• Title/Summary/Keyword: particle flux

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고상법으로 합성한 Sr4-(x+y+z)Al14O25 : Eux, Dyy, Agz계 축광성 형광체 장잔광의 연구 (Research on Afterglow Brightness of Sr4-(x+y+z)Al14O25 : Eux, Dyy, Agz by Solid State Synthesis)

  • 김승우;김정식
    • 대한금속재료학회지
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    • 제49권4호
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    • pp.348-354
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    • 2011
  • Long-lasting brightness $Sr_{4}Al_{14}O_{25}$ : $Eu^{2+}$, $Dy^{3+}$, $Ag^{+}$ phosphor was synthesized by modified solid state reaction and its photoluminescence was investigated. $Sr(NO_3)_{2}$ and $Al(NO_3)_3{\cdot}9H_{2}O$ as starting materials, and $B_{2}O_{3}$ as a flux were mixed with $Eu_{2}O_{3}$ as an activator, $Dy_{2}O_{3}$ as a coactivator, and $AgNO_{3}$ as a charge compensator. The crystalline of target powder showed a single-phase $Sr_{4}Al_{14}O_{25}$ by the XRD characterization and the average particle size was about 20-30 ${\mu}m$ from the FE-SEM observation. $Ag^{+}$ ion doping effects (0-0.06 mol) on $Sr_{4}Al_{14}O_{25}:Eu^{2+},\;Dy^{3+},\;Ag^{+}$ phosphor were measured by photoluminescence spectrometer and luminescence meter. The of photoluminescence intensity of the $Sr_{3.64}Al_{14}O_{25}:Eu_{0.11},\;Dy_{0.22},\;Ag_{0.03}$ phosphor was higher than other compositions and afterglow brightness was 0.186 $cd/m^{2}$.

OGLE-2017-BLG-1049: ANOTHER GIANT PLANET MICROLENSING EVENT

  • Kim, Yun Hak;Chung, Sun-Ju;Udalski, A.;Bond, Ian A.;Jung, Youn Kil;Gould, Andrew;Albrow, Michael D.;Han, Cheongho;Hwang, Kyu-Ha;Ryu, Yoon-Hyun;Shin, In-Gu;Shvartzvald, Yossi;Yee, Jennifer C.;Zang, Weicheng;Cha, Sang-Mok;Kim, Dong-Jin;Kim, Hyoun-Woo;Kim, Seung-Lee;Lee, Chung-Uk;Lee, Dong-Joo
    • 천문학회지
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    • 제53권6호
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    • pp.161-168
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    • 2020
  • We report the discovery of a giant exoplanet in the microlensing event OGLE-2017-BLG-1049, with a planet-host star mass ratio of q = 9.53 ± 0.39 × 10-3 and a caustic crossing feature in Korea Microlensing Telescope Network (KMTNet) observations. The caustic crossing feature yields an angular Einstein radius of θE = 0.52 ± 0.11 mas. However, the microlens parallax is not measured because the time scale of the event, tE ≃ 29 days, is too short. Thus, we perform a Bayesian analysis to estimate physical quantities of the lens system. We find that the lens system has a star with mass Mh = 0.55+0.36-0.29 M⊙ hosting a giant planet with Mp = 5.53+3.62-2.87 MJup, at a distance of DL = 5.67+1.11-1.52 kpc. The projected star-planet separation is a⊥ = 3.92+1.10-1.32 au. This means that the planet is located beyond the snow line of the host. The relative lens-source proper motion is μrel ~ 7 mas yr-1, thus the lens and source will be separated from each other within 10 years. After this, it will be possible to measure the flux of the host star with 30 meter class telescopes and to determine its mass.

자장여과아크소스의 자장필터 꺾임 각도와 아크방전전류에 따라 증착된 ta-C 코팅의 마모 거동 연구 (A Study on the Wear Behavior of Tetrahedral Amorphous Carbon Coatings Based on Bending Angles of the Filtered Cathodic Vacuum Arc with Different Arc Discharge Currents)

