• Journal of Astronomy and Space Sciences
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• 제17권2호
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• pp.317-328
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• 2000

The solar wind contributes to the formation of unique space environment called the Earth's magnetosphere by various interactions with the Earth's magnetic field. Thus the solar-terrestrial environment affects the Earth's magnetic field, which can be observed with an instrument for the magnetic field measurement, the magnetometer usually mounted on the rocket and the satellite and based on the ground observatory. The magnetometer is a useful instrument for the spacecraft attitude control as well as the Earth's magnetic field measurements for the spacecraft purpose. In this paper, we present the preliminary design and test results of the two onboard magnetometers of KARI's (Korea Aerospace Research Institute) sounding rocket, KSR-3, which will be launched four times during the period of 2001-02. The KSR-3 magnetometers consist of the fluxgate magnetometer, MAG/AIM (Attitude Information Magnetometer) for acquiring the rocket flight attitude information, and of the search-coil magnetometer, MAG/SIM (Scientific Investigation Magnetometer) for the observation of the Earth's magnetic field fluctuations. With the MAG/AIM, the 3-axis attitude information can be acquired by the comparison of the resulting dc magnetic vector field with the IGRF (International Geomagnetic Reference Field). The Earth's magnetic field fluctuations ranging from 10 to 1,000 Hz can also be observed with the MAG/SIM measurement.

• 대한핵의학회지
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• 제29권1호
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• pp.79-83
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• 1995

정상기능 이식신장 50예와 비정상기능 이식신장 7예의 $^{99m}Tc-MAG_3$를 이용한 신장스캔에서 EI를 구하여 이식신장의 배설기능을 정량적으로 측정하였다. 이식신장의 $^{99m}Tc-MAG_3$ 신장기능곡선에서 정상기능 이식신장의 평균 EI는 $2.21{\pm}0.51$이었으며, 95% 신뢰구간은 2.01-2.87이었다. 비정상기능 이식신장에서는 평균 EI가 $0.74{\pm}0.18$로 1이하의 수치를 보여, 이식신장의 간질에 임파구의 침윤이나 세뇨관의 괴사등에 의해 관류와 배설기능의 장애를 초래하여 신실질과 수집관내에 방사능 동위원소의 저류가 나타났음을 뜻한다. 그리고 EI, $T_{max}$, $T_{1/2}$, BUN, 혈청 Creatinine의 정상기능 이식신장군과 비정상기능 이식신장군의 비교에서 통계학적으로 유의한 차이가 있었다(p<0.0001). 그러므로 이식 후 EI의 측정으로 이식신장의 기능상태를 알 수 있고 거부반응 및 신세뇨관 괴사 등의 합병증을 조기에 찾아내는 지표로 사용할 수 있을 것으로 사료된다.

• Journal of Magnetics
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• 제7권3호
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• pp.115-125
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• 2002

We proposed a novel method to evaluate the magnetic properties of the initial layer and the columnar structure separately for CoCr-based perpendicular recording media. We show that the thickness of the initial layer and the intrinsic magnetocrystalline anisotropy of columnar structure can be quantitatively evaluated using the plotted product of perpendicular anisotropy to magnetic film thickness versus magnetic film thickness ($K_{u{\bot}}^{ex{p.}}$ $\times$ d$_{mag.}$ vs. d$_{mag.}$ plot). Based on the analyses, it is found that: (1) compared with CoCrPtTa media, CoCrPtB media have relatively thin initial layer, and have fine grains with homogeneous columnar structure with c-plane crystallographic orientation; (2) CoCrPtB media can be grown epitaxially on Ru or CoCr/C intermediate layer, and as the result, the magnetic properties of the media within thin thickness region of d$_{mag.}$ $\leq$ 20 nm is significantly improved; (3) the key issue of material investigation for CoCr-based perpendicular recording media will be focused on how to fabricate c-plane-oriented columnar grains well isolated with nonmagnetic substance in epitaxial-growth media, while maintaining the thermal stability of the media.

• 정보처리학회논문지C
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• 제19C권3호
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• pp.191-208
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• 2012

PMIPv6(Proxy Mobile IPv6)는 MN(Mobile Node)의 이동성을 지원하기 위한 망 기반의 이동성관리 기술이다. PMIPv6의 구성 요소는 네트워크 기반 이동성 지원 프로토콜로서 도메인을 관리하는 LMA(Local Mobility Anchor)와 MN의 이동을 감지하고 MN의 위치 정보를 등록하는 MAG(Mobile Access Gateway) 그리고 MN으로 구성되어 있다. PMIPv6는 LMA와 MAG 사이의 터널을 형성하고 패킷이 LMA를 통하여 전달되도록 설계하여, LMA 병목현상 및 종단 간 지연이 증가하는 문제점이 있다. 이러한 문제점을 해결하기 위해 경로 최적화 수행 가능 감지, 경로 최적화 절차 등의 많은 연구가 진행되고 있으나 추가적인 시그널링으로 인한 오버헤드가 증가하고 다중 LMA 환경에 적용하기에 어려움이 있다. 따라서 본 논문에서는 다중 LMA 환경을 고려한 PMIPv6 기반의 향상된 경로 최적화 방안을 제안한다. PMIPv6 도메인의 모든 LMA는 PIG(Proxy Internetworking Gateway)에 연결되어 PMIPv6 도메인 간 분산 이동성 제어를 수행한다. PMIPv6 도메인 내 모든 LMA의 정보를 MAG가 유지하도록 하여 신속하게 경로 최적화를 수행하도록 하였으며, LMA에 경로 최적화 상태 정보를 PIG로부터 수신 받아 저장하여 추가적인 시그널링없이 경로 최적화를 지원하도록 한다.

