Startseite Naturwissenschaften Numerical Investigation of Electromagnetic Scattering Problems Based on the Compactly Supported Radial Basis Functions
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Numerical Investigation of Electromagnetic Scattering Problems Based on the Compactly Supported Radial Basis Functions

  • Hadi Roohani Ghehsareh EMAIL logo , Seyed Kamal Etesami und Maryam Hajisadeghi Esfahani
Veröffentlicht/Copyright: 10. Juni 2016

Abstract

In the current work, the electromagnetic (EM) scattering from infinite perfectly conducting cylinders with arbitrary cross sections in both transverse magnetic (TM) and transverse electric (TE) modes is numerically investigated. The problems of TE and TM EM scattering can be mathematically modelled via the magnetic field integral equation (MFIE) and the electric field integral equation (EFIE), respectively. An efficient technique is performed to approximate the solution of these surface integral equations. In the proposed numerical method, compactly supported radial basis functions (RBFs) are employed as the basis functions. The radial and compactly supported properties of these basis functions substantially reduce the computational cost and improve the efficiency of the method. To show the accuracy of the proposed technique, it has been applied to solve three interesting test problems. Moreover, the method is well used to compute the electric current density and also the radar cross section (RCS) for some practical scatterers with different cross section geometries. The reported numerical results through the tables and figures demonstrate the efficiency and accuracy of the proposed technique.

1 Introduction

In recent years, the interest in electromagnetic (EM) scattering problems has increased due to their many practical applications in numerous fields of science and engineering such as optics, acoustics, geoscience, and remote sensing. These practical applications led to theoretical investigation of the EM scattering problems. Many of the wave scattering phenomena can be modelled as surface integral equations [1], [2], [3]. The most commonly used surface integral equations are electric field integral equations (EFIEs), magnetic field integral equations (MFIEs), combined field integral equation (CFIE), PMCHWT formulation, and Müller’s integral equation. The EFIE and MFIE formulations are commonly adopted to model scattering from perfectly conducting surfaces [4], [5]. The CFIE, which is a linear combination of EFIE and MFIE, is introduced and formulated to investigate the scattering problem from finite perfectly conducting surfaces [6]. Moreover, the PMCHWT and Müller’s integral formulations are linear combinations of EFIE and MFIE, which are used for analysing the scattering problem from dielectric and composite surfaces [7], [8]. So, to deal with an EM scattering problem, it needs to compute the solution of a proper surface integral equation. In many cases, these surface integral equations are ill-posed and finding the analytic solutions for them is often impossible or very difficult. Consequently, a proper numerical technique should be employed for dealing with these problems. One of the most efficient and powerful numerical methods for solving the surface integral equations is the method of moments (MoM). This method is widely used for solving several types of the EM scattering problems. The efficiency and accuracy of this method have been demonstrated in many reports [2], [3], [5], [9], [10]. In recent years, many numerical techniques such as the mixed-domain Galerkin expansion method [11], the wavelets collocation method [12], [13], the characteristic basis functions method [14], the singular integral equation approach [15], spectral methods based on the block pulse functions [16], [17], etc. have been introduced and improved for solving different types of wave scattering problems.

Nowadays, a new class of developed and advanced computational methods based on the radial basis functions (RBFs) [18], [19], [20], has been introduced and successfully employed for solving several types of practical mathematical models arising from engineering and applied sciences [21], [22], [23], [24], [25], [26], [27], [28], [29], [30], [31], [32], [33], [34], [35]. The RBF’s meshless techniques are very powerful and flexible computational tools for dealing with complicated practical models such as models with complex geometric domains or high-dimensional problems. The standard RBFs based methods can be categorised into two main classes, the numerical methods based on the globally supported RBFs and the compactly supported RBFs (CSRBFs) (see [21] for more details).

In this paper, a numerical technique based on the CSRBFs will be introduced and formulated to solve the EFIE and MFIE arising from the EM scattering problem from infinite perfectly conducting cylinders with arbitrary cross sections. The organisation of this paper is as follows. Section 2 presents some mathematical modelling of EM scattering from perfectly conducting objects. A brief review of compactly supported RBFs and their applications on evaluation surface integral equations will be explained in Section 3. In Section 4, three test problems and some practical examples of scattering from some infinite perfectly conducting cylinders with arbitrary cross sections will be presented to show the accuracy and applicability of the method.

