비스 비트 하나를 揷入한 信號系列과 出力傳送路符號系列의 한 비트를 遲延시킨 信號系列을 Exclusive NOR하여 符號化하기 때문에 redundancy를 줄일 수 있을 뿐만 아니라 復號回路 역시 간단하게 構成할 수 있다. mBIZ符號는 回符號連積數를 (m+1)비트 이내로 抑壓할 수 있으며 傳送路符號系列의 마크率이 1/2이기 때문에 電力 스펙트럼에 存在하는 高低周波 成分들을 抑壓할 수 있다.

• Journal of Astronomy and Space Sciences
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• 제27권2호
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• pp.123-128
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• 2010

This paper analyzes that the global positioning system (GPS) receiver differential code bias (DCB) has effect on the estimation the ionosphere total electron content (TEC). The data from nine permanent GPS sites of the Korea Astronomy and Space Science Institute (KASI) were used for the estimation of the receiver DCB before (Trimble 4000 SSi) and after (Trimble NetRS) the receiver replacement, using the singular value decomposition method. The results showed that the estimated mean value of the receiver DCB varied from 0.11 ns (nanosecond) to 7.54 ns before the receiver replacement, but the receiver DCBs shoed large values than 20 ns except some stations after the replacement. The receiver DCB showed a relatively large difference by types of the receivers, and, as a result, it had a great effect on the estimation the ionosphere TEC using GPS.

• Journal of Positioning, Navigation, and Timing
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• 제12권4호
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• pp.343-348
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• 2023

The ionosphere acts as the largest error source in the Global Navigation Satellite System (GNSS) signal transmission. Ionospheric total electron content (TEC) is also easily affected by changes in the space environment, such as solar activity and geomagnetic storms. In this study, we analyze changes in the regional ionosphere using the Qusai-Zenith Satellite System (QZSS), a regional satellite navigation system. Observations from 9 GNSS stations in South Korea are used for estimating the QZSS TEC. In addition, the performance of QZSS TEC is analyzed with observations from day of year (DOY) 199 to 206, 2023. To verify the performance of our results, we compare the estimated QZSS TEC and CODE Global Ionosphere Map (GIM) at the same location. Our results are in good agreement with the GIM product provided by the CODE over this period, with an averaged difference of approximately 0.1 TECU and a root mean square (RMS) value of 2.89 TECU.

• 대한전자공학회논문지TC
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• 제46권4호
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• pp.64-69
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• 2009

Alamouti 직교 시공간 블록 부호(Orthogonal Space-Time Block Code; OSTBC)에 적용된 BICM(Bit Interleaved Coded Modulation)은 부호율 손실 문제를 가지고 있다. 본 논문에서는 직교 시공간 블록 부호(Orthogonal Space-Time Block Code; OSTBC)를 확장하여 확장된 OSTBC(eXpanded OSTBC; XOSTBC)를 구성하고, 여기에 비트 인터리브 된 부호화 변조(Bit Interleaved Coded Modulation; BICM)을 적용하여 부호율의 손실 없이 다이버시티 이득을 얻도록 하였다. BPSK의 경우에 대한 설계 예제와 이에 대한 모의실험 결과가 제시된다.