In”? a :5: 9x .2 .u. . 2. $112!}. 2.2}... i . 7 K m. . u 11:4 *1! . _ .3 t .xu . :xv , , ‘2. 1 1.13.5 9.3.: .H......:,»Lx,.; 3.}: ‘ “i whine. 30m . LIBRARY El ' Michigan State University This is to certify that the thesis entitled A Combination of Rao-Wilton-Glisson and Asymptotic Phase Basis Functions to Solve the Electric and MagnetiE,——E,, (1.15) Writing —E: using (1.6), and (1.9), I k3 VVA]. (1.16) I Ej’(r)=l:—V(1(:)V-A)—ij = —jw(A + l Expanding A with (1.14) and substituting into (1.16), 1 k2 E:(r = r3.) = jwpUqJ(r')g(rg |r')ds'+ VV-Jl‘J(r')g(r_, |r')ds'] . (1,17) I In the second term of the integrand Of(1.l7), the divergence Operator may be taken inside the integration since it Operates on Observation points while the integration is taken over source points. The notation denoting tangential field components will be suppressed unless required for clarity. V'I.[J(r')ggldv' (1.18) Using the vector identity V-( WV) 2 wV-V + V-Vw on the integrand of the right hand side, V-[J(r')g(r | r')] = g(r | r')V-J(r')+J(r')-Vg(r | r'). Since J(r') is a function of primed coordinates and is a constant with respect to the unprimed coordinates. the unprimed derivative of J(r') = 0 :> V-J(r') = 0. Due tO the symmetry ofthe Green's function, Vg(r | r') = —V 'g(r | r'). Using the same vector identity as above, —J(r')~V 'g(r | r') = —V '-[J(r')g(r | r')]+ g(r | r')V '-J(r') . For closed three—dimensional bodies. if we split the volume into two surfaces. 5. and 53 along a cut c with contours C1 and C3 respectively and in Opposite directions, we can apply a two-dimensional version Of the divergence theorem as in [20] on p17. LV '-[J(r')g(r | r')]ds' 2 L] V 'o[J(r')g(r | r')]ds ' + L V '-[J(r')g(r | r')]ds' = <13 fi,-J(r')g(r 1 r')dl + 43 fi,-J(r')g(r | r')a’l 11.19) = 0. For Open surfaces, this identity follows by straightforward application Of the divergence theorem. Therefore, V-J [J(r')g(r 1 r')]ds'= I gV'-J(r'>ds". (1.20) S S The electric field integral equation (EFIE) is by substitution Of( 1 .20) into (1.17), l k2 V130} | r')V'°J(r')a'S']. (1.21) I Ei = fi><[H"(r') + Him]. 11.22) H5 may be written in terms OfA using (1.14), H”(r)=ivXA=vxI J..(r')g(rlr')crv'. (1.23) A Due tO the physical nature Of the problem, we can safely assume uniform convergence of the integrand. Thus, we can interchange the order Of integration and differentiation. Then. rewriting (1.23) using the vector identity Vx(Vw) : wV x V — V x Vtt', H‘(r) = I Vx[.1,(r')g(r 1 r')] ds' : J;{g(r I r')VXJS(r') -J_,.(|")><[V 'g 3* indicates that s is approached from the outside. Due to the discontinuity at the surface. the integral should be taken in the principal value sense [5]. IWIT-(1’): ¥—§.fiXJ..(r')XV'g(r l r'M’S' (1.27) Equation (1.27) is referred to as the magnetic field integral equation (MFIE), valid for closed surfaces [9]. The BF IE and MF IE are actually integrodifferential equations since the unknown quantity is in the integrand of a differential equation. However, they are commonly referred to as integral equations. In general, they are both classified as inhomogeneous F redholm equations where the EF IE is of the first kind and the MF IE is Of the second kind. For more information on Classification, see [10]. 4. Combined Field Integral Equation (CFIE) Although either the MF IE or the EFIE is sufficient to finding the scattered fields. a combination can also be used. Using only EF IE or M FIE leads to spurious resonances for closed scattering bodies [5]. These are resolved using a method that introduces a mixing constant OLE [0,1] to formulate the CFIE, providing stable, unique solutions for all closed scatterers [1 1,12]. a[EFIE]+—%c—(oz —1)[MFIE] (1.28, J ., In this implementation, or = 1 reduces to a pure EF IE formulation while or = 0 reduces to a pure MFIE formulation. 5. Summary EFIE: E:(r>=./wu[l,~'V new] I MFIE: I5>g(r. 1 r')]ds -- I,fi,-F,,,(r)g(r. 1 rod! = 0 . Therefore, C reduces to, C = — I IV '-J(r') I V-Fm (r) g(rs I r')dsds', Then, after switching order Of integration, we have C = I ‘ I JV-Fm (r)V '-J(r') go; I r')ds 'ds. 12 (0 kafl J; Fm (r).VJ.S' g(rs I r')V 'oJ(rI)CIIS .618. (2.3) (2.4) (2.5) (2.6) (2.7) (2.8) (2.9) (2.10) Introduce an incident electric field as E' (r) = éeil’hwr) where li' = -f' = —.i sine, cosrp, —j/sin 6, sin (I), — 2 c056,. r = )Acx+,vy+éz IE' or = —x sin 6,. cos (I), — y sin 9,. Sin 4),. — 2 cos 9,. and e = O, cosa +951 sina. Incorporate asymptotic phase (AP) expansion and testing functions as discussed in section 2.2 using coefficient fl describing the amount Of phase. The testing function I" becomes, at... Fm(r)=fm(r)e I (A ), (2.11) Expanding the current as the sum Of the currents over all N edges, J (r') = ZJnfn (r,)e—m,,(i'-r'). (2.12) Therefore A, B, and C (redefining C by pulling out a minus Sign) can be written so that N I. A : [wflXJn [:8— k3 C] WI‘ICI‘C n=| o A —"(k(,+[3,,, lf'or A =Isfm(r)-ee /‘ ) d5 (2,13) , 517". [3mr+B,,r' , B = I. I,,f.(r)f.g(r. Ir')e ’ ‘ 'ds ds (2...) C = J; Is" Cintegrand g(rs I r')dS 'dS (2.15) where 13 Cimcgrand_ vl:fm(r)e-Wm(°r)]v i.[fn(rI)e—.//311(k'or')]. (2.16) Using the product rule for differentiation, V'Ifm (r)e—_113,,,(1'.rII = f... (r).VIe—/rr,,,(1l.rII+—_,113,(1.IV.fm (r). Then, differentiating. ‘ij lil'r /' m .rsinOtcos¢,+I'Sin9,sin¢,+:cos9, V6 I I : V6-13 ( . ) :15,,,(xsin6 cosq) + ysinO sinrp +zcosaie) I3 (1‘ ") >113 tie-(”mfk‘tl which means V-f“m[m(r)e ”(i r)I=(V-f,,,(r)- ,,,(r) 1,3,,k) MM“). (2.17) Thus, by substitution Of (2.17) mm (2.16), (V-f. (r)—f.(r)-j/3,.I€’)(V'-f. (r ')—f. (r '>-jI3.I€') Cirrtegrand : e.il;i.(fimr+l3nr') . (2. I 8) For notational Simplicity, define g1r1r’>=g(rIr')e‘t"'"‘*~"+i"). 12.19) 11.11.01.111.me yields (V-f.(r)—f,.(r)-jfiml9)(V'-f.(r')—f.(f.-113.I€’)+(cow/3.12"Mam-113.12") =V-fm]—113,.I€’-f,.[V '-f.] —jl3.I€‘-f. (r '> [V-fmml— am. [1942, [V'-f,,(r')] C: j j IgIrIr'y_IIIII.IIIIIII[VIIIIIIII may. S —JfinkI'fn(r')[V°fm(r)i (2.20) 711.13. [IE’-fm(r>][I€’-f.