nwtc turb sim workshop september 22 24, 2008- boundary layer dynamics and wind turbines
DESCRIPTION
NREL/NWTC TurbSim Workshop: Boundary Layer Dynamics and Turbine Dynamics presentation, Sept 22, 2008.TRANSCRIPT
National Wind Technology Center Neil Kelley Bonnie Jonkman September 22-24, 2008
TurbSim Workshop
National Renewable Energy Laboratory Innovation for Our Energy Future 2
Meeting Purpose
• To give the wind turbine design community an opportunity to hear about the latest improvements we have made in the NREL TurbSim Stochastic Turbulence Simulator Code
• To give the community an opportunity to learn in more detail about the development of the code, its physical basis, and how to use it.
• To have the opportunity to share ideas and questions on how best to use the features of the code.
National Wind Technology Center Neil Kelley September 22-24, 2008
TurbSim Workshop: Boundary Layer Dynamics and Wind Turbines
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Wind Turbines and Boundary Layer Turbulence
• Wind turbines must operate in a wide range of turbulent flow conditions associated with the Atmospheric Boundary Layer (ABL)
• The ABL occupies the lowest 1-2 km of the atmosphere where surface frictional drag has an influence on the movement of the wind
• Wind turbines occupy the lowest layers of the ABL and may eventually reach heights of 200 m or more
• The vertical structure and the turbulence characteristics of the ABL vary diurnally due to the heating and cooling of the solar cycle
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Wind Turbines and Boundary Layer Turbulence – cont’d
• It is this change in turbulence characteristics that has a significant impact on the operations of wind turbines
• Turbulence induces structural load responses in operating turbines which in turn creates wear in components from fatigue
• The purpose of the TurbSim Code is to provide the turbine designer with the ability to expose new designs to flow conditions that induce random or stochastic load responses for a range operating environments
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Some real world examples
• The best way to understand the role of turbulence on the operations of wind turbine is to discuss examples who operating experiences are similar in key respects
• The greatest operating challenges were found to occur during the late afternoon and nighttime hours with the period between local sunset and midnight often the most challenging
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Hawaii • 15 Westinghouse 600 kW Turbines (now
NWTC CARTS 2 & 3) 1985-1996
• DOE/NASA 3.2 MW Boeing MOD-5B Prototype 1987-1993
• Installed on uphill terrain at Kuhuku Point with predominantly upslope, onshore flow but occasionally experienced downslope flows (Kona Winds)
• Chronic underproduction relative to projections for both turbine designs
• Significant numbers of faults and failures occurred during the nighttime hours particularly on Westinghouse turbines. Serious loading issues with MOD-5B during Kona Winds required lock out
Oahu
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Hawaii – cont’d
• 81 Jacobs 17.5 and 20 kW turbines installed in mountain pass on the Kahua Ranch 1985-
• Wind technicians reported in 1986 a significant number of failures that occurred exclusively at night
• At some locations turbines could not be successfully maintained downwind of local terrain features and were abandoned
Hawaii
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2.5 MW MOD-2
• Post analysis showed loads much greater than had been predicted
• Highest loads generally to occurred during nighttime hours
• Terrain induced low-level jet structure developed during nighttime hours
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Uhub = 7.8 m/s Ri = − 0.12
Uhub = 9.0 m/s Ri = + 0.13
Uhub = 9.8 m/s Ri = + 0.26
Uhub = 12.8 m/s Ri = + 0.72
Uhub = 13.1 m/s Ri = + 6.68
Uhub = 6.5 m/s Ri = + 11.7
30-minute smoothed profiles from PNL Met Tower MOD-2 Site Goldendale, Washington MOD-2 Hub Height 61 m Wind speeds normalized by hub-height value - Stability measured between 2 and 107 m )
Time (LST) 16:00 02:00
Turbine Layer Vertical Wind Profile Evolution
wind speed
turbulence intensity
heig
ht
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San Gorgonio Pass California
• Large, 41-row wind farm located downwind of the San Gorgonio Pass near Palm Springs
• Wind farm had good production on the upwind (west) side and along the boundaries but degraded steadily with each increasing row downstream as the cost of turbine maintenance increased
• Frequent turbine faults occurred during period from near local sunset to midnight
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Pacific Ocean Salton
