• 한국의류학회지
• /
• 제41권5호
• /
• pp.929-938
• /
• 2017

This research investigated the effects of cool touch fabrics on thermo-regulating physical properties and subjective evaluation using a 3D fitted women's T-shirts in wear test. Qmax, clothing microclimate, microclimate wettedness, thermogram and subjective vote were observed during rest-right after an exercise-rest protocol. As a result, there was no single determining physical variable to explain the reasons of cool sensations of T-shirts made of cool touch fabric across the entire protocol. Qmax could partly predict a wear sensation at the initial stage when only insensible perspiration was presented. Simultaneous observation of temperature/humidity gradient understand from the inside to the outside of the clothing layer or microclimate wettedness calculated using vapor pressure were helpful to figure out the performance of cool touch fabric, especially at the later stage of the protocol when sweating was excessive. It was especially difficult to connect thermo-regulating physical variables to the subjective evaluation during transient conditions such as 'right after exercise' stage. It is necessary to measure the amount of heat and moisture transferred from the skin to the outside of clothing along with the physical properties measured in this study to understand the detailed mechanisms of why a cool sensation is evoked from tight fitting T-shirts made of newly developed cool touch fabrics.

• Journal of Astronomy and Space Sciences
• /
• 제12권1호
• /
• pp.90-101
• /
• 1995

GPS률 이용하여 보현산 천문대 2지점의 3차윈 정밀좌표를 WGS 84 측지좌표계상에서 결정하였다. 보현산 천문대 2지점에서 1지점은 1.8m 망윈경의 받침대 중앙이고 나머지 l지점은 1.8m 망원경 돔 옆의 언덕에 위치해 있다, 이 연구를 위해셔 1993년 12월18일부터 1 12월22일까지 5일 동안 천문대 GPS 관측소와 보현산 천문대 2지점에셔 동시에 GPS 관측을 실시하였다. 관측에 사용한 장비는 천문대에서 보유하고 있는 3대의 Trimble 4000SST GPS 수신기이다. 관측자료는 Trimble의 자료처리 소프트웨어인 TRIMVEC-PLUS의 MBPS 방식에 의하여 Triple Difference Ll/L2 ION Free 기법으로 처리 되었다. 이 연구를 통하여, 보현산 천문대 1.8m 망원경 축의 WGS 84 좌표값은 위도, 경도, 높이 각각 $36^{circ}9'53".1943N\pm0."0018,\;128^{circ}58'35".6829E\pm0."0029,\;1162.47m\pm0.04m$로 결정되었다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
• /
• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
• /
• pp.31.2-31.2
• /
• 2008

We present the results offar ultraviolet (FUV, 1350-1750 ${\AA}$) auroral observations made by the Far-ultraviolet IMaging Spectrograph (FIMS) instrument on the Korean microsatellite STSAT-1. The instrument was capable of resolving spatial structures of a few kilometers with the spectral resolution of 2-3 ${\AA}$. The observations were carried out simultaneously with the measurement of precipitating electrons using an electrostatic analyzer (ESA, 100 eV-20 keV) and a solid state telescope (SST, 170 keV-360 keV) on board the same satellite. With a careful mapping of the field lines, we were able to correlate the particle spectrum to the corresponding FUV spectrum of the footprints of the FIMS image that varied significantly in fine scales. We divided the FIMS spectral band into the LBH long (LBHL, 1640-1715 ${\AA}$) and LBH short (LBHS, 1380-1455 ${\AA}$) bands, and compared the electron energies with the intensities of LBHL and LBHS for the well-defined inverted-V structures. The result shows a strong correlation between the total LBH intensity and the energy flux measured by ESAwhile the peak energy itself does not correlate well with the LBH intensity. On the other hand, it was observed that the ratio of the LBHL intensity to that of LBHS increased significantly as the peak electron energy increased, primarily due to a smaller absorption by O2 at LBHL than at LBHS.

• 한국정보통신학회논문지
• /
• 제4권5호
• /
• pp.977-984
• /
• 2000

도플러 레이더를 이용하여 적도 해안 지역의 대기 경계층을 분석하였다. 인도네시아의 Serpong 지역(6.4S,106.7E)에 설치된 L밴드 경계층 레이더(1357.5 MHz) 는 1992년 11월부터 지속적인 관측을 수행하고 있다. 건조(10-12 October 1993)에 경계층 내에서 두 가지 형태의 강한 에코를 확인하였다. 첫 번째는 오전에 300 m 이하에서 나타나기 시작하여 오후에 3-5 knl 까지 이르는 강한 에코로써 그 정부는 혼합층의 고도와 일치해보였다. 이 적도 지역에서의 혼합고는 중위도 지역에서의 혼합고 보다 높다. 야간에 2-3 km 에 나타나는 두 번째 에코는 습도의 변화와 관련이 있는 것으로 보인다. 우기(20-21 February 1994)에 관측된 혼합층의 높이는 건기 보다 낮았다.

