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If ~ .l~ I ratioq, It. . - j ~ ~ S~1 I
*(~lATSI to j N --.. on s .emj I* I Ns t
T, chnion Resiearch and Dev2oprment z' --- 1 1,% itGA;I1n
haifa, Israel
3 flEPO'T TITLE
-)N 'Mr BucLfl:B ANID PSIBUCYLIM, OF rCW-M2 AltCi t; uiD) HR1'.
4OE$CRhPTIVE NOTES (7YP* oftor.5ot and 2flcfusve dtoo)
S AUTH4OR(S) fMagt n"me. Ila t ntme. IisfiaIl)
Dyrn L. Clive
6 EPORT OATE 7. TOT&~N a- 0A4 ' 17b to OF PrV,
Ang~ust 1971 V"i 15
8A COVJTRACT OR GRANT NO0 90 orIGINA M0.3 n!:aopy "Sim"E's)
F 61052-69-0-0040h PPOJCCT N~O TAB iep:rt No. 133
C 5b 0114CR r P OWC~I ,,1 o1h,rnuent- a IhL# r',.v b. meqiadChia report)
10 A VA IL AIILITY 'LIITAT1ON1 NOTIC.ES
T',hi! liocument has been approved for puh.Lsh releaso nr vaciu;
: .tribution is unlimited,
II ~1P -,%Fk~y NoTes 12 5P04S~jRlNG MWtTAieP-.IV1TY
___________ jAir Farce Of'f -'.ce 3ciei t 1fic hisuearcL.
________ 1400. *Wiionl1: 1aa2220)Ilk ABSTRACT
This paper treats the buckling and postbuckling oehavit,- or circulararches and rings under conztant directional pressure. Nlew erict andAn rxmte solations are iven for the linearized ei~renval' e 1lrlem.
Apymptoti - ana'yses of erry rnatbuCkline, t'iuior :-!rr, : >--* thetheory of Koiter and the foralism of Budienckg ai:4 :!utch-L.'on- j 3t-buckling behavior is shown to te stable, and unf I-ec d by, Ly -.:onor inextensibility.
CD RI 147"
Security Classification _______ ______ ______
14 LINK A LINK 0 LINK CKYWRSROLE WT ROLE ITW ROLE WT
1. Buckling and Postbuckling.
2. Circular Arahes and Ringt.
3. Imperfection sensitivity.
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SecuritV Classification
F61052-69-C-0040
SR 5 AUGUST 1971
SCIENTIFIC I ,LPORr No. S.
ON THE BUCKLING AND POSTBUCKLING OF CIRCULAR ARCHES
AND RINGS.
by
CLIVE L. DYMDepartment of Aeronautical Engineering
Technion- Israel Institute of Technology,Kaifa, Israel.
T.A.E. REPORT No.133
DDC
IV6_ ..-- |
C
This document has been approved for public release and sale, its distributionis unlimited.
The researth reported in this document has been sponsored in part by the AirForce Office of Scientific Research, through the European office of AerospaceResearch, United States Air Force, under Contract F61052-69-C-0040.
* On leave from Carnegie-.1ellon University, Pittsburgh, ra., U.S.A.
_, a %'ir lidm ],
" " ""'" ':r ,, " >-,., - ,. - , -, -- " L.
TABLE OF CONTENTS
PAGE NO.
ABSTRACT I
NOMENCLATURE II - IiI
1. Introduction 1 - 2
2. General Equations 3 - 5
3. Linearized (Buckling)Solutions 6- 9
4. Postbuckling: The Budiansky-Hutchinson Approach 10 - 16
5. Postbuckling: Kolter's Approach - 23
6. ODiscssinTadcncuin 24 6
REFEPENCES 27 - 28
TABLE 1 28
FIGURE 1
I , -
ABSTRACT
This paper treats the buckling and postbuckling behavior of circular
arches and rings under constant directional pressure. New exact and
approximate solutions are given for the linearized eigenvalue problem.
IL is clearly demonstrated that the assumption of inextensibility is
quite reasonable for the asymmetric buckling of steeper arches and of
rings. Asymptotic aaalyses of early postbuckling behavior are given,
based on the theory of Koiter and the formalism of Budiansky and
Hutchinson. The postbuckling behavior is shown to be stable, and un-
affected by the assumption of :.nextensibility.
