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Collaborative Research: GEM--Asymmetric Entry and Transport of Magnetospheric Plasma During Periods of Northward Interplanetary Magnetic Field

Collaborative Research: GEM--Asymmetric Entry and Transport of Magnetospheric Plasma During Periods of Northward Interplanetary Magnetic Field
合作研究:GEM--北行行星际磁场期间磁层等离子体的不对称进入和输运
批准号:
1003876
负责人:
Lawrence Lyons
金额:
$16.33万
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:
2010-09-01 至 2013-08-31

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中文摘要
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英文摘要
This project will investigate the transport of plasma from the solar wind into and through Earth's magnetosphere during intervals when the interplanetary magnetic field (IMF) has a northward orientation. During periods of northward IMF the plasma within Earth's plasma sheet often is characterized by having two components, one hot and one relatively cold. The cold component has a somewhat higher temperature on the dawn flank of the magnetosphere than on the dusk side and this suggests that the mechanism by which plasma enters the magnetosphere is not symmetric. This project will use kinetic plasma simulations with the PLAsma Transport Numerical Magnetosphere Model (PLATNUMM) to investigate the plasma entry and transport mechanism. The plasma simulations will be done using realistic magnetic and electric field models for northward IMF conditions. The project will characterize the plasma phase space densities that develop in the layer connecting the magnetosphere with the magnetosheath. The results of the simulation will be compared with observations of the plasma from spacecraft. In addition, the project will simulate the plasma circulation within the plasma sheet in order to understand the asymmetries observed in the large-scale features.Although periods of northward IMF are typically not periods of strong magnetic activity it is important to understand the evolution of the magnetically quiet times because they form the initial conditions that determine the dynamics of the magnetosphere during magnetically disturbed times. Understanding the transition from magnetically quiet to disturbed times is important for our understanding of space weather phenomena that can impact humans and human engineered systems. Much of the research will be carried out by a female graduate student and the project involves a collaboration between a university research program at UCLA and an independent research and development center (Aerospace Corporation).
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Collaborative Research: Flow Channel Control of Substorm Expansion Phase Spatial Coverage and Duration
  • 批准号:
    2055192
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $37.99万
  • 财政年份:
    2021
  • 负责人:
    Lawrence Lyons
  • 依托单位:
Collaborative Research: Supersubstorms--Their Driving and Responses in the Magnetosphere, Ionosphere, and Thermosphere
  • 批准号:
    1907483
  • 项目类别:
    Standard Grant
  • 资助金额:
    $18.54万
  • 财政年份:
    2019
  • 负责人:
    Lawrence Lyons
  • 依托单位:
Collaborative Research: Coordinated Radar and Optical Analysis of Flow Channel Disturbances within the Nightside Auroral Oval/Plasma Sheet
  • 批准号:
    1401822
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $52.87万
  • 财政年份:
    2015
  • 负责人:
    Lawrence Lyons
  • 依托单位:
Collaborative Research: PFISR Ion-Neutral Observations in the Thermosphere (PINOT)
  • 批准号:
    1242356
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $13.83万
  • 财政年份:
    2012
  • 负责人:
    Lawrence Lyons
  • 依托单位:
国内基金
海外基金
Research on Quantum Field Theory without a Lagrangian Description
  • 批准号:
    24ZR1403900
  • 项目类别:
    省市级项目
  • 资助金额:
    --
  • 批准年份:
    2024
  • 负责人:
    SATOSHI NAWATA
  • 依托单位:
Cell Research
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Cell Research (细胞研究)