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7/26/2019 5 Chapter6.PDF BUN http://slidepdf.com/reader/full/5-chapter6pdf-bun 1/49 6.1 Basic concepts for enhanced damage control ....................................................................3 6.2 Bearings, isolators and energy dissipation units ................................................................3 6.2.1 General features ...............................................................................................................3 6.2.1.1 Force-Displacement Relationships .........................................................................4 6.2.1.1.1 Hysteretic Behaviour .........................................................................................4 6.2.1.1.2 Viscous Behaviour ............................................................................................. 4 6.2.1.1.3 Friction Behaviour .............................................................................................. 4 6.2.1.2 Isolation/Dissipation Systems Issues ......................................................................5 6.2.2 Elastomeric bearings ........................................................................................................ 6 6.2.2.1 Rubber Bearings and Laminated Rubber Bearings ..............................................6 6.2.2.2 High Damping Rubber Bearings (HRDB) ...............................................................9 6.2.2.2.1 Rubber properties .............................................................................................. 9 6.2.2.2.2 Preliminary Design for HRDB Isolating Systems ..........................................9 6.2.2.3 Lead Rubber Bearings (LRB) .................................................................................10 6.2.2.3.1 Rate dependence and Other factors in rubber bearing design ................11 6.2.2.3.2 Preliminary Design for LRB Isolating Systems ............................................12 6.2.2.4 Allowable Shear Strain and other Code Reccomendations ..............................14 6.2.2.4.1 AASHTO (2000) Reccomendations .....................................................................14 6.2.2.4.2 EC8 Reccomendations ..........................................................................................15 6.2.2.5 Basic Hysteretic Behaviour and Advanced Analytical Hysteresis Models ......17 6.2.2.6 Lead Rubbers Damper and Oil Dampers .............................................................17 6.2.3 Sliding devices ................................................................................................................17 6.2.3.1 The Friction Pendulum System ..............................................................................18 6.2.3.1.1 Basics Hysteretic Behaviour ..............................................................................19 6.2.3.1.2 Modelling Issues of the Friction Pendulum System .......................................21 6.2.4 Metallic and Friction Dampers ......................................................................................22 6.2.4.1 Basic Hysteretic Behaviour and Dynamic Response with Metallic/Friction devices 22 6.2.4.2 Friction Dampers ...................................................................................................... 22 6.2.4.2.1 Advantages and Disadvantages of Friction Dampers and Environmental Effects 22 6.2.4.2.2 Slotted-bolted Connections ............................................................................23 6.2.4.3 Steel Hysteretic Dampers .......................................................................................24 6.2.4.3.1 C-shaped Device ................................................................................................. 24 6.2.4.3.2 The EDU Device .................................................................................................. 25 6.2.4.3.3 ADAS and TADAS Elements .............................................................................26 6.2.4.3.4 Lead Extrusion Devices (LEDs) ........................................................................27 6.2.4.3.5 Conceptual Design: concepts of yield/slip shear and Optimization criterion 27 6.2.5 Viscous and Viscoelastic Dampers ..............................................................................28 6.2.5.1 Viscous Dampers ..................................................................................................... 28 6.2.5.1.1 Basic Hysteretic Behaviour of Viscous Dampers ...........................................28 6.2.5.1.2 Design considerations ........................................................................................30 6.2.5.1.3 Fabrication and Detailing Issues .......................................................................30 6.2.5.1.4 Effects of Supplemental Viscous Damping on Asymmetric-Plan Systems 30 6.2.5.2 Viscoelastic Dampers .............................................................................................. 31 6.2.5.2.1 Basic Hysteretic Behaviour of VE Dampers and Dynamic Analysis of VE Dampers Equipped Structures ............................................................................................ 31 6.2.6 Self-Centering Dampers ................................................................................................ 32 6.2.6.1 Shape Memory Alloys Dampers (SMA) ................................................................32 1 6. 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6.1 Basic concepts for enhanced damage control ....................................................................3

6.2 Bearings, isolators and energy dissipation units ................................................................36.2.1 General features ...............................................................................................................3

6.2.1.1 Force-Displacement Relationships .........................................................................46.2.1.1.1 Hysteretic Behaviour .........................................................................................46.2.1.1.2 Viscous Behaviour .............................................................................................46.2.1.1.3 Friction Behaviour ..............................................................................................4

6.2.1.2 Isolation/Dissipation Systems Issues ......................................................................56.2.2 Elastomeric bearings ........................................................................................................6

6.2.2.1 Rubber Bearings and Laminated Rubber Bearings ..............................................66.2.2.2 High Damping Rubber Bearings (HRDB) ...............................................................9

6.2.2.2.1 Rubber properties ..............................................................................................96.2.2.2.2 Preliminary Design for HRDB Isolating Systems ..........................................9

6.2.2.3 Lead Rubber Bearings (LRB) .................................................................................106.2.2.3.1 Rate dependence and Other factors in rubber bearing design ................116.2.2.3.2 Preliminary Design for LRB Isolating Systems ............................................12

6.2.2.4 Allowable Shear Strain and other Code Reccomendations ..............................146.2.2.4.1 AASHTO (2000) Reccomendations .....................................................................146.2.2.4.2 EC8 Reccomendations ..........................................................................................156.2.2.5 Basic Hysteretic Behaviour and Advanced Analytical Hysteresis Models ......176.2.2.6 Lead Rubbers Damper and Oil Dampers .............................................................17

6.2.3 Sliding devices ................................................................................................................176.2.3.1 The Friction Pendulum System ..............................................................................18

6.2.3.1.1 Basics Hysteretic Behaviour ..............................................................................196.2.3.1.2 Modelling Issues of the Friction Pendulum System .......................................21

6.2.4 Metallic and Friction Dampers ......................................................................................22

6.2.4.1 Basic Hysteretic Behaviour and Dynamic Response with Metallic/Frictiondevices 226.2.4.2 Friction Dampers ......................................................................................................22

6.2.4.2.1 Advantages and Disadvantages of Friction Dampers and EnvironmentalEffects 226.2.4.2.2 Slotted-bolted Connections ............................................................................23

6.2.4.3 Steel Hysteretic Dampers .......................................................................................246.2.4.3.1 C-shaped Device .................................................................................................246.2.4.3.2 The EDU Device ..................................................................................................256.2.4.3.3 ADAS and TADAS Elements .............................................................................266.2.4.3.4 Lead Extrusion Devices (LEDs) ........................................................................27

6.2.4.3.5 Conceptual Design: concepts of yield/slip shear and Optimization criterion 27

6.2.5 Viscous and Viscoelastic Dampers ..............................................................................286.2.5.1 Viscous Dampers .....................................................................................................28

6.2.5.1.1 Basic Hysteretic Behaviour of Viscous Dampers ...........................................286.2.5.1.2 Design considerations ........................................................................................306.2.5.1.3 Fabrication and Detailing Issues .......................................................................306.2.5.1.4 Effects of Supplemental Viscous Damping on Asymmetric-Plan Systems 30

6.2.5.2 Viscoelastic Dampers ..............................................................................................316.2.5.2.1 Basic Hysteretic Behaviour of VE Dampers and Dynamic Analysis of VEDampers Equipped Structures ............................................................................................31

6.2.6 Self-Centering Dampers ................................................................................................326.2.6.1 Shape Memory Alloys Dampers (SMA) ................................................................32

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6.2.6.1.1 Application of SMA restrainer to multi-span bridges ..................................326.2.6.1.2 Macroscopic Hysteretic Behaviour of the SMA ...........................................33

6.2.6.2 SCD Typologies: The Energy Dissipating Restraint ...........................................346.2.6.3 The Friction Spring Seismic Damper ....................................................................34

6.2.7 Electro and Magnetorheological Dampers .................................................................356.2.7.1 Control Strategies with MR/ERDs .........................................................................35

6.2.7.1.1 Optimal Force Control .....................................................................................356.2.7.1.2 Optimal Displacement Control .......................................................................35

6.2.7.2 Magneto-Rheological Dampers .............................................................................366.2.7.2.1 Monotube and Twin Tube Magneto-Rheological Dampers .......................366.2.7.2.2 MR Damper Model ...........................................................................................37

6.2.7.3 Electro-inductive devices ........................................................................................376.2.7.3.1 Viscous and Adjustable friction-type forces for ElectrorheologicalDampers 386.2.7.3.2 Effects on rigidity-plasticity, viscosity of ER dampers with near-fieldground motion .....................................................................................................................38

6.3 Design concepts and analysis of deck – isolated bridges ..............................................396.3.1 Analysis concepts ...........................................................................................................396.3.2 Basics of capacity design ..............................................................................................406.3.3 Considerations on input characteristics ......................................................................40

6.4 Foundation rocking and pier base isolation ......................................................................406.4.1 Basics of foundation rocking .........................................................................................406.4.2 soil – structure interaction (contribution from Alain) ..................................................416.4.3 pier base isolation ...........................................................................................................41

6.5 Controlled rocking of piers and built–in isolators ..............................................................41

6.5.1 Controlled rocking of combined concrete members ..................................................416.5.2 Response of partially prestressed coupled members ...............................................446.5.3 design and analysis of segmented piers .....................................................................466.5.4 built – in isolators (contribution from Kazuhiko) .........................................................46

6.6 References .............................................................................................................................47

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6. Design for enhanced control of damage

6.1 Basic concepts for enhanced damage control

A very attractive way of improving the seismic performance of a structure is given by the possibility of an artificial increase of both the period of vibration and the energy dissipationcapacity of the system. This can be obtained by making use of specific artificial elements designedto isolate part of the structure from the full intensity of the seismic motion (reduction of the sesimicenergy transfer into the structure) and/or to dissipate a large amount of energy (dissipation of theinput energy, thus reducing the plastic deformations in the structure and also concentrating damagein these elements, that can be easily substituted). The first type of elements (Isolation devices) havethe main objective to increase the period of vibration of the structure towards a lower amplificationrange of the response spectrum for the design ground motion, thus reducing the input energy (i.e.force demand) into the structure; The second type of elements (Dissipation devices) provide mainlythe supplemental damping thus reducing the displacement demand on structural or non-structuralelements. The combination of these kind of devices will define an isolation system.In bridges, where the objective is to protect relatively low-mass piers and their foundations,isolators and dissipators are usually placed between the top of the piers and the superstructure. Theviscous damping and hysteretic properties of isolators are generally selected to maintain allcomponents of the superstructure within the elastic range, or to require only limited ductile action.The bulk of the overall displacement of the structure can be concentrated in the isolatorcomponents, with relatively little deformation within the structure itself, which moves largely as arigid body mounted on the isolation system.

6.2 Bearings, isolators and energy dissipation units

In most cases a base isolation is adopted in order to increase the period of vibration of a rigidstructure and thus reduce the amount of the seismic input energy on the system. In the case of

bridges, that usually have a simple structural configuration, made by a continuous deck supportedon the top of the pier by simple bearings only with the function of supporting gravity loads, this can

be easily obtained by designing such bearings as Isolation/Dissipation devices (I/D) or bycombining them with dissipative elements in order to define an isolation system between piers anddeck.

6.2.1 General features

The functions of an isolating/dissipating system are generally one or a combination of thefollowing: (i) supporting gravity loads and providing for (ii) lateral flexibility (period shift), (iii)restoring force and (iv) energy dissipation (either of hysteretic, in the case of displacement activateddampers, or viscous nature, in the case of velocity activated dampers);According to their performance, the anti-seismic devices can be grouped in: rigid connectiondevices (e.g. shear links, lock-up devices), linear devices, non linear devices, viscous dampers,isolators (e.g. sliders, rubber bearings). Common types of anti-seismic devices are:• Elastomeric bearings: Natural Laminated, Lead and High Damping Rubber Bearings (HDRB);• Friction Dampers;• Metallic Dampers (sometimes combined with bearings to form sliders): yielding steel systems,

lead extrusion devices;• Viscous and Viscoelastic Dampers: Taylor Devices;• Self-centring Dampers: Shape Memory Alloys, Energy Dissipation Restraints, SHAPIA Devices;

• Lock-up Devices (sometimes combined with Hysteretic Dampers);

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6.2.1.1 Force-Displacement Relationships

In general, the design properties of isolators/dissipators depend on their behaviour, which may beone or a combination of the following:

6.2.1.1.1 Hysteretic Behaviour

The force-displacement relation of the isolator unit may be approximated by a bilinear relation(Fig.6-1 , left). The parameters of the bi-linear approximation are: the yield force at monotonicloading F y, the force at zero displacement at cyclic loading F 0, the elastic stiffness at monotonicloading K e (equal to the unloading stiffness at cyclic loading), the post elastic (tangent) stiffness K p,the energy dissipated per cycle E D at the design displacement d d, (equal to the area enclosed by theactual hysteresis loop).

6.2.1.1.2 Viscous Behaviour

The force of viscous devices is proportional to v α , where v is the velocity of motion. This force iszero at the maximum displacement and therefore does not contribute to the effective stiffness of theisolating system. The force-displacement relationship of a viscous device is shown in Fig.6-1 (right)(for sinusoidal motion), and depends on the value of the exponent α.

