Abstract

The electromagnetic field in homogeneous plasma anisotropic medium can be expressed as the addition of the first and second spherical vector wave functions in plasma anisotropic medium. The tangential electromagnetic fields are continued in the boundary between the homogeneous plasma anisotropic medium and free space, and the tangential electrical field is zero in the surface of conducting sphere. The coefficients of electromagnetic fields in plasma anisotropic medium expanded in terms of spherical vector wave functions in plasma anisotropic medium are derived, and then the coefficients of scattering fields in terms of spherical vector functions in free space can be obtained. Numerical results between this paper and hybrid finite element-boundary integral-multilevel fast multipole algorithm (FE-BI-MLFMA) are given, and they are in agreement very well. Some new numerical results of a plane wave scattering by an anisotropic plasma-coated conducting sphere are obtained.

1. Introduction

Plasma represents a medium of gas in highly ionized state, and it is a neutral mixture of free ions, electrons, and molecules. For example, when the ionosphere and the sheath of satellite and missile come into atmosphere, they are considered to be plasma in nature. When there is an externally applied magnetic field, a plasma exhibits anisotropic behavior and its permittivity takes a tensor form. The elements of the permittivity tensor are complex functions of wave, plasma, gyro and collision frequencies [13]. Wave propagation in, and scattering by, an anisotropic medium is nonreciprocal, and its analysis becomes very difficult even when the plasma is treated as an incompressible gas [14].

The interaction between electromagnetic wave and anisotropic medium has attracted much interest. It is simply because there are many natural and artificial anisotropic materials, and they are frequently used in optical signal processing (such as constructing signal processing elements at optical frequencies), the radar cross-section control for various objects or scatterers, antennas or airborne radomes, optical fibers, developments of certain types of radar absorbers, and high-performance microstrip antenna designs where the substrates of this nature are desirable.

One of the basic problems in investigating waves in anisotropic media is to accurately and efficiently characterize electromagnetic scattering. Scattering by homogeneous anisotropic objects has attracted considerable interests in recent years. Numerical methods based on integral equations [5] as well as differential equations [6] were developed, and the analytical method based on eigen vector wave functions [7] was also adopted to characterize this kind of problems. Although the efforts in the past were primarily spent on two-dimensional (2-D) geometries, some progresses have been made in the analysis of three-dimensional (3-D) anisotropic scatterers using the method of moments (MoM) [8, 9], the couple dipole approximation method [10], hybrid finite element-boundary integral-multilevel fast multipole algorithm (FE-BI-MLFMA) [11], integral equation method [12], and Fourier transform, eigenvalue and eigen functions, spherical vector wave functions solution [1315]. In the present study, the simple and efficient method proposed in [13] will be employed to tackle the scattering problem associated with an anisotropic plasma-coated conducting sphere by a plane wave.

Electromagnetic fields in plasma anisotropic medium and free space can be expanded in terms of spherical vector wave functions in plasma anisotropic medium and free space, respectively. Applying the continued boundary conditions of electromagnetic fields on the interfaces between the free space and a coated-plasma anisotropic medium, and the vanishing of the tangential field in the surface of the conducting sphere, the coefficients of electromagnetic fields in plasma anisotropic medium and scattered fields in free space can be obtained. Then, radar cross-sections of an anisotropic plasma-coated conducting sphere scattered by a plane wave can be derived. The theoretical analysis shows that the present method can be reduced to these of the homogeneous plasma anisotropic medium when the radius of conducting sphere approaches zero. This analytical solution to electromagnetic scattering by an anisotropic plasma-coated conducting sphere can be used to characterize the targets and their radar cross-sections and also to understand wireless communication channels and radio wave propagation mechanisms.

2. Formulation of the Problem

Consider the geometry depicted in Figure 1 which shows a cross-section of an anisotropic plasma-coated conducting sphere where the outer and inner radii of the plasma anisotropic medium are 𝑎1 and 𝑎2, respectively. Three distinct regions are thus divided into, namely, region 0 for the free space, region 1 for the plasma anisotropic spherical shell, and region 2 for the conducting sphere. This composite structure is illuminated by a plane electromagnetic wave (which is assumed to have an electric field amplitude equal to unity, to be polarized in parallel to the 𝑥-direction, and to propagate in the 𝑧-direction). In the following analysis, a time dependence of exp(𝑖𝜔𝑡) is assumed for the electromagnetic field quantities, but is suppressed throughout the treatment.

