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Transcript of Wing Bending Calculation with a Single set of Equations Deflection... · Wing Bending Calculation...
Wing Bending Calculation with a Single set of Equations
Author : Steven De Lannoy
January 2014
This document and more information can be found on the website Wingbike - a Human Powered Hydrofoil.
Abstract Wing bending calculations are complicated,
especially for hollow tapered wings. If one pursues
an exact solution, the math involved is challenging. If
one uses a numerical integration, one has to perform
a series of calculations along the span of the wing to
finally end with the tip deflection. For preliminary
designs, this is too cumbersome.
This paper builds on a paper of MIT’s
OpenCourseWare as presented by Drela [1] and
presents an improved approximation to calculate
wing tip deflection. It is very well suited for
preliminary designs of wings:
With 3 different equations to calculate Iroot:
• Solid wings
• Hollow wings (non uniform skin)
€
Iroot = Isolid 1− (1− 2Ω)3{ }
• Hollow wings (uniform skin)
€
Iroot = Isolid 1− (1−2Ωλ5)3
Some examples and a quick reference guide can
be found in the back of this paper.
1 Introduction A rectangular wing can be represented by the
following model of a beam:
Fig. 1
One end of the wing is fixed (at the root). The other
end, the tip, is free to move. The lift force generated
by the wing is proportional to the area of the wing. In
this case, since the wing has a rectangular shape,
lift is evenly distributed.
The equations to calculate bending moment, shear
force and wing deflection can be found in most
engineering handbooks as this model is a classic
engineering application of a beam. In this situation, a
rectangular wing can be regarded as a very flat
beam.
When the wing is tapered, the model changes as the
area of the wing decreases towards the tip. The
lifting force follows proportionally. Even this situation
is described in many engineering books and many
standard equations are available.
Fig. 2
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However, the main difference now between the
situation in the engineering handbook and a wing is
that the first assumes a beam of constant width and
thickness whereas a tapered wing gradually
decreases in chord and thickness. So the general
engineering equations are no longer valid.
Since the wing doesn’t have a constant width and
height (chord and thickness) the bending inertia (=
resistance to bending) is no longer constant along
the span of the wing (as opposed to the engineering
situation). So not only does the lift varies along the
span, but so does the wing’s resistance to bending
as well.
The exact calculation of wing deflection involves
integrating a series of equations (Bernoulli-Euler
beam model). These steps and equations are
described by Drela [1]. Since the last two integration
steps in the procedure are complex, the author of the
document presents a numerical scheme and an
approximation. They form the basis of this paper.
In his paper, Drela [1] has derived an approximation
for the calculations of wing deflection:
€
δ =WL
12EIroot1+ 2λ1+ λ
y 2 (1)
Where
δ =deflection [m]
W = total weight [N]
L = ½ span [m]
E = Young’s Modulus [N/m2]
Iroot = bending inertia root [m4]
λ = taper ratio [-]
y= co-ordinate along span [m]
Iroot is the bending inertia at the root of the wing and
consists of an equation by itself. It depends on the
chord and thickness of the wing.
For a solid wing it is:
€
Iroot = 0,0449CT 3 (2)
Where
C = chord [m]
T = thickness [m]
This equation1 is a simplification by representing
the cross-section of the wing by a corrected
rectangular box [2,3].
Equation 1 is based on the assumption that the
wing curvature along the span of the wing is
constant (which is not the case). Therefore, it is
only accurate in certain conditions.
As described previously, the bending inertia along
the span of a tapered wing decreases, but in the
equation above, for simplification reasons, only the
bending inertia at the root is taken. Drela has
pointed out that this approximation is only accurate
for highly tapered wings. Below is a graph that
compares equation 1 with the numerical solution of
a typical hydrofoil case (for λ=0,3).
Fig. 3
The match along the span of the wing is very good
for λ=0,3.
The correlation becomes less accurate for higher
taper ratio, like in the figure below where the
equation shows a discrepancy towards the tip of
approximately 200% (for λ=1).
1The factor 0,0449 is the value for a ClarkY wing. For other shapes, see [2,3]
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Fig. 4
In the next sections we will present a modified
(improved) version of equation 1 so that tip
deflection matches better along the entire range of
taper ratios (from 0,1 to 1).
