|  Model  | 
 parameters  | 
 LS method  | 
 free codes  | 
 speed  | 
 accuracy  | 
 range of applic.  | 
 main purpose  | 
 usage  | 
 
|  H o m o g e n e o u s   p a r t i c l e s  | 
 
|  spheres  | 
 x, m  | 
 SVM (Mie theory) [1,2] | 
 many  | 
 exteremely high  | 
 very large  | 
 no limits in x,m  | 
 As a first approximation for scatterers of any shape,
     structure, etc.  | 
 most often | 
 
|  infinitely long circular cylinders  | 
 x, m, alpha  | 
 SVM [3-5]  | 
 a few  | 
 exteremely high  | 
 very large  | 
 no limits in x,m,alpha  | 
 As a first approximation when one wants to learn possible effects of
     nonsphericity of scatterers.  | 
 seldom  | 
 
|  prolate/oblate spheroids  | 
 x, a/b, m, alpha  | 
 SVM [6] / EBCM [16,17] | 
 several  | 
 good  | 
 very large / large  | 
 certain limits in x,m
     (see, e.g., our fig.) | 
 Study of shape effects
     since spheroids with different semiaxis ratio
     present a set of 2D shapes from needles to disks
     (incl. spheres)  | 
 often  | 
 
|  Chebyshev particles  | 
 x, e, n, m, alpha  | 
 EBCM [16,17] | 
 several  | 
 good  | 
 large (?)  | 
 certain limits in x,m | 
 Study of complex shape effects.  | 
 seldom  | 
 
|  superellipsoids  | 
 a, b, c, e, n, orient.angles  | 
 GMT [15]  | 
 one  | 
    | 
    | 
 certain limits in x,m | 
 Possible study of 3D shape effects.  | 
 --  | 
 
| C o r e - m a n t l e   p a r t i c l e s | 
 
|  spheres  | 
 xc, mc, xm, mm  | 
 SVM [7-9]  | 
 many  | 
 very high  | 
 very large  | 
 no limits in x,m (?) | 
 Study of the simplest case
     of inhomogeneity - two-layered particle.  | 
 somethimes  | 
 
|  infinitely long circular cylinders  | 
 xc, mc, xm, mm, alpha  | 
 SVM [10]  | 
 DOP  | 
 very high  | 
 very large  | 
 no limits in x,m (?) | 
 Study of the simplest case of inhomogeneity and nonsphericity -
     two-layered non-spherical particle.  | 
 very seldom  | 
 
|  prolate/oblate confocal spheroids  | 
 xc, a/bc, mc, xm, a/bm, mm, alpha  | 
 SVM [11] / EBCM [13] | 
 a few  | 
 good  | 
 very large / large  | 
 certain limits in x,m  | 
 Study of the shape effects in the simplest case
     of inhomogeneity - a set of two-layered non-spherical particles.  | 
 seldom  | 
 
|  M u l t i - l a y e r e d   p a r t i c l e s | 
 
|  spheres  | 
 {xi, mi}, i=1,N  | 
 SVM [12]  | 
 a few  | 
 high  | 
 very large  | 
 some limits in x,m (?) | 
 Study of the inhomogeneity,
     e.g. in the case of several well-mixed materials.  | 
 seldom  | 
 
|  axisymmetric particles  | 
 alpha, {xi, a/bi, mi}, i=1,N  | 
 EBCM [13]  | 
 DOP  | 
    | 
    | 
 certain limits in x,m | 
 Possible study of shape and structure effects.  | 
 --  | 
 
|  I n h o m o g e n e o u s   p a r t i c l e s | 
 
|  any shape particles with inclusions | 
 fi, ...  | 
 EMT + basic LS method  | 
    | 
 that of the LS method  | 
 usually very low  | 
 limited in x | 
 Consideration of shape and inhomogeneity effects.  | 
 rather often  | 
 
|  (fractal) aggregates  | 
 x, m, D, rho, N, orient.angles  | 
 DDA [14]  | 
 a few  | 
 very low  | 
 low  | 
 certain limits in x,m  | 
 Study of structure and inhomogeneity effects.  | 
 sometimes  | 
 
 
 
  Parameters: 
  
 -- the size parameter x=2 pi r / lambda,
    where r is the radius (for spheroids, e.g.,
    the radius of the equivolume sphere), lambda
    the wavelength of incident radiation;  
  
 -- m=n+ki is the complex rafractive index
 (see corresponding
  section
  for more details); 
  
 -- alpha is the radiation incidence angle (usually between
     a symmetry axis and the wavevector); 
  
 -- the aspect ratio a/b, where a,b
    are the major and minor semiaxes; 
  
 -- The axisymmetric Chebyshev particles have the surface equation
    R(theta) = r (1 + e cos(n*theta)), where r,e,n
    are free parameters; 
  
 -- fi is the volume fraction of inclusions; 
  
 -- for the meaning of the parameters x, m, D, rho, N
    see here; 
  
 -- for the meaning of the parameters a,b,c,e,n
    see [15].
 
  
  References: 
[1] Mie G. (1908) Ann. Phys. 25, 377. 
[2] Debye P. (1909) Ann. Phys. 30, 57. 
[3] Lord Rayleigh (1881) Phil. Mag. 12, 81. 
[4] Wait J.R. (1955) Can. J. Phys. 33, 189. 
[5] Lind A.C., Greenberg J.M. (1966) J. Appl. Phys. 37, 3195. 
[6] Asano S., Yamamoto G. (1975) Appl. Opt. 14, 29. 
[7] Aden A.L., Kerker M. (1951) J. Appl. Phys. 22, 1242. 
[8] Shifrin K.S. (1952) Izv. Acad. Nauk USSR N2, 15. 
[9] Guettler A. (1952) Ann. Phys. 6, 65. 
[10] Shah G.A. (1972) Mon. Not. Roy. Astr. Soc. 148, 93. 
[11] Onaka T. (1980) Ann. Tokyo Obs. 18, 1. 
[12] Wu Z.P., Wang Y.P. (1991) Radio Sci. 26, 1393.(?) 
[13] Peterson B., Stroem S. (1974) Phys. Rev. D 10, 2670. 
[14] Purcell E.M., Pennypacker C.R. (1973) Astrophys.J. 186, 705. 
[15] Wriedt Th. (2002) Part. Part. Syst. Charact. 19, 256. 
[16] Waterman (1971) Phys. Rev. D 3, 825. 
[17] Barber P., Yeh C. (1975) Appl. Opt. 14, 2864. 
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