• 제목/요약/키워드: wind driven waves

검색결과 22건 처리시간 0.02초

Attenuation of High-Frequency Wave Energy Due to Opposing Currents

  • Suh, Kyung-Duck;Lee, Dong-Young-
    • 한국해안해양공학회:학술대회논문집
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    • 한국해안해양공학회 1993년도 정기학술강연회 발표논문 초록집
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    • pp.20-25
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    • 1993
  • In coastal waters, more often than not, waves propagate on currents driven by tidal forces, earth’s gravity, or wind. There have been a number of studies for dealing with the change of wave spectrum due to tile presence of current. Based on the conservation of wave action, Hedges et al. (1985) have proposed an equation which describes the influence of current on the change of wave spectrum in water of finite depth. (omitted)

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STROMGREN 구가 ALFVEN파 항성풍을 가진 32 Cyg의 선윤곽에 미치는 효과 (EFFECTS OF STR MGREN SPHERE ON LINE PROFILES OF 32 CYG WITH ALFV N WAVES DRIVEN WIND)

  • 김경미;최규홍
    • Journal of Astronomy and Space Sciences
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    • 제15권1호
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    • pp.101-110
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    • 1998
  • 32Cyg의 B형 별 주위에 형성된 $str{\"{o}}mgren$ 구를 가정하고 공전궤도위상 0.06과 0.78에서 이론적인 선 윤곽을 계산하였다. 항성 풍의 속도분포에 따라 alfv n 파 모형의 선윤곽이 누승 함수의 속도 분포를 이용한 모형의 선 윤곽 보다 전체적으로 낮은 세기를 보였다. HII 모형은 HII 영역이 없는 경우보다 약한 선 윤곽을 보였으나 $\phi$ = 0.06에서는 HII 영역이 없는 모형이 HII 영역을 가진 모형에 비해 단지 적색편이 쪽에서만 약간의 차이를 보였다. 한편 $\phi$ = 0.79에서 HII 영역을 가진 $Alfv{\'{e}}n$ 파 모형의 선 윤곽은 적색편이와 청색 편이 쪽에서 각각 다른 속도기울기의 누승 함수 모형으로써 나타낼 수 있었다. 이는 급격한 초기 속도 기울기를 고려하여 2개의 가속영역을 가진 누승 함수 모형이라면 항성 풍의 가속과정을 고려하지 않음으로써 생기는 오차를 줄일 수 있음을 의미한다.의미한다.

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Gamma-Ray and Neutrino Emissions from Starburst Galaxies

  • Ha, Ji-Hoon;Ryu, Dongsu;Kang, Hyesung
    • 천문학회보
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    • 제45권1호
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    • pp.37.1-37.1
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    • 2020
  • Cosmic-ray protons (CRp) are efficiently produced at starburst galaxies (SBGs), where the star formation rate (SFR) rate is high. In this talk, we present estimates of gamma-ray and neutrino emissions from nearby SBGs, M82, NGC253, and Arp220. Inside the starburst nucleus (SBN), CRp are accelerated at supernova remnant (SNR) shocks as well as at stellar wind (SW) termination shocks, and their transport is governed by the advection due to starburst-driven wind and diffusion mediated by turbulence. We here model the momentum distributions of SNR and SW-produced CRp with single or a double power-law forms. We also employ two different diffusion models, where CRp are resonantly scattered off large-scale turbulence in SBN or self-excited waves driven by CR streaming instability. We then calculate gamma-ray/neutrino fluxes. The observed gamma-ray fluxes by Fermi-LAT, Veritas, and H.E.S.S are well reproduced with double power-law distribution for SNR-produced CRp and the CRp diffusion by self-excited turbulence. The estimated neutrino fluxes are <~10-3 of the atmospheric neutrino flux in the energy range of Eneutrino <~100 GeV and <~10-1 of the IceCube point source sensitivity in the energy range of Eneutrino >~60 TeV.

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黃海에서의 波浪과 海底剪斷應力 (Surface Waves and Bottom Shear Stresses in the Yellow Sea)

  • 강시환;최제국
    • 한국해양학회지
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    • 제19권2호
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    • pp.118-124
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    • 1984
  • 黃海의 海上風에 의한 重力波의 波高와 週期를 SMB法을 使用하여 計算 하였다. 그리고 黃海에서 樹勢한 北西風과 南西風이 40knots에 달할 때의 波浪活動 에 의한 海底流速과 海底剪斷應力을 線形波浪理論과 Kajiura(1968)의 暖流振動境界層分析에 의해 구하였다. 計算 缺課를 보면 韓半島의 西海沿近海域 에서 가장 큰 海波와 剪斷應力의 分布를 보이며 이로 인하여 沿近海底面이 持續的인 影響를 받고 있음이 나타났다.