(r ')]I N Combining A, B, C back into A = jwuzJ" [II—ALIC] results in ":1 ’1: If," (r‘)-ée—I‘ ”III" II IIdSZJwfl;Jn Z157, (2.21) where 15 If,,.(r)f,.(r ') f—V-fm (r)[V antr 1)] \ Z'I‘III =1.l..g" +1 +ff3m'9’-fm[V'-f,,] dsvds k0 +113113’°f,.(r ') [V-fm(r)] (2.22) (+£31.13. [k‘-f,,, (r)][k" .1” (r 3] )1 is the EF 1E impedance matrix. For future reference, rewrite (2.21) and (2. 22) 1n a form convenient for discussion; .. N I f (r)oée—I(I”I )" “215: 12011212, I LgIrIr'yjf’Fds ds (2.23) where (—V-fm (r) [V '-fn(r ')] ) .. 1 +j13m/2’.fm(r)[v'.fn(r')] Z,I.I’I=fm(r)fn(r')+—7 . ~,- k0 +JBnk 'fn(rI)[V'fm(r)] (2.24) I+£3.13. [k’-f,,,f,.(r'> = jquJn I I g(r | r') V-fm(r) [V '.r,,(r')] ds 'ds. (2.2s) n=l _ k L. () ..4 If either the testing or the expansion function is AP, one ofthe middle two terms in the brackets of(2.24‘) are added. For matrix elements where both testing and expansion functions are AP, we must compute all the terms in (2.24); the last three of which must be computed at each incident angle. It is important to note that in all cases, the impedance matrix is symmetric, thus we can use specialized solution methods. 4. Magnetic Field Integral Equation Method of Moments A similar application of the method of moments can be applied to the magnetic field integral. Recall the MFIE from equation (1.25), " i __ Js(r) " V V! V d ! nXH (r)——2——-§3,n>< 8(l‘lr) S . (2.26) The sI in equation (2.26) is a reminder that the MFIE is to be evaluated 8 > 0 distance outside the surface, hence should be evaluated in the principal value sense. We test the MFIE, as with the EFIE, with Fm (r) : fm (r)e—IIIIIII(II.r) and expanding the current as the sum of the currents over all N edges, J (r') = fiJnfn (r')e""I”(II'II) 9 l7 yielding, —j[3,,,( (k’o odSr) I f (r)-n>'fi><§..21.f.( (")><[V g(r|r')]e’ I W“ ds ds N :FAIFIE: ; :JZ Zita/FIE m nm ([3,,,,,r+[3 r ’) 23:” =1 WI (”III a. —fm (r)-fz><§ + f" (r')>] Zuni] : fm (r)fn (r ') + —2 - Ai t k0 +1ka ofn(r )[V-fm(r)] K+fimfi.[19490)][19413.0'>] ) and g(r 1 r') = ..+,.e‘j‘Re‘-’"'""~*'+“"">, R = |r - r'l . Observe the form of the above equation is [Z] {J }={_V l, where [Z] is an NxN system and N is the number of edges in the mesh. The tested left hand side of the EFIE becomes A - ' k A?"- 1 A — ' k A”. J fm (r).ee /( 0+I3m) rdS : 1M J‘T+ T— pi (r).ee ./( n+fim) rdS S + . 2.4; (33) Here we have introduced the sign carrying parameter 1, for r in T t, = . (3.4) -l, for r in TI' and used i with the top sign for r in T,,' and the bottom sign for r in T,,‘. The right hand side consists of a constant ( jam ) multiplying the unknown current expansion coefficient EFIE III)! column vector (Jn) times a matrix Z . Matrix elements associated with the nlh row and mth column are then given by ZEFIE _ J' nm T,:+ with 1 — 11,12 —./A7’-(B,..r+/3.r') ”EFIE . T‘J ++T“ 4’” e e Z”’" dS dS (3-5) I" 22 I; FIE Z _ nm In evaluation of anm ,it is useful to . i . recogmze that p, (r), 16 {mm} are expressed . . i 1n global coordinates as p, (1') = i (l‘ — l',-) where r,- is the global position vector to the vertex opposite edge i on Tf' as shown in t—V-fAr) [V '-f.] ‘ 1 +mmléi-f.(r)[V'-f.(r')] -Jf,.(r>f.(r')+—; . ~. k. +1B.k~f.—R—ds = ,.p,- (UTdS ' (3.6) +Ji(P'—P), , 1 R s+(p—pi)J.Ti:Eds where p,p',p,. are projections of position vectors r,r ', r, respectively onto triangle Tf . The first integral is bounded, so it can be numerically integrated, while the second two can be evaluated analytically. Similarly, the scalar integrals can be written ex“ e‘-”"~R -1 1 L ds'=J+——ds'+J+—ds' (37) T: R '1;- R T; R ' ' 4. Coding The code used for testing was primarily a modified version of the program, T riMom, by Dr. Pamela Haddad [8]* implemented at Michigan State University. The modified code, called HotPoppa, is a FORTAN based numerical solver. It allows for solution of the EFIE using the basis function development included in the previous chapter. It was additionally modified to import .grd mesh files created by SkyMesh2TM as well as SDRC IDEAS Universal files (.unv). *Dr. Pamela Haddad performed this work while on NSF Graduate Fellowship at the University of Michigan. She is now a mentor of the technical staff at MIT’s Lincoln Laboratory. 24 CHAPTER 4: RESULTS This chapter presents details regarding numerical solutions of the theory presented above. Results for two different size square plates, a kite, and the EMCC mini-arrow are discussed and compared. We shall analyze the kite in extensive detail as we explore several implications of the mixed basis function method. Additionally, convergence comparisons between various basis function implementations along with mesh density analysis are presented for the kite. Radar cross section (RC S) values are used for comparison as they indicate the scattering characteristics of the object. 1. Square Plate Two square plates are initially considered showing the potential for mixed basis function implementation to perform accurately as proposed. For a 4x4 wavelength plate, a tenth of a wavelength edge length mesh leads to 2240 unknowns while the graded ( or non- uniform) mesh reduces the number of unknowns to 1870. Figure 4.1 shows monostatic RCS results and the graded an. ’0— Rain l n”: l mesh for the 4x4 i§fifi wavelength plate. We observe excellent agreement. The reference ' ' ,, line shows results for tenth he 4 A —-i T 'n in in so “Llr d-l L ofa wavelength Sampling NIOIIOSlilllC Rt goffl-f/Sx-lk plate V\ polarization over the entire square using Figure 4.1: Sample results for a 4M47t plate.[3] 25 only RWG basis and testing 66 . . L . so — Relmence [ V v — Relerm I 0 EEEQPORWGI. 45. 9 EFE‘APiRWG . — we EFIE—RWG functions. EFIE-AP refers to ,0, . . . e *35» AP ba31s and testing functlons (E E E 330» 8 ‘8 on the pictured graded mesh ‘r ‘25 20 while EFIE-RWG + AP ,5 . . ‘ Go in 4b 60 so 100 2i) 40 so so shows the results for us1ng Themdmes, Mamas, VV-polarization HH-polarization RW funct'ons in the o t G 1 u er Figure 4.2: Scattering by a 101x10). plate.