The electric field vector wave equation in such a source-free plasma anisotropic medium can be written in the following form [7, 1215]: ××𝐄𝜔2𝜇0𝝐𝐄=0,(1) where 𝐄 denotes the electric field, while 𝜇0 represents the free-space permeability, and 𝝐 identifies the permittivity tensor of the plasma anisotropic medium. If an external constant magnetic filed is applied in the +𝑧-direction, the permittivity tensor 𝝐 takes the form [14, 13, 14] of 𝜖𝜖=1𝜖20𝜖2𝜖1000𝜖3.(2) Using the Fourier transform as in [7, 1215], the expansion of plane wave factors in terms of spherical vector wave functions of the first kind in isotropic medium [16] and the other three (the second, third, and fourth) kinds of spherical Bessel functions satisfying the same differential equations and the recursive relations of the first spherical Bessel functions, the electromagnetic fields (designated by the subscript 1) in the homogeneous plasma anisotropic spherical medium (region 1) can be obtained as follows: 𝐄1=22𝑙=1𝑞=1𝑚𝑛𝑛𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐴𝑒𝑚𝑛𝑞𝜃𝑘𝐌(𝑙)𝑚𝑛𝐫,𝑘𝑞+𝐵𝑒𝑚𝑛𝑞𝜃𝑘𝐍(𝑙)𝑚𝑛𝐫,𝑘𝑞+𝐶𝑒𝑚𝑛𝑞𝜃𝑘𝐋(𝑙)𝑚𝑛𝐫,𝑘𝑞×𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘,𝐇(3a)1=22𝑙=1𝑞=1𝑚𝑛𝑛𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐴𝑚𝑛𝑞𝜃𝑘𝐌(𝑙)𝑚𝑛𝐫,𝑘𝑞+𝐵𝑚𝑛𝑞𝜃𝑘𝐍(𝑙)𝑚𝑛𝐫,𝑘𝑞+𝐶𝑚𝑛𝑞𝜃𝑘𝐋(𝑙)𝑚𝑛𝐫,𝑘𝑞×𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘,(3b)where 𝑛 and 𝑛 are summed up both from 0 to + while 𝑚 is summed up from 𝑛 to 𝑛; 𝐫 denotes a position vector in the spherical coordinates; the coefficients, 𝐹(𝑙)𝑚𝑛𝑞, are unknown to be determined using the boundary conditions as in [13, 14]; finally expansion coefficient 𝐴𝑝𝑚𝑛𝑞(𝜃𝑘), 𝐵𝑝𝑚𝑛𝑞(𝜃𝑘), 𝐶𝑝𝑚𝑛𝑞(𝜃𝑘) (where 𝑝=𝑒 or ) and the eigenvalues of the coated plasma anisotropic medium 𝑘𝑞(𝑞=1,2) are all functions of 𝜃𝑘 and they have been derived in [13]. The vectors, 𝐌(𝑙)𝑚𝑛, 𝐍(𝑙)𝑚𝑛, and 𝐋(𝑙)𝑚𝑛, denote spherical vector wave functions in isotropic medium and they are defined as follows [1316]: 𝐌(𝑙)𝑚𝑛=𝑧𝑛(𝑙)𝑃(𝑘𝑟)𝑖𝑚𝑚𝑛(cos𝜃)sin𝜃𝜽𝑑𝑃𝑚𝑛(cos𝜃)𝝓𝑒𝑑𝜃𝑖𝑚𝜙𝐍,(4a)(𝑙)𝑚𝑛𝑧=𝑛(𝑛+1)𝑛(𝑙)(𝑘𝑟)𝑃𝑘𝑟𝑚𝑛(cos𝜃)𝑒𝑖𝑚𝜙̂𝐫+1𝑑𝑘𝑟𝑟𝑧𝑛(𝑙)(𝑘𝑟)𝑑𝑟𝑑𝑃𝑚𝑛(cos𝜃)𝑃𝑑𝜃𝜽+𝑖𝑚𝑚𝑛(cos𝜃)𝝓𝑒sin𝜃𝑖𝑚𝜙,𝐋(4b)(𝑙)𝑚𝑛=𝑘𝑑𝑧𝑛(𝑙)(𝑘𝑟)𝑃𝑑(𝑘𝑟)𝑚𝑛(̂𝑧cos𝜃)𝐫+𝑛(𝑙)(𝑘𝑟)×𝑘𝑟𝑑𝑃𝑚𝑛(cos𝜃)𝑃𝑑𝜃𝜽+𝑖𝑚𝑚𝑛(cos𝜃)𝝓𝑒sin𝜃𝑖𝑚𝜙,(4c)where 𝑧𝑛(𝑙)(𝑥) (with 𝑙=1, 2, 3, and 4) denotes an appropriate kind of spherical Bessel functions, 𝑗𝑛(𝑥), 𝑦𝑛(𝑥), 𝑛(1)(𝑥), and 𝑛(2)(𝑥), respectively.

