DocumentCode
1645536
Title
Study on the Differential Scattered Section of a Moving spheroidal Interstellar Dust
Author
Wang, Ming-jun ; Wu, Zhen-Sen ; Li, Ying-le ; Hui, Zhang ; Zhang, Xiao-an
Author_Institution
Dept. of Phys., Xi´´an Yang Normal Coll., Xi´´an
fYear
2008
Firstpage
193
Lastpage
196
Abstract
The laser scattering characteristic of spheroidal interstellar dust moving with a high speed is investigated numerically. The coordinate and vector transformations have been presented to establish a theoretic basis for studying the laser scattering of a moving spheroidal interstellar dust. The laser differential scattered section (DSS) of a moving spheroidal interstellar dust is explained by the electric and magnetic field from Mie scattering theory in detail. Assuming the laser length of 2.2 mum, we had computed the ratio of the laser DSS of the moving spheroidal interstellar dust to that of the static interstellar dust, which changes with radii and scattering angles of the particle. The numerical results showed that the laser DSS of the moving spherical particle is tightly connected with its speed and scattering zenith angle. If a spheroidal interstellar dust moves with high speed, it has a strong forward scattering .The speed of the moving spheroidal interstellar dust is higher, the laser DSS value is larger. If a spheroidal interstellar dust moves with a low speed, the Influence of a high-speed spheroidal interstellar dust´s movement on its scattering characteristics will be neglected.
Keywords
Mie scattering; cosmic dust; interstellar matter; laser beams; Mie scattering; laser differential scattered section; laser scattering; moving spheroidal interstellar dust; Decision support systems; Dielectrics; Laser theory; Laser transitions; Light scattering; Mie scattering; Particle scattering; Physics; Silicon; Space technology;
fLanguage
English
Publisher
ieee
Conference_Titel
Millimeter Waves, 2008. GSMM 2008. Global Symposium on
Conference_Location
Nanjing
Print_ISBN
978-1-4244-1885-5
Electronic_ISBN
978-1-4244-1886-2
Type
conf
DOI
10.1109/GSMM.2008.4534596
Filename
4534596
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