• Title/Summary/Keyword: morphology formation

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The study on the formation of growth steps in the sublimation growth of SiC single crystals (승화법에 의한 SiC 단결정 성장에서 성장 step의 형성에 관한 연구)

  • 강승민
    • Journal of the Korean Crystal Growth and Crystal Technology
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    • v.11 no.1
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    • pp.1-5
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    • 2001
  • SiC single crystals were grown in the various condition of growth pressure and temperature in the sublimation growth. We observed the growth step morphology and the shapes on the surface of as-grown crystals using an optical microscope, and characterized the co-relations among the growth parameters by adapting the Burton, Carbera and Frank theory(BCF theory)for nucleation and crystal growth.

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Relation Between the Growth Twin and the Morphology of a Czochralski Silicon Single Crystal (초크랄스키 실리콘 단결정에서 성장 쌍정과 결정 외형의 관계)

  • 박봉모
    • Korean Journal of Crystallography
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    • v.11 no.4
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    • pp.207-211
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    • 2000
  • In a Czochralski silicon single crystal, the relation between the growth twin and the crystal morphology was investigated. The growth twin is nucleated on the {111} facet planes near the growth ridges. When a {111} growth twin is formed in the <100> silicon crystal, the growth ridge where twin is nucleated will continuous through the twin plane. Other two ridges at the 90。 apart will be displaced about 33° and be deformed to facets. The ridge on the opposite side of twin nucleation will disappear by forming a slight hill. Because the growth ridges of silicon is due to the {111} planes, the variation in the growth ridge formation can be predicted clearly by considering the change of the {111} plane traces in the stereographic projection after twining.

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Star Formation and Gas Accretion in Nearby Galaxies

  • Yim, Kijeong;van der Hulst, J.M.
    • The Bulletin of The Korean Astronomical Society
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    • v.42 no.2
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    • pp.75.3-75.3
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    • 2017
  • We Investigate dust stripping of Virgo cluster galaxies that are known to suffer HI gas stripping. The gas stripping phenomena of these galaxies may result from either ram pressure induced by the hot intracluster medium or gravitational tidal interactions between galaxies. While much efforts have been made to directly detect gas removed from cluster galaxies, the spatial distributions of dust, which should also be affected, are hardly known. Several previous studies have tried to directly detect the morphology of gas or dust using radio or infrared observations, but such approaches are hard to widely apply because of the limit of observational resolution and sensitivity. In this study, we try a different approach using optical data: measuring the background galaxy reddening by the dust stripped from the Virgo cluster members. Based on optical color excess maps of the background galaxies, we compare the ambient dust distribution with the HI morphology of the Virgo galaxies. We discuss how efficiently dust stripping can be detected with this method and how the stripped dust is associated with the removed gas according to HI gas stripping stage over the sample.

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Enhancement of the Surface Smoothness of Cu Ribbon for Solar Cell Modules

  • Cho, Tae-Sik;Cho, Chul-Sik
    • Transactions on Electrical and Electronic Materials
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    • v.16 no.1
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    • pp.20-24
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    • 2015
  • We studied the relationship between the surface smoothness of the internal Cu ribbon and the morphology of the Sn-Pb plating layer for solar cell modules. A bumpy surface was observed on the surface of the solar ribbon, which caused irregular reflection of light. Large, Pb-rich, primary ${\alpha}$-phases were found below the convex surface of the solar ribbon, passing from the surface of the internal Cu ribbon to the surface of the plating layer. The primary ${\alpha}$-phases heterogeneously nucleated on the convex surface of the Cu ribbon, and then largely grew to the convex surface of the plating layer. The restriction of the primary ${\alpha}$-phase's formation was enabled by enhancing the smoothness of the Cu ribbon's surface; it was also possible to increase the adhesive strength and decrease contact resistance. We confirmed that the solar ribbon's surface smoothness depends on the internal Cu ribbon's surface smoothness.

A New Model for the Analysis of Non-spherical Particle Growth Using the Sectional Method (구간해석방법을 통한 새로운 비구형 입자성장해석 모델)

  • Jeong, Jae-In;Choi, Man-Soo
    • Proceedings of the KSME Conference
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    • 2000.04b
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    • pp.416-421
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    • 2000
  • We have developed a simple model for describing the non-spherical particle growth phenomena using modified 1-dimensional sectional method. In this model, we solve simultaneously particle volume and surface area conservation sectional equations which consider particles' irregularities. From the correlation between two conserved properties of sections, we can predict the evolution of the aggregates' morphology. We compared this model with a simple monodisperse-assumed model and more rigorous two dimensional sectional model. For the comparison, we simulated silica and titania particle formation and growth in a constant temperature reactor environment. This new model shows a good agreement with the detailed two dimensional sectional model in total number concentration, primary particle size. The present model can also successfully predict particle size distribution and morphology without costing very heavy computation load and memory needed for the analysis of two dimensional aerosol dynamics.

