• Journal of Astronomy and Space Sciences
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• 제39권1호
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• pp.11-22
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• 2022

It is suggested that magnetosonic waves (also known as equatorial noise) can scatter radiation belt electrons in the Earth's magnetosphere. Therefore, it is important to understand the global distribution of these waves between the proton cyclotron frequency and the lower hybrid resonance frequency. In this study, we developed an empirical model for estimating the global distribution of magnetosonic wave amplitudes and wave normal angles. The model is based on the entire mission period (approximately 2012-2019) of observations of Van Allen Probes A and B as a function of the distance from the Earth (denoted by L^*), magnetic local time (MLT), magnetic latitude (λ), and geomagnetic activity (denoted by the Kp index). In previous studies the wave distribution inside and outside the plasmasphere were separately investigated and modeled. Our model, on the other hand, identifies the wave distribution along with the ambient plasma environment-defined by the ratio of the plasma frequency (f_pe) to the electron cyclotron frequency (f_ce)-without separately determining the wave distribution according to the plasmapause location. The model results show that, as Kp increases, the dayside wave amplitude in the equatorial region intensifies. It thereby propagates the intense region towards the wider MLT and inward to L^* < 4. In contrast, the f_pe/f_ce ratio decreases with increasing Kp for all regions. Nevertheless, the decreasing aspect differs between regions above and below L^* = 4. This finding implies that the particle energy and pitch angle that magnetosonic waves can effectively scatter vary depending on the locations and geomagnetic activity. Our model agrees with the statistically observed wave distribution and ambient plasma environment with a coefficient of determination of > 0.9. The model is valid in all MLTs, 2 ≤ L^* < 6, |λ| < 20°, and Kp ≤ 6.

• 대한본초학회지
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• 제28권3호
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• pp.61-68
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• 2013

Objectives : A precise and simple system of nomenclature was required to avoid error, ambiguity or confusion. Although medicinal plants must be produced or distributed based on a pharmacopoeia described origin including scientific name, the Korean Pharmacopoeia tenth edition (KP 10) had many names against the nomenclature. Therefore, this study aimed at searching correct scientific names for 241 plants in KP 10. Methods : Authoritative databases - The Plant List, International Plant Name Index, YList, Tropicos, eFloras, World Checklist of Selected Plant Families, The Global Compositae Checklist, The International Legume Database and Information Service, et al. - and previously performed researches, floras were cross-checked. Results : The arrangement of this list was designed for four cases, errors including illegitimate, nomenclatural synonyms, recommended names and decision reserved names. Consideration about the scientific names produced nine correct names for ten misspellings and illegitimate, and thirty-six correct names for forty-one nomenclatural synonyms. These results should be reflected in the next of KP 10. Separately, ten recommended names were also suggested for taxonomic synonyms which had been used indiscriminately due to diverse taxonomic opinions. In addition to those, decision reserved names were suggested for thirteen species which had been corridor of uncertainty. Then again, there was need to study about authorship, because KP 10 did not keep recommendations for author citations. Conclusions : Correction of scientific names for some medicinal plants which violated the International Code of Nomenclature would be useful to improve the accuracy of a Pharmacopoeia as the criterional materials.

• 지구물리와물리탐사
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• 제13권3호
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• pp.249-255
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• 2010