Equation 1 can be used for solid wings and some
types of hollow wings provided the correct Iroot is
used. Before we can proceed and derive an
improved equation we need to explain skin
distribution first as it influences the bending inertia
along the span of the wing.
2 Skin distribution When using a single equation to calculate wing
bending, one has to pay extra attention to the skin
distribution along the span of the wing. The
thickness has a large influence on the total bending
inertia of the wing.
Equation 1 calculates wing bending by using the
bending inertia of the root. It does not account for
how the skin is distributed along the span of the
wing.
Two types of skin distribution can be distinguished
for tapered hollow wings: uniform skin or non-
uniform skin.
The first means that the skin thickness is constant
along the span of the wing. The latter means that
the skin thickness decreases towards the tip of the
wing, proportional to the dimension of the chord
and thickness of the wing. It is illustrated in the
figure below.
Non-uniform skin (skin = 0,4 mm)
Uniform skin (skin = 1 mm)
Fig. 5
Three hollow cross-sections are presented. The
largest one, represents the cross-section at the
root of a wing and has a skin thickness of 1mm.
The two smaller cross-sections represent the tip of
the wing (for λ=0,4). One for non-uniform skin
distribution, one for uniform skin distribution.
The non-uniform skin is scaled proportional to the
chord and decreases to 0,4mm. The uniform skin is
constant and remains 1 mm.
It’s not hard to conclude that a uniform skin
distribution will lead to less tip deflection as the skin
is relatively thick towards the tip of the wing (higher
bending inertia).
When using equation 1 to calculate tip deflection it
does not account for this skin distribution and the
bending inertia as the root of the wing is identical in
both cases.
Let’s use an example to illustrate this, but first the
equations of bending inertia are presented. How
these equations were derived can be found in [2,3].
Bending inertia for a hollow wing (non-uniform
skin)2:
€
I = 0,0449C T 3 −T 3(1− 2Ω)3{ } (3)
Where
C = chord [m]
T = thickness [m]
Ω = skin fraction [-]
2 The factor 0,0449 is the value for a ClarkY wing. For other shapes, see [2,3]
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Skin fraction (Ω) is a value between 0 and 1 and
relates the skin to the thickness of the wing.
(4)
So if along the span, T decreases (for a tapered
wing), so will the skin thickness.
The equation for bending inertia for uniform skin
distribution is:
€
I = 0,0449C T 3 − (T − 2Sk)3{ } (5)
Where Sk is the actual skin thickness (and
constant along the span).
We will illustrate the differences with an example:
Chord 150 mm Thickness 20 mm Skin 2 mm Ω 0,1
Chord Wing
Thickn. Uniform Non-
uniform 150 20,0 22.487 22.487 130 17,3 14.164 12.686 110 14,7 8.200 6.503 90 12,0 4.202 2.914 70 9,3 1.778 1.066 50 6,7 532 278
The bending inertia at the root is identical (22.487
mm4) as the skin is equal in both cases. Towards
the tip of the wing, values diverge (almost a factor
2).
We can illustrate that the calculation of the bending
inertia of a solid wing (equation 2) is very similar to
the calculation of the bending inertia of a hollow
wing with non-uniform skin distribution.
We simplify equation 3 by isolating T:
€
I = 0,0449CT 3 1− (1− 2Ω)3{ }
This equals
€
I = Isolid 1− (1− 2Ω)3{ } (6)
So to obtain the bending inertia of a hollow wing
(non-uniform skin) one can take the bending of the
solid wing multiplied by a constant.
In the next sections we will show that equation 1
can be improved for
• Solid wings
• Hollow (non-uniform) wings
• Hollow (uniform) wings
provided that the bending inertia at the root is
corrected accordingly in some cases.
3 Solid and hollow wings (non-uniform)
Finally, before we can derive the improved
equation, we need to discuss the Bernoulli-Euler
beam model in very general terms first as it forms
the basis of the calculations and justifies the
approximations.