2 Mathematical Modelling of EM Scattering from Perfectly Conducting Objects

The solution of any scattering problem depends on a knowledge of the current density distribution on the surface of the scatterer. Once it is known, then the scattered field can be found using the standard radiation integrals. In scattering problems, the current density is an unknown quantity. Therefore, solving the scattering problems involves two steps:

  1. Solving an integral equation for unknown current J created by a known incident field Einc or Hinc.

  2. Integrating the induced currents J to obtain the scattered field Escat and Hscat.

In this section, we will formulate the well-known electric and MFIEs of scattering from infinite perfectly conducting objects. There is not any reflected wave from the ends of an infinitely long object, so the current does not change along the length and the problem, therefore, becomes two dimensional. For more details on this section, the interested reader can see [1], [3], [5].

Figure 1 shows a two-dimensional scatterer of arbitrary cross section with contour C in both transverse magnetic (TM) and transverse electric (TE) modes.

Figure 1: Geometry for two-dimensional scatterer of arbitrary cross section. (a) TM polarisation. (b) TE polarisation.
Figure 1:

Geometry for two-dimensional scatterer of arbitrary cross section. (a) TM polarisation. (b) TE polarisation.

2.1 Two-dimensional EFIE

In general, a time-harmonic EM field satisfies the Maxwell equations

(1)×E=jωμH, (1)
(2)×H=jωεE+J, (2)

where E and H are the electric and magnetic fields intensity, respectively. ω is the angular frequency, ε and μ are the permittivity and permeability of the medium, respectively, and J is the surface electric current density. Moreover, ∇× denotes the curl operator. Let us assume the incident wave is a plane TM wave with Hz=0,E=z^Ez(x,y) propagating in the xy-plane on the direction k=x^kx+y^ky=k(x^cosθi+y^sinθi), where k=ωμε=2πλ is the wave number (λ=wavelength) and θi is the incident angle. Therefore, the incident field may be specified as

(3)Ezinc=ejk.r=ejk(xcosθi+ysinθi), (3)

where r=(x, y).

The induced current Jz and the scattered field Ezscat produced by it, are related by the scalar wave equation

(4)2Ezscat+k2Ezscat=jωμ0Jz. (4)

The Green’s function solution for (4) may be expressed as

(5)Ezscat(ρ)=kη04CJz(ρ)H0(2)(kρρ)dc, (5)

where ρ=(x, y) is the observation point, ρ′=(x′, y′) is the source point on the contour of cylinder, ρρ=(xx)2+(yy)2 denotes the distance between ρ and ρ′ in R2, H0(2) is the Hankel function of the second kind and zero order, and η0≈377 Ω is the free space impedance. Because the current inside a perfect conductor is zero, the integration is over the contour of the cylinder.

To obtain the EFIE, we have to apply the boundary condition that the total tangential electric field vanishes on the conductor surface, that is

(6)Etinc+Etscat=0   ontheconductorsurface, (6)

where the index t in Etinc and Etscat indicates the tangential component of incident and scattered electric field, respectively.

According to the boundary condition (6) and (5), the two-dimensional EFIE has the following form for TM polarisation:

(7)Ezinc(ρ)=kη04CJz(ρ)H0(2)(kρρ)dc,   ρC, (7)

where Ezinc(ρ) is known and Jz is the unknown quantity to be determined. For a two-dimensional scatterer, the RCS is defined as

(8)σTM(θ)=limρ2πρ|EzscatEzinc|2, (8)

and using (5), it can be expressed as

(9)σTM(θ)=kη024|CJz(x,y)ejk(xcos(θ)+ysin(θ))dc|2. (9)

where σTM is the bistatic RCS for TM polarisation, (x′, y′) are the Cartesian coordinates of source points, and 0≤θ≤2π.

