Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank

Lukovsky’s asymptotic formulas for the resulting hydrodynamic force and moment are derived as if they follow from the adaptive (infinite- dimensional) multimodal theory of the liquid sloshing dynamics in an upright circular base container. The result is given in a tensor form in- troduced in nota...

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Datum:2020
Hauptverfasser: Тимоха, О.М., Тимоха, А.Н., Timokha, A.N.
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Sprache:Englisch
Veröffentlicht: Інститут математики НАН України 2020
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Transactions of Institute of Mathematics of NAS of Ukraine
_version_ 1872552921205309440
author Тимоха, О.М.
Тимоха, А.Н.
Timokha, A.N.
author_facet Тимоха, О.М.
Тимоха, А.Н.
Timokha, A.N.
author_institution_txt_mv [ { "author": "О.М. Тимоха", "institution": "Institute of Mathematics" } ]
author_sort Тимоха, О.М.
baseUrl_str https://trim.imath.kiev.ua/index.php/trim/oai
collection OJS
datestamp_date 2020-08-09T15:01:39Z
description Lukovsky’s asymptotic formulas for the resulting hydrodynamic force and moment are derived as if they follow from the adaptive (infinite- dimensional) multimodal theory of the liquid sloshing dynamics in an upright circular base container. The result is given in a tensor form in- troduced in notations of the original paper by Faltinsen, Lukovsky and Timokha (2016).
first_indexed 2026-08-04T01:07:07Z
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fulltext Збiрник праць Iнституту математики НАН України 2019, т. 16, № 2, 188–208 УДК 532.595 Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank⇤ A.N. Timokha 1,2 1 Institute of Mathematics of the NAS of Ukraine, Kyiv; 2 Centre for Autonomous Marine Operations and Systems, NTNU, Trondheim, Norway; atimokha@gmail.com Lukovsky’s asymptotic formulas for the resulting hydrodynamic force and moment are derived as if they follow from the adaptive (infinite- dimensional) multimodal theory of the liquid sloshing dynamics in an upright circular base container. The result is given in a tensor form in- troduced in notations of the original paper by Faltinsen, Lukovsky and Timokha (2016). Виводяться формули Луковського адаптивного асимптотичного типу для результуючих гiдродинамiчної сили й моменту, що пов’язуються з коливаннями рiдини у вертикальному круговому бацi. Результат пред- ставлено в термiнах позначень iз оригiнальної роботи Фалтiнсена, Лу- ковського й Тимохи (2016). Introduction Linear and weakly-nonlinear and fully-nonlinear multimodal theories are common for studying the liquid sloshing dynamics in an upright circular cylindrical tank performing a small-amplitude three-dimensional oscilla- tory motion. The theories reduce the original free-boundary problem to di↵erent kinds of (modal) systems of ordinary di↵erential equations ⇤The work was partly supported by the Grant № 0112U001015. The author acknowledges the financial support of the Centre of Autonomous Marine Operati- ons and Systems (AMOS) whose main sponsor is the Norwegian Research Council (Project number 223254–AMOS). c� Timokha A. N., 2019 Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 189 with respect to the hydrodynamic generalised coordinates – the time- dependent coe�cients in a Fourier–type (functional) presentation of the free surface. By getting either transient (solving the Cauchy problem) or steady-state wave (time-periodic condition) solution of the modal sys- tems makes it possible, using the aforementioned Fourier representation, to describe the free-surface elevation as well as the velocity and pressure fields. Furthermore, substituting this modal solution (the hydrodynamic generalised coordinates) into the so-called Lukovsky’s formulas [1, 4, 5] gives the resulting hydrodynamic force and moment due to the pressure load on the wetted tank surface. I.A. Lukovsky derived his formulas in the most general, fully-nonlinear form. The formulas had to equip the so-called Miles-Lukovsky modal theory [1, 4, 5], which is fully-nonlinear and, therefore, mathematically equivalent to the original free-surface sloshing problem. However, the Miles-Lukovsky theory is of a rather abstract nature so that its usage is disputable to