Fig.6-1. General Hysteretic behaviour (left), and Viscous behaviour (right).

6.2.1.1.3 Friction Behaviour

Type 1) Sliding devices, with flat sliding surface, limit the force transmitted to the superstructure to:

)d(signNF sddmax&µ= (6-1)

where N sd is the normal force through the device ( Fig.6-2 , left). Due to the possible substantial permanent offset displacements, they should be used in combination with devices providing anadequate restoring force.

Type 2) Sliding devices, with spherical sliding surface of radius R b

(e.g. Friction PendulumBearings), provide a restoring force proportional to the design displacement d d (equation (6-2) andFig.6-2 , right), and a force displacement relationship given in equation (6-3) The equation (6-3) is asmall displacement approximation.

db

sdrestoring d

RN

F = (6-2)

)d(signNdRN

F sdddb

sdmax

&µ+= (6-3)

In either of the two cases, the energy dissipated per cycle E D at the design displacement d d is:

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dsddD dN4E µ= (6-4)

Fig.6-2. Sliding Friction Hysteretic behaviour for Flat (left) and Curved (right) Surfaces

6.2.1.2 Isolation/Dissipation Systems Issues

A number of issues are related to the employment of isolator and dissipator devices, among these:

• I/D devices also show some inherent problems: the properties of seismic isolation bearings, infact, vary due to the effects of wear, aging, temperature, history nature of loading, etc.• Advanced Modelling Issues. The illustrated representations of the global force-displacement

relationships of the devices are in general a first approximation of the actual behaviour: thedifferences in advanced and simplified models may lead to differences in the structural responsewhose importance has to be evaluated. Once refined models for different isolation systems aredeveloped, it should be studied how they influence the structural response, in order to find out

protection factors for different isolation systems, when a simplified model of the devices isemployed. In other words, if the seismic demand on piers, or generally on the structure, increaseswhen the refined models are used, the simpler modelling might be allowed, provided thatadequate protection factors are accounted for. The concept of Property Modification Factors has

been introduced by Costantinou et al. (1999) in order to characterise the variability of thenominal properties of an isolator and understanding the consequences on the device andstructural response. EC8 provisions require that, in addition to the set of nominal DesignProperties derived from the propotype tests, two sets of design properties of the isolation systemshall be properly established (Upper and Lower bound design properties). AASTHO provisionsare similar.

• Re-centering problem. The problem of re-centring the bearing in its original position after anevent that cause any kind of offset is relevant in designing the Isolation/Dissipation system. Only

pure spring with zero-damping are perfectly re-centring, while energy dissipation generatesresidual displacements; particularly, anti-seismic devices based on friction may offset due tothermal effects or small earthquakes as long as the friction force is equilibrated by the re-centringforce. On the contrary hysteretic dampers, up to yielding, act as perfect springs.

• The Heat Generation Problem. The heat generation due to the relative movement in the devicemight be a problem for the correct functioning or the life of the isolator/dissipator itself. Marioni(2002) analysed numerical examples of different devices, having the same characteristics interms of period of the isolated structure, design displacement and number of cycles during theearthquake. Table 6-1 shows a comparison among the devices performances in terms oftemperature increase per cycle: it can be easily seen that heat generation may be critical for somekind of energy dissipating anti-seismic devices, for which full scale dynamic tests are envisaged.

• As the whole thrust of seismic isolation is to shift the probable damage level and thereby thedamage costs, the economic factors need also to be considered by an engineer wishing to decidewheter a structure should incorporate seismic isolation: maintenance costs should be low for

passive systems, whilst the construction costs including seismic isolation usually vary by 5-10%from not isolated options.

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Table 6-1. Comparison of Temperature Increase per Cycle for Different Antiseismic Devices

Thermal Capacity(kJ/kg°C) Temperature lncrease/Cycle (°C)

Hysteretic Steel Dampers(under flexure) 0.502 (steel) 5.33°C

LRB 0.129 (lead) 27.3°C

HRDB 0.8 (rubber) 6.4°C

Friction Device 0.502 (steel)

(temperature given by the solutionof Fourier Equation, as a functionof time and distance from theinterface)

Viscous Dampersthermal behaviour as a function ofthe pressure and the size of thedamper

6.2.2 Elastomeric bearings

An elastomeric isolation bearing consists of a number of rubber layers and steel shims, bonded inalternating layers, to produce a vertically stiff but horizontally flexible isolator. The alternating steeland rubber layers act to restrain the rubber layer from bulging laterally.This kind of bearings can provide for flexibility and hysteretic/viscous damping forces. They can beeither low damping or high damping bearings. The insertion of a lead plug in an elastomeric isolator

provides energy dissipation for seismic response and stiffness for static loads.They can be grouped in (i) Natural Rubber Bearings, (ii) High Damping Rubber Bearings (HDRB)and (iii) Lead Rubber Bearings (LRB).

6.2.2.1 Rubber Bearings and Laminated Rubber Bearings

Typical Laminated Rubber Bearings ( Fig.6-3 left, and Fig.6-4 ) characteristic parameters are thevertical load capacity, the bearing horizontal and vertical stiffnesses, the bearing lateral period, the

bearing damping and the allowable seismic displacement, as described hereafter.Low damping elastomeric bearings have an equivalent viscous damping ratio ξ ≈ 0.05 (±20%).Their behaviour may be approximated by that of a linear elastic element, with unscragged secantshear modulus at shear strain of 2.0, G = 1.0 MPa (±15%).

Fig.6-3. Sketch of a Laminated (left) and Lead (right) Rubber Bearings.

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Fig.6-4. Plan and Cross Section of low shape factor Rubber Bearings with doweled (left) and bolted(right) end-plate connection (EERC).

• VERTICAL LOAD CAPACITY W

WGS' AW γ< (6-5)

iBearingCircular

iyxyxBearinggular tancRe

t4/DS

t)bb(2/bbS

=+= (6-6)

In equation (6-5) γW is the allowable shear strain (when rubber is assumed to beincompressible=6S εz, (Skinner et al, 1997)); A’ is the overlap of top and bottom area (A) of bearingat maximum displacement ( Fig.6-5 ), and it ranges from 0.4A to 0.7A, but a value of 0.6 is typicallyused for design earthquake; G ( ≈1MPa), is the shear modulus of rubber; S is the bearing shapefactor, i.e. the loaded to force-free area ratio of the rubber layer and it is a function of the inverse ofthe i th layer thickness t i, generally ranging 3 to 40.The allowable vertical stress on the gross area is on the order of 5 ÷10MPa, but it is indirectlygoverned by limitation on the equivalent shear strain in the rubber due to different loadcombinations and stability requirements.

Fig.6-5. Rubber Bearing with recessed plate connection: undeformed and deformed configurations .

• BEARING HORIZONTAL STIFFNESS K b AND LATERAL PERIOD T b

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h/GAKb = (6-7)

5.0xz

5.0bb ) Ag/' ASh(2)K/M(2T γπ=π= (6-8)

In equations (6-7) and (6-8) h is the total rubber height, i.e. the sum of the layer thicknesses, M isthe beard mass and g the acceleration of gravity. K b is in the order of 1 ÷2MN/m. The actual value

of the lateral stiffness might be affected by the amount of vertical load which depends also on thedisplacement demand (this effect is usually negligible with S=10÷20).There will be some reduction in the bearing height with large displacements, partly due to flexural

beam action and partly to the increased compression of the reduced A’ . The resulting inverted pendulum action, under structural weight, reduce K b, and in extreme cases also re-centering forces,can be reduced by increasing S up to 10 ÷20. This problem has been accurately studied by differentauthors (Kikuchi and Aiken, (1997), Nagarajaiah and Ferrell, (1999), Buckle et Al., (2002)).T b is in the order of 2 ÷3 sec. The second part of equation (6-8) is obtained substituting the (6-5) and(6-7) in the first part: the lateral period results to be a function of the square root of bearing heightto layer thickness ratio, (h/t) 0.5.

• BEARING VERTICAL STIFFNESS K v The vertical deflection of a bearing is the sum of the deflection due to the rubber shear strain and tothe rubber volume change. The respective stiffnesses are:

h/ AK

h/ AGS6K

changevolumez

2strainshear z

κ==

−(6-9)

Where κ (≈ 2000MPa) is the rubber compression modulus; the resulting vertical stiffness,corresponding to the two stiffnesses in series is:

h)GS6/( AGS6K 22z κ+κ= (6-10)

It is in the order of 1000 ÷2000MN/m.

• ALLOWABLE SEISMIC DISPLACEMENT ∆ b It can be limited by either the seismic shear strain γs or the overlapping area factor. In the first caseit is given by:

sstrainshear seismicb hγ=∆ − (6-11)

The allowable limit for the seismic shear strain γs, depends on how much shear strain γW (equation(6-5)) is mobilised by the vertical load. The bearings in fact must withstand the combined rubbershear strains due to structural weight and seismic displacement. For bridges, additional shear strainsdue to traffic loads and thermal displacements must be accounted for. The damaging effect of agiven rubber strain increases with its total duration and number of cycles.Sustainable steady shear strain in a rubber bearing is (Bridge Engineering standards, 1976):

tuw 2.0 ε=γ (6-12)

Where εtu is the short-term failure tensile strain, ranging from 4.5 to 7.Under combined action of uplift and end moments, the rubber undergoes to large negative

pressures, possibly causing small cavities in the rubber, which grow progressively during sustainedand cyclic negative pressures. These cause a large reduction in the axial stiffness, but little in thehorizontal stiffness. It is usual to design bearings so that negative pressures don’t occur, or occurwith low frequencies and durations. Higher negative pressures can be avoided through a proper

detailing. This last issue is also important in modelling of the rubber bearing.A limit to the displacement is provided also by the overlapping area ratio (A’/A). Allowing anoverlapping area ratio of 0.6, the allowable seismic displacement is in the order of magnitude of

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D/3 and b/3 respectively in the case of a circular bearing with diameter D (equation (6-13)) and arectangular bearing with size b in the direction of the displacement (equation (6-14) ) (withdisplacement in any possible direction an approxiamtion is given by equation (6-15)).

⎟ ⎠ ⎞

⎜⎝ ⎛ −≅∆ − A

' A 1D8.0BearingCircularb

(6-13)

⎟ ⎠ ⎞

⎜⎝ ⎛ −=∆ − A

' A 1BB/ /b

(6-14)

⎟ ⎠ ⎞

⎜⎝ ⎛ −≅∆ − A

' A 1b8.0BearinggulartancReb

(6-15)

6.2.2.2 High Damping Rubber Bearings (HRDB)

HRDB consist of alternate layers of rubber and steel plates of limited thickness bonded byvulcanization, being able to support vertical loads with limited deflection, due to very high verticalstiffness. As well, they are able to support operating horizontal loads (e.g. wind), with very lowdisplacements. Their life time is over 60 years.HRDB can provide both period shift and energy dissipation: the rubber compound presentsdamping capability, at least corresponding to 10% of equivalent viscous damping, and normallydependent on the bearing displacement. The rubber compound is designed to withstand very largeshear deformations, much larger than the standard elastomeric bearings. The rubber compoundstiffness is much higher (up to 4 times) for small deformations and reduces for large deformations.The fixation to the structure is based on positive connections: HRDB can transfer very largehorizontal load to the structures, either by recess or dowels or by bolts. In the first case the rubber isnot subjected to tensile stresses, but tan γmax=1.4 to limit bending of the steel plates vulcanised to therubber and prevent risk of roll-over; in the latter case the maximum shear strain is achieved but therubber has to have extremely high mechanical properties due to the high stress level it undergoes.

6.2.2.2.1 Rubber propertiesPhysical-mechanical rubber characteristics refer to CNR10018, AASHTO (sec.14/25), BS5400,European Standards pr EN1337. A range of variability of rubber properties is provided in Table 6-2.Scragging occurs in elastomeric bearings that are subjected to one or more cycles of high sheardeformation before testing. Scragged bearings show a significant drop of the shear stiffness insubsequent cycles. It appears however that the original (virgin) shear stiffness of the bearings is

practically recovered after a certain time (a few months). This effect is prominent mainly in high

damping and in low modulus bearings.Table 6-2. Rubber Properties (Alga Spa, 2003)

Compound Characteristic SOFT NORMAL HARDhardness (Shore A3) 40±3 60 ±3 75 ±3tensile strain (%) 20 20 18tensile strenght (MPa) 750 600 500G (MPa) 0.4 0.8 1.4equivalent viscous damping (%) 10 10 16

6.2.2.2.2 Preliminary Design for HRDB Isolating SystemsIn preliminary design of HRDB Isolating Systems, simplifying assumptions are that the isolators actlike perfect springs connecting deck and piers and that piers will be stiff enough to neglect their

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their deformation. Assuming also that the deck behaves as a rigid mass, the whole bridge can beidealized as a single-degree-of-freedom-system (SDOF system) with mass the deck mass andstiffness the isolation system stiffness. The mass of the structure is known, the designer has tochoose:• The structural period (normally between 2 and 3s) and the relative stiffness (total stiffness of the

base isolators).

