• 자원환경지질
• /
• 제48권2호
• /
• pp.115-130
• /
• 2015

확장 탄성 임피던스(extended elastic impedance, EEI)는 입사각에 따른 음향 임피던스(acoustic impedance, AI) 를 일반화한 탄성 임피던스(elastic impedance, EI)를 확장한 개념으로서 다양한 저류암 물성과 대비가 가능한 것으로 알려져 있다. 하지만 EEI 역산을 적용하여 예측한 저류암적 물성이 실제 물성을 얼마나 정확히 예측하는지를 검증한 사례는 거의 없다. 본 연구에서는 EEI 역산 기법을 이용하여 미국 와이오밍주 Teapot Dome 유전의 주요 저류층 중 하나인 Second Wall Creek 사암층의 P파속도($V_p$), S파속도($V_s$), P파속도-S파속도 비($V_p/V_s$), 포아송비(Poisson's ratio)와 같은 속도 물성들을 유추하고 실제 물리검층 자료와 비교하여 EEI 역산 기법의 정확도를 검증했다. 사용된 자료는 Teapot Dome 유전 남부의 3차원 공심점 모음 자료(CDP gather)와 많은 시추공에서 선택된 4개의 시추공 자료이다. $V_s$ 검층자료는 경험식을 통해 $V_p$ 검층자료로부터 계산되었다. 4개의 속도 물성 EEI 예측 %에러는 한 시추공에서의 포아송비를 제외하면 약 5%를 넘지 않는다. 그러나 속도로부터 직접적으로 계산되지 않는 공극률, 감마선 검층값, 밀도와 같은 물성들은 시추공에서의 EEI 역산 분석 결과가 만족스럽지 못하여 전체 자료에 EEI 역산을 적용할 수 없었다. 따라서 속도 물성의 경우 EEI 역산을 적용할 수 있지만 속도로부터 직접 계산이 되지 않는 물성의 경우는 EEI 역산 적용에 신중해야 할 것으로 판단된다.

• 대한전자공학회논문지SD
• /
• 제41권11호
• /
• pp.21-27
• /
• 2004

본 논문에서는 60 GHz 무선 LAN(wireless local area network) 응용을 위해 0.1 ㎛ Γ-gate pseudomorphic high electron mobility transistor(PHEMT)를 이용하여 V-band용 millimeter-wave monolithic integrated circuit(MIMIC) 저잡음 증폭기를 설계 및 제작하였다. 본 연구에서 개발한 PHEMT의 DC 특성으로 드레인 포화 전류 밀도(Idss)는 450 mA/mm, 최대 전달컨덕턴스(gm, max)는 363.6 mS/mm를 얻었으며, RF 특성으로 전류이득 차단주파수(fT)는 113 GHz, 최대 공진 주파수(fmax)는 180 GHz의 성능을 나타내었다. V-band MIMIC 저잡음 증폭기의 개발을 위해 PHEMT의 비선형 모델과 CPW 라이브러리를 구축하였으며, 이를 이용하여 V-band MIMIC 저잡음 증폭기를 설계하였다. 설계된 V-band MIMIC 저잡음 증폭기는 본 연구에서 개발된 PHEMT 기반의 MIMIC 공정을 이용해 제작되었으며, V-band MIMIC 저잡음 증폭기의 측정결과, 60 GHz에서 S21이득은 21.3 dB, 입력반사계수는 -10.6 dB 그리고 62.5 GHz에서 출력반사계수는 -29.7 dB의 특성을 나타내었다. V-band MIMIC 저잡음 증폭기의 잡음지수 측정결과, 60 GHz에서 4.23 dB의 특성을 나타내었다.

• 지구물리와물리탐사
• /
• 제13권4호
• /
• pp.307-314
• /
• 2010

석유와 가스 등 지하자원 탐사를 위한 탄성파 탐사자료의 처리 및 해석에 있어서 이방성에 대한 연구는 매우 중요하다. 중합 및 구조보정 등 자료처리과정에 필요한 탄성파 속도를 등방성이라고 가정하였으나 실제 지하지질의 속도구조는 이방성을 가지는 경우를 흔히 볼 수 있는데, 특히 셰일층 또는 파쇄 및 절리 등 균열이 발달된 탄산염 저류층에서 이방성 특성을 찾아볼 수 있다. 본 연구에서는 합성수지인 베이클라이트로 만든 VTI매질을 대상으로 탄성파 축소모형실험을 이용하여 탄성파 이방성에 대한 연구를 수행하였다. 탄성파 모형실험에서 등방성 재료는 입사각의 변화에도 불구하고 속도가 항상 일정하지만, 이방성 매질의 경우 측정 방향 및 입사각에 따라 탄성파 P파 및 S파의 속도가 변화하였다. 측정된 탄성파 속도는 군속도로 추정되며 군속도로부터 구한 탄성계수를 이용하여 이방성계수인 ${\varepsilon}$, ${\delta}$, ${\gamma}$를 성공적으로 파악할 수 있었다. 이방성매질에서는 이론적으로 계산된 위상속도와 측정된 탄성파속도는 비교적 잘 일치하였으며, 또한 qP, qS, SH파의 위상속도를 slowness surface에서 나타내면 측정 매질에 대한 이방성 특성이 잘 표현되었다. S파의 경우 매질과 송수신기의 측정 방향에 따라 서로 다른 두 개의 횡파가 분극특성을 나타내며 전파됨을 확인할 수 있었다.