[3] region of the graded mesh and AP functions in the inner region. For a 10x 10 wavelength plate, tenth of a wavelength sampling results in a mesh of 14,600 edges while a graded mesh has only 4,792 edges (67% reduction). Again, the results are very promising as we see in Figure 4.2. 2. The Kite: Description The kite is an infinitesimally thin PEC surface in free space. (Figure 4.3) Its length of 23.495 cm is approximately eight Figure 4.3: The Kite wavelengths at ten GHz. The kite is one face of the EMCC mini-arrow, an object studied in Section 4.4. Additionally, we wish to define two ways of observing the kite for scattering solution discussion. Described using standard spherical coordinate basis. the following “cuts” describe the are of incident and observation angles. 26 l. Waterline cut (WL): Figure 4.4 Z 9:90",¢=0“—>180" / 2. Over-the-Top cut (OTT): Figure 4.5 X f y 9 = —90" ——> 90“, ¢ = 0“ / / Figure 4.4: WL Figure 4.5: OTT Note that these two perspectives use full advantage of the symmetry of the kite. For each perspective, we will consider theta and phi polarized incident waves. However, results are not presented for the WL cut theta polarization since an incident wave thus oriented induces no current. The three remaining cut/polarization combinations, over the top theta pol , over the top cut phi pol and waterline cut phi pol, will be abbreviated OTT-T, OTT- P, and WL-P respectively. The kite presents an interesting geometry for method testing for several reasons. 1. It has features (relatively large, flat, and PEC) that take advantage of the methodology. 2. It is small enough to achieve numerical results in a reasonable amount of time at frequencies in the five to twelve GHz range. 3. It is the largest facet of the EMCC mini-arrow for which the community maintains experimental data. We extend our study to the three-dimensional mini- arrow in Section 4.4. As with the square above, we break the kite into two regions, a proportional inner kite and a border region. Refer again to Figure 4.3. The inner region is formed by taking the 27 intersection of lines parallel to the kite edges and separated by a constant distance d from the edges. Due to geometry, and easily observed, the vertex points of the inner and outer kites are greater than (1 apart. One can specify d to determine the inner kite (afier describing the outer kite). Appendix E contains calculations used to derive the vertices of the inner kite from the parameter d. In general, we want to make d as small as possible because as we will see. a small (1 results in a smaller number of unknowns. However, to ensure accuracy, it is necessary to keep d near half a wavelength to account for edge conditions not incorporated in the AP basis functions. This is discussed flirther when we observe results. Using Skymesh2TM to create a triangular mesh, we can define the edge elements for use in our numerical solution. The division of the kite into inner and outer regions provides two essential levels of control. We can independently control the mesh density in the two regions. This allows us to maintain approximately ten elements per wavelength in the border region and much less in the inner region. Skymesh2TM accomplishes a gradient transition in the inner region. Being able to control the mesh density in the two regions enables us to take full advantage of the different basis functions. The different regions in the mesh allow us to spec1fy which type of ba31s funct1on Figure 41): 10 GHz Kite Mesh 28 (specifically, the value of [3) used for elements in each region. Therefore, as mentioned in chapter 2, we can use a fine (ten element per wavelength) mesh with RWG basis functions near discontinuities (edges in the ease of the kite) and AP basis functions in sparsely meshed regions away from the discontinuities. Note that this method differs from [3] where the basis function for an edge is determined by its length. As we discuss kite results, we will use a mesh density factor fora given region or for the kite as a whole. This number is related to the mesh creation and is proportional to the number of elements per wavelength, but does not describe it directly. A factor of 12 roughly equates to a maximum element size of a tenth of a wavelength. Often the mesh density factor is presented as a pair specifying the entire kite and is written outer/inner. (e.g. A mesh density factor of 12/3 describes a fine outer mesh and a relatively sparse inner mesh.) 3. The Kite: Results Several mesh configurations were solved using a variety of basis function combinations and slightly varying d-spacing for all three orientations (OTT-P, OTT-T, WL-P). A frequency of 5 0112 is used for code validation; 10 0112 is presented for RC S curve comparison while 12 6112 is used for a mesh density analysis. These selections are based on the element size relative to the kite, relative to a wavelength, and the total number of elements as it affects the run time. 29 Table 4.1 illustrates the size ofthe problem for various configurations. The problem quickly becomes quite large with increasing frequency. However, 12 GHz allowed for a larger difference and variation control of the inner mesh density lending itself to the mesh density analysis. Code Validation Case: a 5 12717 1447 674 1060 b 1.5 5 3/12 1267 584 925 'c 10 12/12 5667 2734 4200 111.5 10 3/12 4523 2162 3342 le 1 10 3/12 3787 1794 2790 'f1.25 12 16/16 14294 6989 10641 'g1.25 12 14/14 10957 5340 8148 h1.25 12 12/12 8091 3926 6008 11.25 12 12/9 6787 3274 5030 j1.25 12 12/6 6027 2894 4460 11.25 12 12/2.8 5807 2784 4295 Table 4.1: Problem Size Initially, 5 GHz results were studied, however, the edge number reduction was minimal (1060 vs. 925). It was useful to see that using RWG in both regions, using AP in both regions, and using a combination (RWG outer, AP inner) all produced similar RCS values. The following results correspond to row (b) in table 4.1. The separation, d, is set to 1.5 cm because it becomes impractical to make it any larger from a meshing standpoint (the mesh becomes geometrically constricted). Setting (1 less than half a wavelength is not detrimental to the solution in this case. 30 tie RC8 p101 V‘."aluhne. 