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Codification of Wind Loads on
Wind-sensitive StructuresJohn D. Holmes
Director, JDH Consulting, Australia
Received January, 24, 2008; Revised version February, 24, 2009; Acceptation March, 03, 2009
ABSTRACT: Codified approaches for allowing for along-windresonant response of tall structures are reviewed. In particular the‘gust loading factor’ (GLF) format, used in codes and standardsbased on mean wind speeds (normally with an averaging time of 10minutes or 1 hour) is discussed. The alternative ‘dynamic response
factor’ (DRF) format, generally adopted by codes based on peak(nominally 3-second) gust wind speeds is also described. Theexplicit, or implicit, effective static wind load distribution inherentin these approaches is also discussed. The codification of the cross-wind response of tall structures of rectangular or circular cross-sections is also considered. A comparison of cross-wind forcespectra for some rectangular cross-sections used in current codesand standards is made. Some consideration of the codification of wind-induced fatigue is given. Finally the present use, and futurepotential, of internet-based design methods for dynamic wind loadsis discussed.
Keywords: Buildings; Codes; Dynamics; Fatigue; Towers; Vibration; Wind
loads.
1. INTRODUCTION
It is well known that as structures become taller (or
longer), they become more dynamically sensitive to
fluctuating wind loads in large-scale synoptic wind
events, arising from upstream turbulence, or from
wake- and vortex-induced forces. Many important
structures have specific wind engineering studies
carried out for them, usually involving wind-tunnel
tests. However, there is a large class of structures,
which have some dynamic sensitivity to wind, but for which the time and expense of special wind
engineering studies cannot be justified. In other cases,
such as chimneys, towers or masts of circular cross-
section, wind tunnels cannot give reliable results for
scaling reasons.
There is an important part to play by wind loading
codes and standards, and related desk-top approaches
in the design for wind of dynamically sensitive
structures – either for structures for which extensive
wind engineering studies (including wind-tunnel tests)
cannot be justified, or in preliminary design stages of
more complex structures. This paper reviews the basic
concepts and design approaches adopted by several
advanced wind codes and standards, and related
design-oriented sources, for resonant response to
wind. Both along-wind and cross-wind forces and
response are considered.
The paper primarily focuses on codification
approaches to the dynamic response of tall buildings
and towers, and smaller cantilevered structures such aslighting poles. Structures such as large roofs and
bridges are not discussed in this paper; generally the
behaviour of these structures to winds is too complex
to allow simplified code methods to be applied.
2. ALONG-WIND RESPONSE
2.1 History The earliest modern approach to codification of the
dynamic response of structures was the ‘gust
loading factor’ (GLF) approach proposed nearly
International Journal of Space Structures Vol. 24 No. 2 2009 87
•Corresponding author. E-mail Address: [email protected]
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88 International Journal of Space Structures Vol. 24 No. 2 2009
Codification of Wind Loads on Wind-sensitive Structures
Figure 1. A Simple Dynamic System for Determination of
Gust Loading Factors.
simultaneously by B.J. Vickery [1] and A.G.
Davenport [2]. This followed earlier pioneering work
by Davenport on the application of random process
theory to the wind loading of structures. Davenport
had earlier developed a gust loading factor for the
Danish Standard.
In 1968, Vellozzi and Cohen [3] developed asimilar approach for a ‘gust response factor’ (in fact
conceptually identical to the GLF) that was adopted in
the ANSI wind loading standard of 1972. It
introduced the effect of the along-wind correlation,
which was intended to account for the less than
perfect correlation between windward and leeward
pressure fluctuations on a building. There were a
number of other developments and refinements for
tall buildings in the nineteen-seventies and -eighties.
Amongst these, Vickery [4] in 1971 considered the
variability and reliability of GLF estimates,introduced a size factor based on the cross-spectral
density of the upwind velocity fluctuations, and
considered the effects of nonlinear mode shapes.