  • 김원석;김송길;장영준;김종국
    • Tribology and Lubricants
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    • 제38권3호
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    • pp.101-108
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    • 2022
  • The structure and properties of tetrahedral amorphous carbon (ta-C) coatings depend on the main process parameters and bending angles of the magnetic field filter used in the filtered cathodic vacuum arc (FCVA). During the process, it is possible to effectively control the plasma flux of carbon ions incident on the substrate by controlling the arc discharge current, thereby influencing the mechanical properties of the coating film. Furthermore, we can control the size and amount of large particles mixed during carbon film formation while conforming with the bending angle of the mechanical filter mounted on the FCVA; therefore, it also influences the mechanical properties. In this study, we consider tribological characteristics for filtered bending angles of 45° and 90° as a function of arc discharge currents of 60 and 100 A, respectively. Experiment results indicate that the frictional behavior of the ta-C coating film is independent of the bending angle of the filter. However, its sliding wear behavior significantly changes according to the bending angle of the FCVA filter, unlike the effect of the discharge current. Further, upon changing the bending angle from 45° to 90°, abrasive wear gets accelerated, thereby changing the size and mixing amount of macro particles inside the coating film.

Development of the vapor film thickness correlation in porous corrosion deposits on the cladding in PWR

  • Yuan Shen;Zhengang Duan;Chuan Lu ;Li Ji ;Caishan Jiao ;Hongguo Hou ;Nan Chao;Meng Zhang;Yu Zhou;Yang Gao
    • Nuclear Engineering and Technology
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    • 제54권12호
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    • pp.4798-4808
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    • 2022
  • The porous corrosion deposits (known as CRUD) adhered to the cladding have an important effect on the heat transfer from fuel rods to coolant in PWRs. The vapor film is the main constituent in the two-phase film boiling model. This paper presents a vapor film thickness correlation, associated with CRUD porosity, CRUD chimney density, CRUD particle size, CRUD thickness and heat flux. The dependences of the vapor film thickness on the various influential factors can be intuitively reflected from this vapor film thickness correlation. The temperature, pressure, and boric acid concentration distributions in CRUD can be well predicted using the two-phase film boiling model coupled with the vapor film thickness correlation. It suggests that the vapor thickness correlation can estimate the vapor film thickness more conveniently than the previously reported vapor thickness calculation methods.

Suppression of stray electrons in the negative ion accelerator of CRAFT NNBI test facility

  • Yuwen Yang ;Jianglong Wei ;Junwei Xie ;Yuming Gu;Yahong Xie ;Chundong Hu
    • Nuclear Engineering and Technology
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    • 제55권3호
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    • pp.939-946
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    • 2023
  • Comprehensive Research Facility for Fusion Technology (CRAFT) is an integration of different demonstrating or testing facilities, which aim to develop the critical technology or composition system towards the fusion reactor. Due to the importance and challenge of the negative ion based neutral beam injection (NNBI), a NNBI test facility is included in the framework of CRAFT. The initial object of CRAFT NNBI test facility is to obtain a H0 beam power of 2 MW at the energy of 200-400 keV for the pulse duration of 100 s. Inside the negative ion accelerator of NNBI system, the interactions of the negative ions with the background gas and electrodes can generate abundant stray electrons. The stray electrons can be further accelerated and dumped on the electrodes or eject from the accelerator. The stray electrons, including the ejecting electrons, cause the unwanted particle and heat flux onto the electrodes and the inner components of beamline (especially the temperature sensitive cryopump). The suppression of the stray electrons from the CRAFT accelerator is carried out via a series of design and simulation works. The paper focuses the influence of different magnetic field configurations on the stray electrons and the character of the ejecting electrons.

Verification of a novel fuel burnup algorithm in the RAPID code system based on Serpent-2 simulation of the TRIGA Mark II research reactor

  • Anze Pungercic;Valerio Mascolino ;Alireza Haghighat;Luka Snoj
    • Nuclear Engineering and Technology
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    • 제55권10호
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    • pp.3732-3753
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    • 2023
  • The Real-time Analysis for Particle-transport and In-situ Detection (RAPID) Code System, developed based on the Multi-stage Response-function Transport (MRT) methodology, enables real-time simulation of nuclear systems such as reactor cores, spent nuclear fuel pools and casks, and sub-critical facilities. This paper presents the application of a novel fission matrix-based burnup methodology to the well-characterized JSI TRIGA Mark II research reactor. This methodology allows for calculation of nuclear fuel depletion by combination and interpolation of RAPID's burnup dependent fission matrix (FM) coefficients to take into account core changes due to burnup. The methodology is compared to experimentally validated Serpent-2 Monte Carlo depletion calculations. The results show that the burnup methodology for RAPID (bRAPID) implemented into RAPID is capable of accurately calculating the keff burnup changes of the reactor core as the average discrepancies throughout the whole burnup interval are 37 pcm. Furthermore, capability of accurately describing 3D fission source distribution changes with burnup is demonstrated by having less than 1% relative discrepancies compared to Serpent-2. Good agreement is observed for axially and pin-wise dependent fuel burnup and nuclear fuel nuclide composition as a function of burnup. It is demonstrated that bRAPID accurately describes burnup in areas with high gradients of neutron flux (e.g. vicinity of control rods). Observed discrepancies for some isotopes are explained by analyzing the neutron spectrum. This paper presents a powerful depletion calculation tool that is capable of characterization of spent nuclear fuel on the fly while the reactor is in operation.

