Ionospheric processes

电离层过程

• 批准号: RGPIN-2017-04891
• 负责人: StMaurice, JeanPierre
• 金额: $ 3.35万
• 依托单位: University of Saskatchewan
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2018
• 资助国家: 加拿大
• 起止时间: 2018-01-01 至 2019-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=666000
• 关键词: Ionospheric; processes

After several decades of studies our basic understanding of the ionosphere now rests on solid foundations. Nevertheless, with the constant progress in instrumental capabilities some old topics need to be revisited, not to mention that the new datasets can often reveal interesting surprises, which present new challenges. The basic reason for this state of affair is that the ionospheric plasma and the upper atmosphere/thermosphere are made of rarefied gases and often subject to strong departures from equilibrium, be it through electric field and currents, or large spatial variations in electric fields, temperatures or densities. This produces turbulence more often than not, the origin and evolution of which both need to be understood if the transport of particles momentum and energy through the system is to be properly quantified. I use observations from advanced radar systems, rockets and satellites to query the medium. From this starting point I carefully study the generation of electrical currents, the heating of both the neutral atmosphere and the ionosphere and their consequences through the generation of bulk motions and instabilities, particularly in the plasma component. My long term objective is to gain a deep understanding of the processes associated with these large departures from equilibrium. This is a challenging goal, as many of the phenomena are unpredictable (there are lots of feedback and nonlinear mechanisms involved). Specific short term objectives to be pursued with my students and collaborators are: (1) a renewed study of ion velocity distributions under large Mach number conditions. This subject is due for renewed scrutiny in view of modern radar and satellite data; (2) new linear and nonlinear theories of plasma instabilities in the lower ionosphere and in the upper mesosphere, using new insights from recent datasets; (3) using new radar systems deep in the Canadian polar cap, and Canadian satellite projects to produce a careful investigation of the plasma cusp in the ionosphere, which is the footprint of the region where the solar wind plasma becomes connected with the earth plasma. The origin of atmospheric heating in that region and the response are not well understood; (4) investigating the various responses of the high latitudes to solar wind input. This includes the production and propagation of so-called patches of ionization in the upper atmosphere, and the degree to which magnetic substorms and storms are triggered by changes in the solar wind magnetic field and dynamic pressure; (5) investigating the electrodynamics of low latitude regions both in relation to large solar wind perturbations and for much quieter conditions, which adds an interesting perspective on the whole ionosphere; (6) the study HF radio wave propagation under various conditions will also be scrutinized in order to better locate HF radar echoes, and monitor large scale ionospheric structures.

经过几十年的研究，我们现在对电离层的基本理解建立在坚实的基础上。然而，随着仪器能力的不断进步，一些旧的话题需要重新讨论，更不用说新的数据集经常会揭示出有趣的惊喜，这带来了新的挑战。这种情况的基本原因是，电离层等离子体和高层大气/热层是由稀薄气体组成的，无论是通过电场和电流，还是通过电场、温度或密度的巨大空间变化，电离层等离子体往往会严重偏离平衡。这往往会产生湍流，如果要适当地量化粒子在系统中的动量和能量传输，就需要了解湍流的起源和演化。我使用来自先进雷达系统、火箭和卫星的观测来查询介质。从这一起点出发，我仔细研究了电流的产生、中性大气和电离层的加热及其通过产生整体运动和不稳定性产生的后果，特别是在等离子体组件中。我的长期目标是深入了解与这些大规模偏离均衡相关的过程。这是一个具有挑战性的目标，因为许多现象是不可预测的(涉及到大量的反馈和非线性机制)。我的学生和合作者要追求的具体短期目标是：(1)重新研究大马赫数条件下的离子速度分布。鉴于现代雷达和卫星数据，这一课题应重新加以审查；(2)利用最近数据集的新见解，对电离层下层和中层上层的等离子体不稳定性作出新的线性和非线性理论；(3)利用加拿大极帽深处的新雷达系统，和加拿大的卫星项目，对电离层中的等离子体尖点进行仔细调查，这是太阳风等离子体与地球等离子体连接区域的足迹。该地区大气加热的来源和响应还不清楚；(4)研究高纬度对太阳风输入的各种响应。这包括：(1)研究高空大气中所谓的电离层斑块的产生和传播；(2)研究太阳风磁场和动态气压的变化引起磁亚暴和磁暴的程度；(5)研究低纬地区与太阳风大扰动和较安静条件下的电动力学，这将增加对整个电离层的有趣视角；(6)也将仔细研究各种条件下的高频无线电波传播，以便更好地定位高频雷达回波，并监测大型电离层结构。