X-ray and ultraviolet (UV) observations of the outer solar atmosphere have been used for
many decades to measure the fundamental parameters of the solar plasma. This review …

Dielectronic recombination is a process particularly effective in high-temperature dilute
plasmas such as those observed, for example, in astrophysics. This process was first …

A comprehensive set of accurate atomic data is required for analyses of astrophysical and
solar spectra. CHIANTI provides a database of atomic energy levels, wavelengths, radiative …

Nous décrivons un ensemble complet de programmes informatiques pour calculer diverses
quantités atomiques, comme les niveaux d'énergie, les transitions radiatives, l'excitation et …

B Supplementary mathematics Page 1 B Supplementary mathematics B.1 Linear operators on
Hilbert space General references [1], [2], [3], [4] B.1.1 Hilbert spaces This appendix summarizes …

The magnetic-dipole probabilities for the 1D2–3P2 and 1D2–3P1 transitions in carbon-like
and oxygen-like ions are calculated up to atomic number Z= 12, including relativistic …

Namhafte Autoren, alles hervorragende Kapazitaten auf ihrem Gebiet, definieren Theorie,
Diagnostik, Modelle, apparative Ausrustung und Anwendungen. Sie diskutieren die …

RMATRX1 is a general program to calculate atomic continuum processes using the R-matrix
method, including electronatom and electron-ion scattering, and radiative processes such as …

Atomic data from the IRON Project. 1: Goals and methods ADS Classic is now deprecated. It will
be completely retired in October 2019. This page will automatically redirect to the new ADS …

The CHIANTI spectral code consists of an atomic database and a suite of computer
programs to calculate the optically thin spectrum of astrophysical objects and carry out …