Collaborative Research: GEM--Thermal Electron Anisotropy in the Earth's Magnetotail

合作研究：GEM--地球磁尾的热电子各向异性

• 批准号: 1902684
• 负责人: Ivan Vasko
• 金额: $ 21万
• 依托单位: University of California-Berkeley
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-06-01 至 2022-12-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1902684&HistoricalAwards=false
• 关键词: Collaborative; Research; GEM; Thermal; Electron

One of the most important problems of space plasma physics is understanding how high-energy charged particles are generated. There are a huge variety of mechanisms suggested for accelerating electrons in the region of the geomagnetic field known as the current sheet. This project will help distinguish between these theories to help determine which are at work in the magnetosphere. This is directly relevant to the National Space Weather Plan, since the work can lead to better models and forecasts of space weather, which affects national commercial and defense satellites and space-based communications. Additionally, graduate and undergraduate students will participate in the research.This project quantifies the impact of the electron thermal anisotropy on the magnetotail current sheet structure and investigates the variation of characteristics of electron thermal anisotropy with geomagnetic activity. The anisotropic electron population can be responsible for generation of strong currents (induced by particle curvature drifts) and can serve as an energy source for various electromagnetic wave emissions. The project uses observations from five spacecraft missions (Geotail, Cluster, THEMIS, ARTEMIS, and MMS) covering the entire magnetotail within the radial distances from 10 to 80 Earth radii downtail. Using several years of THEMIS/ARTEMIS observations in the near-Earth and middle magnetotail, the work studies both the radial distribution of the electron thermal anisotropy and the impact of electron anisotropic currents on current sheet structure for different magnetotail configurations. Moreover, using MMS observations with the high-resolution plasma measurements the work will for the first time statistically reveal the fine structure of the electron anisotropic population and its contribution to the current density.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

空间等离子体物理学最重要的问题之一是了解高能带电粒子是如何产生的。在被称为电流片的地磁场区域，有各种各样的机制被认为可以加速电子。该项目将有助于区分这些理论，以帮助确定哪些理论在磁层中起作用。这与国家空间天气计划直接相关，因为这项工作可以带来更好的空间天气模型和预报，这会影响国家商业和国防卫星以及天基通信。此外，研究生和本科生将参与研究。本项目量化了电子热各向异性对磁尾电流片结构的影响，并研究了电子热各向异性特征随地磁活动的变化。各向异性电子布居可以产生强电流(由粒子曲率漂移引起)，并且可以作为各种电磁波发射的能源。该项目使用了来自五个航天器飞行任务(GeoTail、星团、THEMIS、Artemis和MMS)的观测，覆盖了从地球半径10到80个地球半径向下的径向距离内的整个磁尾。利用THEMIS/ARTEMIS对近地磁尾和中磁尾多年的观测，研究了不同磁尾结构下电子热各向异性的径向分布以及电子各向异性电流对电流片结构的影响。此外，使用MMS观测和高分辨率等离子体测量，这项工作将首次从统计上揭示电子各向异性群体的精细结构及其对当前密度的贡献。这一奖项反映了NSF的法定使命，并通过使用基金会的智力优势和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

Electrostatic Solitary Waves in the Earth's Bow Shock: Nature, Properties, Lifetimes, and Origin

地球弓激波中的静电孤立波：性质、特性、寿命和起源

• DOI: 10.1029/2021ja029357
• 发表时间: 2021
• 期刊: Journal of Geophysical Research: Space Physics
• 作者: Wang, R.;Vasko, I. Y.;Mozer, F. S.;Bale, S. D.;Kuzichev, I. V.;Artemyev, A. V.;Steinvall, K.;Ergun, R.;Giles, B.;Khotyaintsev, Y.
• 通讯作者: Khotyaintsev, Y.

Kinetic-scale Current Sheets in the Solar Wind at 1 au: Properties and the Necessary Condition for Reconnection

1 au 太阳风中的动能尺度电流片：特性和重新连接的必要条件

• DOI: 10.3847/2041-8213/ac3f30
• 发表时间: 2021
• 期刊: The Astrophysical Journal Letters
• 作者: Vasko, I. Y.;Alimov, K.;Phan, T. D.;Bale, S. D.;Mozer, F. S.;Artemyev, A. V.
• 通讯作者: Artemyev, A. V.

Configuration of the Earth’s Magnetotail Current Sheet

• DOI: 10.1029/2020gl092153
• 发表时间: 2021-03
• 期刊: Geophysical Research Letters
• 影响因子: 5.2
• 作者: A. Artemyev;San Lu;M. El‐Alaoui;Yu Lin;V. Angelopoulos;Xiao‐jia Zhang;A. Runov;I. Vasko;L. Zelenyi;C. Russell