Equation (3) are the spherical vector wave functions in plasma anisotropic medium, which is different to that in isotropic medium which are shown in (4a) and (4b),(i)first, spherical vector wave functions in plasma anisotropic medium is an integral expression comparing to that in isotropic medium, and(ii)second, the eigenvalues (𝑘𝑞) in plasma anisotropic medium have two different values, but the wave number in isotropic medium is one (𝑘).

The spherical vector wave functions in plasma anisotropic medium is more complex than that in isotropic medium, and electromagetic fields in plasma anisotropic medium can be expressed by that in anisotropic medium.

To characterize the scattering properties of the plasma-coated conducting sphere, the incidence wave (designated by the superscript inc) and the scattered wave (designated by the superscript 𝑠) can be expressed in free space in terms of spherical vector wave functions as follows [1316]:𝐄𝑖𝑛𝑐=𝑚𝑛𝛿𝑚,1+𝛿𝑚,1×𝑎𝑥𝑚𝑛𝐌(1)𝑚𝑛𝐫,𝑘0+𝑏𝑥𝑚𝑛𝐍(1)𝑚𝑛𝐫,𝑘0,𝐇(5a)𝑖𝑛𝑐=𝑘0𝑖𝜔𝜇0𝑚𝑛𝛿𝑚,1+𝛿𝑚,1×𝑎𝑥𝑚𝑛𝐍(1)𝑚𝑛𝐫,𝑘0+𝑏𝑥𝑚𝑛𝐌(1)𝑚𝑛𝐫,𝑘0,(5b)𝐄𝑠=𝑚𝑛𝐴𝑠𝑚𝑛𝐌(3)𝑚𝑛𝐫,𝑘0+𝐵𝑠𝑚𝑛𝐍(3)𝑚𝑛𝐫,𝑘0,𝐇(6a)𝑠=𝑘0𝑖𝜔𝜇0𝑚𝑛𝐴𝑠𝑚𝑛𝐍(3)𝑚𝑛𝐫,𝑘0+𝐵𝑠𝑚𝑛𝐌(3)𝑚𝑛𝐫,𝑘0,(6b)where 𝑘0 denotes the wave number in free space, and the expansion coefficients of incident wave 𝑎𝑥𝑚𝑛, 𝑏𝑥𝑚𝑛, and 𝛿𝑚𝑛 have been obtained earlier in [1315] and are defined by 𝑎𝑥𝑚𝑛=𝑖𝑛+12𝑛+1𝑖2𝑛(𝑛+1),𝑚=1,𝑛+12𝑛+12𝑏,𝑚=1,(7a)𝑥𝑚𝑛=𝑖𝑛+12𝑛+12𝑛(𝑛+1),𝑚=1,𝑖𝑛+12𝑛+12𝛿,𝑚=1,(7b)𝑠,𝑙=1,𝑠=𝑙,0,𝑠𝑙.(7c)The expansion coefficients of scattered fields, 𝐴𝑠𝑚𝑛 and 𝐵𝑠𝑚𝑛 in (6a) and (6b) (𝑛 varies from 0 to + while 𝑚 changes from 𝑛 to 𝑛), are unknown to be determined using the boundary conditions, together with the unknown coefficients 𝐹(𝑙)𝑚𝑛𝑞(where 𝑙=1,2 and 𝑞=1,2) in (3).

From (3), it shows that when the radius 𝑎2 of the conductor sphere is infinitely small, the electromagnetic fields in the coating plasma anisotropic spherical shell origin are still finite, but the value of the second spherical Bessel functions becomes infinitely large in the origin; therefore the expansion coefficients 𝐹(2)𝑚𝑛𝑞 of spherical vector wave functions in (3) will vanish, and in this connection, the present method in this paper can be automatically reduced to a homogeneous plasma anisotropic sphere, which is the same as that in [13].

By applying continuous boundary conditions of tangential electromagnetic field components on the interface between the plasma anisotropic medium and free space (where 𝑟=𝑎1) and utilizing the orthogonality of the tangential spherical vector wave functions [13], the following expressions are obtained:22𝑙=1𝑞=1𝑛=0𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐴𝑒𝑚𝑛𝑞𝑧𝑛(𝑙)𝑘𝑞𝑎1𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘=𝛿𝑚,1+𝛿𝑚,1𝑎𝑥𝑚𝑛𝑗𝑛𝑘0𝑎1+𝐴𝑠𝑚𝑛𝑛(1)𝑘0𝑎1,(8a)22𝑙=1𝑞=1𝑛=0𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐵𝑒𝑚𝑛𝑞𝑅𝑛(𝑙)𝑘𝑞𝑟+𝐶𝑒𝑚𝑛𝑞𝑧𝑛(𝑙)𝑘𝑞𝑟𝑟𝑟=𝑎1×𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘=𝛿𝑚,1+𝛿𝑚,1𝑏𝑥𝑚𝑛𝑅𝑛(1)𝑘0𝑎1+𝐵𝑠𝑚𝑛𝑅𝑛(3)𝑘0𝑎1,(8b)22𝑙=1𝑞=1𝑛=0𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐴𝑚𝑛𝑞𝑧𝑛(𝑙)𝑘𝑞𝑎1𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘=𝑘0𝑖𝜔𝜇0𝛿𝑚,1+𝛿𝑚,1𝑏𝑥𝑚𝑛𝑗𝑛𝑘0𝑎1+𝐵𝑠𝑚𝑛𝑛(1)𝑘0𝑎1,(8c)22𝑙=1𝑞=1𝑛=0𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐵𝑚𝑛𝑞𝑅𝑛(𝑙)𝑘𝑞𝑟+𝐶𝑚𝑛𝑞𝑧𝑛(𝑙)𝑘𝑞𝑟𝑟𝑟=𝑎1×𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘=𝑘0𝑖𝜔𝜇0𝛿𝑚,1+𝛿𝑚,1𝑎𝑥𝑚𝑛𝑅𝑛(1)𝑘0𝑎1+𝐴𝑠𝑚𝑛𝑅𝑛(3)𝑘0𝑎1.(8d) Similarly on the interface of the conducting sphere (where 𝑟=𝑎2), the boundary condition requires the vanishing of the tangential components of the electric field. Hence, we have22𝑙=1𝑞=1𝑛=0𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐴𝑒𝑚𝑛𝑞𝑧𝑛(𝑙)𝑘𝑞𝑎2𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞×sin𝜃𝑘𝑑𝜃𝑘=0;(9a)22𝑙=1𝑞=1𝑛=0𝐹(𝑙)𝑚𝑛𝑞𝜋0𝐵𝑒𝑚𝑛𝑞𝑅𝑛(𝑙)𝑘𝑞𝑟+𝐶𝑒𝑚𝑛𝑞𝑧𝑛(𝑙)𝑘𝑞𝑟𝑟𝑟=𝑎2𝑃𝑚𝑛cos𝜃𝑘𝑘2𝑞sin𝜃𝑘𝑑𝜃𝑘=0.(9b)In (8a) to (9b), 𝑚 and 𝑛 are two arbitrary integers; the radial function 𝑅𝑛(𝑙)(𝑥) has the following expression: 𝑅𝑛(𝑙)1(𝑥)=𝑥𝑑𝑑𝑥𝑥𝑧𝑛(𝑙).(𝑥)(10) From (8a) to (9b), it shows that (i)firstly, there are six equations and six unknown coefficients, namely 𝐹(𝑙)𝑚𝑛𝑞 (where 𝑞=1,2 and 𝑙=1,2), 𝐴𝑠𝑚𝑛, and 𝐵𝑠𝑚𝑛; the unknown coefficients of electromagnetic fields in the plasma anisotropic spherical medium can be obtained; (ii)then, the radar cross-section of an anisotropic plasma-coated conducting sphere by a plane wave can be derived.

3. Numerical Results and Discussion

In the last section, we have presented the necessary theoretical formulation of the electromagnetic fields of a plane wave scattered by an anisotropic plasma-coated conducting sphere. To gain more physical insight into the problem, we will provide, in this section, some numerical solutions to the problem of a plane electromagnetic wave scattered by an anisotropic plasma-coated conducting sphere.