• Journal of Communications and Networks
• /
• 제5권2호
• /
• pp.157-166
• /
• 2003

This paper deals with the problem of channel identification for Single Input Multiple Output (SIMO) slow fading channels using clustering algorithms. Due to the intrinsic memory of the discrete-time model of the channel, over short observation periods, the received data vectors of the SIMO model are spread in clusters because of the AWGN noise. Each cluster is practically centered around the ideal channel output labels without noise and the noisy received vectors are distributed according to a multivariate Gaussian distribution. Starting from the Markov SIMO channel model, simultaneous maximum ikelihood estimation of the input vector and the channel coefficients reduce to one of obtaining the values of this pair that minimizes the sum of the Euclidean norms between the received and the estimated output vectors. Viterbi algorithm can be used for this purpose provided the trellis diagram of the Markov model can be labeled with the noiseless channel outputs. The problem of identification of the ideal channel outputs, which is the focus of this paper, is then equivalent to designing a Vector Quantizer (VQ) from a training set corresponding to the observed noisy channel outputs. The Linde-Buzo-Gray (LBG)-type clustering algorithms [1] could be used to obtain the noiseless channel output labels from the noisy received vectors. One problem with the use of such algorithms for blind time-varying channel identification is the codebook initialization. This paper looks at two critical issues with regards to the use of VQ for channel identification. The first has to deal with the applicability of this technique in general; we present theoretical results for the conditions under which the technique may be applicable. The second aims at overcoming the codebook initialization problem by proposing a novel approach which attempts to make the first phase of the channel estimation faster than the classical codebook initialization methods. Sample simulation results are provided confirming the effectiveness of the proposed initialization technique.

• 한국지반공학회:학술대회논문집
• /
• 한국지반공학회 2000년도 가을 학술발표회 논문집
• /
• pp.705-712
• /
• 2000

The fluid generally flows through fractures in crystalline rocks where most of underground storage facilities are constructed because of their low hydraulic conductivities. The fractured rock is better to be conceptualized with a discrete fracture concept, rather continuum approach. In the aspect of fluid flow in underground, the simultaneous flow of groundwater and gas should be considered in the cases of generation and leakage of gas in nuclear waste disposal facilities, air sparging process and soil vapor extraction for eliminating contaminants in soil or rock pore, and pneumatic fracturing for the improvement of permeability of rock mass. For the purpose of appropriate analysis of groundwater-gas flow, this study presents an unsteady-state multi-phase FEM fracture network simulator. Numerical simulation has been also conducted to investigate the hydraulic head distribution and air tightness around Ulsan LPG storage cavern. The recorded hydraulic head at the observation well Y was -5 to -10 m. From the results obtained by the developed model, it shows that the discrete fracture model yielded hydraulic head of -10 m, whereas great discrepancy with the field data was observed in the case of equivalent continuum modeling. The air tightness of individual fractures around cavern was examined according to two different operating pressures and as a result, only several numbers of fractures neighboring the cavern did not satisfy the criteria of air tightness at 882 kPa of cavern pressure. In the meantime, when operating pressure is 710.5 kPa, the most areas did not satisfy air tightness criteria. Finally, in the case of gas leaking from cavern to the surrounding rocks, the resulted hydraulic head and flowing pattern was changed and, therefore, gas was leaked out from the cavern ceiling and groundwater was flowed into the cavern through the walls.

• 천문학회지
• /
• 제48권5호
• /
• pp.237-255
• /
• 2015

The Interferometric Monitoring of Gamma–ray Bright Active galactic nuclei (iMOGABA) program provides not only simultaneous multifrequency observations of bright gamma–ray detected active galactic nuclei (AGN), but also covers the highest Very Large Baseline Interferometry (VLBI) frequencies ever being systematically monitored, up to 129 GHz. However, observation and imaging of weak sources at the highest observed frequencies is very challenging. In the second paper in this series, we evaluate the viability of the frequency phase transfer technique to iMOGABA in order to obtain larger coherence time at the higher frequencies of this program (86 and 129 GHz) and image additional sources that were not detected using standard techniques. We find that this method is applicable to the iMOGABA program even under non–optimal weather conditions.