e↵ectively conduct numerical simulations and/or make an- alytical studies. This was in many details discussed in reviews [1, 6]. To facilitate analytical studies of the resonant nonlinear sloshing, the theory had to be simplified to a weakly-nonlinear form. The simplification in- cludes an analytical (asymptotic) reduction of both the governing (modal) equations, which couple the hydrodynamic generalised coordinates, and the Lukovsky formulas for the hydrodynamic force and moment. A re- quirement consists of postulating a series of specific asymptotic relations between the non-dimensional forcing magnitude (implies the higher-order asymptotic scale) and the hydrodynamic generalised coordinates, which, because some of them are resonantly excited, are characterised by a lower asymptotic order. The procedure needs neglecting the higher asymp- totic quantities than the non-dimensional forcing magnitude; it leads to weakly-nonlinear modal equations and Lukovsky’s formulas. In the most general case, the aforementioned asymptotic relations take the so-called adaptive form. Recently, an adaptive infinite-dimensional asymptotic modal system was derived in [2] to describe the resonant liquid sloshing in an up- right circular base container. The adaptive intermodal asymptotic or- dering assumes then that all the hydrodynamic generalised coordinates have the same asymptotic order O(✏1/3) where O(✏) ⌧ 1 measures the non-dimensional forcing magnitude. The present paper equips [2] with the corresponding adaptive Lukovsky formulas, which were not derived in the original and forthcoming [3] papers based on the adaptive and 190 Timokha A. N. Narimanov-Moiseev–type multimodal asymptotic ordering. 1 Non-dimensional modal solution We consider the liquid sloshing dynamics in an upright circular rigid tank performing a small-magnitude almost periodic three-dimensional motion with the circular frequency �. The sloshing is analysed in the non- dimensional statement suggesting the tank radius R0 is the characteristic size and T = 2⇡/� is the characteristic time. The time-dependent liquid domain Q(t) is confined by the free sur- face ⌃(t) and the wetted tank surface S(t). The free-surface elevations are considered in the tank-fixed coordinate system Oxyz whose coordi- nate plane Oxy coincides with the mean free surface ⌃0 and Oz is the symmetry axis. The small-magnitude tank motions are governed by the time-dependent vectors vO(t) = (⌘̇1, ⌘̇2, ⌘̇3) and !(t) = (⌘̇4, ⌘̇5, ⌘̇6), which describe the non-dimensional translatory and instant angular velocities of the tank, respectively, and the generalised coordinates ⌘i(t) = O(✏) ⌧ 1, i = 1, ...6 determine the three-dimensional body motions. The adaptive asymptotic modal method introduces the modal (Fourier) representation of the free surface ⇣(r, ✓, t) = X Mi RMi(r) cos(M✓) pMi(t) + X mi Rmi(r) sin(m✓) rmi(t), (1) where RMi(r) = ↵MiJM (kMir) with the Bessel function of the first kind, kMi, i � 1 are the roots of J 0 M (kMi) = 0, and pMi(t) ⇠ rMi(t) = O(✏1/3) are the hydrodynamic generalised coordinates. The normalising multipli- ers ↵Mi are required to provide the identity Z 1 0 rR2 Mi(r) dr = 1 ) ↵2 Mi = 2kMi J2 M (kMi)(k2Mi �M2) . (2) Here and thereafter, the large summation indices imply summation from zero to infinity but small indices mean change from one to infinity. The adaptive asymptotic modal theory neglects the o(✏)-terms in the governing equations and all other hydrodynamic characteristics. A result in [2] is a weakly-nonlinear infinite-dimensional system of ordinary dif- ferential equations with respect to pMi and rMi whose right-hand site is a linear vector-function with respect to ⌘i and their time derivatives. Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 191 The forthcoming derivations adopt notations from [2]. This includes tensors in Appendix A and several shortcuts, e.g., Lk = kLk tanh(kLkh), ZLk(z) = cosh(kLk(z + h)) kLk sinh(kLkh) (3) where h is the non-dimensional liquid depth. 2 Hydrodynamic force Adopting the asymptotic modal solution (1) and the original Lukovsky formula for the dimensional hydrodynamic force F (t) from, e.g., [1, 4], one can write down F (t) = ⇥ MlR0� 2 ⇤ � g � v̇O �! ⇥ vO �! ⇥ (! ⇥ rlC)� !̇ ⇥ rlC � r̈lC � 2! ⇥ ṙlC � = ⇥ MlR0� 2 ⇤ � g � v̇O � !