1; U1 phi—P01 U r v T r v v f ml 1') i 33. q 1 l W- . . x . 40 if so» 1 ‘11 « :11: I ' f-‘1I‘E‘d -70 > - - — WWI} 4 RES (tlBt-xn) '8] A A A L A A A A 0 30 40 EU 80 1|_I';l 1 212' 1 40 1 60 183 Pin (dz-meets) Kite RC8 Plot Over the Top Cut. Cut PhrPol P119 RPS Plot CM?! the T011 Cut, Cut Thetaapol U 1 Y T T r v 1' r v T RCS (strn) PCS (dB-em) £3 .50» —— AP 10 ., , ‘ ~70 A - Mued . ‘ - - -— awe ~ - — we: .. _w A A A A A A A A A . A A A A A A .41 ~80 430 - 40 730 U 20 40 60 8] .81] .11 | .. .10 . :1‘1 1] 20 JD [[1 5.1] Theta (degrees) Theta (degrees) Figure 4.7: 5 GHz Kite RCS Plot, (1 = 1.5 cm. Density Factor = 12/3 RCS Curve Comparison: For a frequency of 10 GHz, three different meshes were considered. The first (c in table 4.1) has a mesh density factor of 12/ 12, approximately ten edges per wavelength across both regions of the kite. RCS curves are shown in Figure 4.8. One can see that the three curves in each figure (AP only, RWG only, and mixed with AP inner and RWG outer) closely match each other. Some discrepancy (3dB max) is apparent in the OTT curves (Figures 4.1] and 4.12) in the —60 to —40 and 40 to 60 degree theta range. However, we can see that the mixed basis function method consistently matches AP only results for this implementation. 31 F :29 PCS Plot Wat-3111119, 1"111 F'hif‘ol 0 fi Y T Y *Y Y — 41:1 .201 _ _' _ 1; 3:3 1 l - '7’“ t 1 A 1 E 1", 11811 ‘1. ..1—“.-‘ m . iv v: .40 . , _ 1 - .13 .11 <92:- 5’3 , 1‘ fill! if 1 {1 1'11 i. \K“; (i r f 2 I I A ' =9 . 1((11 {ii- i“- . 1' 0 4% W ‘ O . ? ED r U a ‘ 4 . 6 .70 > 4 *1) - ‘A A A A A A A A U .‘U 40 60 80 103 1 2'0 1 AU 1E0 1 80 Pm idegvees) Kite PCS Plot Over the Top Cut, Cut PhrPol kite RES F'lot Over the Top Cut, fut Theta-Pol 0 1 U {‘1 1L! 4 It] I! \ EU 10 f N E m ”f 30 u! m in m ‘9‘ TE 3 m '40 * tn 40 | W L) U rx 0: J? -50 , .50 > t 'v 60» {I} » ll AP 70 > . idl‘ed .1 " 7U ' — Riva"; l a] A A A A A I A A A .m A A 1 l- A A {$0 430 40 -2D 0 20 40 60 80 -80 4:30 "50 -Z‘U 0 2'0 Theta (degrees) Theta (dearer-21 Figure 4.8: 10 GHz Kite RCS Plot. Mesh Density Factor = 12/12 The second 10 GHz experiment has a mesh density factor of 12/3 where the inner kite is sampled less. The separation d is 1.5 cm, or half a wavelength. In this case — (d) in table 4.1 — we observe a 20% reduction in unknowns. Figure 4.9 illustrates the element size verses position in the mesh. Figure 10 shows the RC8 values for the various perspectives. In the waterline cut, we begin to see discrepancies in the 145-160 degree phi range where the RWG-only curve does not match the AP and mixed curves. The same mismatch is visible in the OTT cuts across a large range of theta angles with almost lOdB difference for certain angles. These mismatches are expected since RWG typically requires a minimum sampling of ten elements per wavelength over the entire surface for accurate results. Similar discrepancies exist for case (e) in table 4.1 where the border 32 region is shrunk to one cm (see figure 4.1 1). Notice that in case (e), the number of unknowns is reduced 33.5% as compared to (c). RCS (stm) lOGHz Kite (iraded Mesh Edge Length Relative to a Wavelength Figure 4.9: 10 GHz Kite, d = l.5em, Mesh Density Factor = 12/3 Kite PCS Plat Waterline. Cm Phrpul RC8 (stm) U 20 40 80 100 Ph1(degteesl Kite RISE Plot Over the Top Cut, Cut Theta Pol ia 116 W133 P101 (wet the Top Cul. Cut PhtPot n 01> ., .10 . ~10 -2o ‘20 / ' an 30 , 1 E / ' £ I 1 3 340 ‘J ‘1 .‘ ‘ (n 1 . ' \, g 50 ' 11 'I 4 '50 _ 1} l 1. -60 i so 1 ~ 70 .70 ' P ‘ 1 .m ‘ 40 EU 83 83 50 JO JO D 2U 10 U 20 Theta (degrees) Thela (degrees) Figure 4.10: lOGhz Kite RCS Plot, d = 1.5 cm, Density Factor = 12/3 33 Vite PCS; Plot Waterline, Cut PhrPol AP ' f‘diltéi'd -20 r - - R“! 7~13 RC8 (stm) 213 40 60 Ea? 1m 1213 140 161] 1813 Phi (degrees) kite PICS Plot Over the Top Cut. Cut Theta-Pol PCS (stm) RC8 (stm) ‘31 d. 83 ~60 -40 -20 O 20 4O 60 80 Theta (degrees) Figure 4.11: 10 GHz Kite RCS Plots, (1 = lem, Mesh Density Factor = 12/3 Theta (degrees) Particularly visible in Figure 4.11, we see that the mixed basis function RCS curve closely matches the AP basis function curve even with d = 1 cm. The RWG curve does not match because the sampling rate over most of the kite is less than ten elements per wavelength. Remember that the mixed basis function method has a lower implementation cost than using all AP basis functions. Selection of the RWG Region Thickness: If we view the above RCS data plotted differently, we can consider the implications of changing d. Figure 4.12 shows RCS curves for mixed basis function implementation with d = 1 cm, 1.5 cm, and for a uniform mesh (12/ 12). This figure is included here 34 because it is the most interesting of the , , “‘9 p.11... F"f" ""9?B‘S'5-‘3”T"fi'ap°‘ D 1 fl orientations. The other eight orientations 401 [I T 3‘1"?“ - - — D '— l S ‘0’ A i . . . q , are 1neluded in Appendix D. We can see a I” 7;;- 4 1" -.\~._ ,3 q‘ 35-. g 1. \1 1:6 , :1 {‘5' r .1 ,::‘ ' . J 40 ,c 13' ~- 1 mat-1', w / l . that as d is decreased, the RC8 values a ,1 l. 1" (,1 111 (r; .1 (.1 «19., / \1 .‘rr 1- 'I/u 1 i" . .1 1 .9 -- I; . 11 \- ' o [I . . . . 11‘: V: dev1ate from the htghest sampltng rate 993:..- '1‘: .71'1 j. (‘1‘. curve at certain theta angle ranges. Hence, ,0 ll . . . . . 