Sea
wind farms (152 m, 500 ft)
(−65 m, −220 ft)
(793 m, 2600 ft)
San Gorgonio Regional Terrain
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Palm Springs
Mt. Jacinto (
downwind tower
(76 m, 200 ft)
upwind tower
(107 m, 250 ft)
row 37
San Gorgonio Pass
nocturnal canyon flow
(3166 m, 10834 ft)
Wind Farm Nearby Topography
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SeaWest Wind Farm San Gorgonio Pass
• 1000 unit wind farm of 44, 65, 108 kW wind turbines (1989-90) • Significant turbine faulting occurred during late evening hours • Yaw drive slew rings required repositioning every 3 months and
replacement once a year
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Schematic of SeaWest San Gorgonio Wind Park
N
Additional
Operating
Wind Parks
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Park Energy Production and Maintenance & Operations Costs
Highest M&O Costs
Energy
M&O
High
Low
Low
High
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Daytime Flow Patterns Affecting the Wind Park
Westerly flow coming through the Pass
Warm air flows up towards mountain top replacing air heated by sun
Hot Southeasterly flow from Salton Sea
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Nighttime Flow Patterns Affecting the Wind Park
Cooler drainage flows from canyon to the south
Warmer flow coming through the Pass
Strong turbulence generated where two streams meet
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Micon 65 kW Turbine Inflow/Structural Response Testing
Hub-height sonic
anemometer
50 m Outflow Tower
(Row 41) AeroStar Rotor
SERI S-Series Rotor
30 m turbine inflow Tower
Row 37
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NWTC ART Turbine
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NWTC (1841 m – 6040 ft)
NWTC
Great Plains
Terrain Profile Near NWTC in Direction of Prevailing Wind Direction
Denver
Boulder
NWTC Regional Topography
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NWTC (1841 m – 6040 ft)
Marshall Mesa (1768 m – 5800 ft)
NWTC Local Topography
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Diurnal Variations in High Blade Loads
San Gorgonio Wind Farm Micon 65 Turbines at Row 37 Time-of-Day Distribution of Occurences of High Root Flapwise DEL
Local standard time (h)2 4 6 8 10 12 14 16 18 20 22 24
Prob
abili
ty (%
)
0
2
4
6
8
10
12
14sunrise sunrset
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22 24Pr
obab
ility
(%)
0
2
4
6
8OctMay Oct May
NWTC ART TurbineTime-of-Day Distribution of Occurences of High Root Flapwise DEL
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Wind speeds at High Loads
Hub mean wind speed (m/s)
8 10 12 14 16 18Pr
obab
ility
(%)
0
5
10
15
20
25
30
rated wind speed
NWTC ART Distribution of Mean Hub Wind Speeds Associated with High Values (P95) of Flapwise Root BM DEL
San Gorgonio Micon 65 (SERI Blades) Distribution of Hub-Height Mean Wind Speeds Associated with High Values (P95)
of Flapwise Root BM DEL
Hub mean wind speed (m/s)
8 10 12 14 16 18
Prob
abili
ty (%
)
0
10
20
30
40
rated wind speed
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Before we can proceed . . .
• We need to define a range of tools that we can employ to describe both the motions and thermodynamics of the ABL, its vertical structures, and the turbulence characteristics associated with those structures
• We will then be in a position to interpret the observed turbine aeroelastic response seen over a diurnal period
• First some atmospheric thermodynamics . . .
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Adiabatic Temperature Changes
• Air parcels moving vertically (lower pressure) in the atmosphere expand when rising and contract when descending (higher pressure)
• With this expansion/contraction their temperature changes in accordance with the 1st Law of Thermodynamics
• The following discussion assumes that the air we are tracking is dry and not saturated with water vapor
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Adiabatic Lapse Rate It can be shown that for dry air changing height from z1 (p1) and temperature T1 to z2 (p2) its temperature will be T2 as a result of an adiabatic expansion/contraction (assuming no heat is gained or lost in the process) And after taking the anti-logs of both sides This result allows us to define an adiabatic change in air temperature with a change in height (pressure) The rate of (heating/cooling) is 1o C per 100 m height change
2 2
1 1ln ln
dp
Rcp T
p T =
2 2
1 1
dp
Rcp T
p T =
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Potential Temperature
/
( )( )
d pR copT z
p zθ
=
Using the definition of the adiabatic lapse rate we can define the potential (or thermodynamic) temperature as . . .