2.2 Two-Dimensional MFIE

A two-dimensional TE field in isotropic media has no z component of E and only has a z component of H. The most convenient general expression for the magnetic field is in terms of the magnetic vector potential A as

(10)H=1μ×A, (10)

where A is satisfied in the Helmholtz equation

(11)2A+k2A=μJ, (11)

and its solution is of the form

(12)A(ρ)=μ4jCJc(ρ)H0(2)(kρρ)dc, (12)

where the integration is over the cross section C of the cylinder. Now, we want to determine the current on the cylinder and the field produced by this current. This problem can be solved by enforcing the boundary conditions on the magnetic field on the surface of the conducting object as

(13)Jc(ρ)=n^×[Hinc(ρ)+Hscat(ρ)]. (13)

After several steps of mathematical operations, the two-dimensional MFIE can be concluded as follows:

(14)Hzinc(ρ)=Jc(ρ)2+jk4CΔCJc(ρ)[n^.R^]H1(2)(kρρ)dc,ρC, (14)

where n^ is an outer unit vector at source point ρ′ normal to the surface of scatterer, H1(2) is the Hankel function of the second kind of the first order, ΔC is that part of the scatterer perimeter which includes ρ, R^=ρρρρ and Hzinc is the incident magnetic field defined as:

(15)Hzinc(ρ)=1η0ejk(xcosθi+ysinθi). (15)

Equation (14) is an MFIE for TE polarisation that is valid just for closed surfaces in which Jc(ρ′) is unknown to be determined.

In the TE case, the two-dimensional bistatic RCS can be obtained by

(16)σTE(θ)=limρ2πρ|HzscatHzinc|2, (16)

or

(17)σTE(θ)=kη024|CJz(x,y)[n^.R^]ejk(xcos(θ)+ysin(θ))dc|2, (17)

where (x′, y′) are the Cartesian coordinates of source point, and 0≤θ≤2π.

3 Surface Integral Equations Evaluation

As observed in the previous section, the wave scattering problems from the perfectly conducting surfaces have been modelled by linear Fredholm integral equations. So, to analyse the scattering from the infinite conducting cylindrical objects in TM or TE modes, a linear Fredholm integral equations of the first kind (EFIE) (7) or a linear Fredholm integral equations of the second kind (MFIE) (14) should be solved, respectively. Note that the kernels of these surface integral equations are singular, and moreover, the first kind of Fredholm integral equations are ill-posed. Thus, most standard and calssical numerical techniques cannot achieve a good accuracy in solving these singular and ill-posed problems. Now, our interest is to formulate and apply an advanced computational method based on the compactly supported radial functions for solving these surface integral equations.

3.1 Compactly Supported RBFs

Here, a brief review of compactly supported radial functions and their interpolation problems will be discussed.

Definition 1. A function Φ:RdR is called radial if there exists a univariate function ϕ:[0, ∞)→R, such that Φ(x)=ϕ(r) where r=∥x∥, and ∥.∥ is the Euclidean norm in Rd.

The RBFs depend only on the distance to a centre point xj and are of the form ϕ(∥xxj∥), so they are very efficient and effective tools for dealing with high-dimensional problems. There are two general families of RBFs: globally and compactly supported radial functions. The globally supported RBFs such as multiquadrics, Gaussian, and thin plate (polyharmonic) splines have been widely used for solving various types of practical models. In all of the numerical methods based on the globally supported RBFs, the resulting coefficient matrices (interpolation or stiffness matrices) are non-sparse and ill-conditioned. For a large number of collocation or interpolation points, this ill-conditioning increases dramatically and leads to instability and loss of numerical accuracy. To overcome these difficulties, the compactly supported RBFs have been introduced and improved [36], [37], [38]. Wendland’s CSRBFs are the most popular family of compactly supported radial functions in use which was constructed by Wendland [37]. A list of the most commonly used Wendland’s CSRBFs (ϕd,k:RdR) is given in Table 1. In this table, (.)+ denotes the cut-off function which is defined by

(18)(x)+={xforx00forx<0, (18)

and ε is a scaling factor, which dictates the compactness of the RBFs support. These functions are radial piecewise polynomial, strictly positive definite functions on Rd, and also ϕd,kC2k. So, they are very suitable basis for solving large-scale problems.

Table 1:

Wendland’s CSRBFs ϕd,k for various choices of k and l=d2+k+1.

kφd,k
0(1ϵr)+l
1(1ϵr)+l+1[(l+1)ϵr+1]
2(1ϵr)+l+2[(l2+4l+3)(ϵr)2+(3l+6)ϵr+3]
3(1ϵr)+l+3[(l3+9l2+23l+15)(ϵr)3+(6l2+36l+45)(ϵr)2+(15l+45)ϵr+15]

Now, we use the CSRBFs to interpolate the scattered data. Let, x1, x2, …, xN be a given set of distinct points in Rd. Assume that we want to interpolate the given values fi=f(xi)i=1, …, N. We now use the CSRBFs expansion to solve this interpolation problem by assuming

(19)𝒫f(x)=j=1Nλjϕ(xxj)   xRd, (19)

where the unknown coefficients λj are found by enforcing the interpolation conditions 𝒫f(xi)=f(xi) i=1, …, N and thus solving the linear system

(20)Aλ=f, (20)

where

λ=[λ1,,λN]T   f=[f1,,fN]T,

and the elements of the interpolation matrix A are given by

Aij=ϕ(xixj),i,j=1,,N.