3.1 The theory behind the assumptions. To calculate wing bending, one uses 4 differential
equations that have to be solved in 4 subsequent
steps:
Step1: (7)
Step 2: (8)
Step 3: (9)
Step 4: (10)
Step 1 involves integrating q (function of wing
loading) along the span of the wing (dy). This yields
the distribution of the shear force (S) along the
span. Integrating this (step 2) yields the bending
moment along the span M. Step 3 involves
integrating the quotient of M, E (Young’s modulus)
and I (bending inertia) to obtain the deflection angle
(θ) along the span. Finally, the deflection (ω) is
obtained in step 4 by integrating the deflection
angle equation.
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The integration of step 3 is especially difficult as M
and I are by themselves fairly complicated
equations and both dependant of y. The math to
solve this analytically is very challenging. Therefore
a numerical scheme was presented [1] and an
approximation that leads to equation 1 of this
paper.
The quotient of M, E, I in step 3 is called the beam
curvature and it depends on y.
(11)
See figure 6 below for a typical case.
Fig. 6
The wing curvature changes along the span and is
different for different λ. Figure 6 is only presented
for λ=0,3, λ=0,5 and λ=1,0.
The assumption that leads to equation 1 is that the
wing curvature is constant along the span and that
it equals the value at the root (dotted lines).
(12)
Now one can see why equation 1 provides a
relative good match for λ=0,3 (fig. 3) compared to
λ=1,0 (fig. 4). The line is nearer most of the time.
The assumption that the wing curvature is constant
(and equals the value at the root) is more or less
arbitrarily chosen to simplify the last integrations.
One is free to choose other values to obtain a
better match just as long as they are
mathematically correct.
Based on figure 6, it seems logical to correct
equation 1 for different taper ratios although
equation 1 is already dependent on λ (through M
and I). This correction is the basis of the improved
equation that will be presented in the next section
(3.2), but to demonstrate the validity of this choice,
first a final remark on the wing curvature graphs.
Figure 6 was calculated for a typical case of a
human powered hydrofoil. If one normalizes the
wing curvature for the normalized span, one
obtains the following graph.
Fig. 7
This graph is now independent of W, L, E, I, C, T
and Ω. It is valid for solid wings AND hollow wings
(only for non-uniform skin).
This observation is certainly not the case for
uniform skin distribution as will be showed in
section 4.
3.2 Improved equation When improving equation 1, we will focus on
matching the tip deflection. In doing so, we might
lose some accuracy along the span. Since we are
mainly interested in tip deflection, that is
acceptable for now.
We have taken the same values that were used in
fig. 3 and fig. 4. We have set y=L in equation 1
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and kept all other factors constant. Now varying λ
through the entire range (from λ=0,1 to λ=1) has
resulted in a range of tip deflections. Then we have
calculated the same range using the numerical
scheme.
We have normalized the outcome: dividing the
numerical tip deflection by itself and dividing the
outcome of equation 1 (&2) by the outcome of the
numerical method. In this way, the relative
deflection is obtained. Now the result is case
independent as well (meaning independent of W, L,
E, Iroot). The result can be seen in the figure 8.
Fig. 8
Now we have another way to demonstrate that tip
deflection is indeed very accurately calculated for
λ=0,3 and very poorly for λ=1 (up to 200% over-
estimation). At λ=0,1, the equation even under-
predicts the tip deflection by 30%.
As equation 1 is based on an assumption
previously described, it is by no means an exact
solution. This justifies applying an additional
mathematical correction to improve its accuracy.
From fig. 8, one can estimate that the correction to
improve equation 1, has to be dependent on λ as
with increasing λ, the correction needs to be larger.
In appendix 1, a detailed description on how we
have matched the data is presented. For now, we
will describe the method in general terms.
Since equation 1 results in a straight line in the
relative deflection graph (fig. 8) we have used a
curve fitting technique to fit a straight line through
it. From this, we have derived the required
correction factor so that the sloped line (equation
1&2) will match the flat line (numerical solution) .