• The equivalent viscous damping of the HRDB isolators (normally ranging between 10% and16%), through which spectral response values Sa and Sd can be determined and reduced with the parameter (EC8, prEN 1998-1):

55.05

10

eq

≥ξ+

=η (6-16)

• The design shear strain of the rubber tan γ: the thickness can be determined through the relativedisplacement Sd.

γ=

tanS

h d (6-17)

The net rubber thickness shall be increased to allow for the movements due to temperature,creep and shrinkage (Code provisions are presented at §6.2.2.4).

• The rubber shear modulus, through which the total area of the isolators can be found:

GhK

A b= (6-18)

Now dimensions of the single unit can be determined, provided that allowable vertical pressure is 7-15 Mpa (for G=0.7-1.4 Mpa) or 4-10Mpa (for G=0.4-0.7 Mpa) and buckling be prevented.It is generally necessary to reduce the number of different types of isolators and to check themanufacturer availability. The preliminary design of the base isolators has to be followed by a morespecific one.

6.2.2.3 Lead Rubber Bearings (LRB)

The insertion of a lead plug in the laminated rubber bearing provides energy dissipation for seismicresponse and stiffness for static loads ( Fig.6-6 ).Parameters characterising the system are the yielding shear and the sustainable post-yielding shearforce, respectively in equations (6-19) and (6-20). Where τ ly is the lead yield shear strength ( ≅ 10.5MPa), and Gl is the lead initial stiffness ( ≅ 130MPa). The yielding Shear is the total bearingshear at the lead yield displacement, i.e. approximately the lead yielding shear (the rubbercontribution is very small respect to the lead contribution at this displacement), and the sustainable

post-yielding shear force is the shear at the design displacement of the isolator.

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GhK

A b= (6-19)

GhK

A b= (6-20)

G lA l/h+G rAr/h

G rAr/hVly+G rAr∆y/h

y u

Vly+G rAr∆u/h

Lead

Rubber

Fig.6-6. Schematic Bilinear Constitutive Law (left) and Comparison of shear force-displacement loops for elastomeric bearings with and without lead plug (EERC) (right)

The initial elastic stiffness has been estimated from experimental results in the range of 9 ÷16K br (stiffness of the rubber in a horizontal plane). The size of the lead plug is proportional to the yieldstrength of the isolator (at this displacement, the rubber contribution is usually neglected, being verysmall respect to the lead contribution), while the post yielding stiffness is proportional to the rubber

bearing stiffness, varying from it by up to ±40%, but more likely within ±20%.The maximum force has an uncertainty of ±20%. This simplified bi-linear model ( Fig.6-6 , right)has a hysteresis loop approximately 20% greater than the actual one.Most of the self-centering property of the laminated rubber bearing is lost with the lead insertion.

6.2.2.3.1 Rate dependence and Other factors in rubber bearing designIf bridge deck is mounted on LRBs, because of the daily temperature excursion, the bearing has toaccommodate displacements of the order of few millimitres, without producing large forces.It has been found this kind of relationship for the rate dependence:

⎩⎨⎧

×>γ÷×≤γ÷=

γ=τ

−−

−−

14

14

bl

s103035.003.0s10315.013.0

b

a

&&

&

(6-21)

In relationship of type of (6-21), in which a is a constant parameter, was found for the ratedependence, meaning that the rate dependence at typical seismic frequencies (1Hz) is low, in theorder of a force increment of 8% for a rate increase of a factor of 10, while for slow frequencies it ismore important (a force increment of 40% for the same change of rate).The LRB is not strongly dependent on fatigue and temperature excursions within -35° / +45°. Theeffects of vertical load on hysteresis are not relevant if the device is properly designed (e.g. S>10).

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6.2.2.3.2 Preliminary Design for LRB Isolating SystemsThe design of the Lead Rubber Bearing (LRB) System might be done, in a preliminary stage, byreducing the structural system to an equivalent SDOF system in which the contributions of nisolators in parallel are summed.The following parameters have to be designed: the area of the rubber A r , to be split in n isolators;the area of the lead A l, to be split in n isolators; the height of the lead, i.e. of the isolator, h l, that isthe same for the n isolators. The equivalent single LRB can be found comparing the two systems ofone isolator, with A r , A l and h l, and n isolators, with A r /n, A l/n and h l, in Table 6-3, where the indexi corresponds to the individual isolator unit.

Table 6-3. Equivalent SDOF isolator

One isolator (with Ar, Al and h) n isolators (with Ar/n, Al/n and h each)

h/ AGK r r r = h/)n/ A(GK r r ri =

yllr r

uui )n/ A(h

)n/ A(GDV τ+=

yllr r

uu Ah AG

DV τ+= uiu nVV =

It has to be noted that the same stiffness of the two systems can be obtained just imposing thataspect ratio of the equivalent SDOF isolator be n times the aspect ratio of the n isolators.

Nevertheless this would change the ultimate shear, which depends only on the lead area, and theyielding displacement, which depends only on the lead height. Therefore, the dampingcharacteristics of the system would be altered.

Preliminary design is based on the following observations:• The mass of the structure to be isolated is known;• The system is reduced to an equivalent SDOF system with the mass equal to the first mode mass

M1; the 1st mode mass participation factor might be eventually guessed in the order of MPF =0.95, (to be checked).

• The equivalent viscous damping of the system is calculated as the equivalent viscous damping ofthe cycle at the maximum displacement of the system. Clearly the estimated damping results to

be an upper bound, as the energy dissipated over the duration of the earthquake has contributionsof high and low cycles. The spectral response value Sd can be determined and reduced with the

parameter η of equation (6-16).A very preliminary design might follow the steps listed below, assuming the post-yielding

stiffness K 2 as one tenth of the initial elastic stiffness K 1:• Choice of the isolation period T I: (normally of 2-3s) as an initial trial value.• The S d corresponding to the chosen period is taken from the 5% damping Response Spectrum. A

damping value is selected in order to achieve a displacement below a design target value.• The corresponding equivalent stiffness of the system is computed as:

2I

2

eq TM4

K π= (6-22)

• Assuming K 2=0.1K 1, known displacement, yield shear V y and post yielding stiffness are foundsuch that the equivalent viscous damping matches the chosen damping.

This scheme is not the most efficient. ∆d, K r and V y are not independent parameters, and thisdesign procedure may eventually result in an unfeasible isolation system due to a series offactors and limitations. The first one is that choosing an ultimate admissible displacement

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implies a lower bound for the rubber area size (overlapping area limit). This implies a minimumK 2*h. Then, K 1 is a function of K 2, of the lead area, and V y. This is the reason why all the

procedure is in reality a function of one parameter: the isolator height, h l. Based on thisobservation, the following preliminary design is proposed, as a function of T I, h l, andadmissible ∆d.

• STEP 0 (Input Data): input data are the mass, the shear moduli of the rubber and of the lead, and

the yield strength of the lead.Table 6-4. Input Data

Mass G rubber G lead τy,lead

M I 1 MPa 130 MPa 10 MPa

• STEP 1: T I , ∆m , ξ eq are determined. A first trial value of T I is chosen, on the 5% damped ResponseSpectra S a and S d are determined; a value of ξ eq is chosen, considering that the maximumdisplacement ηS d shall be less than ∆d ; the equivalent elastic stiffness K eq for the system iscalculated. Eventually the ultimate shear capacity V u for the system is calculated: V d is checked

to be of the same order of magnitude of V u , nevertheless the shear demand on the system will bedetermined in a more advanced phase then the preliminary design, eventually through nonlinearanalyses of the structure.

Table 6-5. Step 1TI Sd ξeq ∆m K eq Vu Sa Vd

(chosen)(from 5%dampingspectrum)

(chosen to properlylimit ∆m)

dSgη= ( )2IT/2M π= ueq DK= (from 5%dampingspectrum)

a1 SW η=

• STEP 2: A r , h l and h r (effective rubber height) are found. Maintaining the overlapping ratio limit

of 0.6, the minimum size of the rubber for each isolator Bri is derived (from relationships (6-13),(6-14) or (6-15)) (the fact that the lead plug is inside the rubber area can be neglected at thisstage), and A r is calculated. A trial value of h l is chosen, and, considering a ratio of 0.9, h r isestimated.

Table 6-6. Step 2Bri Ari Ar hl a=h r /h l hr

4.0/B mri ∆=

2riB

rir nA A =

(chosen - trial

parameter)(estimate) lah=

• STEP 3: hysteresis loop parameters are determined (Table 6-7). The stiffness of rubber Kr isestimated, and the yielding displacement ∆ y is determined as a function of known parameters(equations (6-23)). The initial system stiffness K 1 is determined from the equation (6-24) , and A l is from the equation (6-25). The system yielding shear V y can now be calculated.

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yll yl yl A K V τ=∆=;

yll yl

ll A h A G τ=∆

(6-23)

)(K K V yur y1u ∆−∆+∆= (6-24)

l

llr1

h

A GK K +=

(6-25)

Table 6-7. Step 3

K r ∆y K 1 A l Vy

r

r r

h AG

l

yll

G

h τ

y

ymr u )(KV

∆∆−∆−

( )l

lr 1 G

hKK − yr yll K A ∆+τ

• STEP 4: known the system hysteresis loop parameters, actual equivalent viscous damping iscalculated (equation (6-26) and Table 6-8).

elastic

loopeq A4

Aπ=ξ (6-26)

Table 6-8. Step 4

A b c D ξeq

∆m-∆y ∆y VU-V y VU 100)ba(dcbacad

2 ×+π−−

• STEP 5: h l is adjusted by a trial and error procedure. The value of h l selected in Step 2 is adjusteduntil ξ eq(STEP5) matches ξ eq(STEP1). In order to avoid heavy mathematical expressions arising from

Step 5 to Step 1, this can be carried out by means of a simple trial and error procedure, easilyachieved by setting up an electronic worksheet and changing the values of the lead height.

The only parameters governing the procedure are T I, h l, and admissible ∆m (based on theoverlapping area ratio), whilst other quantities are evaluated deterministically from their values.The last step is to calculate the real maximum admissible displacement, based on the real B ri,considering that overlapping areas includes the lead area; equations (6-27) refer to the case ofsquare bearing and monodirectional displacement.

riliri A AB +=

riadmissible B4.0=∆(6-27)

This value, which does not differ very much from the ultimate displacement estimated in step 1,will be compared with the maximum displacement coming from non linear analyses on simplifiedor refined models of the structure in more advanced design phases.

6.2.2.4 Allowable Shear Strain and other Code Reccomendations

6.2.2.4.1 AASHTO (2000) Reccomendations

In AASHTO (2000), shear strain components for isolation design are:• The shear strain due to compression by vertical loads γc (γW, referring to the previous

nomenclature), where K is the bulk modulus of the elastomer, to be taken as 2000 MPa if not

measured;k

is an elastomer material constant related to hardness

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⎪⎪⎪

⎪⎪⎪

>+

≤+

15S,SA k G4

)K /Sk G81(P3

15S,)Sk 21(G A 2

SP3

r

2

2r

c (6-28)

The allowable vertical load is indirectly governed by limitation on the equivalent shear strain inthe rubber due to different load combinations and stability requirements. Creep effects on theelastomer shall be added to the instantaneous compressive deflection, when considering longterm deflections (Art. 14.2.2, AASHTO 2000).For rubber E=(3.8 ÷4.4)G; the compression modulus of the bearing E b in equations (6-29) isobtained taking E=4G; for bearings with large shape factors, incompressible rubber assumptionleads to overestimate the compression modulus, and the second expression of (6-28) is used,

based on the empirical relation for the compression modulus given in the second equation (6-29). The shear modulus G is determined from the secant modulus between 25 and 75% sheardeformation.

⎪⎪

⎪⎪

+

+

= rubberlecompressib

K 1

Sk G81

1

rubberibleincompress)Sk 21(G4

E

2

2

b (6-29)

• The shear strain γ s,s , due to imposed non seismic lateral displacement ∆s; the shear strain γ s,eq ,due to earthquake-imposed lateral displacement d t ; the shear strain γ r , due to rotation θ : Thedesign rotation is the maximum rotation of the top surface of the bearing relative to the bottom.T r is the total rubber height:

r

ss,s T∆=γ ;r

teq,s Td=γ ;

ri

2

r Tt2B θ=γ (6-30)

Load combinations to be checked are:

5.55.0

0.55.2

req,sc

rs,sc

c

≤γ+γ+γ≤γ+γ+γ

≤γ (6-31)

6.2.2.4.2 EC8 Reccomendations

The total design shear strain ( ε td ) shall be determined as the sum of the following components: theshear strain due to compression ε c , the shear strain due to the total seismic design displacement ε s and the shear strain due to angular rotations ε α :

sctd αε+ε+ε=ε (6-32)

Maximum allowable values of shear strains ε c , ε s , and ε td are given in Table 6-9.

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Table 6-9. Maximum Allowable values of Shear Strain (EC8)Shear Strain Maximum Value

εc 2.5

εs 2.0

εtd 6.0

The shear strain due to compression shall be determined as in equations (6-33), where G is the shearmodulus of the elastomer, σe is the maximum effective normal stress of the bearing, given by theratio of the maximum axial force Nsd on the bearings resulting from the design seismic loadcombination, over the minimum reduced effective area of the bearing A r. The latter is given inequations (6-34) and (6-35), respectively for rectangular bearings with steel plate dimensions b x and

by (without holes) and for circular bearings with steel plate of diameter D.