̇ ⇥ rlC0 � r̈lC + o(✏) � = ⇥ MlR0� 2 ⇤ � F1(t) e1(t) + F2(t) e2(t) + F3(t) e3(t) + o(✏) � , (4) where the dot means the time derivative in the Oxyz coordinates, ȧ(t) = ȧ1(t) e1(t) + ȧ2(t) e2(t) + ȧ3(t) e3(t) (ei(t), i = 1, 2, 3 are the coordinate units of the body-fixed coordinate system Oxyz), Ml is the liquid mass, g is the non-dimensional gravity vector in the body-fixed coordinate system whose linear (= O(✏)) com- ponents take the form g = g⌘5e1 � g⌘4e2 � ge3, g0 = �ge3 = O(1); (5) and rlC = 1 ⇡h " e1 Z Q(t) xdQ+ e2 Z Q(t) ydQ+ e3 Z Q(t) zdQ # = rlC0 + rlCs = e1 1 h X i Pip1i(t) ! + e2 1 h X i Pir1i(t) ! + e3 0 @� h 2 + 1 h X i p20i + 1 2h X m,i (p2mi + r2mi) 1 A , (6a) 192 Timokha A. N. rlC0 = � 1 2he3, rlCs = r1lCse1 + r2lCse2 + r3lCse3, (6b) ✓ Pi = Z 1 0 r2R1i(r) dr = ↵1n J1(k1n) k21n ◆ (6c) is the non-dimensional liquid mass centre rlC , rlC0 defines its hydrostatic position, but rlCs determines the sloshing-related mass centre motions. Substituting (5), (6a) and (6b) into (4) derives the three scalar force components Fi(t), i = 1, 2, 3: F1(t) = g⌘5 � ⌘̈1 + 1 2h⌘̈5 � h�1 X i Pi p̈1i, (7a) F2(t) = �g⌘4 � ⌘̈2 � 1 2h⌘̈4 � h�1 X i Pi r̈1i, (7b) F3(t) = �g � ⌘̈3 � 2h�1 X i � p̈0ip01 + ṗ20i � � h�1 X m,i � p̈mipmi + ṗ2mi + r̈mirmi + ṙ2mi � . (7c) 3 The Stokes-Joukowski potentials The Lukovsky formula for the resulting hydrodynamic moment rela- tive to the origin O needs to know the free-surface depending Stokes- Joukowski potentials. The non-dimensional scalar Stokes-Joukowski po- tentials, ⌦i(x, y, z; {pMi, rmi}), i = 1, 2, 3, are components of the vector- function ⌦ = ⌦1e1 + ⌦2e2 + ⌦3e3, which is a solution of the Neumann boundary value problem r 2⌦ = 0 in Q(t), @n⌦ = r ⇥ n on S(t) + ⌃(t), (8) where r = xe1 + ye2 + ze3 and n is the outer normal unit vector. Find- ing the scalar Stokes-Joukowski potentials is the same as getting the harmonic functions satisfying the Neumann boundary conditions @n⌦1 = ynz � zny, @⌦2 = znx � xnz, @n⌦3 = xny � ynx on S(t) +⌃(t), (9) where nx, ny and nz are components of the outer normal vector in the Cartesian coordinate system Oxyz. Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 193 The Neumann boundary conditions (9) have a specific form for the upright circular base tank when considering them, separately, on the bottom, wetted walls, and the free surface. On the flat bottom, nx = ny = 0, nz = �1 and, therefore, (9) transforms to @z⌦1 = y = r sin ✓, @z⌦2 = �x = �r cos ✓, @z⌦3 = 0 at z = �h; (10) on the vertical wall, nx = cos ✓, ny = sin ✓, nz = 0 and, therefore, @r⌦1 = �z sin ✓, @r⌦2 = z cos ✓, @r⌦3 = 0 at r = 1. (11) The free surface ⌃(t) is defined by z = ⇣(r, ✓) = 0 or, in other words, by the hydrodynamic generalised coordinates in (1). To write down the corresponding Neumann boundary conditions, one should first introduce the outer normal vector n = rxyz[z � ⇣]/||rxyz[z � ⇣]|| where, according to (53) in Appendix B, nx||rxyz(z � ⇣)|| = � cos ✓ @r⇣ + r�1 sin ✓ @✓⇣, ny||rxyz(z � ⇣)|| = � sin ✓ @r⇣ � r�1 cos ✓ @✓⇣, nz||rxyz(z � ⇣)|| = 1. (12) Using these expressions, the Neumann boundary conditions in (9) on ⌃(t) take the following form r⌦1 ·r(z � ⇣) = r sin ✓ + ⇣ � sin ✓ @r⇣ + r�1 cos ✓ @✓⇣ � , (13a) r⌦2 ·r(z � ⇣) = �r cos ✓ + ⇣ � � cos ✓ @r⇣ + r�1 sin ✓ @✓⇣ � , (13b) r⌦3 ·r(z � ⇣) = �@✓⇣, (13c) where r⌦i ·r(z � ⇣) = @z⌦i � @r⌦i @r⇣ � r�2@✓⌦i @✓⇣. (14) The forthcoming goal consists, after substituting (1) into the Neu- mann boundary conditions (13), of getting an asymptotic approximation of the scalar Stokes-Joukowski potentials in terms of the hydrodynamic generalised coordinates pMi, rMi = O(✏1/3), ⌦ni = ⌦0i + ⌦1i + ⌦2i +O(✏), ⌦ni = O(✏n/3); n = 1, 2, 3, (15) starting with the zero-order approximation, which suggests the gener- alised coordinates pMi and rMi are zero. 194 Timokha A. N. 3.1 Zero-order approximation The zero-order approximation, ⌦0i, is an attribute of the linear sloshing problem. There is an analytical solution of the corresponding Neumann problem in the unperturbed liquid domain (the flat free surface with pMi = rMi = 0 in (13), (14)). This solution can be found, e.g., in the chapter 5 of [1]. For the adopted normalisation, this analytical solution was derived into [3]. It takes the form ⌦01 = �F(r, z) sin ✓, ⌦02 = F(r, z) cos ✓, ⌦03 = 0, (16) where F(r, z) = rz � 2 X n Pn k1n R1n(r) sinh(k1n(z + 1 2h)) cosh( 12k1nh) (17) and Pn is defined in (6c). One can see that ⌦3 has no the zero-order component but ⌦1 and ⌦2 and similar by the coordinates r, z and di↵er only by the azimuthal coordinate ✓. 