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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) and Python to calculate the spectra
from astrophysical plasmas.
- The Chianti wine-producing area of Tuscany, Italy -
CHIANTI Database Version 8.0 released, Sept 2015
In addition, the method for computing the differential emission measure has been changed. Details can be found in Del Zanna et al. (2015), in press (see http://arxiv.org/abs/1508.07631).
Important note: for various reasons, it has been necessary to modify the format of the elvlc and splups files. The elvlc files have been restructured but retain the same name, while the splups files have been significantly revised and are now renamed as "scups" files. For both the updated elvlc and new scups files, an ascii fixed text width format has been retained. We have modified the CHIANTI software to read these new files, but all the main software is left unchanged.
The new database and IDL programs are incompatible with the previous CHIANTI versions and vice-versa.
We are grateful to individual scientists and funding agencies for their support.