Since the curve fitting technique is a statistical
technique, it results in a correction factor with
decimal factors that complicate equation 1. We
have looked at multiples of these factors to see if
we could find a correction factor with (near) integer
number (see appendix 1). This has resulted in the
following correction factor:
(13)
Multiplying with equation 1 results into:
(14)
With for bending inertia at the root (solid wing):
(15)
And for a hollow wing (non-uniform skin):
€
I = 0,0449C T 3 −T 3(1− 2Ω)3{ }
€
= Isolid 1− (1− 2Ω)3{ } (16)
Or simplified into a practical equation:
€
δ =2WLEIroot
Ay 2 (17)
λ A 0,1 0,0661 0,2 0,0583 0,3 0,0524 0,4 0,0476 0,5 0,0437 0,6 0,0404 0,7 0,0376 0,8 0,0352 0,9 0,0331 1 0,0313
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With this new equation (14&2), we have again
calculated the normalized deflection curves,
leading to the following figure:
Fig. 9
The correlation has become near perfect.
Since we have focused on a way to match the tip
deflection, let’s check if this correction has had a
negative effect on the deflection along the span of
the wing.
Fig. 10
Both equation 1 and 14 provide a good match for
λ=0,3. So the correction factor hasn’t changed the
original correlation.
For λ=1 (figure 11), there is a slight mismatch
between the numerical calculations and the result
of equation 14. It seems that halfway the wing,
equation 14 (&2) under-predicts the wing
deflection.
Fig. 11
One could apply an additional correction to
equation 14, but this would complicate this
equation since y has now to be matched. Since
prediction of the tip deflection is more important
than the deflection distribution along the span of
the wing, we will not go further into this.
The correction factor we have applied to convert
equation 1 to equation 14, can be illustrated with
the wing curvature graph we used earlier.
Fig. 12
Equation 1 used the values at the root of the wing
(figure 6). For equation 14, these values were
corrected in such a way that the tip deflection
provided a better match. Compare figure 6 with
figure 12 to see the difference.
We have stated earlier that the normalized wing
curvature graph is equal for solid wings and hollow
wings (figure 7). Therefore equation 14 would be
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valid for hollow wings as well (non-uniform skin).
The reason is that the equation to calculate the
bending inertia of a solid wing, only differs from the
equation to calculate the bending inertia of a hollow
wing by a factor (see equation 6).
To illustrate the validity, we have performed a new
set of tip calculations (numerically and with
equations 1&3 and 14&3 respectively for a hollow
wing). The result can be found in the figure below.
Fig. 13
The line that is determined by equation 1&3 is
identical to the line that was determined by
equation 1&2 in figure 8. Hence, the same
correction factor is valid. In appendix 1, we have
used a curve fitting technique to prove this.
4 Hollow wing (uniform skin) In the previous section, we could simply convert
equation 1 into equation 14 by correcting for λ. The
basis for this was that the normalized wing
curvature graph was independent for all cases
(independent of W, E, L, I, C, T). We used,
depending on the situation, equation 2 (solid) or
equation 3 (hollow) to calculate the required
bending inertia at the root of the wing.
It is logical to use equation 14 in combination with
equation 5 to calculate tip deflection for the uniform
skin scenario.
However, this will not lead to correct values. For
uniform skin distribution, the normalized wing
curvature is not only dependent on λ, but on Sk as
well. This can be seen in the figure below.
Fig. 14
We have taken the wing curvature line from figure
6 (solid wing and λ=0,3). We have then expanded
the graph for three different hollow wings (uniform
skin thickness 1, 2 and 3mm). The normalized
graph is clearly dependent on Sk as well. The
combination of equation 14 with equation 5 is
clearly not universal.
Below we have illustrated this with a deflection
curve for λ=0,3 (using equation 14&5).
Fig. 15
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For λ=1 (below) the match at the tip is perfect,
along the span there is a discrepancy.
Fig. 16
To illustrate the discrepancies, again, we have
performed a range of calculations for a hollow wing
in for the range λ=0,1 to λ=1,0. Then we have
normalized the outcome.
Fig. 17
Equation 1 (in combination with equation 5)
provides an even worse match than previously.
Equation 14 in combination with equation 5
provides at least a better match. Especially for
values close to λ=1. The reason why the match
improves towards higher taper values is that at
λ=1, there is no difference between a wing with
uniform or non-uniform skin. Since the chord does
not decreases toward the tip, the skin remains
constant (equation 3 and equation 5 are equal
now). This is why figure 16 showed a good match
as it is not different from the solution using
equation 14 and 3.
Note that the discrepancy between the numerical
solution and equation 14&5 is no longer linear.
