• 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.

• Journal of Astronomy and Space Sciences
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• v.24 no.4
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• pp.269-274
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• 2007

We established a regional ionospheric model for investigating ionospheric TEC (Total Electron Contents) variations over the Korean Peninsula during major geomagnetic storms. In order to monitor the ionospheric TEC variations, we used nine permanent GPS reference stations uniformly distributed in South Korea operated by the Korea Astronomy and Space Science Institute (KASI). The cubic spline smoothing (CSS) interpolation method was used to analyze the characteristics of the ionospheric TEC variations. It has been found that variations of TEC over the Korean Peninsula increase when a major geomagnetic storm occurred on November 20, 2003. The TEC has increased about one and a half of those averaged quite days at the specific time during a geomagnetic storm. It has been indicated that the KASI GPS-derived TEC has a correlation with the geomagnetic storm indices (eq. Kp and Dst indices).

• Proceedings of the Korean Vacuum Society Conference
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• 1995.06a
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• pp.154-154
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• 1995

The Xu-Tec process is also called the double glow surface alloying technology and is a new method of surface metallurgy which can produce an alloy layers with sp ecial phisical and chemical properties on the surface of common and inexpensive mater ials. Many super alloys and alloy steels, sueh as nickel base alloys, high speed steels and staiinless steels, have been produced by Xu-Tee Process on the surfaces of carbon steels. The depth of the alloy lasyers may vary from several microns up to 300 micr ons with alloying elements in a concentration of few percentage to 100%. World wide patents for Xu-Tec process have been granted in the United states, Canada, United Ki ngdom, Australia and Japan. High performance saw blades have been successfully produced by the Xu-Tee process with much simper processing steps and less cost than bimetal high speed saw blades. A comparison of the cutting times and wear rates of the Xu-Tee blades with the conventional bimetal blades has been made. The Xu-Tee bIases demonstrates sim ilar or better performance than bimetal blades. A Xu-Tec Unit for the commercial pr oduction of Xu-Tec saw blades has been designed and manufactured. This Unit can t reat 10,000 haek saw blades at one time. Three Xu-Tec hack saw blades production I ines have been set up in China. China.

• Journal of Astronomy and Space Sciences
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• v.26 no.2
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• pp.221-228
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• 2009

We estimated the receiver and satellite differential code bias(DCB) based on the ionospheric total electron content(TEC) estimation method. The GPS network which has been operated by the Korea Astronomy and Space Science Institute(KASI) was designed to calculate TEC. The receiver and satellite DCB values were obtained from the weighted least square method with time interval for one hour. The results represented that the receiver DCB values are mostly varying within ${\pm}2m$ meter and are derived comparatively stable within three days. The estimated mean values of the satellite DCB show the maximum and minimum values of 4.09 nano-second(ns), -6.28ns respectively. We could detect great variations of TEC over 9 TECU difference at any time when the DCB sets were applied to TEC estimation.

• Korean Journal of Fisheries and Aquatic Sciences
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• v.26 no.3
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• pp.205-213
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• 1993

The APHA-MPN procedure is the only officially accepted method for classifying shellfish growing areas in U. S. A. The method estimates the levels of fecal coliforms and E. coli, indicators of the sanitary quality of environmental waters. However, the MPN has several disadvantages requiring far more time, labor and expense for assay, as well as providing relatively poor precision. Several membrane filtration procedures have been developed to enumerate these indicators in waters. Of these, the mTEC technique has been shown to provide recoveries of fecal coliforms and E. coli comparable to those of the MPN method. In an abbreviated sanitary survey for Greenwich Bay in Rhode Island, U. S. A., classified as an approved shellfish growing area, the mTEC and conventional MPN methods were again compared for their recoveries of the indicator bacteria. It was found that the recoveries of fecal coliforms and E. coli provided by the mTEC technique are 1.08 and 1.27 times higher than those produced by MPN for water monitoring, respectively, and that the membrane filtration method appears to be a possible alternative to APHA-MPN.