I'
- II -
I"
NOMENCLATURE
a, b, a', b' perturbation solution parameters defined by Eqs. (40) and
(37)
A, Ai displacement coefficientr, dimensionless
A displacement coefficient, dimensional*
A displacement coefficient (=
e, ai extensional strain
E Young's modulus
h arch thickness
H thickness parameter
moment of inertia
K, K curvature, dimensionlessI
L i differential operators
M, 14 imoment rosulta,.1, dimensionless
N, 1. stress resultant, dimensionless
F, P potential energy functionalsm
q load per unit length of arch
Q extensibility parameter defined by Eq. (16)
R arch radius
Si nonlinear extensional strain
v, V i tangential displacement, dimensionless
w, w tangential displacement, dice-nsionless
I'
•- -- .
half anigle of arch vertex
6 first order variationk
C porturbiitiOfl paramfeter
arch coordinate
arch l0ading,dimensionions
Xr Xc rotation of norm~al to arch centerlinles? dimensionless
-- 1
1. INTRODUCTION
This paper treats the buckling and the postbuckling behavior of
pinned arches, under constant directional ('d. ad") pressure, where the
arch radius of curvature is a constant. A linearized treatment of this
problem has been given by Chwalla and Kollbrunner [1]*, who assumed that
the arch was inextensible during buckling. Kaxmel [2] has shown that
extensibility did not have a great effect on the buckling loads, a result
confirmed by the present study. Also, Levy [3] and Carrier (4] have
given "closed form" solutions for the postbuckling of inextensional
circular rings in terms of (implicit) elliptical integrals. It is also
worth noting the recent contribution of Singer and BBc_ , w 0
discuss the relationship of semi-circular arches under dead pressure to
tbat of completn rings, pointing c'it the need to account for rigid body
displacements.
The present work treats the linearized buckling problem both exactly,
within the framework of ring theory, accounting for extensibility, and
anproxiataty: nxtndina Trv'l approximation for iings to arches of varios
vertex angles. A qualitative me.asure of the midplane extension is also
provided from the new exact solution.
Two asymptotic analyses of the early postbuckling behavior are presented,
both based on the theory advanced by Koiter (6]. The first makes use of the
formalism expounded by Budiansky and Hutchinson [7,8,9], and is carried
N I:umbers in brackets refer to entries in the list of References.
- . . --
I
22
out to include terms in the displacement expansion of order e , where c
is the small buckling deflection parameter. It is shown that the post-
buckling behavior of the arch following asymmetric buckling is stable,
and it is not appreciately effected, qualitatively or quantitatively, by
the inextensibility assumption. Further, it is shown that the inclusion
of the second order terms in the displacements has no appreciable effect
on the quantitative outcome.
Finally an anlysis based directly on Koiter's approach is presented,
2also accurate in the displacement expansion to order £ 2D. he- reits are
identical, for ihi pv o d using the Budiansky-
Hutchinson formalism, and serve to confirm the idea that (at least for
*simple" problems) accurate quantitative information can be obtained r-sing
only the buckling mode shapes in the postbuckling analysis. Koiter has
previously considered the elastica [6, and a two-bar frame [101 using only
the buckling mode, while Haftka and Nachbar [li] have conpared results of
a "one-term" solution with an exact solution, and .te comparison was quite
good.
is
-3-
2. GENERAL EQUATIONS
The equations used to describe the arch behavior are those of ring
theory, which are also a one-dimensional subset of the nonlinear shell
equations of Sander 1 " sonle3s form thEy aprear as follows.
e stress and moment resultants are
1 2
M=- f (lb)dO
where e Lnd X are the linear in-plane strain and the rotation,
respectively, which when expressed in terms of a tangential displacement
v and a radial displacement w take the form
dv dwe = - w, = + V (2)
The displacements and the circumferential ixch coordinate have been
nondimensionalized with respect to the arch radius R, while the stress
and moment resultants have been rendereI dimensionless by dividing by
(EI/R2) and (EI/R), respectively. This results in the thickness ratio
being introduced in equation (la), i.e.,
H = 1 (h)2 (3)12 R
Further, a dimensionless applied loading X wili. be defined as
3A = ,-4)El
where q is the load (uniform here) per unit length of arch. The geometry
-4- t
is picttired in Figure 1.
Now the (dimensionless) total potential e.aergy of the transversely
1o~ipa ewritten down as
P = 2R (U+V)El
(e2+2dO + f () do- 2A wdo (5)
-C H d -CL
In eiuation (5) the first integral represents the (linear and nonlinear)
utrain ener v - dle surface extension, the second integral is the
bending contribution to the energy, while the £inr l term is the potential
of the applied load.
