Extremely Large EUV Late Phase of Solar Flares

来源 :The Fourteenth International Solar Wind Conference (第十四届国际太阳 | 被引量 : 0次 | 上传用户：abcd_11840

【摘要】

：

The second peak in the Fe XVI 33.5 nm line irradiance observed during solar flares by Extreme ultraviolet Variability Experiment(EVE) is known as Extreme UltraViolet(EUV) late phase.

【作者】

：

Kai Liu Yuming Wang Jie Zhang Xin Cheng Rui Liu Chenglong Shen

【机构】

：

CAS Key Laboratory of Geospace Environment,Department of Geophysics and Planetary Sciences,School of

【出处】

：

The Fourteenth International Solar Wind Conference (第十四届国际太阳

【发表日期】

：

2015年5期

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The second peak in the Fe XVI 33.5 nm line irradiance observed during solar flares by Extreme ultraviolet Variability Experiment(EVE) is known as Extreme UltraViolet(EUV) late phase.

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Extremely Large EUV Late Phase of Solar Flares

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