1990년대 이후 지진발생과 관련된 ULF 대역 지사가장의 변동이 다수 보고된 후, 분석 분석 방법을 이용한 지자기장 분석은 단기 지진예측에 큰 기여를 할 것이라 기대되고 있다. 본 연구는 기존 연구를 참조하여 개량된 분극 분석 방법을 개발하고, 이를 이용하여 청양관측소의 지자기 삼성분 자료를 분석하였다. 분석 주파수는 지진발생에 가장 민감하다고 알려진 0.01 Hz 대역이며, 수직 자기장과 수평 자기장의 분광에너지 비, 즉 분극값을 일단위로 계산하였다. 총 10개 월 동안의 사료가 분석되었으며, 분석경과를 Kp 인덱스 및 동일기간 발생한 지진이벤트와 비교하였나 청양의 분극값 변동은 Kp 인덱스와 관련성이 적었으며, 두 기간에서 지진발생과 관련한 주목할 만한 분극값의 증가가 관찰되었다. 일본 Kanoya 관측소의 자료와 비교해 본 결과, 청양의 분극값 증가는 광역적인 자기장의 변동에서는 지진발생과 밀접한 관계가 있는 것으로 생각된다. 또한, 자기장의 통계적 특성을 고려한 정규화된 분극값의 변동에서는 이러한 특징이 보다 뚜렷하게 확인된다. 따라서 분극 분석 방법은 지진전조형상 모니터링을 위해 유용하게 활용됨 수 있으며, 향후 추가적인 자료 확보 및 분석을 통해 지진발생과 관련된 ULF 변동을 탐지하는데 큰 기여를 할 수 있을 것으로 기대된다.

• Journal of Oral Medicine and Pain
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• 제6권1호
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• pp.15-18
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• 1981

The author had selected the roots and root-canal as measurable parts and sought the area ratio by measuring the respective areas of the root. Further, heplotted out a root caual index and studied the correlation with age. The teeth used as reserch material were permanent maxillary central incisors of Korean female. Some 296 teeth of known age were selected on condition that there is no caries or filling material and that they were not malformed in showing normal signs in roentgenograms. The $3" {\times} 4"$ printing paper so as to measure easily. On the ocassion of measureing the area of measured parts with a planimeter (Koizumi, type kp-27, Japan), the cervical lines were joined up into a straight line on a photograph (Figure 1) Root canal index = Area of the root / Area of the root canal The results of the root canal index in Korean female age groups were as follows : 1. The root canal index of maxilary central incisor in women was 4.74 im 20 years of age, 5.44 in 30, 5.90 in 40, 6.32 in 50, 6.63 in 60 in the order. 2. Root canal index and age were in positive correlation ; there was a tendency that the root canal index increase as age advances. 3. The regression equation was as follows : Y = 5.36x + 7.71 (r = 0.54, n= 296 ) (Y = estimated age, x = root canal index)

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2004년도 한국우주과학회보 제13권1호
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• pp.86-86
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• 2004

다목적 실용위성 1호의 데이터를 이용하여 관측기간인 2000년 6월 28일에서 2001년 8월1일까지의 고도 685km, 22:50LT(Local Time) 이온층을 조사하였다. 데이터는 이온층 측정 센서(Ionospheric Measurement Sensor)로부터 얻은 전자 온도와 전자 밀도를 이용하였으며, 자기 위도로 -60$^{\circ}$-+60$^{\circ}$ 사이의 중ㆍ저위도의 값을 분석하였다. 관측 기간은 지자기 변화를 나타내는 Kp index나 태양 활동을 나타내는 F10.7이 크게 변화한 태양 극대기 기간으로, 이중 일변화의 F10.7을 통해 전자 온도와 전자 밀도의 변화를 조사하였다. (중략)

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2005년도 한국우주과학회보 제14권2호
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• pp.33-33
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• 2005

• Journal of Astronomy and Space Sciences
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• 제19권2호
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• pp.133-140
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• 2002

다목적 실용 위성 1호는 1999년에 발사되어 운용되고 있으며 , 과학 탑재체로 우주과학센서(Space Physics Sensor)를 탑재하고 있다. 이중 SPS IMS는 2000년 6월부터 2001년 8월에 이르는 태양 활동 극대기 동안 지구 이온층에 관한 정보를 지상으로 전송하였다. 다목적 실용위성 1호가 적도지 역을 통과할 때 전자 밀도가 급격 히 감소하는 플라즈마 밀도 불균일 현상(equatorial bubble)이 자주 관측되었다. SPS IMS가 운용된 기간 동안의 데이터를 통계적으로 분석 한 결과, equatorial bubble 현상은 지구 자기장의 크기가 약한 대서양 지역에서 자주 일어났고, 또한 Kp 간이 낮을 때에 더욱 빈번하게 발생하였다. 이는 기존의 DMSP위성을 통한 관측 결과 및 페루 지역의 라디오 관측 결과 등과 상당한 수준의 일치를 보이고 있다. 밀도 불균일 지역 내의 전자 온도 변화는 전자 밀도 변화와 다양한 상관 관계를 나타낸다.

