• 대한지리학회지
• /
• 제39권6호
• /
• pp.819-832
• /
• 2004

본 연구에서는 한국의 14개 지점의 여름철 강수량을 분석하여 1941-1970년과 1971-2000년 기간 사이의 변동을 파악하고. 순별 강수량의 경년 변동과 해양변동 및 전구평균기온 변동과의 관련성을 파악하고자 하였다. 두 기간의 순별 강수량 차이에 의하여 중서부지역, 호남지역, 영동 및 영남지역. 제주도지역으로 구분하였다. 강수량은 8월에 증가하였고 9월에 감소하였다. 중서부지역에서 8월 강수량의 증가 폭이 크며, 이는 호우 빈도의 증가와 관련이 있다. 순별 강우량의 제 2극대기가 9월 초순에서 8월 하순으로 바뀌거나 출현하지 않는다. 점차 8월의 소우기가 사라지면서 장마가 9월 초순까지 이어지는 경향이다. 8월 중순과 9월 중순(혹은 7월 중순)의 강수량 편차는 1971년을 경계로 음에서 양 혹은 양에서 음으로 바뀌는 경향이며. 그 변동은 서서히 진행되고 있다. 대부분 지역에서 강수량 변동은 해양변동 및 전구평균기온과 높은 상관관계가 있다.

• 한국지역지리학회지
• /
• 제11권1호
• /
• pp.101-113
• /
• 2005

한반도의 남서부에 위치한 호남지방은 수리적, 지리적 요인에 의해 지역에 따라 하계의 강수현상 및 탁월일기의 다소와 그 계절변화가 크다. 본 논문은 AWS 63개 지점을 포함한 호남의 79개 기상관측지점의 하계강수량(1994$\sim$2003)과 그 순변화형(강수특성 표현의 중요한 한 요소임)에 대해 순별 강수량의 다소와 순장수량의 주성분벡터와 진폭계수(Rs)를 이용하여, 호남 각 지역에서의 하계강수량 순변화형을 수량적으로 추출하고, 그 공간스케일의 변동을 규명해, 그에 따른 호남지방의 강수지역 구분을 시도한 것이다. 그 결과 호남지방의 하계강수량 순변화의 전형적 특징은 상위 4개의 순변화형으로 표현되며 그 누적기여율은 78.0%이다. 또한 호남지방의 하계강수량의 순변화형은 A-K형까지 11개가 추출되었고, 강수지역은 18개형 지역으로 구분되었다.

• 천문학회지
• /
• 제48권1호
• /
• pp.1-7
• /
• 2015

The orbital period changes of the W UMa eclipsing binary AU Ser are studied using the (O-C) method. We conclude that the period variation is due to mass transfer from the primary star to the secondary one at a very low and decreasing rate $dP/dt=-8.872{\times}10^{-8}$, superimposed on the sinusoidal variation due to a third body orbiting the binary with period $42.87{\pm}3.16$ years, orbital eccentricity $e=0.52{\pm}0.12$ and a longitude of periastron passage ${\omega}=133^{\circ}.7{\pm}15$. On studying the magnetic activity, we have concluded that the Applegate mechanism failed to describe the cycling variation of the (O-C) diagram of AU Ser.

• 한국대기환경학회지
• /
• 제20권2호
• /
• pp.143-151
• /
• 2004

The chemical composition of PM$_{2.5}$ was measured at Gosan, Jeju for two weeks each in November 2001 and spring 2002. In the latter part of the measurement period of November 2001, designated as the polluted period in this work, secondarily formed ion components as well as primarily emitted elemental carbon were high. PM$_{2.5}$ mass concentration was also high in this polluted period compared with the yellow sand period, in which daily average of PM $_{10}$ peaked up to 520 $\mu\textrm{g}$/㎥. Increase of major components of anthropogenic origin in the polluted period was not correlated with the variation in sea salt components while increase of crustal components in the yellow sand period was highly correlated with the variation in sea salt components. Trace elements were generally higher in the yellow sand period; however, toxic heavy metals such as zinc, cadmium and lead were the highest in the polluted period.d.d.d.

• 한국건축시공학회:학술대회논문집
• /
• 한국건축시공학회 2008년도 추계 학술논문 발표대회
• /
• pp.53-56
• /
• 2008

This paper is to investigate the change of the period of hot weather concrete with elapse of age based on climate data. Climate data for 30 years and 5 years are used respectively. Determination of the period of hot weather concreting on architectural execution in Korea according to the specifications of AIJ, KSCE, and ACI are discussed. According to the research, the period of hot weather concreting with each specification in most regions lasts over 35 days. Compared with the period of cold weather concreting in hillside and inland area, coastal areas have shorter period in the same latitude. The period of hot weather concreting tends to decrease with high latitude. As expected, with the elapse of age, the period of hot weather concrete exhibited to decrease, especially, big city like Seoul, Busan etc had remarkably increased period by as much as a week. This is due to the global warming and industrialization effect with the elapse of age.