1 . . if. ' 190 an - 40 .20 0 .13 40 to to The-ta (degrees) we experience the traditional trade-off of Figure “21 ‘0 (.in Kite RCS, OTT-T Mixed Basis Fttnctions number of unknowns verses quality of solution. Convergence: In numerical methods, rate of iterative solution convergence is a constant concern. Since AP elements in the matrix require computation at every incident angle, we are naturally concerned about the convergence of the matrix solution for each angle. Since we wanted a convergence measure relative to an all-RWG basis function implementation for a given mesh, we chose to observe the matrix condition number, the ratio of largest to smallest eigenvalue. Figure 4.13 shows that although the condition number varies with angle, there is no apparent correlation and the overall variation relative to RWG-only is minimal. Therefore, we can conclude that additional matrix convergence issues do not result from using combined basis functions. 35 'mle Cor-damn Number 19101 Waterime Cut Phi Pol r 1:.- i Uhd-llul' 115mm Plot [M1 tr..- 1”. 1'_ 1.! F». .m 11...” P01 351'; v . . . . r 3500 . T fir AP p i — 9W1} — F.» "L-LIJ 25130 > o‘ . .n . o n g . *3 59001115511 11.111111511 E: 1w: » 3 1:00. 1111- > . 13301 5"? > . {our 1", A 4 A; A 1 1 A ‘ U A‘ L x - L L 4 11 ;-ji .m 1,1;1 an 1m 1m 1411 11.11 1113 '9“ "W "U 1” ‘-' ~'-' "J W ”0 Pm (degveez) 'i'wia dun-re; Figure 4.l3: 10 GHz Kite. d = 1 cm. Condition Number vs. Incident Angle Mesh Density Analysis: We completed a mesh analysis to study two particular issues. First, how dense should the mesh be to provide a converged RCS value? Second, how sparse can the inner mesh be? Using 12 GHz, the number of unknowns necessary increases dramatically (33%) from the 1061-12 case (table 4.1). However, the increased frequency allows more flexibility for this particular analysis. Half of a wavelength at 12 Ghz is approximately 1.25 cm so for the 12 GHz experiments we use d = 1.25. We considered the phi angle of 63 degrees on the OTT-T out since this was the region of maximum discrepancy among RCS curves. Addressing the second question above first, we find that m-“ m 714... 14:1: .":. ‘_ due to physical meshing constraints, a 2.8 mesh density ng. 13.13 34144152347 i‘ RWG' 12.2.8 31.76 2647.6 Mix "14.14 41.40.977.43 Mix 12.1: -3352 515.26 MIX 12.2.21 -3122 3491.1 Table 4.2: Density Analysis (9 = (13". 8 = 0“, Freq = IZGHZ factor is the lowest possible. Below 2.8, the mesh has the same number of unknowns. That is, the kite is geometrically constricted below 2.8 mesh density factor. 36 To answer our first Kite PCS Plot Over the Top Cut, Cut Theta-Pol question, we again consider 0 ' Mixed12 10 - RWG 12 . . ' b O M x d 2.8 1 theta = 0 and phi = 63 Since - — Rivis 2.8 -20 1- (5120 this observation angle P b E -30 - 4 w ‘0 Q & ‘D ’ 9 appears to have the largest 3% 40 _ l i9 9 is) i g a I ' g..o. Q RCS discrepancy. Using 60 - O . 1 - - o l . . . 130 ~ 0 ‘ . RWG basrs functions With a 9 -70 .- density factor of 12/12, we -:1| . 1 l 1 1 1 1 1 1 -80 -60 4:0 -20 o 20 40 so 80 observe from table 4.2 that Theta (degrees) Figure 4.14: 12 GHZ Kite RCS, OTT—T, d = 1.25cm the RC8 value appears to have converged since at a mesh density factor of 14/14 is very close to the value at 12/12. Using mixed basis functions on a uniform mesh, the RC8 value does not converge until a mesh density of 14/14. RCS values for 12/12 and 12/2.8 are compared for mixed vs. RWG basis functions in figure 4.14. Interestingly, the discrepancy in the theta range of discussion shows the RWG 12/ 12 value is most clearly matched by Mix 12/ 12 while RWG 12/2.8 and Mix 12/2.8 match each other, but not RWG 12/ 12. Aside from this observation angle range, such discrepancy does not arise (Appendix D). It appears some other phenomenon may be affecting our results in that observation angle range. 37 Vitr- C undltion #F‘lot Over the Top Cut, Cut Thetmpol 4000 Y 1' f 1 v T Y r :‘\/"’ 3503 » 1111‘. 111/ 1 l. ‘ ' k I i' l /‘ rl i1 1' ii " . .. 'u "4., \ .‘\ 1%}‘4 {10.1 1- ~./ ‘v . .t‘. “I. J ‘ 11 1,1. . t- o ooooooo o‘\./o F‘V/ a \ o 4 ‘JUU ' . t g “i 3003 P E . Mixed 12 1:) ' ' _ H‘t‘nv'l} l? 150] 1 — Mired 2 13 - ewe 2 8 101]] r SCENIFO Warm—«Y o -0 “0—th v 0 L 1 L l 4 1 J. 80 -60 «:0 1'1 0 20 40 60 80 That 5 (degrees) Figure 4.152(‘ondition Number vs. Incident Angle One can see in Figure 4.15 that the condition numbers are much larger for 12/ l 2 than for 12/2.8. This makes sense since the same problem is specified more finely in the 12/ 12 case. The angles studied are shown by the dots plotted in the RWG curve in Figure 4.15. In the 12/2.8 mixed case, we see that we can maintain relatively accurate results (especially for theta angles near 0) for the kite using this methodology to reduce the number of unknowns. 4. Extension to the EMC C Mini-A rrow The kite can be extended to similar shape, in particular, the three-dimensional mini- arrow. The mini-arrow is formed by adding the point (8.935,0,3.932) to the kite and extending a line from each kite vertex to this new point. In figure 4.16 a tenth of a 90' ..__ 180 0‘ ' ”919-1- .L 2111 U +- 3......"""“”““”““ ' . i '. ' M 135': ~13». ¢¢ olarization .. one.” polarization ,. -;:»~ I." P ,. . - _n . ‘ ‘1‘- i. ' ".1: , 3': ."V l' ' Y 2‘3." 1 \ i .43\ l i , I ! 45‘. ‘ K! -50 ' I ' "r“? i o . 0 to ten 150 am 250 sec .150 '1 f‘.‘ 1 .s ‘::u .211 .90 5:32‘ 1:552» thtdegveos: 3': 1:21.] n.w.-.~: Figure 4.16: Mini-arrow scattering at 9 GHz.[3] 38 wavelength sampled RWG only mesh (reference) is compared with a graded mesh using the combined basis function methodology at 9 GHz. This demonstrates the methods ability to simulate three-dimensional objects using CF 1E (alpha = .5) with mixed basis functions. CF IE-AP refers to the implementation of RWG and AP basis functions. It should be noted that UIUC [3] computed these results and duplication at M SU was deemed unnecessary. Next, we consider the mini—arrow at 12 GHz to determine edge reduction potential. However, due to the small surface area of each surface of the mini- arrow, the mesh is geometrically restricted rather than current restricted. We do not achieve a significant reduction in edge unknowns. Hence, the combined basis function methodology is only beneficial for large smooth sections. 