GS1.5 e c σ=ε ; / A N rsde =σ (6-33)

)d-)(bd-b( A Edy yEdxxr = (6-34)

/ 4)Dsin-( A 2r δδ=

)dd(d;/D)2arccos(d 2

Edy2EdxEdEd +==δ

(6-35)

In the above equations d Edx and d Edy are the total relative displacements under seismic conditions, in

the two principal directions, of the two bearing faces, including the design seismic displacements(with torsional effects) and the displacements due to the imposed deformations of the deck (i.e.shrinkage and creep where applicable and 50% of the design thermal effects). d Ed is the total seismicdesign displacement, and S is the shape factor of the relevant elastomer layer.The shear strain due to the total seismic design displacement d Ed , including torsional effects, shall bedetermined as in equation (6-36),where t t is the total thickness of the elastomer.

/ td tEds =ε ; ∑= it tt (6-36)

The shear strain due to angular rotations shall be determined as in equations (6-37) and (6-38),respectively for rectangular bearings of dimensions the b x and b y and for circular bearings ofdiameter D. αx and αy are the angular rotations across b x and b y. Normally in bridges the influenceof ε α is negligible for the seismic verification.

ti y2

yx2x tt2/)bb( α+α=εα (6-37)

ti2 tt2/D α=εα

)( 2

y2x α+α=α

(6-38)

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6.2.2.5 Basic Hysteretic Behaviour and Advanced Analytical Hysteresis Models

The reduction of the seismic forces in the superstructure caused by the fundamental periodlengthening may be accompanied by large horizontal displacements in the isolators, which, togetherwith their lateral flexibility, may lead to significant reduction in their critical axial load.The force-displacement relationship of typical elastomeric isolation bearings is non-linear as aresult of their inherent damping properties. Experimentally obtained shear force-displacement

relationships for elastomeric bearings show strong non-linearities and stiffening behaviourdependent on shear strain magnitude. Tests on individual bearings revealed that beyond a certainstrain level the high-damping bearings exhibit a clear stiffening behaviour. This stiffening is amaterial property of filled rubbers. The lead-rubber bearing, which was made from unfilled rubberand had doweled shear connections, did not show the large-strain stiffening effect (Analyticalmodels, were developed by Kikuchi and Aiken (1997).An other important issue is that the stability of elastomeric bearings may be jeopardised due to largelateral displacements and axial loads, that are responsible for the reduction in the bearing criticalload, in the shear stiffness and in the rotational stiffness; as a consequence, the height, the dampingand the overturning (in case of doweled connections) of the bearing result to be affected.(Analytical models, were developed by Nagarajaiah and K. Ferrell, (1999), and Buckle et Al.(2002)).

6.2.2.6 Lead Rubbers Damper and Oil Dampers

This combined energy dissipation system, tested by X. Lu and Q. Zhou (2002), consists of leadrubber dampers connected in parallel with oil dampers and installed in conventional frame braces.The working mechanism of the combined energy dissipation system is such that under lowerearthquake intensity, the LRB behaves elastically and oil damper provides smaller damping forceand stiffness. Under stronger earthquake the LRB develops elasto-plastic deformation, decreasingthe structural stiffness, and the oil damper provides larger damping force and smaller stiffness: theseismic force on the whole structure is reduced, decreasing the response.

6.2.3 Sliding devices

This class of devices consists of sliding supports providing for frictional damping forces.Modern sliding bearings consist of a sliding interface and a rotational element needed formaintaining the full contact at the sliding interface. The rotational element may take various formssuch as in the pot bearing, the spherical bearing, the disc bearing, the articulated slider in thefriction pendulum bearing or an elastomeric bearing. The type of material at the slider interface may

be:• Unlubricated PTFE: unlubricated interfaces consisting of highly polished austenitic stainless

steel in contact with PTFE or similar composites (as those used in FPS bearings);

• Lubricated PTFE: lubricated interfaces consisting of highly polished austenitic stainless steel incontact with unfilled PTFE; lubrication is applied by grease stored in dimples.

• Bimetallic interfaces: interfaces consisting of stainless steel in contact with bronze or similarmetals impregnated with a lubricant such as lead, PTFE or graphite. The additional issues thatthis kind of interface may lead to those already related to the previous categories make it criticalfor use.

Stainless steel – PTFE bearings are widely used in bridge design to accommodate slow thermalmovements. The friction coefficient of PTFE on steel is 0.02 ÷0.03 (unlubricated and lubricatedPTFE respectively) for very slow slip rates. For typical seismic velocities and typical pressure for

bridge bearings, it ranges around 0.10 ÷0.15, depending on lubrication in both cases.In a system isolated with a set of PTFE bearings, the first isolation period arises from thesubstructure only and is typically very short, leading energy into higher modes, while the second

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isolator period tends to infinity and provides no centring force to resist displacements. Theirapproximately rectangular force-displacement loop gives very high hysteretic damping, and they aregenerally coupled with other centring devices like rubber bearings or steel dampers. In the lattercase all the load is carried by the PTFE bearing and the friction coefficient should be kept as low as

possible, while centring force and additional damping are provided by the dampers. In the formercase they can be mounted in parallel, thus sharing the vertical load, or they can be mounted in seriesto provide flexibility at force levels lower than the bearing sliding forces; part of the vertical load issustained by the rubber.

6.2.3.1 The Friction Pendulum System

The Frictional Pendulum System (FPS) is a sliding recentering device based on the principle of thesliding pendulum motion. It consists of two sliding plates, one of which with a spherical stainlesssteel surface, connected by a lentil-shaped articulated slider covered by a Teflon-based high bearingcapacity composite material ( Fig.6-7 , left). The slider is generally locked on a vertical stud with aspecial hollowed end which allows free rotation of the slider and a perfect contact with the slidingsurface at all times ( Fig.6-7 , right). During the ground shaking, the slider moves on the sphericalsurface lifting the structure and dissipating energy by friction between the spherical surface and theslider, essentially resulting in a pendulum motion with period given in equation (6-40), where F V isthe total weight on the device and R 0 is radius of the spherical stainless steel surface. Considering asystem with mass M , the system stiffness K is easily obtained in equation (6-40).

gR

2T 0π=

(6-39)

0

V 0 V

V

R

FK

g

R

gK

FgK F

2K M2T

=⇒=

π=π=

(6-40)

Detailed descriptions of the basic principles of the FPS devices can be found in literature ofrelatively recent works (Almazan et al., 2002, Wang et al., 1998; Tsai, 1997).One of the most relevant features of the FPS is that residual displacements are reduced due to theself-centering action induced by the concave spherical surface. Typically a FPS device may provideequivalent dynamic periods of vibration within the range from 2 to 5 seconds and displacementcapacities greater than 1 m.

PTFE Bearingmaterial Articulated

Friction Slider

Spherical Concave Surface of harddense Chrome over Steel

Fig.6-7. Radial section of the FPS device (left) and Components of a typical FPS (right): (1)sphericalsurface, (2)slider, and (3)stud

The device can be either mounted in an upward or downward position ( Fig.6-8 ), conceptuallyequivalent in terms of isolation effect, but different for the design implications on the superstructure

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and the foundation system: in the downward position, the P- ∆ effect is transmitted to the portion ofthe structure below the isolation system, usually the foundation; if the FPS is positioned upward, thesame P- ∆ effect is transmitted to the resisting elements of the superstructure.

Fig.6-8. FPS bearing in downward (left) and upward (right ) position

FPS bearings are used in the retrofit of earthquake damaged bridges (e.g. Priestley and Calvi, 2002)or in the design of new bridge structures. The feasibility of using friction pendulum bearings forseismic isolation of bridges has been also investigated by Wang et Al. (1998).

6.2.3.1.1 Basics Hysteretic Behaviour

The hysteretic loop of FPS is approximately rigid plastic with post yielding hardening. The actualhysteresis loop is more complex, depending on a series of factors, the main of which is the strongdependence of its response on the axial force variation on the device. The actual constitutive law ofthe FPS element is an elasto-plastic type with strain hardening: the yielding shear and the post

elastic stiffness depend on the axial force, resulting in a hysteresis loop extremely varying from thestandard constant shape Fig.6-10 . Other issues related to this kind of devices regard the variabilityin the friction coefficient properties, due to the vertical pressure, to the sliding velocity and to thetemperature.The resulting isolator force consists of two main components, namely, the restoring force due to thetangent component of the self-weight, always contributing to the restoring mechanism, and thefrictional force always opposing the sliding, thus contributing or resisting the restoring forcedepending on the direction of motion. The peculiarity of the FPS is the association of the concavesliding surface to a friction-type response: the consequent coupling between the lateral and verticalmotions may produce large deformations in the isolators, but it is not considered in the smalldeformation theory of the most theoretical formulations, because generally small-deformations

hypothesis is accurate enough for estimating global response quantities. The exact force– deformation constitutive relationship of the isolator may be carried out at different levels ofcomplexity.

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Fig.6-9. FPS Equilibrium diagrams in the 2-D and 3-D cases: (b) planar model; (c) three-dimensionalmodel

Considering the planar system 2D in Fig.6-9 (left), the simplest form of the constitutive law is thewell-known force–deformation relationship of the FPS system in one dimension and small

deformations, resulting from the horizontal equilibrium of the isolator:v

0

v F)x(signxRF

F µ+= & (6-41)

The total acting vertical force F V can be identified with the weight W . The two parameterscharacterizing the friction pendulum system behaviour are the friction coefficient and the post-yielding stiffness: these properties are influenced by temperature, velocity, bearing pressure andwearing state. If the small displacements approximation is overcome, the vertical and horizontalequilibrium equations lead to:

⎟⎟

⎠ ⎞

⎜⎜

⎝ ⎛ =θ

0Rx

arcsin (6-42)

µ−θ= )x(sign.cos FN v & (6-43)

θµ+θ=

cosN

)x(signtgFF v & (6-44)

The stiffness of the device seems to be affected by the sliding velocity and the bearing pressure: thedependence on velocity appear to be of the same kind of the friction coefficient. Experimentalmeasures of the actual device stiffness record an increase of it up to the 10% of its theoretical value.The reason of this still need further investigation.

Simplifications in the modeling of the FPS constitutive law lead to an essentially constant, regular, parallelogram shaped hysteresis loop: specifically these simplifications consists in the small angle

approximations, in neglecting the friction at the interface of the socket of the slider, in neglectingthe non-punctual transfer mechanisms of the forces (as pointed out by Casarotti (2004)) and inneglecting the axial force variations when considerable. Among these the real behaviour of theisolator is mostly affected by the axial load variations: it is characterized by a variable yield pointand a post-elastic stiffness that depend on the acting axial force, resulting in a non-linear post-elastic branch. An accurate model of these characteristics can be found in Calvi et Al. (2004):Fig.6-10 shows the responses of two isolators sensitive to the axial force variations, one subjectedto an increasing compression and the other to a decreasing axial load, and a third FPS insensitive tothe axial force variations.

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R e s t o r i n g

f o r c e

V

Displacement ∆s

Hk

V y

∆ N <0 (decompression)

∆ N >0 (compression)

Insensitiveto ∆ N

-0.6 -0.4 -0.2 0 0.2 0.4 0.6

Displacement [m ]

-1300

-975

-650

-325

0

325

650

975

1300

L a

t e r a

l f o r c e

[ k N ]

AM - lef t is olat or AM - ri ght iso lato r NAM

Fig.6-10. Constitutive laws (left) and hysteresys loops (right): simplified and advanced models.

6.2.3.1.2 Modelling Issues of the Friction Pendulum System

Earlier studies developed simplified analytical models capable of representing the predominantly

bilinear FPS behaviour: most of the theoretical formulations were carried out considering small-deformations, however, due to recent seismic event observations, the large-deformations and theassociated P- ∆ effects have been addressed as a possible issue in the isolators design. For thesereasons, large-deformations models should be used in the design of FPS isolated structures, forwhich is particularly important the consideration of the axial force in the isolators as it can induceaccidental torsion effects not accounted for in the current design procedures.

• Modelling of the axial force variation InfluenceCalvi et Al. (2004) developed and tested an analytical model of FPS, that takes into account theeffect of the axial force variations on the isolators: the actual behaviour of the isolator has beenfound to be of relevance in terms of the general response quantities of the bridge structures. Theformulation models both the yielding shear and the post-elastic stiffness of FPS as a function of theacting axial force, resulting in hysteretic loops characterized by non-linear post-elastic branch, asevident in Fig.6-10 . The model of the isolator has been implemented by means of a three-dimentional 2-joint finite element, characterized by cylindrical symmetry.• Analytical Model for the Teflon-Metal Interface and of the Local Bending EffectsTo simulate accurately the behaviour of the teflon-metal interface, including the effects of axialforces and velocities, Tsai (1997) used an analytical model based on visco-plasticity theory:numerical simulations on multi-storey structures have shown that nonlinear local bending momenteffects are substantially important for base-isolated structures and that axial force variations on theisolators are of significant importance for the friction force calculation.

