• 대한원격탐사학회지
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• 제19권4호
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• pp.277-284
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• 2003

이온층 구면을 사각형 격자로 분할하여 각 격자에서 총전자수를 추정하는 지역적 GPS 이 온층 모델을 제시한다. 한반도 상공을 위도와 경도 1$^{\circ}$$\times$1$^{\circ}$의 공간해상도를 가진 격자로 구분하고 칼만 필터(Kalman filter)를 이용하여 격자 상의 총전자수를 추정하였다. 이 연구를 위해 한국천문연구원에서 운영하고 있는 전국 규모의 9개 GPS 상시 관측소의 데이터를 이용하였다. 수신된 의사거리 데이터의 측정 잡음을 줄이기 위해 의사거리와 반송파 위상 데이터를 선형 조합한 위상보정 의사거리(phase-leveled pseudorange) 데이터를 새롭게 만들어 사용하였다. 또한 지역적 이온층의 변화에 적합한 태양-지자기 좌표계(solar-geomagnetic reference frame)를 이용하였다. 태양 활동이 비교적 활발하지 않은 때의 경우, 이 연구의 모델은 이온층 활동이 활발한 낮 시간대의 총전자수가 대략 30-45 TECU 정도로 나타났다. 이 모델의 신뢰성을 평가하기 위해 한국천문연구원(Korea Astronomy Observatory, KAO)의 지역적 모델과 Center for Orbit Determination in Europe의 전 지구적 모델에 의한 총전자수를 동일 지역에 대해 비교했을 때 5일 동안 약 4-5 TECU 정도의 RMS 차이를 보였다.

• 한국항해항만학회:학술대회논문집
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• 한국항해항만학회 2006년도 International Symposium on GPS/GNSS Vol.2
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• pp.195-198
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• 2006

One of the major sources of error in precise GPS positioning since the turn-off the Selective Availability(SA) is the ionospheric propagation delay. For the last decades, a lot of the ionospheric researches based on a GPS network have been implemented throughout the world. Especially researches of the ionospheric modeling for Wide Area Argumentation System(WAAS) have been undertaken and published. In mid-latitude regions, typical spatial and temporal variations in ionospheric models delay tend to minimal. The developed ionospheric model calls for a 1.25 degree grid at latitudes and a 2.5 degree grid at longitudes. The precise grid TEC estimated by the inversion technique is also compared with global ionosphere maps(GIMs) which have been provided by several analysis centers(ACs). The results of initial investigations into the suitability of the proposed ionospheric modeling scheme in north-east Asia are presented.

• 한국항해항만학회:학술대회논문집
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• 한국항해항만학회 2006년도 International Symposium on GPS/GNSS Vol.2
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• pp.199-202
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• 2006

One of the major sources of error in precise GPS positioning since the turn-off the Selective Availability(SA) is the ionospheric propagation delay. For the last decades, a lot of the ionospheric researches based on a GPS network have been implemented throughout the world. Especially researches of the ionospheric modeling for Wide Area Argumentation System(WAAS) have been undertaken and published. In mid-latitude regions, typical spatial and temporal variations in ionospheric models delay tend to minimal. The developed ionospheric model calls for a 1.25 degree grid at latitudes and a 2.5 degree grid at longitudes. The precise grid TEC estimated by the inversion technique is also compared with global ionosphere maps(GIMs) which have been provided by several analysis centers(ACs). The results of initial investigations into the suitability of the proposed ionospheric modeling scheme in north-east Asia are presented.

• 천문학회지
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• 제45권2호
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• pp.39-48
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• 2012

We investigate non-LTE effects on the $H_3^+$ level populations to help the analysis of the observed 2 and 3.5 micron $H_3^+$ emissions from the Jovian ionosphere. We begin by constructing a simple three-level model, in order to compute the intensity ratio of the R(3,4) line in the hot band to the Q(1,0) line in the fundamental band, which have been observed in the Jovian auroral regions. We find that non-LTE effects produce only small changes in the intensity ratios for ambient $H_2$ densities less than or equal to $5{\times}10^{11}cm^{-3}$. We then construct two comprehensive models by including all the collisional and radiative transitions between pairs of more than a thousand known $H_3^+$ rovibrational levels with energies less than 10000 $cm^{-1}$. By employing these models, we find that the intensity ratios of the lines in the hot and fundamental bands are affected greatly by non-LTE effects, but the details depend sensitively on the number of collisional and radiative transitions included in the models. Non-LTE effects on the rovibrational population become evident at about the same ambient $H_2$ densities in the comprehensive models as in the three-level model. However, the models show that rotational temperatures derived from the intensities of rotational lines in the ${\nu}_2$ and $2{\nu}_2$ bands may differ significantly from the ambie temperatures in the non-LTE regime. We find that significant non-LTE effects appear near and above the $H_3^+$ peak, and that the kinetic temperatures in the Jovian thermospheric temperatures derived from the observed line ratios in the 2 and 3.5 micron $H_3^+$ emissions are highly model dependent.

• Journal of Astronomy and Space Sciences
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• 제6권1호
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• pp.1-15
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• 1989

Magnetospheic substorm in the magnetotail region is studied numerically by means of a three dimensional MHD code. The analytic solution for the quiet magnetotail is employed as an initial configuration. The localized solar wind is modeled to enter the simulation domain through the boundaries located in the magnetotail lobe region. As a result of the interaction between the solar wind and the magnetosphere, the magnetic field lines are stretched, and the plasma sheet becomes thinner and thinner. When the current driven resistivity is generated, magnetic reconnection is triggered by this resistivity. The resulting plasma jetting is found to be super-magnetosonic. Although the plasmoid formation and its tailward motion is not quite clear as in the two dimensional simulation, which is mainly because of the numerical model chosen for the present simulation, the rarification of the plasmas near the x-point is observed. Field aligned currents are observed in the late expansive stage of the magnetospheric substorm. These field aligned currents flow from the tail toward the ionosphere on the dawn side from the ionosphere to ward the tail on the dusk side, namely in the same sense of the region 1 current. As the field aligned currents develop, it is found that the cross tail current in the earth side midnight section of the magnetic x-point is reduced.