To rewrite equation 14 in combination with
equation 5 to represent uniform skin distribution,
one would have to dive deep into the Bernoulli-
Euler equations. This would make the math even
more challenging. It is more convenient to rewrite
equation 5 so that it can be used in combination
with 14. Even if it means applying a mathematical
trick.
A wing with a uniform skin is stiffer compared to the
same wing with non-uniform skin as the skin is
relatively thicker towards the tip of the wing.
For a wing with non-uniform skin to have the same
tip deflection as a wing with uniform skin, it would
require a thicker skin at the root to begin with
(provided all other factors are equal).
We could choose this thickness, which is not the
real thickness, in such a way that the tip deflection
matches the tip deflection of the same wing with
uniform skin.
We know that the bending inertia for hollow wing
(non-uniform skin) is:
€
Iroot = Isolid 1− (1− 2Ω)3{ } (18)
Now we will correct (increase) Ω with factor K in
such a way that the tip deflection corresponds with
the uniform skin thickness case.
€
Iroot = Isolid 1− (1− 2KΩ)3{ } (19)
So, by starting with a higher value of Ω, the skin at
the root is thicker and we will end with the same tip
deflection as it were a uniform skin. In this way
equation 14 can still be used. This again is a
mathematical trick rather than based on exact
physics as it will under predict the deflection closer
to the root of the wing.
There are two reasons why this is acceptable.
Firstly, as stated earlier, our main focus is to
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predict tip deflection. Secondly, the assumption
that lead to equation 1 was in fact comparable:
a mathematical trick applied to the root of the
wing.
We have performed a large set of numerical
simulations (varying W, L, E, C, T, λ, Sk and Ω) in
which we matched the tip deflection of the two
methods.
We have found that K is only dependant on λ (see
figure below)
Fig. 18
Figure 18 shows how much the skin fraction (Ω) of
a hollow wing (non-uniform skin) much be
increased to match the tip deflection of the same
wing with uniform skin distribution (all other factors
equal).
The slope (=K) is constant for each specific taper
ratio. Plotting this slope versus taper ratio results in
figure 19.
Fig. 19
We have found that K depends on λ in the
following way (correlation R2=0,999):
€
K =1λ5
(20)
Now the bending inertia equation for uniform skin
is:
€
Iroot = Isolid 1− (1−2Ωλ5)3
(21)
Or simplified:
€
Iroot = Isolid 1− (1− 2KΩ)3{ } (22)
λ K 0,1 1,585 0,2 1,380 0,3 1,272 0,4 1,201 0,5 1,149 0,6 1,108 0,7 1,074 0,8 1,046 0,9 1,021 1 1,000
We have re-calculated the example from above
(figure 15) but instead of using the combination of
equations 14 and 5, we have used the combination
of equations 14 and 21.
Fig. 20
The conclusions are similar to the previous
conclusions: a perfect match at the tip of the wing
in combination with under prediction of the
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deflection along the span. This is logical as the
wing has been artificially made stiffer near the root.
To check the entire range, we have again
performed normalized tip deflection calculations
from λ=0,1 to λ=1,0.
Fig. 21
There is still a small discrepancy for λ=0,1, but
very acceptable.
5 Examples We will illustrate all the equations we have derived
by an example. We have chosen a fairly large span
and weight so that differences are clear.
Span 2,5 [m] Weight 1200 [N] Chord root 0,15 [m] Taper 0,3 [-] th/c 13,33% [-] Youngs Mod 2,0E+11 [N/m2] Skin 0,0015 [m]
Calculate Ω = 0,0015 / 0,02 = 0,075
We will consider 3 scenarios:
• Solid wing
• Hollow wing (non-uniform skin)
• Hollow wing (uniform skin)
We will compare the equations with the numerical
scheme we have composed earlier and we will
discuss the results.
Solid wing
First calculate the bending inertia at the root of the
wing using equation 2:
Now wing bending is calculated with equation 14:
€
δ =2WLEIroot
1+ 2λ(1+ λ)(13+ 35λ)
y 2
€
=2(1200)(1,25)
(2,0∗1011)(5,4 ∗10−8)0,0524{ }y 2 = 0,0146y 2
We have divided the span into 5 sections and
calculated the wing deflection and compared it with
the outcome of the numerical scheme:
y num eq14&2 0,00 0,000 0,000 0,25 0,091 0,091 0,50 0,373 0,365 1,00 1,508 1,458 1,25 2,281 2,278
The deflection at the tip is: 2,3 cm.