• A physical model for the FPS upliftingTo include possible uplift and impact, Almazan et Al. (1998) defined a physical model for the FPS,including an uniaxial gap element between isolator and sliding surface and a restitution coefficientwhich accounts for the energy loss during the impact in the isolators in which the uplift occurs. Theresultant vertical impact of the slider and the spherical surface leads to two effects: column baseshears may increase due to increase in normal force at the isolators interface; this in fact results inthe instantaneous stop of the slider from sliding and in the transmission of significantly larger shearforces to the supported columns.Although local effects such as variation in the normal contact forces, large deformations and upliftseems not to affect considerably the global system response, Almazan et Al. (1998; 2002)recommend to consider them in the isolation modelling and design to compute local responses such

as the superstructure deformations and the normal isolator forces, expecially for near-fieldearthquake with strong initial acceleration pulse and for statistically correlated horizontal andvertical expected ground motion components.

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6.2.4 Metallic and Friction Dampers

This kind of dampers, relatively economic, are used when a control is needed on the level of the provided force, when an increased initial structural stiffness is needed, and/or when the mainconcern is to reduce displacement as opposed to acceleration. Friction Dampers dissipate theseismic energy by friction developing between two solid bodies sliding relatively one to theanother. Typical examples of these devices are:• Slotted-bolted connections;• Pall devices;• Sumitomo Devices.Metallic dampers take the advantage of hysteretic behavior of metals when deformed into the post-elastic range. A wide variety of different types of devices have been developed, with basic shapescut from thick steel plates, among these:• C/E-shaped Hysteretic Dampers;• EDU device;• ADAS and TADAS Elements;

• Lead Extrusion Devices;• Torsional beams, bell dampers, steel tubes, etc;

6.2.4.1 Basic Hysteretic Behaviour and Dynamic Response with Metallic/Friction devices

The macroscopic model and the analysis of the dynamic response of structures equipped withmetallic and friction dampers is basically the same, due to the essentially equivalent elastic-

perfectly plastic exhibited by the devices.In order to understand the nature of the dynamic response of structures equipped withmetallic/friction dampers, a simple single storey braced frame system, excited by a cosinusoidaldriving force, has been investigated by (Filiatrault, (2003)). The optimum yield load depends on the

frequency and amplitude (in particular linearly proportional to this latter) of the ground motion andit is not a strictly structural property.

6.2.4.2 Friction Dampers

In the case of friction dampers, the design philosophy to enhance the structural performance is to provide a way for the structure to yield without damaging the existing structural members: seismicenergy is dissipated by means of friction, i.e. by making steel plates sliding one against the other,while bolts hold the steel plates together providing the normal component of the friction force.Sliding plates are fixed to the cross braces and then clamped together. At a given sliding load, P y,the plates begin to slide and dissipate energy. Varying the sliding load will alter the seismic energy

attracted by the structure.Incorporating the braces adds initial lateral stiffness to the system, thus lowering the natural periodof the structure and providing a margin over which the structure can shift its period if resonance isencountered: any time the current structural period attracts seismic energy enough to activate thefriction dampers, the resonance phenomenon can be avoided by a period shift. When in fact at thelow braced period the structure attracts large amounts of seismic energy, the structure begins tosoften as the friction dampers begin to slip and dissipate energy: the reduced lateral stiffness of thestructure, due to the dampers slippage, causes the desired period shift. If the braced natural periodis moved far from the unbraced natural period, the structure will have a sufficient ability to soften.

6.2.4.2.1 Advantages and Disadvantages of Friction Dampers and Environmental Effects

These devices possess good characteristics of structural behavior. Some of their advantages are thelisted below:

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• They have high capacity of energy dissipation; compared to devices based on yielding of metals,friction dissipators possess a great capability of absorbing energy. This characteristic disappearwith the wearing of the sliding surfaces.

• Their behaviour is not seriously affected by the amplitude, the frequency contents or the numberof cycles of the driving force.

• They have a controllable friction force (through the pre-stressing normal force).

• Frictions dissipators are not affected by fatigue effects; the materials are low maintenance oreven maintenance free.• Friction dampers perform well in various environmental conditions such as temperature.• The damper design is straightforward and low tech: the design does not require expensive

engineering design costs or testing prior to implementation.Some potentially relevant disadvantages exhibited by Friction dissipators are:• The energy dissipated per cycle is only proportional to the maximum displacement instead of the

square of the same displacement, as in the case of viscous damping: this can be relevant forsudden pulses and for inputs stronger than those expected. Moreover, resonance peaks cannnot

be properly cut.• Durability is also a controversial issue, mostly due to the high sensitivity of the coefficient of

friction to the conditions of the sliding surfaces.• High frequencies can be introduced in the response, due to the frequent and sudden changes in

the sticking-sliding conditions. The dynamic highly non-linear behavior of friction dissipatorsmakes their numerical simulation very difficult. This situation has arisen some controversialissues, such as the possible introduction of high frequencies into the structural response, as wellas the lack of studies of these devices when subjected to near-fault pulses.

• Environmental effects, such as localized heating and atmospheric moisture and contaminants,might alter the frictional characteristic of the sliding interface.

6.2.4.2.2 Slotted-bolted Connections

Slotted-bolted Connections are the simplest form of friction dampers: they basically consist inintroducing slotted-bolted connections at the end of conventional bracing members (in multi-bent bridge pier or deck) ( Fig.6-11 ). It is important to ensure that the slippage of the device occurs before the compressed braces buckle or yield.Tests results performed by Pall et Al. (1980) and Tremblay and Stiemer (1993) show that slidingconnections can exhibit a very high energy dissipation capability under extreme loading conditions,

provided that appropriate material and bolt clamping force are used.

Fig.6-11. Slotted Bolted Connection Assemblage (Tremblay and Stiemer, 1993)

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The Pall Device (diagonal brace elements with a friction interface at their intersection, connectedtogether by horizontal and vertical link elements) and the Sumitomo Device (a cylindrical devicewith friction pads that slide directly on the inner surface of the steel casing of the device developed

by Sumitomo Metal Industries, Ltd., Japan) are other devices based on the same basic principleswhere the response is optimize through a proper design of their geometry.

6.2.4.3 Steel Hysteretic Dampers

Hysteretic dampers dissipate energy by flexural, shear or extensional deformation of the metal inthe inelastic range. Typically, mild steel plates with triangular or hourglass shapes are used.These devices are able to sustain repeated cycles of stable yielding, avoiding premature failure.Further, they are reliable, maintenance free, not sensitive to temperature variations and notsubjected to ageing.The steel used for these devices must be characterized by a very high elongation at failure and avery low hardening, in order to grant a very high low cycle fatigue life with negligible performancedecay after many cycles.In continuous span bridges, they may be located either in one position (e.g. one abutment) to allowfree movements of the bridge (in this case they must be designed for very large forces), ordistributed in several locations to allow thermal movements of the structure (normally associated tohydraulic shock transmission units).There are three typical kinds, according to their working principle:• Uniform moment bending beam with transverse loading arms;• Tapered-cantilever bending beam;• Torsional beam with transverse loading arms;Several devices developed in the early 1980’s showed some limits: limited capacity to resist yieldcycles without breaking; characteristics degradation after first cycles, with progressive reduction ofthe yield force up to failure; non-symmetry of the load-displacement cycles, shown stiffnessvariations in tension and compression; difficulty to provide uniform response in any direction.

New devices overcoming these limits have been developed. They are based to the combination ofC-shaped elementary energy dissipators. Tests on these devices have shown long cyclic life, almostno cycle deterioration before failure and very good dissipation thanks to the almost square shape ofthe hysteresis loops ( Fig.6-13 ).These devices may constitute the dissipative part of a system of seismic isolation of the bridge deck,as well as they may simply act as dampers by themselves. Then they can be arranged to be a part ofone-directional or multidirectional bridge bearings.

The conceptual design of the single damper unit is based on optimisation criteria, i.e.:• An optimised shape allows almost constant strain range for each cross section (uniform diffusion

of plasticization);

• Particular design arrangements neutralise the effects of geometry changes, that otherwise cancause strain hardening or softening behaviour and/or dissimmetrisation of the hysteresis cycles,at large displacements: the dissipation effectiveness is improved, and large displacements anddamping of response in all directions are allowed.

6.2.4.3.1 C-shaped DeviceC-shaped elements grant very high energy dissipation, very high fatigue resistance and possibility torealise multidirectional devices. It has a semicircular shape ( Fig.6-12 , left), with constant radius r,while depth varies in order to ensure the uniform plasticization of all sections.Maximum depth is in the middle, and minimum at the supports, obviously not zero, but smallenough to guarantee the shear and axial load transmission to the supports). The angular opening ofthe device is generally of 180°, or greater when the displacement demand is particularly high.

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Fig.6-12. C-shaped Device (left) and EDU Device (right)

Equations (6-45), where α is polar coordinate referring to the centre of the C device, give theyielding and plastic quantities of the device when α does not exceed 180°.

2/1max )sen(b)(b α=α

3

3max

maxmax

2

max

2max

yp

l

ymax

2

y

2max

yy

2

yp

2

yy

r

sbE03455.0K

br

824.4

r 4sb

P

3

2b

r 824.4

r 6sb

P

4)(sb

M6

)(sbM

=

ε=δ

σ=

µ=µ

ε=δ

σ=

ασ=ασ=

(6-45)

The very simple equations (6-45) consider only bending deformation, and do not account for axialeffects (softening in tension and hardening in compression). To avoid these effects, C-shapeddevices are usually coupled, as in the case of the EDU device, where the two opposite elements aresimultaneously one in tension and the other in compression.

Other devices, with a different shape, like the E-Shaped device, (Ciampi and Marioni, (1991)) weredeveloped, following the same principle to achieve a uniform plasticization along the member.

6.2.4.3.2 The EDU Device

The EDU Device is a multi-composed device made up with C-shaped elementary energy dissipators(Fig.6-12 , right): they are combined in such a way that they are forced to deform anti-symmetrically, i.e. for each compressed one, another is in tension; combination of them with radialsymmetry allows uniform behaviour under earthquake loading acting in any direction. This devicecan also be coupled with hydraulic shock transmitters in parallel.

The EDU device has been tested by Marioni (1996) with a real earthquake of 7.4 magnitude with0.8g PGA; it dissipates much more energy ( Fig.6-13 ) than any other system and fulfil Europeanstandards for in-service conditions. It shows self-recentering properties for thermal effects andsmall earthquakes, and used in parallel with HRDB can fulfil any AASHTO requirement. Moreoverit has low costs.

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Fig.6-13. Load Deflection Plot of the EDU device (Marioni, 1996)

6.2.4.3.3 ADAS and TADAS ElementsThe Bechtel Added Damping and Stiffness (ADAS) device is another example of a hystereticdamper (usually installed in conjunction with a chevron brace assemblage). ADAS elements are

designed to dissipate energy through the flexural yielding deformation of X-shaped mild-steel platesconfigured in parallel between top and bottom boundary connections (Fig.6-14). The particularadvantage of an X-plate is that, when deformed in double curvature, the plate deformation isuniform over its height, and when deformed into its plastic regime, the yielding will be distributed.The primary factors affecting ADAS element behaviour are device elastic stiffness, yield strength,and yield displacement (Bergman (1987)).Possible shortcomings with X-shape ADAS are that the stiffness of the device is very sensitive tothe tightness of the bolts and generally much less than that predicted by assuming both ends fixed,then the flexural behaviour might be weakened when the device is subjected to axial loads.

Fig.6-14. Added Damping and Stiffness (ADAS) Element

Triangular ADAS (TADAS) devices using triangular steel plates welded at bottom and bolted at top(Fig.6-15 ) were developed to avoid these inconveniences: Stiffness varies linearly along the height,as well as moment does, implying constant curvature, thus avoidig curvature concentration.

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Fig.6-15. TADAS Element

6.2.4.3.4 Lead Extrusion Devices (LEDs)The Lead Extrusion Dampers take the advantage of the extrusion of lead through orifices.Fig.6-16 illustrates two types of lead extrusion dampers: the constricted tube, that forces theextrusion of the lead through a constricted tube, and the bulged shaft, that uses a bulged shaft

through a lead cylinder.

Fig.6-16. Longitudinal Section of a bulged-shaft (left) and of a constricted-tube (right) extrusion energyabsorber

The main characteristics of these devices are that Lead hysteretic behaviour is essentiallyrectangular, stable and unaffected by number of load cycles ( Fig.6-17 ); it is not influenced by anyenvironmental factor; fatigue is not a major concern, strain rate has a minor effect and aging effectsare insignificant.

Fig.6-17. Lead Force Displacement Curve (left) and test results on a constricted tube absorber (right)

6.2.4.3.5 Conceptual Design: concepts of yield/slip shear and Optimization criterionThe design of structures equipped with metallic/friction dampers can be divided in four stages: (i)the estimation of the optimum parameters for dampers and adjacent elements by hand- calculation;(ii) the design of dampers and adjacent elements to meet the determined optimum parameters; (iii)

the application of capacity design checks for all members of the structure under the expectedultimate force generated by the metallic/friction dampers; (iv) nonlinear time history analyseschecks of the whole equipped structure.

