期刊论文

Xiao FuLiang

英文

中国科学：信息科学(英文版)

1674-733X

2012

55

11

2624-2634

10.1007/s11432-012-4698-0

Acknowledgements This work was supported by National Natural Science Foundation of China （Grant No. 41274165）, Aid Program for Science and Technology Innovative Research Team in Higher Educational Institutions of Hunan Province, and Construct Program of the Key Discipline in Hunan Province, and Open Research Program from Key Laboratory of Basic Plasma Physics, Chinese Academy of Sciences.

本校为第一且通讯机构

The contributions of dayside and nightside gyroresonance of chorus waves to electron radiation belt evolution at L = 6.6 are detailedly differentiated via fully solving the two-dimensional Fokker-Plank equation. The numerical results show that the chorus waves at different regions play significantly different roles. The dayside chorus waves can cause obvious loss of energetic electrons at lower pitch angles and weak energization at larger pitch angles. The nightside chorus waves can yield significant energization at larger pitch angles, but cannot efficiently resonate with the energetic electr...

行星的光面的贡献和合唱团的夜面 gyroresonance 在 L = 向电子放射带进化招手 6.6 详细地经由充分解决二维的佛克板方程被区分。数字结果证明在不同区域的合唱团波浪起显著地不同的作用。行星的光面合唱团波浪能在更低的沥青角度和更全体的弱 energization 引起精力充沛的电子的明显的损失沥青角度。夜面合唱团波浪能产出更全体的重要 energization 搭角度，但是不能高效地在更低的沥青与精力充沛的电子共振角度。由于在充分解决佛克普朗克常数方程的数字困难，生气散开术语经常在以前的工作被忽略。这里，在不同区域的生气散开的效果进一步被分析。在行星的光面上，忽略生气散开在更低的沥青角...