Jtam.dvi JOURNAL OF THEORETICAL AND APPLIED MECHANICS 41, 2, pp. 215-240, Warsaw 2003 ANALYSIS OF PARAMETRIC MODELS OF MR LINEAR DAMPER Bogdan Sapiński Jacek Filuś Department of Process Control, University of Mining and Metallurgy e-mail: deep@uci.agh.edu.pl This work deals with the analysis of parametric models of a MR linear damper, which suit various rheological structures of the MR fluid. The MR fluid structure and properties, damper description and parametric damper models which are connected in various ways with the actual behaviour of the MR fluid are presented. Based on computer simula- tions, the effectiveness of themodels under predictedMR linear damper behaviour is shown. The values of the parametric models used in the simulations were determined in an identification experiment. Keywords:MRfluid,MRdamper, rheological structure,modelling, iden- tification, simulation 1. Introduction MR dampers draw attention not only from a phenomenological point of view, but also from hope associated with their practical application in vibra- tion control of a dynamic structure. From the phenomenological viewpoint, the most important factors are, above all, high non-linear characteristics of these dampers (Gandhi and Chopra, 1996; Kamath andWerely, 1997; Snyder et al., 2000; Stanway et al., 2000; Wereley et al., 1998). Accordingly, a hyste- resis and jump-type phenomenon appears, which characterises the behaviour ofMRfluids. The explanation for these appearances depends on velocity. The relationship between the damping force and piston velocity for a linear MR damper of low efficiency is illustrated in Fig.1. This means that the non- linearity of hysteresis has greater significance for lower velocities, while for higher velocities non-linear jumps dominate. 216 B.Sapiński, J.Filuś Fig. 1. Character of force-velocity curve at: (a) low velocities – hysteresis phenomenon, (b) higher velocities – jump-type phenomenon These non-linearities create difficulties in the acceptance of such pheno- menological MR damper models, which make the behavioural prediction in its whole operating range impossible. They can also create limitations in the practical application of MR dampers. However, MR dampers contain certain features such as, quick response to changes of the control signal, full reflexivi- ty ofMR fluid transformations and low power consumption. These create the assumption that, in the future, MR dampers will be applied successfully to semi-active vibration control systems. Examples of the commercial use ofMR dampers have already been presented in, among others, Carlson and Sproston (2000). In the modelling, MR dampers can be divided into two main methods, parametric and non-parametric. In the parametric method, the damper is characterised by a system of linear and non-linear elements, which define the parameters of springs,dashpots andothermechanical elements, controlling the mechanismsandtheir operatingarea (Dyke et al., 1996). In thenon-parametric method, the damper is characterised by special well- suited functions (such as polynomials, hyperbolic tangent, delay, offset), or by a polynomial with the power of damper piston velocity (Choi et al., 2001), and the artificial intelligence methods (fuzzy logic or neural networks) (Sapiński, 2002). In this paper, the description of parametric models of a MR linear dam- per closely associating the actual MR fluid behaviour (Table 1) have been analytically formulated based on rheological laws. In these models, the dam- per is treated as a stationary system, whose dynamics can be described by differential equations. Analysis of parametric models of MR linear damper 217 Table1.Phenomenological parametricmodels ofMRdampers considering various rheological MR fluid behavioural scenarios MR fluid rheological behaviour No. MR dampermodel viscotic elastic plastic histeresis 1 Bingham ✓ ✓ 2 Bingham body ✓ ✓ ✓ 3 Gamota-Filisko ✓ ✓ ✓ 4 Li ✓ ✓ ✓ 5 Bouc-Wen ✓ ✓ ✓ 6 Spencer ✓ ✓ ✓ The acceptance of various rheological structures for the characterisation of MR fluid properties shows the effectiveness associated with these models as tools for prediction of the actual damper behaviour. Necessary for this is the knowledge of parametric values of themodel, which are designated on the basis of experiments undertaken for different periodic kinematic excitations of the piston and at several levels of the control current in the damper coil (Sapiński, 2002). 