• 한국통신학회논문지
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• 제35권2B호
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• pp.244-251
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• 2010

CSD는 미국 국토안보부(DHS)에서 제안한 Active RFID를 기반으로 하는 컨테이너 보안 장치로 컨테이너 내부에 장착되어 컨테이너 도어의 개폐여부를 감지하는 장치이다. ConTracer는 본 연구에서 개발한 CSD(Container Security Device)로 이 장비의 주기능은 컨테이너 도어 개폐 여부 감지뿐만 아니라 온도, 습도, 충격 센서를 장착하여 컨테이너 내부 환경 상태 및 운송 도중 컨테이너에 가해지는 충격에 대한 이력 조회가 가능하다. 그리고 RFID 동작주파수는 433MHz와 2.4GHz의 두 주파수 대역을 사용하여 각 국가별 주파수 사용제안에 능동적으로 대응 할 수 있도록 하였다. 본 논문에서는 컨테이너 보안 장치의 발전 방향에 대해서 알아본 후 본 연구에서 개발한 ConTracer와 각 회사에서 개발한 CSD를 비교하여 보고, ConTracer를 이용하여 설계 및 구현한 CSD 시스템을 소개한다. 마지막으로 구현된 CSD 시스템은 한국 중국 간 컨테이너 물류에 시범서비스를 실시하여 구현한 CSD 시스템을 검증 하였다.

• 한국정보통신학회논문지
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• 제15권7호
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• pp.1613-1620
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• 2011

CSD는 미국 국토안보부(DHS)에서 제시한 IEEE Standard 802.15.4b를 토대로 하는 컨테이너 보안 장치로 ISO 668 표준 규격으로 제작된 컨테이너에 장착되어 컨테이너 도어의 개폐여부를 감지하는 장치이다. 본 연구에서 개발한 CSD(Container Security Device)의 주 기능은 컨테이너 도어 개폐 여부 감지와 컨테이너 내부 환경 상태 및 운송 도중 컨테이너에 가해지는 충격에 대한 이력 조회이다. 본 논문에서는 글로벌 물류 패러다임 변화를 토대로 컨테이너화물 안전수송에 질적 서비스 향상을 위하여 본 연구에서 개발한 ConTracer를 활용하여 구현된 시스템을 한국 일본 간 컨테이너 물류 경로에 시범 운영 테스트를 적용하여 ConTracer의 시스템 성능 평가를 검증하는데 초점을 두었다.

• 한국자동차공학회논문집
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• 제8권4호
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• pp.1-9
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• 2000

To understand the thermal characteristics around the piston ring gap ring gap positions and piston temperatures are measured simultaneously. The locations of piston ring gap are measured by the radio-tracer method and piston temperature are measured by a K-type thermocouple and scissors type linkage system. From these experiments following facts are clarified. Piston temperatures fluctuate according to the piston ring rotation. And the temperature fluctuation is mainly affected by top ring gap position irrelevant to the second ring fop position. If the top ring gap position increases and the temperature of top ring groove shows maximum value when top rin gap position coincide with temperature measuring point. The maximum amplitude of temperature fluctuation which is proportional to the blow by gas rate is around 12-15$^{\circ}C$.

• Nuclear Engineering and Technology
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• 제46권1호
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• pp.93-100
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• 2014

The paper deals with the application of radio isotopic non-destructive technique in the characterization of two industrial grade anion exchange resins Indion GS-300 and Indion-860. For the characterization of the two resins, $^{131}I$ and $^{82}Br$ were used as tracer isotopes to trace the kinetics of iodide and bromide ion-isotopic exchange reactions. It was observed that the values of specific reaction rate ($min^{-1}$), amount of iodide ion exchanged (mmol), initial rate of iodide ion exchange (mmol/min) and log $K_d$ were calculated as 0.328, 0.577, 0.189 and 19.7 respectively for Indion GS-300 resin, which was higher than the respective values of 0.180, 0.386, 0.070 and 17.0 calculated for Indion-860 resins when measured under identical experimental conditions. Also at a constant temperature of $40.0^{\circ}C$, as the concentration of labeled iodide ion solution increases 0.001 M to 0.004 M, the percentage of iodide ions exchanged increases from 75.16 % to 78.36 % for Indion GS-300 resins, which was higher than the increases from 49.65 % to 52.36 % compared to that obtained for Indion-860 resins. The overall results indicate that under identical experimental conditions, Indion GS-300 resins show superior performance over Indion-860 resins.

