The challenge to understand the zoo of particle transport regimes during resonant wave-particle interactions for given survey-mode wave spectra

Oliver Allanson, Donglai Ma, Adnane Osmane, Jay M. Albert, Jacob Bortnik, Clare E. J. Watt, Sandra C. Chapman, Joseph Spencer, Daniel J. Ratliff, Nigel P. Meredith, Thomas Elsden, Thomas Neukirch, David P. Hartley, Rachel Black, N. Watkins, S. Elvidge
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Abstract

Quasilinear theories have been shown to well describe a range of transport phenomena in magnetospheric, space, astrophysical and laboratory plasma “weak turbulence” scenarios. It is well known that the resonant diffusion quasilinear theory for the case of a uniform background field may formally describe particle dynamics when the electromagnetic wave amplitude and growth rates are sufficiently “small”, and the bandwidth is sufficiently “large”. However, it is important to note that for a given wave spectrum that would be expected to give rise to quasilinear transport, the quasilinear theory may indeed apply for given range of resonant pitch-angles and energies, but may not apply for some smaller, or larger, values of resonant pitch-angle and energy. That is to say that the applicability of the quasilinear theory can be pitch-angle dependent, even in the case of a uniform background magnetic field. If indeed the quasilinear theory does apply, the motion of particles with different pitch-angles are still characterised by different timescales. Using a high-performance test-particle code, we present a detailed analysis of the applicability of quasilinear theory to a range of different wave spectra that would otherwise “appear quasilinear” if presented by e.g., satellite survey-mode data. We present these analyses as a function of wave amplitude, wave coherence and resonant particle velocities (energies and pitch-angles), and contextualise the results using theory of resonant overlap and small amplitude criteria. In doing so, we identify and classify five different transport regimes that are a function of particle pitch-angle. The results in our paper demonstrate that there can be a significant variety of particle responses (as a function of pitch-angle) for very similar looking survey-mode electromagnetic wave products, even if they appear to satisfy all appropriate quasilinear criteria. In recent years there have been a sequence of very interesting and important results in this domain, and we argue in favour of continuing efforts on: (i) the development of new transport theories to understand the importance of these, and other, diverse electron responses; (ii) which are informed by statistical analyses of the relationship between burst- and survey-mode spacecraft data.
了解给定勘测模式波谱的共振波-粒子相互作用过程中的粒子输运机制动物园所面临的挑战
准线性理论已被证明能够很好地描述磁层、空间、天体物理和实验室等离子体 "弱湍流 "情况下的一系列传输现象。众所周知,当电磁波振幅和增长率足够 "小"、带宽足够 "大 "时,均匀背景场情况下的共振扩散准线性理论可以正式描述粒子动力学。然而,需要注意的是,对于预期会产生准线性传输的给定波谱,准线性理论可能确实适用于给定范围的共振俯仰角和能量,但可能不适用于一些较小或较大的共振俯仰角和能量值。也就是说,即使在背景磁场均匀的情况下,准线性理论的适用性也可能与螺距角有关。如果准线性理论确实适用,那么不同螺距角的粒子运动仍然具有不同的时间尺度。我们使用高性能的测试粒子代码,详细分析了类线性理论对一系列不同波谱的适用性,这些波谱在卫星勘测模式数据等呈现的情况下 "看起来是类线性的"。我们将这些分析作为波幅、波相干性和共振粒子速度(能量和俯仰角)的函数,并利用共振重叠理论和小振幅标准对结果进行背景分析。在此过程中,我们识别并划分出了与粒子俯仰角相关的五种不同的传输机制。我们论文中的结果表明,对于外观非常相似的勘测模式电磁波产品,即使它们似乎满足所有适当的准线性标准,也可能存在种类繁多的粒子响应(作为俯仰角的函数)。近年来,在这一领域取得了一系列非常有趣和重要的成果,我们主张在以下方面继续努力:(i)发展新的传输理论,以了解这些以及其他各种电子响应的重要性;(ii)通过对爆发模式和巡天模式航天器数据之间关系的统计分析来了解这些响应。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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