2. Structure and properties of MR fluids MR fluids belong to a group of fluids which are non-Newtonian, rheolo- gically stable, with a shear yield strength, and are controlled by a magnetic field. These fluids are non-coloidal suspensionswithmagnetic particles of high concentration in a non-magnetic fluid carrier. The materials applied as the magnetic particles are soft magnetic compounds (most common ferrous oxide Fe2O3 and Fe3O4 with magnetic saturation of about 1.9T). Water, silicon, mineral or synthetic oil and glycerol act as fluid carriers. Magnetic particles have a diameter of between 0.5µmand 8µm, therefore theMR fluids are also known as microfluids, as opposed to nanofluids and ferrofluids (Bolter and Janocha, 1998). The rheological properties of MR fluids depend on the concentration of magnetic particles, their size, shape, properties of fluid carriers,magnetic field intensity, temperature and also other factors (Jolly et al., 1999; Weiss et al., 1994). The interrelation of these factors is complex. The most important pa- rameters ofMRfluids are; maximum shear yield stress (50÷ 100)kPa,maxi- mummagnetic field ∼=250kA/m, plastic viscosity (0.1 ÷ 1.0)Pa·s, operating 218 B.Sapiński, J.Filuś temperature (−50 ÷ 150)◦C, density (3 ÷ 4)g/cm3. An essential feature of a MR fluid is its insensitivity to contamination. When no separate external magnetic field is applied (H = 0), the concentration of particles is diffused in the fluid carrier (Fig.2a), their magnetic moments are randomly directed and resultantly attain the zero value. The MR fluid shows then Newtonian behaviour. Fig. 2. Behaviour of MR fluid: (a) H =0, (b) H 6=0 In a magnetic field (H 6= 0), the aggregates are polarised and their ma- gnetic moments occur along the field lines in theMR fluid. These aggregates create chain-like structures which run parallel to the field lines (Fig.2b) and do not show thermal movements. The energy of the mechanisms necessary to create the chain structures increases alongside any increase in the magnetic field. TheseMR fluid properties change as a result of a meaningful formation of the shear stress, which in turn creates an increase in the viscosity. In their rheological behaviour, MR fluids can be divided into two charac- teristic areas, pre- and post yield (Li et al., 2000), to which the characteristic shear stresses τy,d and τy,s are respectively connected (Fig.3). The values of τy,d and τy,s respectivelymean that; dynamic shear yield stress (Ginder, 1996) (defined as the point of the zero-rate of the linear regression curve fit) and the static shear yield stress (defined as the shear stress necessary to initiate MR fluid flow) depend on themagnetic field. In the pre-yield area theMRfluid shows visco-elastic properties and a part of the energy required is regained (elastic behaviour) and a part is dissipated in the form of heat (viscotic behaviour). This behaviour can be explained by the linear visco-elastic theory. The Bingham body model is often applied in the research of MR fluid behaviour. In this model, in the post-yield area (for a stress greater than the shear stress, which depends on the magnetic field strain H, i.e. for τ ­ τy,d) Analysis of parametric models of MR linear damper 219 Fig. 3. (a) Shear stress-shear strain relationship ofMR fluid; (b) observed post-yield shear behaviour of MR fluid theMRfluid behaves like a viscoplasticmaterial. Assuming that τy,d = τ(H), the shear stress in theMR fluid is given by τ = τy(H)+ηγ̇ τ ­ τy(H) (2.1) where η – viscosity γ̇ – shear strain rate. However, in the post-yield area (for stress τ < 10−3Pa (Jolly et al., 2000)), the MR fluid behaves as a visco-elastic material and the fluid stress can be expressed as τ =G∗γ τ < τy(H) (2.2) where G∗ =G′+jG′′, is the complex shearmodulus dependent on themagne- tic field (Kormann et al., 1994), in which G′ means the storage modulus, and G′′ – lossmodulus.The storagemodulus is proportionally related to the avera- ge energy required during one fluid deforming cycle in volume units, however, the loss modulus is proportional to the average energy stored during a cycle in fluid volume units. In reality, the MR fluid behaviour shows wide