On the Variation of Turbulence in a High-Velocity Tidal Channel

被引:13
|
作者
Greenwood, Charles [1 ]
Vogler, Arne [1 ]
Venugopal, Vengatesan [2 ]
机构
[1] Univ Highlands & Isl, Lews Castle Coll, Marine Energy Res Grp, Stornoway HS2 0XR, Scotland
[2] Univ Edinburgh, Sch Engn, Inst Energy Syst, Edinburgh EH9 3DW, Midlothian, Scotland
基金
英国工程与自然科学研究理事会;
关键词
turbulence; turbulence intensity; turbulence kinetic energy; ADCP; site measurements; time scale; length scale; DISSIPATION; ENERGY; RATES;
D O I
10.3390/en12040672
中图分类号
TE [石油、天然气工业]; TK [能源与动力工程];
学科分类号
0807 ; 0820 ;
摘要
This study presents the variation in turbulence parameters derived from site measurements at a tidal energy test site. Measurements were made towards the southern end of the European Marine Energy Centre's tidal energy test site at the Fall of Warness (Orkney, Scotland). Four bottom mounted divergent-beam Acoustic Doppler Current Profilers (ADCPs) were deployed at three locations over an area of 2 km by 1.4 km to assess the spatial and temporal variation in turbulence in the southern entrance to the channel. During the measurement campaign, average flood velocities of 2 ms(-1) were recorded with maximum flow speeds of 3 ms(-1) in the absence of significant wave activity. The velocity fluctuations and turbulence parameters show the presence of large turbulent structures at each location. The easternmost profiler located in the wake of a nearby headland during ebb tide, recorded flow shielding effects that reduced velocities to almost zero and produced large turbulence intensities. The depth-dependent analysis of turbulence parameters reveals large velocity variations with complex profiles that do not follow the standard smooth shear profile. Furthermore, turbulence parameters based on data collected from ADCPs deployed in a multi-carrier frame at the same location and time period, show significant differences. This shows a large sensitivity to the make and model of ADCPs with regards to turbulence. Turbulence integral length scales were calculated, and show eddies exceeding 30 m in size. Direct comparison of the length scales derived from the streamwise velocity component and along-beam velocities show very similar magnitudes and distributions with tidal phase.
引用
收藏
页数:21
相关论文
共 50 条
  • [41] HIGH-VELOCITY INTERSTELLAR GAS
    DIETER, NH
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1969, 81 (480) : 186 - &
  • [42] High-velocity optical flow
    Vergeest, Joris
    WSCG 2013, COMMUNICATION PAPERS PROCEEDINGS, 2013, : 112 - 119
  • [43] HIGH-VELOCITY WINDS IN ORION
    ZUCKERMAN, B
    NATURE, 1984, 309 (5967) : 403 - 403
  • [44] Introduction: High-velocity impact
    Nicholas, Theodore
    AIAA JOURNAL, 2008, 46 (02) : 289 - 289
  • [45] HIGH-VELOCITY CLOUDS AS PROTOGALAXIES
    VERSCHUU.GL
    ASTRONOMICAL JOURNAL, 1968, 73 (5P2): : S122 - &
  • [46] VERY HIGH-VELOCITY CLOUD
    WRIGHT, MCH
    ASTRONOMY & ASTROPHYSICS, 1974, 31 (03) : 317 - 322
  • [47] The high-velocity plasma spraying
    Klubnikin, VS
    THERMAL SPRAY, VOLS 1 AND 2: MEETING THE CHALLENGES OF THE 21ST CENTURY, 1998, : 1399 - 1403
  • [48] Where are the high-velocity clouds?
    Quilis, V
    Moore, B
    ASTROPHYSICAL JOURNAL, 2001, 555 (02): : L95 - L98
  • [49] HIGHLIGHTS OF HIGH-VELOCITY CLOUDS
    VANWOERDEN, H
    SCHWARZ, UJ
    HULSBOSCH, ANM
    IAU SYMPOSIA, 1985, (106): : 387 - 408
  • [50] HIGH-VELOCITY CLOUD COLLISIONS
    SAVEDOFF, MP
    HOVENIER, JW
    VANLEER, B
    BULLETIN OF THE ASTRONOMICAL INSTITUTES OF THE NETHERLANDS, 1967, 19 (02): : 107 - +