The Arcetri spectral code for thin plasmas

Details The Arcetri spectral code for thin plasmas The Arcetri spectral code for thin plasmas

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26as..133..411l&link_type=abstract

Astronomy and Astrophysics Supplement, v.133, p.411-425

Astronomy and Astrophysics

Astrophysics

18

Atomic Data, Plasmas, Solar Atmosphere, Stellar Atmosphere, Ultraviolet: General, Astronomical Data Bases: Miscellaneous

Scientific paper

The Arcetri spectral code allows to evaluate the spectrum of the radiation emitted by hot and optically thin plasmas in the spectral range 1 - 2000 Angstroms. The database has been updated including atomic data and radiative and collisional rates to calculate level population and line emissivities for a number of ions of the minor elements; a critical compilation of the electron collision excitation for these elements has been performed. The present version of the program includes the CHIANTI database for the most abundant elements, the minor elements data, and Fe III atomic model, radiative and collisional data.

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