depar- tures from Bingham’s model, the most important of which is non-Newtonian behaviour for H =0. The research on MR fluid reactions sometimes shows that through jump- type changes inmagnetic fields, thefluid stress changes have anasymptotically exponential character and gain 90% of their value in the time less than 10ms. This means that MR fluids change their viscosity rapidly. It was stated in (Snyder et al., 2000) that the changes inMR fluid properties from viscotic to 220 B.Sapiński, J.Filuś elastic follow a stress lower than 0.08% of the limited stress, which may limit the application of aMR fluid to adaptive structures, in which the stability is required in the pre-yield area. 3. Description of a MR damper The construction of aMR linear damper is shown in Fig.4a (longitudinal section) andFig.4b (cross section). The damper has a cylindrical shape and is filledwith aMRfluid.The piston constructionwith an integrated coil ensures that the magnetic field is focused within a gap, inside a volume of the active portion of theMR fluid. Fig. 4. (a) Longitudinal section: 1 – piston, 2 – rod, 3 – coil, 4 – gap, 5 –MR fluid, 6 – wires, 7 – housing, 8 – accumulator; (b) cross-section: 1 – piston, 3 – coil, 4 – gap The damper operation is based on using the MR effect, which amounts to quick changes in the viscosity of the active portion of the fluid in the gap (Kordoński, 1993; Shulman and Kordoński, 1978). In the absence of a magnetic field (I = 0 ⇒ H = 0), the aggregates of magnetic particles are suspended in the carrier fluid (Fig.2a), their magnetic moments are without any ordered structure and the resultant magnetic moment is equal to zero. In situations when external forces act on the piston, the damper resistance force depends, above all, on the fluid flow strain through the gap, resulting from the pressure differences between the cells from the fluid. Then the MR damper behaves like a viscotic damper. In the presence of an external field (I 6=0 ⇒ H 6=0), the aggregates are polarized and their magnetic moments are arranged along the field lines. These aggregates form chain-like structures parallel to the field lines (perpendicular to the fluid flow direction), thereby increasing the shear stress and the fluid viscosity and restricting its motion (Fig.2b). Themagnetic energy required to form such structures increases due Analysis of parametric models of MR linear damper 221 to the increase in the magnetic field. As a result, the fluid flow through the gapbecomes limited,which draws increased hydraulic resistance for the piston movement and creates an additional damping force component, depending on themagnetic field (intensity of the current in the coil). Due to the fact that the height of the gap in the damper is considerably less than its width and length (Fig.4a and Fig.4b) it can be seen that an adequate, accurate and comparative description of themathematical fluid flow through the gap is amodel with parallel plates (Spencer et al., 1998). On this assumption, the input to the damping force consists of three parts: the force resulting from the static friction (depending on the type used in the damper seal), the force depending on the fluid viscosity, and the force depending on the magnetic field (more precisely, on the distribution of the magnetic flux density in the gap). In order to control the MR damper, the pulse width modulation me- thod (PWM) of the current in the coil is used. The PWM controller creates rectangular voltage signals of an amplitude Am, and changeable co-factors αw = Ti/Tp, where Ti means the duration of the pulse, and Tp is set as the pulse repeat period (Fig.5). If the damper coil is supplied by the voltage si- gnal with this shape, the magnetic flux distribution is changed, which results in changes in the field line set-up in the damper magnetic circumference and related the damping force process. Fig. 5. Pulse width modulation The theoretical evaluation of the magnetic flux density set up along the gap l and themagnetic field in thedamper, in the casewhenthevoltage oncoil terminals is U =0V ⇒ I =0A and U =3.0V ⇒ I =0.6A, are shown in Fig.6 andFig.7, respectively (Sapiński et al., 2001). The experimental process of the damping force for sinusoidal kinematic excitation of the damper piston (at the amplitude of 4 · 10−3m and frequency 2.5Hz) and the step voltage input, U = 3.0V (I = 0.6A) and the connection time t1 = 0.488s, and disconnections time t2 =0.992s are shown in Fig.8 (Sapiński et al., 2001). 