您的位置: 专家智库 > >

国家自然科学基金(41204114)

作品数:3 被引量:0H指数:0
相关作者:危达周庆华更多>>
相关机构:长沙理工大学更多>>
发文基金:国家自然科学基金更多>>
相关领域:理学天文地球更多>>

文献类型

  • 3篇中文期刊文章

领域

  • 2篇理学
  • 1篇天文地球

主题

  • 1篇带电
  • 1篇带电粒子
  • 1篇地球
  • 1篇地球磁层
  • 1篇地球磁场
  • 1篇电粒子
  • 1篇投掷
  • 1篇漂移
  • 1篇STUDY
  • 1篇BI
  • 1篇CLUSTE...
  • 1篇EVOLUT...
  • 1篇FREQUE...
  • 1篇HIS
  • 1篇MAGNET...
  • 1篇MODELI...
  • 1篇磁层
  • 1篇ION
  • 1篇CHORUS
  • 1篇ELECTR...

机构

  • 1篇长沙理工大学

作者

  • 1篇周庆华
  • 1篇危达

传媒

  • 2篇Plasma...
  • 1篇长沙理工大学...

年份

  • 3篇2014
3 条 记 录,以下是 1-3
排序方式:
地球磁场中任意投掷角的带电粒子运动轨迹
2014年
磁暴和亚暴过程中等离子体片带电粒子的注入严重影响了地球空间环境,导致环电流的增强或衰减,形成质子极光,影响中高层大气的物理化学过程。本研究利用UBK方法计算了穿越子夜(MLT=0)不同能量和投掷角的质子和电子漂移轨道,分析了粒子的来源区域和后续轨道特征。研究结果表明,穿过L=7的投掷角为90°的质子,能量低于~2keV时会逆时针绕地球作漂移运动,能量高于~4keV时则会顺时针绕地球作漂移运动。能量高于15keV的质子的漂移轨道形成闭合轨道。穿过L=7的投掷角为90°的电子均绕地球逆时针漂移,且能量高于5keV时形成闭合轨道。穿过L=4的质子,除了10keV左右的质子,轨道都呈现闭合状态,说明从等离子片来的10keV左右的质子可以更靠近地球;穿过L=4的电子都处在闭合轨道上。投掷角越小的质子越偏向于向晨侧运动,能量越高的质子受投掷角变化影响越小,投掷角的变化对电子的轨道几乎没有影响。Kp指数较大时,粒子的运动方向随能量变化不明显,但是轨道更难闭合,并更接近地球。
危达高中磊周庆华
关键词:地球磁层
Modeling the Evolution of Chorus Waves into Hiss Waves in the Magnetosphere
2014年
In this study, we analyze Cluster observations of whistler-mode chorus and hiss waves during the event of August 19-21, 2006. Chorus is present outside the plasmasphere and hiss occurs inside the plasmasphere. Using a recently constructed plasma boundary layer model, we perform a ray-tracing study on the propagation of chorus. Numerical results show that chorus can penetrate into the plasmasphere through the plasma boundary layer, evolving into hiss. The current data analysis and modeling provide a further observational support for the previous findings that chorus is the origin of plasmaspheric hiss.
贺艺华周庆华杨昶周晓萍刘斯唐立军肖伏良
关键词:CHORUS
Ray Tracing Study of Electromagnetic Ion Cyclotron Waves Associated with Bi-Ion Frequencies
2014年
Ray tracing study of electromagnetic ion cyclotron (EMIC) waves is conducted based on a realistic plasma density model. The simulation result shows that EMIC waves propagate away from the equatorial source region to higher latitudes basically along geomagnetic field lines, and are reflected at the region where their frequency matches the local bi-ion frequency. H+ band suffers H+-He+ bi-ion frequency reflection at lower latitudes, whereas He+ band suffers He+-O+ bi-ion frequency reflection at higher latitudes. Moreover, the concentration of heavy ions slightly affects the bi-ion frequencies and then slightly determines the reflection location of ray paths of EMIC waves. The current results present the first detailed study on the propagation characteristics of EMIC waves associated with bi-ion frequencies.
周庆华杨昶贺艺华刘斯周晓萍唐立军肖伏良
共1页<1>
聚类工具0