3.2 First- and second-order approximate ⌦1 The first-order approximation of the Stokes-Joukowski potential ⌦1, ⌦11 from (15), is a harmonic function, which satisfies the zero-Neumann con- dition on the wetted tank surface (at z = �h and r = 1) but the Neu- mann boundary condition on the unperturbed free surface is non-zero but derivable from (13a) by keeping the O(✏1/3)-order quantities. It takes the form @z⌦11 = �@2 z⌦01⇣ + @r⌦01@r⇣ + r�2@✓⌦01@✓⇣ at z = 0. (18) Substituting (16), (17) and (1) into (18) yields @z⌦11 = 2 X Mi pMi X a P̃a ⇥ sin ✓ cos(M✓)(R0 MiR 0 1a � k21aRMiR1a) �M cos ✓ sin(M✓)r�2 RMiR1a ⇤ + 2 X mi rmi X a P̃a ⇥ sin ✓ sin(m✓)(R0 miR 0 1a � k21aRmiR1a) +m cos ✓ cos(m✓)r�2 RmiR1a ⇤ , (19) Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 195 where P̃a = Pak �1 1a tanh( 12k1ah). (20) Using the standard projective scheme derives the following solution ⌦11 = X Lk RLk(r)ZLk(z) cos(L✓) X mi O1,r (Lk),(mi)rmi(t) + X lk Rlk(r)Zlk(z) sin(l✓) X Mi O1,p (lk),(Mi)pMi(t), (21) where O1,r (Lk),(mi) = 2 ⇤LL X a P̃a n ⇤L,m1 � �0 (mi)(1a),(Lk) � k21a�(mi)(1a)(Lk) � +m⇤mL1,�̄(mi)(1a)(Lk) o , (22a) O1,p (lk),(Mi) = 2 ⇤ll X a P̃a n ⇤M,1l � �0 (Mi)(1a),(lk) � k21a�(Mi)(1a)(lk) � �M⇤1,Ml�̄(Mi)(1a)(lk) o (22b) within notations from (3) and Appendix B . The second-order approximation ⌦21 is also a harmonic function sat- isfying the zero-Neumann boundary condition at z = �h and r = 1. The only non-zero Neumann boundary condition at z = 0 can be obtained by the Taylor expansion in ⇣ (and its derivatives) applied to (13a). The result is @z⌦21 = ⇣ � sin ✓@r⇣ + r�1 cos ✓@✓⇣ � + ⇣ � @2 zr⌦01@r⇣ + r�2@2 z✓⌦01@✓⇣ � � 1 2@ 3 z⌦01⇣ 2 � @2 z⌦11⇣ + @r⌦11@r⇣ + r�2@✓⌦11@✓⇣ at z = 0. (23) Because @z⌦01 = r sin ✓ at z = 0, two first summands in (23) are equal. Furthermore, using the obvious Fourier expansions following from the Parseval identity r = X a PaR1a(r) and 1 = X a PaR 0 1a(r), the boundary condition (23) itransforms to the following form 196 Timokha A. N. @z⌦21 = X MiNj pMipNj nX a Pa ⇥ sin ✓ cos(M✓) cos(M✓) � 2R0 NjR 0 1aRMi � k21aRNjR1aRMi � � 2N cos ✓ cos(M✓) sin(N✓)r�2 RNjR1aRMi ⇤ + X Ab O1,p (Ab),(Mi) �1 Ab ⇥ sin(A✓) cos(N✓) � R 0 AbR 0 Nj � k2AbRAbRNj � �AN cos(A✓) sin(N✓)r�2 RAbRNj ⇤o + X minj rmirnj nX a Pa ⇥ sin ✓ sin(m✓) sin(n✓) � 2R0 njR 0 1aRmi � k21aRmiR1aRnj � + 2n cos ✓ sin(m✓) cos(n✓)r�2 RnjR1aRmi ⇤ + X Ab O1,r (Ab),(mi) �1 Ab ⇥ cos(A✓) sin(n✓) � R 0 AbR 0 nj � k2AbRAbRnj � �An sin(A✓) cos(n✓)r�2 RAbRnj ⇤o + X Minj pMirnj n 2 X a Pa ⇥ sin ✓ cos(M✓) sin(n✓) � R 0 njR 0 1aRMi+R 0 MiR 0 1aRnj �k21aRnjR1aRMi � + � n cos ✓ cos(M✓) cos(n✓)�M cos ✓ sin(n✓) sin(M✓) � ⇥ r�2 RMiR1aRnj ⇤ + X Ab �1 Ab h O1,p (Ab),(Mi) � sin(A✓) sin(n✓) ⇥ ⇥ R 0 AbR 0 nj � k2AbRAbRnj ⇤ +An cos(A✓) cos(n✓)r�2 RAbRnj � +O1,r (Ab),(nj) � cos(A✓) cos(M✓) ⇥ R 0 AbR 0 Mi � k2AbRAbRMi ⇤ +AM sin(A✓) sin(M✓)r�2 RAbRMi �i at z = 0. (24) The standard projective scheme leads then to the following solution ⌦21 = X Lk RLk(r)ZLk(z) cos(L✓) X Mnij O1,pr (Lk),(Mi),(nj)pMirnj + X lk Rlk(r)Zlk(z) sin(l✓) " X MiNj O1,pp (lk),(Mi),(Nj)pMipNj + X minj O1,rr (lk),(mi),(nj)rmirnj # , (25) where Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 197 O1,pr (Lk),(Mi),(nj) = 2 ⇤LL X a Pa h ⇤LM,1n � �0 (nj)(1a),(Mi)(Lk)+�0 (Mi)(1a),(nj)(Lk) � k21a�(nj)(1a)(Mi)(Lk) � + (n⇤LMn1, �M⇤L1,Mn)�̄(nj)(1a)(Mi)(Lk) i + X Ab �1 Ab h O1,p (Ab),(Mi) � ⇤L,An ⇥ �0 (Ab)(nj),(Lk) � k2Ab�(Ab)(nj)(Lk) ⇤ +An⇤AnL,�̄(Ab)(nj)(Lk) � +O1,r (Ab),(nj) � ⇤AML, ⇥ �0 (Ab)(Mi),(Lk) � k2Ab�(Ab)(Mi)(Lk) ⇤ +AM⇤L,Am,�̄(Ab)(Mi)(Lk) �i , (26a) O1,pp (lk),(Mi),(Nj) = 2 ⇤ll X a Pa h ⇤MN,l1 � �0 (Nj(1a),(Mi)(lk) � 1 2k 2 1a�(Mi)(1a)(Nj)(lk) � �N⇤1M,lN �̄(mi)(1a)(Nj)(lk) i + X Ab O1,p (Ab),(Mi) �1 Ab h ⇤N,Al � �0 (Ab)(Nj),(lk) � k2Ab�(Ab)(Nj)(lk) � �AN⇤A,Nl�̄(Ab)(Nj)(lk) i , (26b) O1,rr (lk),(mi),(nj) = 2 ⇤ll X a Pa h ⇤,1nml � �0 (nj)(1a),(mi)(lk) � 1 2k 2 1a�(mi)(1a)(nj)(lk) � + n⇤1n,ml�̄(mi)(1a)(nj)(lk) i + X Ab O1,r (Ab),(mi) �1 Ab h ⇤A,nl � �0 (Ab)(nj),(lk) � k2Ab�(Ab)(nj)(lk) � �An⇤n,Al�̄(Ab)(nj)(lk) i . (26c) 3.3 First- and second-order approximate ⌦2 Proceeding in similar way with