SHINE: Observationally Constraining the Physical Processes that Generate the Solar Wind

SHINE:观测限制产生太阳风的物理过程

基本信息

  • 批准号:
    1060194
  • 负责人:
  • 金额:
    $ 57.55万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Continuing Grant
  • 财政年份:
    2011
  • 资助国家:
    美国
  • 起止时间:
    2011-04-01 至 2015-03-31
  • 项目状态:
    已结题

项目摘要

The proposers will investigate Alfven waves and magnetic reconnection as primary sources for the heating and acceleration of the solar wind. This research team will analyze new spectroscopic data from the "Extreme ultraviolet Imaging Spectrometer" onboard the Hinode spacecraft in order to resolve the current debate as to whether Alfven waves carry sufficient energy to heat and accelerate the solar wind. The proposers note that these results will provide much needed empirical data to constrain the competing wave-driven and turbulence-driven models of the solar wind, and ultimately help to determine the true solar wind acceleration mechanism.By providing hands-on research experiences for individual teachers each summer at Columbia University's "Summer Research Program for Science Teachers," this team will help improve the commitment and scientific understanding of middle and high school science teachers from the New York City metropolitan area. This activity will have far reaching benefits, since analysis of Columbia's 21-year-old outreach program shows that the teachers who have participated go on to teach about 1,000 students each over the next ten years and also see a 10% increase in the pass rate of their students on the New York State Regents science exam. The proposers will also visit middle and high school science classes to explain their research and answer questions directly from students. Given the fact that New York City has a diverse student population with a high percentage of underrepresented groups and minorities, these education and outreach efforts constitute a high impact program.
提议者将研究Alfven波和磁重新连接,作为太阳风加热和加速的主要来源。该研究团队将分析Hinode航天器上的“极端紫外线成像光谱仪”的新光谱数据,以解决有关Alfven Waves是否具有足够能量以加热和加速太阳风的当前辩论。提议者指出,这些结果将提供急需的经验数据,以限制竞争性波动和湍流驱动的太阳风模型,并最终有助于确定真正的太阳能风能加速机制。通过为每年夏天的哥伦比亚大学教师提供的“夏季科学教师”的教师,为个人的教师提供了新的教师,并有助于介绍“纽约大学的新教师”,并为高高的科学了解,这将有助于诺言。” 区域。这项活动将带来很大的收益,因为对哥伦比亚21岁的外展计划的分析表明,参加的教师在接下来的十年中每人都会教约1,000名学生,并且在纽约州摄政科学考试中的学生的及格率提高了10%。提议者还将访问中学和高中科学课,以解释他们的研究并直接回答学生的问题。鉴于纽约市拥有多样化的学生人口,而人数不足的群体和少数群体比例很高,因此这些教育和外展工作构成了一项高影响力计划。

项目成果

期刊论文数量(0)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)

暂无数据

数据更新时间:2024-06-01

Daniel Wolf Savin的其他基金

Laboratory Measurements of N2 Reacting with H3+ Isotopologues and Implications for Deuterated Astrochemistry
N2 与 H3 同位素体反应的实验室测量及其对氘代天体化学的影响
  • 批准号:
    2002461
    2002461
  • 财政年份:
    2020
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Standard Grant
    Standard Grant
Laboratory Measurements of Dissociative Recombination with Cold Molecular Ions for Ground-Based Studies of Diffuse Molecular Clouds
用于弥散分子云地面研究的冷分子离子解离重组的实验室测量
  • 批准号:
    1907188
    1907188
  • 财政年份:
    2019
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Standard Grant
    Standard Grant
Laboratory measurements of three deuterium substitution reactions important in interstellar chemistry
星际化学中重要的三种氘取代反应的实验室测量
  • 批准号:
    1613267
    1613267
  • 财政年份:
    2016
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Standard Grant
    Standard Grant
Improving Models of Molecular Clouds and Planetary Atmospheres: Dissociative Recombination Measurements for Molecular Ions of Astronomical Interest
改进分子云和行星大气模型:天文感兴趣的分子离子的解离重组测量
  • 批准号:
    1107036
    1107036
  • 财政年份:
    2011
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Development of a Novel Instrument to Study the Cosmic Origins of Organic Chemistry and the Cosmo-Chemical Pathway towards Life
开发一种新仪器来研究有机化学的宇宙起源和生命的宇宙化学途径
  • 批准号:
    0905832
    0905832
  • 财政年份:
    2009
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Standard Grant
    Standard Grant
Improved Understanding of Molecular Clouds and Emission Line Objects with Laboratory Astrophysics Studies at the Heidelberg Ion Storage Ring
通过海德堡离子存储环的实验室天体物理学研究提高对分子云和发射线物体的理解
  • 批准号:
    0807436
    0807436
  • 财政年份:
    2008
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Further Measurements of Thermal Energy Charge Transfer in Support of Ground-Based Astronomy
支持地面天文学的热能电荷转移的进一步测量
  • 批准号:
    0606960
    0606960
  • 财政年份:
    2006
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Continuing Grant
    Continuing Grant
Development of a Novel Laboratory Instrument for Studying Gas-Phase Negative Ion Chemistry
开发用于研究气相负离子化学的新型实验室仪器
  • 批准号:
    0520660
    0520660
  • 财政年份:
    2005
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Standard Grant
    Standard Grant
Improved Simulations of Cosmic Plasmas: Measurements and Modeling Studies of Thermal Energy Charge Transfer in Support of Ground-Based Astronomy
改进的宇宙等离子体模拟:支持地面天文学的热能电荷转移的测量和建模研究
  • 批准号:
    0307203
    0307203
  • 财政年份:
    2003
  • 资助金额:
    $ 57.55万
    $ 57.55万
  • 项目类别:
    Continuing Grant
    Continuing Grant

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