• Title/Summary/Keyword: Form Evolution

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A Research for Tradition and Identity of Saam Acupuncture Method (사암침법의 전통과 독자성에 관한 연구)

  • Jung, Yoo-Ong;Lee, Duk-Ho;Ahn, Sang-Woo
    • Korean Journal of Acupuncture
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    • v.29 no.4
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    • pp.537-553
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    • 2012
  • Objectives : Ever Since it was made in the middle of 17th century by Saamdoin, Saam acupuncture method has been handed down to acupuncturists as a written form, playing a huge role in using for treating diseases of people in Korea. Saam acupuncture method development of any process, and have been propagated in a foreign country to study. Methods : Analysis of ancient medical books, we studied the evolution of Saam acupuncture method. And we looked abroad Saam acupuncture method have been propagated abroad by examining how. Results : At the end of Joseon Dynasty, lots of clinical cases were added to Saam acupuncture method and as a result, it helped acupuncturists understand how it really worked. During the Japanese colonial era, it was introduced to more people thanks to the development of a printing technique. After Korea's liberation from Japan, many scholars have studied Saam's acupuncture method, and they also have applied it to clinical cases in various ways. Conclusions : With its superiority and creativeness, Saam acupuncture method spread to Japanese acupuncturists in the name of Meridian Therapy during the Japanese colonial era. It had a great impact on medicine in China and many other countries, as well.

Ultrastructure of Spermatozoa of a Korean Bitterling, Acheilognathus koreensis (Pisces, Cyprinidae) (한국산 잉어과어류 칼납자루(Acheilognathus koreensis) 정자의 미세구조)

  • Kim, Kgu-Hwan;Kim, Jeong-Ki;Hwang, Ki-Ju
    • Korean Journal of Ichthyology
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    • v.19 no.4
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    • pp.286-291
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    • 2007
  • The bitterling, Acheilognathus koreensis spermatozoon has been examined by electron microscopy. The epididymal spermatozoa of A. koreensis are representing typical characteristic of cyprinid spermatozoa including the lateral insertion of flagellum, the organization of centriolar complex in shallow nuclear fossa and the asymmetrical arrangement of mitochondria. The sperm mid-piece contains a large mitochondrion characteristic enclosed by membranous vesicles. The mitochondria aspect is different from that of other cyprinid spermatozoa, which their mitochondria have a conventional aspect and never fuse to form a mitochondrial derivative. In term of sperm evolution, the fused mitochondria are regarded as the apomorphic character in comparison with the separate mitochondria. The single mitochondrion is not found in cyprinid spermatozoon except for Rodeus and Pungtungia.

OCCURENCE AND LUMINOSITY FUNCTIONS OF GIANT RADIO HALOS FROM MAGNETO-TURBULENT MODEL

  • CASSANO R.;BRUNETTI G.;SETTI G.
    • Journal of The Korean Astronomical Society
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    • v.37 no.5
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    • pp.589-592
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    • 2004
  • We calculate the probability to form giant radio halos (${\~}$ 1 Mpc size) as a function of the mass of the host clusters by using a Statistical Magneto-Turbulent Model (Cassano & Brunetti, these proceedings). We show that the expectations of this model are in good agreement with the observations for viable values of the parameters. In particular, the abrupt increase of the probability to find radio halos in the more massive galaxy clusters ($M {\ge} 2{\times}10^{15} M_{\bigodot}$) can be well reproduced. We calculate the evolution with redshift of such a probability and find that giant radio halos can be powered by particle acceleration due to MHD turbulence up to z${\~}$0.5 in a ACDM cosmology. Finally, we calculate the expected Luminosity Functions of radio halos (RHLFs). At variance with previous studies, the shape of our RHLFs is characterized by the presence of a cut-off at low synchrotron powers which reflects the inefficiency of particle acceleration in the case of less massive galaxy clusters.

