Module Spectrum

Classes

bunch
Calculate the emission line spectrum as a function of temperature and density.

spectrum
Calculate the emission spectrum as a function of temperature and density.

Variables

__package__ = 'chianti.core'

defaults = {'abundfile': 'sun_photospheric_1998_grevesse', 'fl...

Variables Details

Value:

{'abundfile': 'sun_photospheric_1998_grevesse',
 'flux': 'energy',
 'gui': False,
 'ioneqfile': 'chianti',
 'wavelength': 'angstrom'}