<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">AJCM</journal-id><journal-title-group><journal-title>American Journal of Computational Mathematics</journal-title></journal-title-group><issn pub-type="epub">2161-1203</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ajcm.2014.43014</article-id><article-id pub-id-type="publisher-id">AJCM-45995</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>PHYSICS &amp; MATHEMATICS</subject></subj-group></article-categories><title-group><article-title>Supersonic Flutter of a Spherical Shell Partially Filled with Fluid</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Mohamed</surname><given-names>Menaa</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Aouni</surname><given-names>A. Lakis</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Mechanical Engineering, Ecole Poly Technique de Montreal, Montréal, Canada</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>Aouni.lakis@polymtl.ca(AAL)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>17</day><month>04</month><year>2014</year></pub-date><volume>04</volume><issue>03</issue><fpage>153</fpage><lpage>182</lpage><history><date date-type="received"><day>28</day>	<month>November</month>	<year>2013</year></date><date date-type="rev-recd"><day>28</day>	<month>January</month>	<year>2014</year>	</date><date date-type="accepted"><day>5</day>	<month>February</month>	<year>2014</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
	In the present study, a hybrid ?nite element method is applied to
investigate the dynamic behavior of a spherical shell partially filled with
fluid and subjected to external supersonic airflow. The structural formulation
is a combination of linear spherical shell theory and the classic finite
element method. In this hybrid method, the nodal displacements are derived from
exact solution of spherical shell theory rather than approximated by polynomial
functions. Therefore, the number of elements is a function of the complexity of
the structure and it is not necessary to take a large number of elements to get
rapid convergence. Linearized first-order potential (piston) theory with the
curvature correction term is coupled with the structural model to account for
aerodynamic loading. It is assumed that the fluid is incompressible and has no
free surface effect. Fluid is considered as a velocity potential at each node
of the shell element where its motion is expressed in terms of nodal elastic
displacements at the ?uid-structure interface. Numerical simulation is done and
vibration frequencies are obtained. The results are validated using numerical
and theoretical data available in literature. The investigation is carried out
for spherical shells with different boundary conditions, geometries, filling
ratios, flow parameters, and radius to thickness ratios. Results show that the
spherical shell loses its stability through coupled-mode flutter. This proposed
hybrid finite element method can be used efficiently for analyzing the flutter
of spherical shells employed in aerospace structures at less computational cost
than other commercial FEM software.</p></abstract><kwd-group><kwd>Vibration</kwd><kwd> Spherical shell</kwd><kwd> Flutter</kwd><kwd> Hybrid FEM</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Shells of revolution, particularly spherical shells are one of the primary structural elements in high speed aircraft. Their applications include the propellant tank or gas-deployed skirt of spacecraft. Due to the aerodynamic shape combined with thin wall thicknesses, spherical shells are more disposed to dynamic instability or flutter induced by high Mach number gas flow. It is therefore important to understand the effect of different flow parameters and loadings on their aeroelastic response.</p><p>Aeroelastic analysis of shells and plates has been studied by numerous researchers experimentally and analytically [<xref ref-type="bibr" rid="scirp.45995-ref1">1</xref>] . Dowell gives an exhaustive study of the aeroelasticity of shells and plates in his book [<xref ref-type="bibr" rid="scirp.45995-ref2">2</xref>] . After introducing the application of piston theory in the aeroelastic modeling presented by Ashley and Zatarian [<xref ref-type="bibr" rid="scirp.45995-ref3">3</xref>] , a number of interesting experimental and theoretical studies were carried out to investigate supersonic flutter of cylindrical shells. In general, all of this research was concerned with the development of an analytical relation to describe the effect of shell and flow parameters on the critical flutter dynamic pressure. Aeroelastic models in combination with linear or nonlinear piston theory were coupled to the theory of shells to account for fluid- structure interaction. The resulting governing equations were treated numerically using the Galerkin method. A comprehensive experimental test was done by Fung and Olson [<xref ref-type="bibr" rid="scirp.45995-ref4">4</xref>] . They studied the effects of shell boundary conditions and initial stress state due to internal pressure and axial load. It was observed that pressurized cylindrical shell fluttered at a lower level of freestream static pressure than predicted by theory [<xref ref-type="bibr" rid="scirp.45995-ref5">5</xref>] . Later, Evensen and Olson [<xref ref-type="bibr" rid="scirp.45995-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.45995-ref7">7</xref>] presented a nonlinear analysis to take account of this observed effect. Dowell [<xref ref-type="bibr" rid="scirp.45995-ref8">8</xref>] also analyzed the behavior of a cylindrical shell in supersonic flow for different flow and shell parameters. A complete description of panel flutter modeling is given in his book [<xref ref-type="bibr" rid="scirp.45995-ref2">2</xref>] . A study by Carter and Strearman [<xref ref-type="bibr" rid="scirp.45995-ref9">9</xref>] showed that agreement between the theory and experiments reported in the literature exists in cases that involve a small amount of static preload acting on the shell. Amabili and Pellicano [<xref ref-type="bibr" rid="scirp.45995-ref10">10</xref>] included geometric nonlinearities in their study of supersonic flutter of a circular cylindrical shell. By selecting expansion modes to discretize the aeroelastic equations, they were able to facilitate their solution, and therefore succeeded in capturing the nonlinear behavior of the shell correctly.</p><p>There are also some researchers who focused their efforts on the numerical study of this problem. The equations of virtual displacements were solved using the finite elements method. Aeroelastic governing equations were formulated by applying classical shell theory coupled with the piston theory for evaluation of aerodynamic forces. For example, Bismarck-Nasr [<xref ref-type="bibr" rid="scirp.45995-ref11">11</xref>] developed a FEM applied to supersonic flutter of circular shell subjected to internal pressure and axial loading. Ganapathi et al. [<xref ref-type="bibr" rid="scirp.45995-ref12">12</xref>] modeled an orthotropic and laminated anisotropic cylindrical shell in supersonic flow using FEM and analyzed the effect of different shell geometries on the flutter boundaries.</p><p>Aeroelasticity of conical shells has also been investigated by few researchers. The leading work in this field was conducted by Shulman [<xref ref-type="bibr" rid="scirp.45995-ref13">13</xref>] . Ueda et al. [<xref ref-type="bibr" rid="scirp.45995-ref14">14</xref>] investigated theoretically and experimentally the supersonic flutter of a conical shell. Dixon and Hudson [<xref ref-type="bibr" rid="scirp.45995-ref15">15</xref>] studied the flutter and vibration of an orthotropic conical shell theoretically. Miserentino and Dixon [<xref ref-type="bibr" rid="scirp.45995-ref16">16</xref>] investigated experimentally the vibration and flutter of a pressurized truncated conical shell. Bismarck-Nasr and Costa-Savio [<xref ref-type="bibr" rid="scirp.45995-ref18">18</xref>] studied the supersonic flutter of conical shells using finite element method. Sunder et al. [<xref ref-type="bibr" rid="scirp.45995-ref18">18</xref>] successfully applied the finite element analysis to calculate the flutter of a laminated conical shell. In another study they found the optimum cone angle in aeroelastic flutter [<xref ref-type="bibr" rid="scirp.45995-ref19">19</xref>] . Mason and Blotter [<xref ref-type="bibr" rid="scirp.45995-ref20">20</xref>] used a finite element technique to find the flutter boundary for a conical shell (a typical rocket nozzle element) subjected to an internal supersonic gas flow. Pidaparti and Yang Henry [<xref ref-type="bibr" rid="scirp.45995-ref21">21</xref>] completed a theoretical study to predict the onset of flutter instability for composites conical shells.</p><p>An analytical approach to the supersonic flutter of spherical shell becomes very complicated if one wishes to include different parameters. Therefore, the efficiency of numerical methods such as the finite element method (FEM) is an advantage for cases involving changes to all factors affecting flutter boundaries. The aim of the present study is to develop a hybrid finite element method in order to predict the aeroelastic behavior of isotropic spherical shells with different parameters as boundary conditions, geometries, flow parameters, filling ratios and radius to thickness ratios. The finite element is a spherical frustum instead of the usual rectangular shell element. Linear thin shell theory is coupled with linear piston theory. In the case of a fluid filled shell the effect of dynamic pressure acting on the wall is modeled based on a velocity potential formulation and Bernoulli’s equation. It is assumed that the fluid is incompressible and has no free surface effect. The linear mass, damping and stiffness matrices are obtained. The aeroelastic equation of motion is reduced to a standard eigenvalue problem. The flutter boundary is found by analyzing the real and imaginary parts of the eigenvalues as freestream pressure is varied.