• 응용통계연구
• /
• 제29권5호
• /
• pp.807-822
• /
• 2016

LN-GPD 합성 분포는 몸통부분은 로그-정규분포를 두터운 꼬리에 대해서는 GPD분포를 따르도록 합성한 분포로 두터운 몸통과 꼬리를 동시에 가지는 자료를 절삭없이 효율적으로 다룰 수 있는 분포이다. 하지만 임계점을 포함하고 있기에 최대우도추정량은 매우 불안정함이 잘 알려져 있어 본 논문이서는 이를 극복하기 위해서 임계점을 먼저 추정하고 나머지 모수들에 대해서 따로 추정하는 2단계 추정 방법들에 대해서 살펴보고 그 성능을 비교해 보았다. 그 결과 동시 추정하는 최대우도추정량의 경우 불안정한 추정이 GPD 분포의 꼬리 지수에서 두드러 졌으며 임계점에 대해서는 비교적 잘 추정함을 알 수 있었다. 이와 반대로 여러 비모수적인 방법들은 꼬리 지수는 만족스럽게 잘 추정하였으나 임계점의 경우 편의가 있음을 관찰할 수 있었다. 실증자료 분석을 위해 2단계 추정법을 이스라엘 은행의 콜센터에서 수집한 서비스 시간에 대한 자료에 적합해 보았으며 그 결과 LN-GPD 합성 분포를 사용하는 것이 로그-정규분포 혹은 GPD 분포 단독으로 사용하는 것보다 자료의 손실도 없이 더 좋은 적합도를 보임을 알 수 있었다.

• 한국해양학회지
• /
• 제13권1호
• /
• pp.29-34
• /
• 1978

인천항 부근해역은 우리나라 연안에서 가장 조차가 큰 천해역으로서 연안 및 섬주위로 간석지가 매우 잘 발달되어 있다. 따라서 동 해역은 오래전부터 큰 조차를 이용한 조력발전 후보지로 인정되어 왔고 앞으로의 개발전망이 밝을 뿐 아니라 광대한 간석지를 개발하기 위한 간척사업 후보지로 각광을 받고 있다. 이와 같은 개발계획의 대상으로 인정되는 해역에 있어서의 조류에 대한 정확한 조사연구는 중요한 일이라 생각된다. 인천항 부근해역의 조류에 관해서는 이(1963), 강(1972) 및 이(1972)등의 조사보고가 있는데 이들 조사관측 및 국내에서 실시되어 온 일반적인 조류관측은 거의 대부분이 동시관측에 의한 것이 아닐뿐더러 각 조기별 즉, 대조, 중조, 소조,기별로 실시된 것이 아니므로 각 조기별로 또한 각 지역별로 동시에 나타나는 조류의 특성을 비교하는 데에는 문제점이 있었다 하겠다. 우리나라 남해안이나 특히 서해안과 같이 조석이 큰 해역에서는 각 조기별로 조류의 특성이 매우 다르기 때문에 이를 비교파악 하기 위한 여러 지점에서의 조기별 동시 조류관측은 매우 어렵지만 의미있는 일이라 생각된다. 본조사에 있어서는 특히 이러한 점을 최대한으로 고려하여 실시되었다.

• 천문학회보
• /
• 제36권2호
• /
• pp.61.1-61.1
• /
• 2011

We have performed simultaneous observations at 22GHz and 43GHz on AGNs hosted by elliptical galaxies using KVN radio telescope. We have constructed the sample, based on two major surveys in radio and optical band, i.e. Faint Images of the Radio Sky at Twenty-Centimeters (FIRST) and Sloan Digital Sky Survey (SDSS) DR7, respectively. We restricted the redshift range 0.01 < z < 0.06 and the absolute magnitude Mr < -19.4 in order to satisfy volume limited sample. We also checked clear detection of four distinctive emission lines ([NII], [OIII], $H{\alpha}$, $H{\beta}$) so as to utilize on BPT diagram, distinguishing AGNs from star-forming galaxies. Elliptical galaxies have been selected by visual inspection making use of SDSS optical images. Then, we cross-matched the elliptical galaxies with FIRST detections. About 35% of the galaxies have been detected throughout KVN observations. We derive spectral index, applying the flux of different radio frequencies from FIRST (1.4GHz) and KVN (22GHz) and classify into steep, flat or inverted spectrum. We have found that most of the detected galaxies have flat spectrum while the rest of them have steep spectrum. This implies that a number of detected galaxies might have compact structure associated with the central region of the galaxies. The relation between black hole mass and radio luminosity has shown relatively tighter correlation in high frequency than in low frequency, which confirms that high frequency in radio band is appropriate to study the center of the galaxies.