MHD SIMULATIONS OF A MOVING SUB CLUMP WITH HEAT CONDUCTION

  • ASAI NAOKI;FUKUDA NAOYA;MATSUMOTO RYOJI
    • Journal of The Korean Astronomical Society
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    • v.37 no.5
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    • pp.575-578
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    • 2004
  • High resolution observations of cluster of galaxies by Chandra have revealed the existence of an X-ray emitting comet-like galaxy C153 in the core of cluster of galaxies A2125. The galaxy C153 moving fast in the cluster core has a distinct X-ray tail on one side, obviously due to ram pressure stripping, since the galaxy C153 crossed the central region of A2125. The X-ray emitting plasma in the tail is substantially cooler than the ambient plasma. We present results of two-dimensional magnetohydrodynamic simulations of the time evolution of a sub clump like C153 moving in magnetized intergalactic matter. Anisotropic heat conduction is included. We found that the magnetic fields are essential for the existence of the cool X-ray tail, because in non-magnetized plasma the cooler sub clump tail is heated up by isotropic heat conduction from the hot ambient plasma and does not form such a comet-like tail.

Nozzle Clogging Mechanism in Continuous Casting for Titanium-Containing Steel (티타늄 첨가강의 연주 노즐막힘 기구)

  • Jung, Woo-Gwang;Kwon, Oh-Duck;Cho, Mun-Kyu
    • Korean Journal of Materials Research
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    • v.19 no.9
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    • pp.473-480
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    • 2009
  • In order to provide the mechanism of nozzle clogging, recovered nozzles for high strength steel grade were examined carefully after continuous casting. The thickness of clogged material in SEN is increased in the following order: from the bottom to the top of the nozzle, upper part of slag line, and the pouring hole. Nozzle clogging material begins to form due the adhesion of metal to nozzle wall, the decarburization, and reduction of oxide in the refractory by Al and Ti in the melt. The reduction of oxide in the refractory by Al and Ti improves the wettability of the melt on the refractory and forms a thin Al-Ti-O layer. Metal containing micro alumina inclusions is solidified on the Al-Ti-O layer, and the solid layer grows due to the heat evolution through the nozzle wall. Thermodynamic calculation has been made for the related reactions. The effect of superheat to the nozzle clogging is discussed on ultra low carbon steel and low carbon steel.

A New Species of Genus Jaspis (Demospongiae: Astrophorida: Ancorinidae) from Korea (한국 벽옥해면속 (보통해면강: 별해면목: 안코리니과)의 1신종)

  • Sim Chung Ja;Lee Kyung Jin
    • Animal Systematics, Evolution and Diversity
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    • v.20 no.2
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    • pp.155-159
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    • 2004
  • A new species of the genus Jaspis (Demospongiae: Astrophorida: Ancorinidae), Jaspis coreana n. sp., is described on the specimen collected from Geomundo Island, Korea during September 1995 to March 2002 by SCUBA diving. This new species is characterized by two sponges association which is completely covered with Poecilastra wondoensis except for oscules. This new species is similar to J. wondoensis in its spicules type, but different in their spicules size, form of oscules and sponge colour. J. coreana has a large oxyasters and longer megascleres than J. wondoensis, oscule cluster and golden yellow colour in life.

Two New Euryspongian Sponges (Dictyoceratida: Dysideidae) from Korea

  • Lee, Kyung-Jin;Sim, Chung-Ja
    • Animal Systematics, Evolution and Diversity
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    • v.23 no.1
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    • pp.35-38
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    • 2007
  • Two new sponges, Euryspongia coreana n, sp, and E. regularis n, sp., collected from Hataedo, Ulleungdo and Chujado, Korea by SCUBA diving during the period from 2001 to 2005. Euryspongia coreana n. sp, is very close to E. lactea Row, 1911 and E. arenaria Bergquist, 1961 in skeletal structure, but primary and secondary fibres of the new species are thicker than those of E. lactea, E. arenaria is cored with mostly spicule fragments but E. coreana n. sp. is cored with mainly sand. E. regularis n. sp. is readily distinguished from other eurypsongian sponges. by its thickly encrusting growth form, yellowish ivory colour, and thickness of fibres. The bright yellow color and regular ladder-like skeletal structure are major features distinguishing this E. regularis n. sp. from other euryspongian sponges. Most species are brown, violet, red or orange in color except for E. lactea (milky white), E. arenaria (biscuit) and E. coreana n. sp. (yellowish ivory). Other euryspongian sponges have regularly or irregularly well developed secondary fibres, but E. regularis n. sp. has simple and regular secondary fibres.

