• Title/Summary/Keyword: scale formation

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Amber Information Design to Keep Safety-Driving Under Road Structure at Local-Scale Geographic (국지지역 도로 기반 시설에서 안전운전을 위한 경보 정보 설계)

  • Park, Jung-Chan;Hong, Gyu- Jang
    • The Transactions of the Korean Institute of Electrical Engineers P
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    • v.58 no.1
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    • pp.48-55
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    • 2009
  • In order to keep safe driving conditions under road networks, there are several formations such as road structure, road surface condition, traffic occupancy and supplement of an accurate information of traffic status ahead To support safe-driving on each road formation, each formation is supplied with various information to help the driver. However, in some cases like rapid status change at local-scale geography, traffic information systems often displays insufficient information because of the lack of information correlation. In order to accurately aware the driver, all road formation must be in sync. It is important to supply accurate information to the driver because this information directly impacts the drivers on the road. This paper discusses the amber information to keep the least safety driving over road formations including tunnels and bridges. This paper also will propose the informations for safe-driving conditions, information linkage on the road and rule-base safety information, as ITS technology, being displayed for all drivers under the worst weather conditions.

A New Species of Leptostrobus from the Upper Triassic Amisan Formation of the Nampo Group in Korea

  • Kim, Jong-Heon;Kim, Hee-Soo;Lee, Bong-Jae;Kim, Jung-Min;Lee, Hee-Kwon
    • Journal of the Korean earth science society
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    • v.23 no.1
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    • pp.30-37
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    • 2002
  • Leptostrobus myeongamensis sp. nov. is newly described from the well-preserved but broken material occurring in the Upper Triassic Amisan Formation of the Nampo Group in Korea. This species is characterized by its lateral appendages of cone axis, each consisting of a rounded capsule and small scale leaf, and by its cone base covered with small scale leaves, the same size as in cone axis. This species is the first record from the Mesozoic strata in Korea.

Cosmological Information from the Small-scale Redshift Space Distortions

  • Tonegawa, Motonari;Park, Changbom;Zheng, Yi;Kim, Juhan;Park, Hyunbae;Hong, Sungwook
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.2
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    • pp.52.3-52.3
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    • 2019
  • We present our first attempt at understanding the dual impact of the large-scale density and velocity environment on the formation of very first astrophysical objects in the Universe. Following the recently developed quasi-linear perturbation theory on this effect, we introduce the publicly available initial condition generator of ours, BCCOMICS (Baryon Cold dark matter COsMological Inital Condition generator for Small scales), which provides so far the most self-consistent treatment of this physics beyond the usual linear perturbation theory. From a suite of uniform-grid simulations of N-body+hydro+BCCOMICS, we find that the formation of first astrophysical objects is strongly affected by both the density and velocity environment. Overdensity and streming-velocity (of baryon against cold dark matter) are found to give positive and negative impact on the formation of astrophysical objects, which we quantify in terms of various physical variables.

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Formation CubeSat Constellation, SNIPE mission

  • Lee, Jaejin
    • The Bulletin of The Korean Astronomical Society
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    • v.46 no.1
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    • pp.58.4-59
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    • 2021
  • This presentation introduces Korea's SNIPE (Small scale magNespheric and Ionospheric Plasma Experiment) mission, formation flying CubeSat constellation. Observing particles and waves on a single satellite suffers from inherent space-time ambiguity. To observe spatial and temporal variations of the micro-scale plasma structures on the topside ionosphere, four 6U CubeSats (~ 10 kg) will be launched into a polar orbit of the altitude of ~500 km in 2021. The distances of each satellite will be controlled from 10 km to more than 100 km by formation flying algorithm. The SNIPE mission is equipped with identical scientific instruments, solid-state telescope, magnetometer, and Langmuir probe. All the payloads have a high temporal resolution (sampling rates of about 10 Hz). Iridium modules provide an opportunity to upload changes in operational modes when geomagnetic storms occur. SNIPE's observations of the dimensions, occurrence rates, amplitudes, and spatiotemporal evolution of polar cap patches, field-aligned currents (FAC), radiation belt microbursts, and equatorial and mid-latitude plasma blobs and bubbles will determine their significance to the solar wind-magnetosphere-ionosphere interaction and quantify their impact on space weather.

