Fluid damping of cylindrical liquid storage tanks
Habenberger SpringerPlus (2015)4:515
DOI 10.1186/s40064-015-1302-2
Open Access
RESEARCH
Fluid damping of cylindrical liquid
storage tanks
Joerg Habenberger*
*Correspondence:
joerg.habenberger@
baslerhofmann.ch
Basler & Hofmann
AG, Forchstrasse 395,
8032 Zurich, Switzerland
Abstract
A method is proposed in order to calculate the damping effects of viscous fluids in liquid storage tanks subjected to earthquakes. The potential equation of an ideal fluid can
satisfy only the boundary conditions normal to the surface of the liquid. To satisfy also
the tangential interaction conditions between liquid and tank wall and tank bottom,
the potential flow is superimposed by a one-dimensional shear flow. The shear flow in
this boundary layer yields to a decrease of the mechanical energy of the shell-liquidsystem. A damping factor is derived from the mean value of the energy dissipation
in time. Depending on shell geometry and fluid viscosity, modal damping ratios are
calculated for the convective component.
Keywords: Fluid damping, Earthquake, Cylindrical liquid storage tanks
Background
The dynamic behavior of liquid storage tanks and of structures in general is highly influenced by the structural damping. In engineering, an ideal fluid is usually assumed in the
realm of dynamic analysis of liquid storage tanks. In doing this, the potential equation of
the liquid may be divided into two decoupled components: (1) the impulsive component
which describes the interaction of the liquid and the shell and (2) the sloshing motion of
the free liquid surface which may be accounted for by the convective component.
After the modal decomposition of both components, a viscous damping is introduced
to consider the dissipation of mechanical energy. The damping influences the resulting
pressures as well as the amplitude of the convective fluid motion. If the response spectra
method is used to calculate the dynamic response of the tank-liquid-system the spectral
acceleration is determined directly by the damping ratios.
The damping of the impulsive component is mainly affected by the damping of the
shell, and the fluid damping may be neglected. Depending on the material of the shell,
damping ratios between 2 % (steel) and 5 % (reinforced concrete) are suggested for the
Serviceability Limit State (Eurocode 8, Part 4 2006 or Scharf 1989). The damping ratios
are larger for the Ultimate Limit State (4 % for steel and 7 % for concrete structures).
These are typical and well established damping ratios (Stevenson 1980).
For the convective component damping ratios from 0 up to 5 % are proposed. The second draft of Eurocode 8, Part 4, e.g., suggests a damping ratio of 0.5 % “for water and
other liquids”. Scharf (1989) recommends a value of 0 % independent of the content. It is
© 2015 Habenberger. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License
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Habenberger SpringerPlus (2015)4:515
Page 2 of 11
also important to mention that there are no experimental or theoretical justifications of
the proposed damping values concerning the sloshing oscillation and they are more or
less “best guesses”.
With the potential equation of the ideal fluid only boundary and interaction conditions normal to the surface of the fluid can be satisfied. It is not possible to describe the
adhesion of a real fluid to the tank wall and bottom by the potential equation. To fulfill
the boundary conditions though a one-dimensional shear flow is superimposed on the
potential flow of the ideal fluid. For this purpose at first the Navier–Stokes-equation is
applied and simplified with respect to the conditions at the boundary layer of the fluid. A
solution of the simplified form of the Navier–Stokes-equation is derived which describes
the velocity in the boundary layer.
The shear flow in the boundary layer leads to a dissipation of mechanical energy. This
energy dissipation is related to the damping ratio of the fluid oscillation. Damping ratios
for the sloshing component are derived for different shell geometries and fluid viscosities. In Fig. 1 a cross-section of the investigated liquid storage tank with the corresponding material and geometry parameters is shown.
Damping effects of a viscous fluid
Equations of the incompressible, viscous fluid
The fluid is assumed to be incompressible and viscous. The friction pressures are proportional to the velocity of the liquid (Newton’s fluid with kinematic viscosity ν). The
condition of incompressibility (with the velocity field of the fluid v = (vζ vϕ vξ )T ) reads as
follows (Sommerfeld 1988):
∇ · v = 0.
(1)
The Navier–Stokes-Equation without consideration of volume forces is:
1
∂v
+ (v∇)v = νL �v − ∇p.
∂t
̺L
(2)
Fig. 1 Definition of material and geometry parameters of the investigated vertical cylindrical liquid storage
tanks: R radius, H tank height, HL liquid height, d/E/ν thickness, Young’s-modulus and Poisson ratio of the tank
shell
Habenberger SpringerPlus (2015)4:515
Page 3 of 11
Under the assumption of small oscillation amplitudes, the contribution of the nonlinear expression (v∇)v in (Eq. 2) can be neglected:
1
∂v
= νL �v − ∇p.
∂t
̺L
(3)
By using the rotation of the velocity field ω = ∇ × v it is possible to transform the
Navier–Stokes-Equation into a simpler form (Landau and Lifschitz 1987):
∂ω
= νL �ω.
∂t
(4)
According to Eq. (4), the rotation of the velocity field ω corresponds to the heat equation. Hence, there is a convective transport of the velocity vortices from the surface into
the liquid. This process decays exponentially into the interior of the fluid. It is not possible for conservative forces to produce velocity vortices in a viscous fluid. There must
be forces which can not be derived from a potential (Schaefer 1950). In the present case
these are shear forces (frictional pressures) occurring at the tank wall. Concerning the
oscillation of storage tanks, vortices are produced at the tank wall due to frictional pressure. The velocity vortices decrease exponentially into the interior of the liquid. Because
of the exponential damping, the rotational flow occurs practically only in a small layer at
the tank wall. The main part of the liquid is an irrotational flow and can be described by
the following equation:
∇ × v = 0 ∇ · v = 0.
(5)
As derived from Eq. (5), one can see that v = 0 (the Navier–Stokes-equation becomes
the potential equation). Thus, the liquid behavior is everywhere in such a tank like this of
an ideal (incompressible and frictionless) fluid. Only in a thin layer on the tank wall the
potential flow is disturbed. The boundary conditions of a viscous liquid require the consistency of the liquid veloci (...truncated)