By scaling the support of the basic function appropriately, the interpolation matrix A will be a sparse matrix, and therefore, the stability of the interpolation problem will be guaranteed.

In the following, a numerical procedure based on the CSRBFs will be formulated to obtain the approximate solutions of linear Fredholm integral equations.

3.2 EFIE Evaluation

Here, we recall the following EFIE (7)

Ezinc(ρ)=kη04CJz(ρ)H0(2)(kρρ)dc.

Now, the unknown current function Jz(ρ′) is approximated using a linear combination of CSRBFs as

(21)Jz(ρ)=j=1Nλjϕ(rj), (21)

where ϕ(.) is a proper compactly supported radial function and rj=∥ρ′–ρj∥ denotes the Euclidean distance between ρ′ and ρj. ρj, j=1, …, N are centre points on the perimeter of cross-section C. Moreover, {λj}j=1N is a set of N unknown coefficients to be determined. Substituting (21) in EFIE (7) gives

kη04CH0(2)(kρρ)(j=1Nλjϕ(ρρj))dc=Ezinc(ρ),

and therefore,

(22)j=1Nλj(CH0(2)(kρρ)ϕ(ρρj)dc)=4kη0Ezinc(ρ). (22)

In the following, the perimeter of cross section, C, is discretised into N straight boundary elements Ci, i=1, …, N, and the collocation points ρ˜i are chosen as the centre of Ci, see Figure 2. Now, a point matching scheme can be implemented by satisfying (22) at collocation points ρ˜i,i=1,,N, as

Figure 2: Descretisation the perimeter of cross section C.
Figure 2:

Descretisation the perimeter of cross section C.

(23)j=1Nλj(CH0(2)(kρ˜iρ)ϕ(ρρj)dc)=4kη0Ezinc(ρ˜i),i=1,2,,N. (23)

Using the compact support property of the selected trial functions, the above equations can be reduced to the following:

(24)j=1Nλj(SjH0(2)(kρ˜iρ)ϕ(ρρj)dc)=4kη0Ezinc(ρ˜i),i=1,2,,N, (24)

where according to the definition of Wendland’s CSRBFs, Sj={ρC:ρρj1ϵ}C, denotes the support of trial function ϕ(rj). The accuracy and the stability of the process is highly dependent on the scaling parameter ε. The optimal value for the scaling parameter can be found by the Contour-Pade algorithm [21].

Clearly, (24) is an N×N linear system of equations, which can be presented as follows:

(25)Ξλ=4kη0Ei, (25)

where

λ=[λ1,λ2,,λN]T,   Ei=[Ezinc(ρ˜1),Ezinc(ρ˜2),,Ezinc(ρ˜N)]T,

also the elements of the square matrix Ξ are given by

(26)Ξij=SjH0(2)(kρ˜iρ)ϕ(ρρj)dc,   i,j=1,,N. (26)

Now, the unknown coefficient vector λ can be obtained by solving the linear system of equation (25).

In the practical implementation of the method the boundary integral, (26) should be evaluated numerically. For this purpose, the boundary integral (26) is presented as follows:

(27)SjH0(2)(kρ˜iρ)ϕ(ρρj)dc=p=1Nj(CpH0(2)(kρ˜iρ)ϕ(ρρj)dc), (27)

where Sj=p=1NjCp. Now, for computing the above boundary integral, when the collocation point ρ˜i is not on Cp, a simple centroid formulation is employed to evaluate the boundary integrals, which is