39 CHAPTER 5: CONCLUSION We conclude with a surmnary of the research and the knowledge gained along with noting some particular challenges and future work. 1. Summary In the past, people have used Rao-Wilton-Glisson expansion and testing functions to solve the PEC scattering integral equation problem. For accurate results, this method requires element edge sizes at most a tenth of a wavelength or equivalently, approximately one hundred element edges per square wavelength. Thus, increases in frequency yield exponentially larger problems. Aberegg and Peterson [6] addressed the issue by multiplying the RWG function by the phase term of the incident field (i.e. asymptotic phase functions). While AP functions allow for less dense sampling in regions where the surface current phase is not rapidly changing, they require computing each matrix element at each angle of incidence, a costly disadvantage. Since AP functions still require high sampling rates near discontinuities, using RWG functions in those regions eliminates some of the added computation. Thus, the combination of RWG and AP basis and expansion functions on the same surface has the advantages of both methods. This research shows that such a combination of functions, appropriately used, does in fact achieve benefits of both, faster computation time from RWG, less unknowns from AP. We find that the gain is maximized for surfaces where the majority of the element edges (not necessarily the majority of the surface) use RWG functions. We have also shown that the advantages of the methodology are highly dependent on the physical characteristics of the geometry. Unique contributions from this research include: 40 1. Impedance matrix form shown in equation (2.22). 2. Use of the traditional singularity extraction technique [21] with asymptotic phase basis functions over flat triangles. 3. Convergence and mesh analysis for the kite geometry. 4. Investigation of region specific sampling with combined basis functions. Summary of Results from Specific Geometries The kite and square geometries show approximately 35% and 68% (respectively) reduction in unknowns when discretized using a graded mesh and RWG-AP combination as compared to a tenth of a wavelength RWG-only meshing. With the number of AP elements minimized and their usage location chosen wisely, matrix element computation is significantly reduced from an all AP scheme. Therefore, for such geometries, the combination of basis and expansion functions is a more effective solution method than either AP or RWG used by alone. For the mini-arrow geometry, we find that due to the small surface area of its side surfaces, the meshing is geometrically constricted. On such a geometry, the reduction of unknowns is not significant and the introduction of any AP elements to an RWG-only implementation actually increases the solution cost since matrix elements must be recomputed at each incident angle. In a related effort in conjunctions with UIUC [3], we found that the conesphere geometry with C2 continuity across the sphere-cone interface can benefit from an AP only type solution. On the conesphere, the number of elements in the mesh away from the 41 discontinuity is kept large due to the curvature of the object. We found that the introduction of RWG elements near the discontinuity had minimal affect in reducing the design cost since the number of RWG tested and RWG expanded matrix element entries was small compared to the AP tested AP expanded entries, as shown in Figure 5.1. An AP-only solution method may be better than RWG-only; however, this depends on the memory and processor resources available (AP-only is more processor intensive while RWG—only requires more memory). Regardless, for the conesphere geometry a mixed implementation reduces overall costs some, but the geometry lends itself to an AP only mesh. Figure 5.1: Graded Mesh on Square Plate vs. Conesphere Conclusion For all the objects considered, the AP only and RWG-AP combination RCS values we observed were accurate relative to the traditional tenth of a wavelength sampled, RWG tested, RWG expanded method of moments numerical solution. On large, smooth surfaces with low curvature the RWG-AP combined basis and testing function method is a more effective solution that solely an RWG or AP implementation. 42 2. Challenges The usual long run times inherent in most numerical methods always have an impact on the number of different implementations one can study. Several simple and electrically small objects were considered in this research to quickly gain some insight into the fundamental characteristics of each methodology. From this information, we can begin to estimate how each might work on more numerically intensive problems. As computational resources continue to become more powerful with time, we can broaden the scope of our studies. Discretizing an object into a consistently “good” mesh is a particularly difficult task. It is an art form in itself, but is essential to quality numerical results. Since the scattering problem is sensitive to discontinuities, a mesh that accurately describes a testing object is crucial to attempting measured comparisons. Both high quality meshing programs (e.g. SDRC IDEAS, PRO-ENGINEER, etc.) and a highly talented mesh generation engineer are required to obtain high quality meshes. The essential difficulty with the method of moments matrix solution is the requirement for large amounts of computer RAM. As frequency increases, so does the need for memory. 