Capabilities and limitations of a current FORTRAN implementation of the T-matrix method for randomly oriented, rotationally symmetric scatterers

被引:694
作者
Mishchenko, MI [1 ]
Travis, LD [1 ]
机构
[1] NASA, Goddard Inst Space Studies, New York, NY 10025 USA
基金
美国国家航空航天局;
关键词
D O I
10.1016/S0022-4073(98)00008-9
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We describe in detail a software implementation of a current version of the T-matrix method for computing light scattering by polydisperse, randomly oriented, rotationally symmetric particles. The FORTRAN T-matrix codes are publicly available on the World Wide Web at http://www.giss.nasa.gov/similar to crmin. We give all necessary formulas, describe input and output parameters, discuss numerical aspects of T-matrix computations, demonstrate the capabilities and limitations of the codes, and discuss the performance of the codes in comparison with other available numerical approaches. Published by Elsevier Science Ltd.
引用
收藏
页码:309 / 324
页数:16
相关论文
共 39 条
  • [1] [Anonymous], 1997, LIGHT SCATTERING INH, DOI DOI 10.1007/978-3-642-60465-2
  • [2] SCATTERING OF ELECTROMAGNETIC-WAVES BY ARBITRARILY SHAPED DIELECTRIC BODIES
    BARBER, P
    YEH, C
    [J]. APPLIED OPTICS, 1975, 14 (12) : 2864 - 2872
  • [3] BARBER PW, 1990, LIGHT SCATTERING PAR
  • [4] Bohren C. F., 1983, ABSORPTION SCATTERIN
  • [5] DEHAAN JF, 1987, ASTRON ASTROPHYS, V183, P371
  • [6] DISCRETE-DIPOLE APPROXIMATION FOR SCATTERING CALCULATIONS
    DRAINE, BT
    FLATAU, PJ
    [J]. JOURNAL OF THE OPTICAL SOCIETY OF AMERICA A-OPTICS IMAGE SCIENCE AND VISION, 1994, 11 (04): : 1491 - 1499
  • [7] Gel'fand I M, 1963, REPRESENTATIONS ROTA
  • [8] Golub G.H., 1996, Matrix Computations, Vthird
  • [9] LIGHT-SCATTERING IN PLANETARY ATMOSPHERES
    HANSEN, JE
    TRAVIS, LD
    [J]. SPACE SCIENCE REVIEWS, 1974, 16 (04) : 527 - 610
  • [10] HOEKSTRA AG, 1996, P 1 WORKSH EL LIGHT, P7