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A Numerical Study on the Slab Heating Characteristics in a Reheating Furnace with the Formation and Growth of Scale on the Slab Surface (스케일 층의 생성 및 성장을 고려한 가열로 내 슬랩의 승온 특성 해석에 관한 연구)

  • Lee, Dong-Eun;Jang, Jung-Hyun;Kim, Chong-Min;Hong, Dong-Jin;Park, Hae-Doo;Park, Yun-Beom;Kim, Man-Young
    • 한국전산유체공학회:학술대회논문집
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    • 2008.03b
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    • pp.109-112
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    • 2008
  • In this work, a mathematical heat transfer model of a walking-beam type reheating furnace that can predict the formation and growth of the scale layer, which is produced due to oxidative reaction between the furnace oxidizing atmosphere and the steel surface in the reheating furnace, has been developed. The model can also predict the heat flux distribution within the furnace and the temperature distribution in the slab and scale throughout the reheating furnace process by considering the heat exchange between the slab and its surroundings in the furnace, including radiant heat transfer among the slabs, the skids, the hot gases and the furnace wall as well as the gas convection heat transfer in the furnace. Using the model developed in this work, the effects of the scale layer on the heat transfer characteristics and temperature behavior of the slab is investigated. A comparison is also made between the predictions of the present model and the data from an in situ measurement in the furnace, and a reasonable agreement is founded.

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Establishment of in Vitro Culture and Effect of Chilling Treatment of Mother Bulb On Bulblet Formation in Fritillaria thunbergii Miq. (패모의 초기배양과 모구의 저온처리가 자구형성에 미치는 영향)

  • Yu, Kwang-Jin;Paek, Kee-Yeoup;Seong, Nak-Sul;Choi, In-Sick;Cho, Jin-Tae
    • Korean Journal of Medicinal Crop Science
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    • v.2 no.3
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    • pp.211-218
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    • 1994
  • This experiment was conducted to obtain basic information for the establishment of in vitro initial culture system in Fritillaria thuubergii Miq. Methods of surface sterilization of scale segments as explant and effect of antibiotics added into the culture medium on contamination of explant and chilling treatment of mother bulb on bulblet formation were investigated. Portent of contamination of cultured scale segments was significantly higher in the outer scale segments which were unsuitable as initial culture explant than inner scale segments. Contamination of explants taken from inner scale of bulb was reduced by surface sterilizing explants in the solution of $4{\sim}5%$ sodium hypoclorite for $10{\sim}15$ mimutes. Addition of antibiotics such as kanamycin, vancomycia cefotaxim, agrirnycin and agreptomycin and dithane as fungicide and$lncyte^{tm}$ into MS medium was effective to reduce bateriological contamination, but did not work to control fungi. It had effective to delay the degree of contamination caused by fungi and bacteria haboring in cultured explants. Bulblet formation from cultured scale segments was promoted by dry storage for $2{\sim}4$ weeks or moisture storage of mother bulbs for $4{\sim}6$ weeks at $10^{\circ}C$ before excision of explants. Addition of kinetin into medium could not exerted for the bulblet formation from the scale segment of dry storaged bulb compared to control. But explant taken from 6 week moisture storaged bulb formed more than 10 bulblets per explant on the medium containing $3{\sim}5mg/L$ kinetin.