where z is in meters T is in °K p and po are in equivalent units of pressure (mb, kPa, etc) po is a reference pressure = 1000 mb or 100 kPa Rd /cp = 0.286
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Concept of Atmospheric Stability
• Static Stability • Dynamic Stability
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Schematically
cold, dense air
warm, less
dense air
IT IS STABLE
But if . . .
IT IS UNSTABLE
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Static Stability
z
θ oK
z
θ oK
z
θ oK
Parcel has positive
buoyancy and will continue
to rise
Parcel has no net buoyancy
and will remain at this height
Parcel has negative buoyancy
and will return to its original level
It is Unstable It is Neutral It is Stable
If we vertically displace the air parcels below .. .
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Dynamic Stability or Instability
Time
Z
An example of dynamic instability
The right combination of vertical temperature and wind speed stratification can produce an oscillatory or resonant response in the wind field particularly in vertical motions
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Stability is Important
• The vertical stability exerts a significant influence over the nature of turbulence in the atmospheric boundary layer
• We will show that under certain narrow ranges of atmospheric stability, wind turbines can experience significant structural loading and fatigue damage
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Next . . .
• Now lets more on to describing atmospheric motions and their chaotic behavior --- turbulence!
• This is the stuff that wind turbine blades must ride through 24/7 year and year out
• ABL turbulence, while stochastic in nature, does exhibit spatial and temporal organizational structures and that have an impact on wind turbines and we will see
• First some basic definitions and turbulence scaling concepts . . .
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Flow Coordinate Systems
+UE
+VN +Wup Meteorological Coordinates U = E-W flow component V = N-S flow component W = vertical component
+u
+v +w Aligned with the local flow vector ±u = streamwise component (parallel to the mean streamline) ±v = lateral or cross-wind component ±w = vertical component
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Definition of Turbulent Wind Components
This image cannot currently be displayed.
0where
u u u
v v v
w w w
u v w
θ θ θ
θ
′= +
′= +
′= +
′= +
′ ′ ′ ′= = = =
Decompose orthogonal flow velocity components and temperature into mean and fluctuating (eddy) components ( ) ( )′
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The Role of Friction -- Vertical Shearing Stress
x (+u’)
z (+w’)
(-u’w’)1/2 ≡ u*
Downward flux or transport of horizontal momentum
friction or shear velocity
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Shearing Stress The Log Wind Profile
• Has a physical basis • Assumes that the shearing stress in the wind is
constant with height and that the influence of the earth’s rotation can be ignored
• The height of this “constant stress” layer can extend up to 200 m under neutral stability conditions
• This is called the “surface layer” of the atmospheric boundary layer
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The Log Wind Profile
Under these assumptions for a statically neutral boundary layer . . .
