• 농업과학연구
• /
• 제38권4호
• /
• pp.739-745
• /
• 2011

The MUSLE was utilized in this study to estimate soil erosion using daily precipitation which was main influential factor in soil loss estimation. Various scenarios were simulated to evaluate how transition of slope, agricultural products and precipitation could affect soil loss in the field. It was found that slope was the most affecting factor in soil loss estimation. Especially 1.8 times the soil loss was expected with potato at 45% slope compared with codonopsis at same slope with MUSLE model. Fortunately, farmers had planted codonopsis at this slope to reduce soil erosion from this steep slope. As shown in this study, the MUSLE method could be utilized to determine optimum crop type for each field with various slope conditions to minimize soil erosion. This approach utilized in this study could be applied to other agricultural watersheds to evaluate various soil erosion conditions.

• 산업기술연구
• /
• 제21권B호
• /
• pp.223-232
• /
• 2001

This study is finding the most appropriate model of kangwondo watershed. To synthesize each hydrograph, It is found to several parameters which are used in existing hydrographes. then the synthestic hydrograph is compared and investigated with many hydrographes of the rivers in kanwondo. These methods, Nakayasu, Clark, SCS are used to calculate the run-off of this watershed. When the calculated run-off is compared with real rating-curves, then it is found that the SCS method using the Clark's concentrantion time is the best way on this area having large watershed, long river length and gentle water slope, the Nakayasu method is more suitable on this area having small watershed, short river length and steep water slope. Also it is founded from analyzing run-off hydrographes, peak run-off and peak time that the Clark's method applied Kirpich's concentration time way is suitable in the area of kangwondo.

• 천문학회보
• /
• 제38권2호
• /
• pp.48.1-48.1
• /
• 2013

We present galaxy luminosity functions (LFs) of subgroups in the Ursa Major cluster. The membership of galaxies is determined by radial velocities which are compiled from the SDSS and NED. We found that the faint end slope (${\alpha}$) of the LF of all sample galaxies in Ursa Major is ${\alpha}=-1.13$. This is consistent with previous result, but shallower than that of the Virgo cluster. Interestingly, the subgroups in Ursa Major show different slopes in their LFs. The NGC 3992 and NGC 4111, the massive subgroups in the Ursa Major cluster, exhibit steep slopes of their LFs comparable to that of the Virgo cluster. On the other hand, less massive group (NGC 3877) shows a very shallow slope of -0.84. Based on the results, we discuss the evolution of galaxies and the assembly history of the Ursa Major cluster.

• 한국수산과학회지
• /
• 제27권2호
• /
• pp.173-182
• /
• 1994

A numerical experiment on the effective discharge of waste materials caused in recirculating aquaculture basins was performed. The numerical model used in this study was a 4-level hydrodynamic and advection-diffusion model. Flow structures and settling processes of ss in the various mathematical model basins are discussed. The calculated flow fields of the numerical basin corresponded well with the measured velocity in field basin. In the cases of steep bottom slopes in 4/30, the non-dimensional tractive force($U{\ast}/U{\ast}_c$) which is all important parameter for the deposition pattern of waste materials was stronger than with the mild slope one. The settling pattern of ss depended considerably on the degree of bottom slope of basin. To concentrate deposited waste materials into the center discharge pipe, it is useful to design a cylindrical basin with a steeply conical bottom. In addition, to prevent movement of the deposit area away from the center, it is necessary to locate the circulating ducts at diametrically opposed points on the basin sides.

• 대한화장품학회지
• /
• 제31권3호
• /
• pp.259-263
• /
• 2005

혈류량은 자외선 조사량 증가에 비례하여 증가되는 양상을 보였다. 홍반을 유발하는데 필요한 자외선량(MED)의 차이가 혈류량의 변화와 어떠한 관계가 있는지를 알아본 실험에서, MED가 30 mJ로 비교적 낮았던 피험자들의 경우, 혈류량은 MED를 지나서 급격하게 증가되는 양상을 관찰하였으나 30 mJ 이상에서 MED가 관찰되었던 피험자들의 경우에는 자외선 조사에 따른 혈류량의 변화가 급격한 변화 없이 계속 완만하게 증가되는 양상을 보였다.

• 지질공학
• /
• 제24권1호
• /
• pp.69-79
• /
• 2014

본 연구의 목적은 토양침식에 관련되는 강우특성, 토양경사도, 그리고 지질특성의 상대적인 중요도를 규명하는데 있다. 이 목적을 달성하기 위하여, 강우강도, 토양경사도, 지질특성의 각각 다른 조건에서 실내 인공강우실험 및 현장조사를 실시하였다. 실내시험 결과에 의하면, 토양침식량은 토양 경사도가 강우강도보다 크게 영향을 받았다. 유출량은 강우량에 비례하며, 점토함량이 높을수록 증가한다. 따라서 토양의 유기물과 점토 함량이 큰 토양에서 토양침식량이 크게 증가 하였다. 현장시험 결과로는 토양경사가 큰 지역 및 퇴적암 지역보다 변성암 지역에서 보다 큰 침식량이 계산되었다. 이러한 실험의 결과는 토양침식량을 예측하는 모델개발에 있어서 기반암 풍화의 산물인 토양에서의 지질특성이 침식 및 침식후의 퇴적특성을 잘 반영하고 있음을 보여준다.