From equation (5) one can deduce the potential energy corresponding
to the linearized buckling problem (See Eqns. (47)of Section 5), deroted
here as P X
X 1 a 2 a dx1 2 a 2P 2 =- e.d + - f -) d - X f Xd.6)
-i -CL -CL
The subscript one will, throughout this paper, denote a buckling dis-
placement or stress quantity. The Eular-Lagrange equations of the quadratic
functional (6) are straightforwardly obtained as
LIwI + L2v I - 0 (7a)
L3w1 + L 1v - 0 (7b)
where the Li are the differential operators
- U
--
d3 d
de2
L w ( + H) - + XH (8)2 d2
d4 d 23 4 a2
it is immediately of intereat to novs that equations (7) car be uncou;pled
to yield a single equation in v. , or the identical equation in w1 alone.
Fuithermore, that-single equation is identically that given by Chwalla and
Kollbrunnor[11, which they derived by assuming inextensibility in the buckling
state, i.e., eI - 0. That equation is, obtained here with no assumption
regarding the extensibility;
(LL - L 2 VI Vli + (2 + X)vI U + ' (9)
3 2-L 13 1 12 1+~ 1 -
The prime superscripts in equation (9) correspond to d6fferentiation with
respect to ti.e arch coord!iate. The question of inextensibility will be
raised again in the seuel.
For completeness the natural (in terms of stress resultants) and geo-
metric boundary conditions for the linearized prozlem are also noted
Either N1 - = 0 or vI is pre.-cribed
da1Either Ti- - kxl = 0 or wI is prescribed (IC)
~dw 1
Either M 0 or d- is prescribed
The boundary conditions are applied at t a, where 2a is the
arch vertex angle (Figure 1). Results for the complete ring are ol taxn-
ed by setting a = 15].2
f -6-
3. LIEARIZED (BUCKLlIG) SOLUTIOUS
A solution to t.c eigenvalue problem represented by the differential
equation (9) has been given by Chwalla and Kollbrunner (11 for a simply
supported arch, using the boundary conditions (reflecting the inextensibility
conditicn)
V= v1 = = 0 at = 11)
Some of the resulting eigenvalues, corresponding to a solution that is
asymmetric with respect to € = 0, are shown in Table I.
An approximate solutlon for a semi-circular arch (- v/2 < 7/2) has
been given by Levy [31, and recently it has been generalized by Babcock and
Singer [5] to properly account for the vanishing of the displacement v1 at
the arch ends. This approximation, which assvimes an incompressible arch, is
here generalized for arbitrary vertex angle 2%, to take the form:
OIAWI = A sin -, V - ( + cos-) (12)
It is easily verified that the qolution (12) satisfies the inextensible pin
conditions at i = ± a. Then the linearized poLe,.tial ancrgy (6? can be
easily converted into a Rayleigh Quotient to obtain (inextensible) approximate
critical loads. i.e.,
a dXJ P1- I ) dO
A = '13)
Substititn of the assumptions (12) into the quotient (13) yields
-7-
2? 2 2
2 2= c.14)
cr 22+ (--!) 2
2a
Some numerical values of A are given in Table 1. The agreement is
obvious'.y quite good. :.uso, it is noted bere that for the case ,A =1/2,
i.e., a complete ring, the mode shape represented by Eqs. (12) has been
shown to be essentially identical to that obtained by Ch,ialla and Kollbrunner
in their annlysis [5].
Finally, in an attempt to assess the effect of the inextensibility
assumption on the buckling load (aee the work of Kamel [2]) and to lay the
groundwork for the study of the effects of inextensibility on the post-
buckling behavior, an ecct solution to the differential equations (7) ana
the boundary conditions (10) is now given. The asymetric solution to
equations (7) is
Ew1 A1 s'n y r 2 sinO + Y coso
(15)
Av1 =o + (QA3 - A2)cosO +A sinO
where
1+ H{A -1) (16)S= - ( - 1)
and the Ai are constants, determined to within an arbitrary factor by
satisfaction of boundary coisditions.
• This solution is not valid for A = 1. However for 0 < 4 /2, thi is
of no concern here, as A > 3.
-8,,
Using the results (US), the exact in-plane strain and rotation formulae
(for buckling) can be written as:
e= (1- Q) A3 siniz (17a)
E 1f- AcoO s (1 + Q)A 3cos (17b)
The eigenvalue- (buckling loads) are obtained after satisfying the following
boundaryI conditions:
V 0, - 0 at 4. (18)
The resulting transcendental equation from which the buckling load is calculated
is found to be:
2(1 + Q) sin ct (19)( + 2Q - AQ)sinacosa + a(l - X)
For the sake of comparison, the eigenvalue equation obtained by Chwalla and
Kollbrunner is also given.
rX tan Nra = 2 sin2a (20)(3 - X)sinacosa + a(l - X)
It is seen that Ecs, '19) and (20) are identical when Q = 1, which corresponds
to inextensional deformation (Eq. (17a)). Numerical values for the buckling
pressures given by Eq. (19) are presented in Table 1, and again the agreement
is excellent.
