 
          2768
        
        
          Proceedings of the 18
        
        
          th
        
        
          International Conference on Soil Mechanics and Geotechnical Engineering, Paris 2013
        
        
          2 THEORETICAL BACKGROUND
        
        
          1.1
        
        
          
            Fiber-optic Bragg Grating (FBG) sensors
          
        
        
          FBG sensors inscribe stripe-like grating on the photosensitive
        
        
          fiber optic core by exposing the latter to ultraviolet (UV)
        
        
          radiation by periodically distributing the strength of the light.
        
        
          Once formed, FBG sensors serve as reflectors that reflect light
        
        
          with a pattern-specific wavelength. This reflected wavelength is
        
        
          called the Bragg wavelength and is as in Equation (1). In other
        
        
          words, when broad-spectrum light beams are transmitted to the
        
        
          FBG, light with the Bragg wavelength is reflected and
        
        
          remaining light with other wavelengths passes through.
        
        
          
        
        
          
        
        
          = 2
        
        
          
        
        
          Λ
        
        
          (1)
        
        
          where
        
        
          
        
        
          
        
        
          is Bragg wavelength,
        
        
          
        
        
          
        
        
          is the effective refractive
        
        
          index of the fiber-optic core, and
        
        
          
        
        
          is the interval of the grating
        
        
          inscribed on the fiber-optic core.
        
        
          Changes in strain and the temperature affect the effective
        
        
          refractive index,
        
        
          
        
        
          
        
        
          , and the grating period,
        
        
          
        
        
          , so that the Bragg
        
        
          wavelength comes to shift. In comparison with the initial Bragg
        
        
          wavelength,
        
        
          
        
        
          
        
        
          , the shifted amount of wavelength,
        
        
          
        
        
          , is given
        
        
          as
        
        
          Δ/
        
        
          
        
        
          = 1 − 
        
        
          
        
        
           + 
        
        
          
        
        
          + 
        
        
          
        
        
          Δ
        
        
          (2)
        
        
          where the first term of Eq. (2) is the amount shifted due to strain,
        
        
          
        
        
          
        
        
          is the photoelatic constant, and
        
        
          
        
        
          is the strain underwent by
        
        
          the grating. The second term of Eq. (2) shows the shift of the
        
        
          wavelength caused by the change of temperature,
        
        
          
        
        
          
        
        
          is the
        
        
          thermal expansion coefficient of the fiber optic, and
        
        
          
        
        
          
        
        
          is the
        
        
          thermo-optic coefficient of the fiber optic. Because the
        
        
          experiments in the present study were conducted in a controlled
        
        
          laboratory environment, changes in the temperatures of the
        
        
          sensors themselves and their surroundings were negligible such
        
        
          that
        
        
           = 0
        
        
          . Consequently, the second terms was eliminated so
        
        
          that it is possible easily to calculate strain from the wavelength
        
        
          shift as shown in Eq. (3).
        
        
           =
        
        
           
        
        
          
        
        
           
        
        
          
        
        
          (3)
        
        
          where the photoelastic constant,
        
        
          
        
        
          
        
        
          = 0.229, provided by the
        
        
          manufacturer.
        
        
          1.2
        
        
          
            Integration by Gaussian quadrature
          
        
        
          In numerical analysis, a quadrature rule is an approximation of
        
        
          the definite integral of a function, usually stated as a weighted
        
        
          sum of function values at specified points within the domain of
        
        
          integration. An n-point Gaussian quadrature rule is a quadrature
        
        
          rule constructed to yield an exact result for polynomials of
        
        
          degree
        
        
          2 − 1
        
        
          or less by a suitable choice of the points
        
        
          
        
        
          
        
        
          and
        
        
          weights
        
        
          
        
        
          
        
        
          for i  = 1, …, n. The domain of integration for such a
        
        
          rule is conventionally taken as [-1, 1], so the rule is stated as
        
        
           
        
        
           
        
        
          ≈ ∑ 
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          .
        
        
          (4)
        
        
          Gaussian quadrature as above will only produce accurate
        
        
          results if the function
        
        
          
            f(x)
          
        
        
          is well approximated by a polynomial
        
        
          function within the range between -1.0 and +1.0. If the
        
        
          integrated function can be written as
        
        
           = 
        
        
          
            ,
          
        
        
          where
        
        
          
        
        
          is approximately polynomial, and
        
        
          
        
        
          is known, then
        
        
          there are alternative weight
        
        
          ′
        
        
          
        
        
          such that
        
        
           
        
        
           
        
        
          =  
        
        
           
        
        
          ≈ ∑ ′
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          .
        