222 B.Sapiński, J.Filuś Fig. 6. Distribution of magnetic flux density along the gap for I =0.0A and I =0.6A Fig. 7. Distribution of magnetic field lines: (a) I =0.0A, (b) I =0.6A 4. Parametric models of MR linear dampers Theparametricdampermodelsare formulatedusingrheological structures, which, in various ways, approximate to the MR fluid behaviour, have direct influence on the accuracy of the damper behaviour prediction. Assuming, for example, that the MR fluid does not show hysteresis, it may be treated as a visco-plastic or visco-elastic material, which leads in the first case to the Bingham model, and in the second to the Bingham body, Gamota-Filisko and Li models. However, in view of the development in the MR fluids, the appearance of hysteresis leads to the Bouc-Wen or Spencer models. In order to analyse the above models, identification experiments were undertaken, the aim ofwhichwas to designate the parameter values for thesemodels necessary for simulation (Sapiński, 2002). Analysis of parametric models of MR linear damper 223 Fig. 8. Displacement vs. time; curent in the coil vs. time; damping force vs. time 4.1. Bingham model and Bingham body model The idealisation of the visco-plastic MR dampermodel presented in Dyke et al. (1996) uses similarities in the rheological behaviour of ERandMRfluids and the similar techniques in themodelling of ER dampers (Sims et al., 2000; Stanway et al., 2000). Fig. 9. Rheological structure of aMR damper for the Binghammodel In the rheological structure inFig.9, onwhich theBinghammodel is based, there is a Coulomb friction element fc placed parallel to the dashpot c0. According to Bingham’s MR damper model, for non-zero piston velocities ẋ, the damping force F can be expressed as F = fc sgnẋ+c0ẋ+f0 (4.1) where fc is the frictional force, c0 is the viscous damping parameter, f0 is the forcedue to thepresenceof theaccumulator.This last simplification in themo- 224 B.Sapiński, J.Filuś del results from the assumption that the elasticity replacing the accumulator activity has a low stiffness and linear characteristics. Fig. 10. Rheological structure of aMR damper for the Bingham body model The Bingham bodymodel, whose structure is presented in Fig.10, differs from the Binghammodel (Fig.9) by the introducing of a spring k. Thus, the Bingham body model tries merging of three elements, that is, connecting in parallel the elements of St.Venant (plastic bodymodel),Newton (Newtonflow model) and the element ofHooke (elastic bodymodel).Thismodel, through its low shear stress, presents solid body behaviour, however only through a high shear stress, the liquid body. This occurs because, to a certain value of the applied force fc (static friction force of the St. Venant element which refers to the shear stress τy(H) characteristic) only the springwill deform– similarly to the elastic Hooke body. If this force is greater than fc the Bingham bodywill elongate (the body flows). The rate of the deformation will be proportional to the difference of the applied force and the friction force of the St. Venant element (i.e. γ̇∼ [τ −τy(H)]). According to the Bingham bodymodel (see Fig.10), the damping force F can be expressed as F = { fc sgnẋ1+ c0ẋ1+f0 for |F|>fc k(x2−x1)+f0 for |F| ¬ fc (4.2) where the parameters fc, c0, f0 have the same meaning as in equation (4.1) and k represents the stiffness of the elastic body (Hooke model). 4.2. Gamota-Filisko model An extension of theBinghamMRdampermodel is the visco-elasto-plastic model formulated by Gamota and Filisko (Dyke et al., 1996). This extension depends on connection of the Bingham, Kelvin-Voight body and Hooke bo- dy models (Fig.11). The Kelvin-Voight model represents a solid body, whose maximumelongation exclusively depends on the applied force (independent of time). Analysis of parametric models of MR linear damper 225 Characteristic for thismodel is theappearanceof the creepingphenomenon (elongation gradually increases as a result of delayeddamperactivity).Hooke’s model, in turn, for which the spring elongation is proportional to the applied force and independent of time, represents the ideal elastic