The CHIANTI atomic database
The CHIANTI atomic database
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DOI：
10.1088/0953-4075/49/7/074009
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发表时间：
2015-12
期刊：
影响因子：
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通讯作者：
P. Young;K. Dere;E. Landi;G. Zanna;H. Mason
中科院分区：
文献类型：
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作者：
P. Young;K. Dere;E. Landi;G. Zanna;H. Mason
免费可用的基安蒂红酒原子数据库于1996年首次发布，对天体物理等离子体发射的分析和建模产生了巨大影响。它包含用于模拟低密度(≲1013厘米−3)等离子体从X射线到红外波长的光学薄原子和正离子发射的数据和软件。一个关键特点是对数据进行评估并定期更新，版本8于2015年发布。基安蒂红酒中包含了用于模拟246个离子和中性元素发射率的原子数据，以及用于推导直到锌的所有元素的电离分数的数据。这里总结了不同类型的原子数据，并讨论了它们的格式。文中给出了基安蒂红酒对天体物理界影响的统计数据，并给出了各种应用的例子。
The freely available CHIANTI atomic database was first released in 1996 and has had a huge impact on the analysis and modeling of emissions from astrophysical plasmas. It contains data and software for modeling optically thin atom and positive ion emission from low density (≲1013 cm−3) plasmas from x-ray to infrared wavelengths. A key feature is that the data are assessed and regularly updated, with version 8 released in 2015. Atomic data for modeling the emissivities of 246 ions and neutrals are contained in CHIANTI, together with data for deriving the ionization fractions of all elements up to zinc. The different types of atomic data are summarized here and their formats discussed. Statistics on the impact of CHIANTI to the astrophysical community are given and examples of the diverse range of applications are presented.