• Journal of Astronomy and Space Sciences
• /
• 제34권1호
• /
• pp.37-44
• /
• 2017

In this paper, analysis results of the photometric data of DO Dra will be presented. DO Dra had been observed with 1 m LOAO telescope and 0.6 m CBNUO telescope from 2005 through 2014. The data shows kind of periodic oscillation behavior in the orbital period and also in the spin period. It has been found that these QPOs are not observed always and that the periods vary from 30 min to 80 min. We also found that the period variation seems to repeat itself with the period of 13.5 days. It is essential to monitor this object in the future as well as to carry out model calculation in order to have better understanding of these QPO phenomena.

• 전기학회논문지
• /
• 제61권11호
• /
• pp.1578-1583
• /
• 2012

There are 3 systems in incentive-based normal load management in Korea; day or hour-ahead, week-ahead, months-ahead. These are originally similar in their operational implementation, but differ in their pre-notification period. Therefore the incentive of these systems should be different according to prenotification period. This is the key problem in implementing these load managements. Customers participating in these load managements feel their economic differences, depending on the risk by prenotification dates. The shorter prenotification period, the more risk take the customers. This paper proposes the method of incentive variation in prenotification difference, by using the theory of financial yield curve, which is used in analysing short and long duration bond interesting rates and is reflecting risk premium in their period.

• 한국정밀공학회지
• /
• 제15권6호
• /
• pp.33-39
• /
• 1998

This paper is related to economic design of tool-resetting period in NC machining. In NC lathe machining, the mean and variance of components dimension fluctuate in slow time and we should reset tool program to compensate the variation from the fluctuation. In this paper. we propose the procedure determining the optimal resetting period based on the total expected operating cost which consists of resetting cost and the quality cost related to dimension variation. As a case study, using experimental data about dimension changes of a lathe machining, we obtain the regression equations of mean and variance of the dimension fluctuation, total expected operating cost, and optimal resetting period.

• 한국해안해양공학회지
• /
• 제17권1호
• /
• pp.16-20
• /
• 2005

고함수비상태로 준설투기된 준설점토지반에 지반개량을 위한 하중재하시 보통 점토지반에 비해 큰 압밀침하가 발생한다. 미소변형률을 전제로 하고 있는 기존의 열전도형 압밀방정식은 준설토지반과 같이 대변형이 발생하는 지반에 적용하기 어렵다. 따라서 준설토층과 같이 큰 변형이 발생하는 지반에서는 압밀과정 중 층 두께의 변화가 고려되어지는 압밀방정식을 적용해야한다. 본 연구에서는 층 두께의 변화를 고려한 압밀해석을 하고 이들의 결과와 층 두께의 변화를 고려하지 않은 기존 압밀해석의 결과와 비교·분석하였다. 이들로부터 변형률이 큰 지반에서의 압밀기간은 층 두께의 변화를 고려한 이론이 그렇지 않은 경우보다 실측치에 보다 근사하게 산정되었고, 압밀침하량의 경우는 압축지수에 의한 방법보다 변형률에 근거한 계산이 실측치에 매우 근접하게 산정되었다.

• 천문학회지
• /
• 제44권3호
• /
• pp.97-108
• /
• 2011

The photometric light curves of the W-type W UMa eclipsing contact binary system BB Pegasi have been found to be extremely asymmetric over all the observed 63 years in all wavelengths UBVR. The light curves have been characterized by occultation primary minima. Hence, the morphology of these light curves has been studied in view of these different asymmetric degrees. The system shows a distinct O'Connell effect, as well as depth variation. A 22.96 years of stellar dark spots cycle has been determined for the system. Almost the same cycle (22.78 yr) has been found for the depth variation of MinI and MinII. We also present an analysis of mid-eclipse time measurements of BB Peg. The analysis indicates a period decrement of $5.62{\times}10^{-8}$ day/yr, which can be interpreted in terms of mass transfer at a rate of $-4.38{\times}10^{-8}M_{\odot}$/yr, from the more to the less massive component. The O - C diagram shows a damping sine wave covering two different cycles of 17.0 yr and 12.87 yr with amplitudes equal to 0.0071 and 0.0013 day, respectively. These unequal durations show a non-periodicity which may be explained as a result of magnetic activity cycling variations due to star spots. The obtained characteristics are consistent with similar chromospherically active stars, when applying the Applegate's (1992) mechanism.