• Structural Engineering and Mechanics
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• 제74권3호
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• pp.425-434
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• 2020

The present paper is concerned at investigating the effect of hydrostatic initial stress, gravity and magnetic field in fiber-reinforced thermoelastic solid, with variable thermal conductivity. The formulation of the problem applied in the context of the three-phase-lag model, Green-Naghdi theory with energy dissipation, as well as coupled theory. The exact expressions of the considered variables by using state-space approaches are obtained. Comparisons are performed in the absence and presence of the magnetic field as well as gravity. Also, a comparison was made in the three theories in the absence and presence of variable thermal conductivity as well as hydrostatic initial stress. The study finds applications in composite engineering, geology, seismology, control system and acoustics, exploration of valuable materials beneath the earth's surface.

• 자원리싸이클링
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• 제27권6호
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• pp.11-22
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• 2018

자력선별장비는 일반적으로 광산업 및 재활용 분야에서 사용되어 왔으며, 다양한 분야에서 폭넓게 활용되고 있다. 자력선별장비는 비철재료로부터 철 스크랩 분리를 위한 조립자용 선별장비와 3 mm 이하 미립 강자성체를 농축하기 위한 미립자용 선별장비로 구분된다. 또한 미립자용 선별장비는 저자력 선별장비와 고자력 선별장비로 세분된다. 저자력 선별장비는 강자성체나 높은 자화율의 상자성체를 분리하는데 사용되고, 고자력선별장비는 낮은 자화율의 상자성체를 분리하는데 사용된다. 저자력 및 고자력 선별장비 모두 습식과 건식으로 활용된다. 최근 0.7 Tesla미만 영역에서 활용되는 전자석 고구배자력선별장비는 1980년대 이후 상용화된 희토류 영구자석으로 제조된 자력선별장비로 점진적으로 대체되는 추세이며, 환경분야와 생물분야에서 합성자성물질과 관련된 나노기술의 확대는 향 후 자력선별기술의 발전에 긍정적으로 기여할 것으로 기대된다.

• 한국지구과학회지
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• 제38권4호
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• pp.251-262
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• 2017

드론을 이용한 신뢰성 있는 항공자력탐사 수행을 위해서 자력탐사 시스템과 드론 시스템을 구성하여 철광산 지역 자력 탐사에 적용하였다. 드론에 실리는 자력탐사 시스템은 Bartington사의 플럭스게이트 자력계 Mag639를 센서로 사용하고, A/D convertor를 이용하여 태블릿PC에 자력값이 저장되도록 구성하였다. 드론의 비행 컨트롤 모듈로는 확장성이 좋은 Pixhawk를 사용하였고, 적재 중량(Payload) 3 kg, 최대 중량 적재 시 15분 동안 비행이 가능하도록 구성하였다. 드론의 자기장 간섭 범위 측정 실험을 통해 드론에 의한 자기장 간섭효과를 제거하였고, 정확한 위치 정보 확보를 위해 RTK GPS를 적용하였다. 정확한 위치정보를 토대로 동일한 측선에 대해서 고도를 변경하여 두 번 측정해서 자력 변화율 자료를 확보하였다. 또한 지형 정보를 사용하여 지형을 따라 비행하는 비행경로를 설정함으로써 지형 효과를 없앨 수 있었다. 드론 기반 항공자력탐사 시스템을 통해 획득된 자력자료는 Geometrics사의 핵자력계 G-858을 이용해 동일 지역에서 획득한 자료와 양상이 일치함을 확인하였고, 이를 통해 드론 기반 항공자력탐사 시스템을 이용한 탐사 자료에 대한 신뢰성을 확보할 수 있었다.

• 천문학회보
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• 제40권1호
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• pp.66.2-66.2
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• 2015

In today's age when telecommunications using satellite has become part of our daily lives, one has to be employ preventive measures to avert any possible danger, of which solar activity is the major cause. Coronal mass ejections (CMEs) heading towards the Earth can lead to disturbances in the Earth's magnetosphere, if their magnetic field is oriented southward. Monitoring of solar filaments in this case becomes very very crucial, as their eruption is associated with most of the CMEs. Monitoring of solar filaments in this case becomes very very crucial, as their eruption is associated with most of the CMEs. Also, filaments show activation up to a few hours prior to launch of a CME and thus can provide advance warning. In this study, we present an algorithm for the detection of solar filaments seen in the extreme ultraviolet (EUV) from Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO). Various morphological operations are employed to identify and extract the filaments. These filaments are then tracked in order to determine their size and location continuously.

• Journal of Astronomy and Space Sciences
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• 제17권2호
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• pp.233-240
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• 2000

Five scientific instruments are planned on KAISTSAT-4 that is scheduled to be launched in 2002. A far ultra-violet imaging spectrograph and a set of space plasma instruments are currently being designed. The imaging spectrograph will make observations of astronomical objects and Earth's upper atmosphere. The plasma instrumentation is capable of fast measuring the thermal magnetosphere plasmas, cold ionospheric plasmas and the Earth's magnetic fields. Major system drivers and constraints on the payloads as well as the spacecraft are identified. A preliminary analysis of the K-4 mission has been undertaken with the system requirements that are derived from the system drivers. Detailed investigation shows that Sun-synchronous orbits with approximate altitudes of 800km are optimal to satisfy the identified requirements. Comparisons with other orbits of different inclinations are also shown. Four operation modes and a daily schedule of spacecraft maneuver are found from the Sun-synchronous orbital model. It is shown that the scientific objectives of K-4 can be achieved with moderate levels of design and operation risks.

