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Hybrid code simulation of electromagnetic ion cyclotron waves in curvilinear coordinates.

机译:曲线坐标中电磁离子回旋波的混合编码模拟。

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摘要

Electromagnetic ion cyclotron waves, a common feature in the Earth' magnetosphere, can interact with both ions and electrons, leading to an important impact on the dynamics in the radiation belts. These waves are usually driven by the anisotropic and hot ring current protons in the equatorial region, and propagate earthward along the Earth's (nearly dipolar) magnetic field lines. When the waves grow near the equator, they are dominantly left-hand polarized and have small wave normal angle. The inhomogeneity of the magnetic field stretches the wave fronts and causes refraction. While propagating toward high latitudes, the waves become linearly or right-handed polarized with a larger normal angle due to the refraction. If the waves are refracted enough, then they may encounter the bi-ion frequency and reflect; if the waves are not refracted as much, they are reflected at a cutoff frequency lower than the bi-ion frequency. Different wave modes may couple during the course of propagation due to mode conversion, which indicates that some waves may tunnel through the so called stop band to reach frequencies very close to the harmonic of the ion cyclotron frequency, leading to acceleration of the ions. This is a complex process in which a variety of phenomena, including the generation, growth, propagation, reflection, absorption, and coupling of the EMIC waves, may occur. We have developed a nonliner hybrid code using curvilinear coordinates to investigate the EMIC waves in a dipole magnetic field, capable of addressing all of the above issues self-consistently. Both single-ion and multi-ion plasmas are investigated. In the presence of cold heavy ions, such as He+ and O+, the waves are able to accelerate these cold particles at multiple harmonics of the cyclotron resonances, and in some cases the heating is significant so that the cold particles become hot.
机译:电磁离子回旋波是地球磁层的共同特征,可以与离子和电子相互作用,从而对辐射带的动力学产生重要影响。这些波通常由赤道区域的各向异性和热环电流质子驱动,并沿着地球(近乎偶极)的磁力线向地球传播。当波在赤道附近生长时,它们主要是左旋极化的并且具有小的波法向角。磁场的不均匀性会拉伸波前并引起折射。在向高纬度传播时,由于折射,这些波以较大的法线角变为线性或右旋偏振。如果波被充分折射,则它们可能会遇到双离子频率并反射;如果波没有被折射得太多,它们会以低于双离子频率的截止频率被反射。由于模式转换,不同的波模式可能会在传播过程中耦合,这表明某些波可能会穿过所谓的阻带,从而到达非常接近离子回旋加速器频率谐波的频率,从而导致离子加速。这是一个复杂的过程,其中可能发生多种现象,包括EMIC波的产生,生长,传播,反射,吸收和耦合。我们已经开发了一种使用曲线坐标的非线性混合代码,以研究偶极磁场中的EMIC波,能够自洽地解决所有上述问题。研究了单离子和多离子等离子体。在冷重离子(例如He +和O +)的存在下,波能够以回旋加速器共振的多个谐波加速这些冷粒子,并且在某些情况下,加热非常重要,因此冷粒子变得很热。

著录项

  • 作者

    Hu, Yonggang.;

  • 作者单位

    Dartmouth College.;

  • 授予单位 Dartmouth College.;
  • 学科 Atmospheric Sciences.;Physics Fluid and Plasma.
  • 学位 Ph.D.
  • 年度 2010
  • 页码 150 p.
  • 总页数 150
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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