Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000rmxac...9..140l&link_type=abstract
"Astrophysical Plasmas: Codes, Models, and Observations, Proceedings of the conference held in Mexico City, October 25-29, 1999,
Astronomy and Astrophysics
Astrophysics
2
Scientific paper
CHIANTI consists of a critically evaluated set of atomic data and transition probabilities necessary to calculate the emission line spectrum of astrophysical plasmas. The data consist of atomic energy levels, atomic radiative data such as wavelengths, weighted oscillator strengths and A values, and electron collisional excitation rates. A set of programs that use these data to calculate the spectrum in a desired wavelength range as a function of temperature and density is also provided. A suite of programs has been developed to carry out plasma diagnostics of astrophysical plasmas. The state-of-the-art contents of the CHIANTI database will be described and some of the most important results obtained from the use of the CHIANTI database will be reviewed.
No associations
LandOfFree
CHIANTI--An Atomic Database for EUV Emission Lines 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 EUV Emission Lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CHIANTI--An Atomic Database for EUV Emission Lines will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1347146