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All releases of ChiantiPy

  •  11 Aug 2013 14:58
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    Release Notes: This is another bugfix release. The methods and functions for calculating ionization cross section were never properly implemented, and this has been corrected. The calculation of ionization rate coefficients were performed correctly. Errors in the calculation of photo-excitation and stimulated emission have been corrected.

    •  07 Feb 2013 15:30
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      Release Notes: This release fixes a major bug. Users are strongly suggested to upgrade to this version.

      •  24 Jan 2013 16:43
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        Release Notes: This release accommodates the changes made in 7.1 of the CHIANTI atomic database. In addition, there is a new method "emissList" that allows one to print out a list of lines in a given wavelength range. Also, there is a new keyword "wvlRanges" for the chianti.ion.intensityRatio method that allows the user to determine intensity ratios for lines that are widely separated in wavelength. The documentation has been updated and describes these features in the "Quick-Start" guide.

        •  29 May 2012 16:23
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          Release Notes: This is a bugfix release.

          •  02 Nov 2011 18:14
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            Release Notes: 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.

            •  30 Aug 2011 17:08
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              Release Notes: 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.

              •  28 Jun 2011 14:42
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                Release Notes: Various bugs were fixed.

                •  09 Dec 2010 16:01
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                  Release Notes: 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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