body. Fig. 11. Rheological structure of aMR damper for the Gamota-Filiskomodel The damping force in the Gamota-Filisko model (see Fig.11) can be de- scribed as F =      k1(x2−x1)+ c1(ẋ2− ẋ1)+f0 = c0ẋ1+fc sgnẋ1+f0 = k2(x3−x2)+f0 for |F|>fc k1(x2−x1)+ c1ẋ2+f0 = k2(x3−x2)+f0 for |F| ¬ fc (4.3) where c0,f0,fc – parameters representing the viscous damping, force due to the presence of the accumulator, frictional force (Bin- gham model) k1,c1 – parameters representing the stiffness and damping of the body (Kelvin-Voigt model) k2 – parameter representing the stiffness of the elastic body (Hooke model). It should be noted that when |F| ¬ fc, then ẋ1 = 0, which means that when the friction force fc related with the new stress in the fluid is greater than the damping force F, the piston remains motionless. 4.3. Li model Another view of visco-elasto-plastic properties of MR fluids in the model- ling of MR damper behaviour is the model composed by Li (Li et al., 2000). This model is divided into two areas; pre- and post-yield. In these areas the MR fluid shows visco-elastic and visco-plastic body properties, respectively, which conform to the rheological structures presented in Fig.12. 226 B.Sapiński, J.Filuś Fig. 12. Rheological structure of aMR damper for the Li model Li proposed a description of a MR fluid state in the pre-yield area of a visco-elasticmodel, inwhichHooke’s body (spring k2)was joinedwithKelvin- Voight’s body (spring k1 and dashpot c1). Besides the visco-elastic force fve, a contribution to the damping force F in the pre-yield area also carries the static friction force fs, resulting from the applied type of seal in the damper. Accordingly, the damping force F in the pre-yield area can be written as F = fve+fs (4.4) where the force fve is described by the equation ḟve+ k1+k2 c1 fve = k1 ·k2 c1 x+k2ẋ (4.5) where thedamping force F crosses theplastic flow force fc (when τ ­ τy(H)), the damper operates in the post-yield area. Then damping force is also equal to the visco-plastic force, to which, besides the friction force connected with the fluid shear stress fc, the viscotic force and inertial force contribute, which can be written as F = fc sgnẋ+ c2ẋ+mẍ (4.6) where c2 is a co-factor of viscotic friction, and m is the mass of replaced MRfluid dependent on the amplitude and frequency of a kinematic excitation applied to the piston. As such, the damping force in the Limodel is expressed as: equation (4.4) in the pre-yield area (|F| ¬ fc) and equation (4.6) in the post-yield area (|F|>fc). 4.4. Bouc-Wen model In structures showing hysteresis, through dynamic pressure (especially when the considered structure has a non-elastic character), the restoring for- ce depends not only on the moment of the displacement, but also on the Analysis of parametric models of MR linear damper 227 past events of the structure. This fact creates certain problems in the model- ling of structures with hysteresis creating vibration situations. To solve this problem, various approximation methods are applied (Brokate and Sprekels, 1996), which lead to variousmodels allowing the consideration of the hystere- sis in theMR andERdamper behaviour.McClamroch andGavin (1995) and Hsu andMeyer (1995) used trigonometric functions to describe the hysteresis. Fig. 13. Rheological structure of a MR damper for the Bouc-Wenmodel This approach, however, does not allow the consideration of the damping force saturationwhichoccurs inperiodsof highpistonvelocity. In turn,Werely et al. (1998) presented a biviscotic model with hysteresis, Sims et al. (2000) modified Bingham’s plastic model (Dyke et al., 1996), and the Choi (Choi et al., 2001) model, in which the dependence of the damping force on the velocity is a 6th order polynomial with respect to the piston velocity of the damper. A further development of the MR damper model, considering the appearance of the hysteresis and damping force saturation, is the Bouc-Wen model (Dyke et al., 1996), whose rheological structure is presented in Fig.13. In this model the hysteresis approximation method proposed by Wen (1976) is applied. Accordingly, in structures showing hysteresis, the restoring force Q(x,ẋ) is the sum of two components, without the hysteresis g(x,ẋ) and with h(x) Q(x,ẋ)= g(x,ẋ)+h(x)+ ... (4.7) The component h(x) is defined