</p></sec><sec id="s2"><title>2. Formulation</title><sec id="s2_1"><title>2.1. Structural Modeling</title><sec id="s2_1_1"><title>2.1.1. Equilibrium Equations</title><p>In this study the structure is modeled using hybrid finite element method which is a combination of spherical shell theory and classical finite element method. In this hybrid finite element method, the displacement functions are found from exact solution of spherical shell theory rather than approximated by polynomial functions as done in classical finite element method. In the spherical coordinate system (R, θ, ϕ) shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>, five out of the six equations of equilibrium derived in reference [<xref ref-type="bibr" rid="scirp.45995-ref22">22</xref>] for spherical shells are written as follows:</p><disp-formula id="scirp.45995-formula114"><label>(1)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7f1c888b-ccc1-42ac-ad1b-58cc61128020.png"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\daa81ab7-870d-4029-a30c-05fca299528b.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\28918507-d77c-4269-a4dc-a0af5ab9a271.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\54c02025-dce9-4cf1-bafa-ddc08fa96282.png" xlink:type="simple"/></inline-formula>are membrane stress resultants; M<sub>ϕ</sub>, M<sub>θ</sub>, M<sub>ϕθ</sub> the bending stress resultants and Q<sub>ϕ</sub>, Q<sub>θ</sub> the shear forces (<xref ref-type="fig" rid="fig2">Figure 2</xref>). The sixth equation, which is an identity equation for spherical shells, is not presented here.</p></sec><sec id="s2_1_2"><title>2.1.2. Constitutive Relations</title><p>Strains and displacements in axial, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\910ad421-f56d-471e-b37a-f70f9191e618.png" xlink:type="simple"/></inline-formula>, radial, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\912062d6-8560-43df-9645-5d804954bae3.png" xlink:type="simple"/></inline-formula>, and circumferential, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\b550bcd4-1b7e-43ee-89bc-ead262c2a23c.png" xlink:type="simple"/></inline-formula>directions are related as follows:</p><fig id="fig1"><label>Figure 1</label><caption><p> Geometry of the spherical shell</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\b377620d-0b2a-4e45-935e-d383ce973c2f.png"/></fig><fig id="fig2"><label>Figure 2</label><caption><p> Stress resultants and stress couple</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\fb4e577c-24a8-4263-a632-23535e62d1ea.png"/></fig><disp-formula id="scirp.45995-formula115"><label>(2)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a3168607-68e3-46c2-9ef7-698e3996d95e.png"/></disp-formula><p>Displacements<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ebf59ebc-931d-4656-a6df-e7649a5ab322.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\60c03601-d2d8-4afb-ba79-16da44cc10f4.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\22afcc8a-e76d-4efe-a323-cef5ad43d626.png" xlink:type="simple"/></inline-formula> in the global Cartesian coordinate system are related to displacements<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c620617c-f83c-4074-8b5a-cee51c026219.png" xlink:type="simple"/></inline-formula>,</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\032314c4-b89e-4b32-8261-abc4a90faccf.png" xlink:type="simple"/></inline-formula>And <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\4a5fb32b-cd4e-439e-96f0-bade880c554e.png" xlink:type="simple"/></inline-formula> indicated in <xref ref-type="fig" rid="fig3">Figure 3</xref> by:</p><disp-formula id="scirp.45995-formula116"><label>(3)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\90e2d116-e46c-40fc-9212-e0b270760738.png"/></disp-formula><p>The stress vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\d3e7f4df-a0f1-4941-81f1-39bbf938621a.png" xlink:type="simple"/></inline-formula> is expressed as a function of strain <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\b8b72b15-6148-4b95-8bdd-739496172661.png" xlink:type="simple"/></inline-formula> by:</p><disp-formula id="scirp.45995-formula117"><label>(4)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f720eb95-4e8e-417d-9015-e9f6de147850.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c732bdd4-6ea5-4c88-8864-52d5d829fd17.png" xlink:type="simple"/></inline-formula> is the elasticity matrix for an anisotropic shell given by:</p><fig id="fig3"><label>Figure 3</label><caption><p> Spheical frustum element</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c9108a93-0ea1-42bf-80cd-1f2f499d4520.png"/></fig><disp-formula id="scirp.45995-formula118"><label>(5)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\25ae060a-2119-4240-9bec-5ca1184896a0.png"/></disp-formula><p>Upon substitution of Equations (2), (4) and (5) into Equation (1), a system of equilibrium equations can beobtained as a function of displacements:</p><disp-formula id="scirp.45995-formula119"><label>(6)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\fcf2d8ec-d6a7-4738-8006-2c967cc06eb9.png"/></disp-formula><p>These three linear partial differential operators<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7a329c50-023e-4e64-984b-dc73a815653b.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\11578c34-65bc-48fa-b6ee-e0fc395e3943.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\5cf97509-4d28-4cbf-a4e3-adfa461e2fcd.png" xlink:type="simple"/></inline-formula> are given in Appendix A, and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\eea8c950-203d-411f-8703-801c6cae5f64.png" xlink:type="simple"/></inline-formula> are elements of the elasticity matrix, which for an isotropic thin shell with thickness h is given by:</p><disp-formula id="scirp.45995-formula120"><label>(7)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\dd72ab41-177f-4c0b-b1d5-c9dc954f1b71.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a4b37c6b-dafe-4b4c-9115-4076f206b8b3.png" xlink:type="simple"/></inline-formula> is the membrane stiffness and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\1d26fc64-8cd7-452f-9e3a-9f772778ea52.png" xlink:type="simple"/></inline-formula> is the bending stiffness.</p></sec><sec id="s2_1_3"><title>2.1.3. Kinematic Relations</title><p>The element is a circumferential spherical frustum shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>. It has two nodal circles with four degrees of freedom; axial, radial, circumferential and rotation at each node. This element type makes it possible to use thin shell equations easily to find the exact solution of displacement functions rather than an approximation with polynomial functions as done in classical finite element method.</p><p>For motions associated with the circumferential wave number n, we may write:</p><disp-formula id="scirp.45995-formula121"><label>(8)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\83b51f1c-588c-468e-85ee-cf8cbdbbcd88.png"/></disp-formula><p>The transversal displacement <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\95b14927-344d-4684-933a-2496fecc96e5.png" xlink:type="simple"/></inline-formula> can be expressed as [<xref ref-type="bibr" rid="scirp.45995-ref22">22</xref>] :</p><disp-formula id="scirp.45995-formula122"><label>(9)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\9596469a-4870-49a9-b85e-d2f8f0ffc4ea.png"/></disp-formula><p>where</p><disp-formula id="scirp.45995-formula123"><label>(10)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\738d9779-eefa-4b19-b3f8-6fcf96cb21d1.png"/></disp-formula><p>and where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\5847e9fc-44c1-4469-8e60-9b66be7b377b.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ba35bdd7-b375-4920-848e-468809dbac8c.png" xlink:type="simple"/></inline-formula> are the associated Legendre functions of the first and second kinds respectively of order n and degree<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\105d0bac-2878-4161-bb1d-56ee91bad805.png" xlink:type="simple"/></inline-formula>.</p><p>The expression of the axial displacement u<sub>ϕν</sub>(ϕ) is:</p><disp-formula id="scirp.45995-formula124"><label>(11)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\2b25389f-e54b-49be-a905-c3e53288b549.png"/></disp-formula><p>where the coefficient E<sub>i</sub> is given by:</p><disp-formula id="scirp.45995-formula125"><label>(12)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6d5de393-17d2-45c5-97da-b9f18b9bac8f.png"/></disp-formula><p>The auxiliary function ψ is given by the expression:</p><disp-formula id="scirp.45995-formula126"><label>(13)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\727addbc-ca93-464d-90da-934e12e77f77.png"/></disp-formula><p>Finally the circumferential displacement u<sub>ϕν</sub>(ϕ) can be expressed as:</p><disp-formula id="scirp.45995-formula127"><label>(14)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\62a9235e-5193-407e-9b1f-88bc593fa6de.png"/></disp-formula><p>The degree <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\8a56c77a-50ef-4f01-9309-e3174b0e5e8c.png" xlink:type="simple"/></inline-formula> is obtained from the expression</p><disp-formula id="scirp.45995-formula128"><label>(15)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\067c79cc-e2bd-4fb5-b468-8b8ef99fc6b3.