• 한국방재안전학회논문집
• /
• 제12권2호
• /
• pp.65-72
• /
• 2019

한국은 국토의 64%이상이 산지로 구성되어 있어 산지재해에 취약한 지형적 특성을 가진다. 연구대상지역인 태백산국립공원 당골유역은 탐방로 대부분이 급경사지와 인접해 있어 집중호우 시 산사태와 토석류에 취약한 지역이다. 본 연구에서는 결정론적 분석방법인 사면안정성 모델을 이용하여 사면재해 발생예측 가능성을 검토하였다. 모델의 매개변수는 정밀토양도의 토양분류에 따라 토질의 단위중량, 유효점착력, 흙의 내부마찰각, 유효토심, 지표경사 등을 이용하였고 1 m격자의 DEM을 바탕으로 사면안정성 평가를 실시하였다. 사면안정성평가 분석결과 지하수/ 유효토심과의 비가 1.0에 가까워질수록 위험지역이 높게 나타났으며, 국립공원 하류지역의 민가와 상업시설 상당수가 위험에 노출된 것으로 나타났다.

• 한국지반공학회:학술대회논문집
• /
• 한국지반공학회 2003년도 봄 학술발표회 논문집
• /
• pp.469-474
• /
• 2003

Talus topography is that rock clasts that is weathered is accumulated dropping in steep slope to action of gravity. Rock fall talus is formed by the accumulation of rock debris falling as individual particles from a cliff. If the collapse is produced in talus slope, it will be possible the loss of manpower and country. Despite correct access about talus is required, domestic research was scientific access about talus short. The aim of the present study is to review and compare fabric data derived from rock fall talus about orientation, distribution and morphology in Sukam area. These deposits tend to have approximately equal amounts of clasts oriented parallel and perpendicular to the dip direction of the slope. And, platy-shaped clasts dominate the proximal and intermediate parts of the talus, whereas blocky-shaped clasts is more common in the distal part.

• Journal of Astronomy and Space Sciences
• /
• 제30권3호
• /
• pp.163-168
• /
• 2013

Parameters associated with solar minimum have been studied to relate them to solar activity at solar maximum so that one could possibly predict behaviors of an upcoming solar cycle. The number of active days has been known as a reliable indicator of solar activity around solar minimum. Active days are days with sunspots reported on the solar disk. In this work, we have explored the relationship between the sunspot numbers at solar maximum and the characteristics of the monthly number of active days. Specifically, we have statistically examined how the maximum monthly sunspot number of a given solar cycle is correlated with the slope of the linear relationship between monthly sunspot numbers and the monthly number of active days for the corresponding solar cycle. We have calculated the linear correlation coefficient r and the Spearman rank-order correlation coefficient $r_s$ for data sets prepared under various conditions. Even though marginal correlations are found, they turn out to be insufficiently significant (r ~ 0.3). Nonetheless, we have confirmed that the slope of the linear relationship between monthly sunspot numbers and the monthly number of active days is less steep when solar cycles belonging to the "Modern Maximum" are considered compared with rests of solar cycles. We conclude, therefore, that the slope of the linear relationship between monthly sunspot numbers and the monthly number of active days is indeed dependent on the solar activity at its maxima, but that this simple relationship should be insufficient as a valid method to predict the following solar activity amplitude.

• 한국해안해양공학회지
• /
• 제13권3호
• /
• pp.254-261
• /
• 2001

장주기파가 깊은 바다에서 수심이 급격히 감소하는 대륙사면을 지나 대륙붕 위로 전파해 들어오는 경우 육지에서 반사된 파가 대륙사면에서 외해로 전파해 나가지 못하고 재반사되어 들어오기 때문에 육지 쪽에서 커다란 수위진동을 일으키는 것은 잘 알려진 사실이다. Liu(1986)는 반원형 외해 경계를 따라 수심의 불연속이 존재하는 지형을 가정하여 이러한 현상을 해석하였으나 그의 해석해에는 오류가 있었다. 본 논문에서는 직선해안 및 직사각형 항만에 대한 Liu(1986)의 해석해를 수정하고, 이를 정 등(1998)의 확장형 완경사방정식에 기초한 Galerkin 유한요소 모형에 의한 결과와 비교하여 확인하였다.