Propagation of electromagnetic waves in a weakly ionized dusty plasma

Propagation properties of electromagnetic (EM) waves in weakly ionized dusty plasmas are the subject of this study. Dielectric relation for EM waves propagating at a weakly ionized dusty plasma is derived based on the Boltzmann distribution law while considering the collision and charging effects of...

Full description

Saved in:
Bibliographic Details
Published inJournal of physics. D, Applied physics Vol. 48; no. 46; pp. 465201 - 465208
Main Authors Jia, Jieshu, Yuan, Chengxun, Gao, Ruilin, Wang, Ying, Liu, Yaoze, Gao, Junying, Zhou, Zhongxiang, Sun, Xiudong, Wu, Jian, Li, Hui, Pu, Shaozhi
Format Journal Article
LanguageEnglish
Published IOP Publishing 07.10.2015
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:Propagation properties of electromagnetic (EM) waves in weakly ionized dusty plasmas are the subject of this study. Dielectric relation for EM waves propagating at a weakly ionized dusty plasma is derived based on the Boltzmann distribution law while considering the collision and charging effects of dust grains. The propagation properties of EM energy in dusty plasma of rocket exhaust are numerically calculated and studied, utilizing the parameters of rocket exhaust plasma. Results indicate that increase of dust radius and density enhance the reflection and absorption coefficient. High dust radius and density make the wave hardly transmit through the dusty plasmas. Interaction enhancements between wave and dusty plasmas are developed through effective collision frequency improvements. Numerical results coincide with observed results by indicating that GHz band wave communication is effected by dusty plasma as the presence of dust grains significantly affect propagation of EM waves in the dusty plasmas. The results are helpful to analyze the effect of dust in plasmas and also provide a theoretical basis for the experiments.
Bibliography:JPhysD-105789.R2
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0022-3727
1361-6463
DOI:10.1088/0022-3727/48/46/465201