MULTI-LINE SPECTROSCOPY OF GRAINS

机译：谷物的多线光谱

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Ca II H2V bright grains were observed using multi-linernspectroscopy in Ca II H, Hβ, and Fe I in order to study thernrelation between Ca II H2V brightenings and velocity oscillationsrnin the chromosphere and the photosphere. Ourrnobservation indicates that Ca II H2V bright grains are associatedrnwith 5 mHz velocity oscillations in the chromospherernand the photosphere. This result suggests tha CarnII H2V bright grains are explained by acoustic shocks inrnthe chromosphere, which agree with the numerical simulationrnby Carlsson & Stein (1996).

机译：为了研究Ca II H2V增亮与色球和光圈中的速度振荡之间的关系，采用多线光谱技术在Ca II H，Hβ和Fe I中观察到了Ca II H2V明亮的晶粒。我们的观察表明，Ca II H2V亮晶粒与色球层和光球中的5 mHz速度振荡有关。这个结果表明，CarnII H2V明亮的晶粒是由色球中的声震解释的，这与Carlsson＆Stein（1996）的数值模拟是一致的。

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来源
《The dynamic sun: challenges for theory and observations》|2005年|1-4|共4页
会议地点 Leuven(BE)
作者
S. Kamio; H. Kurokawa;
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作者单位

Kwasan and Hida Observatories, Kyoto 607-8471 Japan, kamio@kwasan.kyoto-u.ac.jp;

Kwasan and Hida Observatories, Kyoto 607-8471 Japan;

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原文格式 PDF
正文语种 eng
中图分类
关键词
Sun : Chromosphere; Sun : Oscillation; Sunrn: Photosphere;

机译：太阳：色球；太阳：振荡； Sunrn：Photosphere;

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MULTI-LINE SPECTROSCOPY OF GRAINS

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