• Ocean and Polar Research
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• 제43권3호
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• pp.165-178
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• 2021

Gadolinium (Gd), one of a rare earth element (REE), has been widely used worldwide since the 1980s, as a resource material for contrast agents injected into examiners of magnetic resonance imaging (MRI) test. The organic complexed form of Gd shows an extremely stable behavior in natural environment (water), so is known that the artificial Gd from medical uses is not removed from the waste water treatment plant (WWTP) and eventually introduced into the ocean through the estuary. Since the 1990s, some previous studies have often been conducted on Gd anomalies in natural water and their effects an artificial origin from land or metropolitan areas, but little research has been potential impacts on the ocean water. In this paper, we review and introduce recent studies related to Gd anomaly in natural water and related marine effects, and also propose the future research directions.

• 한국진공학회:학술대회논문집
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• 한국진공학회 1998년도 제14회 학술발표회 논문개요집
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• pp.41-41
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• 1998

Rare earth metal films have been used as a buffer layer for growing ferroelectric t thin film or a seed layer for magnetic multilayer. But when it was deposited on s semiconductor substrates for the application of magneto-optic (MO) storage media, it i is difficult to exactly measure magnetic cons떠nts due to shunting current, and so it n needs to grow metal films on insulator substrate to reduce such effect. Recently, it w was reported that ultra-thin Pt layer were epitaxially grown on A12O:J by ion beam s sputtering in 비떠 high vacuum and it can be used as a seed layer for the growth of C Co-contained magnetic multilayer. In this stu$\phi$, Pt thin film were epi떠xially grown on AI2D3 ($\alpha$)OJ) by RF magnetron s sputtering. The crystalline structure was analyzed by transmission electron microscope ( (TEM) and Rutherford Back Scattering (RBS)/Ion Channeling. In TEM study, Pt was b believed to be twinned on AI잉3($\alpha$)01) su$\pi$ace about Pt(ll1) plane.Moreover, RBS c channeling spectra showed that minimum scattering yield of Pt(111)/AI2O:J(1$\alpha$)OJ) was 4 4% and Pt(11J)/AI2D3($\alpha$)OJ) had 3-fold symmetry.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2006년도 공동학술대회 논문집
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• pp.141-151
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• 2006

차량이 자력계를 끌면서 자기장을 측정하는 자력탐사시스템에서 차량 자체가 발생하는 잡음으로서의 자기장을 제거하기 위한 실험을 하였다. 차량 자체의 잔류자기 및 유도자기를 추출하기 위하여, 먼저 자력계를 고정된 점에 두고 차량을 이동하면서 자기장을 측정하였고, 이 자료로부터 차량을 고정된 점에 두고 자력계를 이동하면서 측정한 자료로 만들었으며, 후자의 자료로부터 역산을 통하여 차량 자체의 잔류자기 및 유도자기를 계산하였다. 한편, 차량 자력탐사시스템으로 측정한 각 측점의 자료로부터, 역산으로부터 계산한 차량 자체의 잔류자기 및 유도자기에 의해 발생하는 잡음으로서의 영향을 벡터적으로 제거 즉, 보정하여 자력이상을 추출하였다.

• 천문학논총
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• 제15권spc1호
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• pp.93-102
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• 2000

We have reviewed the magnetic activity in close binaries. Solar like magnetic activity indicators such as photometric spots, chromo spheric emission, coronal X-ray and radio emission, and flare activity are commonplace in many cool stars with convective envelopes. Using the UV spectra we confirmed the strength of stellar activity increases with more rapid rotation and later spectral types which corresponds to the increasing depth of the star's convective envelope. Apart from very young stellar objects such as T Tauri stars, the stars with the highest levels of activity are close binary systems composed of cool stars, i.e., the chromospherically active binaries such as RS CVn, BY Dra, W UMa and related systems. The IUE low and high dispersion spectra of V711 Tau, VW Cep and SW Lac are used for ultraviolet photometry and for a variation study of chromospheric activity. Evidence of chromospherically activity is indicated by the intensity variation of the Mg II emission line with orbital phase.

• 천문학회보
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• 제37권2호
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• pp.116.1-116.1
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• 2012

When an interplanetary (IP) shock passes over the Earth's magnetosphere, the geosynchronous magnetic field strength near the noon is always enhanced, while the geosynchronous magnetic field near the midnight decreases or increases. In order to understand what determines the positive or negative magnetic field response at nightside geosynchronous orbit to sudden increases in the solar wind dynamic pressure, we have examined 120 IP shock-associated sudden commencements (SC) using magnetic field data from the GOES spacecraft near the midnight (MLT = 2200~0200) and found the following magnetic field perturbation characteristics. (1) There is a strong seasonal dependence of geosynchronous magnetic field perturbations during the passage of IP shocks. That is, the SC-associated geosynchronous magnetic field near the midnight increases (a positive response) in summer and decreases (a negative response) in winter. (2) These field perturbations are dominated by the radial magnetic field component rather than the north-south magnetic field component at nightside geosynchronous orbit. (3) The magnetic elevation angles corresponding to positive and negative responses decrease and increase, respectively. These field perturbation properties can be explained by the location of the cross-tail current enhancement during SC interval with respect to geosynchronous spacecraft position.