Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012apj...744...99l&link_type=abstract
The Astrophysical Journal, Volume 744, Issue 2, article id. 99 (2012).
Astronomy and Astrophysics
Astronomy
3
Atomic Data, Atomic Processes, Sun: Uv Radiation, Sun: X-Rays, Gamma Rays, Ultraviolet: General, X-Rays: General
Scientific paper
The CHIANTI spectral code consists of an atomic database and a suite of computer programs to calculate the optically thin spectrum of astrophysical objects and carry out spectroscopic plasma diagnostics. The database includes atomic energy levels, wavelengths, radiative transition probabilities, collision excitation rate coefficients, and ionization and recombination rate coefficients, as well as data to calculate free-free, free-bound, and two-photon continuum emission. Version 7 has been released, which includes several new ions, significant updates to existing ions, as well as Chianti-Py, the implementation of CHIANTI software in the Python programming language. All data and programs are freely available at http://www.chiantidatabase.org, while the Python interface to CHIANTI can be found at http://chiantipy.sourceforge.net.
Del Zanna Giulio
Dere Ken P.
Landi Enrico
Mason Harris E.
Young Paul R.
No associations
LandOfFree
CHIANTI—An Atomic Database for Emission Lines. XII. Version 7 of the Database does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with CHIANTI—An Atomic Database for Emission Lines. XII. Version 7 of the Database, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CHIANTI—An Atomic Database for Emission Lines. XII. Version 7 of the Database will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-751240