(28)CpH0(2)(kρ˜iρ)ϕ(ρρj)dc=|Cp|H0(2)(kρ˜iρ˜p)ϕ(ρ˜pρj), (28)

where ρ˜p is the centre of Cp. When the collocation point ρ˜i belongs to the segment Cp, then the Hankel function in the boundary integral is a singular kernel and so, it requires a special treatment (note that the boundary integral is convergent). Several numerical and analytical procedures have been introduced in the literature to deal with this singular boundary integral. In particular, an efficient numerical approach based on the sinh transformation has been introduced and formulated by Elliot and Johnson for solving nearly weakly singular integrals with Hankel kernels [39]. This technique is employed for dealing with some scattering problems [40], [41]. As an alternative procedure, it is clear that for small argument ρ, the expansion of the Hankel function is as follows:

(29)H0(2)(ρ)=1j2πlnγρ2+O(ρ2,ρ2lnρ),   ρ0, (29)

where γ=1.781 is Euler’s constant. So, by substituting the relation (29) in the singular boundary integral, we have

(30)CpH0(2)(kρ˜iρ)ϕ(ρρj)dcCp(1j2πlnkγρ˜iρ2)ϕ(ρρj)dc,=Cpϕ(ρρj)dcj2πCplnkγρ˜iρ2ϕ(ρρj)dc. (30)

In our implementation, the first above boundary integral is calculated exactly and the singular integral with logarithmic kernel is evaluated according to [42].

3.3 MFIE Evaluation

Consider the following second-kind Fredholm MFIE (14):

Hzinc(ρ)=Jc(ρ)2+jk4CΔCJc(ρ)[n^.R^]H1(2)(kρρ)dc.

We expand Jc(ρ) with respect to CSRBFs as

(31)Jz(ρ)=j=1Nλjϕ(ρρj). (31)

Here, the centre and collocation points are considered the same as previous section. Substituting (31) in (14) and implementing the same point matching procedure gives:

(32)j=1Nλj(12ϕ(ρ˜iρj)+jk4CΔCiϕ(ρρj)[n^.Ri]H1(2)(kρ˜iρ)dc)=Hzinc(ρ˜i),i,j=1,,N, (32)

where ΔCi is that segment of C which includes the collocation point ρ˜i. Therefore, the boundary integral in (32) has no singularity.

By using the compact support property of the selected trial functions, the above equations can be written as follows:

(33)j=1Nλj(12ϕ(ρ˜iρj)+jk4Sjϕ(ρρj)[n^.R^i]H1(2)(kρ˜iρ)dc)=Hzinc(ρ˜i),i,j=1,,N. (33)

Equation (33) is an N×N linear system of equations that can be presented in the matrix form

(34)Ξλ=Hi, (34)

where

λ=[λ1,λ2,,λN]T,   Hi=[Hzinc(ρ˜1),Hzinc(ρ˜2),,Hzinc(ρ˜N)]T,

also the elements of the square matrix Ξ are given by

(35)Ξij=12ϕ(ρ˜iρj)+jk4Sjϕ(ρρj)[n^.R^i]H1(2)(kρ˜iρ)dc,   i,j=1,,N. (35)

The unknown coefficients λj can be derived by solving the system of equations (34). The integral used in (35) has no singularity and may be numerically calculated as follows:

Sjϕ(ρρj)[n^.R^i]H1(2)(kρ˜iρ)dc=p=1Nj|Cp|ϕ(ρ˜pρj)[n^.R^i]H1(2)(kρ˜iρ˜p)

where Sj=p=1NjCp and ρ˜p is the centre of Cp.

4 Results and Discussion

In the current section, some numerical experiments are presented to illustrate the accuracy and efficiency of the presented method. In the first three examples, some test problems that their exact solutions are available have been investigated. The solutions of these problems are approximated with the presented method using CSRBFs and the MOM using the block pulse trial functions, and then, the absolute errors are computed to analyse the convergence and accuracy of the method. Next, some practical scattering problems will be numerically investigated to show efficiency of the method. In fact, the presented method is used for computing the current density and RCS for some infinite perfectly conducting cylinders with square, triangular, and elliptical cross sections.

In all cases, the Wendland’s CSRBF are chosen as trial function and also a proper and optimal value for the scaling factor ε is computed using the Contour-Pade algorithm for each case.

Example 1: Test problem 1

As the first example consider the following linear Fredholm integral equation of the first kind

(36)f(s)=CH0(2)(k|st|)u(t)dt,   C=[a,b]. (36)

The exact solution of the integral equation is [16], [17]

u(t)=t2e2t+jln|t+ba|.