It is worth noting at this juncture a few featurus of the extensional
strain eE resulting from the exact solution. First, considering the co-
efficient on the right hand side of Eq. (17a), and the definition of Q (Eq.
(1,5), it can be seen that
9-
2H(A - 1) H 1.1 - H( - 1)(21)
rropo'tional to the square of the thickness-to-radius of the arch, and
is thus quite small.
Secondly, it can be observed from Eq. (17a) that the extensional
strain is an odd function of the arch coordinate, i.e.,
e -€1 = -e () (22)
Also, it turns out that there exists another uncoupling of the exact
differential equations (7) that yields the result
2Ed e E+ e = (2:)
Thus, in addition to the odd flnction represented by the sinusoid al-
ready obtained, there is another sclution to the equations for -Which
W and eE(C) are even functions of € , tUe latter being a cosinusoid.1 1
This solution is not considered at all in the present work as attention is
restricted o rly to arches steep enough for asjnetric(biturcation) buckling
to take place.
...I m~ epl!Iwimlm =
-10-
4. POSTBUCKLING: TIE BUDIANSKY-HUTCUINSON APPROACH
In this sectir. the early postbuckling behavior of the ar,- will be
obtained, foliowing the asymptotic analysis outlined in the very lucid
exposition of B' Ciansky [9j. As with the buckling analysis, only asym-
metri- buckling of steeper arches is considered here. For very shallow
arches symmetric buckling can take place at lower pressures [133. how-
ever this snap type of buckling cannot be analysed with the Koiter theory.
The starting point is the virtual work (or variational) statement of the
full nonlinear problem:
f [; 6e + NX 6x+M 6K- Xw]dO = 0 (24)
In addition to the nomenclature defined in the previous section, the
curvature K has been introduced in Eq. (24). Then
H = K , - (.!5)dO
The variational equation (24) must hold fcr any kinezatically consistent
.. d-- .ncc... vr 4 AI-4 nn 5v and 6w. with corresponding strain
field variations le, 6X and 6K.
The following expansions are now introduced:
v = XV 0 cv 1 + c 2v2 +....
w= Xw 0+w 1 + C 2 w2 +
e = )e + Ce1 + C2 e2 +....
S= X° + £X1 + CX 2 +..K 1 2
31
N = 0-o + eN I + C2 N2 + ...
.M 1 + C2 (26)
Here c is a smn&1l parameter such that when C - 0, then X ) Xcr ,
the biturcation buckling pressure. The curvature and moment expansions
begin with terms of order £ to denote that the p.e-buckling state
(zeroth order terms in Eqs. (26)) Is a membrane stae. In fact, as it
is easily demonstrated that a nonlinear membrane state cannot exist for
this problem, the quartity x° shall be henceforth taken as zero, and
thus only a linear membrane pre-buckling state'is considered.
For the "unvariedr quantities in Eq. (24) the expansions (26) are
substituted. After rearrangement by increasing powers of e , the following
new variational equation results:
af [- 1Se - A6w ]d
a.cf [N16e + MI6K- X 1*X]dO
+ C f rN A. ' -(7-a . ..- 2 ... . .. ' I' 1 -^2P ,,,,O , (27)
a+ 3- [N 3
6 e + M36 K + (N1 X2 + N2X No 0X3 )6X]dO
+........= 0.
The pre-buckling state is defined by the vanishing of the zeroth
order variation. After a simple calculation that state is found to be
- 12 -
N A, e =-H, w = 11, v 0 0 (25)0 0 0 0
With the vanishing of the zeroth order term in Eq. (27), an c may
be divided through, and thus the buckling state itself is now found to
be, recalling that e - o implies A - A cr:
fI 511 6e + MS6K - 'crXl6X]dO = 0 (29)
The Euler-Lagrange equations of this variational equation are;
dN1 dM1
d- + A crX1 0 0 (30a)
!~ d g,dx1
Expressed in terms of displacements, Eqs. (30) are identical to the
linearized equations (7? given earlier.
