The Arcetri Spectral Code for optically thin plasmas

Details The Arcetri Spectral Code for optically thin plasmas The Arcetri Spectral Code for optically thin plasmas

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...384.1124l&link_type=abstract

Astronomy and Astrophysics, v.384, p.1124-1132 (2002)

Astronomy and Astrophysics

Astrophysics

4

Atomic Data, Plasmas, Sun: Atmosphere, Stars: Atmospheres, Ultraviolet: General, Astronomical Data Bases: Miscellaneous

Scientific paper

The Arcetri Spectral Code allows one to evaluate the spectrum of the radiation emitted by hot and optically thin plasmas in the spectral range 1-2000 Å. The Arcetri Code consists of a series of files that contain the emissivity of the plasma as a function of electron temperature and density. Both line and continuum emission are considered. These quantities are calculated using a database of atomic data and transition probabilities, mostly taken from the CHIANTI database. In the present work we describe the updates to the spectrum and present the new results. A comparison with the previous version of the code allows us to assess the improvements to the spectrum; comparison with other spectral codes allows us to assess the completeness of the Arcetri Code and of the CHIANTI database.

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