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
基本信息
- 批准号:1902699
- 负责人:
- 金额:$ 24.24万
- 依托单位:
- 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 2022-05-31
- 项目状态:已结题
- 来源:
- 关键词:
项目摘要
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理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中,有各种各样的机制可以加速电子。该项目将有助于区分这些理论,以帮助确定哪些在磁层中起作用。这与国家空间气象计划直接相关,因为这项工作可导致更好的空间气象模型和预报,这影响到国家商业和国防卫星以及天基通信。本研究将量化电子热各向异性对磁尾电流片结构的影响,并探讨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负责产生强电流(由粒子曲率漂移引起),并且可以用作各种电磁波发射的能量源。该项目使用了五个航天器任务(Geotail、Cluster、THEMIS、ARTEMIS和MMS)的观测结果,覆盖了从10到80个地球半径的径向距离内的整个磁尾。利用THEMIS/ARTEMIS在近地和中磁尾的多年观测资料,研究了不同磁尾构型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,利用MMS观测和高分辨率等离子体测量,这项工作将首次从统计学上揭示电子各向异性总体的精细结构及其对电流密度的贡献。该奖项反映了NSF的法定使命,并通过使用基金会的知识价值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
期刊论文数量(7)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
Superthin current sheets supported by anisotropic electrons
- DOI:10.1063/5.0018063
- 发表时间:2020-08
- 期刊:
- 影响因子:2.2
- 作者:S. Kamaletdinov;E. Yushkov;A. Artemyev;Alexander Lukin;I. Vasko
- 通讯作者:S. Kamaletdinov;E. Yushkov;A. Artemyev;Alexander Lukin;I. Vasko
Contribution of Anisotropic Electron Current to the Magnetotail Current Sheet as a Function of Location and Plasma Conditions
- DOI:10.1029/2019ja027251
- 发表时间:2020-01
- 期刊:
- 影响因子:0
- 作者:A. Artemyev;V. Angelopoulos;I. Vasko;A. Petrukovich;A. Runov;Y. Saito;L. Avanov;B. Giles;C. Russell;R. Strangeway
- 通讯作者:A. Artemyev;V. Angelopoulos;I. Vasko;A. Petrukovich;A. Runov;Y. Saito;L. Avanov;B. Giles;C. Russell;R. Strangeway
Beam-driven ECH waves: A parametric study
- DOI:10.1063/5.0053187
- 发表时间:2021-04
- 期刊:
- 影响因子:2.2
- 作者:Xu Zhang;V. Angelopoulos;A. Artemyev;Xiao‐jia Zhang
- 通讯作者:Xu Zhang;V. Angelopoulos;A. Artemyev;Xiao‐jia Zhang
Evolution of Thermal Electron Distributions in the Magnetotail: Convective Heating and Scattering‐Induced Losses
磁尾中热电子分布的演变:对流加热和散射——引起的损失
- DOI:10.1029/2021ja029952
- 发表时间:2021
- 期刊:
- 影响因子:0
- 作者:Shustov, P. I.;Lukin, A. S.;Zhang, X. ‐J.;Artemyev, A. V.;Petrukovich, A. A.;Angelopoulos, V.
- 通讯作者:Angelopoulos, V.
Realistic Electron Diffusion Rates and Lifetimes Due to Scattering by Electron Holes
- DOI:10.1029/2021ja029380
- 发表时间:2021-08
- 期刊:
- 影响因子:0
- 作者:Yangyang Shen;I. Vasko;A. Artemyev;D. Malaspina;X. Chu;V. Angelopoulos;Xiao‐jia Zhang
- 通讯作者:Yangyang Shen;I. Vasko;A. Artemyev;D. Malaspina;X. Chu;V. Angelopoulos;Xiao‐jia Zhang
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Anton Artemev其他文献
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{{ truncateString('Anton Artemev', 18)}}的其他基金
Collaborative Research: GEM--Multi-harmonic Whistler Waves, Their Origin and Contribution to Electron Scattering
合作研究:GEM——多谐波惠斯勒波、它们的起源及其对电子散射的贡献
- 批准号:
2026375 - 财政年份:2020
- 资助金额:
$ 24.24万 - 项目类别:
Standard Grant
Collaborative Research: Quantifying the Effects of Nonlinear Wave-particle Interaction in the Inner Magnetosphere
合作研究:量化内磁层非线性波粒相互作用的影响
- 批准号:
1914594 - 财政年份:2019
- 资助金额:
$ 24.24万 - 项目类别:
Standard Grant
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