Simiu [5,6] corrected the implementation of
windward-leeward wall correlation by Velozzi and
Cohen, and introduced more ‘meteorologically-
correct’ wind spectra and velocity profiles. Solari [7]
developed Simiu’s procedure with closed form
approximations for easier application.
As early as 1976, the Engineering Sciences Data
Unit in the U.K. introduced a detailed calculationmethod for along-wind response of flexible
structures [8]. This did not explicitly use the GLF
format, but was based on the same random vibration
concepts and theory. However, it introduced several
new refinements to the calculations: separate peak
factors for background and resonant response,
calculation of load action effect such as bending
moments and shear forces, and the inclusion of
aerodynamic damping. In these respects it was
significantly ‘ahead of its time’. In the Guide to the
British Standard on Lattice Towers and Masts of 1986 [9], detailed equations were given for the
evaluation of gust (loading) factors for lattice towers;
a particular innovation was the consideration of
cross-bracing members with influence lines with sign
reversal. However, the full dynamic method was not
implemented as part of the Standard itself.
Milford [10] developed a simplified GLF
calculation method for lighting poles and masts, using
simplifications resulting from the small frontal areas
exposed to wind forces. This method was incorporated
into a South African Code of Practice for LightingMasts.
2.1 Gust Loading Factor – Basic Derivation In all the references discussed previously, the gust
loading factor is calculated on the basis of the
generalized deflection of a structure assumed to move
in the first sway mode of vibration. In the derivation of the expressions for the GLF, the dynamic behaviour of
a building, or other tall structure, is usually simplified
to that of a simple single-degree-of freedom system, as
shown in Fig 1. Using this concept and random
process theory, the spectral density of the deflection, x,
can be simply related to the spectral density of the
applied (drag) force as follows :
(1)
where |H(n)|2 is a ‘mechanical admittance’ function.A modification of Eqn 1 replaces the response
variable x, by the internal spring force, k.x, denoted by
D*. Then Equation (1) becomes:
(2)
The velocity fluctuations do not occur
simultaneously over the windward face of a large
building, and their correlation over the whole area
must be considered. To allow for this effect, an
aerodynamic admittance, X 2(n), was introduced.
Then, (3)
X 2(n) is usually determined from the correlation
properties of the upwind velocity fluctuations, on the
assumption that the building does not distort the
approaching turbulence in the wind.
The expected maximum deflection response of the
simple system in Figure 1, can be written :
(4)x̂ x g x= + σ
S (n)1
kH(n)
4D
U. (n).S (n)x 2
22
2
2
u= X
S (n) H(n) S (n)D*
2
D=
S (n)1
kH(n) S (n)x 2
2
D=
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John D. Holmes
International Journal of Space Structures Vol. 24 No. 2 2009 89
where is the mean deflection, σx is the standard
deviation of the deflection, and g is a peak factor,
which depends on the time interval for which the
maximum value is calculated, and the frequency range
of the response.
Then the gust loading factor is given by :
(5)
where σu is the standard deviation of along-wind
turbulence fluctuations, is the mean wind speed, B
and R are background and resonant terms, resulting
from the integration of the right-hand-side of Eqn 3
over all frequencies.
Thus, the GLF is essentially the ratio between the
expected maximum response (e.g. deflection or stress)
in a structure and the mean response, with the implied
representation of wind loading as a stationary random
process. It should be noted that in the simple model of
Figure 1, the GLF for deflection, Gx, is identical to that
for the internal force, GD*, since x and D* are related
by a constant factor, k. However, this simple
relationship does not apply for real structures with
distributed mass and stiffness. The variability of the
GLF with the response parameter is explored in the
following section.
The gust loading factor concept is retained, in its
original form, in the National Building Code of
Canada [11]. A similar form is adopted in the
Architectural Institute of Japan Recommendations
[12]. Other international codes and standards have
adopted a ‘dynamic response factor’ format, discussed
in a later section of this paper.
More details on the application of random process
theory to wind loading of structures are given in [13].
