2014
DOI: 10.7498/aps.63.035203
|View full text |Cite
|
Sign up to set email alerts
|

Numerical study on the effects of magnetic field on helicon plasma waves and energy absorption

Abstract: The propagation properties of electromagnetic waves excited by helicon antenna with a parabolic radial electron density distribution in an external magnetic field were studied. Maxwell equations are numerically solved using the linear disturbance wave assumption to obtain energy distribution, when the magnetic intensity changes from 80 to 800 G. The radial electromagnetic wave and energy deposition intensity distributions were obtained. Results show that when magnetic intensity grows, the helicon wave is littl… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0
1

Year Published

2014
2014
2024
2024

Publication Types

Select...
6

Relationship

0
6

Authors

Journals

citations
Cited by 9 publications
(2 citation statements)
references
References 18 publications
0
1
0
1
Order By: Relevance
“…At the same time, the absorption of energy is gradually concentrated at boundary, indicating that a large magnetic field will lead to a serious uneven distribution of radial energy. [27] This situation will not affect the generation of HWP, but will reduce the deposition effect between antenna and plasma. Through calculation and analysis of the magnetic field range of 200 Gs-1800 Gs, it can be obtained that a small magnetic field cannot produce high relative absorption power at center, and thus cannot achieve a good power deposition effect.…”
Section: Numerical Simulation Analysismentioning
confidence: 99%
“…At the same time, the absorption of energy is gradually concentrated at boundary, indicating that a large magnetic field will lead to a serious uneven distribution of radial energy. [27] This situation will not affect the generation of HWP, but will reduce the deposition effect between antenna and plasma. Through calculation and analysis of the magnetic field range of 200 Gs-1800 Gs, it can be obtained that a small magnetic field cannot produce high relative absorption power at center, and thus cannot achieve a good power deposition effect.…”
Section: Numerical Simulation Analysismentioning
confidence: 99%
“…功率沉积的原因 [12] . 2023年, 更进一步的分析结果 表明大密度梯度引起的模式共振机制可用于电子 加热 [13] . 在国内, 成玉国等 [14] 数值分析了径向电 子密度呈抛物线型分布情况下径向电、磁场强度及 能量沉积特性; 赵高等 [15] 通过实验研究了螺旋波 等离子体的放电特性, 获得了射频功率吸收因放电 模式转变而变化的方式.…”
unclassified