Plan Dimension of the Wooden Architecture with a Special Reference of Yingzaofashi(營造法式) of Song Dynasty (송(宋) "영조법식(營造法式)" 을 통해 본 목조건축(木造建築) 평면(平面) 척도구성(尺度構成)의 고찰(考察))

  • Lee, Yong-Jun
    • Journal of architectural history
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    • v.14 no.3 s.43
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    • pp.119-128
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    • 2005
  • In ancient times, architectural design was seen as a critical task in building technologies. Specifically, form, dimension and structural design are of significant. These aspects are associated with each other and to be emerged as a whole. Designing plan dimension was deemed to be the core of design technology due to its close relationship with module system. Thus, its evolution as well as development process typically represents and reflects the spirits and contents of design technologies in ancient China. In China, the materials regarding ancient architectural technology include Yingzaofashi(營造法式) of Song Dynasty and Gongchengzuofazeli(工程做法則例) of Qing Dynasty. They show many aspects concerning materials, structure, scale system and building. In Yingzaofashi, although the length of objects are decided by 'cai(材)' and 'fen(分)', there are no regulations on length, width and height of a building. However, in the construction of ancient buildings, the above mentioned basic scales are very important in both design and construction. The present paper attempts to discuss the significance, namely, the design principles of length, with and height of ancient chinese architecture.

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Formation and evolution of mini halos around a dwarf galaxy sized halo - Candidate sites for the primordial globular clusters

  • Chun, Kyungwon;Shin, Jihye;Kim, Sungsoo S.
    • The Bulletin of The Korean Astronomical Society
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    • v.40 no.2
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    • pp.34.2-34.2
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    • 2015
  • We aim to investigate the formation of primordial globular clusters (GCs) in the isolated dwarf galaxy (${\sim}10^{10}M_{sun}$) with cosmological zoom-in simulations. For this, we modified cosmological hydrodynamic code, GADGET-3, in a way to include the radiative heating/cooling that enables gas particles cool down to T~10K, reionization (z < 8.9) of the Universe, UV shielding ($n_{shield}$ > $0.014cm^{-3}$), and star formation. Our simulation starts in a cubic box of a side length 1Mpc/h with 17 million particles from z = 49. The mass of each dark matter (DM) and gas particle is $M_{DM}=4.1{\times}10^3M_{sun}$ and $M_{gas}=7.9{\times}10^2M_{sun}$, respectively, thus the GC candidates can be resolved with more than hundreds particles. We found the following results: 1) mini halos with the more interactions before merging into the main halo form the more stars and thus have the higher star mass fraction ($M_{star}/M_{total}$), 2) the mini halos with the high $M_{star}/M_{total}$ can survive longer and thus spiral into closer to the galactic center, 3) the majority of them spiral into bulge, but some of them can survive until the last as baryon-dominated system, like the GC.

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Quasi-distributed Interference Coordination for HSPA HetNet

  • Zhang, Chi;Chang, Yongyu;Qin, Shuqi;Yang, Dacheng
    • ETRI Journal
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    • v.36 no.1
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    • pp.31-41
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    • 2014
  • The heterogeneous network (HetNet) has been discussed in detail in the Long-Term Evolution (LTE) and LTE Advanced standards. However, the standardization of High-Speed Packet Access HetNet (HSPA HetNet) launched by 3GPP is pushing at full steam. Interference coordination (IC), which is responsible for dealing with the interference in the system, remains a subject worthy of investigation in regard to HSPA HetNet. In this paper, considering the network framework of HSPA HetNet, we propose a quasi-distributed IC (QDIC) scheme to lower the interference level in the co-channel HSPA HetNet. Our QDIC scheme is constructed as slightly different energy-efficient non-cooperative games in the downlink (DL) and uplink (UL) scenarios, respectively. The existence and uniqueness of the equilibrium for these games are first revealed. Then, we derive the closed-form best responses of these games. A feasible implementation is finally developed to achieve our QDIC scheme in the practical DL and UL. Simulation results show the notable benefits of our scheme, which can indeed control the interference level and enhance the system performance.