题名 | Equatorial Propagation of the Magnetosonic Mode Across the Plasmapause: 2-D PIC Simulations |
作者 | |
通讯作者 | Min, Kyungguk |
发表日期 | 2019-06
|
DOI | |
发表期刊 | |
ISSN | 2169-9380
|
EISSN | 2169-9402
|
卷号 | 124期号:6页码:4424-4444 |
摘要 | Recent studies have indicated that fast magnetosonic waves (also referred to as equatorial noise) excited far outside the plasmapause cannot propagate deep into the plasmasphere because of the preferential azimuthal propagation of the waves at the source region. Since conditions in the low-density plasma trough are typically favorable for the wave excitation, one possible explanation for the magnetosonic wave origin inside the plasmapause is refraction of the waves excited in the plasma trough but close to the plasmapause. In this study, two-dimensional particle-in-cell (PIC) simulations are carried out at the dipole magnetic equator to investigate the self-consistent excitation and propagation of magnetosonic waves across the steep plasmapause density gradient. The simulations show that the magnetosonic waves grow outside the plasmapause and propagate predominantly in the azimuthal direction. However, the waves excited close to the plasmapause experience refraction toward the density gradient, allowing them to cross the plasmapause and then propagate dominantly toward the Earth. The amount of refraction is in good agreement with a theoretical prediction based on the geometric optic approximation. We find that the refraction at the plasmapause can redirect magnetosonic waves toward the Earth, but an additional mechanism is needed to account for the statistical properties of the wave electric field polarization reported in the plasmasphere. |
相关链接 | [来源记录] |
收录类别 | |
语种 | 英语
|
学校署名 | 其他
|
资助项目 | NASA[NAS5-01072]
|
WOS研究方向 | Astronomy & Astrophysics
|
WOS类目 | Astronomy & Astrophysics
|
WOS记录号 | WOS:000477723100038
|
出版者 | |
ESI学科分类 | SPACE SCIENCE
|
来源库 | Web of Science
|
引用统计 |
被引频次[WOS]:12
|
成果类型 | 期刊论文 |
条目标识符 | http://sustech.caswiz.com/handle/2SGJ60CL/25840 |
专题 | 理学院_地球与空间科学系 |
作者单位 | 1.Korea Astron & Space Sci Inst, Daejeon, South Korea 2.Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic 3.Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen, Peoples R China 4.Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA 5.NASA, GSFC, Greenbelt, MD USA 6.Univ Maryland Baltimore Cty, Goddard Planetary Heliophys Inst, Catonsville, MD USA |
推荐引用方式 GB/T 7714 |
Min, Kyungguk,Nemec, Frantisek,Liu, Kaijun,et al. Equatorial Propagation of the Magnetosonic Mode Across the Plasmapause: 2-D PIC Simulations[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2019,124(6):4424-4444.
|
APA |
Min, Kyungguk,Nemec, Frantisek,Liu, Kaijun,Denton, Richard E.,&Boardsen, Scott A..(2019).Equatorial Propagation of the Magnetosonic Mode Across the Plasmapause: 2-D PIC Simulations.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,124(6),4424-4444.
|
MLA |
Min, Kyungguk,et al."Equatorial Propagation of the Magnetosonic Mode Across the Plasmapause: 2-D PIC Simulations".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 124.6(2019):4424-4444.
|
条目包含的文件 | 条目无相关文件。 |
|
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。
修改评论