• 한국지구과학회지
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• 제33권6호
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• pp.519-533
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• 2012

본 연구는 호주 남동부 Victoria 남부 해안을 따라 발달하고 있는 Otway 산맥 일대에서 지난 5 Ma 동안의 신기지체구조 운동의 성격을 해안 산악 지역을 따라 분포하고 있는 해안단구의 발달상을 통해 밝히고 있다. OSL 연대 측정으로부터 얻은 저위 해안단구면의 융기율은 판 내부 구조운동의 영향이 현생 지형 발달에 미치는 결과를 명확히 보여주고 있다. 또한 본 연구는 제4기 해안단구와 플라이오세 고해수준 기록 간의 층서적 관계를 통해 후기 신제3기 이후에 나타나는 지구조 운동의 변화적 속성을 밝히고 있다. 이와 같은 후기 신제3기 이후 가속화된 지구조 운동 반응은 호주-태평양판의 이동성의 변화와 이에 따른 경계 응력의 증가가 대륙 내부 응력 수준에도 영향을 미친 결과로 이해된다.

• Asian-Australasian Journal of Animal Sciences
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• 제17권7호
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• pp.1000-1006
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• 2004

Selenium and vitamin E are micronutrients essential for normal health and maintenance in poultry. They are necessary in preventing free radical damage to phospholipid membranes, enzymes and other important molecules. Two experiments were conducted in a semi-commercial environment to examine the effect of Se source and vitamin E level in diet on broiler performance and meat quality. Increasing vitamin E from 50 IU to 100 IU did not affect growth performance of broilers although the 24 h drip-loss was tended to be reduced (p=0.06). There was an interaction between vitamin E and the source of Se in glutathione peroxidase activity (GSH-Px) and Se concentration in excreta. Increasing vitamin E from 50 IU to 100 IU elevated GSH-Px and Se concentration in excreta by 42 IU/g Hb and 0.9 ppm for the organic Se group, respectively, but reduced GSH-Px and Se concentration in excreta by 16 IU/g Hb and 1.3 ppm for inorganic group, respectively. Vitamin E played no role in the feather coverage of the birds when scored on day 37. Organic Se is more effective in improving feather score and 24 h drip-loss, with a markedly higher deposition rate in breast muscle and a lower excretion rate in the excreta (p<0.05) compared to the inorganic Se source. Both vitamin E and the source of Se did not affect (p>0.05) the energy utilisation by birds.

• 한국보육지원학회지
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• 제12권4호
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• pp.151-181
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• 2016

This study examined professional development systems in America, England, and Australia, and devised ways to enhance early childhood teachers' professional development in Korea. To suggest effective ways to improve current professional development system and its operation, this research aimed to investigate first, advanced professional development systems and policies in three countries, America, England, and Australia, second, the process of teacher qualification and requirements for acquiring teacher credential and its maintenance, and lastly, the effort of quality control for professional development, its operation, and evaluation systems in three countries. Based on the analysis of the three country's systems, five solutions for effective professional development are suggested. First, it is necessary to differentiate requirements for teachers by the level of teacher credentials. Second, an incessant training process for professional development is required. Third, an individualized professional development plan should be set for an individual teacher for the best outcomes in professional competence. Fourth, instructors for professional development trainings are needed to ensure the quality of training. Lastly, individuals, organizations, and policy and its operation systems need to be considered holistically as a whole in the perspective of convergence in policy making and its operation for effective professional development.

• 천문학회보
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• 제39권2호
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• pp.61.1-61.1
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• 2014

IC 10 is one of the most well-known irregular starburst dwarf galaxies in the Local Group. Its low metal and oxygen abundance together with proximity make it an excellent laboratory to test star formation models, especially in low-metallicity systems like galaxies in the early Universe as well as many other local dwarfs. Among a number of active star forming regions, we have detected H2O kilo-maser emission in the south-east region of IC 10(IC 10 SE) using the Korean VLBI Network(KVN). This maser line is likely to be associated with a giant molecular cloud identified in IC 10 SE by former CO studies. Using the HI and CO data from the VLA and SMA archive, we probe the atomic and molecular gas properties of IC 10 SE. We discuss how the cool gas morphology and kinematics are related with maser and star formation activity in IC 10 SE.

• 한국지구과학회지
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• 제33권6호
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• pp.534-543
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• 2012

본 연구는 호주 남동부 지역 Otway 산맥 일대에서 확인되는 신기 지체구조 운동의 성격과 매커니즘을 규명하기 위해 현상적 융기 패턴과 중력이상 및 현생 응력 체계 등의 지구물리 자료간의 상관관계를 분석하였다. Otway 산맥의 융기축은 높은 중력값을 보이는 지역과 일치하는 반면 주변의 두꺼운 제3기 퇴적층 지역은 낮은 중력값을 보이는 지역과 일치하고 있어 높은 중력값의 이상 구간은 제3기 퇴적층 지역에 의해 구분되는 형태를 보여주고 있다. 한편 단층, 습곡 활동으로 특징되는 연구 지역 일대의 지질 구조 및 분포 패턴은 호주 남동부 지역의 현생 응력 체계와 잘 일치한다. 지형 고도와 중력 간의 양의 상관관계는 가설적으로 연구 지역 일대의 융기 운동이 대규모($10^2$ km 대)의 암석권 휨 현상에 의해 발생하고 있음을 보여주고 있으며, 판 경계 응력에 의한 암석권 내 기존 약대들의 재활성화는 이러한 대규모 변형 양식에 있어 중요한 역할을 담당하고 있는 것으로 판단된다.

