Solar Wind and Illumination Control of Plasma Irregularity Production in the Polar Cap

极冠等离子体不规则性产生的太阳风和照明控制

• 批准号: 1248127
• 负责人: Roman Makarevich
• 金额: $ 23.82万
• 依托单位: University of Alaska Fairbanks Campus
• 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: 2013-09-15 至 2017-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1248127&HistoricalAwards=false
• 关键词: Solar; Wind; Illumination; Control; Plasma

This project seeks to improve our understanding of ionospheric irregularities, building on recent work at high southern latitudes that demonstrated a clear connection between the interplanetary magnetic field (IMF) and irregularity production in the auroral E-region. The fundamental issue to be addressed is solar control of irregularity production via indirect IMF effects versus direct effects of solar-induced ionization. This study will focus on evaluating the extent of IMF control of small-scale irregularities and the relationship to other scales. The project will address the question of whether the presence of the polar patches is a necessary condition for irregularity production, and whether solar illumination suppresses or enhances irregularity generation. Inter-hemispheric differences will be investigated to determine the relative importance of solar wind drivers versus solar ionization.Earlier studies of small-scale plasma irregularities have analyzed local observations using rockets and/or radio techniques. This project will analyze irregularity production in the polar cap in context of its global drivers focusing on observations from the first US Antarctic HF (SuperDARN) radar at McMurdo, Antarctica and complementary instrumentation. The polar cap ionosphere is directly connected to the solar wind; hence, one can expect IMF effects on small-scale irregularity production to be even more pronounced than in the previously studied auroral region. The polar cap also has reasonably uniform solar ionization conditions near solstices and sharp contrasts between seasons, so solar illumination effects can be revealed more clearly. In addition, the polar cap appears to be especially rich in irregularities. This project will leverage data from the NSF-funded Antarctic facilities, providing essential support for a newly-established faculty researcher in the US, and expand a graduate student training program in the geosciences area in Alaska.

该项目旨在增进我们对电离层不规则性的了解，其基础是最近在南半球高纬度地区开展的工作，这些工作表明行星际磁场与极光E区不规则性的产生之间存在明确的联系。要解决的根本问题是通过间接IMF效应与太阳能诱导电离的直接影响的不规则性生产的太阳能控制。这项研究将着重评价货币基金组织对小规模违规行为的控制程度及其与其他比额表的关系。该项目将解决的问题，是否存在的极补丁是一个必要条件的不规则生产，以及太阳照明抑制或增强不规则的生成。将调查半球间的差异，以确定太阳风驱动器与太阳电离的相对重要性。早期的小规模等离子体不规则性研究分析了当地的观测使用火箭和/或无线电技术。该项目将在其全球驱动因素的背景下分析极冠的不规则性生产，重点是南极洲麦克默多的第一台美国南极HF（SuperDARN）雷达和补充仪器的观测。极冠电离层直接连接到太阳风，因此，可以预期IMF对小规模的不规则性生产的影响甚至比以前研究的极光区更明显。在至点附近，极冠也有相当均匀的太阳电离条件，季节之间的对比也很明显，因此太阳照明效应可以更清楚地显示出来。此外，极冠似乎特别丰富的不规则性。该项目将利用NSF资助的南极设施的数据，为美国新成立的教师研究人员提供必要的支持，并扩大阿拉斯加地球科学领域的研究生培训计划。