scholarly journals Study on Propagation Characteristics of Obliquely Incident Terahertz Wave in Non-Magnetized Plasma

2020 ◽  
Vol 1607 ◽  
pp. 012041
Author(s):  
Zheng Tao ◽  
Ziyi Pan ◽  
Qiong Ye
2016 ◽  
Vol 2016 ◽  
pp. 1-6 ◽  
Author(s):  
Yunhua Cao ◽  
Haiying Li ◽  
Zhe Wang ◽  
Zhensen Wu

Propagation characteristics of oblique incident terahertz wave from the nonuniform dusty plasma are studied using the propagation matrix method. Assuming that the electron density distribution of dusty plasma is parabolic model, variations of power reflection, transmission, and absorption coefficients with frequencies of the incident wave are calculated as the wave illuminates the nonuniform dusty plasma from different angles. The effects of incident angles, number density, and radius of the dust particles on propagation characteristics are discussed in detail. Numerical results show that the number density and radius of the dust particles have very little influences on reflection and transmission coefficients and have obvious effects on absorption coefficients. The terahertz wave has good penetrability in dusty plasma.


AIP Advances ◽  
2017 ◽  
Vol 7 (12) ◽  
pp. 125325 ◽  
Author(s):  
Yunxian Tian ◽  
Weizhong Yan ◽  
Xiaoliang Gu ◽  
Xiaolin Jin ◽  
Jianqing Li ◽  
...  

2014 ◽  
Vol 63 (19) ◽  
pp. 194101
Author(s):  
Chen Wen-Bo ◽  
Gong Xue-Yu ◽  
Deng Xian-Jun ◽  
Feng Jun ◽  
Huang Guo-Yu

2016 ◽  
Vol 37 (7) ◽  
pp. 845-851
Author(s):  
胡守重 HU Shou-zhong ◽  
侯尚林 HOU Shang-lin ◽  
刘延君 LIU Yan-jun ◽  
王道斌 WANG Dao-bin ◽  
雷景丽 LEI Jing-li

2019 ◽  
Vol 28 (1) ◽  
pp. 014201 ◽  
Author(s):  
Antao Chen ◽  
Haoyu Sun ◽  
Yiping Han ◽  
Jiajie Wang ◽  
Zhiwei Cui

2016 ◽  
Vol 34 (2) ◽  
pp. 276-283 ◽  
Author(s):  
Deep Kumar Kuri ◽  
Nilakshi Das

AbstractSecond-harmonic generation by an obliquely incident s-polarized laser from an underdense plasma in the presence of a magnetic field has been investigated analytically. An expression for the relativistic factor γ has been obtained in the presence of magnetic field. The efficiency of second-harmonic radiation η has been obtained as a function of angle of incidence θ, normalized electric field amplitude of laser beam a0, normalized electron density ${\rm \omega} _{\rm p}^2 /{{\rm \omega} ^2}$, and magnetic field b. It is observed that γ increases with b. In turn, the conversion efficiency decreases with an increase in b. It is seen that the conversion efficiency is affected by the magnetic field due to the modified relativistic factor. In the absence of magnetic field, η increases with a0 and θ. However, in the presence of magnetic field, the conversion efficiency starts decreasing as the magnetic field is increased.


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