The source function f(s) is extracted from the exact solution and computed numerically using the composite trapezoidal rule. In this case, we let: C=[–0.5, 0.5] and k=2π. We discretise C into N=200 equal segments such that h=baN. Two common Wendland’s CSRBFs in one-dimensional ϕ1,0(r)=(1ϵr)+1 and ϕ1,1(r)=(1ϵr)+3(1+3ϵr) are used as the trial functions. As mentioned before, the Contour-Pade algorithm is applied for determining the optimal shape parameter ε. These optimal values are ϵ=16h for ϕ1,0(r) and ϵ=17.55h for ϕ1,1(r). If we define root mean square error (RMS) as

RMSerror=1Ni=1N[uexact(xi)uapproximate(xi)]2,

in order to confirm Contour-Pade algorithm results, we plot the variations in the RMS-error in respect to ε in Figure 3a and b for ϕ1,0(r) and ϕ1,1(r), respectively, and the optimal values of ε are shown. In Figure 4a and b, the RMS-error as a function of N is plotted. This figure confirms that when N increases, the approximate solution will be converge to exact solution. In Table 2, the absolute error for nine interior points is calculated for both Wendland’s CSRBFs and compared to MOM with N=200 block pulse trial functions. Clearly, all the reported results show the accuracy and efficiency of the presented method.

Figure 3: Optimal ε in the first test problem for N=200 uniformly spaced points based on (a) ϕ1,0, (b) and ϕ1,1.
Figure 3:

Optimal ε in the first test problem for N=200 uniformly spaced points based on (a) ϕ1,0, (b) and ϕ1,1.

Figure 4: RMS-error for the first test problem with (a) ϕ1,0 and (b) ϕ1,1 based on N uniformly spaced points in [–0.5, 0.5] and optimal ε for each N.
Figure 4:

RMS-error for the first test problem with (a) ϕ1,0 and (b) ϕ1,1 based on N uniformly spaced points in [–0.5, 0.5] and optimal ε for each N.

Table 2:

Numerical result for test problem 1.

t|uexact(t) –uappro(t)|(φ1, 0)|uexact(t)–uappro(t)|(φ1,1)|uexact(t)–uappro(t)|(MOM)
–0.44.968e-44.981e-44.668e-3
–0.31.766e-41.525e-43.785e-3
–0.23.507e-43.342e-42.814e-3
–0.13.813e-43.718e-42.416e-3
0.04.049e-44.044e-41.132e-3
0.13.181e-43.219e-42.025e-3
0.21.426e-41.559e-42.403e-3
0.31.111e-40.832e-43.636e-3
0.48.363e-41.520e-45.603e-3

Example 2: Test problem 2

Consider the following second-kind Fredholm integral equation

(37)f(s)=u(s)+CH0(2)(k|st|)u(t)dt   C=[a,b], (37)

with exact solution [16], [17]

u(t)=t2e2t+jln|t+ba|.

The source function f(s) is obtained by inserting the exact solution in (37) using the composite trapezoidal rule. The centre and collocation points, trial functions, and optimal value of ε used in this example are the same as previous example. Table 3 shows the absolute error of the approximate solution obtained by current method for k=2π, a=–b=–0.5, and compare them with the MOM. These results confirm that this method works well and is more accurate than MOM with N=200 block pulse trial functions.

Table 3:

Numerical result for test problem 2.

t|uexact(t) –uappro(t)|(φ1,0)|uexact(t)–uappro(t)|(φ1,1)|uexact(t)–uappro(t)|(MOM)
–0.47.852e-51.209e-44.279e-3
–0.33.403e-55.893e-53.581e-3
–0.21.523e-57.786e-73.150e-3
–0.14.094e-53.169e-52.757e-3
0.05.754e-55.088e-52.463e-3
0.11.851e-52.209e-52.322e-3
0.20.971e-52.251e-52.530e-3
0.33.374e-56.251e-53.485e-3
0.47.392e-51.358e-45.690e-3

Example 3: Test problem 3 (Circular cylinder)

As a practical test problem, suppose that an infinitely perfect conducting circular cylinder of radius a is encountered by a plane wave. Because the circular cylinder has a regular shape, it has been analysed using the method of separation of variables. First assume that the incident wave is a TM plane wave of unit amplitude (E0=1) and zero incident angle. We express it in terms of cylindrical waves as

(38)Ezinc(x,y)=E0ejkx=E0ejkρcosφ. (38)

The analytical solution for surface current density on the perimeter of circular cylinder can be expressed as [1]