by an equation, which refers to the displa- cement x and z (evolutional variable), through which the position of the equation is dependent onwhether n is an even or odd number. For an odd n, the equation is ż=−a|ẋ|zn−βẋ|zn|+Aẋ (4.8) however for an even number ż=−a|ẋ|zn−1−βẋzn+Aẋ (4.9) 228 B.Sapiński, J.Filuś Fig. 14. Influence of parameters: n, β, γ,A, α on force-velocity curves The influence of n on the dependence of the MR damper force on the velocity, through the chosenparameters of theBouc-Wenmodel and for n=1, n=2, n= 3, is shown in Fig.14a. In Wen (1976) it is stated that using this method, the prediction accuracy of behavioural structures with hysteresis is satisfactory as compared with the experimental results gained for n=2. The damping force in the Bouc-Wen model can be written as F = c0ẋ+k0(x−x0)+αz (4.10) where the evolutional variable z is described by the equation ż=−γ|ẋ|z|z|n−1−βẋ|z|n+Aẋ (4.11) Analysis of parametric models of MR linear damper 229 where β,γ,A – parameters representing the control of the linearity du- ring unloading and the smoothness of the transition from the pre-yield to post-yield area α – parameter representing the stiffness for thedamping force component associated with the evolution variable z k0 – parameter representing the stiffness of the spring associa- ted with the nominal damper due to the accumulator c0 – parameter representing viscous damping c1 – parameter representing the dashpot included in the mo- del to produce the roll-off at low velocities x0 – parameter representing the initial displacement of the spring with the stiffness k0. The influence of the parameters β, γ, A, α on the accuracy of hysteresis prediction in the damping force-velocity curve is shown for the Bouc-Wen model in Fig.14b,c,d,e. 4.5. Spencer model The extension of the Bouc-Wen model proposed by Spencer concerns the introduction of an additional dashpot c1 and spring k1. This suits the rheolo- gical structure shown in Fig.15. Fig. 15. Rheological structure of aMR damper for the Spencer model Damping force in Spencer’s model can be expressed as F = az+ c0(ẋ− ẏ)+k0(x−y)+k1(x−x0) (4.12) 230 B.Sapiński, J.Filuś or can be also written as F = c1ẏ+k1(x−x0) (4.13) where the displacements z and y are respectively defined as ż=−γ|ẋ− ẏ|z|z|n−1−β(ẋ− ẏ)|z|n+A(ẋ− ẏ) (4.14) ẏ= 1 c0+c1 [az+ c0ẋ+k0(x−y)] The parameter c1 suits viscotic damping at higher velocities, the parameter k1 corresponds to the stiffness representing the accumulator, the parameter k0 stands for the stiffness at higher velocities, however, the remaining parameters in equations (4.12)-(4.14) have the samemeaning as in the Bouc-Wen model. 5. Identification experiment In order to simulate thedamperbehaviour through theuse of thedescribed models it is necessary todefine thevalues of their parameters.For thispurpose, experimental tests were carried out on the MR damper of RD-1005 type, produced by Lord Corporation. The scheme of the experimental setup for the damper tests is shown in Fig.16. Fig. 16. Scheme of the experimental setup for examinations of aMR linear damper The tests were conducted at the experimental setup, see Fig.16, with a computer-controlled INSTRON test machine, data acquisition system with the multi I/O board of RT-DAC3 type and in the software environment of Matlab/Simulink, and Real Time Workshop Target. The machine was pro- grammed to move up and down in a sinusoidal wave for seven levels of the Analysis of parametric models of MR linear damper 231 frequency f (0.5, 1, 2.5, 4, 6, 8, 10)Hz. The responsesweremeasured for eight levels of the control current I (0.0, 0.2, 0.4, 0.6, 0.8, 1.0, 1.2, 1.6)A. The way of conducting the tests and the parameter identification methods for the Bin- gham and Spencer models is carefully described by Sapiński (2002). Due to the requirements of this work, the identificationwas extended to theBingham body, Gamota-Filisko, Li and Bouc-Wen models. For the parameter computation the following criteria have been adopted (Spencer et al., 1998) εt = T ∫ 0 (Fe−Fm) 2 dt εx = T ∫ 0 (Fe−Fm) 2 ∣ ∣ ∣ dx dt ∣ ∣ ∣ dt (5.1) εẋ = T ∫ 0 (Fe−Fm) 2 ∣ ∣ ∣ dẋ dt ∣ ∣ ∣ dt where Fe and Fm denote the damping force derived from the experiments and models, respectively. The criteria define for each model the difference between Fe and Fm as a function of