Fig. 22
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As stated before, the corrections we have applied,
focus on matching the tip deflections and accepting
a deviation in wing deflection at other stations
along the wing span. However, if we calculate the
correlation, the series yield R2=0,9998
Hollow wing (non-uniform skin)
First calculate the bending inertia at the root of the
wing using equation 3:
€
Iroot = Isolid 1− (1− 2Ω)3{ }
€
= (5,4 ∗10−8)(0,3859) = 2,1∗10−8
Then calculate the deflection with equation 14:
€
δ =2WLEIroot
1+ 2λ(1+ λ)(13+ 35λ)
y 2
€
=2(1200)(1,25)
(2,0∗1011)(2,1∗10−8)0,0524{ }y 2 = 0,0378y 2
Again, for 5 sections we have calculated the wing
deflection and compared it with the outcome of the
numerical scheme:
Y num eq14&3 0,00 0,000 0,000 0,25 0,237 0,236 0,50 0,966 0,945 1,00 3,907 3,779 1,25 5,910 5,904
The deflection at the tip is 5,9 cm.
The correlation between both series is R2=0,9998
Fig. 23
Hollow wing (uniform skin)
First calculate the bending inertia at the root of the
wing using equation 21:
€
Iroot = Isolid 1− (1−2Ωλ5)3
€
= (5,4 ∗10−8) 1− (1− 2(0,075)0,35
)3
= (5,4 ∗10−8)(0,470)
Then calculate the deflection using equation 14:
€
=2(1200)(1,25)
(2,0∗1011)(2,5∗10−8)0,0524{ }y 2 = 0,0310y 2
Again, for 5 sections we have calculated the wing
deflection and compared it with the outcome of the
numerical scheme:
y num eq14 &5 eq14&21 0,00 0,000 0,000 0,000 0,25 0,227 0,236 0,194 0,50 0,888 0,945 0,775 1,00 3,294 3,779 3,101 1,25 4,817 5,904 4,845
The deflection at the tip is: 4,8 cm.
The correlation between both series is R2=0,9998
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Fig. 24
Finally we have combined the wing deflection
graphs for the 3 cases to illustrate the effect:
Fig. 25
Conclusion For preliminary design purposes, the single
equations to calculate tip deflection are surprisingly
accurate. One has to pay attention to the type of
skin distribution.
Deflection calculations can never be made without
checking the shear force and stress in the wing.
IMPORTANT NOTE
It should be emphasized that when performing deflection calculations one should always
simultaneously calculate the shear force (at
least at the root of the wing) and stress as the
wing might fail before the calculated deflection is reached !!!!
References [1] Drela, M, “Wing Bending Calculations”.
MIT OpenCourseWare, Unified
Engineering Course Notes, MIT
Department of Aeronautics and
Astronautics,
http://ocw.mit.edu/courses/aeronautics-
and-astronautics/16-01-unified-
engineering-i-ii-iii-iv-fall-2005-spring-
2006/systems-labs-06/spl10.pdf
[2] Lannoy, De, S., “Section Modulus and
Wing Bending Inertia of Wings”. Website:
Wingbike - a Human Powered Hydrofoil
[3] Lannoy, De, S., “Method to determine
correction factors for Section Modulus and
Bending Inertia Equations of wings.
Website: Wingbike - a Human Powered
Hydrofoil
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Appendix 1 Solid tapered wing and hollow wing with non-uniform skin distribution.