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\500aca1e-3a7f-434b-89a1-1a483177c010.png" xlink:type="simple"/></inline-formula> is one the roots of the cubic equation:</p><disp-formula id="scirp.45995-formula129"><label>(16)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\73902d50-9f9c-4958-8836-41ae30a2ae47.png"/></disp-formula><p>and where</p><disp-formula id="scirp.45995-formula130"><label>(17)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a4b9ca94-0696-48ae-9ba4-93a8d6f5edab.png"/></disp-formula><p>with<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\0ce0ee8e-80b1-429d-b8a9-92d87ea9d743.png" xlink:type="simple"/></inline-formula>.</p><p>The above equation has three roots with one real root and two others complex conjugates.</p><p>The Legendre functions<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\2d7a680f-070a-497a-be2d-ecc41a0cc0c8.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\db842a36-a9cc-4944-8067-60a57fbdf59e.png" xlink:type="simple"/></inline-formula>are real functions whereas<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\566489d4-61d0-441a-8cde-bfa12f052ba4.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7722a061-7c29-4b8d-a933-54f992c00f4e.png" xlink:type="simple"/></inline-formula></p><p>(i = 2, 3) are complex functions. So we can put:</p><disp-formula id="scirp.45995-formula131"><label>(18)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\092f0b14-bdf6-4488-8270-36fe113976d7.png"/></disp-formula><p>Setting</p><disp-formula id="scirp.45995-formula132"><label>(19)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\60db214f-5f28-4934-9adf-47d94291b536.png"/></disp-formula><disp-formula id="scirp.45995-formula133"><label>(20)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6c2b85f9-b016-4dfa-a292-dd685635ea8c.png"/></disp-formula><p>Substituting Equations (18), (19) and (20) in Equations (9), (11) and (14) we have:</p><disp-formula id="scirp.45995-formula134"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\31ada57c-ab0d-4b9f-aab9-f3445ff4dd6d.png"/></disp-formula><disp-formula id="scirp.45995-formula135"><label>(21)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\5a8125db-652d-4951-9d6d-1218c7d788f3.png"/></disp-formula><disp-formula id="scirp.45995-formula136"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\68d73d1c-08c0-4c57-bfab-92b297241a9c.png"/></disp-formula><p>In deriving the above relation we used the recursive relations:</p><disp-formula id="scirp.45995-formula137"><label>(22)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\95f033e6-3671-4d10-8110-a54ef67af19b.png"/></disp-formula><p>Using matrix formulation, the displacement functions can be expressed as follows:</p><disp-formula id="scirp.45995-formula138"><label>(23)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ddc297f7-fd28-4bdc-ae5b-178bcb521756.png"/></disp-formula><p>The vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\942389d7-c5ba-478e-855f-99a03b69419f.png" xlink:type="simple"/></inline-formula> is given by the expression:</p><disp-formula id="scirp.45995-formula139"><label>(24)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\60aa124f-5dea-44a0-b9ce-372b580aa9e5.png"/></disp-formula><p>The elements of matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a8f831e4-2b62-453a-9904-2b68f80ad140.png" xlink:type="simple"/></inline-formula> are given in Appendix B.</p><p>In the finite element method, the vector C is eliminated in favor of displacements at elements nodes. At each finite element node, the three displacements (axial, transversal and circumferential) and the rotation are applied. The displacement of node i are defined by the vector:</p><disp-formula id="scirp.45995-formula140"><label>(25)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\aee6c573-89c4-4237-8b0e-e0e14987a33c.png"/></disp-formula><p>The finite element shown in <xref ref-type="fig" rid="fig3">Figure 3</xref> with two nodal lines (i and j) and eight degrees of freedom will have the following nodal displacement vector:</p><disp-formula id="scirp.45995-formula141"><label>(26)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7173a381-36ae-4a46-a685-a3a65e3cbb8c.png"/></disp-formula><p>with</p><disp-formula id="scirp.45995-formula142"><label>(27)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\d4e596ae-f0c9-4759-a545-8b12768457f5.png"/></disp-formula><p>The terms of matrix, obtained from the values of matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\383c09c7-a0dd-4187-a3d2-5ddc05ec5e3a.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\bc429ff7-4a38-4add-a5a5-f41c84868715.png" xlink:type="simple"/></inline-formula>, are given in Appendix B. Now, pre-multiplying Equation (26) by <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\278b50a0-2153-4b56-9349-ea5b6e30cba6.png" xlink:type="simple"/></inline-formula> one obtains the matrix of the constant C<sub>i</sub> as a function of the degree of freedom:</p><disp-formula id="scirp.45995-formula143"><label>(28)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ba655970-dc0b-4677-afcd-1da7d62e7d7a.png"/></disp-formula><p>Finally, one substitutes the vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\bbe81333-7ae5-47c5-93d7-db3ba2d8ac45.png" xlink:type="simple"/></inline-formula> into Equation (26) and obtains the displacement functions as follows:</p><disp-formula id="scirp.45995-formula144"><label>(29)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\17b50825-35c3-4383-91b1-4dc5df41431c.png"/></disp-formula><p>The strain vector <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7a88500a-a5b8-4fd0-820f-ff23bf16c0cd.png" xlink:type="simple"/></inline-formula> can be determined from the displacement functions <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\daa22950-6263-4d84-bcb8-b97142af88eb.png" xlink:type="simple"/></inline-formula> and the deformation –displacement equation (2) as:</p><disp-formula id="scirp.45995-formula145"><label>(30)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\435891a9-902e-4363-8155-94ebcd6839da.png"/></disp-formula><p>where matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f0fd5f07-e4b7-4447-929f-c59420b9327b.png" xlink:type="simple"/></inline-formula> is given in Appendix C.</p></sec><sec id="s2_1_4"><title>2.1.4. Mass and Stiffness Matrices</title><p>This relation can be used to find the stress vector, Equation (4), in terms of the nodal degrees of freedom vector:</p><disp-formula id="scirp.45995-formula146"><label>(31)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\693ac2ff-18cd-437d-869a-7e0287725650.png"/></disp-formula><p>Based on the finite element formulation, the local stiffness and mass matrices are:</p><disp-formula id="scirp.45995-formula147"><label>(32)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\de7b6a01-0b0f-4850-8103-793ab6252acc.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\34b23621-64ff-4b2a-a281-66a2df876135.png" xlink:type="simple"/></inline-formula> is the density and h is the thickness of shell.</p><p>The surface element of the shell wall is <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\64adda6a-a4be-499b-99e3-e20778fd04df.png" xlink:type="simple"/></inline-formula> (<xref ref-type="fig" rid="fig2">Figure 2</xref>). After integrating over<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\2cf6e6e2-5755-4cd9-80b5-6a4aba8cfb07.png" xlink:type="simple"/></inline-formula>, the preceding equations become</p><disp-formula id="scirp.45995-formula148"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\9b1471e1-ad16-45e0-a13e-8a33b71ed70d.png"/></disp-formula><disp-formula id="scirp.45995-formula149"><label>(33)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\b820b2db-d941-4f2c-a181-d1ba044f13db.png"/></disp-formula><p>In the global system, the element stiffness and mass matrices are</p><disp-formula id="scirp.45995-formula150"><label>(34)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\e47e11bc-2f88-46e2-b9c6-bd6b19dfd50d.png"/></disp-formula><p>where</p><disp-formula id="scirp.45995-formula151"><label>(35)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\8a223e42-3f28-4e4d-8500-1cde82a04af5.png"/></disp-formula><p>From these equations, one can assemble the mass and stiffness matrices for each element to obtain the mass and stiffness matrices for the whole shell: <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\560823af-87bd-42b3-b694-7e31d77bdf59.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\9a91cf46-e1fa-49cd-959c-25b05346efbc.png" xlink:type="simple"/></inline-formula>. Each elementary matrix is 8 &#215; 8, therefore the final dimensions of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\0eb631b4-5554-4163-b5ff-50e6d1681acc.png" xlink:type="simple"/></inline-formula> and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\2f784061-06e0-47e4-a419-abf3e74a8c19.png" xlink:type="simple"/></inline-formula> will be 4*(N + 1) where N is the number of elements of the shell.