2.2 Modification for Cantilevered Towers The GLF was proposed primarily for tall buildings, in
which the resonant response to wind can often be
assumed to be restricted to the lowest sway dynamicmodes. Reducing the structure to a single-degree-of
freedom (mass-spring-damper) and calculating the
GLF for the deflection – as discussed in the previous
section - is equivalent to calculation of the GLF for the
generalized coordinate in the first mode of vibration.
However this GLF is not necessarily identical to the
GLF s for responses such as bending moment or shear
force at any elevation on the structure, or even the
actual deflection at the top of a tall structure. The
model developed by Holmes [14,15] enables the GLF
as a function of response variable to be determined.This model was originally developed for lattice towers,
U
G Gx
x1 g
x1 2g
UB Rx D*
x u= = = + = + +ˆ σ σ
x but can be applied to any prismatic or tapered structure,
for which a uniform drag coefficient is applicable.
The formulae for determination of the GLF s are as
follows:
Generalized co-ordinate:
(6)
Shearing force at any elevation:
(7)
Bending moment at any elevation:
(8)
Deflection at the top:
(9)
Bs, S and E are background, size and gust energy
factors, respectively. r is a roughness factor, equal to
twice the turbulence intensity (σu / ), evaluated at the
top of the structure. gB and gR are peak factors
separately evaluated for the background and resonant
response. s is the height at which the bending moment
or shearing force is required.
The factors F1,F2, ….…… F12 are defined in Refs 14
and 15, and account for the exponents of the mean
velocity profile and mode shape, and the mass
distribution and taper ratio on the structure. They alsoincorporate the elevation at which the shearing force or
bending moment are being evaluated. Note that, unlike
the simple structure of Fig 1, the GLF s for deflection,
and for internal forces such as shearing force and
bending moment, are not identical to each other.
Eqn 6 is representative of the usual GLF
calculations in codes and standards.
Comparisons of GLF calculated for the generalized
coordinate (using Eqn 6), and for the bending
moments and shear forces at various heights (using
Eqns 7 and 8) on a 160-metre tall tapered lattice tower,and a 183-metre tall building, of uniform cross section,
U
G
r g B F gSE
F F F
Fx
B
2
0 11 R
2
1
3 4 12
1
= +
+
1η
00
G
r g B F gSE
F F F
Fm
B
2
s 7 R
2
1
3 4 8
6
= +
+
1η
G
r g B F gSE
F F F
Fq
B
2
s 2 R
2
1
3 4 5
1
= +
+
1η
G 1 r g B gSE
B
2
s R
2
1
= + +
η
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90 International Journal of Space Structures Vol. 24 No. 2 2009
Codification of Wind Loads on Wind-sensitive Structures
Table 1. Comparison of GLF’s for Various Load
Effects – 160m Tapered Tower
(mean wind speed at top of tower = 30 m/s)
Load effect GLF
Generalized coordinate 1.69
BM at 0 m 1.74
BM at 80 m 1.89
BM at 120 m 2.02
SF at 0 m 1.77
SF at 80 m 1.87
SF at 120 m 2.00
Table 2. Comparison of GLF’s for Various Load
Effects – Tall building (183 m)
(urban terrain – mean wind speed at top of tower
= 30 m/s)
Load effect GLF
Generalized coordinate 2.14
BM at 0 m 2.21
BM at 90 m 2.31
BM at 135 m 2.36
SF at 0 m 2.25
SF at 90 m 2.31
SF at 135 m 2.36
are tabulated in Tables 1 and 2, respectively. These
Tables show that the GLF for the generalized
coordinate underestimates the GLF for both BM and
SF at all elevations. The GLF increases with elevation
of the load effect, for both the tower and the tall
building In the case of the tower, the increase is more
significant. The reasons for the last effect are the
greater importance of both the background and the
resonant components at the higher elevations, in
comparison with the mean wind loading. In the case of
the background contribution, this is because of the
reduced height for correlation of the applied
fluctuating forces; for example for a load effect
evaluated at half height, the effective height over
which the wind forces are reduced due to correlation
effects is reduced by a factor of two. In the case of the
resonant contribution, the effective (inertial) loads are
more highly weighted to the top of the structure than is
the mean wind loading.
