fiasco.io Package#
Parsers for raw CHIANTI atomic data. fiasco uses these parsers to transform the raw ASCII files into an HDF5 version of the CHIANTI database.
Classes#
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Data access layer for each distinct CHIANTI dataset |
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Interface layer for CHIANTI data stored in HDF5 format. |
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General parser interface for all CHIANTI datatypes. |
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Base class for CHIANTI files attached to a particular ion |
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Base class for CHIANTI file parsers |
Class Inheritance Diagram#
fiasco.io.sources Package#
Classes for parsing CHIANTI data sources.
Classes#
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Autoionization rates for each level in an ion. |
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Scaled cross-sections for calculating the ionization rate due to direct ionization. |
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Fit parameters for calculating dielectronic recombination. |
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Spline fits to the excitation-autoionization scaled cross-sections. |
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Scaled collision strengths for calculating ionization rates due to excitation autoionization. |
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Energy levels and configurations for each level in an ion. |
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Energy levels and configuration related to the calculation of the free-bound continuum. |
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Free-free Gaunt factor as a function of scaled frequency and energy |
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Total free-free Gaunt factor as a function of scaled temperature. |
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Parameters for calculating two-photon continuum for hydrogen-like ions |
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Parameters for calculating two-photon continuum for helium-like ions. |
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Total (frequency-integrated) non-relativistic free-free Gaunt factor as a function of a scaled temperature. |
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Total (frequency-integrated) relativistic free-free Gaunt factor as a function of a scaled temperature and scaled atomic number. |
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Fit parameters for calculating relativistic free-free Gaunt factor using the method of Itoh et al. [ISK+00]. |
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Free-bound gaunt factor as a function of photon energy for several different energy levels. |
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Spline fits to scaled collision rates for protons. |
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Level-resolved recombination rates as a function of temperature. |
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Fit parameters for calculating radiative recombination rates. |
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Scaled collisions strengths (denoted by upsilon) between energy levels as described in Burgess and Tully [BT92]. |
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Spline fits to scaled collisions strengths (denoted by upsilon) between energy levels as described in Burgess and Tully [BT92]. |
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Fit parameters for calculating partial photoionization cross-sections using the method of Verner and Yakovlev [VY95]. |
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Information about each possible transition in an ion, including level indices, wavelengths, and decay rates. |