Collaborative Research: Physics of Magnetized Dusty Plasmas

合作研究：磁化尘埃等离子体物理

• 批准号: 1301881
• 负责人: Edward Thomas
• 金额: $ 1.5万
• 依托单位: Auburn University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2013
• 资助国家: 美国
• 起止时间: 2013-08-01 至 2016-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1301881&HistoricalAwards=false
• 关键词: Collaborative; Research; Physics; Magnetized; Dusty

Plasmas (i.e., charged, ionized gases) are pervasive. From stellar nurseries to the Earth's ionosphere, plasmas represent a fourth state of matter that is the most common form of matter in the visible universe. Moreover, a phenomenon known as a "dusty" or "complex" plasma is formed when charged particulate matter, such as dust or ices, becomes incorporated in the plasma environment. In space, phenomena such as in comet tails or the rings of Saturn are examples of dusty plasmas. Closer to Earth, control over particulates in plasmas are important in high-technology and microelectronic fabrication. In both astrophysical and technological plasmas, the presence of magnetic fields can have a profound influence on the properties of the plasma. This research project supports a new, state-of-the-art, multi-user, superconducting, high-magnetic device to understand the basic properties of a strongly magnetized plasmas and magnetized dusty plasma. The intellectual merit of this work is that it will enable the study of new regimes of plasma physics and dusty plasma physics that have not been accessible in previous experiments. The main project goal is to investigate how the structural, thermal, charging, and stability properties of a dusty plasma evolve as the system is taken from an unmagnetized state through a progression of regimes where first the electrons, then the ions, and then charged microparticles become magnetized.The broader impact of this work is substantial. This project is a direct collaboration among three US universities (Auburn University, The University of Iowa, and University of California-San Diego) that perform leading research in the field of dusty plasmas. The researchers from these three organizations will coordinate a broad team of collaborators representing universities, national laboratories, and international partners. And, this project will provide excellent opportunities to train the next generation of plasma scientists through the training of graduate and undergraduate students as well as providing partnerships with dusty plasma researchers at predominantly undergraduate institutions.

等离子体（即，带电的、电离的气体）是普遍存在的。 从恒星孕育到地球电离层，等离子体代表物质的第四种状态，是可见宇宙中最常见的物质形式。 此外，当带电的颗粒物质（例如灰尘或冰）并入等离子体环境中时，形成称为“多尘”或“复杂”等离子体的现象。 在太空中，彗星尾巴或土星环等现象都是尘埃等离子体的例子。 在更接近地球的地方，控制等离子体中的微粒对高科技和微电子制造非常重要。 在天体物理和技术等离子体中，磁场的存在会对等离子体的性质产生深远的影响。 该研究项目支持一种新的，最先进的，多用户，超导，高磁设备，以了解强磁化等离子体和磁化尘埃等离子体的基本特性。 这项工作的智力价值在于，它将使研究等离子体物理和尘埃等离子体物理的新制度，在以前的实验中还没有访问。 该项目的主要目标是研究尘埃等离子体的结构、热、充电和稳定性如何随着系统从非磁化状态通过一系列机制而演变，这些机制首先是电子，然后是离子，然后是带电微粒变得磁化。这项工作的广泛影响是巨大的。 该项目是美国三所大学（奥本大学、爱荷华州大学和加州大学圣地亚哥分校）之间的直接合作，这三所大学在尘埃等离子体领域进行了领先的研究。 来自这三个组织的研究人员将协调代表大学，国家实验室和国际合作伙伴的广泛合作者团队。 而且，该项目将提供极好的机会，通过培训研究生和本科生，以及提供与尘埃等离子体研究人员在主要本科院校的合作伙伴关系，培养下一代等离子体科学家。