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Alfven파에 의한 항성풍 밀도분포가 32 Cyg의 선윤곽에 미치는 효과 (EFFECTS OF DENSITY DISTRIBUTION OF THE WIND ON THE LINE PROFILES FOR 32 CYG)

  • 김경미;최규홍
    • Journal of Astronomy and Space Sciences
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    • 제14권1호
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    • pp.24-32
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    • 1997
  • Alfven파에 의한 항상풍을 가정하고 운동방정식을 수치적분하여 속도분포를 구하였다. 질량이 보존된다면 밀도분포 속도분포와 밀접한 관계를 가지므로 가정되는 초기 밀도 개수의 값에 따라 선윤곽이 변화하는 효과를 계산하였다. 실제적인 항성풍 모형을 계산하기 위해 Schroder(1986)의 관측과 잘 맞는 초기 밀도 개수 $N_0=5.5{\times}10^{12}/cm^3$의 경우와 $N_0=10^9,10^{10},10^{11}/cm^3$의 경우를 계산하였으며 초기 밀도 개수가 작을수록 속도분포가 급격하고 더 큰 종속도를 보였다. 또한 공전궤도위상 0.06과 0.78에서의 선윤곽을 계산하였고, $N_0$가 작을수록 더욱 강하고 좁은 흡수요소를 가졌으며 이로 인해 방출선의 극대가 청색편이되어 나타났다.

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목포 북항에서 풍파에 의한 해수범람의 수치 모의 (Numerical Simulation of Surge - Wave Combined Inundation at Mokpo North Harbor)

  • 이정렬;강주환;윤종태
    • 대한토목학회논문집
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    • 제28권3B호
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    • pp.307-313
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    • 2008
  • 방조제 건설로 인한 조석확폭 현상이 목포 북항은 물론 목포북항과 좁은 수로로 연결된 청계만에서도 발생되고 있다. 이러한 조석확폭 현상은 조간대를 증가시키고 특히 폭풍우시 수위 증가와 침수구간의 확대를 초래한다. 본 연구에서의 모의 과정은 광역에서의 풍파 모의와 협역에서의 풍파 범람 모의로 구성된다. 비선형 완경사 방정식이 바람에 의한 풍파는 물론 해일과 범람도 모의하도록 개선되었다. 개발된 모형은 청계만에 적용되었으며 목포 북항에는 청계만에서 발생하는 풍파로 인하여 발생할 수 있는 범람 형태를 파악하기 위하여 적용되었다.

SEASONAL AND SUBINERTIAL VARIATIONS IN THE SOYA WARM CURRENT REVEALED BY HF OCEAN RADARS, COASTAL TIDE GAUGES, AND A BOTTOM-MOUNTED ADCP

  • Ebuchi, Naoto;Fukamachi, Yasushi;Ohshima, Kay I.;Wakatsuchi, Masaaki
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2008년도 International Symposium on Remote Sensing
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    • pp.340-343
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    • 2008
  • The Soya Warm Current (SWC) is a coastal boundary current, which flows along the coast of Hokkaido in the Sea of Okhotsk. Seasonal and subinertial variations in the SWC are investigated using data obtained by high-frequency (HF) ocean radars, coastal tide gauges, and a bottom-mounted acoustic Doppler current profiler (ADCP). The HF radars clearly capture the seasonal variations in the surface current fields of the SWC. The velocity of the SWC reaches its maximum, approximately 1 m/s, in the summer, and becomes weaker in the winter. The velocity core is located 20 to 30 km from the coast, and its width is approximately 50 km. The almost same seasonal cycle was repeated in the period from August 2003 to March 2007. In addition to the annual variation, the SWC exhibits subinertial variations with a period from 10-15 days. The surface transport by the SWC shows a significant correlation with the sea level difference between the Sea of Japan and Sea of Okhotsk for both of the seasonal and subinertial variations, indicating that the SWC is driven by the sea level difference between the two seas. Generation mechanism of the subinertial variation is discussed using wind data from the European Centre for Medium-range Weather Forecasts (ECMWF) analyses. The subinertial variations in the SWC are significantly correlated with the meridional wind component over the region. The subinertial variations in the sea level difference and surface current delay from the meridional wind variations for one or two days. Continental shelf waves triggered by the meridional wind on the east coast of Sakhalin and west coast of Hokkaido are considered to be a possible generation mechanism for the subinertial variations in the SWC.