*( ) lno
u zU zk z
=
The “log” wind speed profile can be written
where zo is the surface aerodynamic roughness length
u* = 0.695 m/s zo = 0.1 m k = 0.4
U(z) (m/s)
0 2 4 6 8 10 12 14
Hei
ght (
z), m
0
20
40
60
80
100
120
140
160
180
200
u* = 0.695 m/s zo = 0.1 m k = 0.4
U(z) (m/s)
0 2 4 6 8 10 12 14
0.1
1
10
100
u* = slope*0.4
linea
r hei
ght
log
heig
ht
U(z) U(z)
zo
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Surface Layer (SL) Characteristics
• Assumes horizontal homogeneity
• The value of u* is approximately constant (> ±10%) throughout its depth ≅ constant shear stress
• The logarithmic wind profile applies
• The effect of the earth’s rotation can be ignored (insensitive to Coriolis accelerations)
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How Turbulence Scales in the Surface Layer Monin & Obukhov developed Similarity Theory using advanced dimensional analysis techniques
If the vertical fluxes of heat, moisture, and momentum are “constant” with height (everything is in a more or less steady state or balance), then the following velocity, temperature, and length scales can be used to scale turbulence in the surface layer: Velocity: * /ou τ ρ= where τo is the shear stress at the surface
and ρ is the air density
Temperature: * */oHT F u= −
Length: 3*
oH
uLkgF
θ= −
where FHo is the vertical heat flux at the earth’s surface
Often referred to as the M-O or Obukhov length
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Measures of SL Dynamic Stability
( )owθ′ ′ =
( )( )( )2
/ /
/
g zRi
u z
θ θ∂ ∂=
∂ ∂
3*
( / )( )/
og wzL u kz
θ θ′ ′= −
Gradient Richardson number, Ri Monin-Obukhov (M-O) stability parameter, z/L
turbulence generation by buoyancy turbulence generation by shear
=
where temperature flux at ground surface
k = 0.4 g = gravity acceleration
Ri, z/L < 0 = unstable; Ri, z/L = 0, neutral; Ri, z/L > 0, stable
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2 2 2
2 2 2
2
' ' ' ' ' '
' ' ' ' ' '
' ' ' ' ' '
, ,
, ,
1/ 2( )1/ 2[( ) (
u v w
u u u v u w
v u v v v w
w u w v w w
u w w u u v v u v w w v
u u v v w w
u v wu w u
σ σ σ
′ ′ ′ ′ ′ ′ ′ ′ ′ ′ ′= = =
′ ′ ′ ′ ′ ′= = =
′ ′ ′+ +
′ ′ ′ ′+
assume
Turbulent Kinetic Energy (TKE) =Coherent Turbulent Kinetic Energy (CTKE) = 2 2 1/2) ( ) )]v v w′ ′+
Reynolds stress tensor
Reynolds stress components (turbulence component
covariances)
1/ 2
* 0( )o
u u w ′ ′= − = momentum flux at ground surface
Turbulent Reynolds Stresses, Fluxes, & Kinetic Energy
Important Turbulence Fluid Dynamics Parameters
Need to be reasonably matched for proper modeling
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Surface Layer Turbulence Spectra Scales with Height Above Ground
v-component
f (Hz)0.001 0.01 0.1 1 10
f Sv(f)(m/s)2
0.01
0.1
1
λ (m)10-1100101102103104105
w-component
f (Hz)0.001 0.01 0.1 1 10
f Sw(f)(m/s)2
0.001
0.01
0.1
10-1100101102103104105
u-component
f (Hz)0.001 0.01 0.1 1 10
f Su(f) (m/s)2
0.01
0.1
1
λ (m)10-1100101102103104105
z = 25 mz = 125 m
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Turbulence Spectra Also Scaled by Stability (z/L)
f = cyclic frequency (Hz)
n = non-dimensional or reduced frequency
S(f) = power spectral density (m/s)2/Hz
3*
kzuε
εϕ = scales dissipation of TKE
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ABL Vertical Structural Characteristics
CBL
SBL
x
z wind
turbines
wind turbines
low-level jet height
zi
h
organized wave motions
convection cells
Convective Boundary Layer
Stable Boundary Layer
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ABL Diurnal Evolution
Local standard time
wind turbines
Mixed Layer (ML) Residual
Layer (RL) (SL)
free atmosphere (geostrophic flow)
transition regions
Real-world Example
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A Real World Example . . .
• Let’s look at the typical diurnal variation in many of the surface layer parameters we just discussed
• The data was derived from measurements at the SeaWest Wind Farm in San Gorgonio Pass California
• We start with what drives the whole shmear
The diurnal variation in incoming solar heat energy . . .
