Space Plasma Transport by Kinetic Alfven Waves

阿尔文运动波的空间等离子体传输

• 批准号: 0612614
• 负责人: Christopher Chaston
• 金额: $ 22万
• 依托单位: University of California-Berkeley
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2006
• 资助国家: 美国
• 起止时间: 2006-09-15 至 2011-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0612614&HistoricalAwards=false
• 关键词: Space; Plasma; Transport; Kinetic; Alfven

This project will asses the ability of the kinetic Alfven waves to transport shocked solar wind (magnetosheath) plasmas across the outer boundary of the Earth's magnetic field (magnetosphere) known as the magnetopause. Classically this boundary should be impenetrable with magnetosheath plasma penetrating not more than a gyro-radius into the Earth's magnetosphere. However in-situ observations show penetration over widths of 10s of gyro-radii and indeed much of the plasma of the Earth's magnetosphere is populated by magnetosheath plasmas. Significantly, the boundary layer at the magnetopause where magnetosheath and magnetospheric plasma mix is invariably filled with low frequency electromagnetic fluctuations. It has been suggested that these waves are kinetic Alfven waves. Theoretical studies have suggested that kinetic Alfven waves may be effective in transporting plasmas across magnetic fields. This project will use multi-point fields and plasma observations from the Cluster spacecraft at the magnetopause to identify the waves that are present and evaluate their ability to account for plasma transport seen there. Although the project is specifically directed at plasma transport at Earth's magnetopause, the problem is central to plasma transport in many physical situations, including in magnetic loops on the sun and plasma transport in tokomaks and other laboratory plasma devices. The results from the research will be incorporated into a series of workshops designed to introduce K-12 teachers to the physics of Earth's space environment.

该项目将评估动力学阿尔芬波将冲击太阳风（磁鞘）等离子体穿越地球磁场（磁层）的外边界（称为磁层顶）的能力。传统上，这个边界应该是不可穿透的磁鞘等离子体穿透不超过一个陀螺半径到地球的磁层。然而，现场观测表明，穿透超过10秒的回旋半径的宽度，实际上，地球磁层的大部分等离子体都是由磁鞘等离子体构成的。值得注意的是，在磁层顶的边界层，磁鞘和磁层等离子体的混合总是充满了低频电磁波动。有人认为这些波是动力学阿尔芬波。理论研究表明，动力学阿尔芬波可能是有效的跨磁场传输等离子体。该项目将使用磁层顶的多点场和来自星团航天器的等离子体观测，以确定存在的波，并评估它们解释那里看到的等离子体传输的能力。虽然该项目专门针对地球磁层顶的等离子体传输，但这个问题是许多物理情况下等离子体传输的核心，包括太阳上的磁环和托卡马克和其他实验室等离子体设备中的等离子体传输。研究结果将纳入一系列讲习班，旨在向K-12教师介绍地球空间环境的物理学。