</p></sec></sec><sec id="s2_2"><title>2.2. Aerodynamic Modeling</title><p>Piston theory, introduced by Ashley and Zartarian [<xref ref-type="bibr" rid="scirp.45995-ref3">3</xref>] , is a powerful tool for aeroelasticity modeling. In this study the fluid-structure effect due to external pressure loading can be taken into account using linearized first- order potential theory. This pressure is expressed as:</p><disp-formula id="scirp.45995-formula152"><label>(36)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\cd2964d9-517b-4e3b-9188-89e4d1b65dbd.png"/></disp-formula><p>where<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\dac69b0d-9502-4f32-9755-6b40186f9abe.png" xlink:type="simple"/></inline-formula>,<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\41ae2c74-df81-485a-b7d2-fd33b6c9688b.png" xlink:type="simple"/></inline-formula> , <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\9bdd7e20-e2be-4796-88d9-1a7243e06edc.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\294da55a-dac0-4293-b8a7-1599d5ab8815.png" xlink:type="simple"/></inline-formula> are the freestream static pressure, freestream velocity, Mach number and adiabatic exponent of air respectively. If the Mach number is sufficiently high<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\8ad25d50-bb99-4687-845a-c04393b0e912.png" xlink:type="simple"/></inline-formula>, and curvature term, <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\b7343f11-c856-48a9-a170-3249e299fc62.png" xlink:type="simple"/></inline-formula> is neglected, the result is the so-called piston theory:</p><disp-formula id="scirp.45995-formula153"><label>(37)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a11181e8-6035-44df-a83c-4ca70237514c.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f240a2d8-e137-4e6d-8f8a-fb192e8ce825.png" xlink:type="simple"/></inline-formula> is the free stream speed of sound.</p><p>Finally, the aerodynamic pressure in terms of radial displacement is written:</p><disp-formula id="scirp.45995-formula154"><label>(38)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7e647ee8-8b00-4e0c-80fd-84f58da4e2bb.png"/></disp-formula><p>and the pressure loading in terms of nodal degrees of freedom is written as:</p><disp-formula id="scirp.45995-formula155"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\1eb8a6f7-c05c-45ca-a29a-1f5ab7f095d5.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\96ec7bf2-a2f4-4e98-9966-7d1bee2b5c04.png" xlink:type="simple"/></inline-formula> the freestream air density and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\9938e734-8d21-4020-9b6c-2a57d65464dd.png" xlink:type="simple"/></inline-formula> is the median radius for each element. Based on thermodynamic relations the freestream pressure and velocity can be linked together using the following relations:</p><disp-formula id="scirp.45995-formula156"><label>(39)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\054c7fae-e54e-4062-a8bf-4c705e54453e.png"/></disp-formula><disp-formula id="scirp.45995-formula157"><label>(40)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\450324a0-f6a8-4f03-9e6a-2ebc9bd68dd0.png"/></disp-formula><p>The matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\4f3db961-9537-4f2d-890f-15e753f1fda0.png" xlink:type="simple"/></inline-formula> is given by:</p><disp-formula id="scirp.45995-formula158"><label>(41)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6258f4f7-690f-4c71-a727-dda697660759.png"/></disp-formula><p>The matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\82ff1665-28b1-4b83-9b8c-d2ec2d1303ed.png" xlink:type="simple"/></inline-formula> is given by:</p><disp-formula id="scirp.45995-formula159"><label>(42)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\336d2d19-f091-4966-90a9-f6c2329ecb0a.png"/></disp-formula><p>where matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\51cdc519-81f2-4c41-876e-a090a0346587.png" xlink:type="simple"/></inline-formula> is given by:</p><disp-formula id="scirp.45995-formula160"><label>(43)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\83cef7fd-57de-48b4-9a17-ee9fff171060.png"/></disp-formula><p>The general force vector due to a pressure field is written as:</p><disp-formula id="scirp.45995-formula161"><label>(44)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\e1646620-a383-4260-9150-276bab737f0e.png"/></disp-formula><p>The local damping matrix is given by:</p><disp-formula id="scirp.45995-formula162"><label>(45)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7f1749ff-53b9-4180-b852-b98e221f0c8a.png"/></disp-formula><p>Finally the local stiffness matrix is given by:</p><disp-formula id="scirp.45995-formula163"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\2513ffd7-94a0-4f02-8cb7-3c2ca96b1589.png"/></disp-formula><p>In the global system, the element damping and stiffness matrices are:</p><disp-formula id="scirp.45995-formula164"><label>(46)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\46ff6d81-b1b6-4341-ab5a-d2781af2a513.png"/></disp-formula><p>From these equations, one can assemble the damping and stiffness matrices for each element to obtain the damping and stiffness matrices for the whole shell: <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a9bb765a-0146-4f03-9cb6-ffdb31f28336.png" xlink:type="simple"/></inline-formula>and<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6a865d4f-b8bb-49c6-9c9c-e3e002043231.png" xlink:type="simple"/></inline-formula>.</p></sec><sec id="s2_3"><title>2.3. Fluid Modeling</title><p>The Laplace equation satisfied by velocity potential for inviscid, incompressible and irrotational fluid in the spherical system is written as:</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\438b09de-3fe1-4386-bb39-24fdeb3e8539.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\21cbb1b1-0031-4cf6-a734-ed735d0ad7ed.png" xlink:type="simple"/></inline-formula> (47)</p><p>where the velocity components are:</p><disp-formula id="scirp.45995-formula165"><label>(48)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f0d511e7-5040-4020-a938-3d899bf3da89.png"/></disp-formula><p>Using the Bernouilli equation, hydrodynamic pressure in terms of velocity potential <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\e2b44319-46a7-451f-9e08-6bf53b9655fc.png" xlink:type="simple"/></inline-formula> and fluid density <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\26a81ab2-3143-46fd-b782-7b8a909d6073.png" xlink:type="simple"/></inline-formula> is found as:</p><disp-formula id="scirp.45995-formula166"><label>(49)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\fd6accab-8715-475b-a2b1-65a6513a2675.png"/></disp-formula><p>The impermeability condition, which ensures contact between the shell surface and the peripheral fluid, is written as:</p><disp-formula id="scirp.45995-formula167"><label>(50)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\8ed4b0ba-f335-4d20-915e-eb9d032d5f8c.png"/></disp-formula><p>with</p><disp-formula id="scirp.45995-formula168"><label>(51)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ae1213f0-027b-437c-b961-7dab9bc9cf97.png"/></disp-formula><p>Method of separation of variables for the velocity potential solution can be done as follows:</p><disp-formula id="scirp.45995-formula169"><label>(52)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c6a021dc-eeaa-47c7-b49e-0b04df646a97.png"/></disp-formula><p>Placing this relation into the impermeability condition (50), we can find the function <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f1d60ee2-8e41-4515-a0ef-0acbcc0b9068.png" xlink:type="simple"/></inline-formula> in term of radial displacement:</p><disp-formula id="scirp.45995-formula170"><label>(53)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\39f9b3ff-ad30-4fb2-93f9-5ed0ae1875df.png"/></disp-formula><p>Hence the equation becomes</p><disp-formula id="scirp.45995-formula171"><label>(54)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ae3594b6-69ce-477b-983a-747ace526096.png"/></disp-formula><p>With substitution of the above equation into Laplace Equation (47), the following second order equation in terms of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\19e0ae97-37a3-493a-8657-4d914d3a5c2e.png" xlink:type="simple"/></inline-formula> is obtained</p><disp-formula id="scirp.45995-formula172"><label>(55)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\fc811847-e8a0-4a5a-8412-0e9fa68774d9.png"/></disp-formula><p>Solution of the above differential equation yields the following:</p><disp-formula id="scirp.45995-formula173"><label>(56)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f653bce3-ee0c-4220-8ad9-0b74f97aad2d.png"/></disp-formula><p>For internal flow <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\0c6d482d-bec2-4870-8578-015bb1764544.png" xlink:type="simple"/></inline-formula></p><p>Finally, the hydrodynamic pressure in terms of radial displacement is written:</p><disp-formula id="scirp.45995-formula174"><label>(57)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\761c5809-684b-430c-9dc3-a3ae82866431.png"/></disp-formula><p>We put:</p><disp-formula id="scirp.45995-formula175"><label>(58)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\737e3bcb-d702-4265-b55a-8e2ced184707.png"/></disp-formula><p>And the pressure loading in terms of nodal degrees of freedom is written as:</p><disp-formula id="scirp.45995-formula176"><label>(59)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\06e1a8b4-55e3-4a42-9e3b-319302c46cf9.png"/></disp-formula><p>where matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c14538b5-59f2-4f9f-851c-f9f1776ea227.png" xlink:type="simple"/></inline-formula> is given by:</p><disp-formula id="scirp.45995-formula177"><label>(60)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a1a97b4c-7328-4c66-a21f-42064ba382ab.