Light scattering by irregular interplanetary dust particles

• Okamoto Hajime

  Kashima Space Research Center, Communications Research Laboratory

• Xu Yu-lin

  Department of Astronomy, University of Florida

Bibliographic Information

Other Title

• Light scattering by irregular interplan

Abstract

We review recent progresses in light scattering for non-spherical particles. Special attention is paid to cluster of spheres in order to improve our understanding of interplanetary dust particles. For scattering by non-spherical particles the discrete-dipole approximation (DDA) has widely been used in many scientific fields. However mainly due to the requirements of large computing memory and long computing time, the applicability of this theory is practically limited for rather small particle compared with wavelength. In order to overcome this practical problem, i.e., the large particle can not be calculated by the DDA, we recently developed the a1-term method, which is a modification version of the DDA where the dipole polarizability is determined by the first term of scattering coefficient in Mie theory. Accuracy of this method is tested by comparing the solutions by the a₁-term method with those by modal analysis, which gives the analytical solutions for cluster of spherical monomers. According to the error analysis mentioned above, the applicabilities of the a₁-term method are established as follows. The maximum size parameter of the monomer in the cluster is 1 and the total size parameter of the cluster can exceed X - 100 when the N - 10⁶ dipoles are used. We show the extinction efficiencies and asymmetry factors for cluster of spheres whose size parameter is larger than the wavelength, e.g., the volume equivalent size parameter X is larger than 30. Finally we summarize the applicabilities of DDA, T-Matrix, modal analysis and the a₁-term method. The a₁-term method can partly fulfill a gap where both DDA and the ray tracing technique based on geometrical optics can not be applied when the target is cluster. However for the target which has edges remains to be problematic. This would be the topic which should be focused on future research.

Journal

• Earth, Planets and Space

  Earth, Planets and Space 50 (6-7), 577-585, 1998

  Society of Geomagnetism and Earth, Planetary and Space Sciences, The Seismological Society of Japan, The Volcanological Society of Japan , The Geodetic Society of Japan , The Japanese Society for Planetary Sciences

Keywords

• Space and Planetary Science
• Geology

Details

• CRID: 1390282681485619456
• NII Article ID: 10002207253
• NII Article ID: 130003955919
• NII Book ID: AA11211921
• DOI: 10.1186/bf03352151
• COI: 1:CAS:528:DyaK1cXntlSis7g%3D
• ISSN: 18805981
• ISSN: 13438832
• NDL BIB ID: 4552212
• Web Site: https://ndlsearch.ndl.go.jp/books/R000000004-I4552212
• Web Site: https://link.springer.com/content/pdf/10.1186/BF03352151.pdf
• Web Site: https://link.springer.com/article/10.1186/BF03352151/fulltext.html
• Web Site: http://link.springer.com/content/pdf/10.1186/BF03352151
• Text Lang: en
• Data Source:
  • JaLC
  • NDL
  • Crossref
  • CiNii Articles
• Abstract License Flag: Disallowed