d speed profiles of typhoon matmo observed u sing doppler...
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海洋工程學刊 第十七卷 第一期
2
督卜勒光達麥德姆颱風風速剖面觀測
蔡原祥 1* 楊雅兆 2 張宛婷 2 楊文昌 3 林博雄 4 陳景林 5 1國家實驗研究院台灣海洋科技研究中心副研究員
2國家實驗研究院台灣海洋科技研究中心佐理研究員 3國家實驗研究院台灣海洋科技研究中心研究員
4國立台灣大學大氣科學系副教授 5台灣電力公司綜合研究所研究員
摘 要
於台灣南部興達港使用督卜勒光達(Doppler Lidar)於 2014 年量測颱風麥
德姆颱風的風速與紊流強度剖面分佈,測量高度介於 48 至 268 m。在風速較
強,大於 10 m/s 的大氣中性穩定條件下,觀測到四種型態風速剖面: 1.所
量測高度區間風速邊界層的發展完全符合對數型態風速剖面;2.明顯受科式
力影響,高度大於表面層 (surface layer) 時,風速偏離對數型態剖風速剖面;
3. 存在一梯度高度(Gradient height)的淺層邊界層; 4.在降雨的條件下,形
成類似於低空噴流型態。本研究顯示,使用指數型態進行最適合化曲線,兩
層模式(two-layer model) 在邊界層上、下層各自有一獨立的冪指數,較能描
述平均風速與紊流強度垂直分佈的演變。
關鍵詞:颱風邊界層、紊流強度、大氣近地表邊界層、指數公式
* 通訊作者 E-mail: [email protected]
Wind Speed Profiles of Typhoon Matmo Observed Using Doppler Lidar
Journal of Coastal and Ocean Engineering, Vol. 17, No. 1 3
1. INTRODUCTION
Atmospheric boundary layer (ABL) near the surface and the turbulent fluctuations generated inside plays significant roles in the field of wind energy. The subject concerns the wind shear and turbulence induced cyclic and fatigue loading on the turbine structure, which can reduce the turbine reliability and expected lifetime as well as the influence of power generation for a contemporarily large size of wind turbine. Also, understanding the ABL improves the accuracy of weather model prediction, for which to know the upstream time history of mean wind speed, gustiness, and direction for several hours or days in advance is crucial for operation of offshore wind farms. This has to be particularly considered for the extreme wind speed in typhoon weather because severe damages on wind turbines are often reported in typhoon prone regions such as in Taiwan and Japan (Ishihara et al., 2005; Chou et al., 2013). To ensure an appropriate protection against the effect of typhoon winds, it is essential to study the detailed formation of typhoon boundary layer (TBL) and turbulence distributed in the range height of turbines to assess the structural dynamics response to the extreme wind.
In the field of wind engineering, literature surveys showed that previous TBL observations were mainly for the depth close to the surface, that is, in the surface layer (SL) using conventional
masts facilitated with anemometers. The universal logarithmic law and empirical power law were remarked to well model the wind speed profile for the strong wind speed. Besides, the decay of turbulence intensity with respect to height was described using the power law (e.g. Choi, 1978; Ishizaki, 1983; Hui et al., 2009; Song et al., 2016). A comparison of wind features between typhoons and monsoons was carried out by Choi (1978), who showed that the along-wind variance of velocity fluctuations in typhoon winds was an order larger than those in monsoon winds, revealing the extreme gustiness and complicated nature of typhoon generated winds.
In addition to tower observations, dropsonde and remote sensing technique have been employed to observe TBL, which are useful to investigate wind profiles over SL to the upper limit of TBL. Using the GPS dropsonde over the sea, Vickery et al. (2009) demonstrated that the development of entire TBL was the type of low level jet (LLJ) with the strong wind speed between 20 and 80 m/s. The logarithmic profile appropriately predicted the vertical distribution of wind speed below the jet noses. Tse et al. (2013) studied the TBL using both Lidar and Sodar. However, the LLJ type was not clearly observed over the land for the hourly mean wind speed profiles. The reason was attributed to the relative low wind speeds below 20 m/s, which were substantially lower than those studied in Vickery et al. (2009). Tse et al. (2013) concluded that the logarithmic law and
督卜勒光達麥德姆颱風風速剖面觀測
4 海洋工程學刊 第十七卷 第一期
power law reasonably explained the vertical distribution of wind speeds with the height up to 300 m.
