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Updated: Mar 7, 2026

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
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Published on: August 25, 2016

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来自DKIST/ViSP的第一个Ca II H和H爆发光谱的光谱分析和RHD建模

Cole Tamburri1,2,3, Adam Kowalski1,2,3, Gianna Cauzzi1

  • 1National Solar Observatory, University of Colorado Boulder, 3665 Discovery Drive, Boulder, CO 80303 USA.

Solar physics
|March 6, 2026
PubMed
概括

使用丹尼尔·K·伊诺耶太阳望远镜进行的高分辨率太阳耀斑观测显示了与当前模型的差异. 这就是Ca II H光谱线.

关键词:
太阳耀斑光谱 太阳耀斑光谱太阳耀斑是发生在太阳上的.

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