the zero-order approximation (16), (17) and the Neumann boundary condition (13b) on the free surface derives the first- and second-order approximations, ⌦12 and ⌦22, as follows ⌦12 = X Lk RLk(r)ZLk(z) cos(L✓) X Mi O2,p (Lk),(Mi)pMi(t) + X lk Rlk(r)Zlk(z) sin(l✓) X mi O2,r (lk),(mi)rmi(t), (27) 198 Timokha A. N. where O2,p (Lk),(Mi) = 2 ⇤LL X a P̃a h ⇤1ML, � � �0 (Mi)(1a),(Lk) + k21a�(Mi)(Lk)(1a) � �M⇤L,1M �̄(Mi)(1a)(Lk) i , (28a) O2,r (lk),(mi) = 2 ⇤ll X a P̃a h ⇤1,lm � � �0 (mi)(1a),(lk) + k21a�(mi)(lk)(1a) � +m⇤M,1l�̄(mi)(1a)(lk) i (28b) and ⌦22 = X Lk RLk(r)ZLk(z) cos(L✓) " X MiNj O2,pp (Lk),(Mi),(Nj)pMipNj + X minj O2,rr (Lk),(mi),(nj)rmirnj # + X lk Rlk(r)Zlk(z) sin(l✓) X Mnij O2,pr (lk),(Mi),(nj)pMirnj (29) where O2,pp (Lk),(Mi),(Nj) = 2 ⇤LL X a h ⇤1MNL, � 1 2�(Mi)(Nj)(1a)(Lk) � �0 (Nj)(1a),(Mi)(Lk) � �N⇤ML,N1�̄(Nj)(1a)(Mi)(Lk) i + X Ab O2,p (Ab),(Mi) �1 Ab h ⇤ANL, � �0 (Ab)(Nj),(Lk) � k2Ab�(Ab)(Nj)(Lk) � +AN⇤L,AN �̄(Ab)(Nj)(Lk) i , (30a) O2,rr (Lk),(mi),(nj) = 2 ⇤LL X a h ⇤1L,mn � 1 2�(mi)(nj)(1a)(Lk) � �0 (nj)(1a),(mi)(Lk) � + n⇤nl,1m�̄(nj)(1a)(mi)(Lk) i Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 199 + X Ab O2,r (Ab),(mi) �1 Ab h ⇤L,An � �0 (Ab)(nj),(Lk) � k2Ab�(Ab)(nj)(Lk) � + an⇤AnL,�̄(Ab)(nj)(Lk) i , (30b) O2,pr (Lk),(Mi),(nj) = 2 ⇤ll X a Pa h ⇤1M,ln � k21a�(Mi)(1a)(nj)(lk)��0 (nj)(1a),(Mi)(lk) � �0 (Mi)(1a),(nj)(lk) � + (n⇤Mn,1l �M⇤,1Mnl)�̄(1a)(Mi)(nj)(lk) i + X Ab �1 ab h O2,p (Ab),(Mi) � ⇤A,nl(� 0 (Ab)(nj),(lk) � k2Ab�(Ab)(nj)(lk)) �An⇤n,Al�̄(Ab)(nj)(lk) � +O2,r (Ab),(nj) � ⇤M,lA(� 0 (Ab)(Mi),(lk)�k2Ab�(Ab)(Mi)(lk)) �AM⇤A,Ml�̄(Ab)(Mi)(lk) i . (30c) 3.4 First- and second-order approximate ⌦3 The scalar Stokes-Joukowski potential ⌦3 is also a harmonic function satisfying the zero-Neumann conditio at z = �h, r = 1 and the non-zero Neumann condition (13c) on the free surface. Using the Taylor expansion by ⇣, the latter condition takes in the first (linear) approximation the following form @z⌦13 = �@✓⇣ = X mi mRmi ⇥ sin(m✓)pMi � cos(m✓)rmi ⇤ at z = 0. One can then get the following harmonic ⌦13 = X mi mRmi(r)Zmi(z) ⇥ sin(m✓) pmi � cos(m✓) rmi ⇤ . (31) Further, the second-order harmonic approximation of the Neumann boundary condition (13c) takes the form @z⌦23 = �@2 z⌦13 ⇣ + @r⌦13 @r⇣ + r�2@✓⌦13 @✓⇣ = X MiNj pMipNjM�1 Mi ⇥ sin(M✓) cos(N✓) � R 0 MiR 0 Nj � k2MiRMiRNj � �MN cos(M✓) sin(N✓)r�2 RMiRNj ⇤ 200 Timokha A. N. + X mnij rmirnjm�1 mi ⇥ cos(n✓) sin(n✓) � k2miRmiRnj �R 0 miR 0 nj � +mn sin(m✓) cos(n✓)r�2 RmiRnj ⇤ + X Minj h RMiRnj ⇥ ⇣ � Mk2Mi Mi sin(M✓) sin(n✓) + nk2nj nj cos(M✓) cos(n✓) ⌘ +R 0 MiR 0 nj ⇣ M Mi sin(M✓) sin(n✓)� n nj cos(M✓) cos(n✓) ⌘ + r�2 RMiRnjMn ⇣ M Mi cos(M✓) cos(n✓) � n nj sin(M✓) sin(n✓) ⌘i at z = 0. Proceeding as in the previous sections derives the Fourier solution ⌦23 = X Lk RLk(r)ZLk(z) cos(L✓) " X Mnij O3,pr (Lk),(Mi),(nj)pMirnj # + X lk Rlk(r)ZLk(z) sin(l✓) " X MNij O3,pp (lk),(Mi),(Nj)pMipNj + X mnij O3,rr (lk),(mi),(nj)rmirnj # , (32) where O3,pr (Lk),(Mi),(nj) = 1 ⇤LL h �(Mi)(nj)(Lk) ⇣ � ⇤L,Mn Mk2Mi Mi + ⇤MLn, nk2nj nj ⌘ +�0 (Mi)(nj),(Lk) � ⇤L,MnM�1 Mi � ⇤LMn,n �1 nj ⌘ + �̄(Mi)(nj)(Lk)Mn � ⇤LMn,M�1 Mi � ⇤L,Mnn �1 nj � i , (33a) O3,pp (lk),(Mi),(Nj) = 1 ⇤ll M Mi h ⇤N,Ml ⇣ �k2Mi�(Mi)(Nj)(lk) + �0 (Mi)(Nj),(lk) ⌘ �MN ⇤M,Nl�̄(Mi)(Nj)(lk) i , (33b) Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 201 O3,rr (lk),(mi),(nj) = 1 ⇤ll m mi h ⇤m,nl ⇣ k2mi�(mi)(nj)(lk) � �0 (mi)(nj),(lk) ⌘ +mn⇤n,ml�̄(mi)(nj)(lk) i , (33c) in which we adopted notations from Appendix A. 4 Hydrodynamic moment According to the Lukovsky formula [1, 4], the resulting (dimensional) hydrodynamic moment (relative to the origin O) may be written down (rlC0 ⇥ g0 = 0) as MO = ⇥ MlR 2 0� 2 ⇤ ⇣ rlC ⇥ (g � ! ⇥ vO � v̇O)� J1 · !̇ � J̇ 1 · ! �! ⇥ � J1 · ! � � l̈! + l̇!t � ! ⇥ ⇣ l̇! � l!t ⌘⌘ = ⇥ MlR 2 0� 2 ⇤ ⇣ rlC0 ⇥ (g � g0) � rlC0 ⇥ v̇O + (rlC � rlC0)⇥ g0 � J1 0 · !̇ � �̈ l! � l̇!t � + o(✏) � = ⇥ MlR 2 0� 2 ⇤ � F4(t) e1(t) + F5(t) e2(t) + F6(t) e3(t) + o(✏) � , (34) where J1 = J1 ij is the non-dimensional liquid inertia tensor (J1 0 is its O(1)-order component), J1 ij = 1 ⇡h Z S(t)+⌃(t) ⌦i @n⌦j dS (35) and l! = 1 ⇡h Z Q(t) ⌦ dQ, l!t = 1 ⇡h Z Q(t) ⌦̇ dQ. (36) The formula (34) contains two framed terms. The first one, rlC0 ⇥ (g�g0), implies a quasi-static moment relative to O caused by a small in- stant pivoting of the tank body by ⌘4 and ⌘5. The second framed expres- sion, l̈! � l̇!t is a rather complicated function determined by the Stokes- Jukowski potentials. By utilising the Reynolds transport theorem and that the normal relative velocity of the free surface un = ⇣̇/ p 1 + (r⇣)2, the second framed terms re-writes in the form ⇡h @t � l̇! � l!t � = @t Z ⌃(t) ⌦undS = @t Z 1 0 Z ⇡ �⇡ r h ⌦|z=⇣ i ⇣̇ d✓dr. (37) 202 Timokha A. N. Because ⇣ = O(✏1/3), getting the O(✏)-order component of (37) should adopt the O(✏2/3)-order solution from the previous section. The adaptive asymptotic approximation of the hydrodynamic moment also requires the zero-order approximation of the inertia tensor J1 0. Sub- stituting (16) into (35) with ⇣ = 0 computes J1 0 = {J1 0ij} whose the only non-zero component is J0 = J1 011 = J1 022 = h2 3 � 3 4 + 16 h X n tanh( 12k1nh) k31n(k 2 1n � 1) . (38) 4.1 Component F4(t) Using expressions for the zero- (16), first- (21) and second- (25) order approximations and neglecting the o(✏) terms computes Z 1 0 Z ⇡ �⇡ r � ⌦01 + @z⌦01⇣ +⌦11 + 1 2@ 2 z⌦01⇣ 2 + @z⌦11⇣ +⌦21 � |z=0⇣̇d✓dr = 2⇡ X a P̃aṙ1a + X Njmi Õ1,pr (Nj),(mi)ṗNjrmi + X Minj Õ1,rp (nj),(Mi)ṙnjpMi + X NjLkmi Õ1,ppr (Nj),(Lk),(mi)ṗNjpLkrmi + X njLkMi Õ1,rpp (nj),(Lk),(Mi)ṙnjpLkpMi + X njlkmi Õ1,rrr (nj),(lk),(mi)ṙnjrlkrmi, (39) where Õ1,pr (Nj),(mi) = ⇤N,1m X a Pa�(1a)(mi)(Nj) + ⇤NN�1 NjO 1,r (Nj),(mi), Õ1,rp (nj),(Mi) = ⇤M,1n X a Pa�(1a)(Mi)(nj) + ⇤nn �1 nj O 1,p (nj),(Mi), Õ1,ppr (Nj),(Lk),(mi) = 2⇤NL,m1 X a P̃a�(1a)(Nj)(Lk)(mi) + ⇤NN�1 NjO 1,pr (Nj),(Lk),(mi) + X Ab �(Ab)(Lk)(Nj)O 1,r (Ab),(mi)⇤ALN, + X ab �(ab)(mi)(Nj)O 1,p (ab),(Lk)⇤N,ma, Õ1,rpp (nj),(Lk),(Mi) = ⇤LM,n1 X a P̃ak 2 1a�(1a)(nj)(Mi)(Lk) Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 203 + ⇤nn �1 nj O 1,pp (nj),(Mi),(Lk) + X ab �(ab)(Lk)(nj)O 1,p (ab),(Mi)⇤L,an, Õ1,rrr (nj),(lk),(mi) = ⇤,1nlm X a P̃ak 2 1a�(1a)(nj)(mi)(lk) + ⇤nn �1 nj O 1,rr (nj),(mi),(lk) + X Ab �(Ab)(lk)(nj)O 1,r (Ab),(mi)⇤A,ln. The moment component F4(t) is then computed as F4(t) = g h 1 2h ⌘4 � h�1 X a Par1a i � 1 2h⌘̈2 � J0⌘̈4 � 2h�1 X a P̃ar̈1a + X Njmi M1,pr (Nj),(mi)p̈Njrmi+ X njMi M1,rp (nj),(Mi)r̈njpMi+ X Njmi N1,pr (Nj),(mi)ṗNj ṙmi + X LkMinj M1,ppr (Lk),(Mi),(lk)p̈LkpMirnj + X lkMiNj M1,rpp (lk),(Mi),(Nj)r̈lkpMipNj + X lkminj M1,rrr (lk),(mi),(nj)r̈lkrmirnj + X LkMinj N1,ppr (Lk),(Mi),(nj)ṗLkṗMirnj + X lkminj N1,rrr (lk),(mi),(nj)ṙlkṙmirnj + X lkMinj N1,rpp (lk),(Mi),(Nj)ṙlkṗMipNj , (40) where M1,pr (Nj),(mi) = �(⇡h)�1Õ1,pr (Nj),(mi), M1,rp (nj),(Mi) = �(⇡h)�1Õ1,rp (nj),(Mi), N1,pr (Nj),(mi) = �(⇡h)�1 � Õ1,pr (Nj),(mi) + Õ1,rp (mi),(Nj) � , M1,ppr (Lk),(Mi),(lk) = �(⇡h)�1Õ1,ppr (Lk),(Mi),(nj), M1,rpp (lk),(Mi),(Nj) = �(⇡h)�1Õ1,rpp (lk),(Mi),(Nj), M1,rrr (lk),(mi),(nj) = �(⇡h)�1Õ1,rrr (lk),(mi),(nj), N1,ppr (Lk),(Mi),(nj) = �(⇡h)�1Õ1,ppr (Lk),(Mi),(nj), N1,rrr (lk),(mi),(nj) = �(⇡h)�1 � Õ1,rrr (lk),(mi),(nj) + Õ1,rrr (lk),(nj),(mi) � , N1,rpp (lk),(Mi),(Nj)= �(⇡h)�1 � Õ1,rpp (lk),(Mi),(Nj)+ Õ1,ppr (Mi),(Nj),(lk)+ Õ1,rpp (lk),(Nj),(Mi) � . 4.2 Component F5(t) In similar to (39), the l2-related quantity takes the form 204 Timokha A. N. Z 1 0 Z ⇡ �⇡ r � ⌦02 + @z⌦02⇣ +⌦12 + 1 2@ 2 z⌦02⇣ 2 + @z⌦12⇣ +⌦22 � |z=0⇣̇d✓dr = �2⇡ X a P̃aṗ1a + X NjMi Õ2,pp (Nj),(Mi)ṗNjpmi + X minj Õ2,rr (nj),(mi)ṙnjrmi + X NjLkMi Õ2,ppp (Nj),(Lk),(Mi)ṗNjpLkpMi + X njlkmi Õ2,prr (Nj),(lk),(mi)ṗNjrlkrmi + X njLkmi Õ2,rpr (nj),(Lk),(mi)ṙnjpLkrmi, (41) where Õ2,pp (Nj),(Mi) = �⇤1MN, X a Pa�(1a)(Mi)(Nj) + ⇤NN�1 NjO 2,p (Nj),(Mi), Õ2,rr (nj),(mi) = �⇤,1mn X a Pa�(1a)(mi)(nj) + ⇤nn �1 nj O 2,r (nj),(mi), Õ2,ppp (Nj),(Lk),(Mi) = �⇤NLM1, X a P̃ak 2 1a�(1a)(Nj)(Lk)(Mi) + ⇤NN�1 NjO 2,pp (Nj),(Mi),(Lk) + X Ab �(Ab)(Lk)(Nj)O 2,p (Ab),(Mi)⇤ALN,, Õ2,prr (Nj),(lk),(mi) = �⇤N1,lm X a P̃ak 2 1a�(1a)(Nj)(mi)(lk) + ⇤NN�1 NjO 2,rr (Nj),(mi),(lk) + X ab �(ab)(lk)(Nj)O 2,r (ab),(mi)⇤N,al, Õ2,rpr (nj),(Lk),(mi) = �2⇤L1,nm X a P̃ak 2 1a�(1a)(Lk)(mi)(nj) + ⇤nn �1 nj O 2,pr (nj),(Lk),(mi) + X Ab ⇤A,mnO 2,p (Ab),(Lk)�(Ab)(mi)(nj) + X ab ⇤L,anO 2,r (ab),(mi)�(ab)(Lk)(nj). The moment component F5(t) is then derived as follows F5(t) = g h 1 2h⌘5 + h�1 X a Pap1a i + 1 2h⌘̈1 � J0⌘̈5 � 2h�1 X a P̃ap̈1a + X NjMi M2,pp (Nj),(Mi)p̈Njpmi + X njmi M2,rr (nj),(mi)r̈njpmi Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 205 + X NjMi N2,pp (Nj),(mi)ṗNj ṗMi + X njmi N2,rr (nj),(mi)ṙnj ṙmi + X NjLkNj M2,ppp (Nj),(Lk),(Mi)p̈LkpLkpMi + X Njlkmi M2,prr (Nj),(lk),(mi)p̈Njrlkirmi + X njLkmi M2,rpr (nj),(Lk),(mi)r̈njpLkrmi + X NjLkMij N2,ppp (Nj),(Lk),(Mi)ṗNj ṗLkpMi + X Njlkmi N2,prr (Nj),(lk),(mi)ṗNj ṙlkrmi + X njlkMi N2,rrp (nj),(lk),(Mi)ṙnj ṙlkpMi, (42) where M2,pp (Nj),(Mi) = N2,pp (Nj),(Mi) = �(⇡h)�1Õ2,pp (Nj),(Mi), M2,rr (nj),(mi) = N2,rr (nj),(mi) = �(⇡h)�1Õ1,rp (nj),(Mi), M2,ppp (Nj),(Lk),(Mi) = �(⇡h)�1Õ2,ppp (Nj),(Lk),(Mi), M2,prr (Nj),(lk),(mi) = �(⇡h)�1Õ2,prr (Nj),(lk),(mi), M2,rpr (nj),(Lk),(mi) = �(⇡h)�1Õ1,rpr (nj),(Lk),(mi), N2,ppp (Nj),(Lk),(Mi) = �(⇡h)�1 ⇣ Õ2,ppp (Nj),(Lk),(Mi) + Õ2,ppp (Nj),(Mi),(Lk) ⌘ , N2,prr (Nj),(lk),(mi) = �(⇡h)�1 ⇣ Õ2,prr (Nj),(lk),(mi) + Õ2,prr (Nj),(mi),(lk) + Õ2,rpr (lk),(Nj),(mi) ⌘ , N2,rpr (nj),(lk),(Mi) = �(⇡h)�1Õ2,rpr (nj),(Mi),(lk). 4.3 Component F6(t) The hydrodynamic moment component relative to O is uniquely function of (36), i.e., F6 = � 1 ⇡h @t Z 1 0 Z ⇡ �⇡ r⌦3|z=⇣ @t⇣ d✓dr. (43) Using expressions (31) and (32) and neglecting the o(✏) terms computes Z 1 0 Z ⇡ �⇡ r � ⌦13⇣̇ + @z⌦13⇣⇣̇ + ⌦23⇣̇ � |z=0d✓dr = ⇡ X mi m�1 mi � pmiṙmi � ṗmirmi � + X LkMinj Õ3,ppr (Lk),(Mi),(nj)ṗLkpMirnj 206 Timokha A. N. + X lkMiNj Õ3,rpp (lk),(Mi),(nj)ṙlkpMipNj + X lkminj Õ3,rrr (lk),(mi),(nj)ṙlkrmirnj , (44) where Õ3,ppr (Lk),(Mi),(nj) = ⇤LL Lk O3,pr (Lk),(Mi),(nj)+�(Lk)(Mi)(nj)(M⇤L,Mn�n⇤LMn,), (45a) Õ3,rpp (lk),(Mi),(Nj) = ⇤ll �1 lk O3,pp (lk),(Mi),(Nj) + �(lk)(Mi)(Nj)M⇤N,lM , (45b) Õ3,rrr (lk),(mi),(nj) = ⇤ll �1 lk O3,rr (lk),(mi),(nj) � �(lk)(Mi)(Nj)m⇤m,ln. (45c) Substituting (44) into (43) derives the final expression for the adaptive Lukovsky moment component F6(t) = �h�1 X mi m�1 mi � pmir̈mi � p̈mirmi � + X LkMinj M3,ppr (Lk),(Mi),(lk)p̈LkpMirnj + X lkMiNj M3,rpp (lk),(Mi),(Nj)r̈lkpMipNj + X lkminj M3,rrr (lk),(mi),(nj)r̈lkrmirnj + X LkMinj N3,ppr (Lk),(Mi),(nj)ṗLkṗMirnj + X lkminj N3,rrr (lk),(mi),(nj)ṙlkṙmirnj + X lkMinj N3,rpr (lk),(Mi),(nj)ṙlkṗMirnj , (46) where M3,ppr (Lk),(Mi),(lk) = �(⇡h)�1Õ3,ppr (Lk),(Mi),(nj), M3,rpp (lk),(Mi),(Nj) = �(⇡h)�1Õ3,rpp (lk),(Mi),(Nj), M3,rrr (lk),(mi),(nj) = �(⇡h)�1Õ3,rrr (lk),(mi),(nj), N3,ppr (Lk),(Mi),(nj) = �(⇡h)�1Õ3,ppr (Lk),(Mi),(nj), N3,rrr (lk),(mi),(nj) = �(⇡h)�1 � Õ3,rrr (lk),(mi),(nj) + Õ3,rrr (lk),(nj),(mi) � , N3,rpp (lk),(Mi),(Nj)= �(⇡h)�1 � Õ3,rpp (lk),(Mi),(Nj)+ Õ3,ppr (Mi),(Nj),(lk)+ Õ3,rpp (lk),(Nj),(Mi) � . 5 Conclusions The derivation scheme from [2] was generalised to derive adaptive weakly- nonlinear expressions for the resulting hydrodynamic force and moments Adaptive Lukovsky’s formulas for the resulting hydrodynamic . . . 207 caused by the pressure loads on the wetted surface of an upright cir- cular container partly filled with a liquid. The expressions follow from the so-called Lukovsky formulas, which give the force and moment writ- ten down in terms of the hydrodynamic generalised coordinates. They are consistent with asymptotic relations of the adaptive modal equations in [2]. The forthcoming derivations should focus on simplifications of the weakly-nonlinear expressions to handle the case of the Narimanov- Moiseev–type modal theory [2, 3]. A Tensors To derive the adaptive modal equations, [2] introduced a set of tensors, which imply an algebra in the angular and radial coordinates. The first, ⇤-type tensor reads as ⇤M...N,i...j = Z ⇡ �⇡ cos(M✓)... cos(N✓) · sin(i✓)... sin(j✓) d✓, (47) whose computations are best done by using the recursive formulas ⇤M,i = 0; ⇤ij = ⇤,ij = ⇤ij, = ⇡�ij ; ⇤MN, = ⇡�MN (M +N 6= 0), ⇤MN, = 2⇡�MN (M = N = 0); ⇤M...NK,i...j = 1 2 � ⇤M...|N�K|,i...j + ⇤M...|N+K|,i..j � ; ⇤M...N,i...jkl = 1 2 � ⇤M...|j�k|,i...l � ⇤M...|j+k|,i..l � . The second, the radial components and functions RMi(r) yield the �- tensors: �(Mi)...(Nk) = Z 1 0 rRMi(r)...RNk(r) dr, (48) �0 (Mi)(Nk),(Cd)...(Ef) = Z 1 0 rR0 Mi(r)R 0 Nk(r) · RCd(r)...REf (r) dr, (49) �̄(Mi)...(Nk) = Z 1 0 1 r2 RMi(r)...RNk(r) dr. (50) B Di↵erentiation rules The analysis suggests the hydrodynamic moments relative to axes of the Cartesian coordinate system Oxyz (with the coordinate units x̂, ŷ and 208 Timokha A.N. ẑ) but the natural sloshing modes and associate derivations deal with the cylindrical coordinates Or✓z (the coordinate units r̂, ✓̂ and ẑ). This implies the gradients rxyz = x̂ @x + ŷ @y + ẑ @z, rr✓z = r̂ @r + ✓̂ r�1@✓ + ẑ @z, (51) the di↵erentiation rule @x = cos ✓ @r � r�1 sin ✓ @✓, @y = sin ✓ @r + r�1 cos ✓ @✓, (52) which, in particular, deduce the expression rxyz[z � ⇣(r, ✓)] = x̂ [� cos ✓ @r⇣ + r�1 sin ✓ @✓⇣] + ŷ [� sin ✓ @r⇣ � r�1 cos ✓ @✓⇣] + ẑ [1] (53) used to identify the outer normal unit on the free surface ⌃(t). [1] Faltinsen O.M., Timokha A.N. Sloshing.