Although characteristics of typhoon wind structure and boundary layer have been studied for decades in aspects of the wind engineering field, it appears that the knowledge gained from observations, particularly, over the height of SL is far from sufficient to fully understand the development of TBL. Also, difficulty is encountered due to the induvial feature of typhoon characterized by the surface roughness, topography, and atmospheric conditions of temperature and pressure gradient. In the present study, typhoon Matmo landfall Taiwan in 2014 was observed using the remote sensing technique of the ground-based Doppler Lidar at Hsingda Harbour, south Taiwan. An attempt was made to study the detailed formation of TBL and vertical variation of turbulent intensity profile, which were analyzed in the hourly mean values and compared with the empirical power law, theoretical logarithmic law and Deaves and Harris model (D-H model, Cook 1997). Among the wind profiles, the D-H model predicts the entire ABL and turbulence intensity profile , which appears to have not been validated for typhoon winds in previous studies.
The problem under consideration and the structure of this paper are as follows. Section 2 discusses the empirical and theoretical wind speed and turbulence intensity profiles. Section 3 introduces the measurement principle and calibration of
the present Lidar used. Section 4 describes the typhoon Matmo, observation site, and data processing. Section 5 presents and discusses the results of the measurements in comparison with the empirical and theoretical profiles and the conclusions are given in Section 6.
2. THEORY
2.1 Power law
In description of the mean wind speed profile, the empirical power law has been widely used in the wind engineering community. The power law is a simple mathematic expression described as follows: ( )( ) = ( ) (1) where denotes the reference wind speed at
the reference height and α denotes the
power exponent, which is the kernel parameter to represent the profile feature. Theoretically,
α is only dependent on the terrain roughness
in the atmospheric neutral stability. It is often quoted for the value of 0.14 in a flat terrain and significantly increases to a value larger than 0.3 in the city centre with tall buildings.
However, site observations experience that α
varies with the range of height and even with the magnitude of the wind speed. The power law is also employed to illustrate the vertical distribution of the turbulence intensity (Choi, 1978; Tamura, 2007) giving the formula as follows: ( )( ) = ( ) (2)
Wind Speed Profiles of Typhoon Matmo Observed Using Doppler Lidar
Journal of Coastal and Ocean Engineering, Vol. 17, No. 1 5
where = / represents the
turbulence intensity; is the standard deviation of the wind velocity in the
along-wind component; represents the reference turbulence intensity at the
reference height; and β represented the
power exponent for the turbulence intensity. Generally, in the atmospheric neutral stratification without the thermal buoyancy effect the turbulence intensity
decrease with respect to height and β is a
negative value.
2.2 Logarithmic law
In the typhoon event with the cooling weather and strong wind speed, the atmospheric stability is that of neutrally stratified flow (Tse et al., 2013). The turbulence generated for the depth immediately over the ground is predominated by the surface friction. In SL, the variation of the shear stress is negligible and assumed to be constant (Panofsky and Dutton, 1984). The universal logarithmic profile well describes this adiabatic layer with the form: U(z) = ∗ ln (3) where ∗ represents the surface friction
velocity and denotes the surface roughness length. Introducing the standard
deviation, , in the along-wind stream
and re-arranging equation (3), the vertical distribution of turbulence intensity is theoretically expressed as follows: TI(z) = k ∗ ln (4)
where / ∗ is the turbulence ratio. In
atmospheric neutral stability, the ratio is usually quoted to be 2.4 (Panofsky and Dutton, 1984). In the present study, the observed turbulence ratio was fed into equation (4) to make a direct comparison with the observed turbulence intensity profile.
2.3 Deaves and Harris model
As interpreted by Cook (1997), Deaves and Harris develops a more complicated D-H model to simulate the formation of entire ABL for the strong wind and neutral stratification in the homogeneous terrain. In contrast to the logarithmic law without an upper boundary condition, the D-H model matches both the upper and surface boundary conditions. A quartic polynomial was added to modify the logarithmic profile expressed as follows: U(z) = ∗ ln + 5.75 −1.88 − 1.33 + 0.25 (5) where denotes the thickness of ABL, calculated using the Rossby-Montgometry formula: z = ∗ (6) where represents the Coriolis
parameter with the value of 5.673×10-5 at
the Lidar measurement site of Hsingda Harbour and C represents the empirical constant equal to 6. The D-H model also
督卜勒光達麥德姆颱風風速剖面觀測
6 海洋工程學刊 第十七卷 第一期
empirically formulates the vertical distribution of turbulence intensity:
TI(z) = . . . ( / ) ( ) . ( ∗ / ) (7) where the scaling parameter = 1 −/ . The D-H model has been widely
used in the wind engineering field to account the wind shear and fatigue loading particularly for tall buildings when the logarithmic law cannot model the wind speed profile over the SL.
