Emission Line Imaging Spectroscopy for Diagnosing of Solar Outer Atmospheres
Emission Line Imaging Spectroscopy for Diagnosing of Solar Outer Atmospheres
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DOI：
10.1585/pfr.2.s1011
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发表时间：
2007
影响因子：
0.8
通讯作者：
Tetsuya Watanabe
中科院分区：
文献类型：
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作者：
Tetsuya Watanabe
日本太阳观测卫星“Hinode”搭载的极紫外成像光谱仪在17-21纳米和25-29纳米两种极紫外波长范围内实现了迄今为止最高的灵敏度。EIS将能够提供有关日冕和过渡区的详细诊断信息。一个新的工具，时间相关的碰撞辐射模型将被开发来分析的数据，这台EIS仪器，并诊断这些等离子体的温度和密度在太阳的外层大气。
The Extreme Ultraviolet Imaging Spectrometer on board the Japanese Sun Observing Satellite “Hinode” realizes the highest sensitivity ever achieved in the two EUV wavelengths of 17-21 nm and 25-29 nm. EIS will be able to provide the detailed diagnostic information on solar corona and transition region. A new tool of timedependent collisonal-radiative model will be developed to analyze the data taken by this EIS instrument, and to diagnose temperatures and densities of those plasmas in the outer atmospheres of the Sun.