• 천문학회지
• /
• 제46권1호
• /
• pp.49-63
• /
• 2013

Nonthermal radiation from supernova remnants (SNRs) provides observational evidence and constraints on the diffusive shock acceleration (DSA) hypothesis for the origins of Galactic cosmic rays (CRs). Recently it has been recognized that a variety of plasma wave-particle interactions operate at astrophysical shocks and the detailed outcomes of DSA are governed by their complex and nonlinear interrelationships. Here we calculate the energy spectra of CR protons and electrons accelerated at Type Ia SNRs, using time-dependent, DSA simulations with phenomenological models for magnetic field amplification due to CR streaming instabilities, Alf$\acute{e}$enic drift, and free escape boundary. We show that, if scattering centers drift with the Alf$\acute{e}$en speed in the amplified magnetic fields, the CR energy spectrum is steepened and the acceleration efficiency is significantly reduced at strong CR modified SNR shocks. Even with fast Afv$\acute{e}$nic drift, DSA can still be efficient enough to develop a substantial shock precursor due to CR pressure feedback and convert about 20-30% of the SN explosion energy into CRs. Since the high energy end of the CR proton spectrum is composed of the particles that are injected in the early stages, in order to predict nonthermal emissions, especially in X-ray and ${\gamma}-ray$ bands, it is important to follow the time dependent evolution of the shock dynamics, CR injection process, magnetic field amplification, and particle escape. Thus it is crucial to understand the details of these plasma interactions associated with collisionless shocks in successful modeling of nonlinear DSA.

• 한국환경과학회:학술대회논문집
• /
• 한국환경과학회 1998년도 가을 학술발표회 프로그램
• /
• pp.1-1
• /
• 1998

Advanced (Chemical) oxidation processes (AOP) differ from most conventional ones in that hydroxyl radical(OH.) is considered to be the primary oxidant. Hydroxyl radicalcan react non-selectively with a great number of organic and inorganic chemicals. The typical rate constants of true hydroxyl radical reactions are in the range of between 109 to 1012 sec-1. Many processes are possible to generate hydroxyl radical. These include physical and chemical methods and their combinations. Physical means involves the use of high energy radiation such as gamma ray, electron beam, and acoustic wave. Under an applied high energy radiation, water molecules can be decomposed to yield hydroxyl radicals or aqueous electrons. Chemical means include the use of conventional oxidants such as hydrogen peroxide and ozone, two of the most efficient oxidants in the presence of promoter or catalyst. Hydrogen peroxide in the presence of a catalyst such as divalent iron ions can readily produce hydroxyl radicals. Ozone in the presence of specific chemical species such as OH- or hydrogen peroxide, can also generate hydroxyl radicals. Finally the combination of chemical and physical means can also yield hydroxyl radicals. Hydrogen peroxide in the presence of acoustic wave or ultra violet beam can generate hydroxyl radicals. The principles for hydroxyl radical generation will be discussed. Recent case studied of AOP for water treatment and other environmental of applications will be presented. These include the treatment of contaminated soils using electro-Fenton, lechate treatment with conventional Ponton, treatment of coal for sulfur removal using sonochemical and the treatment of groundwater with enhanced sonochemical processes.

• Journal of the korean society of oceanography
• /
• 제38권4호
• /
• pp.166-172
• /
• 2003

Multi­Sensor Core Logger (MSCL) is a useful system for logging the physical properties (compressional wave velocity, wet bulk density, fractional porosity, magnetic susceptibility and/or natural gamma radiation) of marine sediments through scanning of whole cores in a nondestructive fashion. But MSCL has a number of problems that can lead to spurious results depending on the various factors such as core slumping, gas expansion, mechanical stretching, and the thickness variation of core liner and sediment. For the verification of MSCL data, compressional wave velocity, wet bulk density, and porosity were measured on discrete samples by Hamilton Frame and Gravimetric method, respectively. Acoustic impedance was also calculated. Physical property data (velocity, wet bulk density, and impedance) logged by MSCL were slightly larger than those of discrete sample, and porosity is reverse. Average difference between MSCL and discrete sample at both sites is relatively small such as 22­24 m/s in velocity, $0.02­-0.08\;g/\textrm{cm}^3$ in wet bulk density, and 2.5­2.7% in porosity. The values also show systematic variation with sediment depth. A variety of factors are probably responsible for the differences including instrument error, various measurement method, sediment disturbance, and accuracy of calibration. Therefore, MSCL can be effectively used to collect physical property data with high resolution and quality, if the calibration is accurately completed.