time (5.1)1, displacement (5.1)2 and velocity (5.1)3. For computation theCONSTR subroutine available inMatlab optimisation toolbox was used. The procedure finds the local minimumof the function of several variables under some constrains imposed on the variables. The parametric values of themodels obtained by this procedure are presented in Table 2-7. Table 2.Parameters of Bingham model Current Value of the parameter I [A] fc [N] c0 [Ns/m] f0 [N] 0.0 43.95 735.90 195.51 0.4 262.13 3948.70 186.28 Table 3.Parameters of Bingham bodymodel Current Value of the parameter I [A] fc [N] c0 [Ns/m] f0 [N] k [N/m] 0.0 43.95 735.90 195.51 895.00 0.4 262.13 3948.70 186.28 3623.00 232 B.Sapiński, J.Filuś Table 4.Parameters of Gamota-Filisko model Current Value of the parameter I [A] fc [N] c0 [Ns/m] c1 [Ns/m] k1 [N/m] k2 [N/m] fs [N] 0.0 43.95 735.90 2026.00 1387.00 895.00 195.51 0.4 262.13 3948.70 16487.00 8421.00 3623.00 186.28 Table 5.Parameters of Li model Current Value of the parameter I [A] fc [N] fs [N] c1 [Ns/m] c2 [Ns/m] 0.0 43.95 195.51 4983.00 12120.00 0.4 262.13 186.28 9987.00 6103.00 Current Value of the parameter I [A] k1 [N/m] k2 [N/m] m [kg] 0.0 998.10 10053.00 0.07 0.4 998.10 61432.00 0.07 Table 6.Parameters of Bouc-Wen model Current Value of the parameter I [A] α [N/m] c0 [Ns/m] A [-] β [m −1] 0.0 7507.50 549.86 125.18 1097222.00 0.4 38988.04 3195.43 215.20 1880301.00 Current Value of the parameter I [A] γ [m−1] k0 [N/m] x0 [kg] 0.0 1340385.00 1610.14 0.13 0.4 1696138.00 2169.09 0.92 Table 7.Parameters of Spencer model Current Value of the parameter I [A] α [N/m] c0 [Ns/m] c1 [Ns/m] k0 [N/m] A [-] 0.0 24830.30 553.90 38519.90 1037.4 25.70 0.4 86665.00 1965.10 20626.50 2807.8 29.37 Current Value of the parameter I [A] β [m−1] γ [m−1] k1 [N/m] x0 [kg] 0.0 1387320.0 3862730.00 651.50 0.30 0.4 1198420.0 52260.00 675.30 0.27 Analysis of parametric models of MR linear damper 233 6. Simulation of behaviour of a MR linear damper Based on the resulting parameters, the theoretical relationships were esta- blished for: damping force vs. time, damping force vs. displacement and dam- ping force vs. velocity, using Matlab/Simulink. As an example, these curves compared with the experimental data for f =2.5Hz; I =0A and I =0.4A are shown inFig.17,Fig.18 andFog.19, respectively.The lines ( ) indica- te the experimentaldata,while the theoretical curves aremarkedwith ( ). Fig. 17. Comparison of force-time, force-displacement and force-velocity curves betweenmeasurement ( ) and prediction ( ) for the Binghammodel: (a), (b), (c), for the Bingham body model: (d), (e), (f) Analysis of the results gained from the simulations and their comparison with the experimental data allows us to estimate the accuracy with which we can predict the actual MR damper behaviour using the consideredmodels with regard to various MR fluid properties (visco-plastic, visco-elasto-plastic, and visco-elastic with hysteresis). The quality of the visco-plastic Bingham model is its simplicity, however its shortcoming is that for zero piston velocity the damping force does not 234 B.Sapiński, J.Filuś Fig. 18. Comparison of force-time, force-displacement and force-velocity curves betweenmeasurement ( ) and prediction ( ) for the Gamota-Filisko model: (a), (b), (c), for the Li model: (d), (e), (f) equal zero, and that the force in the friction element is equal to the applied force. The force-velocity curve, which can be predicted with the use of this model, is one-to-one, but does not suit the experimental data (that is not one- to-one).At thevelocity equal to zero, themeasured force andacceleration have opposite signs: theadditional damping force–negative acceleration (additional displacement) and vice-versa. As a result of the spring employed in theBinghammodel, theMRdamper parametric model representing the visco-elasto-plastic model of the Bingham bodywas obtained. The effect of this spring is the proportional change of the damping force with velocity. The Gamota-Filisko model allows us to predict the force-velocity curve which more closely relates to the experimental data than in the Bingham body model. The characteristic feature of this model is that if the velocity approaches zero, the decrease in the damping c1, may generate the roll-off observed in the force-velocity curve (Dyke et al., 