• 대한환경공학회지
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• 제39권5호
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• pp.282-287
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• 2017

본 연구의 목적은 방사능 사고로 인한 오염물질 유입으로 인한 영향을 최소화하기 위한 제염제의 혼합확산장치 개발에 앞서 장치 가동으로 인한 혼합 및 확산영향을 예측하는데 있다. 유동특성분석을 위해 사용된 추적자는 방사성 동위원소는 Gy, To이며, 이를 검측하기 위해 2인치 NaI 방사선 검출기를 사용했다. 본 연구에 적용된 제염제 혼합확산장치의 임펠러는 3가지 type으로 제작하였다. 방사혼합형 임펠러는 상향류 흐름을 이용하여 수표면으로 확산이 가능하며, 최적의 조건을 찾기 위해 핀 구조를 조정하였다. 방사능 동위원소를 이용한 제염제 혼합확산장치의 유동특성을 분석한 결과, 모델별 혼합확산과 유동패턴특성을 획득하였다. Model 3 type은 별도의 Fin유도부와 보조 Fin이 구성되어 있어 다른 type의 임펠러보다 확산속도가 크고 완전혼합에 도달하는 시간이 짧게 나타났다.

• 천문학회지
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• 제37권5호
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• pp.455-460
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• 2004

There have been many speculations about the presence of cosmic ray protons (CRps) in galaxy clusters over the past two decades. However, no direct evidence such as the characteristic $\gamma$-ray signature of decaying pions has been found so far. These pions would be a direct tracer of hadronic CRp interactions with the ambient thermal gas also yielding observable synchrotron and inverse Compton emission by additionally produced secondary electrons. The obvious question concerns the type of galaxy clusters most likely to yield a signal: Particularly suited sites should be cluster cooling cores due to their high gas and magnetic energy densities. We studied a nearby sample of clusters evincing cooling cores in order to place stringent limits on the cluster CRp population by using non-detections of EGRET. In this context, we examined the possibility of a hadronic origin of Coma-sized radio halos as well as radio mini-halos. Especially for mini-halos, strong clues are provided by the very plausible small amount of required CRp energy density and a matching radio profile. Introducing the hadronic minimum energy criterion, we show that the energetically favored CRp energy density is constrained to $2\%{\pm}1\%$ of the thermal energy density in Perseus. We also studied the CRp population within the cooling core region of Virgo using the TeV $\gamma$-ray detection of M 87 by HEGRA. Both the expected radial $\gamma$-ray profile and the required amount of CRp support this hadronic scenario.

• 천문학회보
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• 제44권1호
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• pp.56.3-56.3
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• 2019

We are currently living in the era of the wide field cosmological surveys, either spectroscopic such as Dark Energy Spectrograph Instrument or photometric such as the Dark Energy Survey or the Large Synoptic Survey Telescope. By analyzing the distribution of matter clustering, we can use the growth of structure, in combination with measurements of the expansion of the Universe, to understand dark energy or to test different models of gravity. But we also live in the era of multi-tracer or multi-messenger astrophysics. In particular, during the next decades radio surveys will map the matter distribution at higher redshifts. Like in optical surveys, there are radio imaging surveys such as continuum radio surveys such as the ongoing EMU or spectroscopic by measuring the hydrogen 21cm line. However, we can also use intensity mapping as a low resolution spectroscopic technique in which we use the intensity given by the emission from neutral hydrogen from patches of the sky, at different redshifts. By cross-correlating this maps with galaxy catalogues we can improve our constraints on cosmological parameters and to understand better how neutral hydrogen populates different types of galaxies and haloes. Creating realistic mock intensity mapping catalogues is necessary to optimize the future analysis of data. I will present the mock neutral hydrogen catalogues that we are developing, using the Horizon run 4 simulations, to cross-correlate with mock galaxy catalogues from low redshift surveys and I will show the preliminary results from the first mock catalogues.

