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SHINE: Kinetic Heating of Coronal Hole Ions for Generation of the Solar Wind by Imbalanced Turbulence

SHINE: Kinetic Heating of Coronal Hole Ions for Generation of the Solar Wind by Imbalanced Turbulence
SHINE:冕洞离子的动力学加热,通过不平衡湍流产生太阳风
批准号:
0962506
负责人:
Philip Isenberg
金额:
$43.41万
依托单位:
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2010
资助国家:
美国
项目状态:
已结题
起止时间:
2010-03-01 至 2014-02-28

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中文摘要
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英文摘要
The project will investigate the turbulent generation of the fast solar wind by using an existing numerical model that solves the coupled quasilinear equations of proton diffusion and resonant wave growth. During this project, the Principal Investigator (PI) will progressively add more physical processes to the numerical model and finally compare the simulation output with observations. At each step, the team will explore the consequences of expanding their model on the heating and acceleration of coronal hole protons and minor ions. The PI asserts that these investigations will lead to more detailed kinetic models of the generation of the solar wind in the corona, enabling improved understanding and predictions of the state of the heliospheric environment. This work will also provide new insights into self-consistent plasma kinetics and the dissipation of plasma turbulence.Specifically, the team will add nonlinear wave effects, such as resonance broadening and turbulent transport, to their simulations in order to yield realistic Alfvén wave growth in the solar wind. They will also incorporate such nonlinear calculations into their inhomogeneous coronal hole model. The team plans to construct a detailed kinetic model for the radial evolution of coronal hole protons as heated by imbalanced wave fields, obtaining predictions for the kinetic particle and wave states. The PI will also compare his model's output with actual coronal hole observations taken by existing spacecraft instruments. The modeling effort will yield predictions of particle and wave fluxes that will guide the development of, and be tested by, future NASA spacecraft missions, such as 'Solar Orbiter' and 'Solar Probe Plus.' The tasks will be performed within the theoretical turbulence and reconnection group at the University of New Hampshire, which will provide opportunities for graduate students and postdoctoral researchers to participate in this project.
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Quasilinear Dissipation of Turbulently-Generated Kinetic Alfven Waves: Kinetics of Ion Heating and Solar Wind Acceleration in Coronal Holes
  • 批准号:
    2005982
  • 项目类别:
    Standard Grant
  • 资助金额:
    $55.3万
  • 财政年份:
    2020
  • 负责人:
    Philip Isenberg
  • 依托单位:
SHINE: Self-Consistent Resonant-Cyclotron Heating of Protons and Alpha Particles in the Solar Wind and Solar Corona
  • 批准号:
    1358103
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $34.34万
  • 财政年份:
    2014
  • 负责人:
    Philip Isenberg
  • 依托单位:
Studies of Wave-Particle Interactions for Interstellar Pickup Ions in the Solar Wind
  • 批准号:
    0635863
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $32.6万
  • 财政年份:
    2007
  • 负责人:
    Philip Isenberg
  • 依托单位:
NSWP: Kinetic Turbulence-Driven Solar Wind Model Through the Resonant Cyclotron Interaction - Protons and Alpha Particles
  • 批准号:
    0719738
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $46.43万
  • 财政年份:
    2007
  • 负责人:
    Philip Isenberg
  • 依托单位:
国内基金
海外基金
关于Kinetic Cucker-Smale模型及相关耦合模型的适定性研究
  • 批准号:
    12001530
  • 项目类别:
    青年科学基金项目
  • 资助金额:
    24.0万元
  • 批准年份:
    2020
  • 负责人:
    金春银
  • 依托单位:
带奇性的 Kinetic Cucker-Smale 模型在随机环境中的平均场极限及时间渐近行为研究
  • 批准号:
    11801194
  • 项目类别:
    青年科学基金项目
  • 资助金额:
    25.0万元
  • 批准年份:
    2018
  • 负责人:
    张雄韬
  • 依托单位:
Kinetic Monte Carlo 模拟薄膜生长机理的研究
  • 批准号:
    10574059
  • 项目类别:
    面上项目
  • 资助金额:
    12.0万元
  • 批准年份:
    2005
  • 负责人:
    郑小平
  • 依托单位: