• Title/Summary/Keyword: Wind Field

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Numerical simulation and experimental study of non-stationary downburst outflow based on wall jet model

  • Yongli Zhong;Yichen Liu;Hua Zhang;Zhitao Yan;Xinpeng Liu;Jun Luo;Kaihong Bai;Feng Li
    • Wind and Structures
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    • v.38 no.2
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    • pp.129-146
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    • 2024
  • Aiming at the problem of non-stationary wind field simulation of downbursts, a non-stationary down-burst generation system was designed by adding a nozzle and program control valve to the inlet of the original wall jet model. The computational fluid dynamics (CFD) method was used to simulate the downburst. Firstly, the two-dimensional (2D) model was used to study the outflow situation, and the database of working conditions was formed. Then the combined superposition of working conditions was carried out to simulate the full-scale measured downburst. The three-dimensional (3D) large eddy simulation (LES) was used for further verification based on this superposition condition. Finally, the wind tunnel test is used to further verify. The results show that after the valve is opened, the wind ve-locity at low altitude increases rapidly, then stays stable, and the wind velocity at each point fluctuates. The velocity of the 2D model matches the wind velocity trend of the measured downburst well. The 3D model matches the measured downburst flow in terms of wind velocity and pulsation characteris-tics. The time-varying mean wind velocity of the wind tunnel test is in better agreement with the meas-ured time-varying mean wind velocity of the downburst. The power spectrum of fluctuating wind ve-locity at different vertical heights for the test condition also agrees well with the von Karman spectrum, and conforms to the "-5/3" law. The vertical profile of the maximum time-varying average wind veloci-ty obtained from the test shows the basic characteristics of the typical wind profile of the downburst. The effectiveness of the downburst generation system is verified.

Study of Flow Field and Pressure Distribution on a Rotor Blade of HAWT in Yawed Flow Conditions

  • Maeda, Takao;Kamada, Yasunari;Okada, Naohiro;Suzuki, Jun
    • International Journal of Fluid Machinery and Systems
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    • v.3 no.4
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    • pp.360-368
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    • 2010
  • This paper describes the flow field and the blade pressure distribution of a horizontal axis wind turbine in various yawed flow conditions. These measurements were carried out with 2.4m-diameter rotor with pressure sensors and a 2-dimensional laser Doppler velocimeter for each azimuth angle in a wind tunnel. The results show that aerodynamic forces of the blade based on the pressure measurements change according to the local angle of attack during rotation. Therefore the wake of the yawed rotor becomes asymmetric for the rotor axis. Furthermore, the relations between aerodynamic forces and azimuth angles change according to tip speed ratio. By the experimental analysis, the flow field and the aerodynamic forces for each azimuth angle in yawed flow condition were clarified.

Parameterization of Along-Wind Dispersion Coefficients based on Field and Wind Tunnel Data

  • Kang, Sung-Dae
    • Environmental Sciences Bulletin of The Korean Environmental Sciences Society
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    • v.10 no.S_1
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    • pp.11-22
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    • 2001
  • Observations related to the along-wind dispersion of puffs were collected from 12 field sites and from a wind tunnel experiment and used to test simple similarity relations. Because most of the date made use of concentration time series observation from fixed monitors, the basic observation was t, the standard deviation of the concentration time series. This data also allowed the travel time, t, from the source to the receptor to be estimated, from which the puff advective speed ue, could be determined. The along-wind dispersion coefficient, x, was then assumed to equal tue. The data, which extended over four orders of magnitude, supported the similarity relations t=0.1 t and x=1.8 $u^*$t, where t is the travel time and $u^*$ is the friction velocity. About 50% of the observations were within a factor of two of the predictions based on the similarity relations.

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Comparison of variations in sea surface height with sea surface temperature and wind field in the Tropical Pacific Ocean

  • Chul, Kang-Sung;Schumann, Robert;Murai, Shunji;Kiyoshi, Honda;Kim, Young-Seup
    • Proceedings of the KSRS Conference
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    • 1998.09a
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    • pp.225-230
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    • 1998
  • The purpose of this study is to contribute the development of an El Nino prediction model. The objectives of the study are to (1) extract sea surface height data from the TOPEI/Poseidon altimeter, and (2) compare the relations among the sea surface height, sea surface temperature and wind field. NOAA AVHRR Multi-channel data is used for sea surface temperature and wind data is derived from ERS 1, 2 AMI wind scatterometer. The results showed that sea surface height has increased significantly during the El Nino season. The sea surface height is positively related to sea surface temperature and negatively related to zonal wind.

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A Experimental Study on Structure Modeling of Ginseng Fields Facility (인삼재배시설의 구조모델링을 위한 실험연구)

  • Oh, Hynn-Kyo;Yoon, Seong-Soo
    • Proceedings of the Korean Society of Agricultural Engineers Conference
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    • 2005.10a
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    • pp.181-186
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    • 2005
  • The ginseng field structure collapses due to snow and wind. In order to study the structural modeling of ginseng field facility wind velocity test with shading material and strength test with used and unused timber were performed. The result of wind velocity test, we knew the characteristic of shading member of ginseng facility is followed linear regression, accurately. So, we made the assigned wind-value according to wind velocity. The result of strength test, the strength value of used-timber is smaller than the unused-timber and the coefficient of variance is larger than the unused-timber.

