Progress in Numerical and Laboratory Simulations of Ionospheric Irregularities
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摘要: 电离层中存在着从厘米至上百千米特征尺度的等离子体密度不规则体. 这些不规则体对穿过其传播的无线电波会造成信号相位与幅度的快速起伏、衰落与散射, 因此电离层不规则体对无线电波传播特性有重要影响. 按纬度分布,电离层不规则体可划分为赤道与低纬电离层不规则体、中纬电离层不规则体及极区电离层不规则体. 过去几十年, 电离层不规则体结构的探测、时空分布特征与理论方面的研究均取得长足进展, 其中北京大学肖佐教授团队在电离层不规则体的探测、理论模式以及装置模拟方面开展了先驱性的工作. 本文主要梳理中国科学技术大学电离层研究团队近年来在电离层不规则体模拟领域取得的部分研究进展,包括地球赤道/低纬、中纬和高纬度电离层不规则体模拟研究, 以及针对部分电离等离子体不稳定性的电离层实验室模拟. 这些方面的工作利用高性能数值模型与空间环境实验室模拟装置, 系统地揭示了中低纬电离层不规则体的形成与演化机制, 为相关物理机理的深入研究提供了重要的依据.Abstract: The ionosphere contains plasma density irregularities with characteristic scales ranging from centimeters to hundreds of kilometers. These irregularities can induce rapid fluctuations, fading, and scattering in the phase and amplitude of radio waves propagating through the ionospheric medium, thereby having a significant impact on radio wave propagation characteristics. According to their latitudinal distribution, ionospheric irregularities are categorized into equatorial and low-latitude, mid-latitude, and polar types. Over the years, great progress has been achieved in both the observational and theoretical aspects of the characteristics of the ionospheric irregularities. Notably, the research group led by Professor Zuo Xiao of Peking University has carried out pioneering work in the observation, theoretical modeling, and even laboratory experiments of ionospheric irregularities. This article reviews the recent research progress made by the team of the School of Earth and Space Sciences, University of Science and Technology of China in the field of ionospheric irregularity simulations. The main topics cover numerical simulation studies of the terrestrial ionospheric irregularities at low, middle and high latitudinal zones and laboratory experiments of ionospheric plasma instabilities under partially ionized conditions. These studies systematically reveal the formation and evolution mechanisms of ionospheric irregularities in the middle and low latitudes, providing powerful tools for further investigation of related physical mechanisms.
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Key words:
- Ionosphere /
- Ionospheric irregularities /
- Numerical simulation /
- Laboratory simulation
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图 1 环形对流测试的初始条件和t=1时使用不同对流方法的结果[13]. (a) t=0时256×256个笛卡尔网格上的开槽圆盘状初始密度分布及绕模拟区域中心顺时针旋转的速度场, (b)~(g) t=1时(绕中心旋转一周)使用不同对流方法计算得到的密度分布
Figure 1. Initial condition of the circular advection test and results at t = 1 using different advection schemes, and the colormap represents the density distribution of the advection test. (a) Initial distribution of a slotted cylinder in Cartesian geometry with 256 × 256 cells at t=0; (b)~(g) simulated density distributions at t=1 s by different schemes
图 2 采用不同PDM参数α取值的电离层不规则体二维模拟结果[13]
Figure 2. Simulated plasma density distribution in ESF with four values for different PDM parameter $ \alpha $
图 5 地磁平静时期t = 0 s, 1200 s, 2400 s 和3600 s时, 积分等离子体密度$ N\text{(a)~(d)} $及扰动等离子体密度$ \delta N $相对于背景积分等离子体密度$ {N}_{0} $的百分比(e)~(h) [17]
Figure 5. Integrated plasma density $ N $ (a)~(d) and the percentage change of perturbed plasma density $ \delta N $ with respect to the initial plasma density $ {N}_{0} $ (e)~(h) at t=0 s,1200 s, 2400 s and 3600 s during geomagnetically quiet condition [17]
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雷久侯 现为中国科学技术大学地球和空间科学学院讲席教授, 博士生导师, 主要研究方向为高层大气和电离层物理. E-mail:
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