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Nano-Soot Particle Formation in Inverse Diffusion Flames (인버스 확산화염에서의 나노 수트 입자 생성)

  • Lee, Eui-Ju;Shin, Hyun-Joon;Oh, Kwang-Chul;Shin, Hyun-Dong
    • 한국연소학회:학술대회논문집
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    • 2003.12a
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    • pp.19-26
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    • 2003
  • Experimental measurements of flame structure and soot characteristics were performed for ethene inverse diffusion flames (IDF). IDF has been considered as the excellent flow field to study the incipient soot because soot particle do not experience the oxidation process. In this study, LIF image clarified the reaction zone of IDF with OH signal and PAH distribution. laser light scattering technique also identified the being of soot particle. To address the degree of soot maturing, C/H ratio and morphology of soot sample were investigated. From these measurements, the effect of flow residence time and temperature on soot inception could be suggested, and more details on soot characteristic in the IDF was determined according to fuel dilution and flame condition. The fuel dilution results in a decrease of temperature and enhancement of residence time, but the critical dilution mole fraction is existed for temperature not to effect on soot growth. Also, the soot inception evolved on the specific temperature and its morphology are independent of the fuel dilution ratio of fuel.

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Fabrication of (110)〈110〉 textured Ag substrate for coated conductors ((110)〈110〉 집합조직을 가지는 박막선재용 Ag 기판의 제조)

  • 임준형;지봉기;이동욱;주진호;나완수;김찬중;홍계원
    • Proceedings of the Korea Institute of Applied Superconductivity and Cryogenics Conference
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    • 2003.02a
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    • pp.72-74
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    • 2003
  • We fabricated textured Ag substrates for coated conductor and evaluated the effects of annealing temperature on microstructural evolution, texture formation, and surface morphology. A strong {110}〈110〉 textured Ag substrate was obtained by cold rolling and annealing at 80$0^{\circ}C$: the full-width at half-maximum(FWHM) value of {110}〈110〉 poles was as sharp as 10$^{\circ}$. Surface morphology was evaluated by using Atomic force microscopy(AFM). Root-mean-square(RMS) roughness of the substrate annealed at 80$0^{\circ}C$ was 39.2 nm. The substrate of strong texture and smooth surface, fabricated in our study, is considered to be suitable for use as a substrate for deposition of superconductor films.

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CCD SURFACE PHOTOMETRY OF SPIRAL GALAXIES: BULGE MORPHOLOGY

  • Ann, Hong-Bae
    • Journal of The Korean Astronomical Society
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    • v.36 no.4
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    • pp.261-270
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    • 2003
  • We have conducted a V-band CCD surface photometry of 68 disk galaxies to analyze the bulge morphology of nearby spirals. We classify bulges into four types according to their ellipticities and the misalignments between the major axis of the bulge and those of the disk and the bar: spherical, oblate, pseudo triaxial, and triaxial. We found that one third of the bulges are triaxial and they are preponderant in barred galaxies. The presence of the triaxial bulges in a significant fraction of unbarred galaxies as well as in barred galaxies might support the secular evolution hypothesis which postulates that the bar driven mass inflow leads to the formation of triaxial bulges and the destruction of bars when sufficient mass is accumulated in the central regions.

Synthesis of Titanium Diboride and Composites by Carbothermic Reduction of Titanium Oxide and Boric Oxide

  • Yoon, Su-Jong;Jha, Animesh
    • The Korean Journal of Ceramics
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    • v.4 no.4
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    • pp.387-393
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    • 1998
  • The formation of titanium diboride ($TiB_2$ ) via the reduction of $TiO_2$ with boric oxide and carbon was studied in a partially reducing atmosphere of argon mixed with 4 vol.%H2. The effect of reaction time, temperature, partial pressure of nitrogen and $TiO_2/B_2_O3$ stoichiometric ratio on the reducibility of oxides has been studied. The phases formed were analysed by using X-ray rowder diffraction and scanning sosctron microscopic techniques. In this paper, we also investigated the presence of $CaC_2$ as a reducing agent on the reducibility of oxide mixtures and on the Ti-B-C-Ca-O phase equilibria. The morphology of $TiB_2$ formed in the presence of $CaC_2$ is compared with the microstructure of $TiB_2$ formed as a consequence of carbothermic reduction. The observed variation in $TiB_2$ crystals formed is also explained.

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Effect of Viscosity on the Morphology of Electrospun Polyacrylonitrile Fibers as a Linear Actuator and Artificial Muscles

  • Kim, Ye-Na;Lee, Deuk-Yong;Lee, Myung-Hyun;Lee, Se-Jong
    • Journal of the Korean Ceramic Society
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    • v.43 no.4 s.287
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    • pp.203-206
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    • 2006
  • Polyacrylonitrile (PAN) nanofibers, which are pH-sensitive and exhibit soft actuation as a linear actuator and artificial muscles, were prepared by electrospinning to investigate the effect of viscosity on the morphology of PAN fibers. Experimental results revealed that higher viscosity is critical for the formation of unbeaded nanofibers because surface tension is almost constant throughout the experiment. Uniform, smooth, and continuous fibers with diameters of about 700 nm were achieved for the 10 wt% PAN fibers at a flow rate of 0.5 mL/h and an electric field of 0.875 kV/cm.