Ground motion selection
Considering far-field earthquakes, the ground motion with a source distance more than 100 km is selected. The intensity of selected ground motions is scaled to the seismic fortification intensity of the HSR bridge, corresponding to 8-degree design earthquake with the PGA of 0.3g (0.1g for frequent earthquake) [8]. The site is located on the medium hard soil associated with the shear velocity of 250–500 m/s, represented as the characteristic period of 0.4 s in the design spectrum. Considering the seismic energy input, the effective time duration of selected ground motion records should be more than 10 times the fundamental periods of bridge–track system models. To obtain more reliable results, at least seven seismic records should be selected for seismic analysis of the structure according to the Chinese code [38]. In this paper, 12 ground motion records from the PEER Strong Ground Motion Database [41] are selected, as shown in Table 3, Rrup is the closest distance to the rupture surface. The mean spectra acceleration (Sa) of selected ground motions is in basic agreement with the design Sa, as shown in Fig. 3.
Table 3 Selected ground motion records Analytical solution of ground motion for V-shaped canyon
To accurately evaluate the canyon seismic effect, this paper adopts the seismic wave analytical model of the V-shaped canyon proposed by Tsaur [42]. The SH waves are used as excitations of the model and the displacement is in the y-direction (Fig. 1). Since this paper only considers the impact of transverse (y-direction) ground motion on the seismic damage of the irregular HSR bridge–track system under the topography effect, only the SH wave is selected as the ground motion input model.
The regional division idea is used to divide the V-shaped canyon into two parts, as shown in Fig. 4. The origin of global coordinate systems \(\left( {x,y} \right)\) and \(\left( {r,\theta } \right)\) is set at the center of the canyon top, while the origin of local coordinate systems \((x_{1} ,y_{1} )\) and \((r_{1} ,\theta_{1}\)) is at the canyon bottom. The model medium is assumed to be elastic, isotropic, and homogeneous, in which only scattered sites exist in region ②, and there are both scattered and free sites in region ①. \(\alpha\) is the incident angle of SH wave, a is the half-width of the canyon, d is the depth of the canyon, and \(c = 400 {\text{m}}/{\text{s}}\) is the velocity of shear wave.
Region ① and region ② should satisfy the wave equation:
$$\nabla^{2} u_{j} + k^{2} u_{j} = 0,\,\,\,\, j = 1,2,$$
(3)
where \(\nabla^{2}\) is the two-dimensional Laplacian operator; \(k = \omega /c\) is the shear wavenumber, and \(\omega\) is circular frequency; uj is the displacement of region j, where j = 1 and 2, representing the total displacement sites in regions ① and ②, respectively.
The displacement and stress continuity conditions of region ① and region ② and the condition of zero stress on the surface of the canyon should satisfy
$$\tau_{\theta z}^{1} = \frac{\mu }{r}\frac{{\partial u_{1} \left( {r,\theta } \right)}}{\partial \theta } = 0,\,\,\,\,\,\theta = \pm \frac{\pi }{2}, r > a,$$
(4)
$$\tau_{{\theta_{1} z}}^{2} = \frac{\mu }{{r_{1} }}\frac{{\partial u_{2} \left( {r_{1} , \theta_{1} } \right)}}{{\partial \theta_{1} }} = 0,\,\,\,\,\,\theta_{1} = - \beta_{1} ,\beta_{2} ,$$
(5)
where \(\tau_{\theta z}^{1}\) and \(\tau_{{\theta_{1} z}}^{2}\) are the stress on the horizontal ground surface and the canyon surface, respectively; \(\beta_{1} {\text{ and }}\beta_{2}\) are angels as shown in Fig. 4. For the region ①, the wave site can be divided into two parts: the free site caused by the incident SH wave when there is no V-shaped canyon and the scattered site caused by the V-shaped canyon. The total free site displacement of region ① can be obtained by superposing the incident wave and the reflected wave:
$$u_{{\text{f}}} \left( {r,\theta } \right) = \exp \left[ {{\text{i}}kr{\text{cos}}\left( {\theta + \alpha } \right)} \right] + \exp \left[ { - {\text{i}}kr{\text{cos}}\left( {\theta - \alpha } \right)} \right],$$
(6)
where i is the imaginary unit and equal to the square root of −1.