A set of wing tip deflection calculations was performed using the numerical scheme explained in [1]. The
range was set from λ=0,1 to λ=1. This outcome was then normalized to itself, meaning that the outcome (tip
deflection) was simply divided by itself. This results in a flat line. Next equations 1 and 2 were used to
calculate the tip deflection for the same interval by setting y=L in the equation. The outcome of this
calculation was then normalized to the outcome of the numerical scheme (divided by the outcome of the
numerical scheme). This results in the following table and figure:
taper num eq1&2
0,1 100% 68% 0,2 100% 83% 0,3 100% 98%
0,4 100% 112%
0,5 100% 127%
0,6 100% 142% 0,7 100% 156%
0,8 100% 171%
0,9 100% 185%
1 100% 200%
Normalizing the outcome of both methods is a way to present relative differences between the two methods
and is an indication on how well both cases match. One can see that both lines intersect at λ=0,3, meaning
that the calculated wing tip deflection is identical for λ=0,3 for both methods. As described in the
introduction, the match becomes worse with increasing λ . Equation 1 under-predicts the tip deflection for
λ<0,3.
Since normalizing presents relative differences, the discrepancy between the normalized numerical
calculation and the normalized approximation of equation 1 is independent of W, L, E, and I.
Using a linear curve fitting technique, one can obtain an accurate fit (R2 = 1) of the normalized line of
equation 1.
The correction factor to match equation 1 to the numerical scheme now is:
Multiplying equation 1 with this factor, will result in a match between the two methods, but this will result in a
new equation with “odd” looking decimal factors. It’s better to try and find a more elegant factor by
multiplying the numerator and the denominator of the correction factor by the same number:
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Linear = 1,4649 λ+ 0,5368 Numerator Denominator
1 1,465 λ+ 0,54 13 19,044 λ+ 6,98 2 2,930 λ+ 1,07 14 20,509 λ+ 7,52 3 4,395 λ+ 1,61 15 21,974 λ+ 8,05 4 5,860 λ+ 2,15 16 23,438 λ+ 8,59 5 7,325 λ+ 2,68 17 24,903 λ+ 9,13 6 8,789 λ+ 3,22 18 26,368 λ+ 9,66 7 10,254 λ+ 3,76 19 27,833 λ+ 10,20 8 11,719 λ+ 4,29 20 29,298 λ+ 10,74 9 13,184 λ+ 4,83 21 30,763 λ+ 11,27
10 14,649 λ+ 5,37 22 32,228 λ+ 11,81 11 16,114 λ+ 5,90 23 33,693 λ+ 12,35 12 17,579 λ+ 6,44 24 35,158 λ+ 12,88
There are several options that yield values close to an integer number: 11, 13, 15, 17, 24. Since equation 1
has a factor 12 in the denominator, it’s best to choose a combination that will simplify the new equation. The
following correction factor meets these criteria:
Now the new equation 1 becomes:
€
δ =2WLEIroot
1+ 2λ(1+ λ)(13+ 35λ)
y 2
Performing the simulation again and comparing it with equation 14, yields the following values:
taper num eq1&2 Eq14&2
0,1 100% 68% 99% 0,2 100% 83% 100% 0,3 100% 98% 100%
0,4 100% 112% 100%
0,5 100% 127% 100%
0,6 100% 142% 100% 0,7 100% 156% 100%
0,8 100% 171% 100%
0,9 100% 185% 100%
1 100% 200% 100%
With the new equation 14, a near perfect match is obtained over the entire range.
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We have stated earlier that the normalized wing curvature graph is equal for solid wings and hollow wings
(non-uniform). Therefore equation 14 would be valid for hollow wings as well. To illustrate this, we have
performed a new set of tip calculations (numerically and with equations. The results can be found in the
figure below.
Equation 14 (in combination with equation 3) gives the same match over the entire range.
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Appendix 2 Quick Reference Guide
Decide on type of cross-section
Hollow Solid Non-uniform skin distribution Uniform skin distribution
€
Iroot = 0,0449CT 3
€
Iroot = Isolid 1− (1− 2Ω)3{ }
€
Iroot = Isolid 1− (1−2Ωλ5)3
or simplified
€
Iroot = Isolid 1− (1− 2KΩ)3{ }
€
δ =2WLEIroot
1+ 2λ(1+ λ)(13+ 35λ)
y 2
or simplified
€
δ =2WLEIroot
Ay 2
λ A K 0,1 0,0661 1,585 0,2 0,0583 1,380 0,3 0,0524 1,272 0,4 0,0476 1,201 0,5 0,0437 1,149 0,6 0,0404 1,108 0,7 0,0376 1,074 0,8 0,0352 1,046 0,9 0,0331 1,021 1 0,0313 1,000