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Diurnal Variation of Vertical Heat Flux FH Mean Diurnal Near-Surface Vertical Heat Flux Over 5-50m Layer
San Gorgonio Pass, CaliforniaJuly-August 1990
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m2
-400
-200
0
200
400
600
800
sunrise sunset
Measured upwind of the wind farm’s first row of turbines
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Variation of Heat Flux and Power Law Wind Shear Across Rotors, α
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m2
-600
-400
-200
0
200
400
600
800
α
0.10
0.11
0.12
0.13
0.14
0.15
0.16
Mean vertical heat fluxα
1/7
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Variation of Heat Flux and Hub-Height (23m) Mean Wind Speed
Local standard time (h)0 2 4 6 8 10 12 14 16 18 20 22
W/m2
-600
-400
-200
0
200
400
600
800
m/s
12.5
13.0
13.5
14.0
14.5
15.0
Mean vertical heat fluxHub mean horizontal wind speed
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Diurnal Variation of Mean Heat Flux, Hub Wind Speed, and Turbulence Level
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m2
-600
-400
-200
0
200
400
600
800
σUH
m/s
2.3
2.4
2.5
2.6
2.7
2.8
2.9
3.0
3.1
0.10
0.11
0.12
0.13
0.14
0.15
0.16
Mean vertical heat fluxHub σUH
Hub TI
HU
hubUσ
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Variation of Heat Flux and Stability
Diurnal Variation of Mean Vertical Heat Flux and Stability Over 5-50m Layer
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m 2
-600
-400
-200
0
200
400
600
800
z/L, Ri
-0.10
-0.05
0.00
0.05
0.10
0.15
0.20
Heat flux
z/L
Ri
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Variation of Heat Flux and Mean Shearing Stress, u*
Diurnal Variation of Mean Vertical Heat and Momentum Fluxes and Stability
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m 2
-600
-400
-200
0
200
400
600
800
z/L
-0.10
-0.05
0.00
0.05
0.10
0.15
0.20
u * m/s
0.64
0.68
0.72
0.76
0.80
0.84
0.88
Heat flux z/L Hub u *
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Variation of Heat Flux and Mean Reynolds Stresses
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m2
-600
-400
-200
0
200
400
600
800
m/s
-1.0
-0.8
-0.6
-0.4
-0.2
0.0
0.2
0.4
Mean vertical heat flux
' 'u w
' 'u v
' 'v w
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Diurnal Variation of Vertical Heat Flux and C D with Stability
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m 2
-600
-400
-200
0
200
400
600
800
z/L -0.10
-0.05
0.00
0.05
0.10
0.15
0.20
C D
0.036
0.040
0.044
0.048
0.052
0.056
Heat flux z/L C D
Variation of Heat Flux, Stability, and Surface Drag Coefficient CD
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Variation of Heat Flux and Turbulent Component Std Devs
σu, σv, σw Diurnal Variation of Vertical Heat Flux and
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22
W/m 2
-600
-400
-200
0
200
400
600
800
σ u
m/s
1.65
1.70
1.75
1.80
1.85
1.90
σ v
m/s
1.2
1.3
1.4
1.5
1.6
1.7
σ w
m/s
0.80
0.82
0.84
0.86
0.88
0.90
0.92
0.94
Heat flux σu σv σw
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Back to the Micon 65 Loads Data …
• Let’s now take a look at the distribution of blade root damage equivalent blade loads as a function of other turbulence scaling parameters
• First vertical dynamic stability, Ri
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Comparison of Measured Turbine Loads as Function of Stability, Ri
San Gorgonio Wind Farm Row 37 (7D spacing) Micon 65/13 Wind Turbines Root Flapwise BM Equivalent Blade Loads
Ri -0.3 -0.2 -0.1 0.0 0.1 0.2
DEL eq (kNm)
8
10
12
14
16
18
20
22
24
SERI Rotor AeroStar Rotor
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Hmmm . . .
How do these compare with our blade root load measurements at on the NWTC ART Turbine?
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Ri Values Associated with High Blade Root Fatigue Loads for the San Gorgonio Wind Farm and the NWTC
San Gorgonio Distribution of Turbine Layer Ri Associated with High Values of Flapwise BM DEL
Turbine Layer Vertical Stability, Ri-0.06 -0.04 -0.02 0.00 0.02 0.04 0.06 0.08 0.10
Prob
abili
ty (%
)
0
10
20
30
40
50
60
Turbine Layer Vertical Stability, Ri
-0.08 -0.06 -0.04 -0.02 0.00 0.02 0.04Pr
obab
ility
(%)
0
5
10
15
20
25
NWTC ART Distribution of Turbine Layer Ri Associated with High Values (P95) of Flapwise BM DEL
Both peaks occur in weakly or slightly stable conditions!