조립질 지반에서의 수평배수재 종류에 따른 배수성능 비교 (Comparisons of Drainage Performance on Coarse Grained Soils with Regard to Horizontal Drainage Type)

  • 방태완;조완제;설승환
    • 한국지반환경공학회 논문집
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    • 제24권11호
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    • pp.25-31
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    • 2023
  • 대표적인 비탈면 배수공법인 수평배수공은 비탈면 내 간극수압을 감소시키기 위해 국내외에서 다수 활용하고 있다. 이에 따라 다양한 연구들이 선행되어 왔으나, 수평배수공의 수량을 산정하기 위한 명확한 설계기준이 없어 획일적으로 시공되고 있다. 따라서 본 논문에서는 다양한 수평배수공의 배수성능과 영향인자에 대한 메커니즘을 규명하고자 현장토를 이용하여 모형토조실험을 수행하였다. 또한, 배수재 형상이나 크기에 따른 배수성능을 비교하고자 입도분포가 다른 시료에서의 유출량 결과를 비교 및 검토하였다. 정상류 상태에서 배수실험을 확인하기 위해 유출량을 측정한 결과, 모든 시료에서 최소 3분에서 최대 15분 뒤 일정한 속도로 배수되는 것을 확인하였다. 조립질 지반에서 단일 시간당 유출되는 양(단위 유출량)으로 비교한 경우, 배수재 형상과 크기에 따른 배수효과가 상이하여 배수성능에 영향을 미치는 것을 확인하였다. 향후 세립질 지반에서의 배수 성능실험과 수량을 결정하기 위한 기초자료로 충분히 활용될 수 있을 것으로 기대된다.

Long-Term Science Goals with In Situ Observations at the Sun-Earth Lagrange Point L4

  • Dae-Young Lee;Rok-Soon Kim;Kyung-Eun Choi;Jungjoon Seough;Junga Hwang;Dooyoung Choi;Ji-Hyeon Yoo;Seunguk Lee;Sung Jun Noh;Jongho Seon;Kyung-Suk Cho;Kwangsun Ryu;Khan-Hyuk Kim;Jong-Dae Sohn;Jae-Young Kwak;Peter H. Yoon
    • Journal of Astronomy and Space Sciences
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    • 제41권1호
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    • pp.1-15
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    • 2024
  • The Korean heliospheric community, led by the Korea Astronomy and Space Science Institute (KASI), is currently assessing the viability of deploying a spacecraft at the Sun-Earth Lagrange Point L4 in collaboration with National Aeronautics and Space Administration (NASA). The aim of this mission is to utilize a combination of remote sensing and in situ instruments for comprehensive observations, complementing the capabilities of the L1 and L5 observatories. The paper outlines longterm scientific objectives, underscoring the significance of multi-point in-situ observations to better understand critical heliospheric phenomena. These include coronal mass ejections, magnetic flux ropes, heliospheric current sheets, kinetic waves and instabilities, suprathermal electrons and solar energetic particle events, as well as remote detection of solar radiation phenomena. Furthermore, the mission's significance in advancing space weather prediction and space radiation exposure assessment models through the integration of L4 observations is discussed. This article is concluded with an emphasis on the potential of L4 observations to propel advancements in heliospheric science.

