• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2007년도 공동학술대회 논문집
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• pp.81-86
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• 2007

Spectral features of the seismic wave propagation from Odaesan Earthquake were evaluated based on the commonly treated random error between the observed data and the prediction values by the stochastic point-source ground-motion spectral model regarding the source, path and site effects. Radiation pattern of the error according to azimuth angle was found to be similar to the theoretical estimate. It was also observed that the spatial distribution of the errors was correlated with the geological map and the Q0 map which are indicatives of seismic boundaries.

• 지구물리와물리탐사
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• 제10권4호
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• pp.241-251
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• 2007

본격적인 지진관측 이래 최대 규모의 내륙 지진으로 기록된 오대산지진의 관측 스펙트럼을 이용하여, 점지진원 스펙트럼 모델의 지진원 크기 및 오차의 공간적인 특성을 평가하였다. 먼저 지진원 스펙트럼을 추정하기 위해, 최근까지 국내에 축적된 지진자료를 기반으로 비교적 상세하게 추정된 추계학적 지진동모델(Boore, 2003)의 지진파 전달, 부지특성(연관희, 2007)을 이용하여 관측 자료를 보정하였다. 추정된 오대산지진의 지진원 스펙트럼을 $1-f_c$(1개의 코너주파수) Brune의 ${\omega}^2$ 지진원모델에 적합한 결과, 기존에 제시된 지진규모-응력강하량 대표모델(연관희 등, 2006)에 의해 잘 예측되었으며, 오대산지진의 지진원 스펙트럼은 최근까지 한반도 인근에서 발생한 중규모 이상의 지진원 스펙트럼으로부터 추정된 $2-f_c$(2개의 코너주파수)의 경험적인 지진원모델에 보다 잘 부합되었다. 또한 일반적으로 무작위 잡음으로 취급되는 점지진원 지진파 스펙트럼 모델링 오차에 대해 방위각에 따른 방향성과 지역별 전달특성을 평가한 결과, 오차가 완전한 무작위 특성이 아님을 확인할 수 있었다. 이러한 모델링 오차의 방향성은 이론적으로 추정된 방사패턴과도 매우 유사한 관측된 방사패턴을 나타내었으며, 지역별로는 지질학적인 경계 혹은 지진파전달의 불연속적 특성과 밀접한 관계가 있는 것으로 판단되는 주파수별로 상이한 공간적인 분포 특성을 보여주었다.

• 지구물리와물리탐사
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• 제11권2호
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• pp.137-147
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• 2008

2007년 1월 20일 발생한 '오대산지진(M = 4.8)'의 특징적인 점은 근거리 지역 관측소인 DGY(기상청 대관령, 진앙거리 = 7 km)에서 기록된 비정상적으로 높은 PGA(최대지반가속도) 관측값(< 0.1 g)이다. 한편 DGY 관측소는 진앙지인근에 위치한 매우 양호한 지진관측소(연관희와 서정희, 2007)로 분류되므로 지진파전달이나 부지증폭특성으로는 설명될 수 없으며, 고주파지진동에 큰 영향을 주는 지진원 특성인 단층파열방향성(rupture directivity)에 의한 것으로 예비 해석될 수 있다. 이 연구에서는 Boatwright (2007)의 방법을 이용하여 단층파열속도(v)의 전단파속도(c)에 대한 상대적 비(= v/c) 및 파열진행방향과의 이격각(${\theta}$, deviation angle)에 대한 함수로 주어지는 일방향 단층파열방향성(unilateral rupture directivity)을 추정하였다. 이러한 단층파열방향성을 평가하기 위해 진앙지 인근 지역의 지진관측소에 대한 점지진원 스펙트럼 모델(Boore, 2003)에 대한 예측오차를 오대산지진의 전 여진 관측자료을 이용하여 계산한 후, 본진 관측자료를 이용한 예측오차와 상대적으로 비교하였다. 본진의 전 여진에 대한 상대적인 스펙트럼 예측오차로부터 관측소별 PGA의 상대적인 크기를 추정하고 이 결과를 이용하여 오대산지진의 단층파열 방향성을 평가한 결과, 오대산지진 인근에서의 높은 PGA 관측값은 NWW-SEE 방향의 북측으로 고각을 갖는 단층면상에서 SE 방향을 따라 거의 수직하게 지표면으로 빠르게 진행된 단층파열의 영향으로 해석되었다.

