• Bulletin of the Korean Space Science Society
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• 2009.10a
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• pp.39.2-39.2
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• 2009

지자기 폭풍이 발생할 동안 중위도 전리권 전자밀도 변화의 가장 큰 특징은 양전리권 폭풍 또는 음전리권 폭풍이다. 양전리층 폭풍은 정상적인 경우보다 전자밀도가 증가하는 것으로 정의되는데 적도방향 중성바람에 의한 극지방 전자밀도의 중위도로의 이동으로 설명된다. 음전리권 폭풍은 F2 층 고도의 O/N2 증가에 의한 전자소멸로 전자밀도가 낮아지는 것으로 알려져 있다. 우리는 지상 GPS 총전자량 자료와 이를 이용한 전리권 토모그래피 모델 결과, 그리고 이온존데 관측에 나타난 한반도 상공의 전리층 폭풍 양상을 제시하고 토의할 것이다.

• Journal of Space Technology and Applications
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• v.4 no.3
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• pp.199-209
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• 2024

In this study, we calculated total electron content (TEC) using ship-borne global navigation satellite system (GNSS) observations and validated the results by comparing the ground-based TEC. GNSS is an effective tool for monitoring the ionosphere as it allows 24-hour observations, is low cost, and is easy to install. However, most GNSS stations are located on land, which leads to a lack of data from the ocean. Therefore, we conducted an experiment collecting GNSS data in the ocean by installing GNSS observation systems aboard the research vessel 'ISABU', operated by the Korea Institute of Ocean Science and Technology. We estimated TEC using GNSS data from July 30 to August 24, 2021. From the results, we confirmed daily and latitudinal variations of TEC as expected. Additionally, we compared the results with TEC derived from nearby ground-based GNSS stations and then verified similar variations. Based on these results, we plan to research ionospheric climatology using long-term data and assess its potential for ongoing ionospheric monitoring.

• Journal of Space Technology and Applications
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• v.4 no.3
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• pp.210-219
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• 2024

This study investigates various ionospheric and thermospheric disturbances around the Korean Peninsula during the G5 geomagnetic storm occurred on May 10, 2024. This level of storm was the first of its magnitude in 21 years, resulting in auroras visible even in South Korea and severe space weather worldwide. The Korea Astronomy and Space Science Institute has been providing ionospheric information over Korea through total electron content (TEC) measurements from the Global Navigation Satellite System (GNSS) and monitoring the impact of ionospheric disturbances on GNSS signals by operating five GNSS scintillation stations in Korea and other countries. During this storm period, large amplitudes of TEC variations were observed over South Korea, along with anomalous TEC enhancements accompanied by strong scintillations at night and persistent TEC depletion on the dayside during the storm's recovery phase. Such daytime TEC depletion disturbances are quite rare, typically occurring only a few times throughout the 11-year solar cycle. While the association of persistent TEC depletion during the daytime with neutral composition disturbances was identified through observations, the causes of TEC enhancement and strong scintillation at night remain unclear. We speculate that the uplift of the ionosphere by storm-induced electric fields is responsible for the TEC enhancement and scintillation, but this hypothesis requires validation based on additional observational data.

• Journal of Positioning, Navigation, and Timing
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• v.13 no.1
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• pp.63-73
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• 2024

NeQuick G is the ionosphere model utilized by Galileo single-frequency users to estimate the ionospheric delay on each user-satellite link. The model is characterized by the effective ionization level (Az) index, determined by a modified dip latitude (MODIP) and broadcast coefficients derived from daily global space weather observations. However, globally fitted Az coefficients may not accurately represent ionosphere within local area. This study introduces a method for regional ionospheric modeling that searches for locally optimized Az coefficients. This approach involves fitting TEC output from NeQuick G to TEC data collected from GNSS stations around Korea under various ionospheric conditions including different seasons and both low and high solar activity phases. The optimized Az coefficients enable calculation of the Az index at any position within a region of interest, accounting for the spatial variability of the Az index in a polynomial function of MODIP. The results reveal reduced TEC estimation errors, particularly during high solar activity, with a maximum reduction in the RMS error by 85.95%. This indicates that the proposed method for NeQuick G can effectively model various ionospheric conditions in local areas, offering potential applications in GNSS performance analyses for local areas by generating various ionospheric scenarios.