• 디지털융복합연구
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• 제13권6호
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• pp.341-350
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• 2015

본 논문은 호주의 국가정신보건전략에 대한 주요 내용과 국가정신보건전략을 통한 정신보건개혁 이후의 변화들, 그리고 정신보건개혁에 대한 논의를 통해서 우리나라의 정신보건정책의 문제점들을 개선하기 위한 현실적인 시사점과 융복합 정책적 함의를 찾는데 그 목적이 있다. 1992년에 발표되어 2008년에 개정된 국가정신보건정책, 1993년부터 2014년까지 네 차례에 걸쳐 수립된 국가정신보건 5개년 계획, 2006년 호주정부협의회에 의해 수립된 정신보건실행계획, 그리고 2012년 호주정부협의회에서 채택한 국가정신보건개혁을 위한 로드맵(2012-2022)을 포함한 국가정신보건전략은 지난 20년 동안 호주의 정신보건개혁의 광범위한 과정을 선도하는 대단히 중요한 정책 준거를 제공하였다. 1992년 시작된 국가정신보건전략을 통해서 정신보건재정 확충, 지역사회 중심의 치료 및 보호시스템 구축, 정신병상의 변화, NGO의 참여와 역할의 증대, 정신장애인과 가족(보호제공자)의 참여 확대 등과 같은 변화를 이루었다.

• 천문학회보
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• 제40권2호
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• pp.35.2-35.2
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• 2015

We present the results of simultaneous observations of the H2O and SiO masers emitted from the circumstellar envelopes (CSEs) of the late-type stars. These observations have been carried out at the four frequency bands (K, Q, W and D bands) using KVN to apply the source frequency phase referencing (SFPR) analysis to the maser lines. We obtain the relative positions between the H2O and the SiO maser spots by using the SFPR method, which are very important to study the physical links between the inner and the outer parts of the CSEs of the late-type stars. The relative positions between the SiO maser spots of the different transitions are also obtained very accurately, which are very crucial to investigate the pumping mechanism of the SiO maser lines. From our results, the capability of the simultaneous multi-band observation of KVN is proved to be powerful to study the complicated physical environments of the CSEs and the stellar evolution of the late-type stars.

• 한국토양비료학회지
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• 제49권1호
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• pp.93-114
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• 2016

As a means of improving Korean Soil Classification System, we have reviewed Australian Soil Classification System by comparing Soil Taxonomy and FAO/WRB Classification System. Australian Soil Classification System is composed of 14 of Order, 87 of Sub-order, 556 of Great-group, 2,451 of Sub-group, and 7,276 of Family. Interestingly, soil order has the Anthroposols which is not classified with Soil Taxonomy, and the classification for some of soils is based on soil texture abruption horizon and soil structure. Seven of 14 soil orders are classified with an old version based on soil color rather than morphological characteristics. The distribution scale of Australian soil order is the largest in Tenosols, and followed by Kandosols, Rudosols, Sodosols and Vertisols in Australia.

• 천문학회보
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• 제41권2호
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• pp.62.2-62.2
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• 2016

We present a newly developed algorithm based on a Bayesian method for 2D tilted-ring analysis of disk galaxies which operates on velocity fields. Compared to the conventional ones based on a chi-squared minimisation procedure, this new Bayesian-based algorithm less suffers from local minima of the model parameters even with high multi-modality of their posterior distributions. Moreover, the Bayesian analysis implemented via Markov Chain Monte Carlo (MCMC) sampling only requires broad ranges of posterior distributions of the parameters, which makes the fitting procedure fully automated. This feature is essential for performing kinematic analysis of an unprecedented number of resolved galaxies from the upcoming Square Kilometre Array (SKA) pathfinders' galaxy surveys. A standalone code, the so-called '2D Bayesian Automated Tilted-ring fitter' (2DBAT) that implements the Bayesian fits of 2D tilted-ring models is developed for deriving rotation curves of galaxies that are at least marginally resolved (> 3 beams across the semi-major axis) and moderately inclined (20 < i < 70 degree). The main layout of 2DBAT and its performance test are discussed using sample galaxies from Australia Telescope Compact Array (ATCA) observations as well as artificial data cubes built based on representative rotation curves of intermediate-mass and massive spiral galaxies.

• 천문학회보
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• 제46권2호
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• pp.71.1-71.1
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• 2021

We perform disk-halo decomposition of the Large Magellanic Cloud (LMC) using a novel HI velocity field extraction method, aimed at better deriving its HI kinematics and thus mass distribution in the galaxy including both baryons and dark matter. We decompose all the line-of-sight velocity profiles of the combined HI data cube of the LMC, taken from the Australia Telescope Compact Array (ATCA) and Parkes radio telescopes with an optimal number of Gaussian components. For this, we use a novel tool, the so-called BAYGAUD which performs profile decomposition based on Bayesian MCMC techniques. From this, we disentangle turbulent non-ordered HI gas motions from the decomposed gas components, and produce an HI bulk velocity field which better follows the global circular rotation of the galaxy. From a 2D tilted-ring analysis of the HI bulk velocity field, we derive the rotation curve of the LMC after correcting for its transverse, nutation and precession motions. The dynamical contributions of baryons like stars and gaseous components which are derived using the Spitzer 3.6 micron image and the HI data are then subtracted from the total kinematics of the LMC. Here, we present the bulk HI rotation curve, the mass models of stars and gaseous components, and the resulting dark matter density profile of the LMC.