(39)Jz(ρ=a,φ)=2E0πaωμ0n=jnejnφHn(2)(ka). (39)

We solve EFIE (7) and MFIE (14) for TM and TE modes, respectively, by the presented method to calculate J. In this case, we consider the radius equal to 2 wavelength, or a=2λ and a two-dimensional Wendland’s CSRBF ϕ2,1=(1ϵr)+4(1+4ϵr) is used as the basis function. The presented technique is employed to approximate the current density by spreading N=300 identical centre and collocation nodes uniformly along the perimeter of cross section C. The shape parameter ε varies in [1], [10], and its optimal value for N=300 is shown in Figure 5a. RMSE is computed for various value of N and plotted in Figure 5b. It confirms the convergence of the approximate solution to the exact solution for large value of N. It should be mentioned that for each N, its optimal shape parameter is considered to calculate the RMSE. To show the validity of this method, EFIE is also solved using MOM ([3]) and absolute error of solution as a function of angle along the perimeter of cylinder is compared to the current method in Figure 6a and b).

Figure 5: Result for EFIE in TM mode; (a) RMS-error vs. shape parameter ε for N=300. (b) RMS-error vs. N.
Figure 5:

Result for EFIE in TM mode; (a) RMS-error vs. shape parameter ε for N=300. (b) RMS-error vs. N.

Figure 6: Absolute error of the current density as a function of angle along the perimeter of the circular cylinder for N=300, k=2π for solution of EFIE in TM mode: (a) by MOM, (b) by presented method.
Figure 6:

Absolute error of the current density as a function of angle along the perimeter of the circular cylinder for N=300, k=2π for solution of EFIE in TM mode: (a) by MOM, (b) by presented method.

Now, let us assume that a TE plane wave is normally incident upon a perfectly conducting circular cylinder of radius a (θi=0). The incident magnetic field can be written as

(40)Hzinc(x,y)=H0ejkx=H0ejkρcosφ,   H0=E0η0. (40)

The current density on the surface of the cylinder can be expressed analytically as [1]:

(41)Jc(ρ=a,φ)=2jH0πkan=jnejnφHn(2)(ka). (41)

Similar to TM mode, MFIE is solved numerically by the method presented in the previous section and the corresponding result of optimal shape parameter and convergency analysis is shown in Figure 7a and b, respectively. A comparison between MOM ([3]) and our method is presented in Figure 8a and b, respectively, in respect to absolute error of current density along the perimeter of cylinder.

Figure 7: Result for MFIE in TE mode: (a) RMS-error vs. shape parameter ε for N=300. (b) RMS-error vs. N.
Figure 7:

Result for MFIE in TE mode: (a) RMS-error vs. shape parameter ε for N=300. (b) RMS-error vs. N.

Figure 8: Absolute error of the current density as a function of angle along the perimeter of the circular cylinder for N=300, k=2π for solution of MFIE in TE mode, (a) by MOM, (b) by presented method.
Figure 8:

Absolute error of the current density as a function of angle along the perimeter of the circular cylinder for N=300, k=2π for solution of MFIE in TE mode, (a) by MOM, (b) by presented method.

This was an interesting test problem to analyse the performance of the method in actual scattering problem. A brief look at the graphs and a comparison between two methods justifies validity, accuracy, and efficiency of the presented method.

Example 4: Square cylinder

In this example, we obtain the current density along a perfectly conducting square cylinder of half-length side a which encountered by a plane wave as shown in Figure 9a. The numerical solution of EFIE (7) and MFIE (14) for a=λ is calculated by the presented method using ϕ2,1 as the basic function and N=296 centre and collocation points. The magnitude of the current density has been shown in Figure 9b. The bistatic RCS is given for TM polarisation in Figure 9c and for TE polarisation in Figure 9d.

Figure 9: (a) Cross section of square cylinder scatterer. (b) Current density magnitude along a perfectly conducting square cylinder for k=2π, a=λ, θi=0, N=296, and ε=5.5 obtained by the presented method for TM and TE polarisations. Its RCS (c) for TM, (d) for TE polarisation.
Figure 9:

(a) Cross section of square cylinder scatterer. (b) Current density magnitude along a perfectly conducting square cylinder for k=2π, a=λ, θi=0, N=296, and ε=5.5 obtained by the presented method for TM and TE polarisations. Its RCS (c) for TM, (d) for TE polarisation.