It was pointed out earlier that the set of displacement variations
constantly alluded to need only be kinematically consistent, and since
the buckling displacements most surely are such a set, they can be
appropriately Iart-cd i-n Eq. !291 to yield the Rayleigh Quotient
(Budiansky's "energy equation") for the critical load,
f(Nl1e 1 + MI1K )dOcr 2(~e= - (31)
(I) 2dO
The same substitution in the more complete variational statement (27)
must be equally valid, and noting the quotient (31), it is found that
Ic -13-
(A -2
(X cr A) !~d
CL
2+ f (N2e1 + M 2K1 + N - XXX]dQ (32)-ai
2 O 2+ C f [rT3e1 + "3N ! + N +yIX2 + N2 X1 - k.lx 3 di 0-Oi
At this point the relationship between (A - A cr appears tci be taking
shape. However, it appears that equations of the third order will have to
be solved in order to obtain the roefficient of C2 above, In order to
avoid this difficulty, an orthogonality condition is introduced as follows
f (?I e + M d = 0; =-2,3,4 ... (33)th
It follows from Eas. (33) and (29), since the m order mode shapes must
be kinematically admissible, that
fX= ; 2,3,4 (34)-ai
in order to appiy the orthogonaiir.y condi-Lion i331 tuiid ,L6 ion ie
(34) successfully, the following consequenccs of constitutive linearity
and geometric nonlinearity must 3e noted:
* The precise meaning of this crthogonality condition has not beenestablishel ar is the subject of some discussion7 see Reissner[14].
:t - 14 -
2 21 2N2e = 2 1 1 N 2 = ll 2 +2 1 )
N3 e1 = N 3S I = N1 S3 = N1 (e 3 + X IX2 ); (35)
M 2K I M 1K2 ; MI3K1 = 1K3 ;
In Eas. (35), S. has been used t: denote the total nonlinear strain of
order c , which is made up in part of lower order terms due to the
geometric nonlinearity. Then notings Eqs. (35), (33) and (34), the
variational equation (32) can be put into the very simple form:
X = A ;- a' + b'e +.... (36)cr
where 2f N X1 d
at = 2 -a (37a)f X 1 dO5
OL 2]df [2NIXIx 2 + N2x1 ]dO
b' -a a 2 (37b)
f xi de
Since
a N -S -(e +-(8H -1 H1 2 H 2 =H 2 x 1)(8
the result (36) can be written in its final form:
A 2l + a + bc +.... (39)cr
where 2fe 1 da ' 3 -cca = j- =-(40a)Acr 2HXcr a 2
- 1
Q 2 1 4f[2ex\ 2 X+e -X xP:
b _b 1 Q _ -- 1 1_2 21 1(40b)
cr Hcr f~d
Recall that according to the %.Leory, .it a 3 0, then the stracture will
be in an unstable state in the cotbucki.ng range, and it will also be im-
perfection sensitive. If a = 0, '. , 0, then t-e poitbuckling stability
and the imperfection sensitivity va.y as the arithmctic !-gl of b.
In the present result it app.2:s at first glance that the existence of
a stable or unstable equilibrium statE in the pcstbuckling range depends on
whether or not inextensicility is assumed. For from equation (40a), ii
e 1() is non-zero, then the coefficient a might be. However, recalling
Eq. (221, it is clear th&t the coefficient in question will always vanLsh
for asymmetric buckling! Thus the exclusion (or inclusion) of the arch
extensibility can at best cnly influence the quantitat.ve nature of the post-
buckling equilibrium state, and not its qualitative nature.
It has already been shown that for asymmetric bucklrng the buckl tng
extensibility eI is quite small in magn:tude, with no appreciabis effect
on the buckling load. With this in mind, as well as the discussion of the
previous paragraph, it seems quite reasonable to stipuletc Lhat
e 0 and e 2 =0 (41)
In this instance the coefficient b reduces toct 4f xld;
b L (42)cr a 2
I ds
- 16 -
Using the excellent approximate solution (12), with its critical load
defined b Eq. (14), it is then a straightforward matter to calculate
the postbuckling relationship:
2 2_[1+3 (--l) + 2- -1) 21CL 2 a (12 a 2 .CA .2
- cr 2) 2 2 -- j (43)[2 +(2- - 1)
(In writing this result cognizance has been taken of the fact that the co-
efficient A in Eq. (12) was nondimensionalixed with respect to the radius*
R, i.e. A = , and of the definition (3)).
It is clear from Eq. (43' that X > Xct, and thus the postbucklingbehavior is always stable, and that the arch (or ring if a = 2) will not
be sensitive to imperfections :in its" behavior.
- 17 -
5. POSTBUCKLING: OITER'S APPROACH
In order to examine the stability of the bifurcation poin% and of
the postbuckling behavior using Koiter's approach directly, the total
potential energy is first divided into the prebuckling contributions,
and into the terms due to the buckling and prebuckling behavior. If
the prebuckling behavior is again linearized, the "expansions" (44) are
now introduced, i.e., let
e = Ae + e0
w = Aw + w (44)
0
X= X
Substituting these expansions into the energy functional (5) yields
2R (U + V) 2 XE =" f (Xe 2 - 2A2wo)do
-a.