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Marioni (1996) proposed a simplified design process for Hysteretic Dampers selecting, by trial anderror, the devices such that the sum of yield forces is of the suggested order of magnitude of:

∑∑

)(07.0

)(1.0

areaseismicitylowW F

areaseismicityhighW F

y

y(6-46)

where W is the total weight of the structure. Nonlinear analyses are always required in order tocheck the design displacement: if it’s too small (too large), the sum of the yield forces have to beincreased (decreased), in order to rise (low) the threshold of the yielding and increase (reduce) theenergy dissipated by the structure.Alternatively the more sophysticated design procedure developed by Filiatrault and Cherry (1990)can be used to define the optimum yield/slip load (i.e. providing in the optimum energy dissipation)of such devices.

6.2.5 Viscous and Viscoelastic Dampers

6.2.5.1 Viscous Dampers

Linear devices produce damping forces proportional to the velocity of the damper deformation,greatly attenuating the higher-mode seismic response, that is only relatively reduced by highisolator damping. Hydraulic dampers (Marioni, 1999 and 2002) utilise viscosity properties of a fluidto improve structural resistance against the earthquake. Such devices are generally used as shocktransmitters, able to allow slow movements (in service conditions) without valuable resistance, andstiffly react to dynamic actions.It should be possible to develop effective velocity dampers, of the adequate linearity, by using the

properties of high-viscosity silicone liquids: a double-acting piston drives the silicon fluid cyclicallythrough a parallel set of tubular orifices, giving high fluid shears and hence the required velocity-damping forces. The force generated by the device can be described by the following equation:

ACVF += α (6-47)

where F is the force applied to the piston, V is the piston velocity, C, A, α are constants dependingon the fluid and circuit properties; α may range between 0.1 and 2, according to the type of valves.Force-displacements plot for devices with different values of α subject to sinusoidal input areelliptical-shaped. Fig.6-19 (left) illustrates type of dependence of the force on the velocity, fordifferent values of α. When energy dissipation is required, α≤1 is preferred in order to increase thehysteretic area and maximise the dissipated energy per cycle. In this case they’re called ViscousDampers (VD), for which a reference value of α is generally 0.1. The parameter α equal or higherthan 1 is preferred when the difference of force at low and high velocity shall be maximised, inorder to react stiffly as soon as the velocity increases, in order to allow slow movements due tothermal variations, creep and shrinkage and to become rigid in case of dynamic actions (brakingforce and earthquake), or when energy dissipation is not required: in this case they’re called Shocktransmission Devices (STD) or Hydraulic Couplers.

6.2.5.1.1 Basic Hysteretic Behaviour of Viscous DampersAssuming a sinusoidal relative axial displacement history (a more extensive discussion can befound in Casarotti, (2004)) that induced axial force in the element is linearly proportional to therelative velocity between its two ends, the force-displacement relationship is represented byequation (6-48) and the energy dissipated per cycle by equation (6-49). Equation (6-48) describesan elliptical loop ( Fig.6-18 , left), in which the amplitude of the maximum induced force in theelement is linearly proportional to the damping, to the displacement amplitude and to the excitation

frequency: this is a reason why in MDOF systems, each mode has an assigned viscous damping. Itis worth to note that during a seismic excitation, the frequency continuously varies, and in the sameway the amplitude of hysteresis loops, i.e. the energy dissipated through viscous damping.

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Therefore, as previously mentioned, the energy dissipated per cycle is also proportional to thesquare of the maximum displacement.

2

00 Xx

1CXF

⎟⎟

⎠ ⎞

⎜⎜

⎝ ⎛ −±=

ω (6-48)

2

0

/2

0D XCdtx)t(FE ωπ== ∫ ωπ

(6-49)

FX 0 C ω

x X 0

1

1

1

FX 0C ω

x X 01

KCω

Fig.6-18. Cyclic Response of a pure Linear Viscous Element (left), Cyclic Response of a pureVE Damper (right).

0

0.2

0.4

0.6

0.8

1

1.2

0 0.2 0.4 0.6 0.8 1 1.2

V

F =

V α

α= 1 α=2

F

δ

α =1.0α =0.3

Fig.6-19. Force-velocity type dependence for different values of the parameter α (left), Hysteresis Loopof a viscous damper with different values of α (right).

An important characteristic of linear viscous dampers is that, differently from e.g. friction dampers,

the acceleration of the damper is out of phase with the floor acceleration, and this is useful inlimiting it. Nevertheless, the fact that viscous damper force is directly proportional to displacement,implies that virtually there is no limit to the damper force itself, that is virtually unbounded, whilee.g. in friction dampers it is limited by the damper yielding.

Non linear viscous devices with α<1 provide a limit for the increase of the force with displacements(Fig.6-19 , (right)). In the practical range of velocity and exponential coefficient (0.2 to 1) the ratio

between the nonlinear damping constant and the damping constant of an equivalent dissipatinglinear system can be approximated, by equating the energy dissipated per cycle, as in equation (6-50). Consistent units must be used as equation (6-50) is not dimensionally homogeneous.

( ) α−ωπ≅

10

L

NL X2C

C(6-50)

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6.2.5.1.2 Design considerationsIn the design process for viscous dampers a non-linear analysis of the structures is always required.Marioni (1996) suggests to select, by trial and error, the VD such that the sum of the constant C isabout of the order of:

∑≅

)(07.0

)(1.0

areaseismicitylowW C

areaseismicityhighW C (6-51)

where W is the total weight of the structure. Then non linear analyses are needed to check thedesign displacement S D; if it’s too small (too large), the sum of the constants C has to be increased(decreased), in order to rise (low) the threshold of the yielding and reduce (increase) the energydissipated by the structure.Alternatively the more sophysticated design procedure developed by Filiatrault (1993) can beadopted.

6.2.5.1.3 Fabrication and Detailing Issues

Fluid dampers mounted in a structure are essentially a “bolt-in” item, of a relatively compact size. A brief discussion on the implementation of fluid dampers is provided in terms of fabrication issues(Size vs. Cost) and detailing (Attachments and Brace Styles).If a given structure requires a specific amount of total macroscopic damping, this latter needs to bedivided among the number of dampers. The end result is a maximum force and damping functionfor each individual damper. The question arises if the engineer should select a large number ofsmall dampers, or a lesser number of large dampers (Casarotti, (2004)).There are three ways to setup dampers into a building or bridge structure:• Base isolation dampers have clevises and spherical bearings at each end. These long stroke

dampers are connected to the foundation and to the building frame respectively, using mounting pins. (the mounting pins must be oriented vertically, to allow proper articulation during out of

plane motion).• Dampers for chevron bracing systems have clevises and spherical bearings at each end (themounting pins are usually oriented horizontally).

• Dampers for diagonal bracing systems have a clevis with spherical bearing at one end, and amounting plate at the opposite end (the mounting plate attaches to a brace extender).

Maintenance is not required for a properly designed and manufactured fluid damper used forseismic and wind damping in structures. Usually, visual inspection of the dampers should occurafter a major seismic or wind storm event: in this case the damper mounting pins may bend orshear. In some cases, regional codes may require that a few dampers be randomly removed from thestructure, and subjected to testing in order to verify the damping output.

6.2.5.1.4 Effects of Supplemental Viscous Damping on Asymmetric-Plan SystemsThe combined effects of irregularities in plan (curves, changes of direction) and in the pier heightlayout of irregular bridges lead to an asymmetric distribution of the centres of mass and of stiffness,

possibly affecting the seismic response of the system: particularly, irregular bridges with flexibledecks constitute torsionally-very-flexible systems.Goel (1998) showed that edge deformations in asymmetric-plan systems can be reduced by a factorof up to about three by proper selection of the supplemental damping parameters alone (particularlyof the plan-wise distribution of the supplemental damping), without any redistribution (oftenunfeasible) of stiffness and/or mass properties of the system.

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6.2.5.2 Viscoelastic Dampers

Typical used Viscoelastic dampers are made of copolymers or glassy substances; they are oftenincorporated in bracing members and dissipate energy through shear deformations of theViscoelastic material ( Fig.6-20 ).

Fig.6-20. VE Damper part of a bracing member: typical scheme (front and 3D views) and picture

6.2.5.2.1 Basic Hysteretic Behaviour of VE Dampers and Dynamic Analysis of VE Dampers Equipped Structures

The response of this kind of dampers is analogous to the previously mentioned viscous behaviourwith an added elastic component. The device is represented by means of G E and GC , respectively theinstantaneous elastic response and the shear viscous damping constant exhibited by the viscoelasticmaterial.The solution for a sinusoidal excitation describes an elliptical shaped loop ( Fig.6-18 , right, andequation (6-53)) inclined with respect to the principal axis of a quantity corresponding to theinstantaneous elastic stiffness: the response can be easily viewed as the sum of a linear elasticcomponent and a viscous elliptical component: still maximum force does not occur at maximumdisplacement, and optimum phasing can be obtained by adjusting the material properties K and C (equations (6-52)).The energy dissipated per cycle is easily shown to be given by the equation (6-49), with C replaced

by C : this can be also deduced observing that the elastic component doesn’t contribute to theenergy dissipation.The equivalent viscous damping ratio of the element is shown in equation (6-54), where ω is theoscillating circular frequency of the element.

h

AGC;

h

AGK CE == (6-52)

2

000 Xx

1Xx

CK

CXF

⎟⎟

⎠ ⎞

⎜⎜

⎝ ⎛ −±

⎟⎟

⎠ ⎞

⎜⎜

⎝ ⎛

ω=

ω (6-53)

ηω=η=ω=ω=ζ

/CK

2/G2/Gm2/C EC (6-54)

In viscoelasticity, G E is the Shear Storage Modulus, that is a measure of the energy stored/recovered per cycle, and ωCG is the Shear Loss Modulus, measure of the energy dissipated per cycle, and theratio of the two is called Loss Factor, η=2ζ.Chang et al. (1993) found that both andEG ωCG decrease with an increase of the ambient

temperature, but η remains fairly constant. Also, damper properties remain fairly independent ofstrain for strain level below 20% for different temperatures and frequencies.

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6.2.6 Self-Centering Dampers

Generally dampers are unable to limit the residual displacements after a seismic event. Somerecently developed damper systems incorporate re-centering capabilities, characterized with a so-called flag-shaped hysteretic loop, among these:• Shape Memory Alloys Dampers (SMA),• Energy Dissipating Restrain (EDR);• The Friction Spring Seismic Dampers;• The Post-Tensioned Energy Dissipating (PTED) steel connections;The main advantage of the self-centring behaviour consists in reducing permanent offsets when thestructure deforms inelastically.

6.2.6.1 Shape Memory Alloys Dampers (SMA)

Shape-memory alloys (SMAs) have the capacity to undergo large strains and subsequently torecover their initial configuration. The basis for this behavior is that, rather than deforming in theusual manner of metals, shape-memory alloys undergo transformations from the austenitic to themartensitic crystal phase (Hodgson, 1988). Sasaki (1989) studied the suitability of Nitinol forenergy dissipation under seismic-type loading, and investigated flexural, torsional, shear, and axialmodes of deformation. Graesser (1991) and Witting (1992) have continued the studies of shapememory alloys for energy dissipation applications in structures. A Nitinol energy dissipator has the

particular advantages of being mechanically very simple and reliable.Currently, there is no reference normative for the design of SMA, even if guidelines weredeveloped recently by the MANSIDE Consortium (1998).

6.2.6.1.1 Application of SMA restrainer to multi-span bridgesThe use of the SMA restrainers in multi-span simply supported bridges at the hinges and abutments

can provide an effective alternative to conventional restrainer systems: the SMA restrainers can bedesigned to provide sufficient stiffness and damping to limit the relative hinge displacement. TheSMA restrainers may be connected from pier cap to the bottom flange of the girder beam in amanner similar to typical cable restrainers, as shown in Fig.6-21 . The restrainers are typically usedin a tension-only manner, with a thermal gap to limit the engaging of the restrainer during thermalcycles. If adequate lateral bracing could be provided, the restrainers can be made to act in bothtension and compression.

Fig.6-21. Configuration of shape memory alloy restrainer bar used in multi-span simply supportedbridges

DesRoches and Delemont (2002) investigated the effectiveness of the SMA restrainer bars in bridges through an analytical study of a multi-span simply supported bridge. The results showed

that the SMA restrainers reduce relative hinge displacements at the abutment much more effectivelythan conventional steel cable restrainers. The large elastic strain range of the SMA devices allowsthem to undergo large deformations while remaining elastic and due to their superelastic properties,

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they are able to maintain their effective stiffness for repeated cycles, differently from conventionalrestrainer cables once yielded. In addition, the superelastic properties of the SMA restrainers resultsin energy dissipation at the hinges.Finally, evaluation of the multi-span simply supported bridge subjected to near-field ground motionshowed that the SMA restrainer bars are extremely effective for limiting the response of bridgedecks to near-field ground motion: the large pulses from the near-field record produced earlyyielding in conventional cable restrainers, thus reducing their effectiveness and resulting in largerelative hinge displacements for the remainder of the response history. The SMA restrainer is ableto resist repeated large cycles of deformation while remaining elastic. In addition, the increasedstiffness of the SMA restrainers at large strains provides additional protection from unseating as therelative hinge opening approaches the critical value.