• 한국환경성돌연변이발암원학회지
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• 제21권1호
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• pp.1-8
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• 2001

We have synthesized $^{99m}$Tc-mercaptoacetyltriglycine (MAG3)-biocytin as a new imaging agent for hepatobiliary scintigraphy. The aim of this study was to evaluate the usefulness of $^{99m}$Tc-MAG3-biocytin scintigraphy in differentiating carbon tetrachloride ( $CCl_4$)-induced hepatotoxicity from $\alpha$-naphthylisothiocyanate (ANIT)-induced cholestasis in mice, which reflecting the differential diagnosis of neonatal jaundice caused by neonatal hepatitis from congenital biliary atresia in humans. Methods: Balb/c mice (female, 20 g, n=4-6) were pretreated with $CCl_4$(0.5 or $1.0m\ell$/kg) and ANIT ($150 or 300 m\ell$/kg) 18 h before scintigraphy. Biochemical and histopathological examinations showed a pattern of typical acute hepatitis (increase of transaminases and hepatocellular necnsis) in $CCl_4$-treated mice and cholestasis (increase of alkaline phosphatase and ${\gamma}$-glutamyltransferase, and biliary hyperplasia) in ANIT-treated mice, respectively, Mice were fasted at least 4 hr prior to the intravenous injection of $^{99m}$Tc-MAG3-biocytin (18.5 MBq/20$\mu\textrm{g}$) in 2% human serum albumin in saline. Scintigraphy was performed with a ${\gamma}$-camera equipped with a 1-mm diameter pin-hole collimator for 30 min and images were acquired every 15 s. We compared the values of physical parameters, such as peak liver/heart ratio ($${\gamma}$_{max}$) and peak ratio time ($t_{max}$) far $^{99m}$Tc-MAG3-biocytin scintigraphy. Results: Scintigraphic parameters of the $CCl_4$-pretreated (0.5 $m\ell$/kg) group showed a 81.9% decrease of r$_{max}$, and 42.2% decrease of $t_{max}$, whereas the ANIT-pretreated ( $150m\ell$/kg) group showed a 53% decrease of $r_{max}$, and 2.36-fold increase of $t_{max}$, (P<0.05). These results demonstrate that the decrease of $r_{max}$ and the shortening of $t_{max}$ are characteristic features for hepatotoxicity, in contrast to the increase of $t_{max}$ and decrease of $r_{max}$ for biliary hyperplasia. Conclusion: $^{99m}$Tc-MAG3-biocytin hepatobiliary scintigraphy can distinguish hepatitis from cholestasis in mice model and may be similarly useful in humans which differentiating the cause of neonatal jaundice in clinical study.cal study.cal study.cal study.

• 천문학회지
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• 제38권3호
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• pp.345-355
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• 2005

We present a photometric study of the star cluster system in the merging galaxy NGC 1487, based on the BI photometry obtained from the F450W and F814W images in the HST /WFPC2 archive data. We have found about 560 star cluster candidates in NGC 1487, using the morphological parameters of the objects. We have investigated several photometric characteristics of the clusters: color-magnitude diagrams (CMDs), color distribution, spatial distribution, age, size and luminosity function. The CMD of the bright clusters with 18.5 < B < 24 mag in NGC 1487 shows three major populations of clusters: a blue cluster population with $(B-I){\le}0.45$, an intermediate-color cluster population with $0.45<(B-I){\le}1.55$, and a red cluster population with (B - I) > 1.55. The intermediate-color population is the most dominant among the three populations. The brightest clusters in the blue and intermediate- color populations are as bright as $B{\approx}18mag$ ($M_B{\approx}-12mag$), which are three magnitudes brighter than those in the red population. The blue and intermediate-color clusters are strongly concentrated on the bright condensations, while the red clusters are relatively more scattered over the galaxy. The CMD of these clusters is found to be remarkably similar to that of the clusters in the famous interacting system M51. From this we suggest that the intermediate-color clusters were, probably, formed during the merging process which occurred about 500 Myrs ago.

