权益分类	功能权益	普通用户	{{item.name}}会员
{{category.name}}	{{benefitItem.name}}

Mathematical Studies of Magnetohydrodynamics with Hall Effect

霍尔效应磁流体动力学的数学研究

基本信息

批准号：
1815069
负责人：
Mimi Dai
金额：
$ 18.88万
依托单位：
University of Illinois at Chicago
依托单位国家：
美国
项目类别：
Standard Grant
财政年份：
2018
资助国家：
美国
起止时间：
2018-08-01 至 2022-07-31
项目状态：
已结题

来源：
https://www.nsf.gov/awardsearch/showAward?AWD_ID=1815069&HistoricalAwards=false
关键词：
Mathematical Studies Magnetohydrodynamics Hall Effect

项目摘要

Magnetic reconnection is a fundamental process in highly conducting plasmas, which allows for rapid changes in the configuration of the magnetic flux lines, with the conversion of magnetic to kinetic energy. Solar flares, violent events with significant impact to telecommunications and the electric grid, may involve magnetic reconnection in a large scale. Magnetic reconnection is inherently a multi-scale process and causes difficulties in laboratory experimental study, satellite observations, and computational simulations. During magnetic reconnection, the magnetic force can create thin localized region wherein the elevated voltage difference generates intense electric currents and dissipation - the Hall effect. The Hall Magnetohydrodynamics (Hall MHD) model has recently received increasing attention because of its improvements in predicting the fast-changing nature of magnetic reconnection compared to other models. Nevertheless, the mathematical theory of this model is far from being complete. This project will address fundamental mathematical questions for the Hall MHD model and provide theoretical insights for experiments and numerical simulations. The project will involve a graduate student in the research. The Hall MHD model is mathematically challenging due to the usual convective nonlinearities and the additional source term given by the Hall effect. The main objectives are: 1) Explore the largest possible space of well-posedness corresponding to the major scalings in the system. 2) Search the optimal Sobolev spaces in which the model is well-posed. 3) Examine ill-posedness of solutions in some physically relevant spaces. 4) Seek minimal conditions for weak solutions to satisfy energy identity. 5) Study the asymptotic behavior of solutions and stability of the steady state. The project will combine known tools from harmonic analysis and partial differential equations, and develop new methods to study these questions.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.

磁重联是高导电等离子体中的一个基本过程，它允许磁通线的配置快速变化，并将磁能转换为动能。太阳耀斑是对电信和电网有重大影响的剧烈事件，可能涉及大规模的磁重联。磁场重联是一个多尺度过程，给实验室实验研究、卫星观测和计算机模拟带来了困难。在磁重联期间，磁力可以产生薄的局部区域，其中升高的电压差产生强电流和耗散-霍尔效应。霍尔磁流体动力学（Hall MHD）模型最近受到越来越多的关注，因为它在预测磁场重联的快速变化的性质相比，其他模型的改进。然而，这个模型的数学理论还远未完成。该项目将解决霍尔MHD模型的基本数学问题，并为实验和数值模拟提供理论见解。该项目将涉及一名研究生的研究。霍尔MHD模型是数学上的挑战，由于通常的对流非线性和额外的源项由霍尔效应。主要目标是：1）探索系统中主要标度对应的最大可能适定性空间。2)搜索模型适定的最优Sobolev空间。3)在一些物理相关的空间中检查解的不适定性。4)求弱解满足能量恒等式的最小条件。5)研究解的渐近性态和定态的稳定性。该项目将结合联合收割机已知的工具，从谐波分析和偏微分方程，并开发新的方法来研究这些问题。这个奖项反映了NSF的法定使命，并已被认为是值得的支持，通过评估使用基金会的智力价值和更广泛的影响审查标准。