        
          (5)
        
        
          For the simplest integration problem, i.e. with
        
        
           = 1
        
        
          ,
        
        
          the associated polynomials are Legendre polynomials,
        
        
          
        
        
          
        
        
          
        
        
          ,
        
        
          and the method is usually known as Gauss-Legendre quadrature.
        
        
          With the nth polynomial normalized to give
        
        
          
        
        
          
        
        
          1 = 1
        
        
          , the i-th
        
        
          Gauss node,
        
        
          
        
        
          
        
        
          , is the i-th root of
        
        
          
        
        
          
        
        
          . Its weight is given by
        
        
          (Abramowitz and Stegun 1972)
        
        
          
        
        
          
        
        
          =
        
        
          
        
        
          
        
        
           
        
        
          [
        
        
          
        
        
          
        
        
          
        
        
          ]
        
        
          
        
        
          (6)
        
        
          A few order rules for solving the integration problem are listed
        
        
          in Table 1.
        
        
          Table 1. Position of Gauss points and corresponding weights.
        
        
          Number of Gaussian
        
        
          points,
        
        
          
            n
          
        
        
          
            gp
          
        
        
          Location,
        
        
          ξ
        
        
          i
        
        
          Weight,
        
        
          
            w
          
        
        
          i
        
        
          1
        
        
          0.0
        
        
          2.0
        
        
          2
        
        
          ±
        
        
          0.57732502692
        
        
          1.0
        
        
          3
        
        
          ±
        
        
          0.7745966692
        
        
          0.0
        
        
          0.555 555 5556
        
        
          0.888 888 8889
        
        
          An integral having arbitrary limits can be transformed so that
        
        
          its limits are from -1 to +1. With
        
        
           = 
        
        
          , and with the
        
        
          substitution
        
        
           =
        
        
           
        
        
          1 − 
        
        
          
        
        
          +
        
        
           
        
        
          1 + 
        
        
          
        
        
          ,
        
        
           
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          =  
        
        
           
        
        
          ≈ ∑ ′
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          .
        
        
          (7)
        
        
          Thus the integrand is changed from
        
        
           = 
        
        
          to
        
        
           = 
        
        
          ,
        
        
          where
        
        
          
        
        
          incorporates the Jacobian of the transformation,
        
        
           = / = 1/2
        
        
          
        
        
          − 
        
        
          
        
        
          
        
        
          . If the function
        
        
           = 
        
        
          is not a
        
        
          polynomial, Gauss quadrature is inexact, but becomes more
        
        
          accurate as more points are used.
        
        
          1.3
        
        
          
            The differential equations of the deflection for a
          
        
        
          
            cantilever beam subjected to a point load
          
        
        
          As shown in Figure 1, lateral displacement, y, which is
        
        
          produced when pile heads are subjected to a lateral load, P,  and
        
        
          not to axial load, is expressed in terms of differential equation,
        
        
          as in Equation (8).
        
        
          
        
        
          
        
        
          
        
        
           
        
        
          
        
        
          =  =  − 
        
        
          (8)
        
        
          where
        
        
          
            E
          
        
        
          is the Young’s modulus of the pile material,
        
        
          
            I
          
        
        
          is the
        
        
          moment of inertia of the section area of the pile,
        
        
          
            x
          
        
        
          is the
        
        
          distance from the pile end, and
        
        
          
            M
          
        
        
          is the sectional moment.
        
        
          Integrating Eq. (8) yields the function of the slope,
        
        
          
            S
          
        
        
          , as
        
        
           =
        
        
           
        
        
          = 
        
        
          
        
        
          
        
        
           
        
        
          
        
        
          
        
        
           
        
        
          =
        
        
           
        
        
           −
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          (9)
        
        
          For the cantilever beam, the slope,
        
        
          
            S
          
        
        
          = /
        
        
          , remains zero at
        
        
          the clamped end (i.e.,
        
        
          
            x
          
        
        
          = 0). Integrating Equation (9) again
        
        
          yields an expression of the lateral displacement,
        
        
          
            y
          
        
        
          , as
        
        
           = 
        
        
           
        
        
          
        
        
           
        
        
          =
        
        
           
        
        
          
        
        
          
        
        
          
        
        
          
        
        
          −
        
        
          
        
        
          
        
        
          
        
        
           =
        
        
          
        
        
          
        
        
          
        
        
          3 − 
        
        
          (10)
        
        
          As a result, the maximum deflection, y
        
        
          max
        
        
          , occurs at the point of
        
        
          the lateral load, given as
        
        
          
        
        
          
        
        
          =
        
        
          
        
        
          
        
        
          
        
        
          (11)
        
        
          Note that two sequential integrations are necessary to obtain the
        
        
          displacement function of Eq. (10) from the moment function of
        
        
          Eq. (8).