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Description du projet

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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System requirement is not defined
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2010-12-10 07:08 Retour à la liste release
0.3

Cette version ajoute la classe mspectrum, qui permet aux utilisateurs d'utiliser plusieurs cœurs de processeur pour les calculs locaux spectrale qui peut prendre du temps. En outre, il existe de nombreux bugs.
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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