Density Troughs in the Ionosphere Sustained by Transport Barriers

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
M. A. Malkov, V. I. Sotnikov, E. V. Mishin
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Abstract

This study explores the relaxation and sustainability of density irregularities and plasma flows in the Earth's ionosphere. To do this, we use a modified model of drift-wave turbulence known as the Hasegawa-Wakatani model. Similar to turbulent processes in laboratory plasmas, we explore a powerful mechanism that can reduce the turbulent plasma transport. This mechanism is associated with the creation of “zonal flows,” cutting across the gradients of particle density and magnetic fields. They work effectively to minimize particles' random movement and reduce the turbulence causing this movement. The zonal flows create transport barriers in areas where the density gradient is steepest and where drift waves grow most vigorously. The transport barriers significantly delay the refill of low-density regions with surrounding plasma. They also lead to changes in the electric potential of the plasma and influence the movement of ions in the direction of the magnetic field. Our research investigates how these zonal flows are generated and how effectively they sustain density irregularities. We also examine the spectral characteristics of turbulence in and around these barriers.

由传输屏障维持的电离层密度波谷
本研究探讨了地球电离层中密度不规则性和等离子体流的松弛和可持续性。为了做到这一点,我们使用了一种改进的漂波湍流模型,即Hasegawa-Wakatani模型。与实验室等离子体中的湍流过程类似,我们探索了一种能够减少等离子体湍流输运的强大机制。这种机制与“纬向流”的产生有关,纬向流穿过粒子密度和磁场的梯度。它们有效地减少了粒子的随机运动,减少了引起这种运动的湍流。纬向流在密度梯度最陡和漂波增长最剧烈的地区造成了运输障碍。传输障碍显著地延迟了低密度区域与周围等离子体的再填充。它们还会导致等离子体电势的变化,并影响离子在磁场方向上的运动。我们的研究调查了这些纬向流动是如何产生的,以及它们如何有效地维持密度不规则性。我们还研究了这些屏障内部和周围湍流的光谱特征。
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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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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