• Bulletin of the Korean Chemical Society
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• 제33권11호
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• pp.3755-3760
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• 2012

Single crystals of lithium potassium phthalate (LiKP) were successfully grown from aqueous solution by solvent evaporation technique. The grown crystals were characterized by single crystal X-ray diffraction. The lithium potassium phthalate $C_{16}\;H_{12}\;K\;Li_3\;O_{11}$ belongs to triclinic system with the following unit-cell dimensions at 298(2) K;$a=7.405(5){\AA}$;$b=9.878(5){\AA}$;$c=13.396(5){\AA}$;${\alpha}=71.778(5)^{\circ}$;${\beta}=87.300(5)^{\circ}$;${\gamma}=85.405(5)^{\circ}$; having a space group P1. Mass spectrometric analysis provides the molecular weight of the compound and possible ways of fragmentations occurs in the compound. Thermal stability of the crystal was also studied by both simultaneous TGA/DTA analyses. The UV-Vis-NIR spectrum shows a good transparency in the whole of Visible and as well as in the near IR range. Third order nonlinear optical studies have also been studied by Z-scan technique. Nonlinear absorption and nonlinear refractive index were found out and the third order bulk susceptibility of compound was also estimated. The results have been discussed in detail.

• 천문학회보
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• 제35권1호
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• pp.30.2-30.2
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• 2010

Numerous operational anomalies and satellite failures have been reported since the beginnings of the "space age". Space weather effects on modern spacecraft systems have been emphasized more and more as increasing their complexity and capability. Energetic particles potentially can destroy and degrade electronic components in satellites. We analyzed the geostationary (GEO) satellite anomalies during 1997-2009 to search possible influences of space weather on the satellite anomalies like power problem, control processor problem, attitude control problem, etc. For this we use particle data from GOES and LANL satellites to investigate space weather effects on the GEO satellites' anomalies depending on Kp index, local time, seasonal variation, and high-energy electron contribution. As results, we obtained following results: (1) there is a good correlation between geomagnetic index(Kp) and anomaly occurrences of the GEO satellite; (2) especially during the solar minimum, occurrence of the satellite anomalies are related to electron flux increase due to high speed solar wind; (3) satellite anomalies occurred more preferentially in the midnight and dawn sector than noon and dusk sector; (4) and the anomalies occurred twice more in Spring and Fall than Summer and Winter; (5) the electron with the lowest energy channel (50-75keV) has the highest correlation (cc=0.758) with the anomalies. High association between the anomalies and the low energy electrons could be understand by the facts that electron fluxes in the spring and fall are stronger than those in the summer and winter, and low-energy electron flux is more concentrated in the dawn sector where the GEO satellite anomalies occurred more frequently than high-energy electron flux. While we could not identify what cause such local time dependences, our results shows that low-energy electrons (~100keV) could be main source of the satellite anomaly, which should be carefully taken into account of operating satellites.

• 한국농공학회논문집
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• 제54권2호
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• pp.127-135
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• 2012

The processes of chemical and physical weathering occur simultaneously. The objective of this study was to estimate the degree weathered using fractal dimension through comparison with chemical characteristic of soil samples from Pohang (PH) and Kimpo (KP). Comparing chemical characteristics with fractal dimension, $SiO_2$, $Na_2O$, $K_2O$ content decreased and loss of ignition increased as fractal dimension increased. And fractal dimension showed high correlation with CWI while ATI, STI CIW, PI, CIA and RR demonstrated different degrees of correlation with fractal dimension. The tendency of the changes in oxide content and chemical weathering index with increasing fractal dimension appeared to be similar with the chemical changes due to weathering. Therefore, fractal dimension could be a good indicator representing the extent of weathering and chemical changes.