3. Future Work Following this research it would be beneficial to study this method with more objects and at higher frequencies to broaden the knowledge base and understanding of the practicality of the combined basis function method. Specifically, extended studies with curved 43 surfaces using six-point second order triangles have been presented in [3] and further research would be very beneficial. From a more general perspective, the possibility for other basis functions with the method of moments has the potential to dramatically improve the scattering problem. Further application of the fast multipole method [3] can impact the solution cost for large matrices. It would be of particular interest to consider applying the AP method to radiation studies since antenna problems involve only one right hand side of the integral equation. Thus, the advantages of AP might be realized without the disadvantage of needing to compute the matrix elements for multiple incidence angles. 44 APPENDICES 45 APPENDIX A: FUNDAMENTAL THEORY There are three sections to this fundamental electromagnetics theory appendix. We begin with the independent large-scale form of Maxwell's equations. the fundamental starting point for electromagnetics theory, and almost all electrical physics for that matter. The vector potential quantities are then developed and finally a brief discussion of the Green's function as implemented in the above research. These are included in an attempt at completeness. Since we very well could have started with the results this development derives, these basic concepts are included as an appendix. Hopefully their inclusion will enable those not familiar with the electromagnetics discipline to understand and critically evaluate the fundamental challenges faced when we apply the theory to real situations. I. Maxwell 's Equations Definitions: (All the following quantities are functions of time and a spatial position vector r.) E = electrical field intensity (Volts) B = magnetic flux density H = magnetic field intensity D = electric flux density J = moving charge density (Amperes per square meter) p = charge density (Coulomb's per cubic meter) 46 Constants: l 80 = 3—6;* 10 Farads per meter ...permittivity of free space 11,, = 47: "‘10-7 Henry's per meter ...permeability of free space Parameters of a medium: 8 = 8,80 describes the permittivity in relation to free space and it = urn.) describes the permeability relative to free space while 6 describes the conductivity of a medium. In general, S is any open surface bounded by a closed contour C. Therefore, our fundamental independent Maxwell's equations include F araday's (A. l) and Ampere's laws (A.2). (fie E'dl = —:,'—l, s fi'B d5 ...Faraday's law (A- 1) 0 (It [1“ 4% B061]: 8 Sh'E d5 + L fi°J d5 ...Ampere's law (A.2) Conservation of electrical charge requires J; fi-J ds = ‘67.le dt. (A.3) Equations (A.l)-(A.3) are in large-scale form. Assuming that C and S are not functions of time, we can pull the time derivative inside the surface integral. Applying Stoke‘s Theorem, I VX Vol? (13 = @V (11 , to the left hand side of(A. l) and moving the right hand side of (A.1) to the left we get JS[VX E + "(,L, B] ‘15 dS = 0 . Since this holds for any surface, the bracketed quantity = 0 or equivalently, 47 VXEZ—iB (A.4) (It If we apply Stoke's Theorem to the left of (A2), move the right hand side to the left and combine the integrals, we can use the same argument as above (equation is true for any S) to get, iVxB=J+eofiE (A.5) If we apply the Divergence Theorem, j'V'V dV = i V°15 0'8 , to the left hand side of the constraint equation, combine the integrals, and note that it holds for all volumes v, we get, — __6L V°J — .1. 0 (A6) Equations (A.4)-(A.6) are the point form of the independent Maxwell equations. If we take the divergence of both sides of (A.4), use the vector identity V-Vx A : 0 , and invoke causality, we observe V-B = O (A.7) Taking the divergence of both sides of (A5), and use the same vector identity to get % p = 8,, 73’: V'E I) if [EOV'E — P] = 0 . Time integrate both sides and invoke causality to get the point form of Gauss' law. V.E = L (A8) 0 In general media (not necessarily free space), we define auxiliary equations to include non-zero magnetization M and polarization P, also functions of time and space. 48 1 . . . H = T B — M (Amperes per meter) ...magnetic field intensrty J = J i + 0' E (Amperes per square meter) ...total free current D = 80E + P (Coulombs per meter) ...eleetric induction, flux density In simple (linear, isotropic) media, we then define P and M in terms polarization susceptibility xc and magnetization susceptibility 1.... P = 8.,XCE and M = X...“ So by substitution D = 80E + P = 80E + eUxCE = eo( 1+xc)E = e(r)E = e._,e..(r)E and B = 1|.)(H + M) = 110(1+Xm)H = “(OH = 11.11.(r)H The above equations are valid even for inhomogeneous media. By substitution into (A4) and (A.5),VXE = ‘:71,#(T)H and tVX#(T)H : J + (%D. Ifwe assume the media is homogeneous (permeability and permittivity are not functions of space), E and u can come out of the derivatives, leaving Vsz—aQ—fiH, (A9) VxH=J+%D. (Am) For use in the frequency domain, it is useful to define phaser notation for the vector field quantities. We can write E(l',t) = E0 (r) 008 (wt +(pE (r)) where a) = 27rf. Using Euler's equation to expand the cosine function into exponentials and considering the real part, the following is equivalent, E(r,t) : E0 (r) Re {61(wl+¢lj(r))} : Re {E(r)e¢5(l‘)elwl } (Al I) 49 We now make the following key observations: 1. All the vector field parameters can be written using a similar argument as for the electric field. 2. The operator Re{ } commutes with addition, subtraction. integration. and differentiation. 3. Time integration transforms to multiplication by jw in the frequency domain. 