To demonstrate the accuracy of the solutions achievable by using the present method, we compare bistatic radar cross-sections (RCSs) in 𝐸-plane (𝑥𝑜𝑧-plane as shown in Figure 1) and 𝐻-plane (𝑦𝑜𝑧-plane as shown in Figure 1) to the FE-BI-MLFMA [11], as shown in Figure 2. The series in (8a), (8b), (8c), (8d), (9a), and (9b) converges rapidly, and it is sufficient to take 𝑁=8 as the upper limit of the summation indices 𝑛 and 𝑛. Certainly, similar as in [1315], it should be pointed out that the convergence rate or the upper limit of the summation depends on the electrical dimension of the sphere (with respect to the wavelength). In Figure 2, the RCSs in both 𝐸- and 𝐻-planes using the formulations in this paper are compared to FE-BI-MLFMA. A good agreement of the RCS results is achieved between those two methods, where the permittivity tensor elements of anisotropic plasma medium are characterized by 𝜖1=3𝜖0, 𝜖2=2𝑖𝜖0, and 𝜖3=4𝜖0. And the electric size of plasma-coated conductor sphere is chosen as 𝑘0𝑎1=1.3𝜋 and 𝑘0𝑎2=1.2𝜋. It partially verifies that the proposed method and the Fortran code developed in this paper are correct.

After the validation studies, we obtain some new results unavailable elsewhere in literature. Three examples are considered herein, and their radar cross-sections are plotted in Figures 35.

Figure 3 depicts radar cross-sections of a more general anisotropic plasma-coated conducting sphere; the plasma is lossless and the permittivity tensor elements of the plasma are characterized by 𝜖1=7𝜖0, 𝜖2=𝑖𝜖0, and 𝜖3=5𝜖0; the electric size of the plasma anisotropic spherical shell is chosen as 𝑘0𝑎1=2.2𝜋 and 𝑘0𝑎2=2𝜋. Figure 4 depicts a thick plasma anisotropic medium coated conducting sphere, and the plasma is lossy, the permittivity tensor elements of the plasma are characterized by 𝜖1=(7+0.2𝑖)𝜖0, 𝜖2=𝑖𝜖0, and 𝜖3=(5+0.1𝑖)𝜖0, the electric size of the plasma anisotropic spherical shell is chosen as 𝑘0𝑎1=2𝜋 and 𝑘0𝑎2=𝜋. In those two figures, the maximum number 𝑛 in (8a), (8b), (8c), (8d), (9a), and (9b) to achieve a good convergence is found to be 12 (slightly larger than the quantity of Figure 2 due to the increased electric dimensions).

To illustrate further applicability of the solution to electromagnetic scattering by an electrically large-sized anisotropic plasma-coated conducting sphere (e.g., in its resonance region), the radar cross-sections of a coated sphere of relatively large electric size with 𝑘0𝑎1=4𝜋 and 𝑘0𝑎2=3.9𝜋, under the illumination by an incident plane wave, are obtained and depicted in both the 𝐸-plane and the 𝐻-plane in Figure 5. The permittivity tensor parameters used for this case are 𝜖1=(4+0.2𝑖)𝜖0, 𝜖2=𝑖𝜖0, and 𝜖3=(2+0.1𝑖)𝜖0. As the electric dimension of our radius of the anisotropic plasma-coated conducting sphere is increased, the maximum number of 𝑛 used in (8a), (8b), (8c), (8d), (9a), and (9b) must be significantly increased to 16 to achieve the convergence.

From the above discussions, it is seen and concluded that(i)the radar cross-sections (RCS’s) (𝜎/𝜆2) in both the 𝐸- and 𝐻-planes vary with the scattering angles;(ii)for a medium-sized anisotropic plasma-coated conducting sphere, the RCS’s in both the 𝐸- and 𝐻-planes vary oscillatingly with amplitude decreasing with the scattering angle; (iii)as the large-size for out radius of an anisotropic plasma-coated conducting sphere, the RCS’s in the 𝐸- and 𝐻-planes have almost the same main beam width.

4. Conclusions

The spherical vector wave functions expansion technique is successfully applied in the present work for an analytical solution to the problem of plane wave scattering by an anisotropic plasma-coated conducting sphere in this paper. The solution has only one-dimensional integral which can be easily evaluated. The theoretical analysis shows that when the radius of conducting sphere approaches zero, the results of present formulation can be reduced to those of a single plasma anisotropic sphere. In addition, the general numerical results, including the lossy plasma-coated conducting sphere and resonance region, are given.

Acknowledgments

The author is greatly indebted to Professor Sheng X. Q. and Dr. Peng Z. in Beijing Institute of Technology for sending us their data. This work is partially supported by Grant no. 60971047 of National Natural Science Foundation of China (NSFC), and Grant no. Y1080730 of Natural Science Foundation of Zhejiang Province of China.