• 천문학논총
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• 제30권2호
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• pp.75-78
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• 2015

A growing body of evidence has been supporting the existence of so-called "dark molecular gas" (DMG), which is invisible in the most common tracer of molecular gas, i.e., CO rotational emission. DMG is believed to be the main gas component of the intermediate extinction region from Av~0.05-2, roughly corresponding to the self-shielding threshold of $H_2$ and $^{13}CO$. To quantify DMG relative to $H{\small{I}}$ and CO, we are pursuing three observational techniques; $H{\small{I}}$ self-absorption, OH absorption, and THz $C^+$ emission. In this paper, we focus on preliminary results from a CO and OH absorption survey of DMG candidates. Our analysis shows that the OH excitation temperature is close to that of the Galactic continuum background and that OH is a good DMG tracer co-existing with molecular hydrogen in regions without CO. Through systematic "absorption mapping" by the Square Kilometer Array (SKA) and ALMA, we will have unprecedented, comprehensive knowledge of the ISM components including DMG in terms of their temperature and density, which will impact our understanding of galaxy evolution and star formation profoundly.

• 생약학회지
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• 제11권3_4호통권43호
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• pp.133-140
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• 1980

In order to develop the radio-immunoassay procedure for the ginsenoside $Rg_1$ we prepared the $Rg_1-BSA$ conjugate and $Rg_1-tyramine$ conjugate by condensing the $Rg_1-azide$, which was prepared by a series of six step chemical modification of the $Rg_1-side$ chain, with bovine serum albumin(BSA) or with tyramine. Rabbits were immunized by repeated injection of $Rg_1-BSA$ conjugate with Freund's Complete Adjuvant for 5 month long to obtain very potent $anti-Rg_1$ serum. The radio-labelled haptene was prepared by direct radio-iodination $(125_J)$ of $Rg_1-tyramine$ according to the chloramine-T method. The radio-immunoassay procedure was successfully furnished by using DCC method (dextran coated charcoal) and the anti-body titer of the anti-serum was found as being $1600{\sim}3200$ by using 15000cpm tracer per test. Calibration test using non-labelled $Rg_1$ showed linear competetive binding response in the $(8-300){\times}34pg$. range of non-labelled $Rg_1$. The cross reaction test using 19 ginsenoside analogues enabled us a full structure-activity analysis on the antigen-antibody reaction that the anti-body in the serum would recognize the full structure of ginsenoside $Rg_1$ except the side chain moiety.

• Bulletin of the Korean Chemical Society
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• 제31권9호
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• pp.2649-2655
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• 2010

$PKC{\delta}$-catalytic V5 Heptapeptide (FEQFLDI, FP7) interacts with heat shock protein 27 (HSP27) and inhibits HSP27-mediated resistance to cell death against various stimuli including radiation therapy. Here, we prepared radio-iodinated heptapeptide and further investigated its uptake properties in HSP27 expression cells. Peptide sequence of FP7 and a negative control peptide (WSLLEKR, QP7) was modified by substituting their C-terminus residue to tyrosine (FP6Y and QP6Y) to label radio-iodine. Iodinated peptides were confirmed by LC mass analysis with cold iodine reaction mixture. Accumulation of [$^{125}I$]iodo-FP6Y and [$^{125}I$]iodo-QP6Y in NCI-H1299 cell line, with higher level of HSP27, and NCI-H460 cell line, with lower level of HSP27, was measured by NaI(Tl) scintillation counter. The modification of substituting C-terminus residue of FP7 to tyrosine (FP6Y) did not affect its interaction with HSP27. Accumulation of [$^{125}I$]iodo-FP6Y in NCI-H1299 cells was 3 fold higher than in NCI-H460 cells. The novel radio-iodinated FP6Y would be used as a tracer for targeting HSP27 protein.