2.3 Dynamic Response Factor In codes and standards which are based on a gust
loading (typically a 3-second gust) rather than a meanwind loading, use of a ‘dynamic response factor’
(DRF) is more appropriate than a GLF or GRF. This
approach is also better for transient, or non-stationary,
winds, such as downbursts from thunderstorms.
The DRF may be defined in the following way:
(10)
The DRF is an expression of the following ratio:
(maximum response including resonant and
correlation effects)
(maximum response calculated ignoring both
resonant and correlation effects)
Note that for codes and standards based on a gust
wind speed, the gusting effects are incorporated in the
wind speed itself. The DRF as defined in Equation
(10) simply modifies the loading to account for
correlation and resonant dynamic effects.
The denominator of Equation (10) is proportional to
the ‘gust envelope’ response calculated using ‘static’
methods in codes and standards. The dynamic response
factor, as defined above, will usually have a value close
to 1.0. A value greater than 1 can only be caused by a
significant resonant response. The turbulence intensity,
Iu in the denominator is usually taken as a single value
– i.e. that at or near the top of the structure. In this case,
a single value of cd results for all heights on the
structure. A direct conversion from a GLF approach
would require the turbulence intensity in the
denominator, and hence cd, to vary with height, z.
The dynamic response factor format has been
adopted for ASCE-7 [16], by the Australian/New
Zealand Standard [17], and by the Eurocode [18]. In
ASCE-7, it is known as a ‘gust effect factor’; this is a
rather confusing terminology (retained from earlier
versions of ASCE-7) as the gust effects are already
incorporated through the use of a 3-second gust speed.
2.4 Effective Static Loading Distributions In the original concept of the GLF, it is implied that thepeak effective loading should be distributed over the
height of the structure with the same distribution shape
as the mean wind loading, but factored by the GLF
itself. For codes and standards using the DRF format,
the basic effective distribution of wind loading with
height is the distribution of gust envelope loading; the
magnitude of this is factored up or down by the DRF.
Zhou and Kareem [19] recommended an approach
for the ASCE-7 Standard in which the resonant
component is distributed correctly as inertial loads,
with the mean and background components distributedas the mean loading. Although this approach is an
c1 2I g B g R
1 2gId
u B
2
R
2
u
=+ +
+
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John D. Holmes
improvement, it is also not completely correct. Figure
2 shows the correct effective distributions of mean,
background and resonant loads for the base bending
moment on the 160 metre tall tapered tower,previously discussed. These distributions are
consistent with Equation (8) for the gust loading factor
for base bending moment, Gm, with s set equal to 0.
The background component has its own distribution
which is neither the mean nor the inertial loading. On
average the distribution of background loading is
proportional to the correlation coefficient between the
load effect (i.e. the base bending moment in the case of
Figure 2), and the fluctuating wind pressure at each
height.
As discussed earlier, the effective static loaddistribution implied by the use of the DRF is
proportional to the peak gust envelope. For a structure
with a small resonant response, this is a better
approximation to the correct combined effective static
load distribution, than is an effective load distribution
based on the mean load distribution, as used in codes
and standards adopting the GLF format.
3. CROSS-WIND RESPONSE
The cross-wind dynamic response of structures can be
as significant as the along-wind response for several
classes of structure:
a) Tall buildings – say greater than about 100 metres
in height,
b) Cantilevered structures of circular cross-section,
such as chimneys or lighting poles,
c) Horizontal structures such as long-span bridges
or stadium roofs of very large dimensions.
On the other hand, open lattice structures, such as
communication towers, do not generally experience
large cross-wind response. The driving mechanism for
cross-wind response is usually regular vortex
shedding, with a lesser contribution from lateral
turbulence.
The codification cross-wind response of tall
cantilevered structures has proved to be difficult, buthas been attempted in a number of documents.
