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Quantifying the Global Spatial and Temporal Behavior of Kinetic Alfven Waves in the Auroral Zone

量化极光区动能阿尔文波的全球时空行为

基本信息

批准号：
2016788
负责人：
Andreas Keiling
金额：
$ 44.64万
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：
2020
资助国家：
美国
起止时间：
2020-05-01 至 2024-04-30
项目状态：
已结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=2016788&HistoricalAwards=false
关键词：
Quantifying Global Spatial Temporal Behavior

项目摘要

Alfven waves have been discovered in many astronomical plasmas, such as the Sun and other planets of the solar system. These are magnetohydrodynamic waves that carry energy inside the magnetosphere and energize particles. They are crucial in understanding the boundary between the magnetosphere and ionosphere and in producing the aurora. This project is a detailed study of this process which is important for predicting and preparing for space weather effects. Graduate students will also be supported in research.This project studies the role of kinetic Alfven waves (KAW) in magnetosphere-ionosphere coupling. The work will focus on a statistical, observational study of multi-year satellite data using superposed epoch analysis, substorm onset lists, and geomagnetic indices for relating the observations to specific geomagnetic conditions. The goals are to answer the following: (1) What is the global spatial distribution and total power of KAW above the auroral acceleration region (AAR) under various geomagnetic conditions (AE index, substorm, storm)? (2) What is the temporal evolution of the global distribution and total power of KAW during different phases of substorms and storms and as a function of time? (3) What is the contribution of KAW to the Alfven wave budget (including MHD regime)? (4) What is their significance in the M-I coupling above the AAR in relation to Alfvenic observations below the AAR and from the generator region?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.

阿尔文波在许多天文等离子体中被发现，例如太阳和太阳系的其他行星。这些是磁流体动力学波，在磁层内携带能量并为粒子提供能量。它们对于理解磁层和电离层之间的边界以及产生极光至关重要。该项目是对这一过程的详细研究，这对于预测空间气象影响并做好准备非常重要。研究生也将在研究中得到支持。本项目研究动力阿尔芬波（KAW）在磁层-电离层耦合中的作用。这项工作将侧重于对多年卫星数据进行统计和观测研究，利用叠加历元分析、亚暴开始列表和地磁指数将观测结果与特定的地磁条件联系起来。（1）在不同的地磁条件下（AE指数、亚暴、暴），极光加速区（AAR）上空KAW的全球空间分布和总功率是多少？(2)在亚暴和风暴的不同阶段，KAW的全球分布和总功率随时间的变化是什么？(3)KAW对阿尔芬波收支（包括MHD区）的贡献是什么？(4)它们在AAR以上的M-I耦合中与AAR以下和发生器区的阿尔文观测的关系有什么意义？该奖项反映了NSF的法定使命，并被认为是值得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的支持。