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Physical modelling of a downdraft outflow with a slot jet

  • Lin, W.E.;Savory, E.
    • Wind and Structures
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    • v.13 no.5
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    • pp.385-412
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    • 2010
  • This article provides a time-resolved characterisation of the wind field in a recently-commissioned, downdraft outflow simulator at The University of Western Ontario. A large slot jet approach to physical simulation was used. The simulator performance was assessed against field observations from a 2002 downdraft outflow near Lubbock, Texas. Outflow wind speed records were decomposed according to classical time series analysis. Length scales, characterising the coarse and fine flow structure, were determined from the time-varying mean and residual components, respectively. The simulated downdraft outflow was approximately 1200 times smaller in spatial extent than the 2002 Lubbock event.

Preliminary Validation of Wind Turbine Generator System Performance Analysis S/W, WINSIM (풍력발전시스템 성능 해석 S/W의 초기 검증에 관한 연구)

  • Mun, Jung-Heu;No, Tae-Soo;Park, Jong-Hyuk;Kim, Sung-Ju
    • Journal of the Korean Society for Aeronautical & Space Sciences
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    • v.37 no.2
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    • pp.209-214
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    • 2009
  • The simulation software for predicting the performance of a wind turbine generator system (WTGS) is validated using the field measured data obtained from the idling test run of a dual rotor wind turbine recently developed and installed in Korea. Both steady-state and transient responses at low and high wind conditions are compared with the theoretically predicted ones from the simulation software WINSIM.

A Study on the Characteristics of Air flow Fields with Velocity Uniformity in a Wind Tunnel (풍동장치 내 공기 유동장과 속도 균일도 특성에 대한 분석)

  • Han, Seok Jong;Lee, Sang Ho;Lee, Jae Gyu
    • Journal of the Korean Society of Visualization
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    • v.16 no.3
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    • pp.59-64
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    • 2018
  • Numerical simulations were carried out to analyze the flow characteristics of the wind tunnel. Flow field characteristics with velocity uniformity at the test sections are largely affected by inlet conditions of air flow rate and temperature. Axial average velocity of the flow field inside the test area was almost linearly decreased by 0.026% each 1m. The uniformity distributions of axial velocity showed the highest reduction rate of about 24% between nozzle outlets 1 ~ 2m. In addition, average velocity and the uniformity are increased with air temperature in the wind tunnel due to density variation. The results of this paper are expected to be useful for the basic design of wind tunnel and to be used for efficient design.

Power and Economic Simulation of Island for the Field Demonstration Test of Smart Microgrid System Based on Stand-alone Wind power (독립형 풍력기반 Smart Microgrid 시스템의 현장 실증 시험을 위한 도서지역 전력 및 경제성 시뮬레이션)

  • Kang, SangKyun;Lee, EunKyu;Lee, JangHo
    • New & Renewable Energy
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    • v.10 no.3
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    • pp.22-30
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    • 2014
  • The isolated self-generating electricity with diesel engine generator has been used in islands far away from main land. It costs high because of increasing oil price, and unsafe to have supplying oil and its related components by ship due to unexpectable marine conditions. Therefore there is the need for the hybrid system of renewable energy like wind or solar energy systems with oil engine generator, which can reduce oil use and extend oil supplying period. In this study, the feasibility of such hybrid system with smart micro grid on the eight islands of Jeon-nam province is surveyed to find good place for the demonstration test of the hybrid system. In each island, 3 wind turbine systems of 10 kW and photovoltaic of 20 kW are tested with already installed diesel engine. The performance and costs of the hybrid system in each island are compared in the given conditions of solar and wind energy potential. As a result of the study, Jung-ma island is recommended for the optimum place to make real field demonstration test of isolated hybrid generating and smart grid systems.

Earthward Flow Bursts in the Magnetotail Driven by Solar Wind Pressure Impulse

  • Kim, Khan-Hyuk;Kwak, Young-Sil;Lee, Jae-Jin;Hwang, Jung-A
    • Journal of Astronomy and Space Sciences
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    • v.25 no.4
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    • pp.375-382
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    • 2008
  • On August 31, 2001, ${\sim}$ 1705 - 1718 UT, Cluster was located near the midnight magnetotail, GSE (x, y, z) ${\sim}$ (-19, - 2,2) RE, and observed fast earthward flow bursts in the vicinity of the neutral sheet. They occurred while the tail magnetic field suddenly increased. Using simultaneous measurements in the solar wind, at geosynchronous orbit, and on the ground, it is confirmed that tail magnetic field enhancement is due to an increased solar wind pressure. In the neutral sheet region, strongly enhanced earthward flow bursts perpendicular to the local magnetic field $(V_{{\perp}x})$ were observed. Auroral brightenings localized in the pre-midnight sector (${\sim}$ 2200 - 2400 MLT) occurred during the interval of the $V_{{\perp}x}$ enhancements. The $V_{{\perp}x}$ bursts started ${\sim}$ 2 minutes before the onset of auroral brightenings. Our observations suggest that the earthward flow bursts are associated with tail reconnection directly driven by a solar wind pressure impulse and that $V_{{\perp}x}$ caused localized auroral brightenings.