ChiantiPy Core Routines¶

ChiantiPy.core Package¶

chianti.core - contains the main classes for ChiantiPy users.

Copyright 2009-2015, 2010 Kenneth P. Dere

 bunch(temperature, eDensity, wvlRange[, ...]) Calculate the emission line spectrum as a function of temperature and density. continuum(ionStr, temperature[, abundance, ...]) The top level class for continuum calculations. ion(ionStr[, temperature, eDensity, ...]) The top level class for performing spectral calculations for an ion in the CHIANTI database. ioneq(z[, verbose]) Reads, calculates, and/or plots the ionization equilibrium for an element as a function of temperature. ipymspectrum(temperature, eDensity, wavelength) this is the multiprocessing version of spectrum for using inside an IPython Qtconsole or notebook. mspectrum(temperature, eDensity, wavelength) this is the multiprocessing version of spectrum radLoss(temperature, eDensity[, ...]) Calculate the emission spectrum as a function of temperature and density. spectrum(temperature, eDensity, wavelength) Calculate the emission spectrum as a function of temperature and density.