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Example of Rotor Encountering a Coherent Turbulent Structure – Aeroelastic Response
edgewise root bending moment (kNm)
AeroStar flapwise root bending moment (kNm)
SERI blade AeroStar blade
Blade 1 Blade 2
Blade 3
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3-D Coherent Turbulent Structure at Hub Height Responsible for AeroStar Rotor Response
Instantaneous local Reynolds stresses (m/s)2
Estimated local vorticity components (rad/sec)
ωy
ωz
v’w’
u’v’
u’v’ v’w’
ωx ωy ωz
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Correlation with Other Turbulence Parameters
• Correlation analysis of root flapwise bending equivalent loads with a range of turbulence parameters found strong correlations with the following:
– The mean hub-height wind speed (as would be expected) – The hub measurement of –u’w’ or its equivalent, u*hub – This suggests that large, transient blade loads are often
associated with strong downward bursts of organized turbulence
– A new fluid dynamics parameter is needed that represents the intensity of coherent or organized turbulence that can be correlated with load parameters such as DEL
National Renewable Energy Laboratory Innovation for Our Energy Future 65
Reflects the larger swept area of the SERI rotor
Underlying response is nearly identical
Variation of 3-Blade Mean Flapwise BM with Hub Mean U-component
Uhub (m/s)
4 6 8 10 12 14 16
kNm
5
10
15
20
25SERI RotorAeroStar RotorSERI trendAeroStar trend
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Correlation of Flap DEL with Uhub
The fatigue response of both rotors is nearly identical except at the highest wind speeds The slightly lower fatigue of the AeroStar rotor is probably due to its rated wind speed is slightly higher
Variation of Flapwise BM DEL vs Mean U-component
Uhub (m/s)
4 6 8 10 12 14 16
kNm
8
10
12
14
16
18
20
22
24
SERI RotorAeroStar RotorSERI trendAeroStar trend
National Renewable Energy Laboratory Innovation for Our Energy Future 67
Correlation of Flap DEL with u’w’ Variation of 3-Blade Average Flapwise BM DEL
with Mean Downward Momentum Flux u'w'
u'w'hub (m/s)-4-3-2-10
kNm
8
10
12
14
16
18
20
22
24
SERI RotorAeroStar RotorSERI trend AeroStar trend
Reflects stall characteristics of rotor blades Both rotors are responding similarly to downward bursts of organized turbulence
National Renewable Energy Laboratory Innovation for Our Energy Future 68
NWTC ART Turbulence-Aeroelastic Response Correlations
• The ART dataset encompasses a much larger record of inflow conditions that occurred over an entire wind season
• There were no large turbines operating upstream so the response was due to the natural turbulence experienced at the NWTC and not enhanced by the presence of multiple rows of upwind turbines
• Five sonic anemometers were employed in an array upstream of the rotor
• We cross-correlated the root flapwise BM DEL with several inflow parameters
National Renewable Energy Laboratory Innovation for Our Energy Future 69
NWTC 43-m Inflow Array
cup anemometer
hi-resolution sonic anemometer/thermometer
wind vane
T temperature, DP dewpoint temperature
FT fast-response temperature ∆T Temperature difference BP Barometric pressure
T
∆T
, DP, BP
NWTC 600 kW Advanced Research Turbine No.1
58 m
37 m
15 m
FT
FT
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Observed Diurnal Blade Root Flap DEL Tail Distributions
Local standard time (h)2 4 6 8 10 12 14 16 18 20 22 24
Bla
de r
oot f
lap
DE
L (k
Nm
)
200
210
220
230
240
