Recursive solution of light scattering problem for multi-layered axisymmetric particles V.G.Farafonov St.Petersburg University of Aerocosmic Instrumentation St.Petersburg, 190000, Russia and V.B.Il'in Astronomical Institute, St.Petersburg University, St.Petersburg, 198504, Russia ABSTRACT Light scattering by inhomogeneous (layered) particles is the problem that often arises in optics of the atmosphere and ocean, biophysics, astrophysics, etc [1]. To solve it, one usually applies the model of concentric spheres or infinitely long circular cylinders. However, real particles have a finite size and a non-spherical shape. Recently, Gurwich et al. [2] have made an attempt to develop a recursive solution of the problem for multi-layered spheroidal particles. The authors were basing on the solutions for homogeneous (and core/mantle) spheroids [3-4] and used the approach that had given satisfactory results for multi-layered spheres [5] and infinite circular cylinders [6]. For spheroids, they obtained infinite systems of {\it non-linear} algebraic equations, from which the coefficients of potential expansions in terms of the spheroidal wave-functions could be obtained. However, it looks rather difficult to realize this algorithm as a computer code and to get numerical results. In this paper we suggest a new recursive solution of the problem of light scattering by multi-layered axisymmetric particles. The algorithm utilizes the solution of the problem for homogeneous axisymmetric particles developed in [7-9] and has the following features (see also [10]). The scalar potentials for each layer are represented by sums of two potentials -- the first one is not singular at the origin of the coordinate system, while the second one satisfies the condition at infinity. These new potentials are equal to surface integrals including only the potentials for the previous layer. The potentials of the internal field in the core (the innermost layer) of a particle can be obtained from solution of integral equations that are analogous to the equations for homogeneous particles. The potentials of the scattered radiation are also determined in a way similar to that for homogeneous particles. All the potentials and the Green function are expanded in terms of the spherical wave-functions. After the substitution of the expansions into the integral equations, one gets infinite systems of {\it linear} algebraic equations for the expansion coefficients of the internal radiation in the core and the scattered radiation. The characteristics of radiation scattered by a multi-layered particle are calculated from the same formula as for homogeneous particles (see, e.g., [7]). We have created a computer code realizing the described approach. Test computations have demonstrated its high efficiency for particles of various shapes and structure. The work was partly supported by INTAS (grant 99/652). References: 1. Bohren C.F., Huffman D.R. (1983) Absorption and scattering of light by small particles. J.Wiley & Sons, NY. 2. Gurwich I., Kleiman M., Shiloah N., Cohen A. (2000) Appl. Opt. 39, 470. 3. Voshchinnikov N.V., Farafonov V.G. (1993) Astrophys. Space Sci. 204, 19. 4. Farafonov V.G., Voshchinnikov N.V., Somsikov V.V. (1996) Appl.Opt. 35, 5412. 5. Wu Z.S., Wang Y.P. (1991) Radio Sci. 26, 1393. 6. Gurwich I., Shiloah N., Kleiman M. (1999) J. Quant. Spectr. Rad. Transf. 63, 217. 7. Farafonov V.G., Il'in V.B., Henning T. (1999) J. Quant. Spectr. Rad. Transf. 63, 205. 8. Farafonov V.G., Il'in V.B. (2000) in: W.L.Smith & Yu.M.Timofeyev (eds.), IRS 2000: Current Problems in Atmospheric Radiation, A.Deepack Publ., Hampton, VA. 9. Farafonov V.G., Il'in V.B. (2000) Opt. Spectr., submitted. 10. Farafonov V.G. (2000) Opt. Spectr., submitted.