Using Eqs. (3)-(6), the wave equation of region ① and region ② in the plane wave site can be obtained by the wave function expansion method:
$$\begin{aligned} u_{{\text{f}}} \left( {r,\theta } \right) = & 2\sum\nolimits_{n = 0}^{\infty } {\varepsilon_{n} \left( { - 1} \right)^{n} J_{2n} \left( {kr} \right)\cos \left( {2n\alpha } \right)\cos \left( {2n\theta } \right)} \\& - 4\text{i}\sum\nolimits_{n = 0}^{\infty } {\left( { - 1} \right)^{n} J_{2n + 1} \left( {kr} \right)\sin \left[ {\left( {2n + 1)\alpha } \right)} \right] \times \sin \left[ {\left( {2n + 1)\theta } \right)} \right]} \\ \end{aligned},$$
(7)
$$\begin{aligned} u_{{{\text{s0}}}} \left( {r,\theta } \right) = & - 2\sum\nolimits_{n = 0}^{\infty } {\varepsilon_{n} \left( { - 1} \right)^{n} \frac{{J_{2n}^{^{\prime}} \left( {ka} \right)}}{{H_{2n}^{{\left( 2 \right)^{^{\prime}} }} \left( {ka} \right)}}H_{2n}^{\left( 2 \right)} \left( {kr} \right) \times \cos \left( {2n\alpha } \right)\cos \left( {2n\theta } \right)} \\& + 4\text{i}\sum\nolimits_{n = 0}^{\infty } {\left( { - 1} \right)^{n} \frac{{J_{2n + 1}^{^{\prime}} \left( {ka} \right)}}{{H_{2n + 1}^{{\left( 2 \right)^{^{\prime}} }} \left( {ka} \right)}}H_{2n + 1}^{\left( 2 \right)} \left( {kr} \right) \times \sin \left[ {\left( {2n + 1)\alpha } \right)} \right]\sin \left[ {\left( {2n + 1)\theta } \right)} \right],} \\ \end{aligned}$$
(8)
$$u_{{{\text{s1}}}} \left( {r,\theta } \right) = \sum\nolimits_{n = 0}^{\infty } {A_{n} \frac{{H_{2n}^{\left( 2 \right)} \left( {kr} \right)}}{{H_{2n}^{{\left( 2 \right)^{^{\prime}} }} \left( {ka} \right)}}\cos \left( {2n\theta } \right)} + \sum\nolimits_{n = 0}^{\infty } {B_{n} \frac{{H_{2n + 1}^{\left( 2 \right)} \left( {kr} \right)}}{{H_{2n + 1}^{{\left( 2 \right)^{^{\prime}} }} \left( {ka} \right)}}\sin \left[ {\left( {2n + 1)\theta } \right)} \right],}$$
(9)
$$u_{1} \left( {r,\theta } \right) = u_{{\text{f}}} \left( {r,\theta } \right) + u_{{{\text{s0}}}} \left( {r,\theta } \right) + u_{{{\text{s1}}}} \left( {r,\theta } \right),$$
(10)
$$\begin{aligned} u_{2} \left( {r,\theta } \right) = & \sum\nolimits_{n = 0}^{\infty } {\frac{{C_{n} }}{{J_{nv}^{^{\prime}} \left( {k\check{a} } \right)}}\sum\nolimits_{m = - \infty }^{\infty } {J_{nv + m} \left( {kr} \right)T_{n,m}^{{\text{C}}} \cos \left[ {\left( {nv + m} \right)\theta } \right]} } \\& - \sum\nolimits_{n = 0}^{\infty } {\frac{{C_{n} }}{{J_{nv}^{^{\prime}} \left( {k\check{a} } \right)}}\sum\nolimits_{m = - \infty }^{\infty } {J_{nv + m} \left( {kr} \right)T_{n,m}^{{\text{S}}} \sin \left[ {\left( {nv + m} \right)\theta } \right],} } \\ \end{aligned}$$
(11)
where \(J_{n} \left( \cdot \right)\) and \(H_{n}^{\left( 2 \right)} \left( \cdot \right)\) denotes the nth-order Bessel function of the first kind and Hankel function of the second kind, respectively; \(J_{n}^{^{\prime}} \left( \cdot \right)\) and \(H_{n}^{{\left( 2 \right)^{^{\prime}} }} \left( \cdot \right)\) denote the derivatives of \(J_{n} \left( \cdot \right)\) and \(H_{n}^{\left( 2 \right)} \left( \cdot \right)\), respectively; n and m are the truncation number of wave function expansion method, and \(\check{a}= a - r_{\text{e}}\); \(T_{n,m}^{{\text{C}}} = {J}_{m} \left( {kr_{{\text{e}}} } \right){\text{cos}}\left[ {m\theta_{\text{e}} - nv\beta_{1} } \right]\) and \({T}_{n,m}^{{\text{S}}} = {J}_{m} \left( {kr_{{\text{e}}} } \right){\text{cos}}\left[ {m\theta_{{\text{e}}} - nv\beta_{1} } \right]\), respectively [42]; \(A_{n}\), \(B_{n}\) and \(C_{n}\) are undetermined coefficients; \(v = \uppi /\left( {\beta_{1} + \beta_{2} } \right)\); \(u_{{{\text{s0}}}} \left( {r,\theta } \right) \,{\text{and}}\, u_{{{\text{s1}}}} \left( {r,\theta } \right)\) are the displacements of scattering site in region ①. Based on Eqs. (10) and (11), the displacement of each point in the region can be obtained.
Ground motion generation of V-shaped canyon
To obtain the topographic magnification in the time domain at each pier position, the following steps are needed: Firstly, the input Fourier spectrum of the incident seismic acceleration time history can be obtained using the fast Fourier transform technique (FFT). Afterward, the corresponding Fourier spectrum of the input acceleration time history should be multiplied by the transfer functions (Eqs. 10 and 11) to obtain the response Fourier spectrum at each pier position. Finally, through the inverse fast Fourier transform (IFFT), the earthquake response in the time domain at each pier position can be obtained accordingly.
To compare the spatial variability of ground motions in the V-shaped site, an analytical solution model of the horizontal site (no topography) was established. According to Eqs. (10) and (11), the magnification of the topography of the horizontal site at each pier position is 2. Then take the selected ground motion in Sect. 3.1 as input. To clarify the influence of the V-shaped canyon topography effect, the seismic incidence angle of this article is determined to be 60°, and the influence of other incident angles will be discussed in future research.
Take record 4 as an example, the magnifications of the V canyon site at different bridge sites relative to the horizontal site are obtained as shown in Table 4 and Fig. 5. Compared with the horizontal site case, after considering the V-shaped canyon effect, the magnification of ground motion on the seismic wave incident side (A1-P4 on the left side of the canyon) is significantly greater than that on the back wave side (P5-A2 on the right side of the canyon).
Table 4 Ratio of the peak acceleration at each pier bottom in the V-shaped site to that of the horizontal site (record 4) The comparison of the Fourier acceleration amplitude of the V-shaped site and the horizontal site under record 4 is shown in Fig. 6. There is a certain difference in the Fourier acceleration amplitude of the V-shaped canyon site and the horizontal site. Under the V-shaped site, the Fourier acceleration amplitudes of the adjacent bridge piers are quite different, which reveals that the V-shaped canyon topography can induce the spatial variability of ground motions.
The acceleration time histories of the V-shaped site and the horizontal site under record 4 are compared in Fig. 7. It can be seen that there are obvious differences in the acceleration time history curves. Especially for the P5 and A2, the PGA of the horizontal site is significantly larger than that of the V-shaped site.