250
260 P90P95
Diurnal Distribution of Number of Hours in DEL Distribution
Local standard time (h)2 4 6 8 10 12 14 16 18 20 22 24
Hou
rs o
f rec
ord
0
4
8
12
16
20
Diurnal Variation of ART High Flap DELs
Data loss due to frequent
wind speeds above turbine
cutout
National Renewable Energy Laboratory Innovation for Our Energy Future 71
Correlation of ART Hub U-component with Flapwise BM DEL
Variation of ART Flap DEL with Hub Mean U-component
Uhub (m/s)4 6 8 10 12 14 16 18 20
kNm
50
100
150
200
250
300
350
National Renewable Energy Laboratory Innovation for Our Energy Future 72
Diurnal Variation of Flap DEL and Hub Mean Wind Speed
Observed Diurnal Relationship Between Blade Root Flap DEL and Hub Mean Wind Speed
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22 24
DEL (kN
m)
200
210
220
230
240
250
260
Uhu
b (m
/s)
8
10
12
14
16
P90 DELP95 DELP50 UhubP90 UhubP95 Uhubrated wind speedmean P50 wind speed
National Renewable Energy Laboratory Innovation for Our Energy Future 73
Variation of Root Flap DEL with Ri Observed Diurnal Variation of Turbine Layer RiTL and Corresponding Flapwise Root BM DEL Distributions
Ri T
L
-0.3
-0.2
-0.1
0.0
0.1
0.2
P10P25P50P75P90
Local standard time (h)2 4 6 8 10 12 14 16 18 20 22 24
kNm
200
210
220
230
240
250
260 P90P95
critical upper limitsignificant turbine response upper limit
Variation of Blade Root Flap DEL with Turbine Layer RiTL
Turbine layer RiTL
-0.25 -0.20 -0.15 -0.10 -0.05 0.00 0.05 0.10 0.15 0.20 0.25B
lade
roo
t fla
p D
EL
(kN
m)
50
100
150
200
250
300
National Renewable Energy Laboratory Innovation for Our Energy Future 74
Little or no correlation with the usual suspects Variation of Blade Root Flap DEL with Hub-Height U
Hub (37-m) U (m/s)0 1 2 3 4 5
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300
Variation of Blade Root Flap DEL with Rotor-Disk Shear Exponent,
Rotor disk shear exponent, a0.00 0.05 0.10 0.15 0.20 0.25 0.30 0.35 0.40
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300 1/7 shear exponentIEC NWP exponent
Variation of Blade Root Flap DEL with Hub Ihub (TI)
Ihub
0.00 0.05 0.10 0.15 0.20 0.25 0.30 0.35 0.40
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300
Variation of Blade Root Flap DEL with Disk-Averaged u*
Disk averaged u* (m/s)0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300
National Renewable Energy Laboratory Innovation for Our Energy Future 75
However with the local value of σw … Variation of Flapwise DEL with w(z)
w(z) (m/s)0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8 2.0
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300
58-m37-m15-m
National Renewable Energy Laboratory Innovation for Our Energy Future 76
And Diurnally with the Hub value of σw . . .
Observed Relationship Between Blade Root Flap DEL and Hub (37-m) w
Local standard time (h)
0 2 4 6 8 10 12 14 16 18 20 22 24
DEL (kN
m)
200
210
220
230
240
250
260
w (
m/s
)
0.3
0.4
0.5
0.6
0.7
DEL P90DEL P95 w P50
w P90
w P95
w P99
National Renewable Energy Laboratory Innovation for Our Energy Future 77
Some Hints
• The strong correlation with the flap DEL and σw as a function of height suggests a strong downward transport mechanism is a work at the NWTC.
• The question is what is being transported? • A detailed examination revealed the existence of
intense coherent turbulent structures entering the rotor disk and its upwind measurement array from above.
• Clearly we needed to define a turbulence parameter that reflected the spatial and temporal organization of these structures and their intensity.
