Mathematical Sciences: Analysis of Collisionless Plasmas

数学科学：无碰撞等离子体的分析

• 批准号: 8801738
• 负责人: Jack Schaeffer
• 金额: $ 4.07万
• 依托单位: Carnegie-Mellon University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1988
• 资助国家: 美国
• 起止时间: 1988-07-01 至 1991-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=8801738&HistoricalAwards=false
• 关键词: Mathematical; Sciences; Analysis; Collisionless; Plasmas

The purpose of this research will be to analyze models of the time evolution of collisionless plasmas moving under the influence of their self-induced electromagnetic fields. These models take the form of systems of partial differential equations, the Poisson- Vlasov system and the Maxwell-Vlasov system. The unknown in each model is the density of the plasma, and the Maxwell-Vlasov system is somewhat more complete of the two systems, exhibiting electrical and magnetic effects as well as relativistic. Globally symmetric solutions were first established in 1952, and numerous extensions followed. However, the problem of global existence of classical solutions for general data is still open for either system. Recent results establish the breakdown of certain solutions in finite time. One goal of this work will be to show that when the initial data is nearly spherically symmetric, global existence of solutions is guaranteed. A second line of investigation proposes to model the interaction between the solar wind and the earth's magnetic field. By this one understands the neutral stream of charged particles moving rapidly away from the sun. It consists mainly of protons and electrons which, when they encounter the earth's magnetic field, induce currents adding to the total magnetic field. The resulting interaction is believed to account for the aurora borealis and geomagnetic storms. Another feature of this interaction is a bow shock wave across which the behavior of the plasma changes abruptly. The precise nature of shock waves in collisionless plasmas is still unclear. A mixed initial value-boundary value problem is proposed to model the above interaction. Initial work to be done will be in establishing global existence results for solutions and to determine conditions under which solutions tend to a steady state as time increases. Applications to the physical sciences are clear.

本研究的目的是分析在其自感电磁场影响下运动的无碰撞等离子体的时间演化模型。这些模型采用偏微分方程组的形式，泊松-弗拉索夫系统和麦克斯韦-弗拉索夫系统。在每个模型中未知的是等离子体的密度，麦克斯韦-弗拉索夫系统在这两个系统中更完整，表现出电和磁效应以及相对论性。1952年首次建立了全局对称解，随后进行了大量扩展。然而，对于一般数据经典解的全局存在性问题对于这两个系统来说仍然是开放的。最近的结果证实了某些解在有限时间内的分解。这项工作的一个目标是证明当初始数据是近球对称时，解的全局存在性是保证的。第二项研究建议建立太阳风和地球磁场之间相互作用的模型。由此我们可以理解中性的带电粒子流是如何迅速远离太阳的。它主要由质子和电子组成，当它们遇到地球磁场时，会产生电流，从而增加总磁场。由此产生的相互作用被认为是北极光和地磁风暴的原因。这种相互作用的另一个特征是弓形激波，等离子体的行为会突然改变。无碰撞等离子体中冲击波的确切性质尚不清楚。提出了一个混合初始值-边值问题来模拟上述相互作用。要做的初步工作将是建立解的整体存在性结果，并确定解随着时间的增加趋于稳定状态的条件。在物理科学上的应用是显而易见的。