3. LIDAR WIND PROFILER
3.1 Measurement of Lidar
Light Detection and Ranging (Lidar) is an advanced remote sensing technology to measure three dimensional wind velocities. The measurement principle is that the emitted laser beam in atmosphere, when encountering to the aerosols, the scattered light returns and detects by the receiver of the system. Because the aerosols move along with the atmospheric airflow relative to the beam direction, the received signal experiences the Doppler
frequency shift. The radial velocity, , in
the line-of-sight (LOS) is calculated from the relation: v = λΔ (8) where represents Doppler frequency
shift and represents the laser wavelength.
The pulsed Lidar employed in the present study is Leosphere Windcube v2
with = 1.543 μm in the near-infrared
range for the eye safety. Adopting Doppler beam swinging technique, the Windcube sequentially sent four beams with a cone-angle of 28o in four directions, north, east, south, and west, respectively and follows a vertical beam directed to zenith. The designation of the independently vertical beam improves the measurement accuracy of vertical velocities, which is in advantage of assessing the momentum flux (Mann et al., 2010). The orthogonal frame of the Windcube v2 is illustrated in Figure 1. The three dimensional velocity of component for u, v, and w velocity can be retrieved from the radial velocities described as follows: u = (9) v = (10) w = Vr (11) where , , , and represented the radial velocity directed to north, south, east, and west, and vertical direction. The wind speed, U, of the along-wind component and wind direction,
θ, are calculated using the following
transformation: U = √u + v (12) = tan v/u (13)
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Wind Speed Profiles of Typhoon Matmo Observed Using Doppler Lidar
Journal of Coastal and Ocean Engineering, Vol. 17, No. 1 11
wind profiles. The results showed that a single power exponent usually cannot well describe the shape of the full observation range. A simple two-layer model was developed to fit the power law in the upper and lower layer, respectively. To compare with the logarithmic law and D-H models, the surface parameters of the friction
velocity ∗ and roughness was calculated using the profile fitting method. Previous studies have confirmed that the logarithmic layer developed for a depth approximate to 100 m in the neutral stratification (Panofsky and Dutton, 1984). Hence, the wind speed measured at the three lowest levels at 40, 50, and 60 m were employed to fit the logarithmic
profile to determine the ∗ and . The
period between July 23, AM 01:00 and July 24, AM 00:00 showed the significant wind speed of MAT with the U48, where the subscribe denoted the observation height, close to or greater than 10 m/s were examined.
5. RESULTS AND DISCUSSION
The evolution of the hourly mean wind speed and direction in the process of MAT is demonstrated in Figure 6. The wind speed started to significantly increase on midday of July 22 when the storm radius touched the land, half day before the typhoon landfall. The maximum wind speed recorded was 24 m/s at the height of 268 m on July 23 AM 06:00 after MAT crossed the Central Mountain and arrived in the western coast while the distance
between the typhoon centre and observation site was shortest. The wind speed subsequently decreased when MAT progressively moved away and the wind pattern finally returned to the originally weather system. A considerable falling of the wind speed is observed on July 23, AM 11:00, which is the heavy rainfall caused phenomenon. Because of the naturally cyclonic typhoon wind, the wind direction reversed counterclockwise from the north-northwest on July 22, PM 23:00 to south-southeast on July 24, PM 14:00.
5.1 Wind speed profile
The vertical distribution of the mean wind speed profile is demonstrated in Figure 7 with the power law curving fitting. As expected for a conventional boundary layer, the wind speed profile generally shows that the wind speed monotonically increases with respect to height. However, it is noted that in the initial stage with relative weak wind speed between Figure 7(b) and 7(e), the wind speed appears not to increase and keep uniform in the upper layer between 148 and 188 m. This is in agreement with Amano et al. (1999), who observes a gradient height in the TBL near the surface. A particular case is g in Figure 7(k) with a reversed wind speed over 168 m in height, forming the profile of low level jet (LLJ) type. In contrast to the time series shown Figure 6 a significant falling and reduction of discrepancy of the wind speed between upper and lower layer is observed. It appeared that a local eddy occurs with a strong down burst flow.