+ (27,s a - 2.A--iwjd1'H 0 0
1 2- 2 2 14-aX
I- (e7 +Xe X 2+ eX2 + I 4]do
+ f (dX)2 do (45)(do
In view of the prebuckling results obtained earlier, the total potential
energy due to deformation beyond the prebuckling state can be written ao
- 18 -
p 2RA A A
- (U + V) +2aiHA 2 = P1 + P2 +P 3 + P4 (46)
where
P = - 2 f (e + w)do (47a)
X i a 2
P 3 f eX do (47c)-a
X 1 2L 41= 1 a 2
P4 iH xdo (47d)
aNow, by the definition of e(4¢) it is clear that
X dvA~ =- f (- w + O DE2(a) - v(-Q (48)
Hence, for a supported arch, P X 0. Thus the potential enezgy change1~
during and after buckling is simply
PX = PA + PA PA (49)2 3 4
where PN, PX and PA are given by equations (47b, c,d).
'2 3 4eutos
Recall that the behavior of interest takes place at loads very close to
A k A the cinod. Thus, to & - . -th.......
functionals (47) can be expanded in Taylor series about the point A = Acr
As P3 ' p4 do not (for this problem) explicitly depend on A, they appear
only as constants, while
A AA +l) dPA2
P1 +(- A)-d- .
2 r A=Acr cr cr
=P 2 + ( - Acr)P 2 +.. (50)
- 19 -
where1a a a
P 2 = e 2+ () 2 d o (51a)
2 acr-OL -aL
pc =- f X2d (51b)-a
Then the total energy change is
P A ;2 + (X - X ) p' + P + P (52)A1
where P3 = P3 and P4 = P4
Now the following displacement and strain expansions are introduced:
2W = Cw + C w2 +
V = CV I + C v 2 +(53)
2e = Ce + C e2 + ...
X = EX1 + £2X2 +
where £ is the same small parameter used previously. Introduction of the
4expansions (53) into the energy functionals yields, to order c
a 1 a, a dX1 5P C4 f ~~ed - X I X d + rc 12 - do2 _a cr-a -a
3 1 a a a dx dX23 2. - c u-+2c f e e2dO - do + do) (54a)
H1 41 Xc _, 2lX f+ 4 1 (e 2 + 2ele3)do - Xv f (X2 + 2XiX3)d
if-a 2 13-a 2 13
a dx 2 2 dX. dX3+ f(-) + 2 jo-- do
do
'1~ -20-
6- =2c f x - 2 (54b)P 2 2 I xld-- f[X2 + 2XIX 3]d(4
-CL t
ac -cc
3 1 2 4 12P 3 = C- H elXl10 + C if f [ex I1 + 2e xiX2])d (540)
P 4 = 4 C r4id
-CL
Then the same orthogonality conditions applied in the Budiansky-
Hutchinson formalism are applied again (written entirely in terms of
kinematic quantities) to tne functtonals (54). These functionals are then
greatly simplified and take the form:
2[1 a e2¢ 2 Ct X 1€+P2 = e ( _i X +r f W d
2 H 1 1 -CL d
(55a)
+4 I e 2d¢ f X2 dO + fL 2d 2H ea2 y cr _Ci 2 -ad
p=_ 2 X~d,- 4 x~cc (Sb-CL -CL
i C d- (55c)
L3 1 CL
U 4 1 1
+ C 4 1 [e2XI + 2elXiX2]do
S4 1_ X 4 do 05d)4 C T, d4l
Note that the term of order c 2 in P2 is simply the Rayleigh
quotient, and thus it vanishes identically. Further, the term of order
4.~£ in P2 will be multiplied by (A - Acr . according to equation (52).
- 21 -
S.nce it in expe:,ted that for this problem that (A - Xcr) will be of
order £2, the te= of order C4 in P2 may be deleted as being of
higher order. Thus the final form of the energy change is:
2 a 2 31a 2C .X( -A cr) f X do + 3 FI e1 2 de-G -a
14 a 2 1 4+ e f [e 2X1 + 2e 1 X1 X2 + -- X] do (56)
-ci
.2 2 a dX2+ -fed -cr I 4d + f (=-,do
H-_a -a -a d
The resemblance between the present approach and the Budiansky-Hutchin3on
approach is now more visible. However, it appears that there will be some
difference due to the term
1 a2 2 dX d 2-,2 [W2,V2 ] f 2do - Acr 2 + d
in the expression of order C4 in Eq. (56). Terms o this type do appear
consistently in Koiter's original analysis (see, for example, Section 3' of
Ref. (6].), although they do not appear in analyses using the Budiansky-
Hutchinson formalism (see, for example, Ref. [91.). For the present work,
under the well established assumption of inextensibility, the terms
P 2 [w2,v2] will be shown to yield no contribution to the result, and the
results will be identical to those already obtained.