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풍파 스펙트럼의 시간발전에 관한 수치 실험 (Numerical Study on Temporal Evolution of Wind-Wave Spectra)

  • 오병철;이길성
    • 한국해안해양공학회지
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    • 제11권1호
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    • pp.20-33
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    • 1999
  • 심해에서 풍파의 성장은 바람에 의한 에너지 입력, 비선형 상호작용에 의한 에너지 전달 및 백파에 의한 에너지 소산에 의하여 결정된다. 본 연구에서는 두가지의 비선형 계산법(IMM 모형과 WAM 모형)을 사용하여 풍파 스펙트럼의 시간발전 특성을 상호비교하였다. 비선형 에너지 전달은 첨두주파수의 저주파 천이, 스펙트럼의 과대평가 현상, 스펙트럼의 자기상사적 발달 등에서 중심적인 역할을 하는 것으로 나타났다. 특히, 고주파 성분의 방향 분포가 쌍봉형으로 발전되는 경향이 있는데 이러한 현상도 비선형 상호작용의 역할로 설명되었다. 주파수 스펙트럼에서 고주파측의 꼬리는 주파수의 -4승에 비례하는 형상으로 발전되는 것이 확인되었다. 외부의 원인으로 스펙트럼에 도입되는 섭동은 자기상사 기구에 의하여 빠르게 제거되는데 이는 파랑수치 모형에서 비선형 상호작용이 모형의 안정화에 크게 기여함을 의미한다.

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제주 우도 홍조단괴해빈의 태풍 시기 지형변화 (Topographic Variability during Typhoon Events in Udo Rhodoliths Beach, Jeju Island, South Korea)

  • 윤우석;윤석훈;문재홍;홍지석
    • Ocean and Polar Research
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    • 제43권4호
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    • pp.307-320
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    • 2021
  • Udo Rhodolith Beach is a small-scale, mixed sand-and-gravel beach embayed on the N-S trending rocky coast of Udo, Jeju Island, South Korea. This study analyzes the short-term topographic changes of the beach during the extreme storm conditions of four typhoons from 2016 to 2020: Chaba (2016), Soulik (2018), Lingling (2019), and Maysak (2020). The analysis uses the topographic data of terrestrial LiDAR scanning and drone photogrammetry, aided by weather and oceanographic datasets of wind, wave, current and tide. The analysis suggests two contrasting features of alongshore topographic change depending on the typhoon pathway, although the intensity and duration of the storm conditions differed in each case. During the Soulik and Lingling events, which moved northward following the western sea of the Jeju Island, the northern part of the beach accreted while the southern part eroded. In contrast, the Chaba and Maysak events passed over the eastern sea of Jeju Island. The central part of the beach was then significantly eroded while sediments accumulated mainly at the northern and southern ends of the beach. Based on the wave and current measurements in the nearshore zone and computer simulations of the wave field, it was inferred that the observed topographic change of the beach after the storm events is related to the directions of the wind-driven current and wave propagation in the nearshore zone. The dominant direction of water movement was southeastward and northeastward when the typhoon pathway lay to the east or west of Jeju Island, respectively. As these enhanced waves and currents approached obliquely to the N-S trending coastline, the beach sediments were reworked and transported southward or northward mainly by longshore currents, which likely acts as a major control mechanism regarding alongshore topographic change with respect to Udo Rhodolith Beach. In contrast to the topographic change, the subaerial volume of the beach overall increased after all storms except for Maysak. The volume increase was attributed to the enhanced transport of onshore sediment under the combined effect of storm-induced long periodic waves and a strong residual component of the near-bottom current. In the Maysak event, the raised sea level during the spring tide probably enhanced the backshore erosion by storm waves, eventually causing sediment loss to the inland area.

The technological state of the art of wave energy converters

  • GURSEL, K. Turgut
    • Advances in Energy Research
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    • 제6권2호
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    • pp.103-129
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    • 2019
  • While global demand for energy increases annually, at the same time the demand for carbon-free, sulphur-free and NOx-free energy sources grows considerably. This state poses a challenge in the research for newer sources like biomass and shale gas as well as renewable energy resources such as solar, wind, geothermal and hydraulic energy. Although wave energy also is a form of renewable energy it has not fully been exploited technically and economically so far. This study tries to explain those reasons in which it is beyond doubt that the demand for wave energy will soon increase as fossil energy resources are depleted and environmental concerns gain more importance. The electrical energy supplied to the grid shall be produced from wave energy whose conversion devices can basically work according to three different systems. i. Systems that exploit the motions or shape deformations of their mechanisms involved, being driven by the energy of passing waves. ii. Systems that exploit the weight of the seawater stored in a reservoir or the changes of water pressure by the oscillations of wave height, iii. Systems that convert the wave motions into air flow. One of the aims of this study is to present the classification deficits of the wave energy converters (WECs) of the "wave developers" prepared by the European Marine Energy Center, which were to be reclassified. Furthermore, a new classification of all WECs listed by the European Marine Energy Center was arranged independently. The other aim of the study is to assess the technological state of the art of these WECs designed and/or produced, to obtain an overview on them.