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...
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Published in | Journal of physics. D, Applied physics Vol. 48; no. 46; pp. 465201 - 465208 |
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Main Authors | , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
IOP Publishing
07.10.2015
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Subjects | |
Online Access | Get full text |
ISSN | 0022-3727 1361-6463 |
DOI | 10.1088/0022-3727/48/46/465201 |
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Abstract | 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. |
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AbstractList | 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. |
Author | Jia, Jieshu Zhou, Zhongxiang Wu, Jian Pu, Shaozhi Yuan, Chengxun Wang, Ying Li, Hui Gao, Junying Gao, Ruilin Sun, Xiudong Liu, Yaoze |
Author_xml | – sequence: 1 givenname: Jieshu surname: Jia fullname: Jia, Jieshu organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 2 givenname: Chengxun surname: Yuan fullname: Yuan, Chengxun email: yuancx@hit.edu.cn organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 3 givenname: Ruilin surname: Gao fullname: Gao, Ruilin organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 4 givenname: Ying surname: Wang fullname: Wang, Ying organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 5 givenname: Yaoze surname: Liu fullname: Liu, Yaoze organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 6 givenname: Junying surname: Gao fullname: Gao, Junying organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 7 givenname: Zhongxiang surname: Zhou fullname: Zhou, Zhongxiang organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 8 givenname: Xiudong surname: Sun fullname: Sun, Xiudong organization: Harbin Institute of Technology Department of Physics, Harbin 150001, People's Republic of China – sequence: 9 givenname: Jian surname: Wu fullname: Wu, Jian organization: China Research Institute of Radio wave Propagation , Beijing 102206, People's Republic of China – sequence: 10 givenname: Hui surname: Li fullname: Li, Hui organization: China Research Institute of Radio wave Propagation , Beijing 102206, People's Republic of China – sequence: 11 givenname: Shaozhi surname: Pu fullname: Pu, Shaozhi organization: Harbin University of Science and Technology Institute of Application Science, Department of Optical Information Science and Technology, Harbin 150080, People's Republic of China |
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SubjectTerms | charging effects Density Dielectric strength Dust Dusty plasmas electromagnetic waves Grains Mathematical models Rocket exhaust Wave propagation |
Title | Propagation of electromagnetic waves in a weakly ionized dusty plasma |
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