6 MeV 전자선의 차폐물질 원자번호와 조사야 크기에 따른 선량변화 연구 (The Study of Dose Change by Field Effect on Atomic Number of Shielding Materals in 6 MeV Electron Beam)

  • 이승훈;곽근탁;박주경;김양수;차석용
    • 대한방사선치료학회지
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    • 제25권2호
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    • pp.145-151
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    • 2013
  • 목 적: 본 연구에서 우리는 6 MeV 전자선의 조사야 확대에 따른 선량변화가 차폐물질 원자번호와 관계가 있음을 알아보고 그 영향인자를 분석 하고자 한다. 대상 및 방법: 먼저 평행평판형 전리함(Exradin P11)을 $25{\times}25cm^2$ 폴리스티렌 팬텀표면에 평탄하게 끼운다. 허용투과율 5% 두께의 알루미늄, 구리, 납 물질들을 팬텀 상단에 차폐시킨 후 조사야 $6{\times}6$, $10{\times}10$ 그리고 $20{\times}20cm^2$별로 측정하였다. 조사조건은 선원-표면간거리 100 cm에서 기준조사야인 $10{\times}10cm^2$에 6 MeV 전자선을 이용하여 100 cGy 조사하였다. 다음으로 MCNP (Monte Carlo N Particle Transport Code)를 이용하여 각 물질 통과 후 발생되는 광자수, 전자수, 그리고 축적에너지를 계산하였다. 결 과: 허용투과율 5% 두께에 대한 차폐물 종류에 따른 측정결과 조사야 $10{\times}10cm^2$을 기준으로 한 $6{\times}6cm^2$$20{\times}20cm^2$의 두께변화율은 알루미늄에서 각각 +0.06%와 -0.06%, 구리에서 각각 +0.13%와 -0.1%, 납에서 각각 -1.53%와 +1.92%였다. 계산결과 조사야 $10{\times}10cm^2$ 대비 $6{\times}6cm^2$, $20{\times}20cm^2$의 축적에너지는 차폐를 하지 않았을 경우 각각 -4.3%와 +4.85%, 알루미늄 사용 시 각각 -0.87%와 +6.93%, 구리 사용 시 각각 -2.46%와 +4.48%, 납 사용 시 각각 -4.16%와 +5.57%였다. 광자수의 경우 차폐를 하지 않았을 경우 각각 -8.95%와 +15.92%, 알루미늄 사용 시 각각 -15.56%와 +16.06%, 구리 사용시 각각 -12.27%와 +15.53%, 납 사용 시 각각 -12.36%와 +19.81%였다. 전자수의 경우 차폐를 하지 않았을 경우 각각 -3.92%와 +4.55%, 알루미늄 사용 시 각각 +0.59%와 +6.87%, 구리 사용 시 각각 -1.59%와 +3.86%, 납 사용 시 각각 -5.15%와 +4.00%였다. 결 론: 본 연구로 조사야 증가함에 따른 차폐물 두께가 저 원자번호에서 감소하며, 고 원자번호에서는 증가함을 볼 수 있었으며, 계산을 통해 저 원자번호물질에서는 저지방사선, 고 원자번호물질에서는 산란전자가 영향을 주는 것을 알 수 있었다.

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ULTIMATE 기법을 이용한 부유사 밀도류 전파 수치모의 (A numerical simulation of propagating turbidity currents using the ULTIMATE scheme)

  • 최성욱;최성욱
    • 한국수자원학회논문집
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    • 제50권1호
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    • pp.55-64
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    • 2017
  • 본 연구에서는 ULTIMATE 기법을 이용하여 밀도류 층적분 모형의 해석을 위한 수치모형을 제시하였다. 개발된 모형을 경사부와 평탄부로 이루어진 실내 실험에 적용하여 경사부에 유입된 부유사 밀도류의 전파 특성에 대해 분석하였다. ULTIMATE 기법의 범용제한자로 인하여 밀도류의 선단부가 수치진동 없이 비교적 급한 형태로 전파되는 것을 모의하였다. 그리고 사류로 전파되고 수로 끝에서부터 상류로 변화되는 밀도류의 내부 도수 발생 과정을 재현하였다. 이러한 내부 도수는 ULTIMATE 제한자를 사용하면 Courant 수가 1 미만일 때 안정적으로 모의되는 것을 확인하였다. 또한 밀도류의 전파 속도에 영향을 주는 인자에 대하여 분석하였다. 입자의 크기는 $9{\mu}m$ 이하일 때 밀도류의 전파 속도에 큰 영향을 주지 않는 반면, 부력 흐름률은 확연한 영향을 주는 것을 확인하였다. 마지막으로 부유사 밀도류에 의한 하상변동에 대해 검토하였다. 수치모형으로 부유사 밀도류의 전파에 의한 하상변동을 정량적으로 적절히 모의하였으며, 도수로 인한 부유사 연행의 차이와 이로 인한 하상의 불연속적인 형태를 관찰할 수 있었다.