• 대기
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• 제33권1호
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• pp.33-47
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• 2023

In this study, for the application of observation errors to the Korean Integrated Model (KIM) to utilize the Constellation Observing System for Meteorology, Ionosphere & Climate-2 (COSMIC-2) new satellites, the observation errors were diagnosed based on the Desroziers method using the cost function in the process of variational data assimilation. We calculated observation errors for all observational species being utilized for KIM and compared with their relative values. The observation error of the calculated the Global Navigation Satellite System Radio Occultation (GNSS RO) was about six times smaller than that of other satellites. In order to balance with other satellites, we conducted two experiments in which the GNSS RO data expanded by about twice the observation error. The performance of the analysis field was significantly improved in the tropics, where the COSMIC-2 data are more available, and in the Southern Hemisphere, where the influence of GNSS RO data is significantly greater. In particular, the prediction performance of the Southern Hemisphere was improved by doubling the observation error in global region, rather than doubling the COSMIC-2 data only in areas with high density, which seems to have been balanced with other observations.

• 제어로봇시스템학회:학술대회논문집
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• 제어로봇시스템학회 2003년도 ICCAS
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• pp.2382-2386
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• 2003

The Global Positioning System(GPS) is a satellite based precise positioning system avaliable worldwide. The GPS have many error sources. The earth's ionosphere and atmosphere cause delays in the GPS signal that translate into position errors. Some errors can be factored out using mathematics and modeling. The configuration of the satellites in the sky can magnify other errors. The problem of accuracy on GPS measurement data can be meaningful. In this study, we propose the method for GPS positioning accuracy improvement. The FUZZY set theory on PDOP(Position Dilution of Precision) and SNR(Signal to Noise Ratio) provide improved for measured positioning data. The accuracy of positioning has been improved by selecting data from original using the FUZZY set theory on PDOP and SNR.

• Journal of Astronomy and Space Sciences
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• 제28권1호
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• pp.71-77
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• 2011

Ionospheric error modeling is necessary to create reliable global navigation satellite system (GNSS) signals using a GNSS simulator. In this paper we developed algorithms to generate Klobuchar coefficients ${\alpha}_n$, ${\beta}_n$ (n = 1, 2, 3, 4) for a GNSS simulator and verified accuracy of the algorithm. The eight Klobuchar coefficients were extracted from three years of global positioning system broadcast (BRDC) messages provided by International GNSS service from 2006 through 2008 and were fitted with Fourier series. The generated coefficients from our developed algorithms are referred to as Fourier Klobuchar model (FOKM) coefficients, while those coefficients from BRDC massages are named as BRDC coefficients. The correlation coefficient values between FOKM and BRDC were higher than 0.97. We estimated total electron content using the Klobuchar model with FOKM coefficients and compared the result with that from the BRDC model. As a result, the maximum root mean square was 1.6 total electron content unit.

• 한국정보통신학회논문지
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• 제14권10호
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• pp.2223-2229
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• 2010

GPS 위성 고장과 같은 GPS 신호 이상에 대한 무결성 감시 연구가 진행되고 있다. GPS 신호의 이상 발생은 GPS 위성의 고장, 이온층 지연 오차의 급격한 증가, 제어부분의 항법 파라미터에 대한 잘못된 모델링 또는 고의적 이상, 전자파 간섭 등이 있는 것으로 알려져 있다. GPS 위성 고장의 경우 반송파, 코드, 항법메시지의 오류에 의해 이상이 발생할 수 있다. 본 논문에서는 항법메시지에 이상이 있는 상황을 GPS 시뮬레이터를 이용하여 재현하고, 항법메시지 이상이 GPS 수신기에 미치는 영향을 분석하였다. GPS 항법메시지를 구성하는 프리앰블, HOW의 TOW 카운트메시지와 서브프레임의 ID를 나타내는 비트, 위성상태 관련 비트, 그 외의 항법메시지 이상에 대해 정리하고 이를 재현하였으며, 이러한 이상이 GPS 수신기에 미치는 영향을 분석하기 위하여 위성의 개수, DOP, 의사거리를 통해 관찰하였다.

• Journal of Astronomy and Space Sciences
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• 제12권1호
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• pp.123-132
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• 1995

인공위성의 추적자료(시선거리, 시선거리변화율, 방위각, 고도)에 영향을 줄 수 있는 여러가지 요인들을 모델링하여 궤도추적 자료를 추적 안테나에서 받은 실제 자료와 가능한 거의 같게 이론적으로 생성하는 S/W를 개발하였다. 개발한 S/W를 이용하여 광시간 효과와 지구 대기에 의한 추적자료의 지연량을 산출하였다. 대기에 의한 추적자료 지연량들의 변화를 살펴본 결과, 대류층에 의한 지연량은 온도, 상대습도, 압력이 클수록 증가하고, 이온층에 의한 지연량은 최대전자밀로와 주파수에 따라 차이가 나는데, 최대전자 밀도가 증가할수록 지연량은 점점 증가하고, 주파수가 증가할 수록 지연량이 감소함을 알 수 있었다. 또한, 광시간 효과에 의한 추적자료의 지연량은 위성의 고도가 낮을 수록 빠른 궤도운동으로 지연량이 커짐을 알 수 있다.