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\42221247-e844-4048-aaf7-430d0ad2d334.png" xlink:type="simple"/></inline-formula> is expressed as:</p><disp-formula id="scirp.45995-formula178"><label>(61)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c5f12e6f-20f2-44f0-9f0c-22bdf6fce45d.png"/></disp-formula><p>The general force vector due the fluid pressure loading is given by:</p><disp-formula id="scirp.45995-formula179"><label>(62)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f4c943c1-a02d-42dc-90ab-0451c6207bf9.png"/></disp-formula><p>After substituting for pressure field vector and matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\773950f4-6521-4c4d-9cc1-4ab68686d1a6.png" xlink:type="simple"/></inline-formula> in the above equation, the local matrix <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f2949cf4-0824-4b15-9be4-093e813e0482.png" xlink:type="simple"/></inline-formula> can be found from the following:</p><disp-formula id="scirp.45995-formula180"><label>(63)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\3e5948f8-da20-4057-8809-3aa2110bae75.png"/></disp-formula><p>In the global system the element stiffness and mass matrices are</p><disp-formula id="scirp.45995-formula181"><label>(64)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\92ecaa6b-5171-446d-b981-6549ec3465fd.png"/></disp-formula><p>From these equations, one can assemble the mass for each element to obtain the mass matrix for the whole shell:<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\0b72e21e-da35-4d80-b35e-d7940114152a.png" xlink:type="simple"/></inline-formula>.</p><p>The governing equation which accounts for fluid-shell interaction in the presence external supersonic airflow is derived as:</p><disp-formula id="scirp.45995-formula182"><label>(65)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\e6080b45-dc2e-4c0a-b62a-1bd9e2650563.png"/></disp-formula><p>where subscripts s and f refer to shells in vacuo and fluid respectively.</p></sec></sec><sec id="s3"><title>3. Eigenvalue Problem</title><p>The global fluid matrices mentioned in Equation (65) may be obtained, respectively, by superimposing the mass, damping and stiffness matrices for each individual fluid finite element. After applying the boundary conditions the global matrices are reduced to square matrices of order 4*(N + 1) − J, where N is the number of finite elements in the shell and J is the number of constraints applied. Finally, the eigenvalue problem is solved by means of the equation reduction technique. Equation (65) may be rewritten as follows:</p><disp-formula id="scirp.45995-formula183"><label>(66)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\134a8910-7c41-43db-a35c-564671e60afc.png"/></disp-formula><p>where</p><disp-formula id="scirp.45995-formula184"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ba0dfbaf-6892-43bd-9f39-777cb8e50b11.png"/></disp-formula><disp-formula id="scirp.45995-formula185"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ba0dfbaf-6892-43bd-9f39-777cb8e50b11.png"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\5affd211-e70a-4db5-bb06-cba712ed289a.png" xlink:type="simple"/></inline-formula>is the global displacement vector. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\9ebb84f5-adf8-4dab-8c43-0ce3b7d04da0.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\72e31d5e-40da-428c-987d-5c10185d6459.png" xlink:type="simple"/></inline-formula> represent damping and elastic forces induced by the flowing fluid. <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\3a062223-6695-4a4b-ae2e-a020c9d90612.png" xlink:type="simple"/></inline-formula>is added fluid mass. The eigenvalue problem is given by:</p><disp-formula id="scirp.45995-formula186"><label>(67)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f13725e0-7ac5-49c7-81dc-43761d429dda.png"/></disp-formula><p>where</p><disp-formula id="scirp.45995-formula187"><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a1da9485-a95b-4992-b3e9-ee5019ee02d1.png"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6a1ddddf-29dc-49cf-88ea-3ecdbc90c1d1.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\ca883ffa-7b89-4359-a1b4-b9b0bd526e7b.png" xlink:type="simple"/></inline-formula> is the identity matrix.</p><p>An in house computer code based on the finite element method was developed as part of this work to establish the structural and fluid matrices of each element based on equations developed using the theoretical approach. The calculations for each finite element are performed in two stages: the first dealing with solid shell and the second with the effect of the flowing fluid. Aeroelastic stability will be examined by studying the eigenvalues in the complex plane. When the imaginary part of ω becomes negative the amplitude of the shell motion grows exponentially with time, thus indicating dynamic instability. The flutter boundary is obtained numerically by tracing the eigenvalues to see when the sign of imaginary part just changes from positive to negative. For the fixed value of circumferential wave number n, the onset of instability is determined by varying the value of freestream static pressure. This procedure is repeated for different values of n until the minimum critical pressure is obtained.</p></sec><sec id="s4"><title>4. Results and Discussion</title><p>In this section numerical results are presented and compared with existing experimental, analytical and numerical data.</p><sec id="s4_1"><title>4.1. Validation and Comparison</title><p>For the cases investigated in the present paper, the predicted dimensionless frequencies are expressed by the following relation:</p><disp-formula id="scirp.45995-formula188"><label>(68)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a41f0455-9be4-4944-8527-962b0f8020d9.png"/></disp-formula><p>where:</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7514560c-12ea-4c5d-a9ba-390a7a8545cf.png" xlink:type="simple"/></inline-formula>is the natural angular frequency,</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\26171589-7a7e-4db5-9ea2-d2e65fe14705.png" xlink:type="simple"/></inline-formula>is the radius of the reference surface,</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\c11bba95-e1e4-4de3-a6a7-97a0ff84bfdd.png" xlink:type="simple"/></inline-formula>is the density, and</p><p><inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\4d30e3b7-b2f5-4a40-91a9-9599901a1d3b.png" xlink:type="simple"/></inline-formula>is the modulus of elasticity.</p><p>Results for different boundary conditions, geometries, flow parameters and radius to thickness ratios compared to experimental, theoretical and numerical analyses are presented (see <xref ref-type="fig" rid="fig4">Figure 4</xref>).</p><sec id="s4_1_1"><title>4.1.1. Spherical Shells in Vacuo</title><p>Case 1: clamped spherical shell with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\e0e4c9fc-125e-475f-b1ca-d4fb28735316.png" xlink:type="simple"/></inline-formula> = 10˚</p><p>Narassihan and Alwar [<xref ref-type="bibr" rid="scirp.45995-ref23">23</xref>] investigated the case of an axisymmetric clamped spherical shell. The analysis is based on the application of the Chebyshev-Galerkin spectral method for the evaluation of free vibration frequencies and mode shapes. Sai Ram and Sreedhar Babu [<xref ref-type="bibr" rid="scirp.45995-ref24">24</xref>] analyzed the same case with the classical finite element method using 80 elements. Each element is an eight nodded degenerated is oparametric shell element with nine degrees of freedom at each node. With our model and using 6 finite elements, the natural frequencies were computed; the results are shown in <xref ref-type="table" rid="table1">Table 1</xref>.</p><p>Case 2: clamped spherical shell with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a92bc5e2-0c33-422d-bf11-8355e804c37f.png" xlink:type="simple"/></inline-formula> = 30˚</p><p>This case was investigated analytically by Kalnins [<xref ref-type="bibr" rid="scirp.45995-ref25">25</xref>] using classical theory and transverse vibration theory. With our theory, we used 8 finite elements to study the spherical shell with the results shown in <xref ref-type="table" rid="table2">Table 2</xref>. The frequencies we obtained with our model are very comparable to Kalinin’s values.