Example 5: Triangular cylinder

The magnitude of current density along the perimeter of a triangular cylinder of length side a which encountered by a plane wave is numerically calculated by the presented method for a=2λ using ϕ2,1 as the basic function and N=296 centre and collocation points. Figure 10a shows its cross section. The results of solving EFIE (7) and MFIE (14) is plotted in Figure 10b and Figure 10c, respectively. The bistatic RCS pattern is plotted in Figure 10d.

Figure 10: (a) Cross section of triangular cylinder scatterer. (b) Current density magnitude along a perfectly conducting triangular cylinder for k=2π, a=2λ, θi=0, N=296, and ε=5.5 obtained by the presented method for TM polarisations. (c) The result for TE polarisation. (d) Their bistatic RCS for TM and TE polarisation.
Figure 10:

(a) Cross section of triangular cylinder scatterer. (b) Current density magnitude along a perfectly conducting triangular cylinder for k=2π, a=2λ, θi=0, N=296, and ε=5.5 obtained by the presented method for TM polarisations. (c) The result for TE polarisation. (d) Their bistatic RCS for TM and TE polarisation.

Example 6: Elliptical cylinder

In the last example, we obtain the RCS and the magnitude of current density along the perimeter of two perfectly conducting elliptical cylinder which encountered by a plane wave. Figure 11a shows the cross section of an elliptical cylinder. This problem is solved by the presented method using the CSRBF ϕ2,1 and N=300 centre and collocation points. Figure 11b shows the result for a=λ4,b=4a, for both TM and TE polarisations. The bistatic RCS is given for TM in Figure 11c and for TE in Figure 11d.

Figure 11: (a) Cross-section of elliptical cylinder scatterer. (b) Current density magnitude along a perfectly conducting elliptical cylinder for k=2π, a = λ4, b = 4a,$a\, = \,{\lambda  \over 4},{\rm{ }}b\, = \,4a,$θi=0, N=300, and ε=5.5 obtained by the presented method for TM and TE polarisations. Its bistatic RCS (c) for TM, (d) for TE polarisation.
Figure 11:

(a) Cross-section of elliptical cylinder scatterer. (b) Current density magnitude along a perfectly conducting elliptical cylinder for k=2π, a=λ4,b=4a,θi=0, N=300, and ε=5.5 obtained by the presented method for TM and TE polarisations. Its bistatic RCS (c) for TM, (d) for TE polarisation.

Figure 12a shows the current density along the perimeter of another elliptical cylinder for a=λ,b=a4 for both TM and TE polarisations. The bistatic RCS is given for TM and TE polarisations in Figure 12b. These figures can be compared with figures in [5].

Figure 12: (a) Current density magnitude along a perfectly conducting elliptical cylinder for k=2π, a = λ,b = a4,$a\, = \,\lambda , b\, = \,{a \over 4},$θi=0, N= 300, and ε=5.5 obtained by presented method for TM and TE polarisations. (b) Their RCS for both TM and TE polarisations.
Figure 12:

(a) Current density magnitude along a perfectly conducting elliptical cylinder for k=2π, a=λ,b=a4,θi=0, N= 300, and ε=5.5 obtained by presented method for TM and TE polarisations. (b) Their RCS for both TM and TE polarisations.

5 Conclusion

The EM scattering from infinite perfectly conducting cylinders with arbitrary cross sections has been modelled mathematically. The EFIE and MFIE for TM and TE modes, respectively, have been derived. The efficient meshless technique based on CSRBFs has been applied to approximate the solution of these surface integrals. The compactly supported and radial property of CSRBFs reduce the computational cost and improve the efficiency of the method. The accuracy, robustness, and efficiency of the method have been tested and validated through two test problems that their exact solutions are available. This method is also well used to compute the RCS and the electric current density on the perimeter of infinite perfectly conducting cylinders with different cross sections. In the case of circular cylinder, the analytical solution exists and the comparison between the analytical and numerical solutions shows a good agreement and confirms the accuracy and validity of the method.

Acknowledgments:

The authors are grateful to the anonymous reviewer for his/her valuable comments and suggestions which helped to improve this paper.

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Received: 2016-2-24
Accepted: 2016-5-10
Published Online: 2016-6-10
Published in Print: 2016-8-1

©2016 Walter de Gruyter GmbH, Berlin/Boston

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