Mie scattering by ensembles of particles with very large size parameters

2004/06/04 by S. Wolf, Н. В. Вощинников, N. V. Voshchinnikov · 6 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics and Star Formation Studies #Atmospheric Ozone and Climate #Galaxies: Formation, Evolution, Phenomena #astro-ph #physics.optics

paper · pdf · doi:10.1016/j.cpc.2004.06.070

published as Comput.Phys.Commun. 162 (2004) 113-123 · Comp. Phys. Comm., in press

arxiv created 2004/06/04 · openalex publication_date 2004/07/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We present a computer program for the simulation of Mie scattering in case of arbitrarily large size parameters. The elements of the scattering matrix, efficiency factors as well as the corresponding cross sections, the albedo and the scattering asymmetry parameter are calculated. Single particles as well as particle ensembles consisting of several components and particle size distributions can be considered.

Citations

• Light Scattering by Small Particles

Cited by

• Constraints on the structure of hot exozodiacal dust belts
• Debris disk radiative transfer simulation tool (DDS)
• Inferring giant planets from ALMA millimeter continuum and line observations in (transition) disks
• The extremely truncated circumstellar disc of V410 X-ray 1: a precursor to TRAPPIST-1?
• Gaps, rings, and non-axisymmetric structures in protoplanetary disks: Emission from large grains
• Modelling of mid-infrared interferometric signature of hot exozodiacal dust emission
• What Sets the Radial Locations of Warm Debris Disks?