6.2.6.1.2 Macroscopic Hysteretic Behaviour of the SMASMAs are binary or ternary metallic alloys that can be found in two different phases, Austenite andMartensite, capable of experiencing thermo-elastic solid transformations; each phase is stable atdifferent thermo-mechanical states. Austenitic structure has a higher degree of symmetry and isstable at higher temperatures and lower stresses, while martensitic structure is generally met at

lower temperatures and higher stresses. For some SMAs, such as Nitinol (NiTi SMA), the phasechange can be stress-induced at room temperature if the alloy has the appropriate formulation andtreatment. The main features of SMA are: (i) the memory effect , i.e. the aptitude to recover the initialshape by heating; (ii) the superelasticity , i.e. the aptitude to recover the initial shape as soon as theexternal action is removed. The stress-induced shape memory property is based on a stress-inducedMartensite formation. The austenitic phase of the material is stable before the application of stress.However, at a critical stress level the martensite becomes stable, yielding and showing a stress

plateau, as shown in Fig.6-22 . Nitinol shape memory alloys possess several useful characteristics for use as restrainers in bridges,as shown in Table 6-10, where they are compared to typical structural steel properties, such as:large elastic strain range, hysteretic damping, highly reliable energy dissipation (based on a

repeatable solid state phase transformation), strain hardening at strains above 6%, excellent low-and high-cycle fatigue properties, and excellent corrosion resistance. Further experimental test onSMA Dampers were conducted by DesRoches and Delmont (2002) and Aiken et Al. (1993), andanalytical models were developed by DesRoches and Delmont (2002), Liang–Rogers (1990) andIvshin–Pence (1994).

Table 6-10. Comparison of NiTi SMA properties with typical structural steel

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Fig.6-22. Superelasticity Property

6.2.6.2 SCD Typologies: The Energy Dissipating Restraint

Fluor Daniel, Inc., has developed and tested a type of friction device, called Energy Dissipating

Restraint (EDR). The mechanism of the EDR consists of sliding friction with a stop located at theend of the range of motion. A full description of the EDR mechanical behavior and detaileddiagrams of the device are given by Nims (1993).

Fig.6-23. External and internal views of the EDR, Nims et Al. (1993)

6.2.6.3 The Friction Spring Seismic DamperThe SHAPIA seismic damper, also known as friction spring damper, uses a ring spring to dissipateearthquake-induced energy (Kar and Rainer 1995, 1996; Kar et Al. 1996). A section through atypical ring spring assembly ( Fig.6-24 ) consists of outer and inner rings that have tapered matingsurfaces.As the spring column is loaded in compression, the axial displacement is accompanied by sliding ofthe rings on the conical friction surfaces: the outer rings are subjected to circumferential tension(hoop stress), and the inner rings experience compression. The ring springs are designed to remainelastic during a seismic event so that no repair or replacement should be required, and the structureshould thus be protected against aftershocks and future earthquakes.The force-displacement response of SHAPIA Dampers has been further investigated by Filiatraultet al. (2000).

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Fig.6-24. Friction Spring Details. 1—Outer Ring; 2—Inner Ring; 3—Inner Half Rin g

6.2.7 Electro and Magnetorheological Dampers

Magnetorheological Dampers (DMPs) typically consist of hydraulic cylinders containing micron-sized magnetically polarizable particles suspended within a fluid. With a strong magnetic field, the

particles polarize and offer an increased resistance to flow. By varying the magnetic field, themechanical behaviour of the MRD can be modulated: MR fluids can be changed from a viscousfluid to a yielding solid within millisecond and the resulting damping force can be considerably

large with a low-power supply. Electrorheological Dampers (ERDs) are the electric analogue ones.ER fluid contains micro-sized dielectric particles and its behaviour can be controlled by subjectingthe fluid to an electric field. Magnetorheological fluids are an alternative solution toElectrorheological ones when very compact devices are needed, as the rheological behaviour issimilar to the ER-fluids but with higher yield stress. In the case of steady fully developed flow, theshear resistance of MR/ER fluids may be modelled as having a friction component augmented by a

Newtonian viscosity component. MR/ER Dampers can be placed between the chevron brace and therigid diaphragm or beam.

6.2.7.1 Control Strategies with MR/ERDs

Control strategies based on semi-active devices combines the reliability of passive systemsmaintaining the versatility of active devices operating on battery power only. A semi-active controldevice doesn’t input mechanical energy into the controlled structural system, but it can becontrolled to optimally reduce the system response. MR and ER dampers can be either employed as

passive and semi-active devices or as active control devices.

6.2.7.1.1 Optimal Force ControlBecause the damper force generated in the semi-active dampers is dependent on the response of theframe structure, the desirable optimal control force cannot always be produced by the j th damper.Only the damper force, F d due to the yielding shear stress in fluids can be controlled through thechange in the applied electric or magnetic field.

The concept of the clipped Optimal force control is the following (Ribakov and Gluck (2002)):when the j th damper is providing the desirable optimal force, the voltage applied to the dampershould remain at the present value; if the magnitude of the force produced by the j th damper issmaller than the magnitude of the desired optimal force, and the two forces have the same sign, thevoltage applied to the damper has to be increased; otherwise it has to be set to zero.

6.2.7.1.2 Optimal Displacement ControlAs the optimal displacement vector cannot be directly controlled, the approach is to control F d suchthat the measured displacement vector traces the optimal displacement vector as close as possible.The concept is the following (Xu et Al. (2000)): when the j th damper displacement is approachingthe desirable optimal value, the friction force in the damper should be set to its minimum value soas to let the damper reach its optimal displacement as soon as possible. When the j th damper movesin opposite direction to the optimal displacement, the friction force F dj in the damper should be setto its maximum value (or to the j th damper force if smaller, otherwise it stops moving and no

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vibration energy can be dissipated) so as to prevent the damper motion away from the optimal targetat most.

6.2.7.2 Magneto-Rheological Dampers

MR fluid is composed of oil and varying percentages of iron particles that have been coated with ananti-coagulant material. When unactivated, MR fluid behaves as ordinary oil, while if exposed to a

magnetic field, micron-size iron particles that are dispersed throughout the fluid align themselvesalong magnetic flux lines. This reordering of iron particles can be visualized as a large number ofmicroscopic spherical beads that are threaded onto a very thin string. Once aligned in this fashion,the iron particles resist being moved out of their respective flux lines and act as a barrier to fluidflow.MR fluid can be used in three different ways, referred to as squeeze mode, valve mode, and shearmode (Fig.6-25). The last mode is the most widely used: the MR fluid is used to impede the flow ofMR fluid from one reservoir to another.When MR fluid is used in the valve mode, the areas where the MR fluid is exposed to magnetic fluxlines are usually referred to as “choking points” (see Fig.6-26). Varying the magnetic field strengthhas the effect of changing the apparent viscosity of the MR fluid. The term “apparent viscosity” isused since the carrier fluid exhibits no change in viscosity as the magnetic field strength is varied.Upon exposure to a magnetic field, the MR fluid as a whole will appear to have undergone a changein viscosity. As the magnetic field strength increases, the resistance to fluid flow at the choking

points increases until the saturation point has been reached. This resistance to movement that theiron particles exhibit is what allows us to use MR fluid in electrically controlled viscous dampers.

Fig.6-25. MR fluid used in squeeze, shear and valve modes

Fig.6-26. Typical MR damper

6.2.7.2.1 Monotube and Twin Tube Magneto-Rheological DampersAmong the MR devices have to be mentioned the Monotube (Fig.6-27, (a)) and the Twin-Tube

Dampers (Fig.6-27, (b)), and also the double-ended MR damper (Fig.6-28, left) and the MR pilotedhydraulic dampers (Fig.6-28, right) (Casarotti, (2004)).

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(a)

(b)

Fig.6-27. Monotube MR damper and Twin tube MR damper section view

Fig.6-28. Double-ended MR damper (left) and MR piloted hydraulic damper (right).

6.2.7.2.2 MR Damper ModelThe MR Damper hysteretic behaviour is nonlinear, and can be modelled by various hysteresysmodels, as proposed by Bingham (in Shames and Cozzarelli, 1992), Spencer et Al. (1997), Bouc,(1967), Wen, (1976), etc.

6.2.7.3 Electro-inductive devices

Principles of operation of the electro-inductive devices are: (i) the generation of electrical powerfrom seismic vibration as a primary energy source for the device mechanical input (passive andsemi-active devices); (ii) the regulation of the sign and of the amount of the instantaneous powerflow exchanged between earthquake and device in order to achieve a real time control of thevibration modes of the structure to be protected (active devices).Two possible working schemes are addressed by Marioni (2002): a linear dissipator (Fig.6-29, left),

basically composed by two plates with permanent magnets and an inner plate of conductive nonmagnetic material moving between the previous two; and a rotating system Fig.6-29 where thelinear earthquake motion is converted into a rotational one through a screw: the advantage of thissolution is the possibility of amplifying the relative velocity by a suitable selection of the ratio

between linear and rotational motion. Advantages of these devices are low maintenance, no ageingeffects, no limitations on life cycles, low scattering of the response and no temperature sensitivity.Passive energy dissipating systems have inherent limitations such as they are generally tuned to the

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first vibration mode, while active ER dampers can be effective over a much wider range offrequencies.The electro-inductive dissipators can be compared to the viscous dampers, due to their capability of

providing both viscous and friction-type forces. The damping force developed by ER Damperdepends on physical properties of the used fluid, on the pattern of flow in the damper and on itssize. When an electric field is applied, the behaviour of the ER fluid is nearly viscoplastic, and theshear stress in it has to exceed the developed ‘yield’ stress to initiate flow. This mechanism isresponsible for their controllable viscoplastic behaviour. The force produced by a linear fluidviscous device, is proportional to the velocity of the piston in the fluid, up to a limiting frequency,

beyond which the device becomes viscoelastic; the resulting damping force f ER (t) in the ER damperis given in equation (6-55) where C d is the viscous characteristic of the viscous ERD, x is thedisplacement at the damper location and F is the controllable yield force.

Fig.6-29. ER Dampers: linear (left) and rotating (right) working schemes (Marioni, 2002)

[ ])t(xFsign)t(xC)t(f dER && += (6-55)

6.2.7.3.1 Viscous and Adjustable friction-type forces for Electrorheological DampersMakris at Al. (1996) showed that under long-period rapid pulses, viscous dissipation combined withcontrollable friction-type dissipation can reduce substantially structural displacements demands bykeeping accelerations at low levels. ER dampers can supply the friction force needed at the

beginning of the shaking through their capability of developing rigid visco-plastic behaviour, butthey are able to avoid residual drifts by removing friction forces at some point of the shaking. ERdampers can operate as passive devices in absence of power, providing optimum response with aminimum amount of power supplied with a battery, being relatively inexpensive when compared tohydraulic dampers with mechanically controlled orificing.Other ER dampers involving shear flow have been designed in past: among these the device

developed by Makris et Al. (1996), which response is extensively discussed in the work of Casarotti(2004).

6.2.7.3.2 Effects on rigidity-plasticity, viscosity of ER dampers with near-field ground motionAdjusting the type of dissipation mechanism allows protecting a structure from totally differentmotions that might be generated from the same earthquake only some kilometer apart. Makris(1997) studied the effects of near-source earthquake motions on one- or two-span isolated bridgesequipped with energy friction-type dissipators: considering dampers exhibiting a behaviour rangingfrom rigid-plastic to purely viscous, in order to avoid the permanent displacements coming fromlarge friction forces, those latters can be relaxed at some instant during the free vibration of thestructure, while using viscous mechanisms to damp free vibrations.

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6.3 Design concepts and analysis of deck – isolated bridges

6.3.1 Analysis concepts

Instead of a non-linear dynamic analysis, a static linear SDOF analysis can be adopted in a preliminary design phase or in the case of bridges with a regular geometric layout and a regularmass distribution. In these cases the coupling effect of the deck can be neglected and the design ofeach bent will be independent from the others.The single bent will be modelled as a SDOF system with an appropriate tributary mass, effectiveglobal stiffness and effective global damping. The SDOF parameters can be defined by:• Effective global stiffness:

DE pyg K K

K /1/1

1+

= (6-56)

where: pyK is the secant stiffness to yielding of the pier and is the secant stiffness at the expected

maximum displacement (displacement demand on the isolator) of the isolation system; DE K

• Effective global damping:In the case of isolation systems with essentially linear response and viscous dampers asdissipative devices:

D p

DV D p pg ∆+∆

∆+∆= ξ ξ

ξ (6-57)

Where pξ is the equivalent viscous damping of the soil-foundation-pier system, DV ξ is the

viscous damping provided by the device and D p ∆∆ , are respectively the displacement of the pier, and the displacement of the isolation system.