National Renewable Energy Laboratory Innovation for Our Energy Future 78
Coherent Turbulence Kinetic Energy (CTKE)
• Turbulent kinetic energy is defined as
TKE = ½ (σu2 + σv
2 + σw2)
it says nothing about the correlations between u, v,& w
• However the off-axis Reynolds stress components represent the covariance and cross-correlation between these three orthogonal components – u’w’, u’v’, and v’w’
• Extending the TKE concept, we define a coherent kinetic energy parameter as CTKE = ½ [(u’w’)2 + (u’v’)2 + (v’w’)2)]1/2 where CTKE is always ≤ TKE and is 0 in isotropic flow
National Renewable Energy Laboratory Innovation for Our Energy Future 79
NWTC ART Flap DEL vs pk CTKE
Max Flap BM RF cycle
1 10 100
kNm
0
100
200
300
400
500
600
700
Flap BM DEL
kNm
0
50
100
150
200
250
300
350
Flap BM DEL
kNm
0
50
100
150
200
250
300
350
Max Flap BM RF cycle
Hub Peak CTKE (m2/s2)1 10 100
kNm
0
100
200
300
400
500
600
700
Entire Population Below-Rated Sub-population
National Renewable Energy Laboratory Innovation for Our Energy Future 80
High Blade Fatigue Loads are Induced by Intense, Fluctuating Vertical Transport of CTKE
Variation of Flapwise DEL with Standard Deviation of Vertical Flux of CTKE
w'CTKE(z) standard deviation (m3/s3)
0 5 10 15 20 25 30 35
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300
58-m37-m15-m
National Renewable Energy Laboratory Innovation for Our Energy Future 81
Variation of Hub Peak CTKE with w(z)
w(z) (m/s)
0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8 2.0
Hub
pea
k C
TKE
(m2 /s
2 )
0
20
40
60
80
100
120
58-m37-m15-m
National Renewable Energy Laboratory Innovation for Our Energy Future 82
Vertical Flux of pk CTKE by Height Variation of Blade Flap DEL with Peak Vertical Flux of CTKE
peak w'CTKE(z) (m3/s3)
-600 -400 -200 0 200 400 600
Bla
de r
oot f
lap
DE
L (k
Nm
)
50
100
150
200
250
300
58-m37-m15-m
Indicates strong vertical transport of coherent turbulence is taking place at NWTC
National Renewable Energy Laboratory Innovation for Our Energy Future 83
San Gorgonio Diurnal Variations of Flap DEL and Inflow Parameters
Hub
pea
k C
TKE
(m/s
)2
10
20
30
40
50
60
P90
Local standard time (h)2 4 6 8 10 12 14 16 18 20 22 24
peak
u'w
' (m
/s)2
-100
-80
-60
-40
-20
P90
Uhu
b (m
/s)
4
6
8
10
12
14
16
Local standard time (h)
2 4 6 8 10 12 14 16 18 20 22 24
3-B
lade
Mea
n Fl
apw
ise
BM
DE
L (k
Nm
)
8
10
12
14
16
18
20
22
24
SERI RotorAeroStar Rotor
P90
rated
P90
Uhub Hub pk CTKE
Flap DEL Pk u’w’
National Renewable Energy Laboratory Innovation for Our Energy Future 84
CTKE – cont’d
• CTKE is easy to measure with the three-axis sonic anemometers we have used to measure the turbulent properties of the inflows to the San Gorgonio Micon 65 turbines and the NWTC ART.
• On the average, the ratio of CTKE/TKE is about 0.4 but it can range from 0.2 to 0.9.
• CTKE represents the intensity of turbulent coherent elements in the flow as they pass through the measurement volume of a sonic anemometer.
National Renewable Energy Laboratory Innovation for Our Energy Future 85
Our Conclusions Are …
• The largest turbine fatigue loads are primarily associated with slightly stable conditions within a narrow range of the turbine- layer gradient Ri stability parameter
• They are often not associated with the high values of σU or turbulence intensity (σU/U)
• The vertical transport of coherent turbulence energy from above and within the wind farm rotor disk layer is a major contributor to high fatigue loads.
• It is important when simulating turbine inflow turbulence to include the ability to (1) model a range of stability conditions and (2) develop a method to include organized, turbulent structures.
National Renewable Energy Laboratory Innovation for Our Energy Future 86
Problem:
• Modern multi-megawatt turbines often operate their rotors simultaneously in both the surface and mixed layers
• No consensus on the best way to scale turbulence in this layer. Some form of a combination of SL and local scaling is generally used
• We have found that the average height of the SL is the order of 50-60 m and higher during the day and lower at night
• We have scaled it in our TurbSim code from actual measurements taken at two locations: the NWTC Test Site and Lamar, Colorado
National Renewable Energy Laboratory Innovation for Our Energy Future 87
Defining Additional Flow Variables for Coherent Turbulence
• We would like a single variable that reflects the intensity of highly correlated turbulent structures seen in the three cross-axis Reynolds stresses