3.1 Tall Buildings of Rectangular Cross-section A random vibration approach to the cross-wind
response of tall buildings of simple rectangular cross-
section is the basis of the methods applied in the
Recommendations of the Architectural Institute of
Japan [12] (AIJ), and in the Australia/New Zealand
Standard [17]. In the former case, a series of
parameters are defined that are each a function of the
side aspect ratio of the cross section. However, in the
AIJ there is no dependence on the height aspect ratio.
In the AS/NZS, data is given which enables estimation
of the cross-wind response of a limited number of
building geometries for two different turbulence levels.
The uncertainty for the designer with regard to
cross-wind response is illustrated in Figure 3, which
shows the non-dimensional spectral density of cross-
wind generalized forces for a simple building of
square cross section, with a height of six times the side
length – i.e. a building with proportions of 6:1:1. This
is the key aerodynamic parameter from which cross-
wind responses are calculated. The Figure shows
experimental data and specified data from the AIJ [12]
(12) and AS/NZS [17].
The ordinate is the non-dimensional cross-wind
force spectrum coefficient, Cfs, as defined in the
Australian/New Zealand Standard [17]. The abscissa
in Figure 3 is the reduced velocity given by:
(11)UU
n.br
h=
International Journal of Space Structures Vol. 24 No. 2 2009 91
0
0.0 0.2 0.4 0.6 0.8 1.0
20
40
60
80
100
120
140
160
Effective pressure (kPa)
H
e i g h t ( m )
Combined
Resonant
Background
Mean
Figure 2. Effective Static Load Distributions for Base Bending Moment on a Tapered Tower.
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is the mean wind speed at the top of the
building; n is frequency, and b is the building width.
The usual range of reduced velocity in practical
situations is 2 to 8.
Considering the logarithmic axes in Figure 3, the
differences between the data lines in Figure 3 are very
large, and would result in very different cross-wind
responses if used by a designer. However, there are
currently moves to ‘benchmark’ wind-tunnel
measurements of tall buildings, with some standardized
building shapes; this may resolve some of the
variability in Figure 3, and similar comparisons for
other shapes.
3.2 Structures of Circular Cross-section Towers, chimneys, masts and poles of circular cross
section are prone to suffer cross-wind response at
lower and more frequent wind speeds than those with
sharp edged sections, such as square or rectangular.
The reason for this is that the fluctuating forces are
primarily induced by vortex shedding. For the same
wind speed and section breadth, the rate of shedding is
approximately twice for circular cross sections than it
is for sharp edged bodies. Hence, resonance with the
natural first-mode vibration frequency of the structureoccurs at a critical wind speed about half that for a
square structure of the same width. The critical wind
speed for circular sections corresponds to a reduced
velocity, as defined by Equation (11), of about 5.
For masts and poles of very small diameter, the
critical wind speeds can be very low (i.e. 2–3m/s) and
vibrations often occur in the early morning or evening
when atmospheric conditions are thermally ‘stable’
with low turbulence. The latter can lead to more
coherent and effective vortex shedding, and hence
more severe vibrations.
Although it is a common phenomenon throughout
the world, the prediction of vortex-induced vibrations
has resisted codification until fairly recently. In many
documents, the advice given does not go beyond a
simple expression for critical wind velocity.
There are two classes of calculation methods for the
cross-wind vibrations of circular sections:
a) Methods based on the assumption of sinusoidal
excitation forces
b) Methods based on random vibration theory.