In the case of isolation systems with essentially hysteretic energy dissipation the term DV ξ have

to be replaced by the effective damping equivalent to the dissipated hysteretic energy ( DE ξ ):( )

π ξ G

DE

/112 −= (6-58)

Where the effective global ductility of the soil-pier-isolation system can be obtained by:

( ) DE S

DE DG ∆+∆

∆−+= 11 µ µ (6-59)

Equation (6-59) shows that the damper ductility ( µD) will be reduced by the additionalflexibility of the soil-pier system ( ∆S).

A non-linear dynamic analysis is always recommended after the preliminary design phase. The

MDOF model should be progressively refined according to design earthquake intensity. For themaximum credible earthquake the deck-isolated bridge should be modelled considering in a morerefined way:• I/D devices: it’s more appropriate to use at least a tri-linear spring model (instead of a linear

equivalent highly damped element), with the third branch to simulate a possible strain hardening(that can develop for example using steel dampers) or the simulation of displacement-limitingdevices;

• Piers: in the case of a large-than-expected earthquake also the piers could have to sustain a plastic deformation with the ductility demand that could soon became excessive, and thus a morerefined bi-linear model should be used (a value of 2% should be adopted for the equivalentviscous damping ratio). It’s also important to account for the actual mass distribution along the

pier height in order to consider a possible amplification of the higher mode response due to the

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response of the pier alone, possible when the lower-frequency modes involving the deck massare isolated;

• Deck: modelled as linear beam elements, with a proper mass distribution;• A linear model of the soil response is adequate in most cases.

6.3.2 Basics of capacity design

The main design objective in a deck-isolated bridge is to concentrate most of the damage in the I/Ddevices thus preventing damage of the remaining part of the structure, whose response is therefore

principally linear elastic with some possible damage localized at movements joints due to largestructural displacements.The design procedure for such structures will follow the same general Capacity Design (CD)

principles. The protection factor to be applied depends on the reliability of the mechanicalcharacteristics of the isolation system: in most cases it is required that the actual strength of an I/Ddevice does not differ by more than 10% from it’s design strength. Then, requiring that the strengthof the device at the expected displacement be equal to 85% of the design nominal strength of the

pier, we will obtain a protection factor against the pier yielding.

The CD principles still have to be applied, although it will no longer to be necessarily to ensure thatcolumn shear strength exceeds column flexural strength. Therefore it is required only to assure anadequate inelastic rotational capacity at the pier base. According to basic CD principles the estimateflexural strength M n, reduced by a reduction factor Φ f , has to be larger than the required strength M r (according to equation (6-60)). Capacity protection factors have also to be applied to the strengthsof supports, connections and abutments.

r n f M M ≥Φ (6-60)

6.3.3 Considerations on input characteristics

Near-field ground motions (characterized by high frequency spike and low-frequency, low-acceleration pulses) include large pulses that may greatly amplify the dynamic response of long

period structures, particularly if structures deform in the inelastic range. In recent years severalseismologists have doubted that base-isolated structures are vulnerable to large pulse-like groundmotions generated at near-fault locations.Makris and Chang (2000), observing that near source ground motions are particularly destructive tosome structure because not of their PGA, but of their ‘incremental’ ground velocity, sustained thatseismic isolation could be effective against near-source ground motions provided that theappropriate energy dissipation mechanism is assured.

6.4 Foundation rocking and pier base isolation

6.4.1 Basics of foundation rocking

It has been observed after several earthquakes that a number of structures had responded to seismicexcitation by rocking on their foundation, and in some cases this enabled them to avoid failure.Such behaviour will occur principally in structures like elevated water or storage tanks,characterized by large masses at some distance from the ground and comparatively narrow bases. Inthese slender structures the overturning moment at the base will govern the response and, if rockingand uplift is possible, it can be limited to the moment needed to lift the weight of the structureagainst the stabilizing moment due to gravity, thus reducing the magnitude of the internal forces andthe deformation demand throughout the structure.

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For these reasons the rocking mechanism will often be considered as a satisfactory response inassessment of existing bridges or useful as an alternative approach in the design of new ones, wheregeometry, mass distribution and foundation characteristics could favour a controlled rockingresponse in the transverse direction, according to the capacity of the superstructure to accommodatesuch movements.The seismic response of a rocking bridge is similar with that of a bridge isolated by FPS, because itfollows the same inverted pendulum concept. The correspondent hysteretic behaviour will beapproximately rigid-plastic with a substantial re-centering force given by the uplift force itself.Rocking, either of spread footings or pile-supported footings without tension connections between

piles and footings, will results in an approximately non-linear elastic behaviour; instead whentension connection between the piles and footings is assessed to be competent (analyses may showthat pile uplift is expected under the column plastic moment capacity) an additional lateral strength,due to the pile tension capacity, and an additional damping, due to the Coulomb friction associatedwith pile friction, will develop (Fig.6-30).

Fig.6-30. Rocking response of a footing with uplifting piles6.4.2 soil – structure interaction (contribution from Alain)6.4.3 pier base isolation

6.5 Controlled rocking of piers and built–in isolators

6.5.1 Controlled rocking of combined concrete members

In order to design (or asses) a rocking bridge a substitute structure design method can be followed,assuming, similar to the case with isolation devices, that the response will depends only on theequivalent elastic characteristics (period and damping) at peak response.The entire structure can be analysed, in a preliminary phase, considering separately each single

bridge bent modelled as a rigid single-degree-of-freedom oscillator with constant damping and period of vibration proportional to the amplitude of rocking. In fact the period of vibration of therocking response will increase with displacement amplitude and thus a trial-and-error design

procedure have to be performed.This design procedure takes its basic principles on the rocking mechanism of a rigid block and it ischaracterized by the following main issues:• Definition of weights: at the deck level will act the seismic weight Ws and at the footing level

the total weight W (which includes also the weight of the pier not included in the seismic weightand the footing weight);

• Soil-footing interface: the foundation is considered as a rigid block and at the soil-footinginterface can be assumed to develop a rigid perfectly plastic pressure distribution in compression

and tension (p c, p t); this results in a rectangular stress block with width a in the compression zone(Fig.6-31):

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( )t c

t

p p BW BLp

a++=

(6-61)

Fig.6-31. Rocking mechanism of a single pier

• Lateral overturning force: its magnitude can be evaluated, in correspondence to the totaldisplacement ∆ (that include also the structural displacement, for slender piers), by the momentequilibrium:

( ) ( )

( ) H a L H

W a LW L RV

r

st E 2/

2/2/−∆+

∆−−+=∆ (6-62)

Simplifications may occur in the above relationship:

o if the pier is stiff: ;r c ∆≡∆→≅∆ 0

o if the pier is tall: ( ) 02/ ≅−∆ H a Lr ;

o or when no tension occurs at the footing level: 0≅t R ;• Effective stiffness of the rocking pier: if the single bent rocking mechanism is more likely to

develop then:( ) ∆∆= / E pier V k (6-63)

• Instead, when a stiff superstructure connects several bents, rocking of the whole structure willoccur and the effective stiffnesses for n bents can be combined to an effective frame stiffness ofthe bridge:

∑ ∆=n

n E frame V k /, (6-64)

• And the correspondent period will be:5.0

,2⎟⎟

⎞⎜⎜

⎛ = ∑

n frame

ns

gk

W T π (6-65)

• Energy dissipation: in the foundation rocking mechanism of a rigid block an important role is played by the energy dissipation, in the form of radiation to the soil half space, that will developas a consequence of the blocks-soil collisions, if these are assumed purely inelastic impacts. This

phenomenon, expressed through the kinetic energy reduction factor r (obtained by equating

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momentum before and after the impact) leads to a progressive reduction of the peakdisplacement amplitude (expressed as a dimensionless quantity ∆n, equal to the actualdisplacement divided by the width of the foundation) as the number of impacts n increase.

( )[ ]{ }5.0201111 ∆−−−−=∆ n

n r (6-66)Then, considering that the equivalent viscous damping of a single-degree-of-freedom oscillatoris related to the relative amplitude of different displacement peaks after m complete cycles bythe expression:

( )m

n

π ξ

2/ln 0 ∆∆= (6-67)

And considering that in the rocking response there are two impacts per cycle the equivalent

damping ratio of a rigid rocking system can be found. Under the hypothesis of andthis relation is rather insensitive to the value of the initial displacement and the

number of cycles, and a linear expression can be used ((6-68), Fig.6-32):

5.00 <∆162 <= mn

( )r −= 148ξ (6-68)

Fig.6-32. Approximate relationship equivalent viscous damping – energy reduction factor

In the case of bridge structures a simplified expression, neglecting the contribution of pier andfoundation mass and assuming deck width larger than the deck height in the computation of themass moment of inertia, for the evaluation of r can be used:

( )( )2

22

2

12/2cos1

1 ⎟⎟

⎠ ⎞

⎜⎜

⎝ ⎛

+−−=

b R R

r α

(6-69)

where α is the angle between a vertical line and the line connecting the mass centroid and thecenter of rotation.

The definition of the amount of damping involved in the rocking phenomenon will be one of themost important issues regarding the rocking mechanism; here only the soil radiation dampingcontribution is considered, but also the amount due to hysteretic response of dampers can beintroduced in those cases where these kind of devices are used.

Based on these basic principles a response spectra design approach for rocking bridges can be pursue, following these steps:

a. Model a bridge bent as a rigid single-degree-of-freedom oscillator with constant dampingand period of vibration proportional to the amplitude of rocking, using equivalent values at

peak response; b. Use the initial no-rocking period and damping ratio to evaluate if the elastic response

acceleration will induce rocking;c. compute the kinetic reduction factor r and then the equivalent damping ratio ξ of the rockingresponse through the equation (6-68);

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d. Assign a displacement ∆1, calculate V E(∆1) through the equation (6-62) and thecorrespondent period of vibration T 1;

e. Calculate from the displacement response spectrum a new displacement ∆2=S d(T1,ξ);f. Iterate until convergence of a couple of values of period and displacement. In order to

achieve a stable response, the use of linearly increasing displacement response spectrashould be avoided, which also do not correspond to reality;

g. Design the structure to behave linearly until rocking takes place and to be able toaccommodate the expected displacement;h. Time-history analyses are finally recommended to check the design (or assessment) of the

rocking bridge since all the simplified expression used in this procedure can be consideredadequate only for a preliminary design.

6.5.2 Response of partially prestressed coupled members

A useful alternative in the design of rocking bridges will be given by the use of unbounded post-tensioning techniques in order to create jointed ductile connections at pier-foundation or pier-deckinterface. They will accommodate the inelastic demand within the connection itself and maintain

the structure in the elastic domain, thus limiting the damage to pier elements achieving themaximum target displacement.This kind of connections are usually defined by a prestressed elastic anchorage or bar/tendon andeventually an energy dissipation devices (typically mild steel reinforcement added at criticalsections to the unbounded post-tensioned elements): the restrainers will provide a smaller rotation(i.e. a reduced value of the kinetic reduction factor r ) preventing the toppling of small slenderrocking blocks, and the dissipative element will increase the energy dissipation capacity of thesystem.The combination of such elements (called controlled rocking systems or hybrid rocking systems )will lead to a flag-shaped hysteresis loop, which properties can be calibrated by changing the design

parameters of each element, such as the magnitude of the post-tensioning load in the unbounded

members or the additional strength provided by the mild steel bars. The main design parameter thatwill govern the design of these connections is the ratio λ between the resisting moment provided bythe axial load components (the weight component M N and the contribution due to the post-tensioning load M pt ) and the moment M s provided by the mild steel elements.

s

N pt

M

M M +=λ (6-70)

As this latter contribute became larger the global response will approximate the elasto-plastic behaviour, resulting in an higher energy dissipation but lost of the re-centering properties; instead,as λ increases the response will approach the non-linear elastic behaviour with any dissipation

properties but providing full re-centering of the system.

Several analytical and experimental studies have been performed in order to evaluate the responseof hybrid rocking systems (Palermo, (2004)), in terms of their moment-rotation relationship andtheir efficiency and potentiality as an alternative solution in the seismic design of bridges. Theyhave pointed out not only the primary role of the parameter λ in their design procedure, but also, asin the case of reinforced concrete sections (Priestley and Kowalsky, (1998)), the invariance of theyielding curvature with mechanical parameter. Consequently the definition of a coefficient K θ y,invariant with respect to structural and sectional parameters, is occurred for every section profile:

L

hK

sy

y y ε

ϑ ϑ =, (6-71)

Where: θ y is the yielding rotation, ε sy the yielding strain of the mild steel, h the height of the section

and L the height of the pier.Through the comparison of the performance of controlled rocking designed bridges and monolithicsystems under static cyclic forces as well as time-history records, it has been found that,

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eqii

iii V

m

mF

⎟⎟

⎞⎜⎜

⎛ ∆

∆= ∑ (6-76)

8) Evaluate the deformed shaped and the pier base shear obtained in the static analysis anditerate until convergence of the maximum displacement to the target one.

6.5.3 design and analysis of segmented piers6.5.4 built – in isolators (contribution from Kazuhiko)

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6.6 References

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