The cecond order displacements, v2 and w2, are obtained as the
solution of the variational equation
~- 22 -
ae2 a ., a OX2d66 { f e~d- ac x.d, + f (-) dIt-CE cr za .W-_ - -a
a 2 1 4+ le X2 + 2,1Yl +-11de 0 (58)
at 2 1-'T2 4
In carryir.; out this variation all terms of first order are of course
considered as knwzn or given quantities. If inextensibility of the arch
is asoswed, e= 2= 0, then the vatiationa1 L.-ation is justI 2
2d1( (2x f X2d = 0 (59)6(I (v ¢:-a
Thus the variational equation leads to set of homogeneous cquati,as that
can have only a trivial solution . :.ence, for thc inextcnsible arch, it
*l is possible to take as solutions for the second order displacements the
trivial ones, i.e.,
w2 =v 2 =o (60)
Hence the energy functional reduces to (recalling eI = 0 again):
2 a 2 4 a- 2 (A - X v2 d ' 4 1. f d. (61)cr d 411-
Using the approximate solution (12), with A = A /R, it is a . ,ht-
forward natter tu cc;ipute the energy char.e 1, asX C 3 2 * 5 2 2
S -[ + '.-- 1)1(X - X) + ( ) -- - - )"- -)2 '2 cr R 4 2
(62)
* A solution linearly deprkndent or, th- buc:zlin s-.0ution i; tu}cl out by
the orthogonality condition.
4'
A ,Jl l .. ,.. .
23-
At tLe c.litical lcad, ' = > *-t is st .h- 1 . and th's iC-cr'
bifurcation (critical) state is iLself stable. The inltLal postbuckling
load-deflection relationship is determined by the condit4 n
dp "
'63= c *3)
d(cA )
from which it follows that
2I + 31- -1) 1) 21
1= r + (12) - (,2 (64)IT2T2 + (r - 1)
C1
This is exactly the result (43) obtained previously.
* This is an approximation to 6P = 0
- 24 -
6. DISCUSSION AND CONCLUSIONS
The present paper has considered the buckling and postbuckling
behavior of circular arches (and rings) under constant directional
loading. For arches steep enough so that asymmetric; bifurcation
buckling is critical, it has been demonstrated that the arch inextensi-
bility is a negligible quantity in magnitude, in its effect on the buckling
load, and in its effect on initial postbuckling behavior. In addition an
approximate solution for the linearized eigenvalue problem was presented
that duplicated almost precisely the buckling pressures obtained from the
exact solution.
The numerical results for the eigenvalue problem as solved by Chwalla
and Kollbrunner and as given by the present approximate and exact sclutions
have been given in Table 1. It is worth pointing out that the approximate
(inextensible? eigenvalues are always greater than or equal to Chwalla and
Kollbrunner's (inextensible) results, in accord with Rayleigh's Principle.
The results when the extensibility is accounted for are always less than the
inextensible results. This is in direct contrast to the analysis of Knmel
[2] which indicated that the buckling pressures would increase if extensi-
bility were accounted for As it has already been pointed out, the
* Singer and Babcock (5] have already pointed out that K nmel's result was
also erroneous in arriving at the coefficient X = 4 for constantor
j directional pressure, assuming inextensible deformations.
- 25 -
differential eauation solved by Chwalla and Kollbrunner, assuming in-
extensibility, is identical to that solved here, without that assumption.
The difference is in the boundary conditions, where the inextensibility
assumption provides less freedom (greater stiffness). Hence it is quite
proper that the inextensible eigenvalues be upper bounds to the (freer)
extensible eigenvalues.
It is also worth pointing out that the results given in Table 1 for
the Chwalla-Kollbrunner eigenvalues are not precisely those given in the
original paper (1]. Rather they were calculated (using a digital computer)
directly from the transcendental equation (20). There ari some dis-
crepancies, although they are very small. For example:
Chwalla and Kollbrunner [I] Chwalla and KollbrunnerE . (20) - Digital Computer
8.725 8.7273
a M 3.265 3.2712
It is easily verified that the original Chwalla and Kollbrunner results satisfy
Eq. (20) to within the precision of limited-accuracy trigonometric tables and
slide rule accuracy that must have governed calculations in the early 1930's.