The sinusoidal model has been adopted for the
Australian/New Zealand Standard [17] – in Section
6.3.3.1 of that Standard. The random model is used in
the American Standard for Steel Stacks ASME STS-1-1992 – Appendix 5.C [20]. Both methods have been
U h
92 International Journal of Space Structures Vol. 24 No. 2 2009
Codification of Wind Loads on Wind-sensitive Structures
0 . 0 0 0 0 1
0 . 0 0 0 1
0 . 0 0 1
0 . 0 1
0 . 1
0 1 0
1 0 0
Reduced Velocity
C f s
A I J - 2 0 0 4
A S / N Z S 1 1 7 0 . 2
I u = 0 . 2 0
A S / N Z S 1 1 7 0 . 2
I u = 0 . 1 2
N D s u b u r b a n 6 : 1 : 1
N D u r b a n 6 : 1 : 1
T K U u r b a n
T K U o p e n
H K U S T 5 : 1 : 1 o p e n
Figure 3. Cross-Wind Force Spectrum Coefficients for a 6:1:1 Building (Showing Code Values and Experimental Data).
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John D. Holmes
adopted as alternative approaches in the Eurocode for
Wind actions – Annex C [18].
In the AS/NZS [17], the following simple formula is
given for the maximum amplitude of tip deflection:
(12)
bt is the average breadth (diameter) of the two third of
the structure, corresponding the region where the
exciting forces have their greatest effect.
Sc is the Scruton Number defined as follows:
(13)
The key parameters in Equation (13) are mt, the
mass per unit height over the top third of the structure,
and ζ, the ratio of structural damping to critical
damping. ρair is the air density.
It can be seen from Equations (12) and (13) that
increasing either, or both, of the mass or the damping
will reduce the vibration amplitude. Interestingly, the
amplitude of vibration given by Equation (12) is
independent of both wind speed and the natural
frequency of the structure. The theory on which
Equation (12) is based is given in Reference (13)
(amongst other places).
The sinusoidal approach to cross-wind response is
somewhat simplified, but enables a quick indication of
the likelihood of vortex-induced vibrations occurring.
If high amplitudes are predicted it is usually better to
reduce these by increasing mass or damping (including
auxiliary damping devices) or by other means (e.g.
aerodynamic devices such as helical strakes, or by
guying, or linking adjacent chimneys to each other).
4. FATIGUE
Fluctuating stress reversals from wind-induced
vibrations has often produced failures either or both of
along-wind and cross-wind vibrations involved. Since
an accumulation of fatigue damage over a period of time occurs with a range of wind speeds, the wind
loading component is complex. This was recognized in
some early work by A.G. Davenport [21] in 1966, in
which he derived an expression for the number of
exceedences of defined amplitudes under long-term
wind loading.
On the material side, the parameters relating to
fatigue damage are very uncertain. For these reasons,
the prediction of fatigue life under wind loading has
not been generally adopted by codes; hence, the
phenomenon has probably been largely ignored bydesigners, until a failure has occurred.
A usable method for estimating the fatigue life of
slender structures under along-wind loading is given in
Refs 22 and 23 (also discussed in Ref 13). A ‘closed-
form’ expression for upper and lower bounds of fatigue
life is given. This requires information on the parameters
of the Weibull distribution of 10-minute mean wind
speeds at the site, as well as the constants of the power law expression describing the fatigue s-N curve. The
simplified Palmgren-Miner Hypothesis for
accumulation of fatigue damage is also assumed. So far
this approach has not been adopted by any code or
standard; however, there is a potential for this to be done.
Since the critical velocity for vortex-induced
vibrations of small diameter steel structures is typically
a wind speed with a high probability of occurrence, a
large number of stress cycles may accumulate in a short
period of time. In that case, the simplest design
approach is to ensure that the maximum stress rangedue to cross-wind vibrations remains below the
‘endurance limit’ of steel [24] – thus theoretically
producing no fatigue damage. This may require
increasing the damping or mass of the structure, as
discussed in the previous section.
5. ESDU ENGINEERING DATA
The Wind Engineering series of ESDU data sheets
published by ESDU International of London, U.K.
contain three volumes of data items concerned with
dynamic response to wind. These are very detaileddocuments with comprehensive examples, and
sometimes with accompanying computer programs.
Along-wind response is covered in ESDU 87035
[25] and 88019 [26], for ‘line-like’ and ‘plate-like’
structures respectively. Cross-wind response, due to
both lateral turbulence and vortex shedding, is treated
in ESDU 89049 [27], 90036 [28] and 96030 [29].
