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 …

Atomic data, such as wavelengths, spectroscopic labels, broadening parameters and
transition rates, are necessary for many applications, especially in plasma diagnostics, and …

The latest published version of GRASP (General-purpose Relativistic Atomic Structure
Package), ie, GRASP2018, retains a few suboptimal subroutines/algorithms, which reflect …

An extensive set of level energies, wavelengths, line strengths, oscillator strengths, lifetimes,
hyperfine structures, Land e´ g J-factors, electric dipole (E1), magnetic dipole (M1), electric …

Employing two fully relativistic methods, the multi-reference configuration Dirac–Hartree–
Fock (MCDHF) method and the relativistic many-body perturbation theory (RMBPT) method …

Using a population of large-scale filaments extracted from an AREPO simulation of a Milky
Way–like galaxy, we seek to understand the extent to which observed large-scale filament …

Comment on “Theoretical Confirmation of the Low Experimental 3C=3D f-Value Ratio in Fe
XVII" Recently, Mendoza and Bautis Page 1 Comment on “Theoretical Confirmation of the Low …

Employing the advanced relativistic configuration interaction (RCI) combined with the many-
body perturbation theory (RMBPT) method, we report energies and lifetime values for the …

The calculations are performed for the lowest 427 fine-structure levels arising from the 2 s 2
2 p 4, 2 s 2 p 5, 2 p 6, 2 s 2 2 p 3 nl (n= 3− 4, l≤ n− 1), 2 s 2 p 4 nl (n= 3− 4, l≤ n− 1), and 2 p …

Employing two state-of-the-art methods, multiconfiguration Dirac–Fock and second-order
many-body perturbation theory, highly accurate calculations are performed for the lowest …