督卜勒光
12 海洋
Fig. 6
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光達麥德姆颱風
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風風速剖面觀測
第十七卷 第一
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Wind Speed Profiles of Typhoon Matmo Observed Using Doppler Lidar
Journal of Coastal and Ocean Engineering, Vol. 17, No. 1 13
Table 1 Parameters of wind profiles for wind speed and turbulence intensity
Time Type U48
(m/s) Dir48
(deg) σU48 (m/s)
u*o
(m/s)zo (m)
α β
α12 αL αU zα (m) β12 βL βU zβ (m)
01:00 2 9.19 302 1.61 0.76 0.39 0.20 - - 248 -0.26 -0.13 -0.60 12802:00 3 8.95 280 1.60 0.87 0.79 0.18 0.21 0.07 128 -0.33 -0.30 -0.64 16803:00 3 10.95 268 1.78 1.08 0.84 0.17 0.21 0.03 128 -0.43 -0.29 -0.53 88 04:00 3 12.11 278 2.42 1.15 0.72 0.15 0.20 0.004 128 -0.36 -0.18 -0.64 10805:00 3 11.63 275 2.21 1.14 0.80 0.18 0.22 0.11 148 -0.20 -0.15 -0.30 14806:00 2 15.43 261 3.05 1.39 0.56 0.25 0.23 0.24 128 -0.29 -0.16 -0.43 10807:00 1 14.68 251 2.58 1.46 0.87 0.23 0.24 0.16 148 -0.39 -0.13 -0.62 88 08:00 2 16.84 223 2.09 1.25 0.22 0.18 0.19 0.15 148 -0.42 -0.14 -0.66 88 09:00 2 16.05 213 2.29 0.85 0.025 0.15 0.14 0.15 128 -0.35 -0.15 -0.82 12810:00 2 13.99 208 2.69 0.83 0.058 0.19 0.15 0.26 108 -0.27 -0.22 -0.45 10811:00 4 11.03 230 4.47 0.29 10-5 0.004 0.08 -0.40 148 -0.036 0.17 -1.07 14812:00 1 13.18 214 2.72 0.99 0.24 0.18 0.19 0.16 148 -0.43 -0.16 -0.91 10813:00 2 13.99 212 2.01 0.78 0.036 0.16 0.14 0.21 128 -0.14 -0.059 -0.51 14814:00 2 14.18 201 2.41 0.94 0.12 0.19 0.17 0.23 128 -0.29 -0.22 -0.47 12815:00 1 14.19 189 2.18 1.32 0.65 0.2 0.21 0.11 188 -0.49 -0.33 -0.95 12816:00 1 13.12 188 1.96 1.24 0.70 0.21 0.22 0.16 188 -0.35 -0.22 -0.50 88 17:00 1 14.05 190 2.37 1.34 0.72 0.21 0.21 0.15 188 -0.44 -0.32 -0.77 12818:00 1 13.80 189 2.14 1.37 0.86 0.21 0.22 0.13 168 -0.44 -0.35 -0.75 12819:00 1 13.78 187 2.08 1.28 0.65 0.19 0.20 0.14 148 -0.35 -0.26 -0.64 12820:00 1 13.19 181 2.15 1.18 0.55 0.19 0.21 0.14 148 -0.28 -0.19 -0.55 12821:00 3 12.66 181 2.05 1.24 0.82 0.19 0.21 0.14 128 -0.37 -0.33 -0.41 12822:00 1 11.86 181 1.82 1.17 0.83 0.21 0.22 0.18 148 -0.30 -0.23 -0.66 14823:00 3 11.17 185 1.87 1.16 1.01 0.22 0.23 0.10 168 -0.43 -0.24 -0.79 10800:00 3 9.70 186 1.74 1.07 1.26 0.20 0.23 0.12 128 -0.29 -0.25 -0.43 128
Subscribe 12, L, and U in the power exponent, α and β, denoting the entire, upper, and
lower layer fitting. zα and zβ representing the characteristic height for the wind speed
and turbulence intensity profile to separate the two layers.
The power law indicated that, a single
power exponent α12 fitted for the entire
height of the Lidar observation matched the observation only given in Figure 7(a), 7(h), 7(i), 7(l), and 7(v). Tse et al. (2013) remarked that a power law modeled the TBL up to 300 m in height. However, the observed wind profiles intrinsically demonstrated two layers. This is displayed in Figure 7 with the individual power exponent in the lower and upper layer,
characterized by the height of zα to
distinguish the two layers. Table 1 displays the basic parameters to represent the mean wind profile and the character height
manually determined for the wind speed and turbulence intensity profile. The velocity gradients in the lower layer, significantly influenced by surface friction, are usually greater than those in the upper layer. The opposite results are given in Figure 7(j), 7(m), and 7(n) with a relative weak surface friction velocity.
