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CHIANTI consists of a critically evaluated set of up-to-date atomic
data, together with user-friendly programs written
in Interactive Data Language (IDL) to calculate the spectra
from astrophysical plasmas.
- The Chianti wine-producing area of Tuscany, Italy - |
CHIANTI Version 6.0.1 Released !CHIANTI 6 includes a complete database of ionization and recombination coefficients for the first 30 elements of the periodic table, as well as IDL programs to read them. Other improvements concern He-like line emission, ionization equilibrium, and new or revised data for ions emitting between 1 and 2000 Angstrom. (see the history file ) Major features (Dere et al. 2009, A&A, 498, 915) in CHIANTI 6 are:
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We are grateful to individual scientists and funding agencies for their support.
Page maintained by Enrico Landi .