</p><p>Case 3: spherical shell with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\2643be49-a467-4ca1-a209-5eea2137e5ed.png" xlink:type="simple"/></inline-formula> = 60˚ under two boundary conditions: clamped, simply supported</p><fig id="fig4"><label>Figure 4</label><caption><p> Definition of angle<img src="htmlimages\4-1100314x\d16ee270-0e69-46cc-bcaa-640483a70c68.png" width="23.2500004768372" height="37.5" /></p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\e489ef3b-20b3-4d11-bb11-80ec5de50c7e.png"/></fig><table-wrap id="table1"  position="float"><object-id pub-id-type="pii">Table 1</object-id><label>Table 1</label><caption><p>. Normalized natural frequencies for 10˚ clamped spherical shell with R/h = 200</p></caption><table><thead><tr><th align="center" valign="middle" >Mode</th><th align="center" valign="middle" >Present theory</th><th align="center" valign="middle"  colspan="2"  >Sai Ram and Sreedhar babu [23] </th><th align="center" valign="middle" >Narassihan and Alwar [24] </th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle"  colspan="2"  >1.4861</td><td align="center" valign="middle" >1.4577</td><td align="center" valign="middle" >1.4588</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle"  colspan="2"  >2.2498</td><td align="center" valign="middle" >2.2931</td><td align="center" valign="middle" >2.2999</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle"  colspan="2"  >4.4779</td><td align="center" valign="middle" >4.5773</td><td align="center" valign="middle" >4.5461</td></tr><tr><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td><td align="center" valign="middle" ></td></tr></tbody></table></table-wrap><table-wrap id="table2"  position="float"><object-id pub-id-type="pii">Table 2</object-id><label>Table 2</label><caption><p>. Normalized natural frequencies for 30˚ clamped spherical shell with R/h = 20</p></caption><table><thead><tr><th align="center" valign="middle" >Mode</th><th align="center" valign="middle" >Presenttheory</th><th align="center" valign="middle" >Kalnins [25] </th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1.169</td><td align="center" valign="middle" >1.168</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >2.224</td><td align="center" valign="middle" >2.589</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >3.303</td><td align="center" valign="middle" >3.230</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >4.200</td><td align="center" valign="middle" >4.288</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >4.923</td><td align="center" valign="middle" >4.683</td></tr></tbody></table></table-wrap><p>Free axisymmetric vibration of the spherical shell in this case was studied by Kalnins [<xref ref-type="bibr" rid="scirp.45995-ref26">26</xref>] , Cohen [<xref ref-type="bibr" rid="scirp.45995-ref27">27</xref>] , Navaratna [<xref ref-type="bibr" rid="scirp.45995-ref28">28</xref>] , Webster [<xref ref-type="bibr" rid="scirp.45995-ref29">29</xref>] , Greene et al. [<xref ref-type="bibr" rid="scirp.45995-ref30">30</xref>] , Tessler and Spiridigliozzi [<xref ref-type="bibr" rid="scirp.45995-ref31">31</xref>] , Gautham and Ganesan [<xref ref-type="bibr" rid="scirp.45995-ref32">32</xref>] and Buchanan and Rich [<xref ref-type="bibr" rid="scirp.45995-ref33">33</xref>] . In the present investigation, the shell was investigated with 10 elements; the results are given respectively for clamped, simply supported hemispherical shells in <xref ref-type="table" rid="table3">Table 3</xref> and <xref ref-type="table" rid="table4">Table 4</xref>.</p><p>Case 4: spherical shell with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\1b1a82c5-905a-4215-a8b4-ec96175f0b00.png" xlink:type="simple"/></inline-formula> = 90˚</p><p>Kraus [<xref ref-type="bibr" rid="scirp.45995-ref22">22</xref>] investigated the case of simply supported spherical shell using a general theory, which included the effects of transverse shear stress and rotational inertia. For cases both with and without these effects, he determined the natural frequencies for the shell motion that was independent of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\09328be1-c596-481b-8038-fa310fa6ff08.png" xlink:type="simple"/></inline-formula> for circumferential mode number<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7c065f88-0cc3-465a-a698-0be0c36effc9.png" xlink:type="simple"/></inline-formula>. Tessler and Spiridigliozzi [<xref ref-type="bibr" rid="scirp.45995-ref31">31</xref>] , Gautham and Ganesan [<xref ref-type="bibr" rid="scirp.45995-ref34">34</xref>] analyzed the case of clamped hemispherical shell. Ventsel et al. [<xref ref-type="bibr" rid="scirp.45995-ref35">35</xref>] studied the case of simply supported spherical shell using the boundary elements method for various circumferential mode numbers<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a55046be-faf2-46a5-a8d7-8a68a0f25119.png" xlink:type="simple"/></inline-formula>. With our model and using 12 finite elements, the natural frequencies were computed for clamped and simply supported shells. The results are shown respectively in <xref ref-type="table" rid="table5">Table 5</xref> and <xref ref-type="table" rid="table6">Table 6</xref>.</p></sec><sec id="s4_1_2"><title>4.1.2. Flutter of Spherical Shells</title><p>The problem treated for validation is the flutter boundary of a simply–supported spherical shell subjected to external supersonic airflow. As there is no information available for flutter of spherical shells, this case has been compared with simply-supported cone studied by various authors. The conical shell has the following data: Young’s Modulus, E = 6.5 106 lb-in-2, Poisson’s ratio, ν = 0.29, material mass density, ρ = 8.33 10-4 lb-s2-in-4, shell thickness, h = 0.051 in, cone semi-vertex angle α = 5˚. The supersonic airflow has freestream Mach number, M∞ = 3, stagnation temperature, T∞ = 288.15 K. The results are shown in <xref ref-type="table" rid="table7">Table 7</xref> where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\f7b83a3c-ea78-477e-83b3-7fef94beab49.png" xlink:type="simple"/></inline-formula> is the dynamic pressure parameter defined as:</p><disp-formula id="scirp.45995-formula189"><label>(69)</label><inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\590372f1-ebbd-4d6b-9ce6-2eff07f2c996.png"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6ba6f02f-94cf-4846-955b-66ac4958de15.png" xlink:type="simple"/></inline-formula> is the bending stiffness.</p><p>When results are summarized and compared with other finite element and analytical solutions, this method shows good convergence using only 15 elements with small disagreements. It should be noted that the previous analytical methods [<xref ref-type="bibr" rid="scirp.45995-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.45995-ref15">15</xref>] use Donnel-Mushtari simplified shell theory while [<xref ref-type="bibr" rid="scirp.45995-ref14">14</xref>] uses Novozhilov’s thin shell with the different method of application of finite element solution. On the other hand, a complete form of the linear piston theory is used by [<xref ref-type="bibr" rid="scirp.45995-ref21">21</xref>] as in the present study and the results are very close; but the expression used by Dixon and Hudson [<xref ref-type="bibr" rid="scirp.45995-ref15">15</xref>] , Ueda et al. [<xref ref-type="bibr" rid="scirp.45995-ref14">14</xref>] for the piston theory does not have a curvature term which has caused greater differences in the results.</p></sec></sec><sec id="s4_2"><title>4.2. Flutter Boundary</title><p>Flutter which is observed in all the papers using piston theory is a coupled-mode flutter. Indeed, let us consider motion of the shell eigenvalues in the complex ω plane. If the freestream pressure is not very high, and the shell is stable, all complex frequencies are located in the top ω half-plane. Let us now increase freestream pressure. The first and the second complex frequencies move toward each other, almost merge, and then go away from</p><table-wrap id="table3"  position="float"><object-id pub-id-type="pii">Table 3</object-id><label>Table 3</label><caption><p>. Normalized natural frequencies for 60˚ clamped spherical shell with R/h = 20</p></caption><table><thead><tr><th align="center" valign="middle" >Mode</th><th align="center" valign="middle" >Kalnins [26] </th><th align="center" valign="middle" >Navaratna [28] </th><th align="center" valign="middle" >Webster [29] </th><th align="center" valign="middle" >Tessler and Spiridigliozzi [31] </th><th align="center" valign="middle" >Gautham and Ganesan [32] </th><th align="center" valign="middle" >Buchanan and Rich [33] </th><th align="center" valign="middle" >Present theory</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >1.006</td><td align="center" valign="middle" >1.008</td><td align="center" valign="middle" >1.007</td><td align="center" valign="middle" >1.000</td><td align="center" valign="middle" >1.001</td><td align="center" valign="middle" >1.001</td><td align="center" valign="middle" >1.031</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >1.391</td><td align="center" valign="middle" >1.395</td><td align="center" valign="middle" >1.391</td><td align="center" valign="middle" >1.368</td><td align="center" valign="middle" >1.373</td><td align="center" valign="middle" >1.370</td><td align="center" valign="middle" >1.496</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.702</td><td align="center" valign="middle" >1.700</td><td align="center" valign="middle" >1.673</td><td align="center" valign="middle" >1.678</td><td align="center" valign="middle" >1.675</td><td align="center" valign="middle" >1.760</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.126</td><td align="center" valign="middle" >2.095</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.094</td><td align="center" valign="middle" >2.089</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >2.375</td><td align="center" valign="middle" >2.387</td><td align="center" valign="middle" >2.386</td><td align="center" valign="middle" >2.260</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.256</td><td align="center" valign="middle" >2.276</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >3.486</td><td