• 국제물리치료학회지
• /
• 제10권1호
• /
• pp.1687-1694
• /
• 2019

Background: Although cranial electrotherapy stimulation (CES) is reported to have positive effects on mental functions such as depression and sleep improvement, detailed studies regarding awakening, attention and concentration among brain waves reflecting brain activity are lacking. Objective: To examine the effects of cranial electrotherapy stimulation (CES) on various electroencephalograms (EEGs) reflecting brain activities. Design: Randomized controlled clinical trial (single blind) Methods: This study selected 30 healthy adult women in their 20s who volunteered for this experiment. A total of 30 subjects were randomly assigned to three groups (Sham group, 0.5 Hz CES group, and 100 Hz CES group). EEGs were measured before and after the single CES, and the results were compared and analyzed. Results: The relative theta, alpha, and gamma waves indicated no significant differences in the interaction effects between time and group. The relative fast alpha wave only showed significant differences in the interaction effects between time and group in P4. The relative slow beta wave only indicated statistically significant differences in the interaction effects between time and group in T3 and T4. The relative mid and fast beta waves showed statistically significant differences in the interaction effects between time and group in all areas. Conclusions: These results suggest that a CES of 0.5 Hz awakens consciousness and has a positive influence on brain activity, while a CES of 100 Hz has a positive influence on thinking activity accompanying mental load during concentrating on one subject.

• 한국해안·해양공학회논문집
• /
• 제35권6호
• /
• pp.146-154
• /
• 2023

본 연구에서는 서해안 해상기상타워 2기에서 관측된 수면변동자료를 이용하여 해양특성을 구분하는 주요 인자인 첨두주기 T_p와 평균주기 T₀₂와 T_{m-1, 0}를 산정하고 이상자료의 비율, 상관관계 분석 및 최적 확률밀도함수를 추정하였다. 산정된 대표주기 중 첨두주기의 경우, 이상 자료의 비율은 각각의 지점에서 5.73 %, 0.67 %로 나타났으며, T₀₂는 4.35%, 0.01%, T_{m-1, 0}는 2.82%, 0.03%로 나타났다. 한편, T₀₂와 T_p 사이의 관계를 분석한 결과 각 지점별로 0.53, 0.63의 관계로 산정됐으며, T_{m-1, 0}와 T_p의 관계는 각각 1.15, 1.32로 나타났다. T₀₂와 T_{m-1, 0}는 서로 1.18, 1.22의 관계를 보이고 있었다. 산정된 대표주기의 최적 확률밀도함수를 추정한 결과, T_p는 각각의 지점에서 'Lognormal', 'Normal' 분포를 따르고 있었으며, T₀₂는 'Gamma', 'Normal' 분포, T_{m-1, 0}는 각각 'Log-normal', 'Normal' 분포가 우세한 것으로 나타났다. 이러한 결과는 서해안을 대상으로 수행되는 파랑 분석에 기초자료로 사용될 수 있을 것으로 판단된다.

• 동의신경정신과학회지
• /
• 제18권2호
• /
• pp.89-100
• /
• 2007

Objective : The purpose of this study is to examine relationship between cognitive function and sasang constitution by analyzing EEG status of company workers in Cheon-An. Method : 59 company workers were tested with cognitive assessment EEG program and questionaire for the Sasang Constitution Classification II. They were assorted by Sasang Constitutions, and we analyzed its correlation with cognitive assessment score and EEG data. Results : 1. According to mean active EEG rhythm of Alpha. H-Beta, Gamma wave, there were no significant difference among Sasang Constitution. 2. According to mean success, error, concentration, response, workload and left/right brain activity score, there were no significant difference among Sasang Constitution. 3. According to mean active EEG rhythm of Theta, SMR, M-Beta wave, Soyangin(少陽人)'s value was significantly higher than that of Taeumin(太陰人) 4. According to mean cognitive strenghth score, Soyangin(少陽人)'s value was significantly higher than that of Taeumin(太陰人). Conclusion : In conclusion, Sasang Constitutional difference has no relevance with cognitive abilities However, Soyangin(少陽人) showed higher mean active EEG rhythm of Theta, SMR, M-Beta wave than that of Taeumin(太陰人). In addition, Soyangin(少陽人) also showed higher mean cognitive strenghth score than that of Taeumin(太陰人).

• 천문학회보
• /
• 제43권2호
• /
• pp.31.3-31.3
• /
• 2018

On August 17th 2017, for the first time in the history, the gravitational wave (GW) detectors recorded signals coming from the merger of two neutron stars. This event was named as GW170817, and more interestingly, gamma-ray emission was detected 2 seconds after the gravitational wave signal, and 11 hours later, telescopes in Chile identified that the GW signal came from the NGC 4993 galaxy at the distance of about 40 Mpc. This is again the first time that electromagnetic (EM) signals are detected for a GW source. The follow-up observations by astronomers all around the world, including our group in Korea, successfully identified the optical emission as the kilonova, the elusive optical/NIR counterpart that has been proposed to originate from a neutron star merger. This whole event started the new era of astronomy, so-called the "multi-messenger astronomy", where the combined information from GW and EM radiation reveals an unprecedented view of the universe. In this talk, I summarize this exciting event, and describe the efforts by Korean astronomers that have led to important discoveries about the kilonova and the host galaxy properties, and finally provide the future prospects.