Probing the Dynamic Ionosphere: A Multifaceted Approach

探测动态电离层：多方面的方法

• 批准号: RGPIN-2017-04857
• 负责人: Knudsen, David
• 金额: $ 2.62万
• 依托单位: University of Calgary
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2020
• 资助国家: 加拿大
• 起止时间: 2020-01-01 至 2021-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=711266
• 关键词: Probing; Dynamic; Ionosphere; Multifaceted; Approach

More than just a beautiful sight, the aurora is the visible manifestation of massive electric currents that thread near-Earth space and inject billions of Watts of electrical power into our upper atmosphere. The aurora affects our atmosphere and possibly our climate, and provides a ringside view of fundamental plasma processes that pervade the universe. It can also pose a threat to technology in space and on the ground. Popular articles and even astronomy textbooks tend to give an oversimplified explanation of the aurora in terms of charged particles from the solar wind “captured” by Earth's magnetic field and channeled to the magnetic poles. In reality the connection between the solar wind and the aurora is more complex, and much more interesting. For example, auroral electrons are accelerated to energies 1000 times larger than those in the solar wind, a fact that cannot be explained by a magnetic field alone. Furthermore, the most intense auroras draw electrons from a source deep in the magnetosphere, with no direct access to the solar wind. Most importantly, the simple explanation misses the point that the aurora is fundamentally part of an electric circuit, powered by a magneto-hydrodynamic dynamo formed from the interaction of the fast-flowing solar wind with the geomagnetic field. This proposal is aimed at resolving key questions pertaining to formation of the aurora, and more generally to sources structure and variability of Earth's ionosphere by taking advantage of a rich and timely opportunity made possible by Canadian leadership in an unprecedented array of space and ground-based instrumentation. Foremost for this project are the Electric Field Instruments (EFIs) on the European Space Agency's Swarm satellites, launched in November 2013. These instruments were developed at the University of Calgary in collaboration with Canadian industrial partner COM DEV International (now Honeywell) and the Swedish Institute for Space Physics. Electric field estimates are derived from low-energy plasma measurements that include ion flow velocity, plasma density, and temperature. Combining these with state-of-the-art magnetic field measurements, Swarm is currently carrying out a precision, long-term, multi-point, pole-to-pole survey of the electrodynamic behavior and plasma properties of the ionosphere. Although Swarm itself has no direct measurements of auroral light nor the energized electrons that cause it, we are able to obtain this information separately through an array of white-light all-sky cameras deployed across the Canadian Arctic as part of the NASA/CSA THEMIS ground-based observatory chain, and soon through the new TREx (Transition Region Explorer) multi-wavelength array, both made possible through a collaboration with the auroral imaging group at the University of Calgary.

极光不仅仅是一幅美丽的景象，它还是巨大电流的可见表现，这些电流流经近地空间，向我们的高层大气注入数十亿瓦的电力。极光影响我们的大气层，可能还影响我们的气候，并提供了弥漫在宇宙中的基本等离子体过程的环边视图。它还可能对太空和地面技术构成威胁。 流行的文章甚至天文学教科书都倾向于用被地球磁场捕获并输送到磁极的太阳风中的带电粒子来过于简单化地解释极光。事实上，太阳风和极光之间的联系要复杂得多，也有趣得多。例如，极光电子被加速到比太阳风中的电子大1000倍的能量，这一事实不能仅用磁场来解释。此外，最强烈的极光从磁层深处的来源吸收电子，而不直接接触太阳风。最重要的是，这种简单的解释忽略了一点，即极光基本上是电路的一部分，由快速流动的太阳风与地磁场相互作用形成的磁流体发电机提供动力。 这项提议旨在利用加拿大在一系列史无前例的空间和地面仪器方面提供的丰富和及时的机会，解决与极光的形成有关的关键问题，并更广泛地解决地球电离层的来源、结构和可变性问题。该项目最重要的是2013年11月发射的欧洲航天局SARM卫星上的电场仪器(EFIS)。这些仪器是卡尔加里大学与加拿大工业伙伴COM DEV International(现为霍尼韦尔)和瑞典空间物理研究所合作开发的。电场估计是从包括离子流动速度、等离子体密度和温度在内的低能等离子体测量得出的。结合最先进的磁场测量，斯沃姆目前正在对电离层的电动力学行为和等离子体特性进行精确的、长期的、多点的、从极到极的测量。虽然Spot本身没有对极光的直接测量，也没有对引起极光的带电电子进行直接测量，但我们能够通过作为NASA/CSA THEMIS地面观测台链的一部分在加拿大北极部署的白光全天相机阵列单独获取这种信息，并且很快通过新的Trex(过渡区探测器)多波长阵列获取这种信息，这两种阵列都是通过与卡尔加里大学的极光成像小组合作实现的。