—Cambridge: Cambridge Uni- versity Press, 2009.— 683 p. [2] Faltinsen O.M., Lukovsky I.A. Timokha A.N. Resonant sloshing in an up- right annular tank // Journal of Fluid Mechanics.— 2016.— 804.— P. 608- 645. [3] Raynovskyy I., Timokha A.N. Damped steady-state resonant sloshing in a circular base container // Fluid Dynamics Research.— 2018.— 50.— Article ID 045502. [4] Lukovsky I.A. Introduction to nonlinear dynamics of rigid bodies with the cavities partially filled by a fluid.—Kiev: Naukova Dumka, 1990.— 296 p. (in Russian) [5] Lukovsky I.A. Nonlinear dynamics: Mathematical models for rigid bodies with a liquid.—De Gruyter, 2015.— 400 p. [6] Lukovsky I.A., Timokha A.N. Multimodal method in sloshing // Journal of Mathematical Sciences.— 2017.— 220, No 3.—P. 239–253.
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institution Transactions of Institute of Mathematics of NAS of Ukraine
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spelling oai:trim.imath.kiev.ua:article-4222020-08-09T15:01:39Z Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank Адаптивні формули Луковського для рузультуючих гідродинамічних сил та моментів у вертикальному круговому баці Адаптивні формули Луковського для рузультуючих гідродинамічних сил та моментів у вертикальному круговому баці Тимоха, О.М. Тимоха, А.Н. Timokha, A.N. Lukovsky’s asymptotic formulas for the resulting hydrodynamic force and moment are derived as if they follow from the adaptive (infinite- dimensional) multimodal theory of the liquid sloshing dynamics in an upright circular base container. The result is given in a tensor form in- troduced in notations of the original paper by Faltinsen, Lukovsky and Timokha (2016). Виводяться формули Луковського адаптивного асимптотичного типу для результуючих гiдродинамiчної сили й моменту, що пов’язуються з коливаннями рiдини у вертикальному круговому бацi. Результат пред- ставлено в термiнах позначень iз оригiнальної роботи Фалтiнсена, Луковського й Тимохи (2016). Виводяться формули Луковського адаптивного асимптотичного типу для результуючих гiдродинамiчної сили й моменту, що пов’язуються з коливаннями рiдини у вертикальному круговому бацi. Результат пред- ставлено в термiнах позначень iз оригiнальної роботи Фалтiнсена, Луковського й Тимохи (2016). Інститут математики НАН України 2020-08-09 Article Article application/pdf https://trim.imath.kiev.ua/index.php/trim/article/view/422 Transactions of Institute of Mathematics, the NAS of Ukraine; Vol. 16 No. 2 (2019): Mathematical problems of mechanics and computational mathematics; 188-208 Сборник Трудов Института математики НАН Украины; Том 16 № 2 (2019): Математические проблеми механики и вычислительной математики; 188-208 Збірник Праць Інституту математики НАН України; Том 16 № 2 (2019): Математичні проблеми механіки та обчислювальної математики; 188-208 3083-7529 1815-2910 en https://trim.imath.kiev.ua/index.php/trim/article/view/422/415 Авторське право (c) 2020 A.N. Timokha http://creativecommons.org/licenses/by/4.0
spellingShingle Тимоха, О.М.
Тимоха, А.Н.
Timokha, A.N.
Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
title Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
title_alt Адаптивні формули Луковського для рузультуючих гідродинамічних сил та моментів у вертикальному круговому баці
Адаптивні формули Луковського для рузультуючих гідродинамічних сил та моментів у вертикальному круговому баці
title_full Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
title_fullStr Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
title_full_unstemmed Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
title_short Adaptive Lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
title_sort adaptive lukovsky’s formulas for the resulting hydrodynamic force and moment owing to sloshing in an upright circular tank
url https://trim.imath.kiev.ua/index.php/trim/article/view/422
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