• Clinical and Experimental Pediatrics
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• v.45 no.10
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• pp.1227-1233
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• 2002

Purpose : Several studies have shown that increases of eosinophil markers are common findings of asthma and Mycoplasma pneumoniae infection, and eosinophil markers reflect the clinical stage of asthma. The purpose of this study was to investigate the change of eosinophil markers according to the clinical stage of Mycoplasma pneumonia. Methods : The patient group consisted of 33 outpatient children with Mycoplasma pneumonia. Peripheral blood total eosinophil count(TEC) and serum eosinophilic cationic protein(ECP) level were measured at both acute and recovery stages and were compared between both stages. The patient group was subdivided into the wheezing(n=16) and the nonwheezing group(n=17), and the TECs and the ECPs of one group were compared with those of the other group. The correlation between Mycoplasma antibody titer and the eosinophil markers of acute stage were analyzed. Results : In the whole patient group, the TECs and the ECPs of the acute stage were significantly higher than those of the recovery stage(P=0.018, P=0.005), but there were no differences in the TEC and the ECP between the wheezing and the nonwheezing group. In the wheezing group, there were no significant differences in the TEC and the ECP between acute and recovery stages. There were no correlations between acute stage Mycoplasma antibody titer and the eosinophil markers. Conclusion : Eosinophil markers reflect the clinical stage of Mycoplasma pneumonia and eosinophilic inflammations may continue even after the acute stage in wheezing patients with Mycoplasma pneumonia.

• Journal of the Korea Institute of Information and Communication Engineering
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• v.16 no.10
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• pp.2335-2340
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• 2012

The detector is an uncooled detector system that functions inside the thermoelectric cooler (TEC) equipped with features instead of the cooler. The function of the thermoelectric device to control the temperature of the detector based on a function of temperature to prevent degradation of image quality to perform the role, the latest technology trend by removing the thermoelectric device size, cost a lot of effort to reduce has been studied. In this paper, It would be proposed of the actual test result using real chamber environment of for the best TECless algorithm as to minimize the degradation of image quality and obtain the low price of the uncooled detector.

• Journal of Powder Materials
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• v.2 no.3
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• pp.223-230
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• 1995

The effects of Mn and Co additions up to 0.6 and 2.0 wt% respectively and the amount of cold-rolled reduction on the thermal expansion coefficient (TEC) of powder rolled Fe-Ni Invar strips were investigated. The compacted strips were sintered, homogenized and cold-rolled to the final thickness of 0.8 mm, 0.65 mm and 0.4 mm. All the strips reached full density except the case of 0.8 mm sample which has a very few porosities. The interstitials which are well known to increase TEC were minimized to the level of 10 rpm C,5 and N,0 by the processing. TEC was found to decrease by increasing the cold reduction. The Mn content had little effect on the TEC. But in Fe-Ni-Co system, TEC decreased with Co content up to 0.4 wt% and then increased, yielding the minimum value of $0.2 {\times} 10-6/^{\circ}C$ at 0.4 wt% Co. This value is much lower than that of commercial Invar product. Such effect of Co is considered to be related with the maxiumum spontaneous- magnetostriction effect.

• The Bulletin of The Korean Astronomical Society
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• v.37 no.2
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• pp.125.2-125.2
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• 2012

최근 아태지역 국제민간항공기구는 GPS의 항공이행을 위한 전리층 연구 태스크포스(Ionospheric Study Task Force, ISTF)를 결성하였다. 안전한 GPS 항공이행을 위해서는 지역적 그리고 전지구적 전리층 특성을 파악한 후 이를 기반으로 실시간 전리층 모델이 필요하다. 한국천문연구원은 ISTF의 전리층 변화 특성 분석에 관한 기술분과를 담당하고 있으며 GPS 항공이행 실시간 전리층 모델개발을 위한 아태지역 전리층 분석방법 및 표준규범을 수립하고 있다. 아태지역 전리층 연구에 앞서 우리나라 전리층 특성을 파악하고자 한국천문연구원이 1998년부터 운영 중에 있는 대전 국제 GPS 기준점으로부터 관측된 자료를 이용하여 태양 11년 주기에 해당하는 GPS TEC를 분석하였다. 또한, 해당 기간 동안 우리나라 양/음 전리층 폭풍 발생 빈도에 관한 통계분석을 실시하였다. 본 발표에서는 GPS TEC의 태양 극자외선 플럭스와 10.7 cm 태양전파와의 상관관계 차이점, 연변화 및 계절적 변화 그리고 이에 대한 시간 변화에 대해 보고한다. 또한 GPS TEC의 27일 주기 변화에 특성에 대해 토의하며, 우리나라 상공 전리층 폭풍의 계절적 분포에 대해 논의할 것이다. 끝으로 최근 한국천문연구원 GPS TEC 상시 관측자료에 나타난 태양 및 지자기 폭풍에 따른 전리층 폭풍 사례에 대해 고찰하고 이를 바탕으로 고층대기 연구가 GPS로 대표되는 현업에 적용되는 최근 현황을 소개할 것이다.

• The Bulletin of The Korean Astronomical Society
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• v.32 no.2
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• pp.46.2-46.2
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• 2007