Another volume in the ESDU series incorporating
ESDU 83009 [30] and 91001 [31] covers natural
vibration parameters of structures – i.e. damping and
natural frequencies.Although expensive and perhaps over-complex in
some areas, in relation to the uncertainties involved,
the ESDU Data Items are an alternative source of
design methods for dynamic response to wind, but
currently not widely used outside the U.K.
6. INTERNET DATABASES
Another alternative to codes and standards is provided
by internet databases such as the one compiled by the
Natural Hazards Modeling Laboratory of the University
of Notre Dame (www.nd.edu/~nathaz/database). Thelatter provides information on the spectral densities of
Scm .
.b
t
air t
2=
4π . ζ
ρ
y0.5.b
Scmax
t=
International Journal of Space Structures Vol. 24 No. 2 2009 93
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three components of base moment for 27 different
building shapes, in two different terrain types. The nine
cross-sections considered are shown in Figure 4. This
information has been obtained from a high-frequency
base balance, the standard technique for determining
wind loading and response of tall buildings. By the use
of standard random vibration relationships, base
moments and tip accelerations can be determined for
basic building shapes. However, only orthogonal wind
directions are considered, and the effects of surroundingbuildings, and complex coupled mode shapes cannot be
treated. Special wind-tunnel studies are required to
adequately cover the latter.
It is likely that internet databases will be further
developed in the future with more comprehensive data
available to the designer.
7. LIMITATIONS OF CODIFIED
APPROACHES
There are many situations of response to wind that are
beyond the application of conventional codifiedmethods to the dynamic response of structures. Some
of these situations are as follows:
a) When modes higher than the fundamental sway
and twist modes contribute significantly to the
load effects. This would be the case for very large
structures such as tall cantilevered towers and
long span bridges. These may be particularly
important for calculation of deflections and
accelerations. Special wind engineering studies,
usually involving wind-tunnel tests, should
normally be undertaken for such structures.b) Cases when surrounding structures can
significantly modify the approach flow
conditions – particularly the turbulence
characteristics. Wind-tunnel testing is an
effective method of predicting the shielding and
interference effects of surrounding structures.
c) Structures such as stadium roofs – particularly
arched and domed roofs. Although the resonant
dynamic response for such roofs may not be
particularly significant, except for cantilevered
roofs and very long structures, the structuralresponses are sensitive to the variety of load
distributions that fluctuating wind pressures can
impose. In these cases simple load distributions
based on quasi-steady principles are inadequate.
Approaches to the development of wind loading
distributions for long span roofs, based on the
appropriate processing of wind-tunnel test data,
are discussed by Holmes [13].
8. CONCLUSIONS
This paper has considered the codification of dynamicresponse to wind of tall wind-sensitive structures.
Methods of treating both along- and cross-wind
response of tall buildings, and other structures such as
towers and chimneys, are discussed. It has been noted
that current codification approaches cannot easily
account for responses to wind in higher modes and for
structures such as long-span bridges and large stadium
roofs. Development of new approaches for these
structures is a topic for future research.
However, the approach to guyed masts adopted by the
British Standard BS8100 [32], in which numerous ‘patchload’ distributions are specified, is a case where a
successful codified approach to structures with a complex
response to fluctuating wind forces has emerged.
The possible future codification of fatigue
calculations has also been discussed in the present
paper. Alternative sources of information for designers
– namely the ESDU Wind Engineering Data items, and
internet databases are also mentioned briefly.
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94 International Journal of Space Structures Vol. 24 No. 2 2009
Codification of Wind Loads on Wind-sensitive Structures
3:1 2:1 1.5:1 1:1 1:3 1:2 1:1.5 1:1 1:1.5
Figure 4. Cross Sections of Tall Buildings for Which Data is Given in the Internet Database of the University of Notre Dame
(www.nd.edu/~nathaz/database).
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John D. Holmes
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