align="center" valign="middle" >3.506</td><td align="center" valign="middle" >3.851</td><td align="center" valign="middle" >3.213</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >3.209</td><td align="center" valign="middle" >3.311</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >3.991</td><td align="center" valign="middle" >3.996</td><td align="center" valign="middle" >4.062</td><td align="center" valign="middle" >3.965</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >3.964</td><td align="center" valign="middle" >3.775</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.159</td><td align="center" valign="middle" >4.151</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.060</td><td align="center" valign="middle" >4.073</td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >4.947</td><td align="center" valign="middle" >5.001</td><td align="center" valign="middle" >5.962</td><td align="center" valign="middle" >4.442</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.427</td><td align="center" valign="middle" >4.826</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >6.037</td><td align="center" valign="middle" >6.208</td><td align="center" valign="middle" >5.773</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >5.740</td><td align="center" valign="middle" >5.777</td></tr></tbody></table></table-wrap><table-wrap id="table4"  position="float"><object-id pub-id-type="pii">Table 4</object-id><label>Table 4</label><caption><p>. Normalized natural frequencies for 60˚ simply supported spherical shell with R/h = 20</p></caption><table><thead><tr><th align="center" valign="middle" >Mode</th><th align="center" valign="middle" >Kalnins [26] </th><th align="center" valign="middle" >Navaratna [28] </th><th align="center" valign="middle" >Greene et al. [30] </th><th align="center" valign="middle" >Cohen [27] </th><th align="center" valign="middle" >Gautham and Ganesan [32] </th><th align="center" valign="middle" >Buchanan and Rich [33] </th><th align="center" valign="middle" >Present theory</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.962</td><td align="center" valign="middle" >0.963</td><td align="center" valign="middle" >0.974</td><td align="center" valign="middle" >0.959</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >0.956</td><td align="center" valign="middle" >0.981</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >1.334</td><td align="center" valign="middle" >1.338</td><td align="center" valign="middle" >1.338</td><td align="center" valign="middle" >1.325</td><td align="center" valign="middle" >1.315</td><td align="center" valign="middle" >1.308</td><td align="center" valign="middle" >1.412</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.653</td><td align="center" valign="middle" >1.652</td><td align="center" valign="middle" >1.646</td><td align="center" valign="middle" >1.639</td><td align="center" valign="middle" >1.612</td><td align="center" valign="middle" >1.646</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >2.128</td><td align="center" valign="middle" >2.131</td><td align="center" valign="middle" >2.162</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.044</td><td align="center" valign="middle" >2.038</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.141</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.059</td><td align="center" valign="middle" >2.115</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >3.176</td><td align="center" valign="middle" >3.185</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >2.965</td><td align="center" valign="middle" >2.934</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >3.988</td><td align="center" valign="middle" >3.933</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >3.837</td><td align="center" valign="middle" >3.871</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.159</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.000</td><td align="center" valign="middle" >4.017</td></tr><tr><td align="center" valign="middle" >9</td><td align="center" valign="middle" >4.575</td><td align="center" valign="middle" >4.601</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >4.148</td><td align="center" valign="middle" >4.138</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >6.031</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >5.608</td><td align="center" valign="middle" >5.773</td></tr></tbody></table></table-wrap><table-wrap id="table5"  position="float"><object-id pub-id-type="pii">Table 5</object-id><label>Table 5</label><caption><p>. Normalized natural frequencies for 90˚ clamped spherical shell with R/h = 10</p></caption><table><thead><tr><th align="center" valign="middle" >Mode</th><th align="center" valign="middle" >Tessler and Spiridigliozzi [31] </th><th align="center" valign="middle" >Gautham and Ganesan [34] </th><th align="center" valign="middle" >Present theory</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.8481</td><td align="center" valign="middle" >0.8439</td><td align="center" valign="middle" >0.8327</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >1.2328</td><td align="center" valign="middle" >1.2317</td><td align="center" valign="middle" >1.1919</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >1.5902</td><td align="center" valign="middle" >1.5808</td><td align="center" valign="middle" >1.5041</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >1.9435</td><td align="center" valign="middle" >1.9267</td><td align="center" valign="middle" >1.9161</td></tr></tbody></table></table-wrap><p>each other in vertical directions (<xref ref-type="fig" rid="fig5">Figure 5</xref>). Thus, interaction of two modes occurs. Physically this interaction of the shell modes happens through the effect of the air flow.</p><p>A simply supported spherical shell with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\962c740a-d21c-4800-9320-8b3e410b98a5.png" xlink:type="simple"/></inline-formula> = 30˚ is treated here. The complex frequencies only for the first and second modes versus freestream dynamic pressure are plotted in <xref ref-type="fig" rid="fig6">Figure 6</xref>. Aerodynamic pressure is evaluated using Equation (36). In <xref ref-type="fig" rid="fig6">Figure 6</xref>(a) the real part of the complex frequency increases for the first mode while for the second mode it decreases as the freestream dynamic pressure parameter <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\52643f10-6602-40ba-8a36-d794faf18038.png" xlink:type="simple"/></inline-formula> increases. For higher</p><table-wrap id="table6"  position="float"><object-id pub-id-type="pii">Table 6</object-id><label>Table 6</label><caption><p>. Normalized natural frequencies for 90˚ simply supported spherical shell</p></caption><table><thead><tr><th align="center" valign="middle" >Mode</th><th align="center" valign="middle" >Kraus [22] R/h = 10</th><th align="center" valign="middle" >Kraus [22]  R/h = 50</th><th align="center" valign="middle" >Ventsel et al. [35]  R/h = 200</th><th align="center" valign="middle" >Present theory R/h = 50</th></tr></thead><tbody><tr><td align="center" valign="middle" >1</td><td align="center" valign="middle" >0.8060</td><td align="center" valign="middle" >0.7548</td><td align="center" valign="middle" >0.7441</td><td align="center" valign="middle" >0.7579</td></tr><tr><td align="center" valign="middle" >2</td><td align="center" valign="middle" >1.2054</td><td align="center" valign="middle" >0.9432</td><td align="center" valign="middle" >0.9281</td><td align="center" valign="middle" >0.9034</td></tr><tr><td align="center" valign="middle" >3</td><td align="center" valign="middle" >1.6179</td><td align="center" valign="middle" >1.0152</td><td align="center" valign="middle" >0.9693</td><td align="center" valign="middle" >0.9499</td></tr><tr><td align="center" valign="middle" >4</td><td align="center" valign="middle" >1.9051</td><td align="center" valign="middle" >1.1082</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.1089</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >2.7205</td><td align="center" valign="middle" >1.2523</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.2759</td></tr><tr><td align="center" valign="middle" >6</td><td align="center" valign="middle" >2.9301</td><td align="center" valign="middle" >1.4576</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.4723</td></tr><tr><td align="center" valign="middle" >7</td><td align="center" valign="middle" >4.0274</td><td align="center" valign="middle" >1.6558</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.6237</td></tr><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >5.5142</td><td align="center" valign="middle" >1.7636</td><td align="center" valign="middle" >-</td><td align="center" valign="middle" >1.7634</td></tr></tbody></table></table-wrap><table-wrap id="table7"  position="float"><object-id pub-id-type="pii">Table 7</object-id><label>Table 7</label><caption><p>. Comparison of critical dynamical pressure parameter (simply supported case)</p></caption><table><thead><tr><th align="center" valign="middle" >Present</th><th align="center" valign="middle" >Dixon and Hudson [15] </th><th align="center" valign="middle" >Udea et al. [14] </th><th align="center" valign="middle" >Pidaparti and Yang Henri [21] </th><th align="center" valign="middle" >Shulman [13] </th><th align="center" valign="middle" >Bismark-Nasr [17] </th></tr></thead><tbody><tr><td align="center" valign="middle" >520(5)<sup>a</sup></td><td align="center" valign="middle" >590(5)</td><td align="center" valign="middle" >609(5)</td><td align="center" valign="middle" >576(5)</td><td align="center" valign="middle" >669(6)</td><td align="center" valign="middle" >702(6)</td></tr></tbody></table></table-wrap><fig id="fig5"><label>Figure 5</label><caption><p> Trajectories of the complex frequencies loci in the complex ω plane during the changing of the dynamic pressure</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\14cbdb2d-2560-41ce-bb04-8a34049a71b9.png"/></fig><p>values of dynamic pressure these real parts, representing the oscillation frequency, eventually coalesce into a single mode. Further increasing the dynamic pressure of the flow causes the shell to lose its stability at <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\0327e29b-1047-4ff2-bec6-0c464f4f1c5f.png" xlink:type="simple"/></inline-formula><sub>cr</sub> = 410. This instability is due to coupled-mode flutter where the imaginary part of complex frequency (representing the damping term of the aeroelastic system) becomes zero for certain critical pressure (<xref ref-type="fig" rid="fig6">Figure 6</xref>(b)).