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COSMIC RAY ACCELERATION DURING LARGE SCALE STRUCTURE FORMATION

  • BLASI PASQUALE
    • Journal of The Korean Astronomical Society
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    • v.37 no.5
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    • pp.483-491
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    • 2004
  • Clusters of galaxies are storage rooms of cosmic rays. They confine the hadronic component of cosmic rays over cosmological time scales due to diffusion, and the electron component due to energy losses. Hadronic cosmic rays can be accelerated during the process of structure formation, because of the supersonic motion of gas in the potential wells created by dark matter. At the shock waves that result from this motion, charged particles can be energized through the first order Fermi process. After discussing the most important evidences for non-thermal phenomena in large scale structures, we describe in some detail the main issues related to the acceleration of particles at these shock waves, emphasizing the possible role of the dynamical backreaction of the accelerated particles on the plasmas involved.

Study on $SF_6$ hydrate Formation and Dissociation Behavior inside of Bench-scale High Pressure Reactor (Bench-scale 고압반응기 내의 미세액적분사에 따른 $SF_6$ 하이드레이트 형성 거동 연구)

  • Moon, Dong-hyun;Lee, Jae-jeong;Shin, Hyung-Joon;Lee, Ju-Dong;Lee, Gang-Woo
    • 한국신재생에너지학회:학술대회논문집
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    • 2009.06a
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    • pp.687-690
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    • 2009
  • 본 연구에서는 가스 하이드레이트 형성과정에서 발생할 수 있는 유도지체시간을 줄이고 전체 가스 저장량과 반응 속도의 향상을 위하여 이류체 분사 방식을 이용하여 물분자의 액적을 최소화하는 실험을 통하여, 미세액적 분사에 따른 하이드레이트 형성 시간을 확인하였으며, 반응기 내부의 온도 변화를 확인하여 반응기 내부의 하이드레이트 형성 거동을 확인하고 이를 통하여 상용화를 위한 반응기 설계의 기초 자료로 활용하고자 하였다.

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Simulation of the SDSS Survey Region of the Universe

  • Park, Chang-Bom;Van De Weygaert, Rien;Wojceich, Hellwing;Kim, Ju-Han
    • The Bulletin of The Korean Astronomical Society
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    • v.35 no.2
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    • pp.43.2-43.2
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    • 2010
  • We reconstruct the large-scale initial density field from the distribution of galaxies observed by the Sloan Digital Sky Survey (SDSS). After adding the small-scale fluctuations to match the power spectrum to that of the standard LCDM model, we make a cosmological N-body simulation of formation of structures from the initial conditions. Properties of the objects formed in the simulation can be statistically compared with those of the observed SDSS galaxies. The simulation makes it possible to know the past history of evolution of objects located in different environments, and also gives us information on the environmental parameters that cannot be directly obtained observationally. It is hoped that this comparative study leads us to better understanding of formation and evolution of galaxies in conjunction with large-scale structures in the universe.

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High-temperature Oxidation of the TiAlCrSiN Film (TiAlCrSiN 박막의 고온 산화 부식)

  • Lee, Dong-Bok;Kim, Min-Jeong;Abro, M.A.;Yadav, P.;Shi, Y.
    • Proceedings of the Korean Institute of Surface Engineering Conference
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    • 2016.11a
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    • pp.107-107
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    • 2016
  • TiCrAlSiN films were developed in order to improve the high-temperature oxidation resistance, corrosion resistance, and mechanical properties of conventional TiN films that are widely used as hard films to protect and increase the lifetime and performance of cutting tools or die molds. In this study, a nano-multilayered TiAlCrSiN film was deposited by cathodic arc plasma deposition. It displayed relatively good oxidation resistance at $700-900^{\circ}C$, owing to the formation protective oxides of $Al_2O_3$, $Cr_2O_3$, and $SiO_2$, and semiprotective $TiO_2$. At $1000^{\circ}C$, the increased temperature led to the formation of the imperfect oxide scale that consisted primarily of the outer ($TiO_2$,$Al_2O_3$)-mixed scale and inner ($TiO_2$, $Al_2O_3$, $Cr_2O_3$)-mixed scale.

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