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项目描述

ChiantiPy is a Python interface to the CHIANTI atomic database for astrophysical spectroscopy. The CHIANTI atomic database for astrophysical spectroscopy provides the information necessary to calculate the emission spectrum from hot plasmas. ChiantiPy provides several top-level classes to access the database and calculate continuum and emission line intensities.

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Information regarding Project Releases and Project Resources. Note that the information here is a quote from Freecode.com page, and the downloads themselves may not be hosted on OSDN.

2013-02-08 10:15
0.5.1

此版本修复了一个主要的 bug。强烈建议用户升级到此版本。
This release fixes a major bug. Users are strongly suggested to upgrade to this version.

2011-11-03 16:46
0.4.1

已进行了修改，以保持与基安蒂数据库版本 7.0 兼容。ChiantiPy 分布的结构已经更改以便安装当前版本之前，必须删除 ChiantiPy 0.4.1 之前的任何版本。
Modifications have been made to remain compatible with the CHIANTI database Version 7.0. The structure of the ChiantiPy distribution has changed so that any version of ChiantiPy prior to 0.4.1 must be removed before installing the current version.

2011-08-31 05:40
0.4.0

此版本添加了类radLoss计算辐射损失和绘制的结果。现在的方法ion.popPlot，绘制直方图的水平人口，如果只有一个指定的温度和密度的单个值。在此之前，它预期多个温度或密度。已作出的一些错误修正。
标签: Major
This release adds the class radLoss to calculate radiative losses and plot the results. The method ion.popPlot now plots a histogram of level populations if only a single value of temperature and density are specified. Previously, it expected multiple temperatures or densities. A number of bugfixes have been made.

2011-06-29 05:38
0.3.1

各种修正了已知错误。
标签: Alpha, Python, Scientific, Astronomy, spectroscopy
Various bugs were fixed.

2010-12-10 07:08
0.3

此版本增加了mspectrum类，它允许用户使用多个用于光谱计算方法，既耗时本地CPU核心。此外，还有许多错误修正。
This release adds the mspectrum class, which allows users to use multiple local CPU cores for spectral calculations that can be time consuming. In addition, there are numerous bugfixes.

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