</p><p>The same behaviour is observed by real and imaginary parts of complex frequencies as the static pressure increases (<xref ref-type="fig" rid="fig7">Figure 7</xref>) but the onset of flutter is at <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7e089997-4eac-47c9-9b1c-fec93789a238.png" xlink:type="simple"/></inline-formula><sub>cr</sub> = 410 if the freestream static pressure is evaluated using Equation (37). Prediction of the critical freestream static pressure using Equation (36) provides approximately the same results when evaluating the pressure field using Equation (37). As expected, using the piston theory with the correction term to account for shell curvature produces a better approximation for the pressure loading acting on a curved shell exposed to supersonic flow.</p><p>In <xref ref-type="fig" rid="fig8">Figure 8</xref> the onset of flutter for different angles is plotted. By increasing the angle<inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\8ecb06ae-beb9-4502-963e-a1175296868b.png" xlink:type="simple"/></inline-formula>, flutter instability occurs at lower pressure. This decrease in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\0ae2b448-e5b0-45f5-aa4d-f2f61748afa3.png" xlink:type="simple"/></inline-formula><sub>cr</sub> with <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\eb289e36-6b9c-4695-85df-2a4fbcb2407a.png" xlink:type="simple"/></inline-formula> is attributed to the fact that the natural frequencies always decrease as the angle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\54e51ba3-6fd6-4146-a8c1-c8c0f0c8da80.png" xlink:type="simple"/></inline-formula> is increased.</p><p>The effect of radius to thickness ratio R/h is presented in <xref ref-type="fig" rid="fig9">Figure 9</xref>. This figure shows an increase of <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\60b4d378-b816-4e50-baa9-b77c25bd292d.png" xlink:type="simple"/></inline-formula><sub>cr</sub> with an increase of radius to thickness ratio. This increase in <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\43bd874b-9f16-4a84-8467-8b08c3046050.png" xlink:type="simple"/></inline-formula><sub>cr</sub> is attributed to the fact that the mass of shell is greater when the shell is thick, and the effect of pressure is less important for a thick shell than for a thin shell. On the other hand, when the shell is thin it becomes unstable at higher dynamical pressure levels due to an increase in stiffness because of a decrease in thickness. The same conclusion is reported in [<xref ref-type="bibr" rid="scirp.45995-ref12">12</xref>] for the flutter of</p><fig-group id="fig6"><caption><title>Figure 6</title><p> (a) Real part and (b) imaginary part of the complex frequencies versus the freestream static pressure parameter; static pressure evaluated by Equation (36)</p></caption><fig id ="fig6_1"><label>(a)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\cdcbe8ed-e557-46c3-bea5-cd78cbe1cff0.png"/></fig><fig id ="fig6_2"><label>(b)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\48e87665-83b5-457b-86ee-bff503b7616e.png"/></fig></fig-group><p>cylindrical shells.</p><p>In order to study the effect of filling ratio, <xref ref-type="fig" rid="fig10">Figure 10</xref> shows the critical value of freestream static pressure for different filling ratios, H/R. Shell geometry and flow parameters are the same as the previous case study with liquid filled density ρf =9.355 &#215; 10-5lb s2 in-4. It is seen that the value of critical dynamic pressure parameter decreases as the filling ratio increases from a low value. This rapid change in critical dynamic pressure at low filling ratios and its almost steady behaviour at large filling ratios indicates that the fluid near the bottom of the shell is largely influenced by elastic deformation when a shell is subjected to external supersonic flow.</p><p>The effect of boundary conditions on the flutter onset is presented in <xref ref-type="table" rid="table8">Table 8</xref>. It is seen that for freely simply supported ends, v = w = 0, flutter onset occurs at <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\7199ba46-2218-45d7-8f46-63c4433bc525.png" xlink:type="simple"/></inline-formula> = 510.5 which indicates more flutter resistance compared to simply supported or clamped ends. It is indicated that there is no difference for flutter onset when the shell is either clamped or simply supported. We obtained the same results in the conical shells subjected to supersonic flow.</p></sec></sec><sec id="s5"><title>5. Conclusion</title><p>An efficient hybrid finite element method is presented to investigate the aeroelastic stability of an empty or partially liquid filled spherical shell subjected to external supersonic flow. Linear shell theory is coupled with first order piston theory to account for aerodynamic pressure. The effect of curvature correction in piston theory was</p><fig-group id="fig7"><caption><title>Figure 7</title><p> (a) Real part and (b) imaginary part of the complex frequencies versus the freestream static pressure parameter; static pressure evaluated by Equation (37)</p></caption><fig id ="fig7_1"><label>(a)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\285d78f0-e5fb-47eb-ab1f-acca4ec14762.png"/></fig><fig id ="fig7_2"><label>(b)</label><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\47f23510-e0fd-4a30-90e8-3596021e7518.png"/></fig></fig-group><fig id="fig8"><label>Figure 8</label><caption><p> Variation of the critical freestream static pressure parameter with angle <img src="htmlimages\4-1100314x\83dc707e-688a-47be-bba6-69edd99d2632.png" width="23.2500004768372" height="37.5" /> for simply supported shell</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\6fc05cc7-a7d3-46a6-a196-88a92c29fac2.png"/></fig><table-wrap id="table8"  position="float"><object-id pub-id-type="pii">Table 8</object-id><label>Table 8</label><caption><p>. Critical freestream pressure parameter for different boundary conditions</p></caption><table><thead><tr><th align="center" valign="middle" >Boundary conditions</th><th align="center" valign="middle" ></th><th align="center" valign="middle" >Mode no.</th></tr></thead><tbody><tr><td align="center" valign="middle" >Freely simply supported (v = w = 0)</td><td align="center" valign="middle" >510.5</td><td align="center" valign="middle" >Coupled 1<sup>st</sup> and 2<sup>nd</sup></td></tr><tr><td align="center" valign="middle" >Simply supported (u = v = w = 0)</td><td align="center" valign="middle" >410</td><td align="center" valign="middle" >Coupled 1<sup>st</sup> and 2<sup>nd</sup></td></tr><tr><td align="center" valign="middle" >Clamped</td><td align="center" valign="middle" >410</td><td align="center" valign="middle" >Coupled 1<sup>st</sup> and 2<sup>nd</sup></td></tr></tbody></table></table-wrap><fig id="fig9"><label>Figure 9</label><caption><p> Variation of the critical freestream static pressure parameter with R/h for simply supported shell</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\84691daf-47f6-4503-945a-9edf3b2fb79a.png"/></fig><fig id="fig10"><label>Figure 10</label><caption><p> Variation of the critical freestream static pressure parameter with R/H for simply supported shell</p></caption><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\a6d4577d-afad-40e2-af09-75f94b6fd2ae.png"/></fig><p>analyzed. Fluid structure interaction due to hydrodynamic pressure of internal fluid is also taken into account. The study has been done for shells with various geometries, radius to thickness ratios, filling ratios and boundary conditions. In all study cases one type of instability is found; coupled-mode flutter in the first and second mode. Increasing the radius to thickness ratio leads the onset of flutter to occur at higher dynamic pressure. Decreasing the angle <inline-formula><inline-graphic xlink:href="http://file.scirp.org/Html/htmlimages\4-1100314x\4d141897-2461-49fd-8d97-e7dfea886561.png" xlink:type="simple"/></inline-formula> of the spherical shell causes the flutter boundary to occur at lower dynamic pressure. A lower filling ratio has more flutter resistance than a higher filling ratio. 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