• 천문학회지
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• 제52권1호
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• pp.1-9
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• 2019

We present the results of the spectral and temporal analysis of eight X-ray point sources in five nearby (distance < 20 Mpc) galaxies observed with Chandra. For spectral analysis, an absorbed powerlaw and an absorbed diskblackbody were used as empirical models. Six sources were found to be equally fitted by both the models while two sources were better fitted by the powerlaw model. Based on model parameters, we estimate the X-ray luminosity of these sources in the energy range 0.3 - 10.0 keV, to be of the order of ${\sim}10^{39}ergs\;s^{-1}$ except for one source (X-8) with $L_X>10^{40}ergs\;s^{-1}$. Five of these maybe classified as Ultraluminous X-ray sources (ULXs) with powerlaw photon index within the range, ${\Gamma}{\sim}1.63-2.63$ while the inner disk temperature, kT ~ 0.68 - 1.93 keV, when fitted with the disk blackbody model. The black hole masses harboured by the X-ray point sources were estimated using the disk blackbody model to be in the stellar mass range, however, the black hole mass of one source (X-6) lies within the range $68.37M_{\odot}{\leq}M_{BH}{\leq}176.32M_{\odot}$, which at the upper limit comes under the Intermediate mass black hole range. But if the emission is considered to be beamed by a factor ~ 5, the black hole mass reduces to ${\sim}75M_{\odot}$. The timing analysis of these sources does not show the presence of any short term variations in the kiloseconds timescales.

• 한국음향학회:학술대회논문집
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• 한국음향학회 1994년도 FIFTH WESTERN PACIFIC REGIONAL ACOUSTICS CONFERENCE SEOUL KOREA
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• pp.791-795
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• 1994

In this paper, the echo phenomena of Yingying Pagoda(ancient Chinese architecture), which may be resulted from interferences of reflection and diffraction by the pagoda eaves when pulse sound source is at some suitable positions, are investigated by an 1:2 scale model. There are valleys in frequency spectrum due to the interferences. On the other hand, taking eaves as wedges approximately, numerical spectral estimates are obtained from the closed-form impulse solution for diffraction of pulse point-source radiation by an infinite rigid wedge. The results of the numerical computations are similar to those of the model experiments. The study is a helpful guide to reconstruction or maintenance of this kind of ancient buildings.

• Journal of Astronomy and Space Sciences
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• 제15권2호
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• pp.291-295
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• 1998

We investigate models for the IRAS LRS)Low Resolution Spectra) of OH/IR stars. OH/IR stars often show the silicate features at 9.7 ${mu}m$ and $18{mu}m$ in the spectra obtained by the IRAS LRS as well as remarkably red values in the IRAS photometric colors such as [60]-[25] and [25]-[12]. We compare the radiative transfer model results with observed spectral energy distributions (SEDs) of the stars including IRAS PSC(Point Source Catalog), IRAS LRS and ground based observational data.

• ETRI Journal
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• 제39권3호
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• pp.398-405
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• 2017

In this paper, an artificial stereo extension method that creates stereophonic sound from a mono sound source is proposed. The proposed method first trains deep neural networks (DNNs) that model the nonlinear relationship between the dominant and residual signals of the stereo channel. In the training stage, the band-wise log spectral magnitude and unwrapped phase of both the dominant and residual signals are utilized to model the nonlinearities of each sub-band through deep architecture. From that point, stereo extension is conducted by estimating the residual signal that corresponds to the input mono channel signal with the trained DNN model in a sub-band domain. The performance of the proposed method was evaluated using a log spectral distortion (LSD) measure and multiple stimuli with a hidden reference and anchor (MUSHRA) test. The results showed that the proposed method provided a lower LSD and higher MUSHRA score than conventional methods that use hidden Markov models and DNN with full-band processing.

• Earthquakes and Structures
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• 제8권5호
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• pp.1055-1067
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• 2015

A theoretical procedure to estimate spectral displacement of a hysteretic oscillator with bilinear stiffness excited by band-limited excitation is presented. The stochastic method of ground-motion simulation is combined with the random vibration theory to compute linear and nonlinear structural response. The response is obtained by computing the root-mean-square oscillator response using dissipation energy balancing by integrating over all energy levels of system weighting with the stationary probability density of the energy. The results are presented in a convenient form, and the accuracy of the procedure is assessed by comparison with results obtained with the time-domain method using the recorded data. The model shows little or no bias at the structural period of engineering interest.

• 한국지진공학회논문집
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• 제28권3호
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• pp.159-164
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• 2024

Recent earthquakes in Korea, like Gyeongju and Pohang, have highlighted the need for accurate seismic hazard assessment. The lack of substantial ground motion data necessitates stochastic simulation methods, traditionally used with a simplistic point-source assumption. However, as earthquake magnitude increases, the influence of finite faults grows, demanding the adoption of finite faults in simulations for accurate ground motion estimates. We analyzed variations in simulated ground motions with and without the finite fault method for earthquakes with magnitude (Mw) ranging from 5.0 to 7.0, comparing pseudo-spectral acceleration. We also studied how slip distribution and hypocenter location affect simulations for a virtual earthquake that mimics the Gyeongju earthquake with Mw 5.4. Our findings reveal that finite fault effects become significant at magnitudes above Mw 5.8, particularly at high frequencies. Notably, near the hypocenter, the virtual earthquake's ground motion significantly changes using a finite fault model, especially with heterogeneous slip distribution. Therefore, applying finite fault models is crucial for simulating ground motions of large earthquakes (Mw ≥ 5.8 magnitude). Moreover, for accurate simulations of actual earthquakes with complex rupture processes having strong localized slips, incorporating finite faults is essential even for more minor earthquakes.