4. Since every parameter contains an e’l‘”t term, we can suppress it for notational purposes. The resulting time harmonic Maxwell Equations and the continuity equation, with vector itm field quantities having spatial dependence and a suppressed e term are: Vsz—jwuH (A12) VxH=J+jwa=J‘+(o+jwe)E (A13) _ l V-E——p(r) (A. 14) 8 V-H = 0 (A15) V-J = jwp(r) (A.l6) Notes: 0 To convert to the time domain, unsuppress the e""l term and take the real part. 0 The above form of the equations is under the relatively strong assumption of linear, homogeneous, isotropic media. 0 lfthe medium is free space, 8 = 80, u = 110, o = 0. If source free, .1 i = 0. 50 2. Boundary Conditions For a comprehensive explanation of boundary conditions. see [9]. page 13. A summary is stated here. At the interface of two media with differing electrical properties, Maxwell's equations dictate the following: o The tangential components of the electric field across an interface between two media with no impressed magnetic current densities along the boundary of the interface are continuous. nx(E2—El)=0 (A17) 0 The tangential components of the magnetic field across an interface, along which there exists a surface current density Js (A/m) are discontinuous by an amount equal to the electric current density. 15X(H2—H1)=Js (A.l8) In a medium with infinite conductivity, the tangential components of E and H = 0. Thus on the surface of a perfect electrical conductor (PEC), the tangential component of the total electric field equals zero and the tangential component of the total magnetic field is equal to the surface current density. 3. Vector Potentials By making a change of variables, we can represent the electric and magnetic fields in terms of intermediate variables, the electric and magnetic vector potentials. Using the Lorentz gauge condition, we can manipulate the equations into a standard differential 51 equation with solutions. In this section, we will define the vector potentials and derive the scalar Helmholtz equation. Metic Vector Potem Since we know VopH = 0 and the vector identity Vo(Vx V) = 0 . define A such that aH=V>VX(E+ja)A)=O (A20) Since we have the vector identity Vx(—VV) = 0 , define (I)c such that E = -V(I>, —j£0A. (A21) Substitute (A. 19) and (A21) into (A.l3), Vx[VXA]=J'+(o+jme)(—VVx(H+ja)eF)=O, (A27) We can then define “-Vwm 3 H = -V(Dm — jwllF . Using the same vector identities and substituting into (A. 12), VxVxF = jwp(—V(I>m —jpr). (A28) _ jwé‘ By choosing the Lorentz gauge condition again, (pm “ T V°F and the same vector identity as above, we can write (A.28) as V2F+k2F =0. (A29) Recall that A, F, E, HA)”, , and s are all functions of position. 4. Scalar Green 's Function Let us consider the scalar Helmholtz equation from section 2 of this appendix, V2w(r)+k2w(r)=—s(r), (A30) 53 Recall from above that u! is the unknown wave function, s (r) is a known volume source density, and k is the wave number. For a single point source r' observed at r, s(r) = 5 (r —r') , we define the Green's function, g(r|r'), as the field at any r due to Figure A-li Pit-51110" Vectors r'. Thus the Green's function for the scalar Helmholtz equation is V2g(r | r')+k2g(r| r') = —6 (r— r'). (A3 1) can be solved using the integral transform technique. First, take the Fourier transform. —(Af +Af +Af)g(2t|r')+k3g(}. Then solve for g . e—jix' (3- 1).!" ~ A r' = = g( I ) (if—k3) (A-k)().+k) Then. take the inverse Fourier transform. 00000 g(r|r')= (sir i .l lgo‘fl'flr'mdil —oo—oo—oo I") = —c '1'" (A31) (A.32) (A33) (A34) To analytically evaluate the above integral (which has poles at :k = A ), switch to polar A-space, evaluate over a pole excluding contour in the upper and lower half planes exploiting Cauchy's Integral Theorem resulting in g (r l I") = 3%,;6_"/AR where R = lr—r'l. 54 (A35) Since g(r|r') is the point source solution and J(r') includes the magnitude and distribution throughout a source region, by superposition, A=uJ,J(r'>g(r1r')dV' (A...) is a solution to (A25). For a surface current density, (A36) reduces to A =uJSJtr9g- — Slraighl 2° - - — 0:1 4 0:15 .3). . 1‘ 40» , ‘ e i I .s 8‘ 8" “‘§ __ 3 N75}; . 148 1m 133 K11. Pattern Plot; AP-OTT Cut Phi Pol —— Straight - - — [i=1 . D=1 5 momma) 3030.404001] Theta (dogmas) Theta (degrees) Figure DJ: 10 GHz Kite RCS, AP Basis Functions 58 tha Pattern Plot: Mil-WL Cut Phi Pol Kite Pattern Plot: Muir-OTT Cut Phi Pol ‘15 v r 1 Y Y Y T I r Y v v 7 — Stral ht 0 ‘ ‘ ‘20 9 ‘ — Straight - . — 0:1 - - — D=1 -25 . a 0:1 5 40 .. . 0:1 5 , .m P .35 . ‘ 4 l E 40 ' 1 < 2 1 u '45 h 1 \' 60» , i ' ' “ . l | ' on F." .fi 1 . . | l “I -( i " 'f U i l L | m '4 ‘I ‘ f -4 56 . . t’. 4 .70 A A A A A A A A A A A A A A A A. A 0 23 49 80 m 1(1) 120 110 160 TM -33 ~83 40 ~23 D Z) 40. 50 m Phi (dogma) ' Theta (dagraas) Figure D.2: 10 GHz Kite RCS, Mixed Basis Functions Kite Pattern Plot: RWG-WL Cut Phi Pot ‘15 r v v v V I. r r 1 —— Straight '20 — 0:1 ‘ - 0:1 5 .25 . . .39 . . .35 l , 1 E 40 " I i 9 | I g "5 ‘ a < . 0 l \. ‘50 ' i | i I I .. I . . 455, ' . . g . ‘ i 1 m ' ‘0’ a 1 F V a 455 - , " 4 .70 A . A . A A A 4‘ A .1 D 23 40 H) m 100 120 140 1G] 1m Phi (dagraaa) Kite Pattern Plot" RWG-OTT Cut Theta Pol Kite Pattern Plot: RWGOTT Cut Phi Pol 0 r 0 — Straight — Straight . _ 0:1 — 0:1 -10 _ o D=1 5 D“ 5 20 30 ' s i E ' A 3 ' ~ 5 l .3 .. .' 1 r x. .. .‘0 I i“ a a .j .50 > a l, A 80 ~ 4 _70 L . A . A . A I . m A A A '1 A A A I A an ~60 ~40 ~23 D m 40 an m 33 ~60 40 -.’.0 U 20 40 so a) Theta (degrees) Theta (degrees) Figure D.3: 10 GHz Kite RCS, RWG Basis Functions 59 BIBLIOGRAPHY 6O [1] [8] [9] [10] [11] [121 [I31 [141 [15] BIBLIOGRAPHY S. Rao, D. R. Wilton, and A. W. Glisson, “Electromagnetic Scattering by Surfaces of Arbitrary Shape,” IEEE Trans. Antenna Propagat, p. 409, May 1982. K. R. Aberegg, Electromagnetic Scattering Using the Integral Equation-Asymptotic Phase Method, Ph.D. Dissertation, Georgia Inst. of Tech., Nov. 1995. M. A. Kowolski et al, “On the Three-Dimensional Integral-Equation Asymptotic Phase (IE-AP) Method,” PIERS, p. 136, 2000. R. F. 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