Typhoon observations to the height of
70 m from Choi (1978) showed that α was
between 0.19 and 0.26, which was slightly larger than the present observation between 0.15 and 0.25 for the entire layer and between 0.14 and 0.23 for the lower layer. The power exponents in the both
督卜勒光
14 海洋
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風風速剖面觀測
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督卜勒光達麥德姆颱風風速剖面觀測
16 海洋工程學刊 第十七卷 第一期
three types of profiles in Figure 8(q) at PM 17:00 for Type 1, Figure 8(n) at PM 14:00 for Type 2, and Figure 8(c) at AM 03:00 for Type 3 as shown in Figure 9.
The LLJ type profile demonstrated considerable variation of 25o for the vertical discrepancy of wind direction between 48 to 268 m in height. Besides, the vertical velocity significantly moved downwards with the maximum of -1.34 m/s at 128 m in height. In contrast, for the other three types the directional differences were 6.2o, 3.57o, and 1.65o and the vertical velocities were 0.27, 0.4, and 0.11 m/s at 48 m in height for the Type 1, Type 2, and Type 3, which are significantly less than the LLJ type profile. Aitken et al. (2012) studied the rainfall effect on the Windcube Lidar measurement. They remarked that the observed horizontal wind speeds were not affected by rainfall. However, the Lidar observed terminal velocities of raindrops rather than the truly vertical velocity of the airflow. Hence, the significantly downward flow shown in Figure 9(b) represents the heavy rainfall condition. It is likely that the interaction of the atmospheric turbulence and droplets generated local vortex, producing a complex flow with considerable variation of the wind direction as explained in Figure 9(a).
5.2 Turbulence intensity profile
Turbulence intensity profiles were depicted in Figure 10. The turbulence intensity decreased with the increase of the height, generally varying between 15% and
20% at the height of 48 m. The logarithmic law, D-H formula, power law, the two-layer model using power law are employed to fit the observed profile of turbulence intensity as given in Figure 10. The turbulence intensity discrepancy calculated from both the logarithmic and D-H model are insignificant, however, usually greater than the observation. Reasonable agreement between the D-H and observed profiles is shown in Figure 10(j), 10(m), and 10(n), for which the wind speed profile also agrees with the D-H predictions. The power law for the entire observation height does not well fit the mean profile. In analogous to the boundary layer of wind speed, there also exists two layers with the different power exponent in the upper and lower layer. The power
exponent considerably varied with β12
between -0.14 and -0.43, βL between -0.13
and -0.35, and βU between -0.41 and -1.07
in the typhoon process of MAT. The turbulence decay rate in the upper layer is significantly larger than the lower layer.
The characteristic height zβ is between 88
to 148 m in height. Apart from the heavy rainfall condition, there appears in lack of direct relation between the wind speed and turbulence intensity profile. Nevertheless, the current data demonstrates that for Type 1 profile of the entirely logarithmic layer the decay of the turbulence intensity with respect to height is faster than other two types of profiles. In the typhoon turbulence study of Choi (1979), the power exponent
showed β=-0.31. The long-term mean
values in the present study give β12=-0.34,
βL=-0.21, and βU=-0.56 through averaging
the hoexpone
Figco
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督卜勒光達麥德姆颱風風速剖面觀測
18 海洋工程學刊 第十七卷 第一期
Generally, the power law with a single power exponent cannot well model the growth of the wind speed with respect to height between 48 and 268 m. The simple two layers distinguished in the upper and lower layer with the different power exponent appropriately fits the wind profile. This two layer phenomenon is also observed in the profile of turbulence intensity with a more rapid decay rate in the upper layer. However, the present data appears not to observe a clear relation between the wind speed and turbulence intensity profile. In discussion the TBL using the dimensionless wind speed U/u*o, four types of the profiles are observed in the typhoon process of MAT. Type 1 shows the consistent with logarithmic profile for the entire observation layer under a relative strong wind shear. Type 2 reveals the significant effect of Coriolis force over SL and well modeled using the D-H profile under a weak surface friction velocity. Type 3 forms a gradient height under a relatively weak wind speed. Type 4 is a LLJ type profile occurred in the rainfall condition.
Finally, the detailed information of the TBL and turbulence intensity concluded in this study can widespread be used to account the wind shear loading of typhoons on tall structures. Particularly, for wind turbines the ICE standard (ICE 61400-3 2005) prescribes to use either the power law or logarithmic profile as wind shear model may not be completely appropriate for typhoon winds.
ACKNOWLEDGEMENTS
The authors wish to express their acknowledgement to Ministry of Science and Technology (MOST) to support and founding this research.
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督卜勒光達麥德姆颱風風速剖面觀測
20 海洋工程學刊 第十七卷 第一期
Manuscript Received: Apr. 25, 2017Revision Received: May. 24, 2017
and Accepted: May. 24, 2017