• 핵의학기술
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• 제20권1호
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• pp.59-65
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• 2016

동적신장검사는 신장기능을 영상화하는 대표적인 방법이다. 동적신장검사에서 저선량 방사성의약품의 사용으로 기존 동적신장검사와 저선량을 사용한 신장검사의 비교를 통한 동적신장검사의 재현성을 평가해 보기로 했다. 본 비교실험을 통해 재현성이 우수할 경우 환자에 투여하는 방사선량을 줄인 동적신장검사법을 활용하고 환자의 피폭을 줄이고자 한다. 감마카메라 장비로는 Orbiter, SymbiaE (Siemens, Germany)를 사용하였고, 2013년 1월부터 2014년 2월까지 370 Mbq (10mCi)을 사용한 환자와 동일 환자 중 2014년 3월부터 2015년 7월까지 185 Mbq (5 mCi)을 사용한 환자를 대상으로 $^{99m}Tc-DTPA$사용 검사 21명과 $^{99m}Tc-MAG_3$사용 검사 20명 총 41명을 대상으로 데이터를 선별하였다. 결과 영상의 Renogram에서 Peak 지점의 프레임을 선택하여 신장의 관심영역과 배후방사능의 관심영역을 설정하고 K/B ratio를 구하여 비교하였다. $^{99m}Tc-DTPA$를 사용한 검사에서 370 Mbq을 사용하였을 때의 K/B ratio는 평균 $5.67{\pm}0.8$이었고, 185 Mbq을 사용하였을 때는 평균 $5.62{\pm}0.87$로 큰 차이를 보이지 않았다. $^{99m}Tc-MAG_3$를 사용한 검사에서도 신장/배후방사능 비는 370 Mbq을 사용 시 평균 $14.95{\pm}2.58$과 185 Mbq을 사용 시 평균 $14.56{\pm}2.02$로 큰 차이를 보이지 않았다. Paired sample t-test결과 p-value는 $^{99m}Tc-DTPA$ 0.566, $^{99m}Tc-MAG_3$ 0.363로 같은 비교집단 간 차이점이 없음을 확인하였다. 동일 환자를 대상으로 선량을 370 Mbq에서 185 Mbq로 줄였을 때의 동적신장검사의 재현성은 우수한 것으로 확인 되었다. 저선량 동적신장검사는 기존 감마카메라의 성능 개선 없이 재현성이 우수한 결과를 얻을 수 있고 환자의 피폭 또한 줄일 수 있을 것으로 사료된다.

• 대한방사선협회지
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• 제29권1호
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• pp.152-152
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• 2003

• 천문학회보
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• 제36권2호
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• pp.142.1-142.1
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• 2011

UBVI and $H{\alpha}$ CCD photometry of IC 1848, one of active star-forming regions in Cas OB6, is carried out as a part of Sejong Open cluster Survey (SOS) project. An OB association is an ideal laboratory for studying the triggered star formation and star formation history. Our purposes are to provide deep photometric data up to 21 mag in V and physical parameters of IC 1848. We classify 79 early-type stars and 186 pre-main sequence (PMS) stars as being the members of the cluster using photometric criteria. The IR excess emission PMS stars by Koenig et al. (2008) are also included as members of IC 1848. Total number of members is 414. We derive the interstellar reddening (=$0.659{\pm}0.058$ mag), reddening law ($R_V=4.0{\pm}0.1$), distance modulus ($V_0-M_V=12.0{\pm}0.1$ mag) using the early-type members of IC 1848. We also determine the age of the cluster ($3.5{\pm}1.5$ Myr) by placing the theoretical isochrones on the HR diagram.

• Animal cells and systems
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• 제16권2호
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• pp.114-120
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• 2012

In echinoderms, the SALMFamide neuropeptides sharing the SxL/FxFamide motif seem widespread throughout the phylum and may be important signalling molecules that mediate various physiological functions. Recent identification of S1 and its analogues, MagS3 and MagS4, along with the S2 analogue, MagS2 from the starfish $Marthasterias$ $glacialis$, indicated that SALMFamides in the class Asteroidea are more diverse than previously thought. Further, isolation of the neuropeptides from the radial nerve cord and studies on pharmacological actions of the neuropeptides on the cardiac stomach warrant studies on the tissue distributions of these peptides in both the nervous and digestive systems. In the present study, antisera raised against an S1 analogue, KYSALMFamide, and an S2 analogue, KYSGLTFamide, were used to localize the distribution patterns of the S1- and S2-like immunoreactivities (S1-IR/S2-IR) in the nervous and digestive systems of the starfish. In the nervous system, cell bodies in the ectoneural part were immunostained for both S1 and S2 peptides, while in the digestive system, the basiepithelial plexus and mucosal cell bodies were immunoreactive. These immunocytochemical data support the notion that the SALMFamides may play a neuroendocrine role in mediating feeding behaviour of the starfish. Further studies including identification of peptide binding sites and differential expression pattern of mRNAs encoding the peptides are required to elucidate their physiological functions.