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- W3022707984 abstract "The Arcetri-95 spectral code for optically thin plasmas computes the continuum and line emission of the ions of the most abundant elements. It includes the most updated atomic models and the main atomic processes for ions from Fe IX to Fe XXIII and for ions of the Belike, C-like, and N-like isoelectronic sequences. The power emitted per unit emission measure is produced as a function of temperature and density. Comparison with observations requires the knowledge of the differential emission measure (DEM) as a function of temperature. A numerical code evaluates the best DEM distribution that satisfies observations and theoretical predictions. The spectral code together with the DEM code allows to compute synthetic spectra for any specified temperature distribution model of the plasma." @default.
- W3022707984 created "2020-05-13" @default.
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- W3022707984 date "1996-01-01" @default.
- W3022707984 modified "2023-09-23" @default.
- W3022707984 title "The Arcetri Spectral Code for Optically-Thin Plasmas" @default.
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- W3022707984 doi "https://doi.org/10.1017/s0252921100036526" @default.
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