首页> 外文期刊>The Astrophysical journal >Extreme Ultraviolet Explorer Spectra of the 1993 March Flares on AD Leonis: The Differential Emission Measure and Implications for Coronal Structure
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Extreme Ultraviolet Explorer Spectra of the 1993 March Flares on AD Leonis: The Differential Emission Measure and Implications for Coronal Structure

机译:1993年3月在AD Leonis上爆发的极端紫外线探测器光谱:差分发射量度及其对冠状结构的影响

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摘要

The flare star AD Leonis was observed by the Extreme Ultraviolet Explorer (EUVE) from 1993 March 1 to 3 UT. Two flares were detected by the EUVE Deep Survey detector and spectrometer and also seen in optical photometry on 1993 March 2 UT. The DS Lexan/boronband and optical results have been discussed in the previous paper by Hawley et al. In this paper, we describe the spectra observed by EUVE during quiescence, the peaks of the flares, and the decay phase following the first flare and analyze the spectra to investigate the stellar atmospheric structure during these time periods.
机译:1993年3月1日至UT 3期间,极紫外探测器(EUVE)观测到火星AD Leonis。 EUVE深度探测探测器和光谱仪探测到两个耀斑,并在UT于1993年3月2日的光学光度法中看到。 Hawley等人在先前的论文中讨论了DS Lexan /硼带和光学结果。在本文中,我们描述了EUVE在静止期间观察到的光谱,耀斑的峰值以及第一次耀斑之后的衰减阶段,并分析了这些光谱以研究这些时间段内的恒星大气结构。

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