1996). The advantage of the visco-elasto-plastic model proposed by Li lies in the possibility ofmore accurate capturing ofMRdamper dynamic properties than Analysis of parametric models of MR linear damper 235 Fig. 19. Comparison of force-time, force-displacement and force-velocity curves betweenmeasurement ( ) and prediction ( ) for the Bouc-Wenmodel: (a), (b), (c), for the Spencer model: (d), (e), (f) in theGamota-Filiskomodel. That is due to distinguishingpre- andpost-yield areas of the MR fluid operating range. In addition, this model enables us to investigate the influence of the MR fluid inertia on the damping force (Li et al., 2000). The force-displacement curves predicted by the Bouc-Wen model are ac- curate in comparison to the experimental data (more accurate than in the visco-elasto-plastic models described above). However, at low velocities (si- milarly to the Bingham model) there appears a nonlinear character of the force-velocity curves, and therefore, it does not apply to the area in which the accelaration and the velocity have different signs. The visco-elastic model with the hysteresis formulated by Spencer enables us to the most accurately predicted actual MR damper behaviour (from the discussed models) in the whole operating range, also in the area of low velo- cities in which the acceleration and the velocity have different signs. It refers to all curves, i.e. force-time, force-displacement and force-velocity ones. 236 B.Sapiński, J.Filuś Fig. 17. Comparison of predicted force-velocity curves for consideredMR damper models: f =2.5Hz, I =0.4A 7. Summary In this paper, analysis of parametric models of MR linear dampers has been undertaken. The analysis has been concerned with various behaviour characteristics of a MR fluid, which fills the damper, i.e. visco-plastic, visco- elasto-plastic and visco-elastic with a histeresis. Based on the identification experiment, the parameters for these models were designated for a sinusoidal kinematic excitation and constant control current. The analysis showed that basic difficulties in formulation of the models, which could effectively portray Analysis of parametric models of MR linear damper 237 the actual behaviour of the MR damper were caused by the hysteresis and a jump-type phenomenon resulting from the specific properties of theMRfluid. This is illustrated in Fig.20, in which the force-velocity curves computed for each considered model are presented. It can be clearly seen that if the rheological structure representing the fluid behaviour in the model is too simple, then the predicted curves (force vs. time, force vs. displacement and force vs. velocity) becomes less accurate. The consequence of this is limitation of the applied models, an example of which may be Bingham’s model, which captures damper features well, but inaccurately represents its behaviour for near-zero piston velocity. Thismeans that Bingham’s model is not useful in control problems. The key factor is to take into account the magnetic field saturation, which is an inherent MR damper feature. There are also difficulties in finding the solution to some equations of the analysed models. This concerns, in particular, extended models taking into account the appearance of a hysteresis (Bouc-Wen and Spencer), which are difficult to solve analytically. 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Wereley N.M., Pang L., Kamath G.M., 1998, Idealized hysteresis mode- ling of electrorheological and magnetorheological dampers, Journal of Intelli- gent Material Systems and Structures, 9, 642 Analiza modeli parametrycznych liniowego tłumika magnetoreologicznego Streszczenie W pracy dokonano analizy parametrycznychmodeli fenomenologicznych liniowe- go tłumika magnetoreologicznego (MR), które odpowiadają różnym strukturom re- ologicznymcieczyMRwypełniającej tłumik. Przedstawionowłasności cieczy, budowę 240 B.Sapiński, J.Filuś tłumika orazmodeleparametryczne tłumikaprzybliżającewrożny sposób rzeczywiste zachowanie cieczy MR. W oparciu o symulacje komputerowe pokazano efektywność modeli do przewidywania rzeczywistego zachowanie liniowego tłumika MR.Wartości parametrówmodeli wykorzystywanew symulacjachwyznaczono na podstawie ekspe- rymentu identyfikacyjnego. Manuscript received October 1, 2002; accepted for print January 14, 2003