The postbuckling behavior for the constant-directionally arches ard rings
has been shown to be quite stable, and thus imperfection sensitivity is not
an issue here. Also it has been shown, under the reasonable assumption of in-
extensible buckling and posthuckling deformation, that the second order dis-
placement solution does not change the results that would be obtained if
only first order (buckling) displacementswere used in the calculations.
- 26 -
Finally it has been showm that, ror the special circumstances of
this problem, the approach of Koiter as originally given and the variation
proposed by Budiansky and Hutchinson lead to identical results.
ACKNOWLEDGEMEUTS
The author is grateful for the partial financial support offered by
Carnegie-Mellon University that made his visit to the Technion possible.
It is also a great pleasure to thank Professor Josef Singer for
arranging the visit, and Professors Singer and Menachem Baruch for many
helpful and informative discussions and critiques.
V-27-
REFERENCES
1. Chwalla, E., and Kollbrunner, C.F., " Beitrage sun Knickproblen des
Bogantragers und des Raimen", Stahlbau, Vol. 11, No. 10, May 1938,
pp. 73-78.
2. K)aMel, G., "Der Einfluss der angsdehnung auf de elastische Stabilitat
geschlossener Kreisringe", Acta Maohanica, Vol. 4, 1967, pp.34-42.
3. Levy, M., "Memoire sur un nouvea cas integrable du problem* de l'elastque
et 1'une des ses applications", Journal de Mathematiques pures et
Appliquees, Liouville, Series 3, Vol. 10, 1884, pp.5-42.
4. Carrier, G.F., " On the Buckling of Elastic Rings', Journal of Mathematics
and Physics, Vol. 26, 1947, pp. 94-103.
5. Singer, J., and Babcock, C.D., " On the Buckling of Rings tnder Constant
Directional and Centrally Directed Pressiure", Journal of Applied Mechanics,
Vol. 37, No. 1, March 1970, pp. 215-218.
6. Koiter, W.T., " Over de stabiliteit van het .elastisch evernvicht" ("On
the Stability of Elastic Equilibrium". Thesis, Delft, N.J. Paris,
Amsterda!m; 1945. Enalish trns1ation issued a, ?$5A 70k F-10:833,1967.
7. Budiansky, B., and Hlutchinson, J.W., "Dynaic )auckling of Imperfection -
Sensitive Structures", Proceedings of the X! International Congress of
Aplied Mechanics, H. Gortler, Ed., Springer Verlag, New-York,1964,pp.636-651.
8. Budiansky, B., "Dynamic Buckling of Elastic Structures: Criteria and
Estimates," Proceedings, Internatioz" Confererce on Dynamic Stability o!
Structures, Pergamon, flew York, 1966, pp.83-06.
C
- 28 -
9. Budiansky, B., "Post-Buckling Behavior of Cylinders in Torsion", Theory
of Thin Shells, F.L. Niordson, Ed., Springer Verlag, Berlin, 1969.
10. Koiter, W.T., " Post-Buckling Analysis of a Simple Two-Bar Frame",
Recent Progress in Applied Mechanics, Ali~ruist and Wiksell, Stockholm,
1966, pp.337-354.
11. Haftka, R., and Nachbar, W., "Post-Buckling Analysxs of an Elastically-
Restrained Column," Intmenational Journal of Solids and Structures,
Vol. 6, No. 7, 1970, pp.1433-1449,
12. Sanders, J.L., "Non-Linear Theories for Thin Shells", Quarterly of
Applied Mathematics, Vol. 21, No. 1 , 1963, pp. 21-36.
13. Schreyer, H.L., and Masur, E.F., "Buckling of Shallow Arches", Journal
of the Engineering Mechanics Division, ASCE, Vol. 92, No. EM4, August
1966, pp.1-19.
14. Reissner, E., " A Note on Postbuckling Behavior of Pressurized Shallow
Spherical Shells", Journal of Applied Mechanics, Vol. 37, No. 2, June
1970, pp.533-534.
15. Roorda, J., "The Buckling Behavior of Imperfect Structural Systems",
Journal of Mechanics and Physics of solids, Voi. 13, 1965, pp.267-280.
-29-
TABLE 1: ASYM14ETRIC BUCKLING PRESSURES FOR CIRCULAR ARCHES; 1 = qR3 /EI.
Solution of Chwalla Present Present Exactand Follbrunner Approximation Result Eq. (19)Eq. (20) Eq. (14) (h/R = 1/10)
- 99.979598 99.979598 99.97954110
63.967766 63.967766 63.967676
35.941318 35.941320 35.9411516
15.859006 15.859031 15.858590
1 3.271245 3.272727 3.269233
k____